00:00 | this conference will now be recorded. can all see my slides. |
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00:09 | Yes sir. Okay. All Just reviewing what we covered yesterday |
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00:16 | Um We talked about with psalms ratio it's called an elastic module. I |
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00:23 | it's a little bit different from the module i in that instead of a |
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00:31 | between stress and strain, it's a of two strengths and these are the |
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00:39 | strain. So why is the vertical X. And Z. Or horizontal |
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00:44 | ? It's the ratio of the horizontal I'm sorry, excuse me. I |
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00:52 | it back uh Z. Is the axis. So uh this is the |
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00:59 | of the horizontal axis and it would equal in both directions horizontally. So |
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01:07 | X. X. Or X. Y. Y. To the vertical |
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01:13 | . That ratio. Trans verse two strength, his foot sans ratio. |
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01:19 | as I said, sometimes it's represented this uh this creek v like it |
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01:26 | like an italics. The um sometimes represented by sigma but you can see |
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01:32 | sigma's representing stresses. So a different for persons ratio and exploration. |
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01:40 | We typically use sigma for persons ratio in rock mechanics, sigma is stress |
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01:47 | structural geology. Sigma is stressed. I mentioned this minus sign. This |
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01:53 | all a matter of how you choose coordinates. Uh So I wouldn't worry |
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01:58 | it too much. Um For our . Hassan's ratio is positive for Franny |
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02:08 | rocks. We also talked about the wave modules. And this was a |
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02:17 | situation for Hassan's ratio were laterally So if you squeeze the rock |
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02:25 | it's gonna strain laterally for the P module lists. Um we constrain the |
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02:33 | laterally, so we can't strain And this is analogous to what happens |
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02:40 | you pass a compression all way through . Any volume elements, any infinite |
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02:47 | , volume element of the rock is as you're compressing it and it wants |
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02:54 | expand laterally but it can't because it's to another infant intestinal volume element which |
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03:02 | is trying to stretch laterally. And those forces cancel out. And the |
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03:11 | is that the volume element shortens but doesn't get better. So this is |
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03:18 | kind of module, is that a wave? See and you can see |
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03:24 | is equal to roe V. P also K plus four thirds view. |
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03:31 | So uh this is the uni axial sigma's easy in the vertical direction and |
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03:42 | the shortening in the vertical direction. strain in the vertical direction. And |
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03:47 | the P wave modules is that uh constant. Notice that the other strains |
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03:57 | all zero. Okay. So um huh. It is not allowed to |
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04:03 | in other directions. And the difference the P wave module lists and Young's |
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04:10 | list is uh the youngs module list unconstrained. Therefore the stresses the other |
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04:19 | with the zero right? And it's to straight in the other directions. |
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04:28 | , so all the other applied stresses zero. Now which brings us to |
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04:36 | relationship between the essenes ratio and So we said Parsons ratio is the |
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04:45 | verse strain to the ratio of the strain to the vertical strain with the |
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04:52 | strain. And it could also be in terms of the velocity ratio. |
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05:02 | we said that any elastic modules can expressed in terms of any two other |
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05:08 | module? It well the B. . V. S ratio is has |
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05:14 | modules and sheer modules in it. cancels out the density. So you |
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05:19 | see we have bulk unsure module lists here. So actually this expression is |
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05:24 | way of uh equating facades ratio to other elastic module. I both modules |
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05:31 | cheer modules. And keep in mind is for an icy tropic material. |
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05:36 | there are only two independent module I all the other module. Light Can |
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05:41 | expressed in terms of those two. is an interesting expression because it relates |
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05:49 | to rock properties. I mean to . Now if we measure Hassan's ratio |
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05:57 | measuring VP and Bs, then that a what we would call a dynamic |
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06:05 | modules. So it's derived from velocity . Now we can make some statements |
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06:13 | Uh huh. What uh the relationship was songs ratio and the V. |
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06:20 | . B. S pressure for when Parsons ratio is zero, what |
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06:26 | the V. P. V. ratio? You'll have to you'll have |
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06:29 | do the math here. So I'm you to do the math And calculate |
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06:40 | PBS when persons ratio is zero. when persons ratio is zero, B |
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06:57 | B s squared minus two is equal zero. B P B s squared |
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07:02 | two. Then So be PBS is square root of two. So 1.41 |
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07:12 | the minimum practical. VPBS remember we zero is a practical limit of Hassan's |
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07:18 | although it can be negative. Um , I'm not personally aware of measurements |
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07:26 | Hassan's ratio below or V PBS below root of two on rocks. Not |
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07:33 | , I believe. So that is our minimum be PBS ratio for our |
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07:42 | . Let me ask you a more question. Uh what is Hassan's |
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07:49 | When the V pDS ratio is In other words, when the shear |
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07:54 | velocity is zero, the B P s ratio is infinity. So in |
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07:58 | fluid, what is Hassan's ratio No, for fluid With sons ratio |
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08:10 | .5. And we could uh if use a crazy math, if you |
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08:16 | my kind of math, that's easy see We have the PBS. This |
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08:22 | . So we have infinity squared -2 infinity. And we have twice in |
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08:27 | infinity squared -2. That equals twice . Infinity Divided by twice infinity is |
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08:35 | . of course that mathematics doesn't You have to take the limit of |
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08:40 | expression as V P B s approaches . And you'll find that as being |
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08:47 | approaches infinity for persons ratio approaches point And as I said, if you |
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08:54 | to convince yourself of that, an math problem would be to maintain the |
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09:02 | constant and try to compress a If you compress it is gonna spread |
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09:11 | because it's not constrained. And if go through the math holding the volume |
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09:17 | that new shape equal to the volume the first, the original shape, |
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09:22 | get a possum's ratio .5. So can do that easily by compressing a |
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09:28 | or a a square or something like , not a square, a |
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09:35 | something like that. And and work the volumes as you compress the rock |
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09:40 | cetera. So from that equation between ratio and be PBS We see that |
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09:50 | is a 1-1 relationship between persons ratio the v. ratio. If I |
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09:57 | B P B S, I know ratio and vice versa. Um Now |
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10:04 | V. P B s ratio. I if I take Vp over bs |
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10:10 | , that's K plus quarters mu That's K over mu plus four |
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10:17 | So you can see that the BPBS also has a 1-1 relationship with Ko |
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10:23 | you. And so, okay, is k overview is uh conceptually and |
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10:31 | or or an easy concept to So it helps you conceptualize in terms |
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10:38 | in compressibility and rigidity What the different ratios. Me now, it turns |
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10:45 | that there's a a bit of a in the literature about the use of |
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10:53 | ratio in geophysics. Uh There's a of workers prefer to use the |
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11:00 | P. B. S ratio and personally prefer to use the V. |
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11:05 | . B. S rations. Um fred Hiltermann on the other hand, |
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11:12 | works in very similar areas that I prefers to use those odds ratio. |
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11:17 | you can see there is no except if you're dealing with Heidi PVS |
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11:24 | . Hassan's ratio varies very little, it might be a little bit clumsy |
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11:28 | deal with with sons ratio, which why I prefer the B. |
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11:31 | B. S ratio similarly at very since ratios. Uh huh. You |
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11:39 | there's a lot more variation with sons than in the B P. |
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11:42 | S friction. So if you're dealing very low uh with songs ratios, |
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11:48 | the V. P. B s is uh more interesting. I'm |
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11:53 | the person's ratio shows a greater range it's somewhat easier to deal with, |
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12:01 | really there's no difference. Uh The reached a point where leon, Thompson |
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12:09 | a paper in the leading edge entitled was not a geophysicist. In other |
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12:15 | , he argued that there is that should not use Hassan's ratio. Uh |
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12:21 | geophysical equations. I'm agnostic on I prefer V. PBS but I'm |
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12:28 | to use persons ratio. In fact has come up with some useful approximations |
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12:34 | Hassan's ratio. So my school of is whatever works for you, whatever |
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12:40 | you through the night. Use Yeah. Now there are theoretical limits |
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12:51 | the elastic module. It uh for , rigidity is greater than zero. |
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12:57 | module is is greater than or equal zero. Similarly, the both modules |
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13:01 | greater than equal to zero, Lama is constant can be negative because |
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13:10 | you work through the math Land of two, you over Third is greater |
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13:16 | or equal to zero. So you lambdas is greater than equal to minus |
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13:23 | mu over three. So lambda can negative. But also interestingly, Hassan's |
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13:30 | from the negative. We said the lower limit Of uh four songs ratio |
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13:37 | zero but the theoretical limit is So I'm going to ask you to |
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13:44 | a little exercise right now and calculate B P B s ratio When persons |
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13:52 | is -1. So what is the theoretical, the minimum theoretically uh smallest |
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14:02 | . P. V. S ratio you can have. So I'm gonna |
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14:06 | recording and ask you to make that . This conference will now be |
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14:19 | I was muted. Uh so the is square root of 4/3 1.15 is |
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14:28 | . Yeah or pretty close to square theirs. And so this is |
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14:37 | We have two minus two V. . B s squared on this |
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14:42 | Um Is that right to minus to P B s squared. And so |
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14:50 | we have uh subtract two from both . So you have uh two |
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14:57 | P. B. S squared and . P. V. S. |
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15:04 | so uh that's K. Plys four view over twice. K plus four |
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15:13 | view. And and so You work it and you get square root of |
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15:26 | . Ok, so coming back to velocity equations, if we look at |
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15:32 | ratio of BP over bs quantity you could see that's K plus four |
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15:39 | view. Uh huh, overview. is k overview plus four thirds. |
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15:46 | you could ask yourself what is the possible V. P. B. |
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15:50 | ratio. Uh Well uh we'll have problem if we send you to zero |
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15:57 | then we'll be dividing by zero. won't work. Uh But uh we |
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16:03 | let both modulates the zero. And then we have the density cancel |
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16:09 | When we take the ratio rigidity cancel . When we take the ratio. |
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16:14 | what we got get is VP over . S. is the square root |
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16:17 | 4/3. So that's when you can the minimum be PBS ratio is when |
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16:24 | have some rigidity but you have both of zero. Again, we know |
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16:29 | no rocks uh that that are obey mm Okay, so as I mentioned |
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16:39 | , there are various different ways to uh the elastic module I and |
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16:46 | psychotropic material. Given any two, can calculate the others, for |
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16:51 | in this case, uh they're calculating is constant from young's modules and persons |
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16:59 | . And they're arriving at the solving the V P. B. S |
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17:06 | here. So, or the V . V P ratio, beta is |
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17:10 | . S. Alpha is VP on slide. Uh So you can uh |
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17:18 | for the V P V S ratio terms of innocence ratio. Another interesting |
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17:25 | , llamas constant over here Is equal K -2/3 of you. Now, |
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17:32 | been another controversy in the industry where claim is that lamb is constant is |
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17:40 | sensitive to hydrocarbons uh than other things the D P. B. S |
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17:46 | or so forth. And you can that the change in LAMAs constant due |
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17:54 | high departments is exactly the same as change in the bulk modules. The |
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18:00 | is not affected by hydrocarbons. Lamb constant. Then can be no more |
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18:08 | than the bulk modules. So that put that idea to rest like somehow |
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18:15 | constant has some magical properties that are to other. All right. |
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18:23 | quantities. Mhm. Okay. I want to talk about History |
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18:31 | History says uh but can have different in different applications, but in our |
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18:41 | it means that the velocity you measure the module is that Iraq has, |
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18:48 | depends on its history of deformation. which then depends on the history of |
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18:55 | apply to it. So in other , the velocity of Iraq doesn't depend |
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19:01 | on the current day pressure regime, depends on pressures that were fired in |
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19:09 | past. So history says at least has the word history in it. |
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19:17 | . So it means the properties of rock depend on its history. And |
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19:25 | here we have some velocity measurements. are on uh uh igneous metamorphic |
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19:33 | And so these, you can presume to be very low porosity rocks. |
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19:39 | you see that when the the death here is as you're increasing the |
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19:46 | so you're increasing the stress um pressure an omni directional stress. So uh |
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19:56 | pressure is increasing the velocities go but then they level off, why |
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20:02 | they level off? Because essentially you've all the cracks that that might exist |
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20:09 | the rock or the large majority of . And then the mineral itself is |
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20:16 | in compressible. It's relatively insensitive to pressure. It's mostly the closing of |
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20:22 | space and forcing grains against each other firmly. Right, so you you |
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20:30 | up the rock and let me get point, you're here, you pressure |
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20:37 | the rock, you close crash, force brains against each other more strongly |
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20:43 | then you've done all the work, know, most of the work. |
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20:46 | then just a very minor increase things leveled off, you then deep pressure |
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20:52 | rock, which is the solid So we're going from high pressure to |
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20:57 | . And you see that uh, a certain point, you start opening |
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21:01 | cracks again that had previously been But the final velocities are higher. |
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21:08 | when you were pressuring the reason the velocities are higher is because you permanently |
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21:17 | the rock, you've closed them for that then won't open up again or |
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21:23 | changed certain grain contacts. Maybe you've those brain contact stronger and um, |
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21:34 | don't completely go back to the original . So here we're seeing some kind |
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21:41 | irreversible deformation. Right? So there's plastic behavior here. Uh, and |
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21:48 | resulting velocities are higher. And we that here, we see that |
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21:55 | uh, we see no history since this case. So all the fractures |
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22:02 | opened or or that closed when you pressuring then opened back up as you |
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22:08 | deep pressure. Now, interestingly, of these curves come back to the |
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22:15 | situation. So, at intermediate some of the cracks have not opened |
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22:23 | . Some of the cracks that have closed, don't open back up. |
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22:27 | if you take enough pressure off, all open back up. And so |
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22:32 | come back to your original velocities. a few cases, we talked about |
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22:45 | void and Royce pounds previously. And , we're going to go over that |
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22:51 | because essentially Boy and Royce bounds are medium theories. What is an effective |
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22:59 | theory? It says given for a arrangement of constituents. I'm going to |
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23:09 | the module lists of the composite from module I of the individual constituents. |
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23:16 | if I know exactly how the constituents arrays are arranged, I can do |
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23:22 | calculation analytically. And so I can the properties of the effective media. |
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23:29 | we said that for the void this would be the highest possible module |
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23:34 | you could get would be when uh you're applying uh you have columns here |
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23:43 | you're playing compression is parallel to those . So, imagine a plate |
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23:49 | Imagine I have this thing in a and I'm applying a uni actual stress |
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23:57 | along an entire plate. And what is the strong columns. Say they're |
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24:03 | dark grey. We'll do we'll provide of the resistance to that compression. |
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24:12 | And the resulting module, this is volume weighted average of the module I |
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24:19 | the individual constituents. So, here have to constituents. Is the module |
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24:25 | . So, the effective module lists the medium? Is the volume weighted |
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24:31 | ? Where f is the volume The volume weighted average of the individual |
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24:37 | are, by the way, is is the screen cutting off? Are |
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24:42 | not seeing the very bottom of the ? Um Yes, so the screen |
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24:48 | customs. Oh, okay. That's . Um So maybe uh you may |
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24:56 | to follow me on on your Um Yeah, I don't I don't |
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25:02 | an easy way to fix this right . Let's see if I. All |
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25:10 | , Well this is one way. , so we'll try going doing it |
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25:22 | this for a while. We'll see that works. Um Now that does |
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25:28 | , but now you have the whole , right? So for the void |
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25:35 | , it's a linear volume weighted So we've seen this before, on |
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25:41 | other hand, we have the Royce where we have parallel layers. And |
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25:46 | course, you can just imagine uh planks or metal place with foam rubber |
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25:53 | between. Right? If I sit that stack of layers, the foam |
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26:00 | is going to compress much more than planks of wood. Right? So |
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26:07 | foam rubber is a common, is for most of the strength. So |
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26:14 | in the Royce configuration, that's the compressible situation. The softest layer is |
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26:21 | uh most of the work, it's reciprocal bye and weighted average here. |
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26:32 | the strain in each layer is different this configuration. You can see that |
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26:37 | that played if I have, if have a plate here compressed against those |
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26:43 | vertical columns, all the columns are to strain that are going to shorten |
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26:48 | same amount, right? The week or the highly compressible columns can't compress |
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26:56 | than the in compressible columns and that's columns are used in architecture, in |
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27:03 | . You have the column, which be stone or cement? And you |
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27:07 | the weak layer being air in between columns. Right? Um So the |
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27:14 | layers can't compress any more than the layers, whereas here the strong layer |
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27:19 | hardly compress and the weak layers accommodate of the compression. Okay, |
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27:30 | I think we could go full strength this one. So um here we |
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27:38 | we've seen a lot of velocity versus and we're seeing some things that we've |
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27:44 | before. So the Royce equation is lower bound that's also called woods relationship |
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27:52 | devoid averages. The higher bound. you can't have velocities higher than the |
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27:57 | average or lower than the Royce When you do get velocities below |
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28:03 | There's either experimental error or you don't that. You haven't calculated the bound |
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28:12 | properly. Probably using the wrong constituent . Right? So, but we're |
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28:20 | far wrong here. All right. we have a variety of data |
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28:25 | there seems to be an upper bounds , a practical upper bound which is |
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28:30 | from the void average. And this be described by the critical porosity |
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28:37 | But then in between uh that upper and and the voice pounds, you |
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28:42 | a lot of points in between. why would you get points? You |
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28:47 | if these are the most fully liquefied ? Why do you get these points |
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28:53 | between the upper bound and the lower ? What would be a hypothesis if |
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28:59 | see points down in here, what you guess about the rock? Why |
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29:20 | rock spot closer to the lower You see out here past the critical |
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29:26 | , you have a bunch of, know, these are ocean bottom sediments |
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29:30 | at the lower bound or slightly These are completely unlit defied rocks. |
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29:37 | if the Royce band represents completely unlit and the critical porosity model represents fully |
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29:48 | , why might you be in between up? You know, the just |
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30:04 | different degree of uh speaking. exactly, that's it. So, |
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30:11 | these rocks maybe slightly cemented or slightly , such that they're interlocking and have |
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30:18 | rigidity, but they're not fully liquefied this. Yeah, okay, so |
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30:29 | we have various velocity versus pressure And as we're increasing the pressure, |
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30:35 | velocity goes up. But you we have different uh degrees of velocity |
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30:44 | . Notice that at high pressures, of these rocks tend to level off |
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30:52 | presumably with this stance down. If want to even higher pressure, it |
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30:56 | level off. So at some point level off and we talked about Uh |
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31:03 | initial increase in velocity as having to with four space and cracks closing. |
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31:11 | here we see different relations, for , this limestone has a very small |
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31:17 | . This dolomite has a very big . So, could you hypothesis differences |
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31:25 | the poor structure of this limestone and dolomite. Can you make an inference |
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31:33 | as to why you have this different to pressure, if you don't |
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31:42 | Um they were going to their So we'll be seeing some key points |
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31:47 | the Dolomites compared on some micro porosity the limestone. Okay, so, |
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31:53 | gonna say it's it's in this I'm gonna say it's exactly the |
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31:57 | Right? I'm going to say, , buggy pores have a poor, |
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32:02 | velocity is poorly sensitive to the buggy . If I increase the pressure, |
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32:08 | buggy poor is still going to be buggy poor. Right? So, |
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32:11 | going to close it a little I'm going to close some micro |
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32:15 | maybe some fractures, but I'm going suggest that this limestone is dominated by |
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32:21 | poor. So, it doesn't have big change. The dome light on |
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32:26 | other hand, when you re crystallize into dolomite, you can introduce inter |
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32:34 | ferocity between the faces of the dolomite and those pores, uh, will |
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32:43 | to be very flat and act like . Or it's possible that this particular |
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32:50 | happens to be more fractured than that . So, generally, when I |
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32:55 | a large sensitivity to pressure at low , that generally indicates cracks closing. |
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33:03 | , I would argue that this dolomite more low aspect ratio ferocity in |
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33:10 | like step, the sand pack, are no fractures here. It's a |
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33:16 | pack. Right, but I'm suggesting the grain context themselves are acting like |
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33:24 | . So they have the effect of same effect as cracks. And as |
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33:30 | mentioned uh stand stones tend to have aspect ratio an effective aspect ratio on |
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33:37 | order of .1. Their velocities behave if They were composed of ellipse soil |
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33:45 | with an aspect ratio .1. Now I'm the stand pack as I increase |
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33:51 | pressure, how do we how is done in the laboratory? They take |
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33:56 | sand pack and it's jacketed, it's . So as as I increase the |
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34:03 | pressure on this thing, I really have a lot of opportunity to rearrange |
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34:08 | grains, especially if it's a high confining pressure from all directions. So |
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34:17 | I increase that confining pressure, the are going up. Not because I'm |
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34:23 | the grains and reducing the ferocity very I don't change the ferocity very much |
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34:28 | all in this experiment. But the do level out. And what that |
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34:35 | is underperforming the grain contacts and I'm the grain contacts flatter and flatter. |
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34:41 | the grain context becomes stronger and stronger you platinum. So a point contact |
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34:48 | easy to compress, but once it's compressed it gets harder and harder to |
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34:54 | it as the contact area between the increases. Okay, so here we |
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35:06 | Iraq where the shear wave velocity is increasing very much with pressure and we |
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35:13 | have that sharp increase in p wave . Uh This is a dry |
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35:21 | We do have and it's apparently not fractured because we're not having a very |
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35:26 | change of velocity By the way, is the compressibility of the rock. |
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35:32 | compressibility is one open the bulk module . Uh So you can see that |
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35:38 | I compress the rock, it becomes compressible. So the bulk modules is |
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35:44 | and again it levels off. so again here you can see pores |
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35:50 | , maybe grain contacts, maybe micro ferocity, maybe fractured ferocity, these |
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35:58 | are closing and then things level Okay. We already talked about the |
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36:08 | between static and dynamic module I and just to review um dynamic module I |
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36:15 | derived from velocity static module, I a constant stress and these these values |
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36:23 | typically different um dynamic module I are larger than static module. I uh |
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36:33 | reasons. Uh First of all dynamic I involved much smaller variations in |
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36:44 | Uh in in in stress you are small changes in uh devia turyk |
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36:51 | So the strain amplitudes are much smaller static stresses tend to be a lot |
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36:58 | . So there's the ability with a stress to uh induce some plastic deformation |
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37:07 | will cause the rock to be more compressible or less rigid as you plastic |
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37:13 | to form the rock. Whereas a measurement, you're strictly uh in the |
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37:19 | range also dynamic measurements you have an , You have a frequency of the |
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37:27 | and the higher the frequency, uh higher the velocity. And you can |
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37:33 | that fundamental laws of physics. Using Cramers chronic relationships, you can prove |
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37:40 | if you have a frequency depend if have attenuation, you have frequency dependent |
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37:47 | . And for body weighs, the frequencies are faster than the low |
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37:53 | So for both reasons, the dynamic I tend to be larger than the |
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37:58 | modules. So here is just a of dynamic to static Young's module lists |
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38:08 | a variety of rocks. And this the ratio. And you can see |
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38:12 | most rocks the dynamic module is is than the static modules. But there's |
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38:21 | rock here where the dynamic modules is then the status modules. Uh |
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38:28 | do you want to offer a hypothesis explain that? That seems to be |
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38:33 | unusual behavior. So what if there no porosity? And uh and you |
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39:00 | a material that was so uh competent under the static compression it's not going |
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39:07 | undergo any kind of plastic deformation. statically is going to be elastic and |
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39:14 | . It's elastic then. And there there's no porosity. So there's no |
|
39:21 | negligible attenuation. So you don't really anybody wave dispersion. In that |
|
39:27 | the ratio would be one to get ratio smaller than one is difficult to |
|
39:34 | theoretically. So, I personally do have a reasonable hypothesis to explain this |
|
39:41 | . And I've asked students for many to offer hypothesis. I've not come |
|
39:46 | with a reasonable one. So this a case where I'm going to resort |
|
39:52 | experimental error. Maybe a the module are measured on different rocks. Maybe |
|
40:01 | the sample if it's the same maybe there's history sis effect. Um |
|
40:08 | for the two measurements, um maybe just experimental error. I I hate |
|
40:18 | resort to experimental error as an but uh it's possible that that is |
|
40:24 | we're dealing with. That's always the resort. Always try to come up |
|
40:29 | a physical explanation first. Okay, here we're looking at the ratio of |
|
40:40 | dynamic to static modules and similar to we were seeing with cracks, |
|
40:48 | affecting the velocities. Uh it also to affect the ratio of static to |
|
40:55 | module. So the greater the the smaller the ratio and at low |
|
41:02 | you have where you have more open space, more open microfractures and more |
|
41:11 | contacts between brains. Uh Your ratio dynamic to static module i is |
|
41:23 | Now, uh here's an important rock lesson. Uh here we have relationships |
|
41:32 | different quantities, all velocity related So these are quantities that can be |
|
41:38 | from seismic data. So, uh I cross plot and these are for |
|
41:45 | and shells. The sands are the points and the shells are the red |
|
41:54 | . And if I cross plot, wave impedance versus shear wave impedance. |
|
41:58 | see that I break out into two and that there is a line more |
|
42:03 | less dividing those populations. If I flood the D. P. |
|
42:08 | S. Ratio versus and penalize you I now have a horizontal line separating |
|
42:16 | looks like I have more spread. remember the I can get the elastic |
|
42:24 | I by multiplying the velocity times So I could calculate uh lambda times |
|
42:35 | and I could calculate new times So what would a new times density |
|
42:42 | uh if I take uh Rovi Rovi squared uh and multiplied by density. |
|
42:51 | rho squared rho squared B. Square. So that would be |
|
42:56 | And I could do a similar thing lamb because remember uh it's lander plus |
|
43:03 | plus two. I'm sorry. lambda plus two U. Is equal |
|
43:09 | K plus four thirds view. So I could get euro from V. |
|
43:14 | . M. V. S. could also get lambda rho from |
|
43:17 | P. M. V. And again, lambda rho has been |
|
43:23 | as being more sensitive to the rock uh than uh these other parameters. |
|
43:33 | uh why don't you look at these cross plots and tell me which of |
|
43:41 | has greater sensitivity to live theology to type. I would say the d |
|
44:01 | the V. P. V. . Against the PM opinions. Well |
|
44:06 | V. P. B. S PM penis in my mind is the |
|
44:09 | convenient one because I don't even need impedance to distinguish fill apologies. Apparently |
|
44:15 | straight from the V. P. . S ratio. I could distinguish |
|
44:19 | anthologies here. So I could say and easier distinction to make. It's |
|
44:26 | convenient, but is it more Can I better differentiate uh the stands |
|
44:34 | the shell stands from the shelves? I better differentiate that using V. |
|
44:40 | . B. S and P Then I can using any of the |
|
44:43 | methods keep in mind that as I a coordinate transformation, remember these all |
|
44:57 | exactly the same information. They were derived from the impedance and Sharon |
|
45:06 | So um essentially lambda Roland euro come PMP Vince and Sharon P even |
|
45:17 | And so what that does is it out, it spreads out the |
|
45:26 | but the overlap is exactly the same all these cases. Look at these |
|
45:31 | that overlap with the other points where with Allah jeez, where there is |
|
45:38 | in the law theology, there's the amount of ambiguity in every case. |
|
45:45 | so the very important lesson here which people, many practicing geophysicists don't get |
|
45:54 | that a coordinate transformation does not improve content. The coordinate transformation never improve |
|
46:05 | or signal to noise ratio. If transform the axis, I not only |
|
46:14 | out the points, but I spread the arab or is associated with those |
|
46:20 | . So I would argue that these all exactly equivalent. So you know |
|
46:31 | by swearing and combining p wave impedance shear wave impedance to get land around |
|
46:38 | or taking their ratio to get P. B. S. I |
|
46:43 | get more sensitivity so that's kind of optical illusion. Okay. Any questions |
|
47:01 | then move on to the next Yeah. I'm sorry I need to |
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47:20 | this conference will now be recorded. . Professor. It's not it's not |
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47:27 | . I mean I I see blank slide Dennis. Do you see a |
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47:33 | slide author? Yes sir. Next our cash. I will stop recording |
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47:43 | conference will now be recorded. so I've mentioned this before. What |
|
47:52 | pressure? uh 40% well that's stress pressure is a stress but uh when |
|
48:03 | I use the term press pressure as to stress? Um It's uh stress |
|
48:13 | affected, pressure might not might not um Yeah. Well okay. Yeah |
|
48:20 | another way of saying it. So is on on the direction, |
|
48:25 | Where stress will depend on direction. do we measure pressure? So essentially |
|
48:48 | we use hooks law we can create mechanical devices where we have a known |
|
48:57 | . And from the strain of that we could measure the pressure. So |
|
49:03 | see how much uh it's been calibrated that we know a certain amount of |
|
49:09 | corresponds to a certain amount of So that involves knowing the spring constant |
|
49:17 | the, of the pressure gauge, , okay. Um pascal's principle uh |
|
49:27 | that you might not have off the of your head. So what is |
|
49:31 | principle? Um What pascal's principle says that so the pressure, If I |
|
49:41 | pressure in a fluid, it is immediately transmitted to the throughout the fluid |
|
49:52 | the edge of the container, we'll back to that in a bit. |
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49:57 | first let's talk about the units of and pressure. Um We talked about |
|
50:05 | we had mentioned dimes per centimeter Remember stresses force per unit area pressure |
|
50:13 | an omni directional stress as a So it's units will be some |
|
50:20 | the unit of force such as a , for example. We prefer to |
|
50:26 | Dines in at least I do. prefer to use Dines. Um And |
|
50:32 | for uh it could be per square , for example. So pascal's |
|
50:46 | If I apply pressure to an enclosed , it is transmitted undiminished to every |
|
50:54 | of the fluid and the walls of containing vessel. Um kind of a |
|
51:03 | thing to accept. If you think really giant containers, like the atlantic |
|
51:11 | , for example, if I apply pressure in new york does, it |
|
51:15 | a transmitted undiminished instantaneously to London. right, so we're gonna have to |
|
51:23 | you know, Suspend this belief a bit and say, well if the |
|
51:28 | is small enough for practical purposes, could assume this to be true. |
|
51:37 | Pascal was an interesting guy that made variety of very important contributions and this |
|
51:45 | in the 1600s. So this was early on. But uh he had |
|
51:51 | mystical experience uh before he died in abandoned his scientific work and uh became |
|
52:02 | philosopher and theologian. So uh maybe of us are just have not reached |
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52:09 | point of enlightenment yet or uh we're privileged enough that we can abandon our |
|
52:18 | . So now, uh if I a pressure at the surface of a |
|
52:29 | , I could calculate the pressure at death in the fluid just based on |
|
52:36 | weight of the fluid. So the at any death is equal to the |
|
52:43 | pressure. Plus grow jeezy. So is the depth. You aren't a |
|
52:49 | . She is the acceleration due to . And row is the density of |
|
52:55 | fluid. This is sometimes expressed as G. H. Where h is |
|
53:01 | hype of the fluid. Yeah. one way of measuring uh pressure is |
|
53:13 | the strain gauge. Uh excuse uh with a tube of mercury. |
|
53:21 | if you have a tube of mercury on top of a bath. Uh |
|
53:29 | , the atmosphere will push down on mercury and that will push up through |
|
53:34 | tube. And so the height in tube uh would be an indication of |
|
53:40 | atmospheric pressure and you have to be uh to do that. So the |
|
53:52 | static paradox here, we have three with the same fluid level. |
|
54:06 | if I go to the base, or Rogue Easy is the same for |
|
54:15 | three of these containers. Uh The has the same length for all of |
|
54:21 | containers, but you can see the of fluid is different. So this |
|
54:26 | the greatest volume. This is the volume. And so this is why |
|
54:31 | vessel is the heaviest, which container the highest pressure at the base. |
|
54:42 | the answer is they're all exactly the . On the other hand, if |
|
54:51 | put if I put these rested these on you, if you were laying |
|
54:57 | , I mean if we were truly to face, we could do an |
|
55:02 | where I could have tubs of different and I could have a hose and |
|
55:06 | them with water and place them on stomach. Which of these is going |
|
55:12 | exert the greatest force on your Obviously it's this one. Right, |
|
55:21 | , had what is the hydrostatic paradox ? How is it that this one |
|
55:29 | exerts the greatest force on you. the pressure at the bottom is exactly |
|
55:34 | same in all three. And the is the base of the container makes |
|
55:41 | big difference. If you're underneath the you feel the full weight of the |
|
55:48 | . If you're above the base. only feel the the pressure of the |
|
55:55 | which has to do only with the level, not the amount of |
|
56:00 | So you're essentially at the same death you're feeling very different pressures. And |
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56:06 | key is this base is impermeable right , put yourself in the earth. |
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56:14 | I'm the need the base say this an impermeable shell. If I'm beneath |
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56:24 | base, I'm feeling the weight of entire vessel. If I'm above the |
|
56:31 | uh the impervious layer, I'm only the column of water above me, |
|
56:43 | . So, uh can you imagine situations where this might result in a |
|
56:50 | change of pressure beneath the impermeable I'm feeling far more pressure than immediately |
|
57:01 | . You could say beneath the impermeable . I'm uh feeling the entire |
|
57:07 | a static load, the weight of above me. Whereas above the impermeable |
|
57:14 | , I'm only if all my fluids imperfect communication, I would only be |
|
57:21 | row G. H. Okay, we're going to assume that the overburden |
|
57:32 | is hydrostatic. So the poor is the same pressure in all directions. |
|
57:43 | poor pressure is pushing out. And we are in equilibrium then uh |
|
57:51 | These forces have to balance if the pressure is bigger than the poor |
|
58:00 | that poor is going to want to . So there's a pressure being applied |
|
58:06 | that for and how much it closes depend on the material the solid material |
|
58:14 | the poor some material will allow that to compress very easily. Other material |
|
58:20 | so strong that it won't allow the to compress compress at all. So |
|
58:25 | will be some poor volume reduction which going to depend on the module lists |
|
58:30 | the solid material outside the poor and module lists of the material inside the |
|
58:38 | . Now, if I have a pour, it also depends on the |
|
58:42 | shape. So in the case of sphere is the uh is going to |
|
58:47 | the compression the most. But if up a flat poor then the fluid |
|
58:53 | that platform is definitely going to be and is going to have to help |
|
58:58 | the compression. So in that case a flat pour it matters what type |
|
59:03 | fluid is in the poor. If have gas in the portal close more |
|
59:09 | than if I have water in the that can't get out right. So |
|
59:14 | that water is confined I'm gonna as poor compresses is going to try to |
|
59:21 | the water. Um So if there's gas in that poor and the poor |
|
59:27 | compressing the gas would accommodate most of compression. Okay, So uh we |
|
59:38 | the overburden uh with a static load creating an overburden pressure. And we |
|
59:46 | call that confining pressure in the laboratory a confining pressure which is usually applied |
|
59:54 | placing the sample in an oil bath some kind and the pressure in that |
|
60:01 | is increased um Now we calculate the pressure from the weight of the overlying |
|
60:12 | fluid column. So that way it depend on the density of the rock |
|
60:19 | fluid together. So it depends on total weight above you. And that's |
|
60:25 | on the order of £1 per square for foot. And with the conversions |
|
60:31 | can convert that to to give the per meter. But it's convenient to |
|
60:39 | in terms of one PC for that's an easy thing to remember. |
|
60:44 | , it's not exactly one pc per . It depends on the density of |
|
60:49 | rock fluid column so that will vary we'll see in an exercise how that |
|
60:55 | vary. And again the effective pressure assumed to be hydrostatic. In other |
|
61:02 | it's equal in all directions. There also be tectonic stresses supply. So |
|
61:09 | it would not be the confining pressure not be equal in all directions. |
|
61:16 | That's given a lot of consideration in mechanics. So if you go to |
|
61:21 | Mechanics laboratory, they have what are tri axial cells where they could bury |
|
61:27 | stress in different directions in rock physics normally dealing with confining pressures. Uh |
|
61:38 | pore pressure as we said, is pressure pushing out and if it's normal |
|
61:44 | pressure, that is the fluid pressure from the weight of the overlying fluid |
|
61:49 | the pore space. So when I row G. H. Is not |
|
61:55 | of the rock, it's row of overlying fluid. So the average density |
|
62:01 | the overlying fluid. Now, normal pressure Is on the order of .465C |
|
62:11 | what it is, depends on the densities, right? So it depends |
|
62:16 | uh the salinity of the fluid, depends on temperature, it depends on |
|
62:23 | fluid saturation But typically .465 pc So any poor pressure greater than that |
|
62:32 | called overpressure or geo pressure. And I said, if you're underneath an |
|
62:39 | layer, uh you could have significantly pressure because you're now bearing the weight |
|
62:47 | all the material above you. Uh just the weight of the poor |
|
62:54 | Now, the effective pressure is a assumed to be equal to the differential |
|
63:04 | , which is the difference between the and the fluid pressure. Uh That's |
|
63:11 | always the case. Uh Often you see effective effective pressure on a graph |
|
63:19 | rock physics measurements when in fact it's differential pressure. And I like to |
|
63:27 | the difference between these two because the of pressure is not necessarily equal to |
|
63:33 | differential pressure as we'll see. so it's the differential pressure which is |
|
63:44 | difference between the overburden and the a pressure. Okay, so now as |
|
63:51 | pressure up, Iraq here we have wave velocity here we have shear wave |
|
63:58 | as I increase the pressure and that's cut off. Let's see if I |
|
64:04 | . Um Yeah, so you can the whole slide down um In this |
|
64:10 | the shear wave velocity seems to be flattening out before the p wave |
|
64:17 | but both is showing the tendency of increase with pressure, a rapid increase |
|
64:24 | low pressure and then leveling off at pressures. If you just plot uh |
|
64:34 | vs stress versus the pressure and again is differential pressure. Um You tend |
|
64:42 | have a a greater strain for a change in effective pressure. Uh Given |
|
64:53 | in differential pressure, uh things strain a higher rate until you level off |
|
64:58 | then you have a a slower change strength with increasing pressure. Again, |
|
65:12 | first order, assuming effective pressure is to differential pressure. You could look |
|
65:18 | effective pressure versus death, assuming it's to the differential pressure. So you |
|
65:24 | calculate the overburden pressure versus death from density of the rocks and the poor |
|
65:31 | versus depth from the density of the . These would be perfectly straight |
|
65:36 | If your density was constant all the to the surface. Uh If there |
|
65:42 | the density is changing with death then curve is going to change. It's |
|
65:49 | going to be a perfect straight But you have the overburden pressure at |
|
65:54 | given depth, you have the four at a given depth and the differential |
|
65:59 | is the difference between us now on at the surface you have zero weight |
|
66:14 | overlying rock. I mean, you want to include the atmosphere but we |
|
66:18 | ignore that way. So at the you have zero pressure. On the |
|
66:25 | hand, uh if we're offshore uh the water bottom uh above the water |
|
66:34 | , we have no uh rock. we have no contribution from the |
|
66:39 | So above the the ocean bottom, we are just the weight of the |
|
66:47 | fluids which continues as we go Right? So this is the weight |
|
66:54 | the fluids in the four space plus weight of the fluid layer layer on |
|
67:01 | . Whereas at the at the ocean , uh we now start adding the |
|
67:07 | to brock. So now we the have an increased density above you. |
|
67:16 | so things offshore you would for the debt rock density. You would you |
|
67:21 | parallel the on shore line and you deviate from the hydrostatic pressure. But |
|
67:26 | at the ocean bottom lip, the and the hydrostatic pressure will be the |
|
67:32 | . So you can see that if have an increasing density, this is |
|
67:35 | extreme example of it. But compacting will do the same thing. You |
|
67:41 | a flattening of the curve here, ? Where you have a greater increase |
|
67:47 | pressure with death as you get So we have a concave upwards uh |
|
68:02 | . Okay, so here's another example increasing and decreasing pressure. Uh Again |
|
68:12 | is um the effective pressure is really reported as effective pressure but it's really |
|
68:21 | differential pressure and what it's showing in case I'm pressuring up, I'm pressuring |
|
68:28 | and pressure down higher velocities. Um this is by the way the pressuring |
|
68:46 | and pressuring down is just by varying poor pressure. Okay so here I |
|
68:54 | zero pore pressure. Here I have higher pore pressure and you can see |
|
69:00 | it's not exactly um equivalent right? differential pressure is the same in both |
|
69:09 | but the effective pressure is different is . This could be a history suspect |
|
69:16 | in this case or it could be a deviation from the effective pressure law |
|
69:22 | . And from this data alone we know if it's uh due to history |
|
69:29 | or it's a due to deviation from stress law. So in fact the |
|
69:37 | effective pressure uh we need uh an factor here. So whereas the differential |
|
69:46 | is the confining pressure minus the four . The effective pressure is the confining |
|
69:53 | minus some constant times the poor Or let's say some scalar, I |
|
70:00 | know how constant it is but let's it a scalar value now and is |
|
70:06 | close to one but it's not necessarily to one. Uh Just for your |
|
70:18 | we have a conversion table for units and this is a good time to |
|
70:25 | an exercise. So, uh so fought the overburden pressure versus death and |
|
70:38 | Using uh one C per foot and what that and plotted in giga pascal's |
|
70:48 | see what that plot looks like. think you can guess just looking at |
|
70:53 | question that is going to be a simple plot. But go ahead and |
|
70:57 | it and I'll stop recording while you're you're doing that. This conference will |
|
71:03 | be recorded. So just to So it's on the recording, the |
|
71:11 | to given death is equal to the density down to that death. So |
|
71:16 | average of all the dead cities above times the acceleration due to gravity, |
|
71:22 | the depth your act. And uh have the units for acceleration due to |
|
71:28 | here. Similarly poor pressure is is the weight of the overlying or |
|
71:37 | average density above you times acceleration due gravity times the height and this one |
|
71:47 | think we can go full screen So, these are some notes from |
|
71:55 | Mapco. We just retired from stanford was the head of their Iraq physics |
|
72:02 | project there for many years. Um ways that poor pressure impacts velocities. |
|
72:11 | I increase the poor pressure, I the compressibility and rigidity of the rock |
|
72:19 | by opening up cracks and pushing grains and that will lower the velocities, |
|
72:28 | increasing the poor pressure tends to make pore fluids in the rock less |
|
72:39 | you know, if I have a and I put that gas under |
|
72:43 | I'm forcing the molecules closer together. means they're harder to push together. |
|
72:49 | I'm making the port fluid more Excuse me, less compressible as I |
|
72:56 | the pressure and that will tend to the philosophy. So, these are |
|
73:02 | effects. The first effect is usually than the second effect. Uh |
|
73:09 | if I have a fluid mixture, the poor pressure can also change the |
|
73:15 | uh as gas can go in and of solution, especially if I have |
|
73:20 | gas oil mixture. Uh If I the pressure, I could go above |
|
73:26 | bubble point and I could dissolve all gas in the oil and that could |
|
73:31 | the velocities to increase also. Um the poor pressure is existing over geological |
|
73:43 | , that could result in dire genetic . Um in sand stones that can |
|
73:50 | die genesis and preserve ferocity. On other hand, it shells that could |
|
73:57 | uh it could result in de uh etcetera. No, I'm |
|
74:03 | the high pore pressure, high confining would result in uh the water in |
|
74:09 | pore pressure. I would push the apart. Okay, so here we |
|
74:17 | a bunch of measurements on Shelly sand that are supposedly dry. Yeah. |
|
74:27 | , uh we don't know to what they've been drive. We don't know |
|
74:31 | they they've been oven dried or if room dried, but they're not fully |
|
74:38 | let's say with water. And uh individual individual laboratory measurements uh you see |
|
74:50 | both modules change and a significant ferocity . And so this suite of measurements |
|
74:57 | as we're changing the pressure. so at low pressure we would have |
|
75:04 | porosity, low bulk modules, increase pressure. We reduce the ferocity. |
|
75:11 | in shale, you're going to get porosity reduction than in the sandstone or |
|
75:17 | if you have a strong solid uh It's hard to reduce the porosity |
|
75:23 | much but in a shell with a compressible matrix and with micro porosity and |
|
75:29 | forth, it's easy to reduce the by increasing the pressure. Okay, |
|
75:41 | we were looking at a velocity versus , uh the facts um so we |
|
75:53 | a high pressure, our philosophies level . Uh we won't get all the |
|
75:59 | to the mineral velocity because we have remnant ferocity. We don't close all |
|
76:06 | pores. So how close you get the mineral velocity is an indication of |
|
76:14 | ferocity. Uh huh. The change velocity uh is an indication of the |
|
76:25 | of soft, close herbal ferocity you . So as I'm increasing the differential |
|
76:32 | , cracks are closing or pores are , how long it takes you to |
|
76:39 | off is an indication of the crack . So the very flat poor is |
|
76:48 | close uh with a small pressure improvement as we go to higher and higher |
|
76:56 | , what you have remaining are the and rounder pours until you get to |
|
77:02 | point where you have only the very pours left now uh fracture pressure is |
|
77:16 | engineering concept. It's the it's the way you have to use in order |
|
77:23 | fracture the formation around the well So the drilling mud weight is usually |
|
77:31 | higher and high enough to counteract the pore pressure. If I drill into |
|
77:40 | geo pressure brock, if I were with just water, uh remember the |
|
77:47 | pressure in the rock is much higher row G. H. In the |
|
77:51 | bore. And so uh the fluids the formation can burst out of the |
|
77:58 | and you could have what is called blowout. And these can be very |
|
78:03 | if you have hydrocarbons associated, you lots of friction going on blow gas |
|
78:09 | of the well bore. And it ignite especially as you get to the |
|
78:16 | . Uh So you have to be about this. Um So you have |
|
78:23 | have your mud weight fire than the pressure. But if the mud weight |
|
78:27 | too high, that makes trillion more . You know, you've got that |
|
78:34 | is heavy and it wants to stay it is. You have to move |
|
78:37 | with the drill bit so it slows trilling, It also gives you more |
|
78:44 | into the formation, which is undesirable you may push hydrocarbons away from the |
|
78:52 | and you may never even know there hydrocarbons there. But the other thing |
|
78:57 | can happen is you can fracture the and then the formation starts to eat |
|
79:02 | drilling fluid and you have a loss fluids in that case, which is |
|
79:08 | expensive proposition and causes drilling problems. uh you keep the mud way as |
|
79:16 | as possible to avoid blowouts but low such that you don't fracture the |
|
79:24 | In fact, when we in hydraulic for intentionally, for stimulation to improve |
|
79:33 | permeability of the formation, we do on purpose, but that's under controlled |
|
79:40 | . We don't want to do that and down the bore hole. And |
|
79:43 | especially don't want to do that uh in in formations above our reservoir. |
|
79:54 | uh and important you to application of physics is to try to design the |
|
80:01 | program correctly, to be able to the drilling engineers based on what we |
|
80:07 | about the rocks, how high should poor pressures be and how high do |
|
80:13 | not want them to get? So causes these abnormally high pore pressures? |
|
80:25 | , we talked about an impermeable cap pressures from a quick liberating vertically. |
|
80:34 | We talked about the weight of the rocks. Remember the hydrostatic paradox |
|
80:40 | slightly below the impermeable layer. The can't get out and they are experiencing |
|
80:46 | weight of the little static load above . So that causes the poor pressure |
|
80:52 | increase another cause of high pore pressures fluids are trapped and can't get |
|
80:58 | Is aqua thermal pressuring. So as get deeper you get hotter. And |
|
81:04 | the fluids want to expand. Uh if they can't get out they can |
|
81:10 | the molecules get pushed closer together and increases the pressure. Uh If I |
|
81:18 | trapped fluids that can escape, if have abnormally high tectonic stresses that could |
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81:25 | the fluids and caused the poor pressure increase, I could also add more |
|
81:35 | to the poor space by the By taking water out of minerals. |
|
81:42 | are two ways that water is and in clay's, it could be trapped |
|
81:48 | the crystal lattice non stoking symmetrically. , as I compress that crystal |
|
81:54 | I could force the water out of crystal. But there could also be |
|
82:00 | transformations where I have bonded by drops . I could force I could have |
|
82:07 | diabetic reaction where water is generated. that will also increase the poor pressure |
|
82:16 | if the fluids are not free to . And similarly, if I generate |
|
82:22 | , so I have solid organic material I start cooking that solid organic |
|
82:28 | I will generate hydrocarbons that will be into the pore space. And if |
|
82:33 | can't get out they'll create an abnormally pressure as well. Let's say it's |
|
82:44 | for a Short break. So let's at a quarter after 10. This |
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82:56 | will now be recorded. Yeah Now mentioned previously that the pressure gradient is |
|
83:05 | change in pressure with the change in . Um So if I have a |
|
83:12 | versus death curve from a scientific point view it would be the derivative of |
|
83:19 | curve. Right? So it would the tangent line at any and any |
|
83:27 | . But that's not the way When engineers talk about pressure gradient they |
|
83:34 | something else. Uh It's not the of pressure with death. It's the |
|
83:41 | divided by the depth. Um Why divided by depth mm Because the engineers |
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83:54 | to know how heavy their mud should and how heavy their mud should be |
|
84:00 | equal the formation pressure is the pressure by the death. Remember it's row |
|
84:08 | . H. Pressure is equal to G. H. So pressure divided |
|
84:16 | h. Is equal to rho Right so the pressure gradient tells them |
|
84:26 | what density there mud drilling mud needs be in order to balance the formation |
|
84:37 | . Mhm. So if you plot an engineer's point of view uh pressure |
|
84:47 | death. Uh huh. What you or pressured radiant versus death as you |
|
84:57 | a an increasing pressure gradient gradient with suggesting lower rows lower densities shallow which |
|
85:08 | sense. And as you get deeper the pressure gradient uh The pressure berries |
|
85:16 | slowly with death. And um older have a higher density. So they |
|
85:28 | a higher pressure gradient than younger Yeah. So this increase in pressure |
|
85:36 | with death has to do with the increasing density with death. All |
|
85:46 | And then just another table relating different . Okay, so now we're going |
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86:01 | do an exercise which is going to some time. So I'm going to |
|
86:07 | recording. And what we're gonna do uh we have a table of measurements |
|
86:14 | a table of empirical fits density versus trends. And we're going to convert |
|
86:22 | into pressure versus death. Um uh we applaud density versus staff average |
|
86:32 | versus that. That's the average density all the rocks above you. The |
|
86:39 | stress versus death. The true pressure , which is the derivative of the |
|
86:49 | the change of stress with the change death and depth divided by I mean |
|
86:56 | divided by depth versus death. this is the engineering pressure gradient. |
|
87:01 | true pressure gradient. So lots of . The plots hit plot here. |
|
87:08 | so this is gonna take a So, I'm going to stop |
|
87:13 | And I would suggest that the original for show me for the first |
|
87:23 | Each of these plots. And then would be a simple matter to do |
|
87:26 | for other curves. Right? as you get results for the first |
|
87:33 | , show me, show me the . Uh Show me each of these |
|
87:37 | you get them. All right. , I'm going to stop here. |
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87:41 | conference will now be recorded. And see this. I would say in |
|
87:52 | measurements. Remember we talked about things off the velocity, leveling off. |
|
87:58 | here we have cracks closing and now have leveled up. So you could |
|
88:03 | trends to these curves. And uh you could get a relationship between velocity |
|
88:11 | pressure, right? And uh and you could for example, with a |
|
88:19 | like that where you have the velocity by the high pressure velocity than can |
|
88:27 | expressed as a function of pressure. filling an exponential curve given the |
|
88:34 | you could calculate the pressure. So the question I have is should core |
|
88:42 | be used to determine the instant C velocity versus pressure. In other |
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88:48 | will rocks in the earth. The this expression that you've determined in the |
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89:02 | . Mm. So Exactly right. as I corps, as I drill |
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89:10 | I corps, I'm going to be the rock. That chorus had all |
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89:15 | of torture channel stress on it and worse than that. It's got stress |
|
89:23 | . You bring that court to the , you take it out of the |
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89:26 | barrel and you've relieved the pressure on thing. In fact on the drilling |
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89:32 | , you could sometimes see these cores right in front of your eyes. |
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89:39 | you're changing the core right now you that core, put it in the |
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89:47 | and you pressure it up and you're a lot of the damage to the |
|
89:53 | . So here look at that. almost a doubling of velocity from note |
|
90:00 | pressure to high pressure. What you've is you remove the cord a lot |
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90:06 | the core damage as well as any fractures in Iraq or low aspect ratio |
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90:14 | in Iraq. But I think given massive velocity difference, I think you |
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90:20 | guess that most of that is core which is being uh fixed. So |
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90:27 | very careful about Using laboratory derived pressure and using those in c. |
|
90:42 | Now again this is differential pressure. even my papers, I've been guilty |
|
90:50 | using effective pressure instead of differential So this was a paper where we |
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90:57 | suggesting using the PBS ratios to find high pore pressures. Be PBS ratios |
|
91:05 | be determined seismically with greater resolution then V. P. Or V. |
|
91:13 | . So here was an empirical trend the red in the black curve. |
|
91:19 | the red curve was a laboratory laboratory . And uh you can see the |
|
91:27 | in V. PBS ratio becomes very . We're seeing BP Ds ratios that |
|
91:33 | extremely high compared to liquefied rocks had low and very low pressures. And |
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91:45 | this was the example I showed This is this is the inverted of |
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91:50 | PBS ratio by simultaneously inverting PP data PSV data acquired with ocean bottom |
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92:02 | So we have B. PBS ratios approaching seven. Uh in the very |
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92:10 | rocks as we get deeper we have and lift ification and the B. |
|
92:18 | ratios are decreasing. So you see compaction trend in the V. |
|
92:23 | V. S. Operations. Uh uh This is a priest like amplitude |
|
92:32 | in virgin or it has nothing to with with with with the empathy of |
|
92:36 | data. Just purely velocity work. now it's uh it has to do |
|
92:41 | the with the velocity velocity in this with the priest. Let me take |
|
92:50 | back. This is using um Yeah right. It has nothing to do |
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92:58 | the HBO at this point with inverting p wave impedance and inverting for shear |
|
93:06 | impedance and taking that ratio. Okay so this is yes the B. |
|
93:17 | . B. S ratio. But actually the ratio of the E. |
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93:20 | and penis to shear wave in And so here we have high |
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93:25 | PBS ratios as we approach the water . Uh But down here we have |
|
93:31 | layer with relative to the rocks around . With a very high V. |
|
93:36 | . V. S ratio. Normally would expect that to be a geo |
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93:41 | shell. But in fact these are pressured sands. Um It's the stands |
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93:50 | with very high pore pressures get very B. P. V. S |
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93:54 | . Like in this slide here if v. PBS ratios well over six |
|
94:06 | into seven right now. So you look at the difference between if you |
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94:11 | the normal compaction trend of the P. V. S ratio and |
|
94:16 | subtract that uh from this there you your anomalous li hai the PBS |
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94:26 | You're anomalous li lo be PBS ratios to be sands, you're anomalous lee |
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94:32 | tend to be your shells. And anonymously hy vee PVS ratio is an |
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94:38 | pressured sand. And that was, I mentioned last time, that's where |
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94:43 | had a shallow water flow. But is how we got there. |
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94:52 | that's the end of our pressure Are there any questions on that? |
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94:57 | , I move on to what we've uh building up towards which is seismic |
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95:14 | . There are no questions. I'll on. Oh I should be |
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95:19 | Yeah. The lecture slides for this an open blood body here. |
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95:25 | was it not? Okay, I know for a fact. So what |
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95:31 | do then is we'll take a quick and I'll quickly put them onto |
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95:38 | So let me do that. This conference will now be recorded. |
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95:50 | , You'll remember from Jeff physics one we have two types of velocities, |
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95:59 | shear waves and p waves. Two of body waves for share waves. |
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96:05 | have a transverse wave and the analogy if I have a string attached to |
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96:14 | wall. For example. Uh professor we got the blank screen probably |
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96:21 | Shit, I'll stop the recording This conference will now be recorded. |
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96:29 | , So, uh I don't know you were a kid. Maybe you |
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96:33 | jump rope? Actually. Uh we to do that with the girls in |
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96:37 | neighborhood. We would play jump We attach a rope to the |
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96:42 | I mean to a wall and we flying up and down motion on the |
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96:49 | . And that broke with produce an . All right. So uh the |
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96:57 | displacement of the rope is left right this in this image, but the |
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97:05 | is moving vertically. So the displacement trans verse to the direction of |
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97:13 | On the other hand, if I a spring and I pushed on |
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97:18 | spring on one end, that spring move along the length. Uh and |
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97:26 | compression would then be a longitudinal compression moves through the spring. And that |
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97:34 | would be associated with a rare faction what is stretching only uh other end |
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97:41 | the strengths. As I'm moving in out, I'll have a compression, |
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97:46 | faction, etcetera. They are the of the spring. You know, |
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97:51 | guys have come to have relative to guys. The displacement is longitudinal. |
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97:58 | this is the analogy to compression. waves. And this this is the |
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98:03 | to share waves. So now we're to look at the waves propagating through |
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98:11 | body, a solid body. And going to divide this body up into |
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98:18 | testimonial volume elements. All right, these are these little cubes here. |
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98:25 | before any deformation there were all the size and they're in a regular |
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98:30 | So now if I push this parallel it, if I push it on |
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98:36 | side, that compression will move through rock. So I'm pushing and |
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98:42 | So I have compression moving through the and rare factions uh which we refer |
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98:49 | as debilitation case that we have compressions village stations. Now look carefully at |
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98:58 | volume elements. You notice that the width of the volume elements, whether |
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99:05 | being compressed or stretched the width that that doesn't change right. The width |
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99:13 | doesn't change only the length along the changes. So the mind elements are |
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99:20 | shape and they're changing in body. These compressed funds are smaller volume than |
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99:32 | . The reason they don't the volume don't get fatter trans verse to the |
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99:38 | of propagation is because they have adjacent that are else. Also trying to |
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99:44 | Uh huh better and can't because the are pushing against each other. So |
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99:52 | these volume elements are being constrained trans to the direction of propagation. So |
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100:01 | elastic module is controlling the relationship between and strain in these following elements is |
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100:08 | the plane wave module. Escape was 13. That's why in the p |
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100:15 | velocity equation is square root of Cape four thirds view of arrow square root |
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100:21 | em over row now share waves are different here. The displacement is transferred |
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100:32 | to the direction of propagation and sometimes being displaced upwards, sometimes you're being |
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100:40 | downwards and the result is it change the shape of the volume element. |
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100:47 | changes the shape but not, you , it's strata graphic thickness. So |
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100:53 | fact the volume of these volume elements change only the shape. And that's |
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101:02 | shear waves don't depend on the boat . They don't depend on the ratio |
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101:08 | biometric stress to biometric. Strange, only depend on the ratio of shear |
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101:15 | to shear strength. So uh shear have no volume change associated with. |
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101:24 | can see that if I if I a point in the middle of the |
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101:29 | element as time passes. Sometimes this be a rhombus where the apex on |
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101:36 | right side is up and the left is down. And sometimes as this |
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101:42 | passes it will be the other way love side is the right side of |
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101:46 | camp. So that's why shear waves called rotational waves because it's a rotation |
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101:53 | the shape of that volume element as the way passes. So this is |
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102:05 | the same thing. But at different in time. And now we can |
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102:12 | on one particular volume element, as wave passes. Remember the wave as |
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102:20 | associated with it. And it has factions or debilitation associated with it. |
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102:27 | these compressions and rare fractions are moving the rock as a function of |
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102:33 | you see that. So any one volume element maybe uh stretched at a |
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102:43 | time. So here it's being stretched it could be squeezed here, it's |
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102:48 | squeezed. So that volume element is experiencing a volumetric metric compression and a |
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103:02 | in shape. However, for the wave, the volume of that volume |
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103:08 | is staying the same and all that's is rotation around the share with. |
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103:14 | this difference in behavior greatly affects the fluids in the rock behavior. Now |
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103:23 | a porous rock. And we're going call that a poor oh elastic medium |
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103:30 | the pores are connected and fluids can through the pore space. What we |
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103:37 | with the compression all wave as we while one buying element is being |
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103:45 | another volume element is being compressed. did we say happens when we increase |
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103:51 | pressure on a fluid? It's going want to move to low pressure. |
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103:55 | the poor pressure is high here, low there. That fluid is being |
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104:01 | to move to the to the into the right. You see that |
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104:08 | it's a fluid movement in the direction propagation, right. Either to the |
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104:15 | or to the right, from the pressure volume elements to the low pressure |
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104:22 | elements. On the other hand, at a different time, the volume |
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104:31 | here is now being stretched. So in here and here are one are |
|
104:38 | told to move back to that volume . Now, if this is a |
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104:44 | low frequency wave and the rock is , or and or the rock is |
|
104:51 | , the fluid will have plenty of to move. So the fluid here |
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104:57 | all the way there and then at time it is time to move all |
|
105:02 | way back. But think about if a very um high frequency way or |
|
105:10 | a very low permeability such that the rate is very low. In that |
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105:16 | the fluid doesn't have time to make . The fluid here. The fluid |
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105:22 | is being told to move there, before it has a chance to move |
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105:26 | far, it's being told to move to where it was. So it's |
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105:33 | high frequency. That fluid is essentially being kept in place it vibrates, |
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105:41 | it never gets to go very So uh this is uh what we |
|
105:48 | call B. O. Flow. this is uh we also refer to |
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105:53 | as sloshing type of flow. It's to the size of of a given |
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106:00 | element. It's a very long distance travel which can be achieved at low |
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106:07 | or very high permeability ease or can't achieved at high frequencies. Uh So |
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106:15 | call that B. O. He was the physicist who was working |
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106:19 | a consultant, Michelle in the 19 , who developed the theory that we |
|
106:25 | to this day. On the end other hand, look at the shear |
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106:32 | , the shear waves, there is pressure differential between volume elements. So |
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106:39 | pressure differentials must be very local. , let's talk about local flow as |
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106:47 | deforming the rock, we're changing its . So that means we're going to |
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106:53 | deforming the poor space. The pores changing the shape, their shape and |
|
106:59 | pores will be preferentially closed and others be preferentially open depending on their |
|
107:06 | So for his closing will squirt fluid , essentially induce a poor a local |
|
107:14 | pressure gradient from the closing pour to open pore. So that's what we |
|
107:21 | local flow. And both p waves she waves exhibit local 12 P waves |
|
107:33 | the longer range flow generally involved more , solid movement or movement between fluids |
|
107:41 | solids and therefore more friction between fluids solids. So, p waves |
|
107:47 | you have higher absorption, higher frequency continuation. Both are affected by local |
|
107:56 | but only p ways are affected by long distance flow. Alright now we |
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108:08 | this idea before that there is a between the physical properties of Iraq, |
|
108:14 | as length. Ology ferocity pore, permeability, also the environmental conditions and |
|
108:23 | elastic properties of Iraq, which we geophysical properties. Both modules. Sarin |
|
108:29 | rigidity and density. Uh These elastic affect the seismic or acoustic properties. |
|
108:39 | wave velocity shear wave velocity P wave . This is the quality factor. |
|
108:46 | a measure of attenuation and share wave facts. And it's the three dimensional |
|
108:53 | of these things which results in the response. And we have a come |
|
109:03 | to our velocity equations which I really you to have memorized. And the |
|
109:12 | equations show the relationship between the elastic I these are for ice, a |
|
109:18 | rocks and the velocities. Now I'm to ask you, what do you |
|
109:25 | to happen if I replace the brine Iraq or the water in Iraq if |
|
109:34 | replace it with hair or gas, going to happen to V. |
|
109:39 | M. V. S and So everything else is the same. |
|
109:52 | have the same rock frame, same . I'm just taking out some of |
|
109:57 | water and I'm replacing it with a of some kind. What's going to |
|
110:04 | to these different quantities. And so going to happen to DP NBS awake |
|
110:10 | you to answer V. S. remain the same. I'm sorry, |
|
110:20 | sorry. I'm sorry. I'm The effect of the density will will |
|
110:24 | the Yes. Right. So the stays the same. The density drops |
|
110:33 | will go up. Yeah. What BP? Um It's a bit more |
|
110:39 | because then we have two very key density. Uh huh. I think |
|
110:46 | effect of the dynasty at the beginning would be big but then the effect |
|
110:54 | the bulk would take over. I looking at that curve from jasmine |
|
111:01 | substitution and uh it was showing variation both but each one was limited to |
|
111:07 | certain gas situation I guess. if I add just a few bubbles |
|
111:13 | gas, am I going to change density very much now? But if |
|
111:20 | add a few bubbles of gas from equation, because it's a reciprocal |
|
111:26 | I'll reduce the both modules of the . And if the rock frame is |
|
111:32 | , the rock frame, uh both will decrease. So the effect of |
|
111:39 | , the initial edition of gas is leave rigidity unchanged, reduce the both |
|
111:48 | lists and reduce the density but reduce bulk module, it's more so the |
|
111:54 | few percent of gas, reduce the . Uh huh. Now, as |
|
112:00 | continue to add gas, the bulk is that the fluid won't change very |
|
112:07 | the fluid that the gases so that it doesn't matter how much I |
|
112:12 | just a few percent of gas and all of the compression. So as |
|
112:18 | continue to add gas, the bulk , that the fluid doesn't change very |
|
112:23 | . So, the bulk modules of rock doesn't change very much but the |
|
112:28 | continues to go down linearly with the saturation. So the effect then after |
|
112:35 | initial drop in velocity. When I a little bit of gas, I |
|
112:39 | more gas in the p wave velocity up. We're gonna be talking about |
|
112:47 | substitution at great length So we're going come back to this idea. Okay |
|
112:58 | in the laboratory in the old days start record our acoustic wave forms that |
|
113:07 | pass through the rock. We start look at these on in a silla |
|
113:14 | and before we digitally recorded them we take pictures or in fact just read |
|
113:20 | off the scope. What the arrival of the wave form is. So |
|
113:25 | is still a scope is measuring the of these transducers. We have a |
|
113:33 | generator. It generates a pulse that trigger the transducer to deform and therefore |
|
113:43 | a wave through the sample. We another transducer which will respond to the |
|
113:51 | defamation. So it will deform and a voltage or current which will be |
|
113:59 | and sent to an a silla At the same time we send a |
|
114:05 | directly to the oscilloscope. So we where, you know, we know |
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114:11 | at what time the post was generated that scene on the oscilloscope and then |
|
114:17 | could see when the host that has through the sample when that arrives and |
|
114:24 | its arrival time and knowing the length the sample, we could measure the |
|
114:30 | . You can imagine that there are lot of complications in this process. |
|
114:36 | lot of possible sources of error. , this is a dex desktop measurement |
|
114:43 | by the way before covid in the learning center we actually had desktop example |
|
114:56 | making these measurements, students could actually and do it themselves. It gets |
|
115:02 | it's very easy to do on the . Um And of course we don't |
|
115:07 | it to sell a scope. We the PC to collect the wave forms |
|
115:12 | then we could digitally measure the arrival . Um But so doing this on |
|
115:20 | a desktop is fine but that's not of in C2 conditions. So this |
|
115:27 | has to be put in a pressure and that's when things start getting very |
|
115:33 | and very complicated. We put the in in the vessel, we have |
|
115:39 | jacket the sample because the pressure is transmitted through a fluid. So we |
|
115:46 | want that fluid at the confining We don't want that fluid getting into |
|
115:50 | sample. So the sample is jacketed that starts making uh starts making life |
|
115:57 | difficult. That keep in mind the of this must be such that we're |
|
116:05 | getting guided waves dominating through the Right? We want to transmit a |
|
116:11 | wave through the sample without interference you know, multiples off the sides |
|
116:18 | the sample and other things indirect travel . Right? We want so we're |
|
116:24 | to want the measurement to be very frequency such that the direct wave can |
|
116:31 | cleanly at the transducer on the other of the sample. So these wavelengths |
|
116:38 | have to be very short compared to sample. If the wavelength of the |
|
116:45 | were very long, then we would a guided way through the sample analogous |
|
116:50 | surface wave. Right? So uh we don't want that. And so |
|
116:58 | have here is an example of a picture of an acela scope waveform. |
|
117:04 | This happens to be a digital oscilloscope the time. And so uh mm |
|
117:11 | measuring amplitudes at even time increments. why it started there. But here's |
|
117:19 | trigger. And you notice there's a frequency noise associated with the trigger and |
|
117:26 | there's high frequency noise before this Have this high frequency noise is uh |
|
117:35 | might be, for example using shear transducers. These might be p waves |
|
117:41 | got there before the shear wave. so a p wave arriving before the |
|
117:47 | way that the p waves are very . They can interfere with your arrival |
|
117:54 | . Now think about this. If measuring the velocity of this way, |
|
117:59 | just measuring the velocity at one source facing right. It's the velocity at |
|
118:09 | spacey for the length of the Um Can you see an inherent area |
|
118:19 | ? Where do I pick the onset the way for where where is the |
|
118:26 | arrival time at the wave form? it? Uh The first trap here |
|
118:32 | the first peak here? Or do have to extrapolate back into the noise |
|
118:39 | figure out precisely where the first arrival is. So anyway, there is |
|
118:44 | uncertainty in that arrival time. Also I'm pressuring the sample up, I |
|
118:52 | be changing its length. So I to be monitoring the length to get |
|
118:58 | velocity right yet at every pressure. um so in fact there is error |
|
119:09 | with making these measurements and the more the rock is the week or my |
|
119:15 | forms are the more error there is with detecting the way for. It |
|
119:21 | be nice if we could measure the time difference across two receivers. Those |
|
119:27 | generally much more accurate than just measuring arrival time. Okay, so how |
|
119:38 | and precise our laboratory measurements and so need to distinguish between what we mean |
|
119:45 | accurate and what we mean by precise means how correct is the measurement in |
|
119:55 | terms. So I have a true velocity of the rock. What is |
|
120:01 | measured velocity? And how different is from the true intrinsic velocity. That's |
|
120:08 | accuracy of the measurement precision means, repeatable is the measurement? You could |
|
120:16 | precisely wrong but hit the same answer . So uh you know, to |
|
120:23 | extent that uh you know, picking first arrival depends on the noise. |
|
120:29 | might be an indication of precision. if there is bias in the |
|
120:34 | like I'm always picking too late in waning form or something like that, |
|
120:38 | affects the accuracy of the measure. The other thing that affects the accuracy |
|
120:44 | the measurement. And is the biggest in core measurements is a how representative |
|
120:52 | that rock sample after you've acquired it shaped it and put it in your |
|
120:59 | apparatus and maybe had variations and stress it before this particular measurement. The |
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121:10 | then of the rock physics measurements is much in question When comparing them to |
|
121:16 | c. two measures. Also keep mind that there are sampling differences. |
|
121:21 | are resolution differences. Sampling can be by your ability to actually acquire a |
|
121:30 | and shape the core into a If the rock is highly fractured you |
|
121:34 | lose the core. If it's very , you may lose the core. |
|
121:41 | and if you have a mixture of uh rocks that have high integrity versus |
|
121:49 | that won't be cord well will be in the court. Then your measurements |
|
121:53 | biased towards those samples with high So there are all kinds of reasons |
|
122:02 | we we have reason to suspect the of the rock physics measurements. Usually |
|
122:09 | are more precise than accurate. If the case then how are they |
|
122:16 | Why do we bother to make measurements the laboratory? If they're not |
|
122:24 | I'm going to let you answer You don't think they're useful at |
|
123:01 | What do we spend the money to these measurements, anybody. Well they |
|
123:10 | give us idea of your physical properties we're trying to measure in the |
|
123:16 | But the compared to the come the largest experiments are controlled compared to |
|
123:24 | in the field where we have the and other factors out there. |
|
123:28 | Very good point. Very good. the laboratory. It's a controlled |
|
123:36 | So we could vary the parameters. could vary the pore fluids. We |
|
123:42 | bury the poor pressure, We can the confining pressure, We can characterize |
|
123:48 | sample very well. We could create samples and therefore the laboratory measurements can |
|
123:57 | us understand what is happening. The measurements help us predict how velocities will |
|
124:06 | with the other factors that we control . And so that's where the laboratory |
|
124:13 | are really important. They help us a conceptual understanding. And the empirical |
|
124:21 | can often be used because the inaccuracies comparing to a particular insitu rock tend |
|
124:33 | cancel that on a trend because we're comparing to a particular rock. We're |
|
124:41 | the variation over a group of So there may not be a 1-1 |
|
124:48 | to what the velocity of that sample be in the earth uh for a |
|
124:54 | type of measurement. But the systematics still be applicable. And we found |
|
125:00 | to be very true. The empirical we establish in the laboratory have been |
|
125:08 | useful when applied to real data. what are these factors, You |
|
125:21 | what are these variables that cause velocities bury. So, we'll start with |
|
125:28 | wave velocities. We'll find that with exception of pore fluid shear wave velocities |
|
125:34 | affected very much in the same way congressional philosophy. First of all, |
|
125:41 | have mythology, the composition and We've already seen that effect ferocity, |
|
125:49 | amount of ferocity and the type For us now there are a variety |
|
125:55 | factors that are depth related pressure uh pressure, confining pressure and deferential or |
|
126:09 | pressure. Then there are factors that the degree of lift ification. The |
|
126:18 | the rock, the more liquefied it to be, the longer it's been |
|
126:23 | at high temperature and high pressure uh liquefied. So also the greater the |
|
126:31 | , the greater the degree of lip generally on the average, the degree |
|
126:38 | cement, ation and compaction, not as it affects porosity reduction, but |
|
126:47 | it affects coordination between graves and so and interlocking of brains. So compaction |
|
126:56 | not only decrease ferocity, it could the degree of little indication. Then |
|
127:03 | have, as we've seen, we the pore fluids in Iraq affecting primarily |
|
127:07 | compression wave velocity and a second order on the sheer weight philosophy, temperature |
|
127:16 | affect the velocity through the pore The solid won't be very dependent on |
|
127:21 | temperature as we deal with in the few miles. But they will affect |
|
127:26 | poor fluids greatly frequency. Especially from to laboratory frequencies. And of course |
|
127:37 | Satrapi. So the direction of the counts. So this is just one |
|
127:48 | of measurements that was reported about 60 ago. Um These are history, |
|
127:56 | of velocities and various rock types and that they didn't separate sandstone and |
|
128:04 | But for the most part you had unconsolidated sediments which were lower velocity and |
|
128:12 | can see they could be lower than velocity here. So some of these |
|
128:16 | above the water table. They're you have sand stones and shells. |
|
128:22 | , if dry, they can be than water velocity, which is 5000 |
|
128:27 | per second, higher velocity or Then you have your igneous metamorphic rocks |
|
128:37 | you're in Hyde rights will tend to the highest philosophy salt uh generally around |
|
128:44 | , but you're vaporize can be very philosophy Now. Uh in the same |
|
128:54 | , they report fiduciary limits. What the fiduciary rule limits? So you |
|
128:59 | say Between what range does 80% of data occur. So the, you |
|
129:07 | , those that can be represented as bar. And so this is the |
|
129:13 | data just represented in terms of The for with 80% of the data occurs |
|
129:20 | you see that there's tremendous overlap. fact of these reported values for sandstone |
|
129:26 | shale are quite low. I as we drill deeper, we find |
|
129:31 | sand stones and shells both could have higher velocities. So I would pull |
|
129:38 | stones all the way up to say. And shells not quite so |
|
129:44 | . So, velocity alone, it's enough to distinguish uh the mythologies, |
|
129:52 | the mythology, the pathology is enough give us an expectation for the relative |
|
129:58 | of velocity. Not necessarily right, there is overlap. So it's a |
|
130:04 | sand tight sandstone can be faster than porous limestone, for example. |
|
130:16 | same concept just showing overlap between different types. Now, we talked previously |
|
130:29 | the velocity of the suspension. um this would represent the lowest velocities |
|
130:39 | we can have uh in Iraq as loses cohesion. So well, interesting |
|
130:49 | here that should say x courts. now I'm just going to ask you |
|
130:57 | make the calculation. So, uh the volume of courts from 0 to |
|
131:04 | . The other material will be And so you could use a any |
|
131:13 | . I and then as you um I could suggest starting module i |
|
131:19 | debt cities. Uh for ports use giga pascal's and for water used 2.5 |
|
131:28 | Pascal's that would be, you either fresh water under some pressure or |
|
131:36 | faulty water. So use 2.5 giga for water In a density. You |
|
131:44 | use one the water or 1.5 grams cc. It's up to you. |
|
131:52 | courts use the density of 2.65. go ahead and create this spreadsheet. |
|
132:01 | it's a it's worth doing. But , this is vp computation. I'm |
|
132:22 | , I was muted. Yes, Bp. And I'm going to stop |
|
132:26 | them. This conference will now be . Which are you seeing this |
|
132:37 | Are you seeing fast empirical relationships? , sir. Okay. So the |
|
132:45 | thing is showing, Sorry, that cut off and that's something I have |
|
132:49 | figure out how to fix. So going to uh escape. And so |
|
132:56 | can see the full slide here. in the early 50s when uh sonic |
|
133:05 | were first being acquired bounced, collected lot of data and he realized that |
|
133:15 | older Iraq was, the higher the and the deeper Iraq was on the |
|
133:22 | . The higher the philosophy. And came up with this empirical relationship where |
|
133:31 | . Is A. Is a Now, um It's not clear how |
|
133:39 | arrived at this form. T to 16 is the to the 16. |
|
133:44 | at the same time, theoretical calculations suggesting that sphere packs Should be related |
|
133:52 | the 1/6 power of pressure. And that may have steered fast into this |
|
134:01 | of relationship. We're not sure what justification was. Uh huh. Now |
|
134:08 | is catching the overall tendencies, but doesn't capture the fact that uh more |
|
134:16 | rocks of lower velocity than low ferocity . And so he came back and |
|
134:24 | tried to incorporate ferocity into the equation including increases Stephanie. So yes, |
|
134:31 | L and I think L. That meant to imply with little logic |
|
134:38 | And so he has true resistive itty . So so the resisted any of |
|
134:44 | rock depends on the ferocity. The mark site, the higher the ferocity |
|
134:50 | the lower the resistive Itty, so higher the conductivity. Uh So uh |
|
134:58 | he has as the resistive itty the velocity increases. And so another |
|
135:05 | relation of a very similar form. gas men about the same time published |
|
135:15 | relationship. Now these are not the equation. This is not the famous |
|
135:20 | equations that we're going to use for substitution. This was an equation he |
|
135:26 | up with for a pack, a packing of spheres. And um he |
|
135:35 | various quantities in here But raised to 1 6th power. So Depth to |
|
135:42 | 16 powers, he's in a homogeneous of spheres. So he knows the |
|
135:50 | of this of the sphere pack. he'll know uh you know what depth |
|
135:56 | the sphere packed corresponds to what So he's basically got pressure to the |
|
136:03 | power. Um Also this factor is to uh the properties of the spheres |
|
136:11 | when here he's got the young youngest of the spheres. The acceleration to |
|
136:15 | gravity, 1 -2 persons ratio of year's the prosperity of the medium, |
|
136:22 | is forgiven spear pac arrangement is And that's the density of the |
|
136:31 | And so you see this mimics this a theoretical equation which is very much |
|
136:37 | same form as fast equations. So justifies this 16 power relationship. By |
|
136:46 | way we use fast equations to this with empirical calibration and modification. But |
|
136:53 | use a form like this to this to predict pseudo velocity locks And um |
|
137:05 | you plot velocity versus depth trends, see a general tendency for velocity to |
|
137:13 | with death. So these are found well fits to the data that Faust |
|
137:26 | the rocks of different ages. And he's got velocity versus death. And |
|
137:34 | for different ages you have different empirical but you can see uh that the |
|
137:43 | the rock is at a given the higher the velocity. So this |
|
137:49 | is showing a age dependency which is related to the degree of with ification |
|
137:57 | a depth relationship uh which again is to a degree of lift. |
|
138:03 | ferocity in semente shin and other So both greater age and greater depth |
|
138:11 | a variety of reasons increase the Let's see if I could go back |
|
138:18 | full screen. Okay, We already about the time average equation and when |
|
138:24 | expressed it, I said the transit is equal to the ferocity times the |
|
138:29 | time in the fluid Plus 1 - Times The Transit Time in the |
|
138:36 | And instead of transit time here, is expressed in terms of slowness. |
|
138:42 | the transit time is equal to one the velocity which is also called the |
|
138:49 | . Uh Now it would be good be able to write to extend this |
|
138:59 | to multiple constituents. And uh earlier I kind of did that with the |
|
139:10 | balance equation where we compute a uh grain density from the constituent densities. |
|
139:21 | , well you could do the same with transit time, you can get |
|
139:26 | grain transit time or a matrix transit here they say matrix velocity is a |
|
139:35 | weighted average of the transit times of solid constituents. Uh So you can |
|
139:42 | extend the time average equation to mix ology is that way. Now, |
|
139:50 | though this looks like it could be derived, it can't be, in |
|
139:58 | , it could be shown to probably theoretically wrong except under certain circumstances. |
|
140:06 | it tends to work for poorest and at high pressure and by poorest. |
|
140:11 | mean reservoir quality sand stones that are lit defied at high pressure. But |
|
140:20 | seen there are many velocity ferocity relationships depending on the local circumstances, the |
|
140:28 | degree of consolidation and lift, Uh The pressures and so forth. |
|
140:35 | relations will work in different areas. , so uh gardens relation we already |
|
140:43 | at and that relates to density to . And because density is directly related |
|
140:53 | velocity then it relates ferocity to Uh so let me escape to get |
|
141:03 | full figure here. And um Here have some of the data that wally |
|
141:11 | and Gardner used this later reprinted in review paper, but I think these |
|
141:16 | were made in the in the 50's these were kind of reservoir type sand |
|
141:23 | , and that's where the wily time equation was fitting. He also included |
|
141:29 | very high porosity rocks, radio larry earth in triple light. Uh presumably |
|
141:38 | are related to uh salacious shells. they're the shells tend to be |
|
141:45 | So, an aggregation of these not only is it a sphere |
|
141:51 | but also the grains themselves have So you can get to some very |
|
141:56 | ferocity is here. And Gregory noted they deviate from the time average |
|
142:10 | Now I mentioned a few times now rain manhunt Gardner equation and this equation |
|
142:17 | from my point of view, I call it an improvement to wireless |
|
142:22 | but I do feel that it's a fit to highly liquefied rocks. |
|
142:26 | Did you have something? Yes, . I have a question on the |
|
142:30 | line. Yeah. So, so though these are beyond 40, we're |
|
142:36 | calling them suspended 40% ferocity or they suspended. Well, they may |
|
142:42 | I'm not sure. I doubt they're by the time they were in the |
|
142:47 | . So the grains are at least against each other. One test would |
|
142:53 | to calculate where the Royce bound is . That would be a nice |
|
142:59 | Right? Uh Let's see how close are to the void to the Royce |
|
143:04 | . I suspect they're not I suspect process, these are so high because |
|
143:09 | grades themselves are Horace. Okay, , because they're empty shells basically. |
|
143:18 | , so so so porosity can be 40% and we can still have uh |
|
143:27 | . Okay. Yes, that's Thank you. And uh so getting |
|
143:36 | to this roemer equation basically, he they The equation has two parts really |
|
143:44 | parts. So for rocks with he found this relationship which as we'll |
|
143:56 | has them very satisfying aspects to But there's a complication, The solid |
|
144:03 | is squared. Uh But so the is one minus porosity square times the |
|
144:10 | of the matrix because ferocity titus the of the fluid. Um There are |
|
144:18 | of this equation that work better than widely equation and we'll come back to |
|
144:24 | later in the course. The other he did is for high porosity. |
|
144:29 | notice here we're above the critical Um He has something that's like the |
|
144:36 | equation except what is roe V. square, that's the plane wave module |
|
144:43 | . So here we have the plane module, lists for the composite. |
|
144:48 | we have the both module lists of fluid and here we have the same |
|
144:53 | modules and solid. So this is exactly a suspension, it's a reciprocal |
|
144:59 | weighted average like a suspension, but actually has some rigidity uh because where |
|
145:08 | is in the plane wave modules instead bulk modules. And so there you |
|
145:13 | , we're not a pure suspension, have some rigidity. I have to |
|
145:19 | this is an empirical, I wouldn't call it empirical, I would close |
|
145:24 | horrific equation. It's just a way adding some rigidity to the result with |
|
145:32 | knowledge that you could have high porosity that are not purely uh suspensions, |
|
145:40 | the grains are in some contact with other. So this allows you to |
|
145:45 | some rigidity. So it would be slightly higher velocity than uh than the |
|
145:51 | equation. And this is what we previously the would like equation. So |
|
145:57 | are two branches of the Ramayana Garden fit to the data he had and |
|
146:03 | in between and notice he's going higher critical ferocity here. Uh In between |
|
146:10 | just Interpol, it's between the So there are three parts, the |
|
146:15 | porosity part, the intermediate ferocity which is just an interpretation. And |
|
146:21 | the hype ferocity part And notices saying . Well, yeah, we're above |
|
146:27 | so called critical porosity of 40%. uh and we still have some |
|
146:34 | So this is a little bit at with the critical porosity model. He's |
|
146:39 | out to higher porosity is than 40% Sandstone and still having the rock with |
|
146:49 | . Okay, okay, so here have the different branches of the Raymond |
|
146:56 | equation and we're comparing it to the equation by the way. This is |
|
147:01 | the original paper of the Raymond Gardner . And so these guys were slumber |
|
147:09 | , they were well log analysts. instead of velocity, they're using sonic |
|
147:13 | time. Remember that's the slowness went velocity against ferocity. So they're going |
|
147:19 | to very high porosity is here. uh, at the types of ferocity |
|
147:25 | in the rocks we're dealing with He has the wildly equation uh, |
|
147:32 | uh, the properties of uh, about this 55 would be slower. |
|
147:43 | . So this one, this curve using the properties of courts, the |
|
147:48 | properties of courts and this other he's or widely curve, he's using |
|
147:55 | , is using a slower matrix ferocity course courts only 18,000 ft/s. And |
|
148:02 | found is often for clean sands, have to use a lower matrix velocity |
|
148:08 | though physically there's no way to explain . And the result of that, |
|
148:15 | that basically it's going through the Ramayana equation. All right, So the |
|
148:24 | Gardner equation will match the widely equation this matrix velocity here, with this |
|
148:32 | velocity there and then back to the matrix velocity there? The high the |
|
148:40 | porosity branches is uh, is this line? Over here, Out to |
|
148:50 | . And he also to complicate matters more, he gives another empirical relation |
|
148:55 | fit the same data. That's pretty to that 1st 1. I tend |
|
149:00 | to use this one because it requires information. You need to have the |
|
149:05 | density as well. Um and it's little bit more cumbersome. Um Then |
|
149:15 | got his high porosity branch. So is the would like equation here and |
|
149:22 | in between the two he inter plates between so kind of a very rapid |
|
149:32 | where he's losing uh integrity of the . The sample is losing its rock |
|
149:43 | characteristics and it's becoming more sediment like you see that's happening around 40%. |
|
149:49 | that is uh somewhat in agreement with critical ferocity model. Although you've got |
|
149:56 | uh rocks out here which are greater 40%, which have rigidity. And |
|
150:04 | this is the would like equation, the wood equations. So there's rigidity |
|
150:08 | as well. And just plotting some points and I'm sure these are cherry |
|
150:18 | data points. What is cherry Cherry picking means picking only the good |
|
150:23 | . So this is an example of data that falls on your trend. |
|
150:29 | believe me, there are a lot data points that don't fall on the |
|
150:33 | . So we could say these are types of rocks that obey the Raymond |
|
150:38 | equation. And these would be the liquefied rocks. And you can see |
|
150:43 | this compares to the widely equation. I use the properties of course in |
|
150:49 | , the wildly equation seems to be . But here you would need to |
|
150:54 | a different wildly equation because of the charity. Whereas the Raymond Gardner equation |
|
151:02 | to work. Yeah. And so his would like equation and you notice |
|
151:14 | are a lot of points that are than the would like equations. So |
|
151:18 | the voice bounds would be further uh the right here. Uh so uh |
|
151:26 | are seeing some development opportunity here. , mm now I could change the |
|
151:38 | velocity and I could consider different rock . So these are different Raymond and |
|
151:44 | curves for different, fully brine saturated . Or I could change the velocity |
|
151:50 | the fluid to do a crude fluid and look at the effect of hydrocarbons |
|
151:59 | the velocities. Now this is not correct, but it is more correct |
|
152:07 | doing the same thing in the widely . So this is one aspect of |
|
152:12 | Raymond Gardner equation that is better than wildly equation. You get reasonable answers |
|
152:18 | you use the correct fluid velocity. , so, uh it's time for |
|
152:31 | exercise. And what I'm going to you to do is compare uh the |
|
152:38 | uh mm velocity ferocity hair transforms for sandstone. And so I'm giving you |
|
152:52 | courts and the fluid velocities. You use any of these equations. And |
|
153:02 | from uh velocity, you could either with velocity and predict ferocity or start |
|
153:09 | for us and predict velocity for most these transforms. It's easier to start |
|
153:14 | ferocity, plug plug the numbers into equation and get the velocity for the |
|
153:20 | of sandstone equation. You'll have to the other way, You'll have to |
|
153:24 | with velocities, predict the density and predict the ferocity associated with it. |
|
153:31 | you have the gardener sandstone equation in notes. Um and uh then use |
|
153:38 | rest of these uh equations to predict velocity ferocity transform. So I'll stop |
|
153:46 | here and let me know when you're conference will now be recorded, start |
|
153:53 | and I'm going to escape. So can see the full slide and we |
|
153:59 | at this previously, this is the relationship. And again, the |
|
154:05 | the point to draw from here is course as a density increases, velocity |
|
154:13 | , so definitely a strong correlation The gardener relation that we all know |
|
154:19 | love and is very famous is a average for all rock types. If |
|
154:25 | compare the gardener stand, stone trend the other trends, velocity transforms. |
|
154:33 | find it's between the would like equation the roemer Hunt Gardner equation. So |
|
154:40 | not for fully liquefied rocks. Uh we could call these semi liquefied or |
|
154:47 | lit defied rocks. It's not for Raymond Gardner relation would be fully liquefied |
|
154:55 | , the wood like equation would be virtually unlit ified rocks and the gardener |
|
155:01 | would be in between. So this a plot from dr Hahn and again |
|
155:13 | showing the wide variation and um velocity transforms. So here is their lower |
|
155:22 | , they're using the true lower bounds is the voice equation, which is |
|
155:27 | same as the wood equation. The like equation would be slightly faster then |
|
155:34 | . So you can see when we're the voice bound, that's probably more |
|
155:39 | a more like a pure suspension when slightly above the Royce found the grains |
|
155:46 | be in contact. And so you've some rigidity there. You can see |
|
155:51 | critical ferocity model, which is this line which kind of acts like a |
|
155:58 | upper bound. Uh of course uh know, it does suggest that you |
|
156:06 | unlit defied at 40 ferocity. Uh fact maybe uh you're not entirely unlit |
|
156:14 | I'd write some of these plots have degree of rigidity. The roemer equation |
|
156:21 | similar, gives a similar result to critical ferocity model. So it is |
|
156:27 | acting as an empirical upper bound, the critical ferocity model would be a |
|
156:33 | upper bound, but they pretty much . Um You see the widely equation |
|
156:39 | slightly below that. So the widely not perfectly lit defied rocks, but |
|
156:46 | is good for typical reservoir type Uh the gardener relation would fly even |
|
156:55 | and so a lot of these you could see if I was fitting |
|
156:58 | of these points, that would give something like the gardener relationship there. |
|
157:04 | these straight lines represent I think uh the most part where you have many |
|
157:11 | forming along the line, that would an individual sample with an individual degree |
|
157:17 | consult of lift, ification. Uh the variation along the line would be |
|
157:23 | the dependence on pressure. So the dependence is moving you up and down |
|
157:30 | that. Okay, so we already about the critical porosity model, but |
|
157:43 | at these equations and the critical ferocity , they basically say that the the |
|
157:50 | frame properties are essentially linearly related. is uh with as ferocity changes, |
|
157:59 | have a reduction in the bulk module of the grain. And so essentially |
|
158:07 | have a linear relationship between ferocity and bulk modules of the dry rock, |
|
158:14 | a similar relationship for the share Uh What this suggests is that the |
|
158:25 | of the dry bulk module lists to dry sheer module list is exactly equal |
|
158:31 | the ratio of the mineral bulk modules the minerals share modules and that's not |
|
158:37 | far wrong for sand stones, but as a caution, it may be |
|
158:44 | wrong for other length. Allah jeez the critical property model is not developed |
|
158:50 | theory, it's just a heuristic model was developed based on experience. |
|
158:59 | um anyway, that's the answer to question that the frame modules ratio is |
|
159:06 | equal to the mineral modules ratio. are some more uh measurements from stanford |
|
159:18 | you may remember we looked at a like this previously where we looked at |
|
159:23 | was apparent volume, but we could expressed in terms of ferocity. We |
|
159:27 | at ferocity versus the mixture of coarse fine particles. So in this case |
|
159:34 | coarse particle is courts, the fine is clay and the same thing is |
|
159:41 | . There's some minimum value here uh is achieved. So if I have |
|
159:48 | framework of course particles, the clays filling the spaces between the courts particles |
|
159:55 | the velocity goes down. And similarly I put courts particles into play, |
|
160:04 | displacing porous materials so the ferocity goes . Um so there's some some mixture |
|
160:12 | the two which gives you minimum And oddly enough, as a, |
|
160:20 | happens as the ferocity decreases, the modules increases. So the compression module |
|
160:29 | , it's not exactly mimicking this, it's pretty close to be maximum at |
|
160:36 | point where this is pretty close to minimum. However, by the state |
|
160:42 | token, the sheer modules is relatively . So one question is, why |
|
160:49 | the sheer module is not changing too and in fact, this may be |
|
160:56 | result of the fact that the court packing has about the same share modules |
|
161:05 | um as the pure clay uh So these have similar sheer module is |
|
161:14 | varying the amounts doesn't seem to change too much. Now, here's an |
|
161:29 | way to prove the effect of micro . Remember we said that if I |
|
161:37 | a rapid increase of velocity with I'll be closing micro crafts. Um |
|
161:44 | here we have a gap bro, and the measurements of velocity are made |
|
161:50 | the dobro and you see a relatively change that's about maybe a 5% change |
|
161:57 | velocity. And then this this sample cracked and the way it's cracked, |
|
162:04 | heat treated, it's brought to a high temperature and then it's cooled very |
|
162:10 | and that induces micro cracks. And see the effect here that it's almost |
|
162:18 | change in velocity with pressure. So that is two cracks closing. Now |
|
162:25 | never are able to close all the , so we never come back to |
|
162:30 | original velocity before micro factory that starts level off. And part of the |
|
162:37 | , part of the reason might be this is very specifically an axial pressure |
|
162:43 | opposed to a confining pressure. In case, I'm sorry, you can't |
|
162:47 | that in this case, it's an pressure. And so what that means |
|
162:54 | it's the sample is putting a piston it's compressed from from one end. |
|
163:01 | much like our young module. This of experiment, right? It's a |
|
163:06 | axial depression. And so if the which were induced by heat seat |
|
163:13 | heat treating um are closed. The they're randomly oriented, the horizontal fractures |
|
163:22 | close. But the vertical fractures may open up so it may never achieve |
|
163:30 | the under the velocity of the Ian rock. Now here we have the |
|
163:39 | of a grab it. It's a low velocity, excuse me, Very |
|
163:47 | ferocity. And it's left on a and the velocities are measured as a |
|
163:55 | of time. So this sample has been jacketed is measured as a function |
|
164:01 | time and you see that the velocity down and it's initially a big decrease |
|
164:08 | velocity and then it's a slower decrease velocity that continues on as the sample |
|
164:16 | left there. And what's happening is are draining out of the sample and |
|
164:22 | sample is drying. So even though a low porosity granite, apparently it |
|
164:29 | microfractures with fluids in them. As fluids leave those micro fractures, the |
|
164:36 | , the rock becomes more compressible and the velocity comes down. So actually |
|
164:43 | flu is in the fractures are helping the compression. Uh This is a |
|
164:55 | which is uh somewhat complicated. Um there are measurements of VP VS. |
|
165:04 | again in a granite and here for line and this line the poor pressure |
|
165:14 | equal to the external pressure and again he go so that you can see |
|
165:21 | is pressure applied with the poor So this is the external pressure. |
|
165:29 | pressure is another word for confining So I'm increasing the combining pressure, |
|
165:35 | I'm keeping the poor pressure equal to combining pressure. Uh And you see |
|
165:41 | velocity changes very little now if So the differential stresses zero in all |
|
165:48 | these cases, if differential stress were to effective stress, then the velocity |
|
165:55 | be constant because if I'm holding the stress constant uh and the effective stress |
|
166:02 | equal to the differential stress, then effective stresses constant. So what this |
|
166:07 | telling me is that the effective stress not equal to the difference of uh |
|
166:13 | to the differential pressure. And we find this to be the case in |
|
166:21 | impermeable rocks. Now, another aspect these measurements is that If I look |
|
166:31 | the measurements at poor pressure equal to the shear wave velocity um for the |
|
166:40 | rock is faster than the shear wave . For the saturated rock. Unless |
|
166:46 | get to very low, very low . And there may be actually these |
|
166:54 | pressures, There may be some chemical happening like repulsion between grains or or |
|
167:02 | surface tension effects. Holding things for example. So things might be |
|
167:09 | little complicated here, don't worry about . But here we have the saturated |
|
167:15 | shear wave velocity being slower than the shear wave velocity that potentially could be |
|
167:23 | pressure effect. And you notice that difference gets less and less as we |
|
167:29 | that the confining pressure. So presumably got a significant force base enough to |
|
167:39 | that velocity difference which has all So maybe this is a highly fractured |
|
167:45 | , You have a big increase in with pressure early on. So lots |
|
167:51 | these fractures are closing and so the space closes completely by the time you |
|
167:57 | to high pressure and there's no difference the dry and saturated rock and you're |
|
168:04 | a similar effect here. Uh The rock is actually faster than the dry |
|
168:11 | because fluid within the small micro cracks resist the compression as you're squeezing those |
|
168:20 | crafts. But uh you uh with pressure, you close them to a |
|
168:26 | extent and the difference becomes negligible. , here's an example of the effective |
|
168:39 | law working, you know, here have or what is called the external |
|
168:49 | . I'm sorry. This is the pressure here and f is the Uh |
|
168:58 | . The difference between the external pressure the four pressure. So that's the |
|
169:03 | pressure and they're referring to that as skeleton pressure here is equal to the |
|
169:09 | , confining pressure minus the poor Or you could say external pressure minus |
|
169:17 | fluid pressure. Um So, when is constant, when the differential pressure |
|
169:24 | constant, the velocities are constant. the differential pressure is equal to the |
|
169:36 | pressure as you increase the external then you increase the differential pressure and |
|
169:42 | velocities go up. So in this you can see that what controls the |
|
169:49 | is the differential pressure. So that this case is the effective pressure. |
|
169:57 | with me on that. Yes Okay. Now these are other sand |
|
170:08 | and what you can see is that some cases uh the external, you |
|
170:16 | the effective pressure seems to be working the differential pressure being equal to the |
|
170:21 | pressure seems to work over a given or given range of pressures. But |
|
170:29 | see here the velocity buried. Uh velocity is not constant at a constant |
|
170:37 | pressure here. They seem to be of linearly related. So the differential |
|
170:42 | to first order you could say is the effective pressure, but not |
|
170:57 | Okay, so here we have a versus transit time thought. Um And |
|
171:06 | we see are velocities measured over a range. So the velocities here are |
|
171:13 | from 1000 ft depth To 13,000 ft death. And here is pure |
|
171:23 | And for the deeply buried rocks they to be overbearing, obeying the time |
|
171:28 | equation. Of course you need a uh grain velocity there, but more |
|
171:35 | less obeyed the time average equation a relationship. But then you go below |
|
171:42 | certain death. And you now deviate the time average relations. And the |
|
171:48 | you get the further away you deviate the time average equation. So |
|
172:00 | why, why is this happening? , these rocks are liquefied to some |
|
172:07 | . Can uh beneath, below a debt or above a certain death than |
|
172:12 | rocks become more and more poorly lit . So we're seeing a deviation from |
|
172:18 | widely equation. Uh here we see same thing. Um so this is |
|
172:28 | trend curve fit fit to velocities versus . In fact, these are average |
|
172:36 | and uh average velocities for 1000 well or so. And this is in |
|
172:43 | gulf coast. And uh so you at a low velocity, uh you |
|
172:51 | velocity rapidly with increasing depth and then kind of roll over by the way |
|
172:58 | are sandstone. So you reach a where you're fully compacted and you're pretty |
|
173:05 | lit defied. And at that point follow more or less the time average |
|
173:12 | . Um so uh pretty close to when you're liquefied with ferocity being the |
|
173:20 | factor by the way, if you a sand pack and measure its velocity |
|
173:26 | pressure and then convert the pressure to equivalent debt death, you get a |
|
173:31 | more well behaved Trent right here, uh we're not uh rearranging brains, |
|
173:38 | not getting the rapid ferocity reduction that saw from compaction here, the grains |
|
173:44 | just getting pushed against each other more more so this is the pressure |
|
173:50 | And you can see that at the average equation is the dash line. |
|
173:55 | actual data has a slightly different slope the time average equation and you could |
|
174:02 | some of that to the changing So there is some pressure dependence |
|
174:08 | which the time average equation is ignorant . Remember just pushing the grains against |
|
174:17 | other more tightly doesn't change the ferocity much. You're primarily changing the contact |
|
174:25 | of the brain context. So that's a big ferocity reduction associated with |
|
174:36 | So here's a pretty difficult fly to . Uh, but it's a, |
|
174:42 | a really great one. So I'm to take the time to explain |
|
174:47 | This was a, an empirical study in europe, uh in the vicinity |
|
174:56 | the helps. And what happens here if you're in the basis. So |
|
175:04 | you're away from the mountains, you to have a fairly linear variation of |
|
175:11 | versus death in shells. You also a fairly linear relationship in limestone |
|
175:19 | Of course the lime stones are much than the shells. If you then |
|
175:25 | lime stones and shells together, maybe inter bedded. Uh, you can |
|
175:32 | interpolate in between. So, if were mostly limestone, uh, maybe |
|
175:39 | limestone and 40% shell I would You know, 40% from limestone, |
|
175:46 | from shale. So I would have line more or less like that. |
|
175:53 | you go to the mountains for rocks this ratio of shell to line to |
|
176:01 | . And instead of um instead of along this line, they're much faster |
|
176:13 | they should be. So what is on here at a given depth in |
|
176:25 | mountains? The velocity for the same logic mix is much best is much |
|
176:34 | . And the argument that was made this is a velocity versus death |
|
176:43 | Suppose the rocks and the mountains were once buried to this death and then |
|
176:51 | uplifted to this location and suppose they the velocity, the faster velocity. |
|
176:59 | I suppose we have history says buried this step over geologic time, they've |
|
177:05 | liquefied to this extent. Then you them to the surface and your velocities |
|
177:12 | haven't changed too much. So it tells you how much uplift or it |
|
177:19 | you a ballpark figure for how much may have occurred as a result. |
|
177:26 | this is an important aspect of understanding . If you're in areas that have |
|
177:35 | uh, you know, mountain uh if you had wraps of rapid |
|
177:41 | followed by some degree of uplift, the velocities may do things that you're |
|
177:48 | expecting them to do because of the now in uh poorly lit defied |
|
178:00 | Uh Typically there is a log arrhythmic between shell transit time and death. |
|
178:09 | , we're normally pressured. And so an example of a very well defined |
|
178:14 | . These points come from, logs. So you go to the |
|
178:18 | log you find the pure shells, plot their velocities and they follow depth |
|
178:25 | very well. So this is called you fit a curve to that, |
|
178:31 | called the normal compaction curve. Uh so here's an example in one well |
|
178:42 | we have our normal compaction curve and see the shallow rocks, the points |
|
178:48 | following that normal compaction curb quite And then at some point the velocities |
|
178:55 | much slower. The explanation is excess pressure. If you have abnormally high |
|
179:03 | pressure, you reduce the effect of . And so the velocities are slower |
|
179:09 | in fact here were below 10,000 ft the velocities are acting as if you |
|
179:15 | at 4000 people. So significantly slower . And from how much slower the |
|
179:23 | are, you can estimate the amount geo pressure that has occurred. So |
|
179:32 | few more examples of this, here's normal compaction trend and uh you go |
|
179:39 | below a certain death and the velocities to be much lower. So uh |
|
179:46 | some kind of permeability barrier here preventing escape of fluids and you go into |
|
179:53 | high four pressures. Another example we go on and on with these, |
|
180:00 | the reason I'm showing this is because reason festivity log is doing the same |
|
180:06 | , this is shale conductivity and you it's doing the same thing. So |
|
180:12 | in shells the abnormally and by the , density logs, you'll see it |
|
180:17 | too. So the abnormally high pore is literally increasing the ferocity of Iraq |
|
180:25 | these cases. So you're seeing it velocity, you're seeing it in connectivity |
|
180:31 | you're seeing it in density. One more examples that we're on a |
|
180:39 | trend. The velocities are slower in this case, the sands happened |
|
180:45 | have very similar velocities to the We often assume that the sands are |
|
180:53 | affected by pressure than the shells by pressure than the shells. Uh So |
|
181:00 | a result, a sand shell combination have a different impedance contrast above pressure |
|
181:08 | in in pressure. Uh huh If stands tend to tend to be low |
|
181:15 | normally, if we go into pressure , we might find we have very |
|
181:21 | impedance. All right. So if sands were lower velocity above pressure, |
|
181:27 | shells get slower and then the sands similar velocity below pressure. That will |
|
181:35 | the kind of, the magnitude of spots are amplitude anomalies and the kind |
|
181:42 | amplitude anomaly that we'll see. these are some actual cases of predicting |
|
181:51 | pressure for drilling purposes. Uh These seismic velocities. So they tend to |
|
181:57 | inaccurate. Of course you want to able to do this before you've drilled |
|
182:03 | well, but here we have seismic velocities and you're following not too bad |
|
182:10 | the normal compaction trend and then you to deviate from the normal compassion |
|
182:16 | So, from the magnitude of the you predict the poor pressure. Now |
|
182:24 | drillers drilling the well need to keep their mud weights which are the thin |
|
182:32 | here, need to keep their mud above the poor pressure of the, |
|
182:41 | the formation for fluids. And so is an actual Julian result. What |
|
182:46 | see here is that the drilling engineers being cautious, they didn't quite |
|
182:52 | you know, the the prediction. so they stay up the mud rate |
|
182:56 | little bit early And they tried to two or £3 per gallon above the |
|
183:04 | predicted ferocity. But you see in couple of cases they've skipped the seismic |
|
183:11 | of pore pressure is higher than the mud mud way. Now, if |
|
183:16 | happen to have, if that prediction correct and you happen to have a |
|
183:20 | zone permissible zone right there, you the potential for a blowout as the |
|
183:28 | pressure exceeds the mud way. But fact these are interval velocities. So |
|
183:35 | one, they applied to the middle the interval, it doesn't mean that |
|
183:41 | uh that velocity is constant throughout that . Right? So, um, |
|
183:47 | that may be an artifact of the analysis. So maybe it wasn't a |
|
183:52 | for that reason. And then there's the fact that maybe there wasn't permeability |
|
183:58 | that precisely at those points where these cross. And we see the same |
|
184:07 | again here, the predicted poor pressure in black and the actual mud |
|
184:14 | it looks like we're under balanced but in fact, we're in the |
|
184:21 | and the seismic velocity analysis is not precise. So, uh maybe the |
|
184:30 | were okay, it looks like the were kind of ignoring what the seismic |
|
184:36 | was, right. They up the way early on being safe and then |
|
184:41 | ignored the seismic prediction here. Uh and or here. So in |
|
184:49 | you can see why sometimes the geophysicists are not taken seriously by the drilling |
|
184:57 | because this well, had no problems all. Another effective pressure is to |
|
185:10 | the anti Satrapi. So, uh this case we're looking at compression. |
|
185:16 | waves measured parallel to betting or perpendicular Betty as the pressure is increased. |
|
185:26 | for parallel to betting we're going to faster if we're perpendicular to betting, |
|
185:32 | the betting this is a shell. betting has facility. There's partying along |
|
185:39 | bedding planes. So the bedding planes like fractures. Uh And so if |
|
185:45 | perpendicular to betting, we're going to a slow velocity, if we're parallel |
|
185:50 | betting we're going to have a high , but apparently that facility is being |
|
185:56 | as you're increasing the pressure. So anti Satrapi is decreased similarly with the |
|
186:03 | wave uh If we're going across Um So the wave is propagating |
|
186:11 | It's abetting um it could be polarized two different directions. It could be |
|
186:19 | parallel to betting, or it could polarized perpendicular today? I'm sorry, |
|
186:25 | is propagation parallel to Betty, In case if we're moving parallel to |
|
186:31 | I could have vertical polarization which would perpendicular or horizontal polarization, which would |
|
186:38 | parallel to that. And so the wave is selling that showing the same |
|
186:43 | the anti Satrapi is decreasing as you the pressure, suggesting that these bedding |
|
186:50 | are being healed. They're being forced . Now, here we have an |
|
187:00 | case of fluid effects. I have wave velocity here, P wave |
|
187:09 | Here I have a dry rock velocity with pressure, then add kerosene and |
|
187:20 | velocity goes down. I add brian the velocity goes down more um likely |
|
187:29 | be a density effect. Right? density is uh is uh increasing when |
|
187:38 | change the the poor fluid from a to a heavy brine. So the |
|
187:45 | wave velocity goes down while the p velocity goes up. But the density |
|
187:53 | kerosene is much closer to the density brian. And yet the effect of |
|
188:03 | is to slow the velocity disproportionately to density difference. Is everybody with me |
|
188:11 | that kerosene being a liquid dry being air kerosene is closer to water in |
|
188:22 | than it is to air. um how could you explain what's happening |
|
188:32 | ? Give me a hypothesis to explain fact that water reduces gives you an |
|
188:41 | reduction in velocity as compared to Do you understand the question? Um |
|
188:56 | think he has something to do with bulk models. The compressibility. |
|
189:05 | it does, but why? now it's also the rigidity. It |
|
189:14 | the both modules. But this is velocity, remember? So we're seeing |
|
189:20 | rigidity being decreased because it's bigger than the density effect. So why would |
|
189:30 | in water decrease the rigidity of You think it might make the grains |
|
189:44 | slippery? I like to call it banana peel effect. Right? And |
|
189:50 | , walking around in Houston, you , wet mud is a lot more |
|
189:54 | than dry mud. Okay, especially when you have clays in |
|
190:01 | the effect of water can chemically interact the place and reduce the rigidity as |
|
190:08 | result. And uh as an we could have made these calculations. |
|
190:20 | but I'm gonna skip that exercise right . Yeah, you do see kerosene |
|
190:29 | a density that's Much closer to water it is to zero. So, |
|
190:36 | , this effect is the on the wave velocity is too big to because |
|
190:42 | by the density. Yeah, so, I've got different rocks with |
|
190:55 | kinds of behavior and again, the pressure here is just the differential |
|
191:01 | So, again, mislabeled. Um , I have a VP and uh |
|
191:11 | s being measured and I'm comparing brine to dry. So, you can |
|
191:20 | the effect on this limestone, The of dryer wet is much bigger on |
|
191:26 | p wave velocity than on the shear velocity. Mhm. That could be |
|
191:31 | from both modules. Right. Um effect on this granite is much smaller |
|
191:40 | that could be explained by the fact the granite may be much lower ferocity |
|
191:44 | the limestone. Here, we have dull might also probably low porosity, |
|
191:51 | it has this very rapid increase. is likely suggesting microfractures um And |
|
192:02 | microfractures or into crystalline force. Remember we re crystallize calcite, we could |
|
192:10 | could create low aspect ratio for us the dolomite crystals, oddly enough in |
|
192:18 | dole might the saturated rock has the shear wave velocity than the dry |
|
192:25 | Uh one way to explain that is that the fracture for the low expectations |
|
192:35 | us are such low permeability that the can't get out of the forest. |
|
192:41 | actually, as I share the I'm actually trying to compress something for |
|
192:46 | . And if the fluids can't get , they will resist the poorest will |
|
192:52 | compression caused by the sharing of Um That that means that Uh |
|
193:02 | The permeability is low. If the was zero. If they were perfectly |
|
193:08 | , you should see you should not that increase as you couldn't get fluids |
|
193:14 | those micro fractures at all. Uh yeah, but the permeability is such |
|
193:24 | over time, if you give it time to be fully saturated. You |
|
193:28 | get fluids into those very flat ports then you have this sullen often limestone |
|
193:36 | , which the velocities are essentially in stolen. Often limestone is almost pure |
|
193:44 | , right? It's Essentially a ferocity zero and very little change with pressure |
|
193:51 | no change with saturation. Right. , we're looking at the effects of |
|
194:10 | fluid on p wave velocities. And here we're looking separately at the both |
|
194:16 | lists the velocity and the impedance. here you have dry oil, saturated |
|
194:27 | saturation and that's pretty typical case the , the oil is usually somewhere in |
|
194:39 | the water saturating the result and the results. So, we have some |
|
194:45 | variations here beaver sandstone velocity increases with in the sponsor blow sandstone, we |
|
194:54 | this rapid increase at very low So maybe that sandstorms fractured. Um |
|
195:03 | you look at velocity, it's uh is confounding things a little bit because |
|
195:10 | the sheer modules is included in Um And if you look at velocity |
|
195:19 | in this sponsored blow sand sound, enough, the dry rock is faster |
|
195:29 | the water and oil saturated rock that to be entirely due to density. |
|
195:34 | the only way to make the dry faster unless the water is somehow softening |
|
195:39 | rock frame, there's a density effect on and it's odd that the density |
|
195:46 | becomes larger with increasing pressure. uh, maybe that's not the entire |
|
195:54 | , but interestingly, if you look impedance, then uh some of these |
|
196:01 | are being complicated in velocity. Uh at in peter's it acts a lot |
|
196:07 | like the both modules. So multiplying velocity times density sorts things out of |
|
196:21 | . Now, I mentioned that temperature the fluid philosophy. Uh These are |
|
196:30 | measurements of uh heavy oil velocities uh a function of temperature and as temperature |
|
196:40 | , the velocity goes down, that the bulk module list is going down |
|
196:44 | than the density is going down now , the higher pressures, the higher |
|
196:56 | is here, sorry, have lower . And so that's a bit |
|
197:04 | Uh So what kind of pressure is ? I'm guessing that these are four |
|
197:14 | . So I'm sorry, this is rock saturated with oil. So this |
|
197:18 | the rock blossom and so the higher pressures you get lower velocity, but |
|
197:24 | rock velocity is changing the temperature because both modules of the oil is changing |
|
197:30 | temperature. Um Okay, so we temperature here on the horizontal axis, |
|
197:41 | have velocity on the vertical axis. is in Maria sandstone, which is |
|
197:46 | clean liquefied, since uh people like make laboratory measurements on and you can |
|
197:53 | as the temperature increases the p wave decreases and these are different differential |
|
198:01 | Um So that makes sense. The expands now for shear wave velocity and |
|
198:10 | water becomes more compressible for sure. velocity and high pressure. We're seeing |
|
198:17 | change at lower pressure. They're suggesting change. I'm not sure. I |
|
198:24 | that if we invoke experimental error, that point out, this is pretty |
|
198:32 | . And here we don't have measurements here. Uh So that's pretty |
|
198:37 | So maybe that line is overemphasizing the of that gun shear wave velocity. |
|
198:43 | keep in mind the temperature effect could itself in the fluid expanding and forcing |
|
198:51 | grains apart somewhat. Um That would suggest a different pore pressure, but |
|
198:59 | supposedly controlling the poor pressure. But can't be sure how well that poor |
|
199:04 | is being controlled. So, you , theoretically we should uh we should |
|
199:13 | as the share weather as the as go to higher temperature and the density |
|
199:21 | the fluid becomes less. We would stuck uh the shear wave velocity to |
|
199:29 | , not to decrease. So this kind of going in the wrong |
|
199:34 | So, I'm suggesting some kind of error at work. Of course, |
|
199:43 | extreme case of temperature has to do you freeze the rock. And this |
|
199:49 | a real problem in arctic areas where are times of the year where the |
|
199:54 | surface rocks have partially melted and you low velocities. And then in the |
|
200:01 | it's all frozen and you have high . In fact, the seismic acquisition |
|
200:07 | is in the winter. You don't to be in this range where you've |
|
200:11 | pockets of low pockets of five. creates all kinds of near surface |
|
200:17 | So, you want to be either or here, but certainly you don't |
|
200:21 | your vibrator trucks trying to travel around . All right. So you want |
|
200:28 | to be on a hard surface. , this is the acquisition season. |
|
200:41 | now in the next section, we're to talk about the factors that control |
|
200:48 | bulk modules of the rock and in , but this is correct. Have |
|
200:54 | this a few times and sometimes it coming back. So I'm going to |
|
201:00 | it now, insert ferocity. Oh, no. Okay, I'm |
|
201:08 | gonna do it now. I'm going do it another time. That's not |
|
201:10 | question mark. That should be That should save ferocity. So, |
|
201:15 | are pore spaces, right? and I think it's funny the way |
|
201:20 | attention to Iraq's is cheese. But think of these as fungi |
|
201:25 | Okay, so there are areas, module and we need to think about |
|
201:30 | order to describe the effects of one is the fluid module list |
|
201:37 | Another is the modules of the solid , which is right here. There's |
|
201:43 | modules of the rock without the That is called the dry frame module |
|
201:48 | . I don't like that term, I'll complain about it repeatedly for the |
|
201:53 | of the course. We don't want actual dry frame. We want the |
|
201:59 | of the frame independent of the mechanical from the fluids, but in chemical |
|
202:07 | with the fluids as the fluids in with the grain, uh with the |
|
202:13 | material can actually change the skeleton So we could call what people call |
|
202:19 | dry frame modules. I prefer to the frame modules or the skeleton |
|
202:26 | Keeping in mind that that's in the of the fluids and that's different from |
|
202:32 | saturated modules. That's the modules of rock. If you can find the |
|
202:38 | , keep the fluid in the poorest or don't let them escape from the |
|
202:44 | and then squeeze the rock and measure modules. That's the saturated both |
|
202:56 | And um if you plot uh as result of the bulk module has changed |
|
203:04 | fluid properties. If you for a water mixture, if you plot velocity |
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203:11 | water saturation, you typically get a like this for p wave velocity, |
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203:17 | water saturation of 100%. So there's gas in the rock here, you |
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203:22 | a high velocity, I add gasp air and just a little bit of |
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203:27 | . The first five or 10 drops velocity most of the way. And |
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203:35 | as I continue adding gas, the rebounds and comes back up. So |
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203:42 | drop in velocity is caused by the in bulk module lists this increase in |
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203:50 | is caused by the reduction in density the both modular stays relatively constant. |
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203:57 | two effects. Both module is the and the density effect. And you |
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204:02 | there is no bulk module, its on the shear wave velocity. So |
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204:06 | have only the density effect. Uh , uh we're in the next |
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204:16 | we're going to go through some uh complicated equations to be able to predict |
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204:22 | curve like this. So you're going be able to do that on the |
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204:27 | , but there's a simpler way to a rough idea remember? These are |
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204:32 | equations. So they're not going to exactly right. Anyway, so there |
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204:38 | a couple of different empirical relations one use and I'll give this the equation |
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204:44 | this line later. This is if cross bought gas stand velocity versus brian |
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204:51 | velocity. If they were equal, would be on this red line |
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204:57 | So, empirically we find uh that gas and velocity in practice tends to |
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205:05 | slightly low compared to the brian sand . Now, the effect of gas |
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205:15 | a percent change gets bigger and bigger we go to lower velocities. |
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205:21 | when I have a low velocity, means I have a compressible rock frame |
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205:27 | will mean the hydrocarbon effect is big , you know, low velocities near |
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205:34 | water bottom, that effect could you know, pretty enormous, |
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205:40 | 100% change here in velocity. Um , um That effect gets as a |
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205:52 | gets smaller and smaller appear at high that might be on the order of |
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205:57 | or two change. So you can that uh gas being in the rock |
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206:03 | cause huge amplitude anomalies deep but can almost negligible or not. Observable in |
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206:11 | little logic variation. I'm sorry, be huge, shallow but negligible |
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206:22 | By the way you can think of stand velocity as a proxy for death |
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206:27 | remember we said velocities increase with So uh you know given a philosophy |
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206:34 | dense depth relationship, you could have depth scale here and so shallow a |
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206:42 | change. Deep small change. And this produces amplitude anomalous. So |
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206:55 | to say an overlying shell which would the square here. So I have |
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206:59 | impedance of the shell density times If my brian stand is low |
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207:07 | what happens when I add gas? lower density. I lower a |
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207:11 | So I make the impedance even So in this case we go from |
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207:16 | negative reflection to a bigger negative And this is what we call a |
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207:22 | spot. Yeah because the polarity issues so forth, europe versus the |
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207:28 | S. What's negative and what's positive people use it in different ways. |
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207:35 | So this I would call a soft and that covers all the possibilities. |
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207:41 | I have a soft reflection due to due to brian, I have a |
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207:47 | , softer reflection due to gas. that's if your sand uh No no |
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207:54 | ready for is low impedance relative to shell. What if your brine, |
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207:58 | rock is high impedance relative to the ? Well, in that case, |
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208:03 | gas reduces the impedance. So it reduce the magnitude of the reflection. |
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208:11 | you go from a very hard reflection a lead guard reflection. That's called |
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208:16 | dirty spot. In fact, sometimes amplitude could go all the way to |
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208:22 | and you don't see a reflection from gas sand at all. So you |
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208:27 | have an invisible reservoir in that Now, when the hydrocarbon effect is |
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208:33 | big or when the brian stand is slightly hard, adding gas can flip |
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208:41 | polarity so you can go from a reflection to a soft reflection. Remember |
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208:48 | is at the top of the at the base of the sand. |
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208:51 | it's the same shell underneath, you see an equal and opposite effect. |
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208:59 | , sometimes it's desirable to have an of what kind of reflection to |
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209:07 | what kind of amplitude should I expect I have hydrocarbons. And one way |
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209:12 | can do that if you have well in the basin is, you can |
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209:16 | depth trend curves. So you could density versus death in jail density versus |
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209:23 | in brian sand and then you could fluid substitution as well due next week |
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209:29 | predict what the gas and uh density be? Well, we could use |
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209:34 | mass balance equation for this. We do that with transit times also and |
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209:39 | would require Gassman situations that we're going talk about next week. And then |
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209:44 | can see what your average reflection coefficients going to be for a gas |
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209:48 | And brian sand. And you can in all of these cases the average |
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209:53 | coefficient is negative. You know, sand is uh or as soft, |
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210:01 | ? The sand is low density, brian stand is low density, low |
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210:05 | . So it's always going to give a lower impedance than the shell. |
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210:10 | always going to give you a negative reflection. Um but you had |
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210:17 | you're even lower impudence in both lower , uh slower transit time. So |
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210:24 | impedance and that gives you a stronger reflection. So these would all be |
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210:30 | bright spots. Now it's not always like that. Sometimes you get variable |
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210:40 | is a function of death. So a shell compaction trend. This is |
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210:45 | versus death. This is a brian compaction trend. So you see the |
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210:53 | Sanders starting out at the very near , higher velocity surface higher velocity than |
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210:58 | shell, but then it becomes lower than Michelle. And then back to |
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211:04 | velocity than the ship. You can substitute oil using gas mints equations. |
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211:10 | that gives you for a he lied , but not a very volatile light |
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211:18 | . Its properties are pretty similar to and down deep. The results is |
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211:23 | indistinguishable from crime or gas, which to be much slower than brian. |
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211:30 | then by comparing if you do the thing for density and construct impedance versus |
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211:37 | trends, you could predict at a death what kind of amplitude anomaly you're |
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211:43 | to have now. Unfortunately these are values. So I'm talking about an |
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211:55 | . Again, actually, these particular came from about 1000 well logs and |
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212:02 | a trend line was spit to average versus death, but there are always |
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212:10 | . And so in fact, at any particular death, you should |
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212:18 | at the history graham for brian for shells for gas stands. And |
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212:23 | you'll find is even though the average may be different, there is potentially |
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212:30 | lot of overlap between this. and so that means, uh, |
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212:36 | know, even though a gas ban this case on the average is din |
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212:43 | I'm sorry, lower impedance than the . Um, you might find particular |
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212:50 | vans, which might be say low which can in fact be higher impedance |
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212:57 | a particular brian stands for example. if you convert that to reflection |
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213:06 | what you'll find, is there a where you can have and you're likely |
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213:13 | could have either gas and their mind . Uh, there's usually some probability |
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213:20 | a reflection coefficient of a certain magnitude be uh, either or okay, |
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213:27 | I have a very large negative reflection this particular case, you have almost |
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213:34 | probability of being brian, but there some finite probability most likely to be |
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213:41 | . But here with still a negative coefficient, It's about a 5050 probability |
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213:48 | been a brian or guests. Uh Hiltermann is has done one better than |
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214:05 | . He looked at thousands of well and he could construct instagram's versus |
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214:11 | Uh and this happens to be for velocity versus death and shale velocity versus |
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214:19 | . And oddly enough, the DP get the more variation you seem to |
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214:24 | . So the average fit that these here represent the average, you can |
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214:31 | the average fit seems to be mon increasing, but you're not always dealing |
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214:37 | the average rock. Right. So , coming back to the average properties |
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214:50 | see this discover the um we could at the average reflection coefficient versus death |
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214:57 | we could look at that for wet and we could look at that this |
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215:02 | gas stamps and there's a crossover point of these curves where the reflection goes |
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215:10 | soft to hard or an american polarities to positive. So here my brian |
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215:18 | are negative. My gas stands are negative. We have bright spots. |
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215:25 | here uh the brian stands are the gas ends are negative, so |
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215:32 | have polarity reversals and here you're brian are positive, your gas fans are |
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215:39 | positive. So you have them Now, if you go into |
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215:48 | you're making your shell impedance is If you go into gear pressure and |
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215:55 | will tend to make the crossover move . So if I were in JIA |
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216:01 | rocks, I uh would would change depth at which you switch from bright |
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216:11 | clarity reversal to dim spot. Now get the idea that all rocks, |
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216:16 | is just a tendency. Don't get idea that all rocks will do this |
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216:22 | any depth. You could have any kind of response. Remember this is |
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216:28 | area dependent curve that's come up that come up with. So uh what |
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216:39 | Idol did is he plotted the crossover at which he moved from uh hard |
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216:47 | soft. He plotted the death at that crossover point occurs and he plotted |
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216:56 | depth for rocks of different ages. . And what he finds is that |
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217:06 | the uh the younger you are, shallower that death occurs. And so |
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217:14 | older rocks that I'm sorry, the that death occurs, I'm sorry, |
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217:19 | is increasing upwards. So older the crossover for shallower younger rocks, |
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217:28 | crossover occurs deeper and that's all I for this section and we've only got |
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217:40 | uh 20 more minutes and I don't to start a new section. I |
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217:45 | to give you time to absorb So actually we moved a little faster |
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217:49 | normal, |
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