WEBVTT Kind: captions Language: en-US 00:00:00.392 --> 00:00:04.208 Hi, I’m Chris DuRoss with the USGS in Golden, Colorado. 00:00:04.240 --> 00:00:08.000 I’m excited to share new research on a portable optically stimulated 00:00:08.000 --> 00:00:11.253 luminescence age map of a paleoseismic exposure. 00:00:11.253 --> 00:00:14.800 I’d like to acknowledge my co-authors, Ryan Gold with the USGS in Golden, 00:00:14.800 --> 00:00:18.320 Colorado; Harrison Gray with the USGS Luminescence Dating 00:00:18.320 --> 00:00:22.000 Laboratory in Denver, Colorado; and Sylvia Nicovich with the 00:00:22.000 --> 00:00:25.416 Bureau of Reclamation in Denver, Colorado. 00:00:25.440 --> 00:00:29.736 Okay, so, as those who have worked with paleoseismic data know 00:00:29.760 --> 00:00:32.216 geochronological data can be messy. 00:00:32.240 --> 00:00:35.680 Noisy age data can typically relate to the depositional 00:00:35.680 --> 00:00:39.096 and geomorphic setting of the trench or exposure. 00:00:39.120 --> 00:00:43.176 Mechanisms, either known or unknown, of sediment transport and deposition. 00:00:43.200 --> 00:00:44.800 Age inheritance, such as recycled 00:00:44.800 --> 00:00:48.696 charcoal, and post-depositional modification, including burrowing. 00:00:48.720 --> 00:00:51.440 These factors lead to a poor understanding of the contextual 00:00:51.440 --> 00:00:54.456 uncertainties of samples and the resulting ages, 00:00:54.480 --> 00:00:58.000 inconsistent methods of constructing Bayesian models, and over- and 00:00:58.000 --> 00:01:00.696 under-constrained models of earthquake timing. 00:01:00.720 --> 00:01:04.320 This is illustrated in the conceptual figure here, which plots earthquake 00:01:04.320 --> 00:01:07.496 timing uncertainty versus the number of ages. 00:01:07.520 --> 00:01:10.160 This is simply meant to illustrate that models with limited ages 00:01:10.160 --> 00:01:13.736 do a poor job of refining earthquake timing uncertainties. 00:01:13.760 --> 00:01:16.400 For example, at some stages, timing uncertainty may actually 00:01:16.400 --> 00:01:20.216 increase with an increase in the number of samples. 00:01:21.120 --> 00:01:25.200 So considering these processes and uncertainties, how do we develop 00:01:25.200 --> 00:01:30.160 sampling strategies for geochronology that maximize the accuracy and, 00:01:30.160 --> 00:01:33.976 critically, the reproducibility of paleoseismic rupture histories. 00:01:34.000 --> 00:01:37.040 In this presentation, I’ll argue that portable optically stimulated 00:01:37.040 --> 00:01:40.240 luminescence, or portable OSL, can help. 00:01:40.240 --> 00:01:43.840 I’ll go through the background of the method, results from a field site, 00:01:43.840 --> 00:01:46.456 and end with some practical applications. 00:01:46.480 --> 00:01:49.256 Okay, so back to our conceptual diagram. 00:01:49.280 --> 00:01:52.880 This is where we want to be, highlighted in yellow, constructing 00:01:52.880 --> 00:01:57.736 Bayesian models of earthquake timing based on abundant age control. 00:01:57.760 --> 00:02:01.680 So what is portable OSL? Portable OSL is the determination of 00:02:01.680 --> 00:02:06.240 bulk luminescence as measured in a portable reader from small samples. 00:02:06.240 --> 00:02:09.040 The measurement is made without the usual procedures used for 00:02:09.040 --> 00:02:12.400 traditional OSL, for example separating quartz grains 00:02:12.400 --> 00:02:17.256 of a uniform grain size, and thus does not yield absolute ages. 00:02:17.280 --> 00:02:21.440 However, with constant lithology, dose rate across the exposure, 00:02:21.440 --> 00:02:24.080 and some pretreatment, bulk luminescence can reveal 00:02:24.080 --> 00:02:28.696 relative age and also show zones of partially bleached sediment. 00:02:28.720 --> 00:02:32.000 We applied these methods to a natural exposure of the Wasatch Fault at 00:02:32.000 --> 00:02:35.760 the Deep Creek site in central Utah. The figure in the upper right shows 00:02:35.760 --> 00:02:38.960 a slope shade map of the site with the Wasatch Fault scarp on a 00:02:38.960 --> 00:02:43.360 Holocene alluvial fan surface marked by black arrows. The red arrow marks 00:02:43.360 --> 00:02:46.456 a natural exposure of the fault shown here in the photograph. 00:02:46.480 --> 00:02:49.360 At the site, several meters of exposed alluvial fan gravel 00:02:49.360 --> 00:02:53.120 have been vertically displaced about 1.8 meters by a single 00:02:53.120 --> 00:02:56.456 prehistoric surface-rupturing earthquake. 00:02:56.480 --> 00:02:59.600 We studied the Wasatch Fault exposure hidden behind the gray trap 00:02:59.600 --> 00:03:02.613 here and highlighted by the white box. 00:03:03.280 --> 00:03:06.000 The exposure consisted of faulted alluvial fan gravel 00:03:06.000 --> 00:03:09.096 with a 30-centimeter-thick paleosol. 00:03:09.120 --> 00:03:12.560 The paleosol is faulted and buried by about a 1.5-meter-thick 00:03:12.560 --> 00:03:16.160 scarp drive colluvial wedge. The colluvial wedge consists of 00:03:16.160 --> 00:03:20.616 moderate- to steeply dipping silt, sand, and gravel interbeds, 00:03:20.640 --> 00:03:22.936 shown there with the dashed lines. 00:03:22.960 --> 00:03:26.240 Our principle goal was to test whether we could generate an age map for 00:03:26.240 --> 00:03:31.256 the exposure using portal OSL. So related questions included, 00:03:31.280 --> 00:03:35.440 are we able to resolve spatial trends in the portable OSL data, 00:03:35.440 --> 00:03:39.496 how do sedimentary and pedogenic processes affect the results, 00:03:39.520 --> 00:03:43.416 and do the data help us understand earthquake timing. 00:03:43.440 --> 00:03:47.840 To help make sense of how portable OSL data relate to age, we also extracted 00:03:47.840 --> 00:03:52.240 samples for radiocarbon and traditional OSL dating, with the results shown here 00:03:52.240 --> 00:03:57.680 in thousands of years before present. In total, 23 radiocarbon ages shown 00:03:57.680 --> 00:04:01.440 here by the black pluses, and 11 traditional OSL ages shown by 00:04:01.440 --> 00:04:04.640 the white pluses, constrain the timing of sediment deposition 00:04:04.640 --> 00:04:08.800 and soil formation at the site. These results suggest that alluvial fan 00:04:08.800 --> 00:04:13.040 deposits at the site are as old as about 13,000 to 7,000 years in the footwall 00:04:13.040 --> 00:04:15.656 and 8,000 to 5,000 years in the hanging wall. 00:04:15.680 --> 00:04:18.560 Paleosol formation occurred between around 4,000 years and 00:04:18.560 --> 00:04:21.920 shortly after around 1,000 years. With some exceptions that 00:04:21.920 --> 00:04:24.320 I’ll discuss in later slides, colluvial wedge sediments 00:04:24.320 --> 00:04:27.736 were deposited mostly in the past 1,000 years. 00:04:27.760 --> 00:04:31.360 With then extracted 342 samples for portable OSL, shown here 00:04:31.360 --> 00:04:35.200 by the white circles. The samples were arranged in a grid across the site 00:04:35.200 --> 00:04:39.416 without regard to the stratigraphic contexts or faults. 00:04:39.440 --> 00:04:43.760 Just a few notes about these samples. We collected small 3- to 4-centimeter- 00:04:43.760 --> 00:04:48.136 diameter samples using film canisters in darkroom conditions. 00:04:48.160 --> 00:04:50.480 The samples were spaced 10 centimeters vertically and 00:04:50.480 --> 00:04:55.200 about 15 centimeters horizontally. We sieved the sediment on-site, 00:04:55.200 --> 00:04:58.000 and off-site weighed similar-size aliquots before measuring 00:04:58.000 --> 00:05:01.920 in the portable OSL reader. We normalized the photon counts 00:05:01.920 --> 00:05:05.360 by sample weight because of the extreme range in low to high 00:05:05.360 --> 00:05:09.256 OSL results, plot the log of the photon counts. 00:05:09.280 --> 00:05:12.320 The portable OSL results are colored here by luminescence. 00:05:12.320 --> 00:05:15.576 In this and later slides, the color scheme will be the same, 00:05:15.600 --> 00:05:18.320 gradient from yellow to blue, with yellow indicating the 00:05:18.320 --> 00:05:21.496 greatest luminescence signal and blue the least. 00:05:21.520 --> 00:05:26.136 These results correspond well with the radiocarbon and traditional OSL ages, 00:05:26.160 --> 00:05:30.720 thus we used a simple linear regression shown here at the lower left to relate 00:05:30.720 --> 00:05:34.719 photon counts from the portable OSL reader to age. 00:05:35.360 --> 00:05:39.176 Here’s a surface interpolation based on the portable OSL results. 00:05:39.200 --> 00:05:41.440 Again, the color grades from yellow to blue, 00:05:41.440 --> 00:05:45.096 showing decreasing OSL signal and thus age. 00:05:45.120 --> 00:05:48.400 Here the radiocarbon and traditional ages are also shown and colored in the 00:05:48.400 --> 00:05:51.920 same way as the portable OSL map, and you can see the general agreement 00:05:51.920 --> 00:05:56.616 across the alluvial fan, paleosol, and colluvial wedge. 00:05:56.640 --> 00:06:00.776 In the next series of slides, I’ll focus just on the portable OSL age map 00:06:00.800 --> 00:06:04.696 and highlight fine to coarse gradients in age across the exposure. 00:06:04.720 --> 00:06:08.640 For example, as expected, the alluvial fan age of both the footwall and 00:06:08.640 --> 00:06:13.256 hanging wall decreases vertically, but not horizontally. 00:06:13.280 --> 00:06:17.976 We also observe a strong age gradient from the paleosol to the colluvial wedge 00:06:18.000 --> 00:06:23.157 and also across the buried free face from the footwall to the hanging wall. 00:06:23.920 --> 00:06:27.976 However, we find more nuanced age complexity in the paleosol. 00:06:28.000 --> 00:06:31.600 For example, on the right side, adjacent to the fault and buried free face, 00:06:31.600 --> 00:06:35.736 the portable OSL map suggests rapid burial of the paleosol. 00:06:35.760 --> 00:06:38.320 In comparison, at a more fault-distal position, 00:06:38.320 --> 00:06:42.640 the map suggests continued soil formation at the top of the paleosol 00:06:42.640 --> 00:06:46.296 and possibly after the rupture may have occurred. 00:06:46.320 --> 00:06:49.360 Within the wedge, we note a prominent area of poorly bleached sediment 00:06:49.360 --> 00:06:53.600 close to the fault and buried free face. Sediment in this part of the wedge 00:06:53.600 --> 00:06:58.000 was likely not fully exposed to sunlight during transport, either as 00:06:58.000 --> 00:07:01.920 the result of block formation or a short transport path. 00:07:01.920 --> 00:07:04.800 Elsewhere within the wedge, the age decreases laterally 00:07:04.800 --> 00:07:09.016 from the fault and vertically toward the surface, as expected. 00:07:09.040 --> 00:07:11.920 I just wanted to quickly show that, with these data, we can quantify 00:07:11.920 --> 00:07:15.920 horizontal and vertical trends in the portable OSL data. 00:07:15.920 --> 00:07:18.640 In all cases shown here, we’re plotting the model 00:07:18.640 --> 00:07:23.200 portable OSL ages or, that is, the OSL photon counts converted to 00:07:23.200 --> 00:07:27.256 age using our linear regression versus distance. 00:07:27.280 --> 00:07:31.280 The left column highlights horizontal trends as portable OSL age is plotted 00:07:31.280 --> 00:07:35.520 against distance from the fault. So 1 meter on the X axis indicates 00:07:35.520 --> 00:07:40.000 a meter outboard of the fault. The data are shown in the upper figure, 00:07:40.000 --> 00:07:44.856 and in the lower figure, grouped into 0.5-meter distance bins. 00:07:44.880 --> 00:07:48.136 Horizontal trends in age are especially apparent in the lower figure. 00:07:48.160 --> 00:07:52.400 For example, the blue and orange arrows show that the colluvium age decreases 00:07:52.400 --> 00:07:56.560 laterally with distance from the fault, whereas, red and black arrows mark 00:07:56.560 --> 00:08:00.696 more laterally constant paleosol and alluvial fan ages. 00:08:00.720 --> 00:08:03.920 In the right column, distance above or below the paleosol is plotted 00:08:03.920 --> 00:08:08.880 against age to highlight vertical trends in the data. In these figures, the paleosol is 00:08:08.880 --> 00:08:13.896 marked by the shaded area between the solid and dashed and dotted lines. 00:08:13.920 --> 00:08:17.120 In these figures, 1 meter on the Y axis is a meter above 00:08:17.120 --> 00:08:21.176 the top of the paleosol and negative 1 meter is a meter below it. 00:08:21.200 --> 00:08:23.280 In the lower panel, the portable OSL results 00:08:23.280 --> 00:08:27.896 are grouped into 0.1- to 0.3-meter distance bins. 00:08:27.920 --> 00:08:31.200 In this case, vertical trends in portable OSL are apparent. 00:08:31.200 --> 00:08:34.960 For example, the red and black arrows show that the alluvial fan and paleosol 00:08:34.960 --> 00:08:38.456 ages decrease consistently toward the ground surface. 00:08:38.480 --> 00:08:41.520 In contrast, the blue arrow shows that the colluvium age 00:08:41.520 --> 00:08:44.296 is mostly constant vertically. 00:08:44.320 --> 00:08:47.920 Finally, we can use these results to explore how the spatial age 00:08:47.920 --> 00:08:50.456 variability relates to earthquake timing. 00:08:50.480 --> 00:08:53.496 Here we compare two earthquake horizons. 00:08:53.520 --> 00:08:57.440 The first is the stratigraphic event horizon, or stratigraphic position 00:08:57.440 --> 00:09:00.720 at which sediments are interpreted as pre-dating or post-dating the 00:09:00.720 --> 00:09:03.576 earthquake, shown here by the white arrows. 00:09:03.600 --> 00:09:07.760 We also define a chronologic event horizon, or position at which sediments 00:09:07.760 --> 00:09:10.216 are older or younger than the earthquake. 00:09:10.240 --> 00:09:14.000 Here we show three chronologic event horizons based on Bayesian model 00:09:14.000 --> 00:09:18.160 variations with the mean earthquake times converted to portable OSL age 00:09:18.160 --> 00:09:22.960 contours and shown on the age map. We find that the portable OSL contours 00:09:22.960 --> 00:09:27.120 at around 500 to 700 years, which are shaded gray and labeled 00:09:27.120 --> 00:09:30.240 as the apparent chronologic event horizon, have the greatest 00:09:30.240 --> 00:09:33.736 spatial overlap with the stratigraphic event horizon. 00:09:33.760 --> 00:09:36.880 However, notably, the stratigraphic and chronologic event horizons 00:09:36.880 --> 00:09:40.400 diverge close to the fault. This suggests that there are sedimentary 00:09:40.400 --> 00:09:44.160 facies within the fault-proximal colluvial wedge that were not mappable 00:09:44.160 --> 00:09:47.280 from sedimentary texture alone. Although these sediments are 00:09:47.280 --> 00:09:49.440 interpreted as younger than the earthquake based on the 00:09:49.440 --> 00:09:52.720 stratigraphic event horizon, the chronologic event horizon 00:09:52.720 --> 00:09:55.736 suggests a pre-earthquake sediment age. 00:09:55.760 --> 00:09:58.880 This shows that portable OSL can provide important chronological 00:09:58.880 --> 00:10:03.360 context for interpreting radiocarbon and traditional OSL ages as well as 00:10:03.360 --> 00:10:07.520 Bayesian models of earthquake timing and that these timing interpretations, 00:10:07.520 --> 00:10:12.056 based on stratigraphy alone, can be misleading. 00:10:12.080 --> 00:10:15.280 Okay, at this point, I’d like to shift gears and talk about practical 00:10:15.280 --> 00:10:18.800 applications of this method. If you recall, in portable OSL, 00:10:18.800 --> 00:10:21.600 we were measuring luminescence from bulk sediment samples. 00:10:21.600 --> 00:10:25.816 Because we don’t correct for organics, grain size, or class lithology, 00:10:25.840 --> 00:10:29.416 it’s ideal to try to keep variations in these factors to a minimum. 00:10:29.440 --> 00:10:33.656 So ideal site conditions would include low variability in sediment texture, 00:10:33.680 --> 00:10:37.760 minimal post-depositional modification, consistent dose rate across the 00:10:37.760 --> 00:10:41.736 exposure or information on how dose rate changes spatially, 00:10:41.760 --> 00:10:45.576 and sediments that are generally suitable for luminescence dating. 00:10:45.600 --> 00:10:48.400 Data density is also an important aspect of this. 00:10:48.400 --> 00:10:51.040 For the Deep Creek data set, we generated a 10-centimeter 00:10:51.040 --> 00:10:53.760 cell raster, however lower-resolution rasters 00:10:53.760 --> 00:10:57.576 are also suitable for resolving the spatial age relations. 00:10:57.600 --> 00:11:01.040 The figure here shows variations in raster density from 10 centimeters 00:11:01.040 --> 00:11:04.480 in the upper left to 100 centimeters in the lower right. 00:11:04.480 --> 00:11:07.680 We find that key details in the portable OSL data, such as the strong 00:11:07.680 --> 00:11:11.680 age gradient from the alluvial fan, the colluvial wedge sediments, and the 00:11:11.680 --> 00:11:14.560 area of poorly bleached sediment in the fault-proximal part of the colluvial 00:11:14.560 --> 00:11:19.576 wedge are still resolvable with the 20- to 47-centimeter cell rasters shown here. 00:11:19.600 --> 00:11:21.840 Thus, even in a lower density field application, 00:11:21.840 --> 00:11:26.376 this method could be useful for interpreting paleoseismic exposures. 00:11:26.400 --> 00:11:29.496 The last aspect to consider is sampling strategy. 00:11:29.520 --> 00:11:32.480 Although our sampling density is quite high for the Deep Creek site, 00:11:32.480 --> 00:11:36.320 we found the lower-density sampling strategies also reproduce the primary 00:11:36.320 --> 00:11:39.976 spatial relations observed in the full density data set. 00:11:40.000 --> 00:11:42.960 This figure shows portable OSL rasters generated using 00:11:42.960 --> 00:11:46.400 subsets of the original data. Points in black were included 00:11:46.400 --> 00:11:49.976 in the raster calculation, and those in white were excluded. 00:11:50.000 --> 00:11:52.640 So, for example, in the upper left-hand corner, the raster 00:11:52.640 --> 00:11:57.176 was generated using every other point, or 50% of the data. 00:11:57.200 --> 00:12:01.040 For the Deep Creek site, rasters generated using about 40 to 50% 00:12:01.040 --> 00:12:04.560 of the data reasonably reproduce the spatial age relations 00:12:04.560 --> 00:12:07.465 apparent in the original results. 00:12:08.320 --> 00:12:10.640 In general, sample transects oriented normal to the 00:12:10.640 --> 00:12:13.416 stratigraphic contexts are preferable. 00:12:13.440 --> 00:12:17.120 Again, this highlights that portable OSL, even with a low-density sampling 00:12:17.120 --> 00:12:23.096 strategy of, say, 100 or so samples can be used in a rapid field application. 00:12:23.120 --> 00:12:26.640 In conclusion, portable OSL is an additional tool to consider 00:12:26.640 --> 00:12:30.480 in paleoseismic investigations. At the Deep Creek site, the portable 00:12:30.480 --> 00:12:35.016 OSL age map yields insight into how spatiotemporal age variability 00:12:35.040 --> 00:12:38.160 relates to sedimentary and pedogenic processes. 00:12:38.160 --> 00:12:42.536 Our work suggests that stratigraphic and chronologic event horizons may diverge, 00:12:42.560 --> 00:12:45.920 which has implications for paleoseismic sampling strategies 00:12:45.920 --> 00:12:48.696 and Bayesian models of earthquake timing. 00:12:48.720 --> 00:12:52.960 In summary, portable OSL, even in a moderate-density field application, 00:12:52.960 --> 00:12:56.160 has the potential to provide insight into pre- and post-earthquake 00:12:56.160 --> 00:12:59.200 depositional processes and improve the accuracy 00:12:59.200 --> 00:13:02.800 of paleoseismic rupture histories. And so finally, a huge thanks to 00:13:02.800 --> 00:13:06.456 Harrison Gray and Sylvia Nicovich who spent many hours sampling. 00:13:06.480 --> 00:13:10.160 And I’m excited to announce that this research was just released in Geology. 00:13:10.160 --> 00:13:11.040 Thank you.