00:03 | Okay then. So we can the time we we managed to get through |
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00:10 | first half of lecture seven and tonight going to finish that one and I'll |
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00:17 | on the, on the final we should probably be able to get |
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00:21 | through through all of it even though spent whatever 10 minutes messing around with |
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00:27 | with the exam. Alright, so , complex basis. So, so |
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00:35 | we look back at our Wilson cycle , our little uh you know, |
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00:40 | cycle of phases of opening and closing of basins and then my sort of |
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00:48 | of base informing, you know, fundamental elements regarding force and crystal types |
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00:55 | deformation down here at the bottom, have this sort of multiple phase |
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01:01 | And to be sure, I mean you think you can think of a |
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01:05 | margin as having multiple phases of deformation it's rifting but beneath every passive margin |
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01:12 | one half of a rift basin. you can sort of think of it |
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01:16 | way that it's a rift or some just call them drifted margins because they |
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01:22 | lifted margin. But um yeah, don't know, I like to say |
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01:27 | margin because I'm thinking in terms of composition of the cross. Um but |
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01:34 | know that your auntie um van Dijk teaches basin modeling and for john she |
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01:43 | caused a rift and passive virus and of course there's um you know, |
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01:50 | my sort of three groups of of groups of of whatever classification scheme here |
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02:03 | , you know, a continental mobile based on the composition of the |
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02:08 | you know, the substrate and whether continental oceanic or sort of mobile |
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02:13 | people talk about and each one can single anyway, So, so complex |
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02:20 | or basins with complex histories. This what we're talking about. We're talking |
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02:25 | some some sort of complicated complication that's things, uh, you know, |
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02:35 | sort of, well, sometimes I'm what's going on sometimes just making the |
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02:40 | look differently. Right? So, for example, this session here, |
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02:44 | talk about basin and version. Now version is a word that you see |
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02:49 | lot, we talked about inverse, modeling, but that's not what people |
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02:55 | about when they say basin version and word inversion have to be careful about |
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03:00 | . It's a bit hackneyed because, know, she used in so many |
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03:03 | ways and almost doesn't mean anything. say, for example, you have |
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03:08 | sort of pro grading delta system where have, you know, you have |
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03:15 | faults, growth fault as they uh forming, you know, beneath |
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03:24 | beneath the delta or passive barge or . And this system is, you |
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03:29 | , just kind of a slope sort thing. But then if there's some |
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03:34 | of contraction where there's, you conversion forces compression, all forces acting |
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03:42 | this. Then sometimes these things, things will pop up and that's an |
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03:48 | and inversion of the structure. It once down. Now it's up. |
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03:53 | . So these are all being drifted , you know, they're going down |
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04:00 | whoops and then all of a sudden pushed up. So that's an inverse |
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04:05 | basin inversion and a very famous one called the central basin platform. Have |
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04:12 | heard of the central basin platform? ? It sounds familiar. I know |
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04:20 | gone over but it's just, it's a while, I would hope you |
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04:23 | of that. I mean this is Permian, this whole thing, the |
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04:28 | plus the midland plus the central basin . This is called the Permian basin |
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04:36 | it's called the premier basin. If before pennsylvania time. This is this |
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04:43 | when this inversion happened that the structure pushed up in pennsylvania at the very |
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04:52 | closure of Pangea. Okay, when America finished closing, finished crashing into |
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05:02 | America to make Pangea. This is this popped up this, what you |
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05:09 | hear people talk about the ancestral Those are a bunch of Pennsylvanian structures |
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05:17 | are sort of sub parallel to this here and they're all up into new |
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05:23 | all the way up into colorado. ancestral rockies. In other words, |
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05:28 | were, they were structural highs that before present day rockies. That's why |
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05:36 | call it the ancestral, they have to do with how the rockies farm |
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05:41 | they're not related in that way. are much younger. Rockies are formed |
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05:46 | guess severe Lehrman time. But Okay, so this is Pennsylvanian and |
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05:53 | before then this was all one big basin. There's a gravity low, |
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05:58 | mean the basin is thickest right through Delaware and down into the val verde |
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06:03 | then it's thins away from it. mean, yeah, so it's it's |
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06:10 | that classic typical asymmetric geometry words deepest through here and then it gets thinner |
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06:21 | ways, it gets thinner, you , very sharply to the southwest, |
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06:25 | gradually to the to the northeast. that basin was called the turbos A |
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06:30 | to bosa is a, you comes whatever it's a it's not a |
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06:36 | anymore. So that's why they but they call this whole area the Permian |
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06:39 | . All right. Um And here's couple of cross sections through it. |
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06:45 | one right through the very center of here. This is the Delaware |
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06:49 | Delaware basin, the middle and base the central basin platform. Again, |
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06:54 | whole thing is called Permian basin. just in case you, you |
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06:59 | in case you don't get, I , so you don't get confused if |
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07:01 | have people talking about these things. so the Delaware, we just know |
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07:05 | in the Permian basin or the So and so forth. And this |
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07:10 | here is further to the south south and it's shorter. But again, |
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07:18 | you can see the geology is pretty and everything like that. So this |
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07:23 | um a three D. Model that done in the premium basin by my |
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07:29 | Zhang. Um and this is the depth I think. And this is |
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07:38 | anomalies over here. This outline is the Abilene gravity minima. And she's |
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07:45 | it in over here. It's just name given to this gravity anomaly. |
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07:50 | big low sort of trough through But you can see the platform. |
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07:55 | really easy to see. You can the Delaware basin. In fact, |
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08:00 | looks deeper here than here because it now. I don't know see the |
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08:06 | , there's no basin over here. why, why, why do you |
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08:10 | there's this low is So it's like . I mean if there's not a |
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08:17 | here. Um There might be, might be. I think the |
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08:24 | I think that the, Oh this is I think I think this |
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08:30 | the fourth worst basin over here. think this is the paddle dural basin |
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08:34 | here. I don't think that's a , but it could be but why |
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08:40 | I so undecided. You have a a guess at why I'm um sort |
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08:46 | wondering about this low here. I , I don't remember it being a |
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08:51 | . Um I should remember stuff like but I don't but tolerant wise it |
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08:57 | it looks quite like this but I that the Download bases quite deeper than |
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09:01 | one. What's what's causing my uh confusion here. Um hmm. I'm |
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09:21 | at wave legs. I'm thinking about . I'm thinking those. That's what's |
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09:27 | me. Our wavelength. So remember wavelengths for gravity can be related to |
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09:41 | uh some gravity. That's the It's the mojo crystal thickness. Why |
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09:58 | I always get that wrong? Alright. So um Right. So |
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10:05 | , so I'm confused here because even I think I know that the Palo |
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10:10 | is up here, the Delaware is , the midland basin is here. |
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10:14 | thinking that I'm thinking that this could this could be, you know, |
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10:21 | on the base of the crust. crust could just be thicker here. |
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10:25 | even though there's not a base in crust can be thicker for some other |
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10:30 | . So yeah. Alright. Okay. So she made a model |
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10:36 | . I think we're looking at this right here. A two D. |
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10:40 | is controlled by some refraction stations, like our model from our exercise. |
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10:48 | so the interesting thing about this is she's modeling the premium basin, the |
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10:56 | basin platform as a structural high, is correct. Um She's really constrained |
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11:05 | well controlled for this shape. So just putting in some lower densities up |
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11:11 | . I see the way. I think that's the right way to do |
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11:15 | . But I mean I mean I on her committee. I was not |
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11:17 | advisor. I did. I did her. I don't think no explain |
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11:24 | discomfort with this. But here's what thinking. So she's almost got the |
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11:28 | here if these are basement terrain then need to drop all the way down |
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11:34 | the to the through the top through upper crust. Maybe not so much |
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11:40 | lower crust because that's that's a little you know that's lower crust is typically |
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11:47 | and stuff. But And so she this 2.64-2.75 for the basement rocks. |
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11:56 | me that's just too big of a . And if you made these things |
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12:00 | all the way down, I mean whole made a hole like a basement |
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12:06 | then you have to make that density . And so the contrast between the |
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12:13 | this pink basement and this yellow basement be far less. That's what I |
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12:20 | I think that and that would be reasonable to me. Right. I |
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12:24 | large density contrast with that sort of . Just just don't make sense to |
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12:29 | . Why would why would that be mean if that were the case, |
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12:33 | would why would the top of I guess you could argue it's been |
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12:38 | away. I don't know. But that's that's what sort of budget about |
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12:42 | model? Well but I still start thesis. So yeah. Um And |
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12:51 | she made so here's on the lack the mojo depth. So it is |
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13:04 | she hasn't getting deeper beneath this I tend to think that this is |
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13:11 | a compositional change. So and then did the density inversion on the on |
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13:19 | upper crust. And see it ranges 2.74 to 2.77. So it's just |
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13:27 | . Right? I mean it's not of a contrast at all through |
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13:31 | So even though you have all these and lows, they're very subtle, |
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13:36 | And I agree with that. And she made some basement trade interpretation. |
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13:44 | she did that based on her modeling . So that was kind of kind |
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13:48 | Okay, alright. Um I think talked about this. I think this |
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13:57 | be the third time we've seen this . I think we saw it |
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14:01 | Already saw it for four arts. I think I showed it to |
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14:05 | We looked at it once before But remember this is the caribbean plate |
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14:09 | how the fair line plate tore As you know, the subduction flipped |
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14:17 | the caribbean plate tore away. So caribbean plate, the southern rim, |
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14:22 | we call the southern rim of the plate right here. Is that a |
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14:27 | history. And there are basins formed along here. Um uh They're not |
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14:35 | indicated, but there's bases that formed uh in Colombia and Venezuela, all |
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14:43 | the northern uh coastline of south America what I'm going to call the southern |
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14:51 | rim, but there's also part of place as being subduction, even though |
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14:57 | northern part, there's no subduction. all just, there's just a |
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15:01 | it's like slip boundary up there. that's kind of an interesting thing. |
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15:05 | did this part? Why is There's such convergence down here, but |
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15:12 | a little bit up here. In case, we're going to take whatever |
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15:16 | steps across and look at all these that are forming along here. And |
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15:21 | complex because this is a right, is a passive margin. And then |
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15:29 | plate, the caribbean plate is moving it, uh you know, trans |
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15:34 | the transverse direction. It's not like not, there's the tectonics is |
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15:39 | you know, normal to the passive , which is kind of like, |
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15:43 | know what you what you normally It's this is being, you |
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15:47 | the place just driving right past like scraping bits off. And that's |
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15:52 | crazy things are happening. So that's idea. So we're going to start |
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15:56 | uh Columbia over here and then we're go, we're gonna look at the |
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16:03 | , at the base is right the falcone basin. And then there's |
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16:08 | basin here and it's called, well a rift in here and then there's |
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16:15 | more basics. We're gonna look I'm sorry, two more bases on |
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16:18 | . We're gonna look at in through . Um but this isn't really |
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16:24 | This is a uh really, I like these figures because they're showing, |
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16:31 | , so they say there's six tectonic separated by these dash lines. I |
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16:36 | know, I really agree with but it's okay you can do that |
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16:40 | of thing. Um Yellow arrows, they have relative gps motion relative to |
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16:46 | fixed south America. In other these blocks are moving relative to fixed |
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16:53 | America down here. And as well up here, these arrows are |
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16:59 | you know, they're all scaled to same but they're showing the relative motion |
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17:04 | these blocks. So yeah, there in motion right now. I mean |
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17:09 | a lot of convergence plan, There's here, you know, sub ducting |
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17:14 | the southern part of the Caribbean plate here and then also going back here |
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17:20 | G. A. C. Is great arc of the Caribbean. Uh |
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17:25 | and as as it was plowing through , right beginning right here, there |
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17:32 | bits of it that were kind of and kind of left behind abandoned as |
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17:38 | arc moved to the east relative to America. So that's great art from |
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17:45 | America. You see that a And so that's what all these islands |
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17:50 | . These are parts of the great . And in fact they they dashed |
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17:57 | yeah. And it goes right up the abs Ridge which remember is a |
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18:02 | island arc. Remember that of course lesser Antilles is an active island arc |
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18:08 | . There's volcanism happening right now. they call the southern caribbean deformed belt |
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18:18 | through here and it consists of the Antilles. So these are these bits |
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18:23 | the great arc that were abandoned. let's see this is the Wahida Wahida |
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18:34 | which is right there and then the peninsula which is right here. Um |
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18:43 | marta. Uh let's see who Bucaramanga . So that's that's going right through |
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18:53 | and then the iPCC. This is L. P. Large fault zone |
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18:57 | is thought to be a transformed body money. And below it's free air |
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19:03 | . And we know it's free air because it looks like both um a |
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19:07 | , right? It looks like The island arc is a big |
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19:11 | Big honkin gravity high that's ready island . The Aves ridge is a |
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19:19 | the basin is a big low, all these islands producing gravity high. |
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19:25 | we know it's free air gravity because looks like now they divided it into |
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19:33 | types and they did some age This is the part that I find |
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19:37 | crazy they have. So this is age of the dating which is |
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19:46 | Remember that the caribbean? When did arrive? It arrived? You know |
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19:52 | ? You see it arrived between 90 75 M. A. right 75 |
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19:58 | . A. It still wasn't in , But they have rocks here dated |
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20:03 | . Is that right, 74. they have cretaceous cretaceous, that's older |
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20:09 | 60. So in my notes let me see, I got my |
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20:14 | . They say they have great argument . Great arc of the Caribbean magnetism |
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20:21 | between 128 occurred from 1 28 AM 2 70. For yes. So |
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20:30 | 74 is a. Is a date 28. Wait a 2nd. 1 |
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20:38 | . I mean that's way to hang here. So what does that |
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20:43 | That means you see when did this , when did the polarities change? |
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20:49 | after 90. I mean after 90 . A. So that means there's |
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20:54 | 28 rocks if they found something. do they do they have any data |
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20:59 | ? 1 10 1 28 right there are rocks these these are are the |
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21:08 | as Tobago remember was Tobago Tobago. off it's dead. Tobago's off the |
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21:18 | up here. That means they these is 110-128 I would say 1-14-1-15 I |
|
21:28 | say. Those are bits of arc the previous arc. The one where |
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21:34 | polarity was um where the slab was to the east instead of to the |
|
21:42 | as it is today. So that's really interesting. I mean that's that's |
|
21:48 | quite interesting. I've never talked to about that but I should probably |
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21:52 | That's paul man. He was this vince. I don't know I don't |
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21:56 | never met vince but I mean palma a professor on campus. So I |
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22:02 | have talked to paul about that. that's something that's that's really interesting. |
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22:07 | Yeah and then below is a two time basement structure map showing the debt |
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22:14 | two way travel time. So that's yeah that's really interesting. Okay. |
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22:23 | . And then I'm gonna show you seismic lines just so you can see |
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22:26 | the structure is a lot on the caribbean room. Let me show you |
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22:31 | C. D. And E. . B. Is right? There |
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22:34 | a C. D. And And here you go. So you |
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22:43 | I mean here's the thrust front and , you know, seductive. So |
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22:48 | you know this is like non rigid , right? So that's the it |
|
22:53 | like a subduction zone. It looks there's convergence. But the convergence is |
|
22:57 | , right? Remember this part? caribbean plate is like moving towards you |
|
23:02 | of the plane of this, of cross section. So the structuring is |
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23:07 | complicated. I've done a bunch of along this large and for different |
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23:11 | Yeah. I mean it's if you you're thinking about forces then they're orthogonal |
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23:19 | this picture or I would say more oblique. Okay. Um now let's |
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23:31 | at Columbia. Um So here are bunch of terrain that were created onto |
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23:38 | northwest part of Colombia. Um As Caribbean plate was shoved in here, |
|
23:44 | ? Or as it formed while while know, while the arc, great |
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23:50 | crashed into here and see they've identified say realms. I would just say |
|
23:58 | but I guess I don't know I anyways um Yeah Guiana shield uh cabo |
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24:13 | . And then this is so this this is just a nice picture. |
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24:19 | I don't know how to pronounce it but then then Sanchez Rojas and Palma |
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24:28 | Rojas and Palma made a three Gravity model based on a bunch of |
|
24:33 | . They had refraction data, they seismicity from you know earthquake um They |
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24:39 | reflection data, they had all kinds data in here and they made a |
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24:43 | D. Model because there's subduction going here from a couple of different |
|
24:48 | There's subduction from the Nazca plate out in the uh pacific ocean that's sub |
|
24:58 | beneath you know south America and central . You know that subduction zone plunging |
|
25:05 | know, dipping to the east. then there's this southern part of the |
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25:11 | plate which is also sub ducting beneath corner of south America of Colombia. |
|
25:18 | it is way, way complicated tectonic . It is not a nice static |
|
25:24 | but there's a bunch of features They're all labeled but I'm going to |
|
25:29 | you three cross sections A. And C. And here's kind of |
|
25:33 | A three G. And are you in here with these beach balls with |
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25:39 | uh play solution. Beach balls I learned about them before. Yes and |
|
25:45 | and intro video. Okay so this like a three D. Volume with |
|
25:51 | things plotted in three D. So is kind of manager friendly I |
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25:57 | And yeah here's the seismicity depth I that's in these. Is that I |
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26:06 | . Yeah because there's some red ones maybe some blue ones down here |
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26:10 | Okay so that's a nice little And here are the three cross sections |
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26:16 | . B and C. Um um has a lot of control. He |
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26:23 | done depth estimates. He has seismicity ? He has the magnitude of seismicity |
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26:29 | in the size of these circles And oil or depth estimated estimation with two |
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26:39 | um zeros and ones. So that's a lot of these symbols are all |
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26:44 | here. Um He's done mojo depth from spectral analysis. So how do |
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26:58 | do that? He's probably done that spectral analysis, gravity data. So |
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27:03 | then he's calculated nice a static This just this place is this |
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27:07 | This region is not an isIS static . So I don't know what |
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27:12 | I have no idea what that But if he's using that to constrain |
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27:16 | his model, I think that's incorrect basically what he's done is the they |
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27:25 | their control and that's all these symbols they mean a lot of different things |
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27:30 | basically you can look at it kind so you know that these these are |
|
27:35 | you um sort of like a minimum of the top of their saying upper |
|
27:45 | and lower crust right in here. then they have the atmospheric mantle down |
|
27:52 | beneath the white line. The white is the white line is the base |
|
27:55 | the crystalline crust. And then for for continent and then just this two |
|
28:03 | dark green is oceanic crust. Light is oceanic atmosphere, right? |
|
28:08 | With a severe mental issues here in density contrast is 3.343 point 353.341. |
|
28:20 | . So if you notice there's not of a density contrast for the deep |
|
28:25 | , 3.4 versus three point Well, 4141 She got here three 35. |
|
28:39 | is something I've seen people trying to subduction zones. It's really hard because |
|
28:46 | I said, they're not static Which is sort of how these models |
|
28:52 | , right? But do not mistake . Plus, they don't really produce |
|
29:01 | anomalies. I mean, you um is this gravity low produced by |
|
29:07 | slab? Probably a little bit, know, but if you look at |
|
29:11 | density contrast, there's not much of density contrast, you know, they |
|
29:16 | a big one here. So this the crazy part here is this this |
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29:19 | the caribbean slab, this green one this purple one that's the Nazca slab |
|
29:25 | in from the pacific side which is know, you're looking at sort of |
|
29:30 | sort of bent or flexed. So really crazy. Um, I'm kind |
|
29:40 | ambivalent about these three models. I , as, as a rule, |
|
29:45 | don't like to see so many segment , especially with density. I mean |
|
29:52 | Magnetics, you almost have to, with gravity, it's just really sort |
|
29:57 | painful for me to look at that . I just think that there has |
|
30:01 | be a better way. But maybe tried other ways. I don't |
|
30:05 | Um, in any case, you , I'm not even talking about the |
|
30:11 | fits the fits pretty good. I , it's probably the fit is probably |
|
30:15 | than, than the model, I mean the models shaky is on |
|
30:20 | set. Okay. And then of they made, they rolled all this |
|
30:25 | into a 3D model, which is ambitious and I mean, you |
|
30:29 | hats off to these guys for tackling problem, but it is pretty |
|
30:34 | I think that it certainly would be you could use if you want to |
|
30:38 | into this part of the world a bit more. Here's the base of |
|
30:42 | crust. So these are contours in kilometers subsea. So there's the, |
|
30:48 | , I mean in kilometers subsea, the 45 35, 25, 2015 |
|
30:59 | , 15 km. Now the water out here is, I guess three |
|
31:04 | probably I don't think it gets much than that, maybe 3.5. So |
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31:10 | it's, if it's 25, 15 , That means the crust is 10 |
|
31:19 | more Kalala stick. So that's why call it. They think it's all |
|
31:25 | plated or large parts of it are plated, especially up here in the |
|
31:31 | ridge, underplayed by the, you , magnets from the Galapagos plume as |
|
31:40 | is that part of the, at time Farrell and plate passed over and |
|
31:47 | the right here. Our friendly little transect but also they've contoured the dipping |
|
31:56 | from north to south right, The slab is dipping south this way. |
|
32:01 | it's kind of just like the corner the places or the place, you |
|
32:06 | , so it's just the corner of America and then here's the dash lines |
|
32:12 | the nascar play, which is part the pacific pacific. So it's really |
|
32:18 | a sharp bend in it there. don't know that seems that seems pretty |
|
32:26 | to me, but yeah, so if we step over to |
|
32:34 | to the east a bit, we to the beneath this um, what |
|
32:39 | the name of that peninsula? the paraguana paraguana peninsula, there's this |
|
32:52 | column basin and it has some intrusions through the middle of their uh, |
|
33:01 | , what did they say? They ? The uh, Igneous intrusive buys |
|
33:09 | crop along the axis of the okay, along the axis of the |
|
33:13 | . So through this way, I'm . Okay. And um, they |
|
33:22 | a model. They did this model here. So this, this map |
|
33:25 | is uh, gravity anomalies. let's see here. That's a |
|
33:34 | So this is, this is free data and I'm not and I know |
|
33:39 | because again, it looks like This is the water, it's |
|
33:44 | It's a gravity low so high here the islands are to grab you |
|
33:48 | So this is all three year data least the obstacle part is free |
|
33:52 | It looks like it's bouquet on In any case they have a cross |
|
33:56 | that goes through right through here. this is where the falcon basin |
|
34:01 | right, right, right in there going from, let's see this in |
|
34:14 | case north is on the left something on the right side. I |
|
34:19 | make bottles that way. But in case, so the falcone basin is |
|
34:25 | here and see they made us this . So, so I'm not doing |
|
34:31 | disregard. I mean, I think very believable with these geometries. They're |
|
34:35 | they are using some multiple densities, just very few. So I just |
|
34:40 | their reasons for doing that. It interesting that they have to change the |
|
34:44 | of here, right above the So maybe there's some problem with how |
|
34:49 | densities for use it for that. any case. I still think it's |
|
34:55 | pretty good model and why is the what's going on with that? I |
|
34:59 | , you can see it's high It's interesting that it fends right near |
|
35:05 | end of where the slab it so it's a trans tension all feature. |
|
35:10 | , Because along this margin, You see the same thing like along |
|
35:16 | san Andreas were depending on how the bends, how that and in this |
|
35:21 | , how the subduction zone bends, could have transgression or trans intentional |
|
35:28 | So you can have a case where producing a little basin and right next |
|
35:36 | it, a long strike along the caribbean rim. You can be producing |
|
35:41 | little, you know, convert structures convergence or whatever uplifted area. But |
|
35:56 | you catch my gist with these is that what I'm doing is I'm |
|
36:02 | looking at this and I'm taking what we've already learned about rift |
|
36:07 | passive margins and, you know, basins for our base and just taking |
|
36:14 | we learned from those. And I see elements of all of those in |
|
36:19 | complex zone here. So, throughout , there are uplifts and there are |
|
36:25 | trans attentional basins and structural highs that a result from this oblique convergence of |
|
36:32 | caribbean plate. But you can just that down into the smaller bits and |
|
36:37 | you can understand it in that So this is the uh gua deco |
|
36:45 | , would you say that that What would you say? How would |
|
36:49 | say that? Um Ok, Ok, ok. Yeah. So |
|
37:03 | is this is actually a little four . Right? But it's remember the |
|
37:08 | that produced. It is oblique. um disorientation for these lines seems to |
|
37:19 | should be actually be this way. they did them anyway, they did |
|
37:24 | this way. So this is the sorry, terry Randall. What's |
|
37:30 | So they're calling these geodynamic transect And have reflection data along parts of |
|
37:38 | I think they have refraction data as . Um what we're looking at here |
|
37:44 | residual blue gay from a 10 climber continuation. Just because I want to |
|
37:49 | if you can see any structures in , um residual glue for land. |
|
37:57 | still freer. Right, It's still out here. Yeah, I think |
|
38:02 | , yes. And then yeah. this is the thrust front through here |
|
38:10 | you got the san sebastian, the slip fault and the el pilar. |
|
38:14 | all of this has to do with , you know, the caribbean slate |
|
38:19 | moving east relative to south America. then this range is formed from the |
|
38:28 | and it's produced a little foreland basin . This is the magnetic data. |
|
38:36 | magnetic data, we're looking at that all of a sudden you have these |
|
38:39 | wavelength here. So the basis getting . You kind of get a better |
|
38:43 | for how this basin is formed if can trust this mag data. Um |
|
38:49 | then it's kind of smooth out here you can see that things are shallower |
|
38:54 | then deeper of course. Um There's low over the mountain range here or |
|
39:00 | little this little part of the northern . So I would just interpret that |
|
39:09 | a compositional thing because I mean, don't know, I don't have to |
|
39:14 | if you do it. And in case. Yeah. Um I think |
|
39:18 | gonna. So these are line interpretations reflection data, right? So A |
|
39:27 | a prime is right here and Two B. Prime. So this |
|
39:30 | going right into the well this is this is a four land for this |
|
39:36 | . But then there's a rift The Espino rip Espino grab in which |
|
39:42 | through here. Now. Is this trans intentional feature? I mean you |
|
39:49 | convergence. This is why I'm calling complex examples because or complex basin because |
|
39:56 | here you definitely have kind of an right? For B. And in |
|
40:02 | part of a you have this your classic foreland asymmetric geometry. But |
|
40:09 | right over here you you run into grabbing that's so maybe this is maybe |
|
40:15 | four land again. And I guess how it works. The four land |
|
40:19 | just this southern this this northwestern sort bit from here. Let's look at |
|
40:25 | gravity again. So the four land here and then the sp no drift |
|
40:33 | no grabbing is right there minute next the monitoring base. So. |
|
40:42 | Um Yeah, I don't know, mean you have to play around. |
|
40:45 | see what they did with their So this is going to make the |
|
40:52 | that these are not the whole these just decided that and they make a |
|
40:58 | of these longer profiles. Okay. that the models I'm going to show |
|
41:02 | are these long profiles and they include work from this from, you |
|
41:09 | interpreted from these smaller sections. This my understanding from the paper. So |
|
41:15 | , so here's the little the seismic right in here and right in |
|
41:21 | Mhm. Um Yeah. Okay. look at the range. This is |
|
41:34 | or minus 75 mil ago. So 100 and 50 mila. Go. |
|
41:39 | is. So these anomalies are really anomalies. And what they've done is |
|
41:45 | said there's this little thrust, this cordillera thrust belt, you know, |
|
41:51 | sort of obliquely been, you kind of causing, you know, |
|
41:56 | this deformation here and then you You have this other basis. So |
|
42:02 | Espino grabbing, It's all the way . And it seems to be unrelated |
|
42:08 | this thrusting here. It's amazing I mean, this is, you |
|
42:11 | , you have a grab. The explanation for that grabbing is that it's |
|
42:16 | it's a fossil grabbing right that that formed with with the break up of |
|
42:23 | and the only you can't really figure out with just what we have |
|
42:27 | But that's a possibility. Okay. we can step uh east a little |
|
42:35 | further to the east. Here's our Espino Gavin, here's the Mcferrin |
|
42:42 | It's a big giant and now this a foreland basin and it actually turns |
|
42:47 | a passive margin. It's a four in this direction from Northwest of South |
|
42:55 | , with the 8th symmetric part being here because of the convergence. But |
|
43:02 | here this is a passive margin dipping the south into the, you |
|
43:07 | whatever the equatorial atlantic ocean, the ocean. So way way complicated. |
|
43:14 | we have to just sort of use tools or use what we know about |
|
43:17 | basins and try to investigate that. you can see gravity low right |
|
43:27 | What's interesting to me is that Espino . I mean, it doesn't have |
|
43:31 | of a much of uh you uh it doesn't have much of a |
|
43:38 | signature today. And in fact look what they do, they don't really |
|
43:43 | call this thing a gravity but it seem to be they didn't even model |
|
43:48 | much relief on it at all. fact. Yeah, I mean it's |
|
43:53 | an afterthought, I mean, it's interesting. So this isn't really |
|
44:01 | mean, I I really liked how overlaying this map. I was really |
|
44:05 | with, you know, I like map quite a bit there. |
|
44:10 | Comey their math because they're showing all regional structures. Of course the the |
|
44:17 | time for the subduction zone, but got the ball to matt in |
|
44:21 | in the prism and then the Tobago here. Barbados, there's Tobago and |
|
44:28 | Basin, then all these these these of the great arc that were abandoned |
|
44:35 | the plate kind of scrape them And then it's showing the christian prison |
|
44:41 | top of the caribbean plate as So, and then this little thrust |
|
44:45 | over here. So I think this a really well done matt. That's |
|
44:49 | gravity. This is the bouquet, is okay, so this is boogie |
|
44:55 | freer offshore. But now its bouquet . You want me to ask you |
|
45:04 | I know that. You know the . Um because it's a low over |
|
45:15 | ocean. No, where is Where's the ocean at? This is |
|
45:22 | ocean over here. This is it's the blue over the Venezuela. |
|
45:29 | , I don't know the land goes the way up to here. |
|
45:35 | oh ship. Okay, I'm really on the spot. I'm sorry, |
|
45:45 | promise. I'm smart. So it's it's boo gay because it's a high |
|
45:54 | the ocean crust. The crust is . The mojo is coming up. |
|
45:58 | mojo density is 3.3 crust. Dancing 2.9. So there's a big |
|
46:03 | it's the second biggest density contracts, is the biggest content to contrast. |
|
46:10 | when you move that, remove that , then the second biggest density contrast |
|
46:15 | the base of the crust. So mean many times many ways. |
|
46:23 | so that's bouquet, here's the residual it. And uh you can see |
|
46:32 | trace of subduction zone in the christian doesn't really make much an anomaly. |
|
46:37 | yeah, you can see um before am based in here, you can |
|
46:43 | the shape of the asymmetric shape where getting really deeper, right into the |
|
46:48 | into the foothills. Here's the magnetic . This state is very average. |
|
46:56 | think it's kind of sparsely stations are of sparse. So it's not really |
|
47:03 | what's going on here. But you , but if you just Okay, |
|
47:11 | just gonna if you just ignore areas you know, basically there's no |
|
47:16 | But you can definitely there is some up here. So again, what |
|
47:20 | we know from magnetic data? It's about wavelengths, short wavelengths, things |
|
47:24 | shallow basement, shallow long wavelengths basement deep. So the matter Marine |
|
47:32 | I mean there's some shallow stuff going here. And the Robin the |
|
47:38 | oh grab in and uh Gwahd Ico here. You know, there's not |
|
47:46 | days that the date is pretty, mean it's pretty smooth. So it's |
|
47:51 | with being deep or it's just not . So but this is interesting. |
|
47:58 | you let me just go back and . So the deepest part of the |
|
48:03 | four land, the monitoring basin and just ramps right up onto the Guiana |
|
48:08 | which great parts of our outcropping. so it's getting and you can see |
|
48:16 | how the how it's smooth here. then it's getting shorter and shorter wavelengths |
|
48:21 | though it's negative. Which doesn't mean deep because it's magnetic data. What |
|
48:28 | this blue and red mean? Does mean it's deep or what does it |
|
48:36 | ? Is it I'm sorry. Can repeat the question? So this is |
|
48:41 | data and we know this is getting because of the wavelengths are getting |
|
48:47 | Yet it's colored blue and this is . Why what's going on there? |
|
48:52 | isn't that for me is it steepness shallow? Well I. Yeah |
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48:58 | I was saying that we know it's deeper here and getting shallower because of |
|
49:02 | wavelengths but but the intensity of the one. This is red, this |
|
49:08 | blue this broad blue and this What what does that mean? You |
|
49:15 | ? Wouldn't that just be like a drop like a because if it's it's |
|
49:27 | shallow. That just means it's a park surrounded by why is it if |
|
49:33 | shallower why is it blue instead of ? Why why is the magnetic |
|
49:41 | Blue. Why is it a minimum minimum? It has superimposed on these |
|
49:46 | wavelength anomalies which tells you that things shallow perverse. Yes. Yes. |
|
49:54 | you. Good job I'm there but not I don't know how to say |
|
49:58 | . Okay, the field is That's the only explanation I can think |
|
50:05 | because I know it's getting shallow. shield is the outcropping shield is right |
|
50:11 | and this actually shows you terrain within outcropping shield, right? Because you |
|
50:16 | see that this is changing. So are not, you know, are |
|
50:22 | the same everywhere, so Okay um , so we're gonna, this is |
|
50:29 | are cross sections, you can see down here below and these cross sections |
|
50:33 | going from, these are kind of . It should be northwest on the |
|
50:37 | side for me, but they're doing southeast to northwest. So they're going |
|
50:44 | from close to the shield Into the land base. And so this is |
|
50:50 | to show you the japanese, these on two way time, but you |
|
50:55 | see that you're coming up onto the , right? The base is |
|
51:01 | you know, it's the deepest part you know, classic asymmetry. So |
|
51:07 | are going, those are going from southeast on the left to northwest on |
|
51:13 | right, so they're coming right right off the shield into this four |
|
51:20 | , which is, you know the geometry, you know, I look |
|
51:25 | this for a while. What is thing, what's going on then? |
|
51:27 | realized that they're not, you most people would plot this northwest of |
|
51:33 | , you know, because because they're , you know, in that way |
|
51:38 | , I don't know. Um so um we're gonna end our little |
|
51:48 | along the southern caribbean rim kind of into an area inside this motorin uh |
|
51:58 | and its river basin? S premier Espino grabbing. There's another line |
|
52:05 | A model to model was that was along these seismic refraction stations. And |
|
52:11 | had some wide angle reflection data as . So in here there's there's the |
|
52:18 | of squares, uh um White stars shot point squares are recording points. |
|
52:24 | receivers and shots and okay, there's kinds of three kinds of recording |
|
52:34 | And then here's that on top of bouquet anomalies. So again, here's |
|
52:40 | right, here's the outcropping Guiana Here's our little four land turns into |
|
52:45 | passive margin as you go to the of to the coast. And then |
|
52:51 | Espino grabbing is right over here. the magnetic data. Remember here's our |
|
53:00 | polarity. You can see the depth the base and you can see the |
|
53:04 | getting deeper as you go to the . And then all of a sudden |
|
53:07 | gets shallower. Again, all these wavelengths here. And this is their |
|
53:15 | . So this is their model they with basically with the seismic velocities. |
|
53:20 | then these are all velocities posted So this, remember we looked at |
|
53:28 | last 5.55.9. So this is this probably the, I wouldn't make it |
|
53:34 | deep. I would make it I think 5.9 is a little high |
|
53:40 | um I guess it's okay. I that's okay. You can make that |
|
53:43 | top of the basement And then 6.0 6.7 into lower crust. 8.1. |
|
53:51 | definitely mantle. So yeah. here's a question. How would you |
|
53:57 | these velocities to density? What would do? Um converts into dense |
|
54:10 | Oh, there's a formula. Um right, that's right. There's |
|
54:22 | the velocity velocity to density conversion. , so and then here is oh |
|
54:30 | the gravity model. So here's the model and here's the gravity model for |
|
54:38 | . So they're calling this the oriental . But this is the most |
|
54:42 | this is the most serene. And don't know if this shape is if |
|
54:45 | like the shape that much. But , upper crust lower crust. |
|
54:53 | quick question for the for the I mean, I know there's a |
|
54:59 | but it's not like the because I it's like mass divided by volume. |
|
55:04 | how do you know that? You do the mass. So what was |
|
55:07 | name of the formula that we use ? Are you can quantify, I |
|
55:14 | you a table. I showed you table. Um And there's a settlement |
|
55:22 | like Gardner. Um I think I it right in here. Hold |
|
55:28 | I'll show it to you. Um actually think I did that with dr |
|
55:39 | like the both module assess and okay. I was just like, |
|
55:44 | know it's not like I see Oh no, here it is. |
|
56:09 | right, there's a paper by bro that summarizes a bunch of these |
|
56:14 | Um Jerry Gardner used to teach at University of Houston, Really smart |
|
56:20 | Um he did a bunch of laboratory and that's probably what you learned. |
|
56:24 | gardener equation. Um can you see screen? Can you see the table |
|
56:38 | ? Okay, so there's the knife which is from Ludwig and others in |
|
56:46 | of the volumes of the C Right? People still use it like |
|
56:54 | and that's this black line here, black diamonds. So the velocity in |
|
57:02 | per second along the bottom axis and and gravity per cubic centimeter in this |
|
57:08 | one. And then christian ceremony have some of this work and they for |
|
57:14 | . That's plotted on this here. Godfrey and others have done some here |
|
57:22 | culture actually summarized all this work. um jerry Gardner did did laboratory measurements |
|
57:31 | individual rock compositions, types, sandstone shells, limestone, salt, |
|
57:40 | and hydrate. That's all these other little ones. Right? So if |
|
57:45 | have your velocities, you just go this thing, you can just look |
|
57:49 | up but there is a formula Here it is. So this is |
|
57:55 | is in meters per second. So one, these are the terms |
|
58:01 | The the whatever the uh right, this is, you know, this |
|
58:13 | . Right? Uh It would be a 0.32 plus one point oh five |
|
58:19 | 10 to the minus three X. mean x data accident, Y of |
|
58:25 | . Why is it density? And this is like X one, X |
|
58:29 | x cubed X. You know like . So you can actually fit |
|
58:35 | oh wow, you can actually fit to these. So someone did this |
|
58:42 | me and then they see they even the whole derivation down here. What |
|
58:52 | this mean? Does that mean the too big for the for the |
|
58:56 | I'm not I'm not an Excel They did it in feet per second |
|
59:02 | well. Solid. Yeah, because a there's a there's a number there |
|
59:12 | , whatever. So yeah, so how you would do it. So |
|
59:17 | would look at those um you look at these velocities, you could |
|
59:24 | do that. I mean this is , you know, this is not |
|
59:28 | a two D model, this is a continuous function. So you can |
|
59:33 | do that continuously for here. All different velocities. So that's what they |
|
59:39 | 2.89 C2.8 something around there. So was that? 2.8 something or |
|
59:44 | Yeah. Anyways, I should get table back up. Okay, so |
|
59:52 | see what they did. So they 8.1 is 3.3 and So 8.1 is |
|
60:04 | over here so see that's right about right right there it is. I'm |
|
60:10 | looking at Nate Drake 2.8522 point They 2.52.92 for lower across 2.85 2.92. |
|
60:21 | that's 6.5 kilometers 6/6 kilometers. And was yeah I don't know 7.1 |
|
60:37 | That gives me at 6.5. Yeah don't know. Anyways that's how that's |
|
60:45 | you could do it. But this pretty typical. I mean you know |
|
60:50 | have they have I guess this outcropping up here so you have to catch |
|
60:55 | anomaly by changing the geometry of the of the crust. Now. That's |
|
61:01 | not a bad thing because I mean you only have one thing to do |
|
61:06 | all you can do. So that of gives you some you know kind |
|
61:11 | pins down this part of the model a way. Right? I mean |
|
61:16 | if you change anything in here you change everything. So that's okay. |
|
61:25 | crust That's tank oceanic crust is like km sick. Um Yeah I don't |
|
61:34 | so. Oh yeah I think I I think everything in here is I |
|
61:49 | this whole thing I think everything in is dinner. So this is going |
|
62:00 | to 40 con like I don't The only way do they have, |
|
62:07 | a second. They have refraction data you, don't they? That must |
|
62:15 | what these are 35. I'll bet that's what these lines are here. |
|
62:20 | are from their stations because they have these refraction stations here. That's |
|
62:27 | That's really sick. So what does mean? What does that mean? |
|
62:35 | how far just go? Let's look that. So why Star Shop |
|
62:45 | So does the model go all the ? Doesn't even go to the |
|
62:51 | does it? Oh wait, the is right here. The coast is |
|
62:59 | here. So the market goes way beyond the coast. Oh, |
|
63:04 | dash line. But it doesn't really . Okay. I don't I don't |
|
63:09 | how far it goes offshore, but goes up quite a bit. I |
|
63:14 | know. I think, I think way too thick. I mean, |
|
63:19 | don't know if this part is thinking , you know, the hot |
|
63:23 | but I don't think so. I think there's a I think there's |
|
63:29 | issue here. Yeah. Alright, just move forward. Ok, so |
|
63:38 | flood the salts. Remember? Large provinces. They can exist also on |
|
63:45 | here. The Siberian traps. Here's Columbia River basalt. These are on |
|
63:50 | . The deccan traps are actually um part of India India is very faded |
|
64:00 | , but that's all on top of . So they can also exist on |
|
64:05 | And then remember that I have the , the paranoia over here and the |
|
64:10 | flood basalt are really, uh, steel. The volcanism covers an area |
|
64:18 | 1.2000 km2. Um, they estimate km3 of basalt. So yeah. |
|
64:30 | it's those assaults sit atop overlying a called the paradigm basin. So that's |
|
64:40 | , I mean, they're, they're big. So they're huge, |
|
64:46 | The decade traps flood the salt. from the reunion hotspot, that |
|
64:52 | It erupted a big outpouring, but one actually lived longer and produced hotspot |
|
64:59 | all the way down into the indian . Here's a picture of it right |
|
65:05 | and the thickness of them Up to km. Now, wait, most |
|
65:12 | this is in the range of I think. I don't know why |
|
65:17 | might be some, I don't but this is what they look |
|
65:21 | Just alternating layers just flooded. You've of, you've seen the Colombian, |
|
65:27 | assaults, Have you seen Colombia? , structuring whatever columnar basalt? |
|
65:36 | yeah. And then here are the traps. Now they're not very thick |
|
65:40 | all. But look at look at is from the ocean, how they're |
|
65:47 | to erosion there. Good, except traps. Okay. They erupted in |
|
65:55 | , their pennies look in the um, Their thickness, their main |
|
66:01 | seven, only 700 m. So not as thick, but they're all |
|
66:08 | here on this side of the western Canada basin huge. And then we |
|
66:16 | our own here in the United we have the Columbia of river basin |
|
66:21 | a Columbia plateau right here in Washington Oregon. And then here's the extent |
|
66:28 | the flood assaults. The Columbia, river basalt, I guess is what |
|
66:34 | call them. And uh they they're c they're Mycenaean age. So there's |
|
66:46 | bunch of wells in here and there some exploration, they actually drill, |
|
66:52 | drilled through the Columbia flood assaults, are about 11,000 ft and they produce |
|
67:00 | from them out here in the Washington the, you know, eastern |
|
67:06 | Um And then here's the cascades come here, right, and then right |
|
67:13 | and then the coastal ranges are out , right, right through here. |
|
67:19 | So this was, I've been up three times the first time I did |
|
67:23 | little project for a company, they to, you know, a little |
|
67:27 | company in southern Southern Canada in british and they wanted to explore for some |
|
67:34 | . And because this is right, know, it's right near there, |
|
67:36 | markets, there's lots of population and guy was working for, he was |
|
67:43 | local geologist in Tacoma and he asked if I'd ever been out there and |
|
67:48 | said no, he said, well got to come out to there, |
|
67:50 | got to see that, you got see the basin, which was very |
|
67:54 | . He was a total geologist and spent like a few days, you |
|
67:58 | , exploring the geology out there. course this is wine country. |
|
68:03 | you know, we had a pretty old time. Um The winds out |
|
68:10 | just F. Y. I. is this is a really important |
|
68:16 | The winds out here, the best are west of the river, see |
|
68:21 | Columbia river comes down here and it out that it's the border of Washington |
|
68:25 | Oregon. It's east of the And there's a little college town of |
|
68:31 | , Little Liberal Arts College in a called Wallawalla right here in us |
|
68:38 | You stick east of the river, of Walla Walla and north of the |
|
68:44 | north of the state line. There's 300 wineries in there and the wines |
|
68:51 | this part of the Columbia River Basin ridiculous. They're as good as anything |
|
68:56 | California, I swear. Um It to do with some flood flooded soils |
|
69:03 | came down here, but it also to do with the assaults. You |
|
69:08 | , I mean, the meteorology of assaults, It's really good for |
|
69:11 | so yeah. Um Yeah, so , that was sort of like an |
|
69:17 | I guess. Um Okay. Uh you want to take a, I've |
|
69:24 | talking about our 20 you want me , I only have, I probably |
|
69:28 | have maybe, I don't know Less 10 slides to go to finish this |
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69:35 | . You want to finish this and take a break. Yeah, that's |
|
69:39 | . We can finish this. alright, so okay, so back |
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69:44 | the serious business now. This this a busy figure, but here's a |
|
69:48 | map of the Columbia River of There's the, the Yakima fold belts |
|
69:53 | are big long basalt and declines, there's a there's a plot here, |
|
70:01 | a gram here and the left side kind of wraps around things and what |
|
70:07 | showing is it showing that there are are six units. I think there |
|
70:10 | more. I think there's 12345. seven different units, but these are |
|
70:16 | six of the units that have the outpouring of the salt by volume. |
|
70:24 | whole basin is filled up with the , right? And by volume, |
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70:29 | is the different units. So the one, the biggest one by |
|
70:33 | 85% of the assault in here are grand run assaults. And over here |
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70:40 | the timing, here's our little chart millionaires 17 million. This is all |
|
70:46 | . The Grand Run erupted at about I guess 15 0.75 M. |
|
70:54 | Right here. The very first ones here, about 17 M. |
|
70:59 | But it wasn't very much. In this Uh that's this one right |
|
71:06 | so it's just about 5%. And um this one's not here. Snake |
|
71:13 | . Snake River is not there. , Snake River, that's down |
|
71:18 | that's why. Okay, this is just from the Columbia River. There's |
|
71:22 | couple different this is back seat for material here. And this is this |
|
71:27 | plots from Tolan. So I'm kind crossing things up. But anyways it's |
|
71:33 | to look at this because this is very favorite geomagnetic polarity reversal scale which |
|
71:40 | identified five A. Five B. and so forth. Five C. |
|
71:44 | here. Okay, five B. . R. Means reverse. See |
|
71:50 | solid colors are positive correlation. And at the Grand Run. The Grand |
|
71:55 | is negative polarity and we know that from rock samples. Okay, so |
|
72:05 | it erupted during 5b.1 are the normal for these crowds. It gets pretty |
|
72:12 | because every time we get more data keep subdividing these things. But |
|
72:18 | that shows you the the deposition of difference. Assault units in the Columbia |
|
72:25 | . Um Remember the wells. So some cross sections drawn through the |
|
72:31 | This one starts in the northwest To a prime and it connects up |
|
72:36 | these different wells. And the basalt . Is this sort of plus symbol |
|
72:41 | . This center here. So there paleo jing sediments. But ain't that |
|
72:46 | there's I think paley uh there's a I know maybe a legacy. I |
|
72:53 | there's a scene and a legacy. if I remember correctly and then you |
|
72:58 | the and then you have you have know, sediments piling on top of |
|
73:03 | . So that's what's happening now. is the ice a pack of the |
|
73:08 | run in terms of meters. So 800 m to over 33 a half |
|
73:15 | thick this unit. So it's really . It's a bunch of it's a |
|
73:20 | pile of assault without a doubt. , now going from southwest to northeast |
|
73:29 | through, you know, we're crossing of the one of the same wells |
|
73:32 | think to be in 19. That's show. Yeah. B. |
|
73:36 | 19 is intersect that well was No, maybe I think it was |
|
73:41 | maybe Shell or Exxon. And it's this one was a gas producer and |
|
73:49 | , so this is the the other section. So it's really well |
|
73:54 | I've made probably here there are four that I made through here. But |
|
73:59 | probably made You know 10 more. mean there's the paper there but I |
|
74:06 | to get someone to release that in case. So here's the topography showing |
|
74:12 | showing the contours the ice pack of of the flood assault unit and here's |
|
74:19 | bouquet gravity. So finally getting some , all that background material and it's |
|
74:24 | big gravity high this is a big high over a basin. It's a |
|
74:30 | broadway that it can mean a lot things. It could be crustal, |
|
74:37 | could also be what else It could crossed also what else could it |
|
74:51 | What is the density of the It's um Oh my gosh. Very |
|
75:02 | don't think I asked you to. it's it's the density of the salt |
|
75:07 | like the density of ocean floor. . So in our two D. |
|
75:11 | , what was the density of the upper oceanic crust? Oh we didn't |
|
75:16 | do that. We don't even do . Never mind. So it's it |
|
75:20 | be it should be on the order 2.8. So and when you compare |
|
75:27 | with the density of sediments, do have a do you have a sense |
|
75:33 | density of sediments? What they would to be. Remember a little exponential |
|
75:37 | function? Yeah. It was like . know how far Between there and |
|
75:48 | did it go up to? Was like 2.3 or 6? Getting there |
|
75:55 | a little a little plot went from to 2.7. So I mean 2.7 |
|
76:03 | really hot for sedimentary rocks. I give them more like 2.65. But |
|
76:10 | basalt are 2.8. So what does mean? Look at that? Look |
|
76:13 | the ice pack how thick it is compare the density of basil to the |
|
76:19 | of sediments? So just Mhm. mean just that big red area. |
|
76:35 | just that's the high density. Well I mean the can too I |
|
76:42 | if the assault is constant density it's filling it up. Right. I |
|
76:48 | it's just hired. That's that's one . So it could be a |
|
76:53 | it could be crossed it could be density contrast of the thick of the |
|
76:58 | with dense with sediments. Any other it could be. Is this the |
|
77:07 | ? No I said that I say crustal. I mean that's what I |
|
77:14 | . Yeah the thickness of the What else could it be? Let's |
|
77:21 | Mount Hope salt down. No no out here. It could what would |
|
77:28 | think about processing? Okay. What's what is the bouquet correction? Dancing |
|
77:46 | ? What is the book? A , density correction density. Remember I |
|
77:55 | a big deal. I said it's the same. No matter what. |
|
77:58 | though it doesn't make any sense it's the same number. Oh um You |
|
78:05 | it's like a legacy data. If bouquet you can back out the bug |
|
78:10 | correction and you know what that number gonna be. 2.67 Oh that's granted |
|
78:22 | it? That's actually courts but But yeah so. Right that's what we |
|
78:30 | think from our from our plots that went through was granted was the average |
|
78:38 | or something like that or 2.662.66. got our test here because you answered |
|
78:48 | question correctly. 2.66666. So two 67, which is very close to |
|
79:04 | , right? Very good, very . Um so what it could be |
|
79:09 | you don't remember this is this is topography is flat and it could be |
|
79:17 | bug a correction. So it could a lot of things. I |
|
79:23 | And how would you figure that What would you do to figure that |
|
79:27 | if it was crustal or or if was the contrast with sentiments or if |
|
79:32 | was the the bouquet correction, how you figure that out? Couldn't you |
|
79:38 | look at your mag data? you just make a model through |
|
79:44 | stick in those values and see what . Yeah, you just you just |
|
79:49 | a model of that would help you figure it out. That's true of |
|
79:51 | lot of things. But now speaking MAg data just here it is now |
|
80:04 | is a mess, right? I it's just full of high short |
|
80:08 | you know, chatter and that's because the assaults right there at the surface |
|
80:14 | near the surface. So you're getting that catches. There are some longer |
|
80:18 | though in here that these things are opposed on. Um Now these blues |
|
80:27 | reds, they don't bother me that's telling me it's reversed polarized. There's |
|
80:31 | some remember all these but here's the that I think is interesting is that |
|
80:37 | are a lot of positive anomalies, though the grand run is reversed And |
|
80:43 | is 90% of these flood. That's interesting to me. That's really |
|
80:57 | I'm gonna send, I'm gonna send note with friends of mine because I'm |
|
81:05 | send a note. Terrific blakely about . He's done a lot of work |
|
81:12 | here. Um Okay, anyways, , right, so um yeah, |
|
81:34 | you're looking at here is just very way. I think its surface |
|
81:37 | Um we can look at that Um Again, this this is, |
|
81:45 | some blake, here's some map from work here. Both of these are |
|
81:50 | he's showing um, gravity anomalies here , different color scheme. And he's |
|
81:58 | some modeling in here and here's zooming here that the Yakima fold, Yakima |
|
82:06 | belt. I know that. I , I don't know what T stands |
|
82:10 | , but it's all these little lines outlines of the Yakima fold belt and |
|
82:18 | see them here again. So, the Columbia River, Columbia River over |
|
82:23 | is um it's right here is right , Columbia Washington. I don't, |
|
82:40 | , can't find a ripper doesn't haven't in, but it has to |
|
82:45 | oh, there it is, right . There's a Columbia river right |
|
82:48 | Um but you can see those four in the magnet. Look at |
|
82:52 | a lot of these lines are lining up with the full belt here. |
|
82:56 | are there now, blood vessels. liquid right there. They have a |
|
83:07 | , low viscosity they flow. So in the world is producing these these |
|
83:16 | lines. These are all structural. big fools, big declines in the |
|
83:22 | of this, of this, of basin, of the of the on |
|
83:26 | of the plateau here, there's many them. Um Let's see where are |
|
83:32 | at? He's modeled some of Like this line here goes right through |
|
83:37 | . He's modeled some of these Um What in the world are |
|
83:45 | We're gonna look at that in a . But I think I got another |
|
83:48 | study here by withers. Withers. . Um he's saying there's an unexplored |
|
83:55 | tectonic basin just to the south So here's one of these big giant |
|
84:05 | uh falls here right here. And one of these folds up here. |
|
84:13 | see this is the blue mountain and . It's one of these basalt |
|
84:18 | Let's see cemetery rocks and the site yeah, right. Columbia River. |
|
84:30 | , I see. Everything is Columbia basalt except was recorded at the city's |
|
84:35 | . Okay. Um so, uh says that he did some gravity modeling |
|
84:47 | Dave actually. So this is a data showing the the uh the base |
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84:52 | the basalt right here. And he that it's prospective beneath it. |
|
84:57 | I guess, I think I'm just you this. Oh, yeah, |
|
85:01 | . And then this is where he the models. So, this model |
|
85:04 | is right here going from northwest to . And it's right, you |
|
85:11 | it's right on the flank of this basalt thickness. And here's here's the |
|
85:17 | model right here. There's three different of the same model where he has |
|
85:23 | , which is, that's Columbia river , which is just thick bit |
|
85:29 | And then um, then he has other john day and clerical and the |
|
85:40 | , the hair and are the different , these are page in sediment |
|
85:46 | So he's thinking that there's a there's basin in here based on this |
|
85:51 | Yeah. So, okay, let get back to this part again because |
|
85:58 | a question I want to ask You have all these assaults, these |
|
86:04 | lines that have formed on top of basin, on top of the |
|
86:08 | And the here, this is really good figure in the Yakima fold belt |
|
86:16 | . Um, but the salts they don't like make an declines. |
|
86:24 | these these antique lines are actually, know, growing today. In |
|
86:33 | I stomped up on one of We pulled over, I went right |
|
86:37 | on one because there was some beautiful columnar assault blocks. And I had |
|
86:43 | . I had one of lining one the beds in the backyard. I |
|
86:46 | up with a suitcase that weighed £28 came back with the same suitcase laying |
|
86:52 | £50. So I took a big giant from up there um in any |
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86:58 | Um uh uh what do you think causing these things to, what's causing |
|
87:09 | folds? I mean they're growing today right out who used to be a |
|
87:14 | up there at this university up in . I was talking to him about |
|
87:19 | and he told me that. he said that they're growing like |
|
87:22 | a few centimeters a year or something that. I mean something, some |
|
87:27 | that's actually measurable. So what in world do you think is causing |
|
87:37 | Could it be um I don't want say like a hot spot, but |
|
87:43 | like still erupting underneath or something causing to uplift. Well you're thinking in |
|
87:48 | right direction. So let's think about another way. Do you remember that |
|
87:53 | show you a, did I show a heat flow as a function of |
|
88:00 | age plot? Didn't I show you ? Or did maybe I didn't. |
|
88:04 | don't know. I believe so. . So what's the time frame on |
|
88:09 | flow is a function of age. drops quickly over the first how many |
|
88:22 | ? I mean, it flattens its log rhythmic, right? It |
|
88:25 | drops and then it just flattened, plateaus out. I don't remember the |
|
88:34 | off the top of my head about million years. So if you go |
|
88:39 | to this mid atlantic ridge is and met there their depth as a function |
|
88:46 | age? They all flattened out 20 40 million years. When did |
|
88:55 | when did these eruptions happen? What I say? You said these eruptions |
|
89:10 | ? No, that was the I'm just looking for one. |
|
89:19 | sorry, You have it on the . Okay. Yeah. 16 - |
|
89:30 | . They're my C. Okay. . So 16, 17 million years |
|
89:37 | . Where would that be on that of of the ocean cooling? They |
|
89:46 | still have a lot of cooling to , wouldn't they? Like in the |
|
89:50 | ? Not even Right. I I think these are from cooling. |
|
89:58 | think their wrinkles, some people have to say that they're from some sort |
|
90:05 | structuring, but they're they're all different this way this way. This |
|
90:11 | they're all different directions. I think are wrinkles on the, around the |
|
90:17 | , the basin is still subsiding and wrinkles and and that's and that's why |
|
90:22 | still growing. Hmm. Some people like that idea a lot because they're |
|
90:31 | invested in other ideas, but but mean, I'm just thinking, I |
|
90:35 | , you look at their different What in the world's wonder what's causing |
|
90:39 | ? You know? I mean, me it's just Yeah, Anyways |
|
90:44 | that's enough. We can take a . It's 2 43. You want |
|
90:48 | come back at three o'clock. Alright, Okay, so The last |
|
91:02 | . this is going to be gravity and hate flow thermal properties. This |
|
91:07 | kind of like he follows still a field. So I mean it's all |
|
91:13 | fields. This is extra stuff this I haven't taught before so we'll see |
|
91:19 | it goes. Um I think what gonna do is I'm gonna start with |
|
91:26 | flow and then go back to gravity and then I might end up just |
|
91:32 | the time to introduce gravity gradients. you understand conceptually what's going on because |
|
91:38 | went through those slides this morning and there's just a lot of lot of |
|
91:42 | histories and a lot of high highly stuff and I don't know if we |
|
91:49 | I don't really know if yeah maybe can just uh maybe I'll just start |
|
91:56 | the heat flow. Um Where's that ? Here we go. Yeah I'll |
|
92:06 | with heat flow and thermal profit. is stuff I've been actually working |
|
92:12 | I don't know if you know I a presentation that the experience of field |
|
92:17 | last month a couple weeks ago and I made I'm making one next week |
|
92:21 | the G. S. H. luncheon. Uh Same material, it's |
|
92:26 | be heat flow and and uh machine predicting heat flow. So f. |
|
92:36 | . I. That's going to be Wednesday. It's gonna be online too |
|
92:40 | you can watch it. Are you member of the local societies Geophysical geological |
|
92:47 | I believe so I don't I think needed a new my membership, it's |
|
92:50 | up but yeah it's always it's a idea to be a member of you |
|
92:56 | , a couple whatever international groups like S E G A P. |
|
93:00 | But also your local ones, the . S. H. And the |
|
93:03 | G. S. Because you know in Houston because you know you get |
|
93:07 | good quality presentations, there's no shortage material being being presented. I mean |
|
93:15 | you look at like the the if like the calendars for like the Permian |
|
93:21 | or the Dallas Geophysical Society, there's on it. I mean they got |
|
93:25 | planned. So it's the Houston is very societies are very active because there's |
|
93:31 | many people obviously anyways. Yeah, a good idea to to to to |
|
93:38 | those things and check it out Okay, so heat flow definitions, |
|
93:43 | flow, the formula of heat this is called Four Years Law. |
|
93:49 | it's just basically the it's the thermal D. T. D. |
|
93:55 | Or in this case dy but for we think in terms of up and |
|
94:00 | time and it's just scaled by the conductivity. So heat flow is flux |
|
94:06 | like gravity field or a magnetic field It's it's the the units are mila |
|
94:12 | per meter squared so that is Um And thermal conductivity is a linear |
|
94:20 | . It's just a measurement. It's the right here. I wrote it |
|
94:24 | the rate of temperature increase within the as a function of depth. In |
|
94:28 | words, I'm sorry. That's the conductivity is down here. Yeah, |
|
94:32 | just a Iraq's ability to trance trance transport thermal energy. Right? And |
|
94:40 | just it's what's per meter kelvin is unit. I don't have them |
|
94:47 | So he follows something to thermal gradient by thermal conductivity, right? Hate |
|
94:54 | . Production in in the earth is associated with crystal and rocks in the |
|
95:02 | continental crust. Because it's old, still a lot of radioactive elements like |
|
95:08 | and potassium and thorium. And as decay, they produce heat. So |
|
95:14 | heat production. Oceanic crust is thought to be is not to be able |
|
95:23 | produce heat because it's you know, recycled. There's no it's it's the |
|
95:27 | they use to describe oceanic crust is , depleted in radia genic sources, |
|
95:34 | other words, radio developments. So , and this is why oil and |
|
95:40 | . People who explore for oil and , I don't like to be on |
|
95:44 | of oceanic crust because they don't think there's one, I don't think there's |
|
95:49 | source rock on it. And to don't think there's any heat source or |
|
95:54 | any heat, there's background heat coming from every part of the planet. |
|
96:00 | ? But there's but there's but for you get background heat also called reduced |
|
96:10 | plus radio genic heat. So heat is a knot and then d is |
|
96:17 | thickness of the heat producing layer. is not really, it's the thickness |
|
96:26 | the layer, I think. So is written um by his chief and |
|
96:33 | the folks that do this heat production , they're always working at outcropping |
|
96:38 | So they have what they call the depth of of the characteristics depth of |
|
96:48 | heat producing layer. In other words standing on the top of it because |
|
96:54 | working on an outcrop, then you , the bottom of that is actually |
|
97:00 | . Which is the thickness of but for a basin you're not standing |
|
97:06 | it. So it's actually the thickness the heat producing layer, not the |
|
97:11 | of the basement. So that's a it's a little, it's a little |
|
97:16 | , a little wrong. They're basically is the thickness of the heat producing |
|
97:22 | and anna is heat production. Um , so what you measure over continents |
|
97:31 | the background heat flow plus the heat just over ocean, we just have |
|
97:36 | one variable. Okay. And what chapman found was that um from a |
|
97:44 | study That the background heat flow is , the signal um 3/5 of the |
|
97:52 | flow. And that means that the produced by radojevic sources, it's two |
|
98:02 | . Okay, so yeah, this just the units again, mila watts |
|
98:06 | meter squared, which is flux heat is micro watts per square meter. |
|
98:13 | note that if you go back to equation here, this is, this |
|
98:17 | volumetric for cubic meter, but this distance in terms of meters for |
|
98:23 | So that means the meters cancel And the second term is flux. |
|
98:30 | , watch premier covenants, linear. . Alright. So I was explaining |
|
98:37 | about heat production and how it's So this is a really nice |
|
98:41 | how that formula works that in By the way this formula down |
|
98:46 | this is what I'm calling equation That is a empirical formula and it |
|
98:53 | that was discovered given a credit to guys named Birch and others in 1968 |
|
99:04 | some obscure journal. Not, I a book. It was in a |
|
99:08 | of the book. Okay, So how it works. They go out |
|
99:13 | to an outcrop, several outcrops in in a whatever zone or a particular |
|
99:21 | that sort of uniform. And they a device that measures its heat |
|
99:27 | It probably some kind of a Geiger that measures radioactive decay. And then |
|
99:33 | do some math and figure out what heat production value is according in terms |
|
99:38 | micro watts per cubic meter. And they plot that for each terrain plus |
|
99:45 | error bars. And then they also heat flow. So they have some |
|
99:51 | drill down a little hole and they a unit and they measure, you |
|
99:56 | , they measure temperature in two places then they measure that depth and then |
|
100:02 | measured thermal conductivity. And so they heat flow. Okay, so they |
|
100:07 | heat flow in the same location as sample from the production with the error |
|
100:13 | on that. So what you're looking is all these different these seven different |
|
100:17 | is plotted with error bars. So once you do that, you can |
|
100:24 | that you can find the best fit line through those. And and that |
|
100:31 | line. The slope of that regression that is D. Oh, that |
|
100:40 | D. D. Is the slope the regression line. And it's also |
|
100:44 | thickness of the heat producing layer. where that intercepts the intersects the |
|
100:54 | the y intercept that is Q. the background heat flow. So background |
|
101:01 | flow is here. And then you D. Which is that. And |
|
101:10 | have the heat production values. And you you can satisfy that equation and |
|
101:18 | equation. So that's how that So this is a little figure |
|
101:22 | this is what I was talking about . You have background heat flow, |
|
101:26 | is everywhere. And it's from comes from beneath the little sphere. And |
|
101:33 | you have heat flow that's produced by continental crust from radioactive decay. So |
|
101:40 | little cross section here shows a passive , you know, ocean basin, |
|
101:46 | margin, rift basin, continental upper and lower and then the upper |
|
101:51 | is kind of shaded black. And also showing it. And of course |
|
101:56 | mojo, which is the basic I'm also showing you to temperature horizons |
|
102:03 | dashed lines. So the look of dance your boundary which is called the |
|
102:07 | . A. B. And the point depth. Those are both temperature |
|
102:12 | so they can be found in But they also have a temperature associated |
|
102:17 | them. For the L. B. It's thought to be about |
|
102:20 | 30 degrees. Kingery Carry point is temperature at which rocks gain or lose |
|
102:29 | magnetization. Alright so and in this 580. That's for magnetite. So |
|
102:38 | , if you're heating it up once hits 580° it will no longer be |
|
102:44 | . And once it cools back down 500° it will become magnetic. So |
|
102:53 | remember we did death to source So we can map the basement surface |
|
102:59 | magnetic anomaly. We can also map key point depth from magnetic anomaly |
|
103:08 | Key point is thought to be produced the very longest wavelengths um in the |
|
103:15 | after after of course it's core corrected you remove the I. G. |
|
103:19 | . F. Dead. And so then of course we learned about depth |
|
103:25 | estimation. And so the basement. this magnetic layer is um is where |
|
103:35 | continents is where you have radios being from. So we actually see what |
|
103:47 | this say. This says the remaining makes use of magnetic Permian basin. |
|
103:52 | we did a study uh me and colleague and uh beneath the premium for |
|
103:58 | Permian basin. We we did a of uh magnetic layer and tried to |
|
104:05 | determine different thermal parameters, thermal So the idea is of course we |
|
104:14 | to use debate the curie point death of the L A. B. |
|
104:18 | it's, you can map it with data. We mapped a near surface |
|
104:24 | using open file borehole temperatures and then define pre temperature horizons, the near |
|
104:34 | temperature and the temperature at the basement . And then of course, we |
|
104:40 | the Cherry Point Championship. And then those three temperature horizons, we congratulate |
|
104:47 | thermal gradients between those and other thermal . So let me just work through |
|
104:53 | and I'll show you what I'm talking . So, again, here is |
|
104:55 | Permian basin. As we've seen This is the topography, here's the |
|
105:02 | basin, the middle air base in basin platform. This is whatever the |
|
105:07 | arts, the Val verde basin and Marathon or genic bill. Now, |
|
105:14 | is um heat flow stations, these circles, there's some thermal conductivity |
|
105:21 | these green and yellow circles and there's heat production stations down here in the |
|
105:27 | plus sides, there's a basement So the basement ranges, you |
|
105:35 | uh over over a kilometer deep. sorry, it goes from a kilometer |
|
105:41 | over six km deep, which is right most most remember most platonic basins |
|
105:48 | only about maybe seven km deep You can really see the shape of |
|
105:52 | base in here too. Um and here's the, oh sorry, So |
|
106:00 | the basement with contours and here's the without country. It's okay. And |
|
106:06 | heat flow. Miller asked for me square uh just credit up those stations |
|
106:15 | then here's another review of what we for years. Law. This is |
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106:21 | equation, this is the empirical equation birch and this is the relationship of |
|
106:29 | and chapman. Now there are two sources, there is heat flow heat |
|
106:38 | sourced from deep in the earth beneath little sphere. And there's heat that |
|
106:44 | in the crystalline rocks. But but been recognized for a while that there's |
|
106:49 | heat produced um in the sentiments, for example, if you have some |
|
106:58 | , these are all plastics by the . So if you have some classics |
|
107:02 | are eroded from them from nearby mountain , like in a foreland basin, |
|
107:08 | may, they're probably not going to well sorted. You might have minerals |
|
107:13 | in there that include uranium and thorium potassium elements. So you can have |
|
107:21 | flow in particularly plastic rocks in cemetery . This is understood. It's very |
|
107:27 | though, right? So, so folks sushi and others Developed five different |
|
107:37 | based on heat production values of ranging from 0.5 to 1.5 micro watts |
|
107:45 | cubic meter. Um And this is they plot. Uh here's here's how |
|
107:53 | well, using these calculating these they can they can also calculate heat |
|
108:03 | as a function of base and Okay, so this is the heat |
|
108:08 | versus the thickness of the base. you can see they range from, |
|
108:15 | know, for the deepest part for kilometer basin, deep kilometer basin, |
|
108:19 | is very, very thick Up to million square. But really, what |
|
108:26 | are we in? We're in a of around here. Most platonic bases |
|
108:30 | around here. So now we're down less than 10 million watts. So |
|
108:35 | can see it's not a lot. in fact, the Permian basin, |
|
108:39 | use function three just because it's in middle Permian Basin is about seven kilometers |
|
108:47 | . So right about here. And means it's about a maximum of adding |
|
108:53 | million watts per meter cube. what does that look like? |
|
108:56 | here's the range of heat flow. flow goes from basically, you |
|
109:03 | uh let me see, we're in in the light, the greens, |
|
109:08 | goes from about 35 to almost 100 this thing. Well, six million |
|
109:17 | premiere six. gonna watch per meter , is not really that much, |
|
109:24 | it? So, anyways, it's correction that we made. Um here's |
|
109:29 | station data and this is um the of right, okay, so that's |
|
109:36 | correction that we make. And the thing is to make the near surface |
|
109:39 | . Right So we take the well's take the well depth. This is |
|
109:45 | the T. D. S. you can calculate the temperature at the |
|
109:49 | that I mean you are calculated it's . So the wells have all these |
|
109:56 | have temperatures and they measured the heat as well. Okay so there's their |
|
110:03 | there's the temperature of the wells. then we can between those temperatures and |
|
110:11 | service temperatures which have been measured by is the University of Delaware. They've |
|
110:18 | 25 well they have they have terrestrial temperature for for the Earth Monthly going |
|
110:29 | to 1900. So what I did I just took this two standard deviations |
|
110:36 | this for the date range, the , the range of the dates that |
|
110:41 | wells were drilled on And just took averages and that's what you're looking at |
|
110:47 | . So over the premium basis as can imagine, it's not very much |
|
110:52 | . This whole thing goes is about So it's not a lot but the |
|
110:58 | interpretation between this and and and the temperatures gives you this. So this |
|
111:07 | the near surface temperature at 100 m the surface and it goes from about |
|
111:12 | to 20. So it's about seven . So the reason I'm doing |
|
111:16 | I want to establish a temperature horizon a near surface temperature rise and then |
|
111:21 | can calculate the thermal gradient from there to the basement. Now the reason |
|
111:27 | picked 100 m depth was because I to capture as many of these wells |
|
111:31 | I could. Some of them are very deep. Okay now I didn't |
|
111:36 | very much very many thermal conductivity I have since discovered there's a lot |
|
111:41 | so this this this study needs to updated but it doesn't really matter for |
|
111:48 | what I'm talking about right now. ideas are all the same. |
|
111:54 | so here is the radio genic heat in the basin, that correction that |
|
112:00 | made for the basin heat flow. here's the basement temperature. So this |
|
112:07 | at the at the stations I can forays law because they have where's my |
|
112:14 | sir, I have near surface temperature at the stations that I have you |
|
112:21 | he for all the stations and I thermal conductivity and I know the death |
|
112:28 | the to the surface as well as basement. So rearranging four years |
|
112:32 | I can calculate the temperature of the . That's what I've done here. |
|
112:40 | let me see where I'm at Yeah. So right so I have |
|
112:45 | temperature horizons. I can calculate thermal now because I have these three |
|
112:50 | I can calculate the gradient between the service in the basement and the basement |
|
112:55 | three point which again is the magnetic . What I'm calling the magnetic layer |
|
113:03 | . Uh Yeah. So we have too, which is basically the total |
|
113:08 | flows equal to reduce plus that crystal sources. We have the two empirical |
|
113:15 | Park and chapman. Um Yeah, therefore the basic background he follows .6 |
|
113:26 | the measure minus the correction from the . Right. And thermal conductivity of |
|
113:32 | basement. So we can calculate the conductivity of the magnetic layer, recognizing |
|
113:38 | if you know the background heat flow the base and then we know it |
|
113:41 | . So we can rearrange forays law and thermal conductivity of the magnetic layer |
|
113:48 | the from the basement to the So here's security Point depth And there's |
|
113:59 | thermal gradient calculated by rearranging four years . So the format here is what |
|
114:05 | doing is I have some I have text blocks where I explain everything what |
|
114:12 | going to be doing. And then So the workflow one here, I |
|
114:17 | this text block and it tells near temperature based on thermal conductivity based on |
|
114:23 | flow of energetic sources, based on . So, I worked through all |
|
114:28 | , there's two stations, there's the borehole temperature depths for cold temperatures. |
|
114:38 | is the borehole depth. This is borough temperatures, service temperature, average |
|
114:43 | temperature. And then interpolated between the and the surface, the thermal conductivity |
|
114:51 | regional source. Then he flow from basin, the basement temperature. So |
|
114:56 | I go to work flow too. we take those three temperature horizons. |
|
115:01 | can calculate the thermal gradients and then calculate calculate the uh the background heat |
|
115:12 | that will calculate thermal conductivity in the . So that's what these next |
|
115:16 | A Series of slides are. Key depth thermal be great at the base |
|
115:22 | the thermal grading of the magnetic The heat heat flow from the |
|
115:28 | This is 3/5 of the total. . And then the thermal conductivity of |
|
115:32 | magnetic layer. So all those steps follow. And then then we're looking |
|
115:39 | basement terrain. So this is a interpretation by Whitmire, Whitmire and Castro |
|
115:54 | Geo Sphere 2007. And what they was they combined a bunch of outcrop |
|
116:00 | and um well penetrations to crystalline And they used magnetic data as well |
|
116:09 | map all these boundaries so that the and these light pink and these oranges |
|
116:15 | here in the northern part. Those all our key and rocks with the |
|
116:19 | part in these. And then the ones to the south. These are |
|
116:25 | protozoa Going from I think 1.76. the Riley? One point So I |
|
116:36 | it's 1.76 but one point seven should in there. You have applies as |
|
116:43 | in any case these are successive accretions juvenile crust onto the court is our |
|
116:52 | and core of Lorenza. So remember key in time Is 2.5 gigi |
|
117:00 | 2.5 billion years and older proto resort . The Protozoa Eon lasted from 532 |
|
117:10 | years ago to 2.5 gig. So like a two billion year. You |
|
117:15 | , it's five, it's five times long of a time from the earliest |
|
117:23 | or so. Yeah. And so are, these represent five accretion. |
|
117:31 | mean, I'm sorry, juvenile accretions the Yama pie, which is this |
|
117:37 | wedge here, the which is this one here And the olive colored here |
|
117:44 | the granite Riley and then the reds to the outward, Those are Grenville |
|
117:53 | out of the other ones. And with those were some granite IQ |
|
117:59 | Granite toys is what they call them what what what college would call. |
|
118:04 | those are the light greens, the blues and some of these dark greens |
|
118:08 | so they, they were intruded at same time. These, these uh |
|
118:17 | IQ collisions were occurring but also later those. So these basement to reigns |
|
118:26 | radio genic elements in them. They , you know, uranium and thorium |
|
118:30 | . So they have radioactive elements in . So yeah, here's the, |
|
118:35 | the big terrain here. Um I'm not sure. Oh yes, |
|
118:41 | have a pie for this area. just have sell um, granite rye |
|
118:48 | and Grenville and the bright greens in . The granite intrusions. So our |
|
118:53 | area, the premium basin is right . And we also have the this |
|
118:58 | intrusion. There's a well that was in into the central basin platform. |
|
119:09 | uh right, so all these terrains mapped and then uh interpreted. So |
|
119:17 | so we integrated those uh we're costumes map with the magnetic susceptibility and version |
|
119:26 | believe. Yeah. So here's the field, here's the susceptibilities. So |
|
119:32 | that's a that is a that's a a linear inversion. Remember we talked |
|
119:38 | inversion modeling inversion. So this so total fuel anomalies here were inverted um |
|
119:49 | magnetic susceptibility for the rock property. structurally but for the right property. |
|
119:57 | . And then this basement terrain map made. Yeah. And this kind |
|
120:15 | shows you uh what that looks So here you can see these terrain |
|
120:23 | that are interpreted. Remember some of things were I mean There were three |
|
120:30 | that three elements uh tools I guess were used to map the terrain. |
|
120:37 | had they had some outcrops, they some well penetration and then they used |
|
120:42 | data to kind of like connect the . So remember this is the abilene |
|
120:47 | from Zhang's paper which also had a anomaly over it. Um and you |
|
120:55 | see these outlines here, they are together. So I'm overlaying the trains |
|
121:00 | top the susceptibilities. And you can what I'm tracing here. Right? |
|
121:08 | why am I doing this? I'm this because we have heat production |
|
121:12 | Remember that? We have those We have them for the world. |
|
121:16 | the idea is to assign heat production to each of these polygons. And |
|
121:25 | use that with that. Remember we that empirical formula which has the total |
|
121:31 | . The total heat flow is the of the background heat flow plus the |
|
121:37 | flow produced by these terrain. And heat club is the product of the |
|
121:47 | production of the trains with how thick layer is. So this is a |
|
121:53 | thickness that hangs off the basement. if you can visualize we have a |
|
121:58 | layer of sedimentary rocks, we have layer beneath that that we're calling the |
|
122:04 | layer which extends from the basement down the key point. So in our |
|
122:10 | layer model right we go from the surface to basement to carry in our |
|
122:14 | layer model. We have different rock . We have we have we have |
|
122:19 | temperature of the horizons. We have heat flow within each layer and we |
|
122:24 | the thermal conductivity with each layer. in addition in the basement we also |
|
122:29 | heat production but that heat production within magnetic layer basement to Kerry point there |
|
122:40 | it is subdivided bye whatever thickness this production layer is. We know that |
|
122:48 | heat is produced in the magnetic layer we don't know where it is. |
|
122:53 | don't know that until we examine the production data. So that makes sense |
|
123:00 | you. Is that really confusing? a little confused. But it makes |
|
123:06 | . Like it's like okay. So , I'm sorry but you know I've |
|
123:11 | presenting this material and my presentations have over time but I prepared this last |
|
123:19 | and I've been doing this work. let me just let me just quickly |
|
123:24 | everything because now that I look, breezed through these this morning. I |
|
123:28 | I understood that. So okay, this is how peak production and this |
|
123:34 | you know, we have these basic , right? We have the basic |
|
123:39 | flow equation which is forays law which very simple. It's just the thermal |
|
123:46 | D. T. D. Scaled by the thermal conductivity. That's |
|
123:51 | simple. Then we have this other which is empirical which is says that |
|
123:57 | you measure over continents is the is some of the background heat flow plus |
|
124:04 | heat flow coming from radioactive decay in basement rocks. And that heat flow |
|
124:11 | the product of heat production times the of that heat producing layer. So |
|
124:18 | I look at my little cross section horizons are we have a near surface |
|
124:24 | which basically tracks the topography here. we have a then we have a |
|
124:30 | horizon, right? And then we a query point. So we're really |
|
124:35 | looking at the near surface the basement the curie point. But when we're |
|
124:42 | about the heat production separately, there's another layer that hangs off this, |
|
124:48 | we don't really know what it is we go through a bunch of |
|
124:52 | Because even though we know the ridge flow exists in this layer in the |
|
124:58 | layer, we don't know what its is. That distribution is is is |
|
125:06 | by the product of how many you what the heat production is, how |
|
125:13 | how concentrated the radioactive decay is and thick that layer of radioactive decay |
|
125:20 | Right? So there's a there's a in here that that is a heat |
|
125:27 | layer. So that is that is that that Yeah. Right. |
|
125:33 | So this is a bit a sunrise kind of explains all that's gonna |
|
125:39 | So then I show you the topography then the station data, right? |
|
125:44 | have three kinds of stations. We uh heat flow, thermal conductivity and |
|
125:49 | production. Now this I sample an much larger than this. Um and |
|
125:56 | we have, of course, the surface is just topography minus 100 |
|
126:01 | The the the basement. Is this by uh Rupel from 2009. |
|
126:11 | And so we have the measure heat a grid of that. And I'm |
|
126:15 | the same color scale for all the flow maps. It's a linear color |
|
126:21 | . That's why this one starts up around 35 because I have the near |
|
126:28 | , I mean the basin heat Okay. And then I'm repeating again |
|
126:33 | equations, So I'm starting into this for this example. So it was |
|
126:38 | days law that the birch uh empirical here and then follow chapman's empirical study |
|
126:48 | the world, where they found that each of these are 3/5 and 2/5 |
|
126:54 | what's measured on average, on And then we make this little correction |
|
127:01 | heat flow that he that's produced is in the basin. It's a tiny |
|
127:09 | and it might not be necessary, we're doing it anyways. So we |
|
127:13 | that. Okay, so again, here's developing the near surface horizon, |
|
127:21 | the stations, there's the depth, the temperature at those depths. Then |
|
127:28 | have the very surface terrestrial temperature. there's what that is averaged over |
|
127:35 | you know, the range of well . Well, the days of wells |
|
127:40 | drilled down and then here's the linear from the borehole temperatures to the surface |
|
127:47 | . So now I have a surface um a near surface temperature in depth |
|
127:56 | temperature. Right? So here's the conductivity of the basin, here's the |
|
128:02 | flow produced by cemetery rocks in the and here's the basement temperature. And |
|
128:10 | I went through another set. So looked at the temperature horizons and since |
|
128:15 | have three horizons, we have two gradients, the gradient between their service |
|
128:20 | basement, the gradient between basement and point. And we can calculate background |
|
128:26 | flow using equation two and correcting it Paul Chapman. And then we're saying |
|
128:32 | you know the background heat flow in basin then we know it everywhere. |
|
128:38 | can do that. Then we can the film gradient In the magnetic later |
|
128:44 | just using equation one again. So through all those all those things, |
|
128:50 | security point tap, here's the thermal of the basin democratic and the magnetic |
|
128:58 | Background Heat Flow. This is 3/5 the total and then through the conductivity |
|
129:03 | magnetic. Later then we're looking at deeper into the basement terrain. So |
|
129:10 | can map those basement terrain. And just using already work that was already |
|
129:17 | . You can download these shape files the internet and um they spent a |
|
129:23 | of time mapping mapping the. Well least the protest. I don't there |
|
129:28 | be more detail up here but I know why um In any case these |
|
129:32 | the trains in in our area the granite, right? Like the |
|
129:38 | All created all the created in the resort. You know all created uh |
|
129:45 | 500 million years before paleozoic time. yeah. Um And then here is |
|
129:54 | basement terrain. This is a total . I can totally feel unique |
|
130:01 | Total magnetic intensity in that one. we wanted Do a three d. |
|
130:07 | of those. A three D. for magnetic susceptibilities. Remember that's a |
|
130:14 | relation and a linear inversion and that's that looks like. So the magnetic |
|
130:22 | range here from about pleasure minus 3000 CGs units. Which is pretty |
|
130:29 | Okay so Do a three D magnetic and version of the total fuel |
|
130:40 | And now we use that with the from what Mark Whitmire and Kallstrom to |
|
130:50 | make our final interpretation of the basement . And yeah I mean it looks |
|
130:57 | good I think. Um Yeah. so workflow # three We have basement |
|
131:08 | . We have heat flow from regional production and then we can figure out |
|
131:16 | the heat production layer thicknesses. So the heat flow from raging sources. |
|
131:22 | is two fists of the total and the heat production layer thickness and that's |
|
131:33 | in the workflow. Yeah. So and this sort of shows a summary |
|
131:38 | that thermal conductivity from stations heat flow the basin. We raging sources in |
|
131:46 | basin that sushi. Then we used one for the first time to calculate |
|
131:52 | temperature then thermal gradient basement to surface a thermal gradient curie point to |
|
132:01 | Then using Polident chapman background heat Then we used the background heat flow |
|
132:06 | calculate from the conductivity in the magnetic then we then we interpreted basement trains |
|
132:14 | we integrated the public data with our susceptibility inversion. Then we used it |
|
132:21 | to get the heat flow produced by sources. And then finally, we |
|
132:27 | it empirical equation to to captivate the of producing later. You have any |
|
132:42 | with that? No. What did do have? Just the image question |
|
132:54 | slide. Go ahead. I'm trying find this slide. I was I |
|
133:03 | , just page through, did you passing already? It's 73. What |
|
133:12 | causing those like um like towards the of the map, Like those two |
|
133:18 | right there. Like what are, are those there? Hmm. I'm |
|
133:24 | curious. Well, okay, I , so this is the thermal gradient |
|
133:29 | the basin. Right. This is thermal gradient from the basement to the |
|
133:36 | the near surface. And um that's good question. I don't know what |
|
133:41 | causing it. So, let's just at the oh, look at |
|
133:44 | So this is the basement temperature. there's let's let's look at the basement |
|
133:55 | . Ah, okay. So the , I mean, I think the |
|
134:04 | elements to to this thermal modeling are geometries, the geometries and the temperatures |
|
134:14 | the, of the near surface. basement in the curie point. And |
|
134:19 | you think about that kind of makes , right. I mean, because |
|
134:23 | their properties are what control the heat . So, you see here, |
|
134:28 | isn't, this is called, I Arizona arch. So this is these |
|
134:32 | structural highs and if we look so he club, you really |
|
134:40 | This is the thing about heat It doesn't, it does not correlate |
|
134:43 | the base and depth as you can . It doesn't correlate at all. |
|
134:49 | what does correlate with invasive death? Does the near surface temperature? Not |
|
134:59 | um thermal conductivity? No. Now heat flow from raging sources, it |
|
135:08 | correlate, but it has to because because this dysfunction, our correction is |
|
135:18 | function of basic things. So it's , you know, it's no surprise |
|
135:24 | the this this little correction we which is tiny. Right? I |
|
135:29 | , it's not even, it's just few million watts per meter squared. |
|
135:33 | we can really discount this. But at the basement temperature is strongly |
|
135:41 | And how do we do this with temperature is calculated by rearranging for law |
|
135:49 | at the stations we have heat we have thermal conductivity and we know |
|
135:55 | depths to the, you know, know, you know, disease to |
|
136:00 | basement. And the only thing we have, we only have one of |
|
136:04 | temperatures we have the temperature of the surface. So we can rearrange all |
|
136:10 | that. Right. Let me just just go back to the formula trying |
|
136:22 | see do I have it in Okay. To use So at the |
|
136:31 | we have Q. We have We have Dy DZ this case DY |
|
136:38 | And we only have one t. have the temp the near surface |
|
136:42 | So we can we can arrange that to calculate temperature of the basement by |
|
136:56 | rearranging that formula. And that's where are coming from. Those highs are |
|
137:07 | , which makes sense. Right? temperatures go up as a basement as |
|
137:11 | , as the basins get deeper, ? Or thicker. Right. |
|
137:17 | So that's where those are coming Oh, okay. Yeah, that's |
|
137:23 | . Yeah, that's where those are from. Because because if if the |
|
137:33 | about it, you have the heat is not only the same throughout |
|
137:38 | And the throne conductivity is as So what's controlling this is is the |
|
137:46 | ? The basin, the basin is basic temperature here, temperature is |
|
137:55 | So the tea is low but in thickness is small. That means you |
|
138:02 | to have high gradient to produce the heat flow. It's just a trade |
|
138:08 | . Mhm. It's really pretty. mean, Yeah, Yeah. |
|
138:22 | ask me questions on this if you later. I mean, I'm not |
|
138:26 | what I'm gonna do. I might test you on anything in these things |
|
138:30 | the slides are not obviously, I to do some work on these |
|
138:35 | So, I might ask you a of general questions that are in the |
|
138:39 | . But yeah, I won't blame for being a little confused. This |
|
138:45 | new material for me. In this is when I presented this, |
|
138:49 | presented this this work, not these , but I presented this work like |
|
138:56 | from the Denver Jill's berg and potter basins at the image conference last |
|
139:03 | And and yeah, and I've been I said I've got other presents. |
|
139:11 | new stuff that I'm trying to, to do. What I did was |
|
139:16 | my cover on my title slide, slapped across it what I did on |
|
139:22 | pandemic vacation because this is material. is all stuff that I that I |
|
139:29 | um in 2020, 2021. So , anyways because you know the industry |
|
139:38 | changing a lot and there may be geothermal opportunities and anyways. Yeah, |
|
139:44 | I'll just, I might ask you basic stuff out of here but not |
|
139:48 | , nothing that you have to, know, be too concerned. Probably |
|
139:53 | other stuff to the great allergy stuff well. I didn't used to teach |
|
139:57 | stuff, so you're getting new new . Um Yeah, so such as |
|
140:03 | is so um if you want, we take a take 10, come |
|
140:11 | at four and I'll finish up with at least introducing the gradient stuff. |
|
140:20 | . Okay. Alright let's just finish up and celebrate. Okay, so |
|
140:29 | this is more new material. Um gravity gradients um and no they do |
|
140:40 | do collect magnetic grades but it's just just, what they do is they |
|
140:45 | fly uh with like two stingers where airplane would have one sting and have |
|
140:52 | right below it. So they just a physical measurement of the field and |
|
140:57 | locations. And then their difference is , is the gradient, is the |
|
141:04 | gradient. You can do that horizontally they put stickers on the wings and |
|
141:10 | they measured the, you know, magnetic, you know, than just |
|
141:14 | to those across the wings and you a horizontal grade or whatever. So |
|
141:21 | done. Um gravity graders can be that way as well. I |
|
141:25 | you could you could just measure gravity two different elevations and their difference would |
|
141:30 | the great the, you know, grading of the field. Right? |
|
141:34 | there's there are instruments. In the very first measurements of gravity were |
|
141:41 | instruments back in the, You 19,000,000 Early 1900 1910, 1920. |
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141:50 | that. The cost of Romberg Instrument developed until 1930. So yeah, |
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141:59 | so gravity and magnetic data are acquired measured in quantities. Uh What they |
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142:06 | are the fields of course, write vector fields and those can be expressed |
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142:11 | in Cartesian X, Y. Components. Now, when now the |
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142:17 | commonly, what we what we Okay, let me go back |
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142:21 | Standard values how many good contour maps scalar is right. So when we |
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142:26 | at all the anomaly maps we've been at are basically the scalar of the |
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142:32 | field values. We're not, we're getting any vector information criminals Right? |
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142:37 | mean, nothing is telling us what direction of the vector is. We're |
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142:40 | looking at the, you know, the the amplitude, so to |
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142:47 | But in some cases the actual components measured of the vector field. For |
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142:54 | , flux gate instruments measure the components the magnetic field. Okay. And |
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143:02 | are geodetic instruments. Remember we talked land measurements of the ge Oid? |
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143:08 | actually measure the deflection of the gravity relative to vertical relative to, you |
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143:15 | , steroid. So if you want think about the whole idea the whole |
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143:26 | you know mathematically from from potential to . Right? We have force |
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143:35 | The force fields are the drifters or of potential and the gradients are the |
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143:42 | of of the force fields. and then inverse mathematically integration. You |
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143:48 | go backwards from gradient field to So I made this little table |
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143:56 | We have the field, the type quantity and then math direction of math |
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144:07 | derivative versus integral. Right. So field um it's it's derivative as a |
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144:15 | field. It's driven a gradient A scalar to vector two tensor. |
|
144:24 | ? So that's just kind of a that way. I think of |
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144:26 | And I imagine a mathematician might tell there's some problems with this, but |
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144:31 | just think it's convenient to sort of them that way. Okay, so |
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144:37 | data. What is the earth's gravity effective fuel with xy components. Thank |
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144:43 | . The grading field consists of excellent for each X. Y. Field |
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144:50 | . So no these could say I'm T here but I can say G |
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144:57 | as well. Okay so T X Y T. Z. Are the |
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145:02 | components of the gravity field and then . X. T. X. |
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145:05 | . T. X. E. . Yeah these break down into three |
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145:10 | each of these right now there's some because fields are conservative, you know |
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145:20 | Illinois elite center it center that supply plot. They satisfy the plaza's |
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145:25 | There's symmetric about along this axis X. X. Y. |
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145:31 | Z. Z. That means X. Z. Is equal to |
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145:35 | . X. Y. Z. . And so forth. Okay so |
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145:41 | kind of a visual way to think it. How how do we measure |
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145:46 | ? Um They have these instruments basically accelerometers and So the gradient of the |
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145:55 | Chicago by subtracting the measured field values pairs of accelerometers monitor opposite each other |
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146:02 | spinning disk. Right? They have for the F. T. |
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146:07 | Instrument. There's three spinning discs and all inclined. And so each opposite |
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146:17 | of measurements so each measuring the gravity . That means their their difference is |
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146:25 | gradient. And these little things are called G. I. S. |
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146:33 | This paper from 1988 um gravity gradient survey system. This is this shows |
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146:41 | little G. I. S. and vertical. So the gravity great |
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146:47 | survey system G. S. Was in the late 19 sixties this is |
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146:53 | a military thing, like lots of . It's either developed most of our |
|
146:58 | is either developed in the military by government Nasa or D. O. |
|
147:04 | . Or in universities. Very few actually generate new technology. Um So |
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147:15 | gravity grading amateur, I'm reading this block down here theoretically is insensitive to |
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147:22 | accelerations since it measures the difference in . Okay right. Just a little |
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147:30 | . Um So this is the the of the first instruments Grady after instruments |
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147:37 | it was this enclosed box and this this is development Bell Aerospace and now |
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147:45 | spin off from the Bellagio space which the F. T. G. |
|
147:51 | . Okay. Um and the platforms that are the dynamic platforms. I |
|
147:59 | they have, you can measure you on the bench or on land if |
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148:04 | like but there are dynamic plant one fixed wing, here's a here's |
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148:13 | this is a Cessna caravan. See B. And D. This is |
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148:20 | you look closely that says bellagio space fly, there's with the Dc |
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148:25 | So they're expensive surveys and then they've there's a lot of the very first |
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148:30 | were marine and then de beers, famous diamond company flew with a |
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148:38 | this is in South Africa, that crashed I don't know crashed two years |
|
148:45 | . Um Right so if we have little square prism and we want to |
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148:53 | the gradient, the gradient field over for each of these components. So |
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148:59 | X X Y I'm sorry, this gravity, gravity ingredient components. So |
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149:11 | , X Yeah, X X, X, Y X. Said, |
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149:15 | y y zed said said um this is, this is the shape |
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149:25 | you get. So if you X means um yeah, the gradient is |
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149:36 | for the X component in the X . Okay, so for the X |
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149:43 | component of the field, it's it's the X component of that. |
|
149:51 | , and then these two are for Y component and this is for the |
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149:54 | component of the vector. Um in example is a 10 kilometer square |
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150:03 | 28 kilometers thick where the top is kilometers down in the desert contrast is |
|
150:09 | g per cubic centimeter and here's here's just the gravity signature of |
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150:16 | So the gravity looks quite like Z. Z looks quite like the |
|
150:20 | looks like a vertical derivative. No, that's because that's what it |
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150:26 | the vertical component. We know a about we calculate this all the |
|
150:31 | Now, what is the conversion from to eat boats? Right, so |
|
150:36 | is, there is a conversion, tell you what it is. I |
|
150:47 | I had it right here in front me. I don't, I think |
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150:50 | have it in my notes here in in the class notes here. Oh |
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151:00 | . Okay, this is nice. is nice. This is this is |
|
151:06 | this parts of this is in wellings on Grady actually. But so if |
|
151:12 | take instead of I think I think problem was using a square where the |
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151:18 | the sides are are, you oriented north, south and east west |
|
151:25 | china doesn't really help you understand. And that's because these data are processed |
|
151:34 | the N E. D. According the N E. D. |
|
151:37 | any D stands for Northeast down in words, the gradient is calculated from |
|
151:49 | to north west to east and top down N E. D. So |
|
151:57 | the direction that the gradient are I mean when you look at data |
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152:05 | data, that's how it's displayed. , this helps make the point. |
|
152:10 | let's just look at let's just look X. Said and why is it |
|
152:17 | ones that have the arrows and the lines? Those both of those lines |
|
152:25 | to this profile with a red red Over this. This model was |
|
152:31 | So this is a .1 g per centimeter contrast of this three D |
|
152:37 | So this is a this is a deficiency. It's a cavity And the |
|
152:43 | with the Cavity of zero. The is .1 and this profile goes from |
|
152:50 | to east or south to north here . And you can see when you |
|
152:57 | this body from east to west from to east. This is the there's |
|
153:06 | there's a minimum of closure directly over edge of the source and a maximum |
|
153:15 | over the edge of uh of the side of it. So not only |
|
153:23 | this peak and trough does this these anomaly. Men max tell you where |
|
153:31 | edge of the sources and it also you which direction is getting uh lower |
|
153:39 | or higher density. That's really I mean that's really useful. You |
|
153:44 | just make that inference directly from looking these data. And that is something |
|
153:50 | until our paper just came out is described in the literature. And it's |
|
153:56 | and when I explain these data to , this is the first thing I |
|
154:02 | . I go through and say, , this is X x, |
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154:04 | you know, x, Y And Y said blah blah blah, |
|
154:08 | these things and explain what they And then I say, you |
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154:12 | this any d standard. And I , let's just look at these two |
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154:19 | I explained what I just explained to that X and Y. Is that |
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154:25 | the most useful components. Now. people say that is because it's, |
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154:29 | know, it's it's looking at, know, it's centers over the mass |
|
154:33 | I think there's a really good point that, right? As you look |
|
154:37 | here, Z. Z. That they're the same as just regular gravity |
|
154:45 | . That's what this is just Z. Right? It's just regular |
|
154:50 | data. But those look quite like are quite similar. Right? I |
|
154:55 | why did you do that if you that, you don't need to do |
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154:57 | right? You don't need to collect the other components. So why do |
|
155:02 | ? And the answer I think is you can map the edges of sources |
|
155:07 | from these data. And um I we had a hard time getting that |
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155:14 | published. It was it was in for 16 months because we just couldn't |
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155:20 | to these mathematically biased folks that really think about geology very much that that |
|
155:30 | though this is very simple minded, not described and people should should be |
|
155:36 | to look at these data and understand . So let's just compare them. |
|
155:41 | look at this is this is even is going and the reason I like |
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155:46 | more than the boxes because it's showing it's showing different directions, right? |
|
155:51 | . Anything that's generally north styles, ? You can have to be at |
|
155:58 | angle, the high will be west the edge will be over the western |
|
156:05 | and the low will be over the edge. The high will be over |
|
156:09 | eastern edge. Right? Let's look look at this one. Okay. |
|
156:18 | know that from this but you don't know it for something that's at an |
|
156:24 | . It's just it's not clear. plus this thing is too deep and |
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156:30 | thick. You don't really see That's why I made this one with |
|
156:35 | such a small feature so I could see these anomalies. Really isolate |
|
156:41 | Anyways, I spent a lot of on it, but I think it's |
|
156:44 | , it's really important because this side explains to you how these things work |
|
156:50 | the most the two most useful ones X and Y. And if |
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156:56 | you can amaze people, you if you ever see these data asked |
|
157:01 | see, let me see Exit a because you'll know that you can match |
|
157:06 | from those directly without having to do inversion. And yeah, okay, |
|
157:13 | now in version is pretty much the of choice for these data because they |
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157:18 | so complicated and this is just from paper uh and they're just doing |
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157:23 | you know, one of these laminate that we've covered for for just the |
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157:31 | gravity data, it's pretty standard Okay, here is now now there's |
|
157:38 | bunch of a bunch of examples So this is a an example from |
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157:44 | and Barbosa and I think this is brazil Oliviera, those sound like Brazilian |
|
157:51 | to me. Um We'll see. . It's slide slide 12 oh here |
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158:15 | yeah. Um Yeah, maybe Why am I thinking this anyways? |
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158:26 | , in any case. So they the components here. This this one |
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158:32 | um yeah A. S. X. B. S. |
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158:38 | Y. X. Said why why is it? Okay so here are |
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158:45 | two that we would look at to . Okay going okay so this is |
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158:53 | this one has to be um X. X. X. |
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159:00 | Right? So that means action. can't be right. That can't be |
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159:11 | . I think they're backwards I Yeah this is this is easy. |
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159:19 | is the vertical one. These these but it just has to be |
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159:24 | Said these two are backwards. You make that correction. C. |
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159:29 | And C. And E. Are . In fact A. And |
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159:37 | Are reversed as well. A. to be Y. Y. And |
|
159:42 | . Has to be excellent. You why? I know that don't |
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159:44 | Because it's because it's kind of like long strike. They don't change |
|
159:48 | Right? Yeah. X. That's where the big changes anyways. |
|
160:01 | what do we know? Okay so is going from we go from south |
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160:05 | north. Low density high density. means the low density is north of |
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160:13 | source body. And the high density I mean this this means it's a |
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160:18 | density feature between you because the high gonna be north of the source. |
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160:28 | ? Yeah. The highest north of the the highest north of the low |
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160:34 | source. That's right. That's That's right. This is a |
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160:41 | right? That's so that's what this . This is not simple because it's |
|
160:47 | circle. I think that's what's getting messed up here. Yeah. |
|
160:52 | it doesn't matter. We're not gonna not gonna worry about that. So |
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160:58 | there are two in, there are two instruments, there's the bell instrument |
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161:04 | really not austin, we can forget those. There's the bell instrument and |
|
161:12 | this is what it looks like. it's three inclined spinning disks that are |
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161:20 | in in in this carousel that rotates they each in each one of |
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161:27 | there's an inclined G. I remember with two pairs, so there's six |
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161:32 | of spinning disk in these. And carousel can also rotate with any |
|
161:41 | And here's some of the very first that this was donated to University of |
|
161:45 | over Vincent dome Louisiana. And this some noisy data. I mean, |
|
161:51 | dome is producing this broad, she said, and there's a cap |
|
161:56 | over Vincent dome in Louisiana. And just, yeah, this is really |
|
162:03 | to look at and this is what FTN are what they call their tensor |
|
162:16 | reduction. So on the right, reduced noises, it's reduced, it's |
|
162:21 | . But I mean, here's another of their noise reduction. So you |
|
162:28 | see it's just just chatter and it's it. It's improved it. But |
|
162:34 | don't know, I get the sense , like there's some artifacts that stretching |
|
162:39 | stuff. Um Okay now this is . Oh this is a paper I |
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162:49 | this is more F. T. . Noise reduction. Yeah. Method |
|
162:58 | use notion. I don't think I'm test you on that. I wouldn't |
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163:04 | you on that. That would be mean of me more sort of filtering |
|
163:10 | . So there's there's a whole bunch folks that sit around and think about |
|
163:14 | James brewster. He's a really nice and just ridiculously smart. He's that's |
|
163:21 | mentioned a lot of these a lot this stuff he works for Belgian |
|
163:29 | Okay. Um this is a case . Now some of the tools they |
|
163:36 | besides inversion they use what they call variant calculations and invariants are basically um |
|
163:45 | of the tents of components. You these. So in variant one um |
|
163:52 | this combination of texture components and variant in very zero? Is the traces |
|
164:00 | laplace. Um It's del squared. T X X plus two Y Y |
|
164:04 | Z. So that's and and there's called. And the reason these I |
|
164:13 | through eye to eye not I one two, they're called rotational invariance because |
|
164:20 | you once you do these combine the components in this way the data or |
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164:28 | the rotational doesn't matter what direction you at them. The N. |
|
164:31 | D. D. N. D. Is is accommodated so there's |
|
164:38 | directional about it but what you also with it is you lose that ability |
|
164:44 | know which direction is getting lower or , you know high debt to your |
|
164:48 | density and then there's this horizontal invariants are independent of just the vertical |
|
164:56 | Yeah. So you know, Oh no, I'm just kidding. |
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165:02 | I either to know is that the tools for gradient interpretations are inversion, |
|
165:14 | inversion and in various calculations and direct of TXN and T. Y. |
|
165:30 | . So right, so here is is this one? This is this |
|
165:37 | this Newfoundland study? So they did just study in Newfoundland. I don't |
|
165:43 | . We can just look at the TXN T Y Z. So we |
|
165:49 | here the highest also. Right. if the high is north of the |
|
165:57 | density that means it's south of the density and vice versa. So the |
|
166:02 | right in here. Yeah. Yeah. Yeah. Yeah. Same |
|
166:05 | here. The source. You can the source so that goes, let |
|
166:09 | go back to that when it was was confounding. So. Right. |
|
166:16 | . Yeah. Yeah. So it's going to be in here. |
|
166:19 | Yeah, I get it. Alright. Um here's some demonstration of |
|
166:26 | invariants again. Is this the same ? Yeah this is from the same |
|
166:32 | so that they apply to invariants The rotational ones are too. Uh |
|
166:41 | . What do they call our-2 and too with the first vertical driven. |
|
166:46 | it's the first, yeah The thing gravity gradients gradients it's relatively new. |
|
166:54 | mean it's they've only been doing this of work for 20 years or so |
|
167:01 | it's the literature I mean there's just ton of literature but it's dominated bye |
|
167:10 | my view folks that don't know a of geology that they really they know |
|
167:15 | about math and geology because they're geophysicist kinda geophysicists that don't know a |
|
167:23 | I mean you know geology I I hate straight lines. I mean I |
|
167:28 | think that's where geology is anyways. Yeah here's the last map so they |
|
167:34 | some sort of horizontal in various map . So from this from this analysis |
|
167:40 | drew these lines. I'm betting you really need to do all this work |
|
167:44 | draw these lines. I bet you just draw those lines probably just from |
|
167:48 | mag data or just a vertical derivative gravity. That's just my blast more |
|
167:58 | variant work with a different Murphy and . So call Murphy and James brewster |
|
168:04 | their bellagio space. Um This is state of brazil. Um Maybe this |
|
168:11 | what I was thinking of. So did a power spectrum residual. Remember |
|
168:15 | talked about those on the T. . Z. Component and they separated |
|
168:20 | into two bits. This actually looks nice. I mean I mean they're |
|
168:25 | teasing out some stuff in here but still got a lot of noise if |
|
168:31 | ask me. I think it's really . David. Yeah. Um Yeah |
|
168:45 | don't know. And I'm not I looked at this and this morning |
|
168:48 | was staring at it for a long . So this is a linear analysis |
|
168:54 | Murphy brewster and I don't know. just picking a bunch of regional field |
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169:02 | direction. I don't know what that's for. Okay so the bell instrument |
|
169:09 | is the which is the three cara of inclined spinning disks. That's one |
|
169:19 | . The other instrument is is owned C. G. And it's called |
|
169:24 | falcon instrument. And it has a disk, a single big broad spinning |
|
169:35 | . And you might ask why one . Well this was developed by BHP |
|
169:42 | even though there's an hasn't an oil to it. It's basically a mining |
|
169:49 | and it always has been. So those targets they're all near surface. |
|
169:57 | death is not an issue. Everything near surface. I mean no one's |
|
170:02 | know one's mind go at the bottom the anatomical base and it's eight kilometers |
|
170:08 | . Right? I dig down through kilometers just to just to start |
|
170:13 | you know to strip mining or Right? So so miners everything is |
|
170:19 | the surface. They don't even think terms of death. Everything is if |
|
170:22 | listen to them talking about structures. just talking about surface features. They're |
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170:26 | talking about anything with any vertical It's just the way they talk. |
|
170:32 | So for that reason they have they have a disc that's bigger. But |
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170:37 | has four pairs of um of opposite accelerometers. So in fact because it |
|
170:48 | a it has a bigger disc. error is a little bit less just |
|
170:56 | of that geometry, but also it such redundancy in it because it's it's |
|
171:02 | as measurements. It's actually a better for measuring in the horizontal plane. |
|
171:08 | it doesn't do like, you it doesn't do like any, it |
|
171:13 | calculate directly anything with a Z component it. Obviously. Now this is |
|
171:26 | is the other, where was where there it is? Austin. |
|
171:34 | . Bridgeport's is, well, it's a new company anymore, I think |
|
171:39 | just called Bridgeport's now, Austin, dropped Austin but Bridgeport, They're trying |
|
171:48 | make a three access system. So kind of combined Everything. We're trying |
|
171:58 | have an instrument that has a big disc with eight accelerometers each Instead of |
|
172:05 | mine on a carousel. They've been to do that for a long |
|
172:12 | And by the way, when I they, when I say there's two |
|
172:17 | , they're all built by Lockheed they're all built by Lockheed, all |
|
172:22 | them. They build every instrument. build bells instrument. They build CGs |
|
172:27 | and they're working on Bridgeport's instrument. you know how in the world does |
|
172:33 | work? I have no idea because guys really hate each other. They |
|
172:37 | hate each other. Um Yeah, that's what that instrument is and they |
|
172:47 | . Okay so that's it. Now talk about this core NG test |
|
172:51 | There's a famous gravity and great geometry gravity test site in uh in western |
|
173:00 | . Just you know just east of . And uh basically data has been |
|
173:11 | has been donated and you can download . If you go into you know |
|
173:16 | car NG test site, it will you to a place where you can |
|
173:20 | a bunch of data, gravity and data and granularity data. So here's |
|
173:24 | the test site is. This is size of the of theirs to |
|
173:29 | So this is the ties of the data and I think this is the |
|
173:33 | , the site of the aero mag . Right? So this is the |
|
173:38 | data outline I think right uh and is the airborne gravity, the magenta |
|
173:49 | then the A. G. The grad geometry is the green. So |
|
173:55 | airborne air gravity grade geometry. All data has been donated. Here's the |
|
174:02 | gravity, There's the coastline. Perth right over here. That's that's the |
|
174:07 | test site. So here's the Here's the gravity data, the regional |
|
174:14 | gray to data with the airborne Their resume into the airborne gravity. |
|
174:20 | the airborne gravity and this is the geometry flowing at three different line spacing |
|
174:28 | oriented southwest northeast. So assuming and you can see this line spacings are |
|
174:35 | and then zooming in even more. is um topography and here is uh |
|
174:45 | and data integrated uh into um basically well it's it's it's the it's aero |
|
175:02 | in the korean death site integrated with guess land bouquet. So its gravity |
|
175:10 | the great it's the A. Converted to gravity. And then and |
|
175:14 | that stitched in with the airborne Bradley you can see that the resolution is |
|
175:19 | right in there. They have a mag and you can see all the |
|
175:26 | because this is outcropping basement. I all of these are little intrusions and |
|
175:33 | crust here is our key and it's very old crust. So here's some |
|
175:40 | noise application on the korean test So it's just this narrow strip in |
|
175:47 | middle and this is um standard And then so so that there's just |
|
175:55 | not CG anymore. It's Excalibur. just recently so CG just sold this |
|
176:00 | they call their their multi physics uh to a new company called Excalibur and |
|
176:15 | they have an ongoing battle with It's just two companies who can deny |
|
176:21 | the data the best. And so is just one of the many, |
|
176:25 | , many papers out there where they different Denoix zing techniques and here's a |
|
176:33 | a repeatability test over the car. using CGs noise testing difference. The |
|
176:43 | is uh I guess plus or minus at bars. So I think, |
|
176:51 | don't know why, I can't remember . I mean, I thought I |
|
176:54 | it, I thought I had Yeah. Right, That's it, |
|
177:04 | it. Um yeah, here's the from elbows to mill igel. It's |
|
177:16 | had to do milligram per meter, head boss equals one over 100 mg |
|
177:26 | meter. Okay, In other and that boss is essentially 10,000 |
|
177:36 | 10,000,000 of a middle gail. So very tiny. So This is like |
|
177:44 | , 7 over 10,000 mg. So really tiny and they're very, you |
|
177:51 | , very tiny units. So they're sensitive obviously. Okay, so the |
|
177:57 | and version of occurring test data by School away. So let's say they've |
|
178:02 | okay. So they did uh they the car in test data and um |
|
178:10 | see joint inversion. So that means they're in this term, the |
|
178:16 | the phrase joint inversion can mean a of different things to a lot of |
|
178:22 | people remember I told you inversion means lot of them things talk in this |
|
178:30 | with great amateur. What they mean they're inverting all the components, they |
|
178:35 | considering all the components when they're doing inversion, that's what they mean. |
|
178:43 | , so this table. I think is from a paper in A. |
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178:46 | . L. E. It looks a T. L. E. |
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178:49 | of table. And let's say this all for the CGs instrument again, |
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179:00 | difference, repeat surveying commons, estimated amplitude, estimated. Yeah, it's |
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179:09 | it's just more more on the battle noise between the two contractors. Um |
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179:22 | A and Peterson presented adverse method to strike and depth of thin sheet |
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179:29 | So I was reading this, let get to this point. This is |
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179:33 | 41. So, so these are dykes and contacts. There are models |
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179:47 | strike in the in the Y. . So from south to north this |
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179:53 | and projection of the dip angle into line. Yeah, I'm not sure |
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179:59 | this what this is about. We're gonna worry about it. So here's |
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180:08 | uh F. T. G. or is it F. T. |
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180:12 | . Or is it? Um who's the authors, robert said |
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180:17 | Uh No, this is a Falcon , but they flew it over the |
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180:27 | part of Lake Tanganyika. So here's East African Rift one. This is |
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180:30 | eastern branch and this area here, is their peak, their their permit |
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180:39 | energy permit area right down here. it's kind of hatch erred in in |
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180:44 | figure here. So just on half the half of the lake and this |
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180:48 | topography. Yeah. So let's see just looks like. So there's a |
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180:55 | seismic line shot right here. So is this is this is the lake |
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181:01 | here. This is their half of of uh Tanzania. And here's the |
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181:07 | . So you can see there's some drop blocks here and uh there's some |
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181:13 | centers in there. So they're they're that from these data and then they |
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181:20 | this structural interpretation where this this blocks ? To see uh They have little |
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181:28 | structures that they've mapping in here. that saying saying? My notes. |
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181:35 | have highlighted two major depot centers were in the magnetic, in the magnetic |
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181:41 | thickness is in excess of weight, the magnetic depth of basement in north |
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181:48 | west central parts of the survey area sediment thicknesses in excess of four and |
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181:53 | kilometers. So let's just look at . I see it's getting deeper. |
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182:01 | yeah, so this is their magnetic . So these are the deep half |
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182:09 | right here in the center as That's it. Did you learn something |
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182:27 | that? Did any of that make to you? It's a lot but |
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182:33 | makes sense. I just have to through it again. Yeah. So |
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182:38 | , I think it's important to just that gradients, you know, they're |
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182:42 | the derivative of the field except in case is they're actually measured gradients. |
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182:47 | ? So I think that's the key understand that's why I made the point |
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182:51 | the beginning about measured magnetic gradients you know, in this case it's |
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182:57 | the same. It's two accelerometers that separated but it's all encased in one |
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183:04 | and these surveys are really, really . I mean only the big oil |
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183:11 | can afford to pay for these Um yeah. And then they go |
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183:16 | like I said listen this is this 1988 and this picture looks like it |
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183:20 | taken out of you know, should things should be sitting on a model |
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183:24 | or something. But yeah, this the 90s they started sailing around collecting |
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183:32 | data in the gulf of Mexico and did it and then they did some |
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183:37 | they were driving around with the instruments vans and then they only started flying |
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183:42 | them Jeez around 2000. I mean want to say it was. |
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183:52 | Yeah. Yeah. Because I was business I want to say it's only |
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183:58 | 15 years, 10 to 15 years they've been collecting gradient data reliably reliably |
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184:06 | airborne platforms. So it's rarely really stuff. I think I think this |
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184:12 | a really good figure because it explains , you know, the relationship between |
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184:18 | and why is it? So that's way, remember that's one way you |
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184:22 | interpret these the way it's not used many people but I think it's an |
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184:26 | one. And then of course the way is inversion inversion is the most |
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184:32 | used way to interpret these data. remember inversion you start with a model |
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184:38 | the closer you are to the the better the inversion works okay. |
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184:44 | then um there's the bell instrument and of course the CG instrument coming |
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184:51 | Don't worry about all, they're all about the noise. That's, that's |
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184:54 | thing, the instrument companies, I the acquisition companies and then a lot |
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185:00 | these examples are about that um in , so this direct mapping inversions and |
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185:08 | variant calculation because they are irritation. right. Some are completely irritation in |
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185:14 | direction and some are just irritation of horizontal I believe. And then just |
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185:21 | of some, I like this one best, this is just a |
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185:24 | I mean slope, everything else you know, really kind of hard |
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185:29 | understand. There's the falcon instrument. it's a big giant just in Bridgeforth |
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185:36 | trying to make a hybrid of both those and there's the famous korean test |
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185:41 | where I think Bell has done some , conscious and test data there as |
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185:48 | . And yeah, more inversion stuff then more, yeah, more techniques |
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185:57 | map these things. I'm not sure are map from but yeah, |
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186:09 | So I also noted in my I still got, I got the |
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186:14 | wrong, I said, I said the 14th but Wednesday is the 50 |
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186:20 | , but Wednesday is the exam Yes, I believe so yes, |
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186:28 | do the same thing on Tuesday, send it up, I'll send it |
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186:31 | then and then you just give it me whatever thursday morning. Okay. |
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186:37 | that that should be fine and then , I'll just score it and then |
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186:43 | guess I got to get into, can get into the thing, the |
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186:46 | center in my US thing and I go ahead and give you a |
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186:52 | So you're doing fine. No, worry about anything, so thank |
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187:04 | Alright then. So um that's It's uh I've had it, I've |
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187:11 | enough. Um yeah, just send any notes. You have any questions |
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187:18 | this? So this is gonna be this this test is gonna be 567 |
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187:25 | eight. Right? Yes, I whatever. 6, 6, 7 |
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187:30 | eight. There's just three, there's It's just three elections because apparatus ah |
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187:46 | sorry 5678. So it's gonna be super continents and basic classification rules of |
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187:57 | . And then and then um the , Wilson cycle and coastal sites and |
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188:05 | maybe a question or two about gradients heat flow but nothing nothing too heavy |
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188:10 | this stuff. It's new material and understand that. My notes, my |
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188:16 | be a little bit better so. , alright, well I'll send you |
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188:23 | thing on Tuesday. Okay, thank so much. |
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