NASA ARSET Overview and Applications of OPERA-DISP to Monitor Groundwater Changes Part 3
The Story
Welcome to Part 3 of our advanced series on environmental monitoring and radar data: "NASA ARSET: Overview and Applications of OPERA-DISP to Monitor Groundwater Changes."In this episode of the NASA Live Video Podcast, we shift our focus underground to address one of the most critical resource challenges of our time—groundwater depletion. While groundwater cannot be seen directly from space, its movement and extraction cause subtle surface displacements. To track these changes, we dive deep into OPERA-DISP (Observational Products for End-Users from Remote Sensing Analysis - Displacement Product), a state-of-the-art radar dataset designed to map land subsidence and surface deformation with incredible precision.
Through the framework of NASA’s Applied Remote Sensing Training (ARSET) program, we break down how OPERA-DISP utilizes Interferometric Synthetic Aperture Radar (InSAR) to detect surface changes over time. We discuss how hydrologists, geologists, and water resource managers apply this high-resolution displacement data to infer aquifer compaction, monitor groundwater storage changes, and build sustainable water management strategies.
Whether you are a water management professional, a GIS analyst, an environmental scientist, or someone fascinated by how satellite radar technology reveals hidden underground resources, this episode concludes our series with vital real-world insights. Subscribe to the NASA Live Video Podcast to catch up on previous parts and stay connected with the frontier of space exploration and earth science!
Speaker 1: Hello, everyone, Welcome back to this training on monitoring groundwater
Speaker 1: changes for Water Resources Management. This is Part three and
Speaker 1: the topic today is overview and applications of OPERA disp
Speaker 1: to monitor groundwater changes. OPERA is observational products for end
Speaker 1: users from remote sensing analysis and this is a splacement product,
Speaker 1: so we will be talking about that, and our guest
Speaker 1: picker for that today is doctor Eric Fielding from NASA
Speaker 1: Jet Proposion Laboratory. This is the final part of this
Speaker 1: training and there's one homework that's posted today. It opens
Speaker 1: today and it's available from the training website and the
Speaker 1: homework will be due on fifteenth of May. A certificate
Speaker 1: of completion will be awarded to those who attend all
Speaker 1: live sessions and complete the homework assignment before the two date.
Speaker 1: His brief review of what we saw in the last set.
Speaker 1: In Part two, we talked about Global Land Data Assimilation
Speaker 1: System version two point two. Land data assimilation systems, or altas.
Speaker 1: They integrate data from various sources using algorithms that represent
Speaker 1: knowledge of physical processes to fuel special and temporal gaps.
Speaker 1: Gilda's two point two integrates grace and grace followen observations
Speaker 1: we talked about these in part one of the Straining
Speaker 1: and so Gildas assimilates terrestrial water storage with other information
Speaker 1: using data assimilation techniques enabling spatial and temporal downscaling and
Speaker 1: vertical desegregation. Child's two point two soil moisture and groundwater
Speaker 1: output has been evaluated extensively using ground based observations. There
Speaker 1: are a couple of limitations to this data. The model
Speaker 1: does not simulate water management, that is, groundwater pumping, so
Speaker 1: it cannot effectively downscale grace or grace follow on observations,
Speaker 1: but direct human impacts are significant, and the model does
Speaker 1: not simulate confined a prefer storage changes, which may be
Speaker 1: an important components of total water storage changes observed by
Speaker 1: Grace and greasewallowing in certain regions. Gilda's two point two
Speaker 1: output are updated monthly on GEES disc site, and associated
Speaker 1: wetness and drought indicator maps and monthly forecasts are updated
Speaker 1: weekly on the National Drought Mitigation Center website. This brings
Speaker 1: us to today's session and so objectives for today are
Speaker 1: that by the end of part three you will be
Speaker 1: able to identify characteristics of opera surface displacement, product access
Speaker 1: and visualize opera dis data to infragroundwater change is at
Speaker 1: regional scale for applications. As in the previous two sessions,
Speaker 1: Please put your questions in the questions box and we
Speaker 1: will address them at the end of the webinar. Feel
Speaker 1: free to enter your questions as we go. We will
Speaker 1: try to get to all of the questions during the
Speaker 1: Q and A session after the webinar, and the remainder
Speaker 1: of the questions will be answered in the Q and
Speaker 1: A document which will be posted on the training website
Speaker 1: about a week after the training. With that, I want
Speaker 1: to introduce our guest speaker for today, doctor Eric Fielding.
Speaker 1: Doctor Fielding is a senior research scientist at NASA's Jet
Speaker 1: Proportional Laboratory and California Institute of Technology. He received his
Speaker 1: undergraduate degree in Earth sciences from Dartmouth College and his
Speaker 1: PhD in geological sciences from Cornell University. His expertise in
Speaker 1: processing synthetic aperture radar data and especially SAR interferometry. His
Speaker 1: research interests include mechanics of landslides, including transition from stable
Speaker 1: to unstable sliding, and effects of climate variations active tectonics,
Speaker 1: especially in the alpine Nimalayan Tibetan system on a variety
Speaker 1: of time scales, then fault interaction via the transfer of
Speaker 1: stresses through the lithosphere, and the possible implications for earthquake
Speaker 1: risk assessment. Doctor Fielding has received several awards including agu geotes,
Speaker 1: Ivan Muller Award for Service and Leadership, several NASA Exceptional
Speaker 1: Scientific Achievement Medals, and Edward Stone Award for Outstanding Research Publications.
Speaker 1: Doctor Fielding has more than one hundred peer defeat publications
Speaker 1: and so we invite doctor Fielding to talk about Opera
Speaker 1: disk Eric.
Speaker 2: Thanks Amitia for the introduction. I'm going to be covering
Speaker 2: the use of the Opera displacement products to monitor groundwater changes,
Speaker 2: and I'm using some slides from Grace Ponto, who is
Speaker 2: also a JPL and part of the Opera Displacement Validation team.
Speaker 2: So I'm going to be doing an overview of the
Speaker 2: Opera displacement products and show some specific applications to understand
Speaker 2: how this particular type of product can be used for
Speaker 2: groundwater mount during. These are the objectives. I'm going to
Speaker 2: do a very quick overview of sorrow defrometry just to
Speaker 2: get the basic concepts we have previous rset trainings that
Speaker 2: cover this topic in much more detail, so I will
Speaker 2: to those as a good play to get the more
Speaker 2: details about the background. A little bit about what the
Speaker 2: interferometric phase, which is the basic measurement of soorro intofrometry
Speaker 2: tells us about the land surface and surface subsidence. And
Speaker 2: then understand what the opera which OPERA stands for the
Speaker 2: observational products for end users from Remote Sensing Analysis program
Speaker 2: displacement product measurements mean. And then we'll in the demonstration
Speaker 2: show some examples of what the OPERA displacement time series
Speaker 2: reveals about land subsidence in one of the larger subsidence
Speaker 2: areas in the United States, the California Central Valley. These
Speaker 2: are the previous are set, so these are good places
Speaker 2: to start if you want more detailed information on the
Speaker 2: process InSAR and SORROW analysis. So here's a review of
Speaker 2: the synthetic APPETU radar or sorrow interfrometry. The twenty seventeen
Speaker 2: R set training and twenty nineteen are set training on
Speaker 2: sorrow defrometry. I have much more details. I've reduced that
Speaker 2: it here to make it fit into the time that
Speaker 2: we have available. So the key thing there is that
Speaker 2: what we measure with sorrow defrometry is the phase of
Speaker 2: the radar signal. You may have seen in other sor
Speaker 2: analysis training or papers that there's the radaritude, but for
Speaker 2: interferometry we don't really pay attention to the amplitude when
Speaker 2: you look at the phase of the SAR signal, and
Speaker 2: the SAR phase is a measurement of how many oscillations
Speaker 2: of the radar wave there are between the antenna and
Speaker 2: the satellite and the ground. And one of the things
Speaker 2: to keep in mind is that we have the radar
Speaker 2: resolution and all the elements are objects within that resolution
Speaker 2: element which is roughly ten by ten or twenty by
Speaker 2: twenty meters, are added together into one phase measurement, and
Speaker 2: we also have this very large number of cycles of
Speaker 2: the radar wave between the satellite in the ground. But
Speaker 2: by taking the difference or interferogram, we basically subtract the
Speaker 2: phase from one observation from them the phase of another observation,
Speaker 2: and by that cancels out almost all of these effects,
Speaker 2: and we then get a measurement that's just the surface displacement.
Speaker 2: So basically we can simplify the phase as just being
Speaker 2: due to the distance, which is the letter row. Here
Speaker 2: at some other consonants that are due to the the
Speaker 2: radar of propagation and distance from the satellite and noise.
Speaker 2: And by taking the same measurement of a second image
Speaker 2: uh these other constants, we assume that these other constants
Speaker 2: are are the same. And when we then subtract phase
Speaker 2: one from phase to these other constants, then cancel out
Speaker 2: and therefore get rid of those and the remaining signal
Speaker 2: is the difference between the distances between of the two
Speaker 2: satellite images plus some amount of noise. So this is
Speaker 2: just a graphical representation of the same thing. At we
Speaker 2: take two different images at time one and time two,
Speaker 2: and the distance to the ground can change up by
Speaker 2: a small amount, and the phase tells us how much
Speaker 2: that distance changed between time one and time two. One
Speaker 2: of the key things about the sarfrometry. I didn't have
Speaker 2: time to get into the fact that we can also
Speaker 2: measure topography with SAR in defrometry. But here we're using
Speaker 2: SARN difframetry to measure displacement. That's this equation here, This
Speaker 2: this equation the second equation here, and you can see
Speaker 2: that the sensitivity to displacement is depending on the wavelength
Speaker 2: of the radar lambda four pi over lambda. That's the
Speaker 2: sensitivity to displacement, and we were using here today. We're
Speaker 2: going to be talking about data from the Sentinel one
Speaker 2: satellite that the radar wavelength is six centimeters. Other satellites,
Speaker 2: including the the nice Are NASA is SAR satellite that
Speaker 2: was just launched last year and now being calibrated, has
Speaker 2: a radar wave length of twenty four centimeters. So the
Speaker 2: Sentinel one satellite has a greater sensitivity because the radar
Speaker 2: wavelength is shorter. There is a sensitivity to topography, but
Speaker 2: we're not going to talk about that here. So the
Speaker 2: Opera Observational Products for end Users from Remote Sensing Analysis
Speaker 2: Project does systematic measurement of displacements from the Sentinel one project,
Speaker 2: but they also do several other types of analysis. It's
Speaker 2: a large scale project that's supported by the NASA Satellite
Speaker 2: Needs Working Group, which gets money directly from the Office
Speaker 2: of Management and Budget to support these products that are
Speaker 2: requested by other US government agencies. And all of the
Speaker 2: data is free and open, and we've been working hard
Speaker 2: to make this data what we call analysis ready, which
Speaker 2: means that the data is processed to a level where
Speaker 2: you can start using the data without having to do
Speaker 2: your own sophisticated processing. So there's these different products and
Speaker 2: I'll go into more in the next slide and Offergos
Speaker 2: uses data from a wide variety of missions, including a
Speaker 2: lance AT eight, lance AT nine, Sentinel one the SAR
Speaker 2: from the Copernicus European constellation, and Sentinel two is the
Speaker 2: optical imaging from the Copernicus uh constellation, and then NISAR,
Speaker 2: which is the new NASA satellite that is obviously a
Speaker 2: SAR mission. So these are the products that are that
Speaker 2: Opera is producing. H there's level two products. These are
Speaker 2: basically intermediate products that we don't that we are producing
Speaker 2: for the as part of the processing, but could be
Speaker 2: useful for other people. They're not so easy to use directly. There.
Speaker 2: Level three products are what most people are going to
Speaker 2: be using. There's the dynamics surface water extent that's a
Speaker 2: map of the surface water over time. It's dynamic because
Speaker 2: it's over time, and there's two different versions of the
Speaker 2: surface water extent. One is made from the the harmonize HLS,
Speaker 2: the harmonized Lancet Sentinel two data sets. So that's optical
Speaker 2: imaging and then a second version that's been It's made
Speaker 2: from the Sentinel one SAR imagery and in the future
Speaker 2: will be made from ANSAR. Those products are near global
Speaker 2: wherever the data is acquired, and they're updated as often
Speaker 2: as we get new images from Sentinel one and the
Speaker 2: harmonized Lancet Sentinel two. Similarly, the disturbance product. This is
Speaker 2: a measurement primarily of a disturbance to vegetation and other
Speaker 2: other things that happen to the surface, could be due
Speaker 2: to fires or people cutting down tree or whatever. These
Speaker 2: are very similar in there both there's two different versions,
Speaker 2: one made from the harmonized LANSATS Sentinel two and one
Speaker 2: made from the Sentinel one, and again these are near global,
Speaker 2: available on land almost everywhere. Today I'm going to be
Speaker 2: talking about the surface displacement product. This is mapping surface
Speaker 2: displacement from the Sentinel one and soon from Sentinel from NYSAUR.
Speaker 2: The coverage of this data set is in North America,
Speaker 2: not global, because of the large amount of cost of
Speaker 2: doing the more advanced processing for necessary for the displacements.
Speaker 2: In the future, the Opera Project is going to be
Speaker 2: making a vertical land motion product. The present placement product
Speaker 2: is in the radar line of sight, not UH separated
Speaker 2: into vertical or horizontal motion, and it's not tied to
Speaker 2: any any datum, whereas the vertical land motion product will
Speaker 2: be separated into vertical and horizontal displacements and it will
Speaker 2: be tied to GPS or other absolute datum. To make
Speaker 2: a product that's directly usable for measuring vertical land motion.
Speaker 2: UH from North America, similarly to the displacement product, and
Speaker 2: just recently just UH released is a troposphere e zenith delay.
Speaker 2: One of the effects that I didn't mention on radar
Speaker 2: you know from tree is that as the radar beam
Speaker 2: goes through the atmosphere, it can be slowed down slightly
Speaker 2: by the presence of water vapor in the atmosphere. And
Speaker 2: this tropospheric zeenus delay product can be used to correct
Speaker 2: for those atmospheric delays, and it is useful for applying
Speaker 2: to the opera displacement product. But it's actually a generic
Speaker 2: global estimate for any place in the world and can
Speaker 2: be used for any sore mission. I won't have time
Speaker 2: to go into that today. So this is the map
Speaker 2: of the displacement products for North America. This is the
Speaker 2: the the descending track. Now this is the assending track map.
Speaker 2: The assending is where the satellite is going north relative
Speaker 2: to the Earth's surface. Due to the way that the
Speaker 2: Copernicus system operates the Sentinel one satellite, they have good
Speaker 2: coverage of the eastern part of North America. Only with
Speaker 2: the assnding tracks. They have limited capacity to do two
Speaker 2: different look directions there, so for the eastern part of
Speaker 2: the US, only assending data is available. You'll notice that
Speaker 2: the the displacement product is only available for the part
Speaker 2: of Canada that's within two hundred kilometers of the border
Speaker 2: with the United States. Due to the wide spread a
Speaker 2: snow cover in northern that we decided to not include
Speaker 2: that in the processing. But the processing also goes down
Speaker 2: through Central America to the southern border of Panama. The
Speaker 2: coverage is North America with an asterisk because it doesn't
Speaker 2: cover the northern part of Canada. The Sentinel one data
Speaker 2: coverage varies with time. In some time intervals time periods,
Speaker 2: the passes were acquired with six day separation, other times
Speaker 2: twelve days, or another times that's twenty four days, and
Speaker 2: that depends on also on the location. For the western
Speaker 2: part of the US, especially the west coast because of
Speaker 2: the larger amount of deformation due to groundwater and earthquakes
Speaker 2: and other processes. They tend to they acquire bold assending
Speaker 2: and descending data and generally have more frequent coverage. And
Speaker 2: the opera processing starts in July twenty sixteen. The satellite
Speaker 2: Sentinel one A, the first Sentinel one satellite, was operating
Speaker 2: before that, but the coverage was less, so we just
Speaker 2: decided to start with July twenty sixteen. Nice Are data
Speaker 2: processing is waiting on the final calibration of the nice
Speaker 2: ART data, which should be completed by June this year,
Speaker 2: and the Opera team is working hard on getting that ready.
Speaker 2: And this is the first insur product from anywhere that's
Speaker 2: been certified by the Committee on Earth Observation Systems COOS
Speaker 2: as application ready data. So OPERA products have a number
Speaker 2: of layers. I'm going to be talking about some of
Speaker 2: these in detail. The frame number here is part of
Speaker 2: the final name because the OPERA products are processed on
Speaker 2: a frame on a frame basis using a frame definition
Speaker 2: that was created by the ASM. So I'm going to
Speaker 2: be specifically talking about the main primary data later the
Speaker 2: displacement and meters, but there's a second version of the displacement,
Speaker 2: which is what we call the short wavelength displacement. The
Speaker 2: short wavelength displacement layer has the the larger scale variations
Speaker 2: in displacement filtered out. Everything over about twenty five kilometers
Speaker 2: in spatial scale has been filtered out, and that short
Speaker 2: wavelength displacement is what they use for display in the
Speaker 2: ASF displacement portal, which I'll be talking about later. And
Speaker 2: then there's a whole set of these different quality metrics.
Speaker 2: I'm not going to go into this in great detail
Speaker 2: because it's kind of an advanced topic, but these years
Speaker 2: can be used to determine which which pixels of the
Speaker 2: of the product have good quality measurements and which may
Speaker 2: have a more noisy measurement. Okay, so that's the we're
Speaker 2: ready to go to the demonstration. I'm going to be
Speaker 2: giving a demonstration of that displacement portal and then doing
Speaker 2: some analysis. The displacement portal, as I mentioned, uses these
Speaker 2: short wavelength displacement filter versions. Then I'm going to show
Speaker 2: a Jupiter notebook for more into this analysis of the
Speaker 2: displacement products. And when you go to the displacement portal
Speaker 2: which is here, the displacement dot A SF DOT Alaska
Speaker 2: dot E d u uh. It comes up with this.
Speaker 2: This a disclaimer, which is just a reminder that what
Speaker 2: they're showing is the filtered displacement, which can work. It
Speaker 2: works well to highlight small scale deformation features, but large
Speaker 2: features like the Central Valley that I'm going to be
Speaker 2: talking about later are not very well image by this
Speaker 2: short wavelength. Okay, So now I'm going to go to
Speaker 2: the demo. Okay, So now I'm in the displacement portal.
Speaker 2: Right now, I'm looking at the descending track upward displacement
Speaker 2: products from Sentinel one. As I mentioned earlier, there's kind
Speaker 2: of a gap here in the eastern part of the
Speaker 2: United States where they have not been acquiring the data
Speaker 2: with the descending tracks. That's going to be one of
Speaker 2: the big advantages of nice Are is the nice Are
Speaker 2: has global coverage with both ascending and descending tracks. The
Speaker 2: nice Are engineers spent a lot of time developing a
Speaker 2: whole hardware and data system and downlink it did downlink
Speaker 2: to be able to cover the whole world with assending
Speaker 2: and descending data. There is coverage in the very northeast
Speaker 2: part of the United States and also around Houston, but
Speaker 2: most of the eastern part of the US is not
Speaker 2: available in the descending tracks, So I'm going to zoom
Speaker 2: in here. You could just zoom in with a with
Speaker 2: a scroll bar or or the plus button over here.
Speaker 2: The scroll bar works for a nicely if you have
Speaker 2: a scroll a wheel on your mouse. And here we
Speaker 2: can see that these are groundwater subsidence areas in Arizona,
Speaker 2: in New Mexico and Texas, and also I think northern Mexico.
Speaker 2: Because these are relatively small areas of subsidence, the short
Speaker 2: wavelength filter is not changing the values too much. You
Speaker 2: can see that there's kind of a halo of what
Speaker 2: looks like apparent uplift around the edges. That's a filtering artifact.
Speaker 2: But we can click on a point here and the
Speaker 2: displacement portal goes out and gets the opera displacement products
Speaker 2: for that point and will show us a time series
Speaker 2: for the whole data set at that point. Takes a
Speaker 2: little bit of time because they have to go through
Speaker 2: a lot of files. And here we can see the
Speaker 2: time series from July twenty sixteen or August twenty sixteen
Speaker 2: through the last point here is September twenty twenty two.
Speaker 2: They are working on continuously updating this time series, so
Speaker 2: they're trying to get up to the very most recent
Speaker 2: data soon. And one of the things to notice here
Speaker 2: is that this is subsidence due to groundwater extraction, and
Speaker 2: it's highly seasonal. During the winter, when it's raining and
Speaker 2: they're not trying to grow so many crops, the surface
Speaker 2: is relatively stable. And then in the summer, when they're
Speaker 2: using lots of groundwater to irrigate their crops and extracting
Speaker 2: it out of the subsurface, then the ground surface subsides.
Speaker 2: So that's why we can see this very systematic level
Speaker 2: and then subsidence pattern over the whole almost almost ten
Speaker 2: years here, and we can see the same thing on
Speaker 2: other groundwater basins. It's a very common feature. That first
Speaker 2: point had a total subsidence of zero point four meters
Speaker 2: that's forty centimeters in nine years, and this new point.
Speaker 2: So the portal has a way of showing points that
Speaker 2: are not well determined as these kind of open or
Speaker 2: dash circles. Because I clicked on a point that has
Speaker 2: probably some agricultural fields in it during the time that
Speaker 2: they're plowing those fields. The opera displacement product cannot be measured,
Speaker 2: so then it ends up being these dashed circles. But
Speaker 2: the way that the opera displacement product is processed is
Speaker 2: able to get an overall time series even when there's
Speaker 2: these gaps where the measurements are not good quality? Can
Speaker 2: we erase those points? Uh? Oh before I go away
Speaker 2: from this area, I'm gonna just switch. You could use
Speaker 2: this little uh flight direction button here to change the
Speaker 2: flight direction. So these are This is now the assnding
Speaker 2: track data. Yeah, we can see that the groundwater line
Speaker 2: of sight displacement in the radar line of sight is
Speaker 2: very similar for the ascending and descending tracks. In this
Speaker 2: particular area, it seems that there's more gaps in the
Speaker 2: ascending track than they are in the descending track.
Speaker 1: Uh.
Speaker 2: Where you don't see a dot, that means that they
Speaker 2: didn't actually turn on the satellite on that date. So
Speaker 2: I'm gonna zoom out again. This is the ascending track.
Speaker 2: As I showed earlier in the slide. It has much
Speaker 2: more complete coverage, including all of the eastern US. Most
Speaker 2: of the eastern US doesn't have so much groundwater extraction,
Speaker 2: but there are some hotspots. Houston Texas in Galveston is
Speaker 2: one of the areas where there's a lot of groundwater extraction. Yeah,
Speaker 2: we can look at a point here and you can
Speaker 2: actually zoom in here to see the full resolution thirty
Speaker 2: meter pixels if you want to get the pixel that
Speaker 2: includes your house or whatever or some other feature. So
Speaker 2: here we can see that the ground the groundwater extraction
Speaker 2: seems to be more constant without that strong seasonal variation,
Speaker 2: and the total subsidence here is a little bit more
Speaker 2: than it's around twelve zero point one one two or
Speaker 2: meters or twelve centimeters. Now I'm going to take a
Speaker 2: quick look at the California Central Valley and here you'll
Speaker 2: notice that it looks very well. If you know what
Speaker 2: the subsidence in the Central Valley looks like, this is
Speaker 2: going to look very strange. And that's because the overall
Speaker 2: subsidence over a long spatial scale has been filtered out,
Speaker 2: and what we're seeing is just local variations. So it
Speaker 2: looks like there's little areas that are going up and down.
Speaker 2: But that's because the overall subsidence has been subtracted out.
Speaker 2: And that's why I'm going to show you next how
Speaker 2: to look at the full the full unfiltered data with
Speaker 2: a notebook Jupiter notebook. This other feature over here is
Speaker 2: the signal from the twenty nineteen Ridgecrest earthquake. It was
Speaker 2: a nineteen seven point one earthquake that was actually preceded
Speaker 2: by a six point four earthquake. This line here was
Speaker 2: the six point four and this was the rupture of
Speaker 2: the seven point one. This is also a little bit
Speaker 2: affected by the filtering, but it shows the earthquake signal. Okay,
Speaker 2: so I'm going to switch to a different tab now. Okay,
Speaker 2: So this is a Jupiter notebook that was Yes, this
Speaker 2: is a Jupiter notebook that we're going to use to
Speaker 2: download a subset of offer our displacement products for a
Speaker 2: part of the Central Valley and then look at the
Speaker 2: full unfiltered displacement products. I'm not going to go into
Speaker 2: a lot of detail on this first set up part.
Speaker 2: It's possible to run. You can run this by setting
Speaker 2: up a condo environment and then running these commands here here.
Speaker 2: So this next, this is the cell where we actually
Speaker 2: specify what area we want to look at. You'll remember
Speaker 2: earlier I said that the opera products are processed on frames.
Speaker 2: I was about to mention that the in the displacement portal,
Speaker 2: when you click on a point, it shows you what
Speaker 2: frame I D that point is part of. So that's
Speaker 2: the kind of the easiest way to get the frame
Speaker 2: I D. But you can also get it by searching
Speaker 2: for yeah upper products in the regular Earth data or
Speaker 2: or asf vertex search. Then I specify a bounding that's
Speaker 2: just a pulling on with the four corners of the
Speaker 2: rectangle that I want to analyze this particular notebook. I'm
Speaker 2: using just the data from August twenty twenty two to
Speaker 2: August twenty twenty four. This is a time interval that
Speaker 2: was very I had had a lot of rainfall. The
Speaker 2: twenty twenty two twenty twenty three winter in California was
Speaker 2: extremely wet, one of the wettest in the last century,
Speaker 2: and the twenty twenty three twenty twenty four winter was
Speaker 2: also well above normal. So this time interval is a
Speaker 2: very wet period for California rainfall. So once you've specified
Speaker 2: your area, then the system will prompt you to enter
Speaker 2: your NASA Earth Data log in. You can't downlo load
Speaker 2: than there uper displacement products without having a NASA Earth
Speaker 2: Data log In account. This is free, but it requires
Speaker 2: registration and you have to enter your username and password.
Speaker 2: Here you can set up a file called net rc
Speaker 2: in your home directory with that Earth Data log in information,
Speaker 2: which is what I do to avoid having to enter
Speaker 2: this every time. It just reads from that file in
Speaker 2: your home directory. So this sell checks to make sure
Speaker 2: that I have the credentials for Earth Data, and then
Speaker 2: it's going to go out and download the data. Because
Speaker 2: I've already downloaded this data. It's going to very quickly
Speaker 2: realize that I've already downloaded it. So then it finishes.
Speaker 2: It can take quite a while, depending on your internet speed.
Speaker 2: It could take twenty minutes or or longer too, and
Speaker 2: depending on how big of an area you're trying to download.
Speaker 2: So it's now put those files in this subfolder called
Speaker 2: subset NCS. That's net CDFs and frame thirty eight five
Speaker 2: h two. So these are all the files. It's fifty
Speaker 2: nine files for that two year time interval. This this
Speaker 2: just checks to make sure there's nothing wrong with the files.
Speaker 2: So the next step looks at the files and gives
Speaker 2: basic information about each file. I didn't have a chance
Speaker 2: to I didn't make a slide earlier but the opera
Speaker 2: data is process and what we call mini stacks, about
Speaker 2: fifteen dates in a row are combined into a mini stack.
Speaker 2: This is a key part of the processing efficiency because
Speaker 2: we can't process the whole time series together. But in
Speaker 2: this case, over those two years, there's four different mini stacks.
Speaker 2: Each one has fifteen scenes except for this one that
Speaker 2: seems to be missing one scene, and within each mini stack,
Speaker 2: the reference date is the first date in the mini snack,
Speaker 2: but the last date of a mini snack is the
Speaker 2: same as the first date to the next mini stack,
Speaker 2: So this notebook is able to then reconstruct the whole
Speaker 2: time series without any any real additional calculation. So we
Speaker 2: can see here the first date is August tenth, twenty
Speaker 2: twenty two, and the last date is remember fifty eight,
Speaker 2: it's between. So the first day here is the reference
Speaker 2: date of that mini stack. This mini stack goes from
Speaker 2: February to July, and the last date is July thirtieth,
Speaker 2: twenty twenty four. So this then quickly does the referencing
Speaker 2: of those mini snacks. It sees all the files and
Speaker 2: then we need to choose a reference point.
Speaker 3: As MH the opera products and as with most in
Speaker 3: is our products.
Speaker 2: They're not referenced to any absolute reference system. They have
Speaker 2: their own internal it's just basically relative to the satellite orbit.
Speaker 2: So we need to choose a point that we think
Speaker 2: is not moving. In this case, I chose a point.
Speaker 2: It makes this plot here. This is the whole time series.
Speaker 2: I made a point that over here on the side
Speaker 2: of the of the central valley where it's stable ground
Speaker 2: and not not affected by the subsidence, as the reference point.
Speaker 2: But you can pick one here and it'll tell you
Speaker 2: what lat long. What the lat long of the point
Speaker 2: that you picked is here, and then you can enter
Speaker 2: this value into this next cell. I already entered in
Speaker 2: the reference point here that I had chosen earlier. But
Speaker 2: you can also use this tool to choose another point
Speaker 2: that's in an area of subsidence and get that latitude
Speaker 2: and longitude. And then this next cell. If you enter
Speaker 2: in the point for the plumbing the time series, then
Speaker 2: this next cell shows the full time series for that point. First,
Speaker 2: it shows the map it's from. Now re reference the map. No,
Speaker 2: that's the that's the w's this one. We're going to
Speaker 2: use that reference point.
Speaker 3: Uh.
Speaker 2: The opera products are actually in UTM coordinates. But the
Speaker 2: notebook is is converting the long point that I gave
Speaker 2: it into UTM coordinates to uh use with the Opera
Speaker 2: data product. Yeah, it's now re referenced the time series
Speaker 2: of that reference point that I gave it. It's going
Speaker 2: to make a new map here. Yeah, ok yeah, Okay,
Speaker 2: So this is now the accumulative displacement over the over
Speaker 2: the four years relative to the reference point. And the
Speaker 2: reference point is this point up here with the yellow dot.
Speaker 2: You can see it's at the edge of the Central Valley.
Speaker 2: This is all the big Central Valley of California, near
Speaker 2: the city of Fresno, and there's a small city here
Speaker 2: called Corcoran. This point here is near the city of Corcoram,
Speaker 2: and we can see the time series for that point
Speaker 2: in this next plot. In this case, I chose a
Speaker 2: point which in this time in a whole actually had
Speaker 2: very little net displacement. There was a little bit of
Speaker 2: displacement here in twenty twenty two before the heavy rains
Speaker 2: of the winter of twenty twenty two twenty twenty three started,
Speaker 2: and then it started moving back up later. So this
Speaker 2: is one of the things that is very which is
Speaker 2: a little bit unusual about this time interval, you can
Speaker 2: see this is the fully This is not the filtered
Speaker 2: time series. This is the full time series. And you
Speaker 2: can see that the eastern part of the central Valley
Speaker 2: here has continued to subside, but this western part over
Speaker 2: here has actually rebounded, and that's because there was enough
Speaker 2: rainfall that it started recharging the shallow aquifers enough that
Speaker 2: the ground surface actually started moving back up during this
Speaker 2: time at aval we have seen this before. There was
Speaker 2: a previous time between twenty fifteen and twenty nineteen where
Speaker 2: we also got a lot of rainfall, and there was
Speaker 2: a previous time when this western part of the Great
Speaker 2: Valley also moved upwards. So this is one of the
Speaker 2: This is one of the key pieces of information that
Speaker 2: the InSAR can provide where Grace is going to be
Speaker 2: averaging over this whole area and showing that maybe there's
Speaker 2: a reduction in the water groundwater extraction, but it won't
Speaker 2: show you the spatial distribution of the surface effects of
Speaker 2: what the groundwater is doing. And with the ins are
Speaker 2: we here we can see that the western part of
Speaker 2: the Grade Valley is actually moved up in these two
Speaker 2: years due to significant groundwater recharge, and this eastern part
Speaker 2: is still moving down, but as I'll show you shortly,
Speaker 2: the rate of subsidences much less than in a previous
Speaker 2: time at all.
Speaker 1: Yeah.
Speaker 2: So then there's a bunch of more notebooks that show
Speaker 2: more information about the details of the equality metrics. This
Speaker 2: first one is the there's a number of different quality metrics.
Speaker 2: I don't really have time to get into all of them.
Speaker 2: Here there is a layer that you could look at.
Speaker 2: It's the short wavelength displacement. I'm not gonna we already
Speaker 2: saw that in the displacement portal, ah, one of.
Speaker 4: The yeah, yeah, yeah, the main it's.
Speaker 2: So I'm gonna show the here.
Speaker 1: Yeah.
Speaker 2: So this is showing the whole set of time of layers.
Speaker 2: This is the overall displacement, with the subsidence in the
Speaker 2: eastern part of the valley and in the a slight
Speaker 2: uplift in the western part. This is the short wavelength displacement, which,
Speaker 2: as I mentioned in the in the portal, it has
Speaker 2: this very strange fact where there's very large scale long
Speaker 2: wavelength displacement has been removed. One of the layers is
Speaker 2: called the recommended mask, and this is a starting mask
Speaker 2: to mask out the less accurately measured locations, and you
Speaker 2: can see that there are many of these fields that
Speaker 2: were not well measured int This area here was actually
Speaker 2: flooded for almost a year due to the extremely high
Speaker 2: precipitation in twenty twenty three. It formed a lake there
Speaker 2: they called Lake Tulari, which was a historical lake but
Speaker 2: then was drained for agriculture, but came back because there
Speaker 2: was enough rainfall. These are some of the other quality metrics.
Speaker 2: Temporal coherence is showing how coherent the measurements are with time.
Speaker 2: Corcorant is this in cities show up as very highly
Speaker 2: coherent because the buildings reflect the radar very well. Estimated.
Speaker 2: Phase quality is similar to the temporal coherence, and you
Speaker 2: can see this area here with the low phase quality
Speaker 2: is the area of that lake that formed in twenty
Speaker 2: twenty three, Yeah, causing the measurements to be inaccurate during
Speaker 2: that time in the hole. And then there's there is
Speaker 2: a water mask where permanent water is massed out, but
Speaker 2: there's very few permanent lakes here. This Lake Tulare is
Speaker 2: a temporary lake. There are some other types of measurements
Speaker 2: that I'm not going to go into here for the
Speaker 2: sake of time. So Finally, this cell here does a
Speaker 2: velocity estimation, and it's just going to take a linear
Speaker 2: fit to all the points in each pixel to estimate
Speaker 2: the average volney over the two year interval. And this
Speaker 2: particular step can actually take a lot of time to
Speaker 2: run and and quite a bit of memory. So I
Speaker 2: wouldn't run this unless your computer has at least thirty
Speaker 2: two gigabytes of round for for this very large area.
Speaker 2: For smaller areas, it doesn't use so much memory. It's
Speaker 2: something that I want to improve later. And then down here,
Speaker 2: this is the estimated UH average velocity for the for
Speaker 2: the two year time in a hole. And here we
Speaker 2: can see UH this western part where the recharge occurred
Speaker 2: with velocity on the order of six to six centimeters
Speaker 2: a year, or a little bit more in some places.
Speaker 2: And over here in the in the east part of
Speaker 2: the central valley it was subsiding around six centimeters per
Speaker 2: year during these two years. So this is a this
Speaker 2: is a significant a product that you can extract from
Speaker 2: the opera time series using this notebook. Then this later
Speaker 2: part is actually taking these products that we generated, the
Speaker 2: velocity and other other products and exploiting them to file
Speaker 2: formats that we can load into a time series program
Speaker 2: called mint pie or q GIS. And I'm not going
Speaker 2: to go through all these details the QGIS products.
Speaker 1: It.
Speaker 2: Actually there's different versions of the recommended mask. This is
Speaker 2: the most strict. It removes the most area, especially in
Speaker 2: this area of Lake Chuwari, whereas this one over here
Speaker 2: is a more lenient mask that allows it to try
Speaker 2: to estimate the velocity in that area from the points
Speaker 2: before and after the formation of the lake. And so
Speaker 2: it actually exports three these different files and it writes
Speaker 2: out the geotfs here. They can be loaded into h GIS.
Speaker 2: It also makes images for all the dates, so those
Speaker 2: export files go into this export directory. UH. These are
Speaker 2: the different files.
Speaker 1: UH.
Speaker 2: These are the as As I mentioned, there's three different
Speaker 2: versions of the recommended mask.
Speaker 1: UH.
Speaker 2: And then there's a velocity UH file here. It's based
Speaker 2: on the recommended mask converted to sentimeters. So now I'm
Speaker 2: going to bake a quick jump to the UH pretty
Speaker 2: popular q g I s g I S program. UH.
Speaker 2: This is available for Mac, PC Linux and so it's
Speaker 2: a very multi purpise international, free and open source GIS package. UH.
Speaker 2: It's can also be the same thing kind of things
Speaker 2: can be done with r g I S for those
Speaker 2: who have the commercial r GIS package or or other
Speaker 2: GIS packages. Okay, okay, So this is the the average
Speaker 2: velocity map loaded into q g i S. It's the
Speaker 2: notebook actually reprojected it from the UTM coordinates to allow
Speaker 2: long coordinates to make it easier to look at. But
Speaker 2: i've I'm actually using QGIS to to re display it
Speaker 2: in the in UTM coordinates, so it's not as a
Speaker 2: more accurate map coordinate system. And here I have also
Speaker 2: added in QGIS a Google satellite image, which is one
Speaker 2: of the layers that q I GIS offers as a background.
Speaker 2: It's a I can wait a minute. This is This
Speaker 2: is the twenty twenty four velocity map with the rebound
Speaker 2: in the western part of the Central Valley. And if
Speaker 2: we turn this off you can see the all the
Speaker 2: agriculture and you can see that they Google Earth actually
Speaker 2: captured this when there was so a significant part of
Speaker 2: the Tolare Lake here. So this is the twenty twenty
Speaker 2: twenty four average velocity. And I did the similar analysis
Speaker 2: with the time interval from August twenty twenty nineteen to
Speaker 2: twenty twenty two. This was a three year time interval
Speaker 2: of precipitation, and here you can see that the average
Speaker 2: subsidence rate is much much higher. This is the the
Speaker 2: color scheme here is that the the notebook converted the
Speaker 2: subsidence rate into centimeters per month, and these areas of
Speaker 2: deep blue here are subsiding at one and a half
Speaker 2: centimeters per month, or over thirty centimeters per year. That's
Speaker 2: that's a big amount. Whereas if we go back to
Speaker 2: the twenty twenty two twenty twenty four we can see
Speaker 2: that these subsidence rates are are much much lower in
Speaker 2: the area that's still subsiding and the western part is rebounding.
Speaker 2: So that's just a very quick introduction to how we
Speaker 2: could load these products into QGIS or other GIS programs
Speaker 2: to have a better view of what the results look like.
Speaker 2: And these particular versions of the are using the recommended
Speaker 2: mask with a pretty with a moderately strict coverage. So
Speaker 2: the Tlare lake is largely massed out here in the
Speaker 2: twenty twenty two twenty twenty four image, but more complete
Speaker 2: in the twenty nineteen to twenty twenty two image. There's
Speaker 2: also a lake down here that actually stayed even longer.
Speaker 2: I forget the name of that lake. So now I
Speaker 2: think that's a very quick demonstration, but I hope that's informative.
Speaker 2: And I'm just going to go back to these slides
Speaker 2: to show some resources of web pages that you can
Speaker 2: use to go back and look at the background for
Speaker 2: Opera and the displacement products. Okay, so these are some
Speaker 2: web page resources about the NASA Earth Data System, that
Speaker 2: is where all the Opera of Data products are stored,
Speaker 2: Satellite Needs Working Group, which supports the Opera project and
Speaker 2: other projects. In fact, the Harmonized landsat Sentinel to data
Speaker 2: products are another Satellite Needs Working Group product that we
Speaker 2: in the Opera project build on their product for some
Speaker 2: of those displacement I mean disturbance and water extent products.
Speaker 2: This is the displacement portal that I demonstrated. There's some
Speaker 2: product information about OPERA in general. There's a link to
Speaker 2: the GitHub page where the Opera Jupiter notebooks are shown,
Speaker 2: and in fact, you can also look at the Opera
Speaker 2: products in NASA Worldview. It's not as effective for the
Speaker 2: displacement products, but is very effective for the other OPERA
Speaker 2: products such as the water extent and disturbance products and
Speaker 2: I'd be happy to answer questions and I'll hand it
Speaker 2: back to a reader.
Speaker 1: Thank you so much, Eric for your presentation and information
Speaker 1: about opera disp especially for your demonstration about ASF disc
Speaker 1: portal and sharing your Jupiter notebook code with everyone. Just
Speaker 1: to summarize, we had a review of SAR interferometry, especially
Speaker 1: that phase of SAR signal is very important when you
Speaker 1: consider interferometry. So when two observations are made from the
Speaker 1: same location in space but at different times, the interferometric
Speaker 1: phase is proportional to any change in the range or
Speaker 1: distance of a surface feature, and that is used in
Speaker 1: producing opera DISP. It is derived from sentinel ones are
Speaker 1: imagery using interferometry. Opera disk products provide information or movements
Speaker 1: of the Earth's surface such as subsidence due to groundwater
Speaker 1: or oil and guest extraction, uplift due to water injection,
Speaker 1: and ground motion from tectonic faults, landslides and volcanoes. We
Speaker 1: also had an overview of opera displacement visualization portal available
Speaker 1: from Alaska sur Facility and after filling demonstrated Jupiter notebook
Speaker 1: code for in depth analysis of opera disc products. We
Speaker 1: saw how subsidence in Central Valley, California, looked at from
Speaker 1: disp indicated groundwater changes. This brings us to the end
Speaker 1: of this training. And in this training we focused on
Speaker 1: three different ways of looking at groundwater. So we first
Speaker 1: looked at Grace and Grace follow On, then Gilda's model
Speaker 1: and then Opera data products and we saw their characteristics.
Speaker 1: So Grace and Grace follow On they provide measurements of
Speaker 1: variations in mass or gravity changes over Earth surface and
Speaker 1: these gravity variations are interpreted in terms of changes in
Speaker 1: equivalent water thickness or terrestrial water storage t WS. Gled's
Speaker 1: version two point two integrates Grace and Grace follow on
Speaker 1: observations of t WS with other information using data assimilation
Speaker 1: enabling spatial and temporal downscaling of soil, moisture and groundwater.
Speaker 1: And finally Opera which uses central ones are as displacement
Speaker 1: product or disks that is also useful for monitoring groundwater
Speaker 1: depletion and recovery. As we saw, these are the characteristics
Speaker 1: of these data sets. Grace and Grace follow on missions
Speaker 1: they provide terrestrial water storage change data. These are global
Speaker 1: data sets. Resolution original is approximately three degree by three degree.
Speaker 1: Let you to longitude, but they're reprocessed at one degree
Speaker 1: by one degree and also at half a degree resolution.
Speaker 1: Temporal coverage is February two thousand and three to present,
Speaker 1: and there is a gap between July twenty seventeen to
Speaker 1: May twenty eighteen. That's the gap between Grace and Grace
Speaker 1: Fallen data are available on monthly timescale. Gilda's groundwater storage
Speaker 1: data that's also global and it's available at higher resolution
Speaker 1: quarter degree by quarter degree latitude longitude the same time
Speaker 1: period as Grace and Grace follow on as they're assimilated
Speaker 1: in here, and these data are available on daily timescale. Finally, Operatis,
Speaker 1: which is based on Centinel one data as a higher
Speaker 1: resolution thirty meters. It's right now away label only for
Speaker 1: North America and the duration of the data is July
Speaker 1: twenty sixteen to twenty twenty five and revisit time is
Speaker 1: about six to twenty four days depending on the location.
Speaker 1: We also had demonstrations and you had exercises for data access,
Speaker 1: analysis and visualization for Grace and Grace fall on terrestrial
Speaker 1: water storage changes. We looked at Grace data analysis tool.
Speaker 1: I want to bring another visualization tool which we did
Speaker 1: not have time to go through. But this mask on
Speaker 1: visualization tool is similar, but it also includes a GSFC
Speaker 1: mask on data at half a degree so you can
Speaker 1: explore that. But we looked at maps and time series
Speaker 1: based on this original Grace data analysis tool. Then we
Speaker 1: used GEO one n QGIS to look at Gilda's groundwater data.
Speaker 1: We had maps and time series and also looked at
Speaker 1: difference in groundwater so Groundwotter story change over different periods. Finally,
Speaker 1: today we had a demonstration on opera disc using ASF
Speaker 1: displacement portal and we will have some exercise based on that.
Speaker 1: There's one homework that's posted today on the training web
Speaker 1: page and answers must be submitted via Google forms. The
Speaker 1: homework is due on fifteenth of May. The certificate of
Speaker 1: completion will be awarded to those who attend all three
Speaker 1: live webinars, complete the homework assignment by the deadline, and
Speaker 1: then you will receive a certificate email approximately two months
Speaker 1: after completion of the course. Just to note here that
Speaker 1: for each train session we had exercise and some questions
Speaker 1: are based on those exercises, so please go through the
Speaker 1: exercises before you go to the homework. Once again, we
Speaker 1: want to thank our guest speakers, doctor Matthew Rottel and
Speaker 1: doctor Eric Fielding for their presentations and information about different
Speaker 1: data sets. You can see the trainer information here Doctor
Speaker 1: Rodell and doctor Fielding. You can contact them if you
Speaker 1: have any questions. This is the ourset team, my colleague
Speaker 1: Sean McCartney and edicup bodies. Along with that, you can
Speaker 1: contact any of us if you have any questions. This
Speaker 1: is our set website, our set YouTube link and for questions, comments,
Speaker 1: or to share how you have applied our training to
Speaker 1: your work or studies, please email at NASA dot R,
Speaker 1: set at gmail dot com and join our quarterly newsletter
Speaker 1: to stay up to date on our latest trainings. And
Speaker 1: for that you can send an email with no subject
Speaker 1: line to this email address and follow the instruction sending
Speaker 1: the response. Here are some useful resources used in this training.
Speaker 1: Thank you all, and we'll start with our question and
Speaker 1: answer session. We have a doctor Fielding here and so
Speaker 1: we can start with the question answer session. Welcome America
Speaker 1: and thank you for being here. So we'll start with
Speaker 1: question one. Is downscaling important for looking at groundwater drought
Speaker 1: index in a particular region? And Eric, you can unmute
Speaker 1: and answer the question.
Speaker 2: Please hello, Yes, this is a The drought index that
Speaker 2: the National Oceanic the National Weather Service in the United
Speaker 2: States makes is a estimate of the availability of surface
Speaker 2: water and shallow saw moisture. It does not directly measure
Speaker 2: ground water, so uh downscaling of that would would be possible,
Speaker 2: but they they estimate that based on the weather including
Speaker 2: precipitation and temperature, which are not which they use only
Speaker 2: a large scale measurements. The conversion of the drought index
Speaker 2: to the drought index is not directly measured groundwater, but
Speaker 2: areas of drought are often places where cities or farms,
Speaker 2: especially farms, will extract groundwater to continue their farming operations.
Speaker 2: So it's not the same thing. It's a different type
Speaker 2: of measurement, but they are related to.
Speaker 1: Great Thank you. Question two is what happens during a
Speaker 1: storm if opera has difficulty due to distance to capture data.
Speaker 2: So the opera surface water and disturbance products that use
Speaker 2: the optical harmonized landset Sentinel two inputs will be blocked
Speaker 2: by cloud cover and they will not have any measurement
Speaker 2: for the dates and pixels. Where there's cloud cover, the
Speaker 2: OPERA products based on SORROW measures, including the Sentinel one
Speaker 2: and soon Nice hours are images are not affected by clouds,
Speaker 2: and they have measurements for every past.
Speaker 1: Great question three. Can we apply OPERA DISP anywhere? For
Speaker 1: example the Middle East?
Speaker 2: So NASA only has funding to process the displacement products
Speaker 2: for North America, but the software that Opera uses is
Speaker 2: fully open so people could use the same software to
Speaker 2: process other areas.
Speaker 1: Thank you. Question for is I want to process Sentinel
Speaker 1: one data into displacement for small area of interest in
Speaker 1: different regions outside North America. Since Opera DISP is limited geographically,
Speaker 1: how difficult would it be to build a similar workflow?
Speaker 2: As I mentioned, the Opera software is available. Well, it's
Speaker 2: open source and on a GitHub. Processing a small area
Speaker 2: should be relatively easy. The main time series program is
Speaker 2: a program called Dolphin, and it can be used with
Speaker 2: Sentinel one or other SOUR data to analyze the time
Speaker 2: series and using the same algorithm that is used by Opera.
Speaker 2: The OPERA system does have a sophisticated workflow to enable
Speaker 2: continental scale processing, but you don't need that for processing
Speaker 2: a small area.
Speaker 1: Thank you. Question five. If we generate s pas insur
Speaker 1: time cities for a region using tools like by GMTSR,
Speaker 1: MINTBI or list s POS. How can we distinguish groundwater
Speaker 1: driven defamation from other processes like oil and gas extraction, tectonics,
Speaker 1: earthquakes or snow loading. How should we handle intracomparison and validation,
Speaker 1: and how to operate up products ensure consistency between seabands
Speaker 1: andinel one and ALB and NYSAR for long term monitoring.
Speaker 2: So the full separation of different geophysical and groundwater effects
Speaker 2: is beyond the scope of this training, but the time
Speaker 2: series data that's provided by the just Opera displacement product
Speaker 2: is very helpful for distinguishing different effects within the earth.
Speaker 2: The groundwater extraction in most places is typically seasonal, more
Speaker 2: in the dry seasons and less in the wet seasons,
Speaker 2: So if you see a seasonal variation in the displacements,
Speaker 2: that's a strong clue that the displacement is due to
Speaker 2: groundwater and not tectonic effects. Cut The second part of
Speaker 2: the question is about the how to opera products ensure consistency.
Speaker 2: The opera displacement products are processed separately for each Sentinel
Speaker 2: one track or and soon each nice our track. There
Speaker 2: is no additional processing to ensure consistency between the tracks,
Speaker 2: but the future Opera vertical land motion products, so that
Speaker 2: will have an additional processing to make to combine different
Speaker 2: sentinel one displacement tracks ascending and descending and with calibration
Speaker 2: with the local GNSS or g GPS data to make
Speaker 2: a consistent map of the vertical land vertical and horizontal
Speaker 2: land mush.
Speaker 1: Question six is for the Python demonstration, what is the
Speaker 1: velocity accuracy of this result? See five millimeter per year.
Speaker 2: Yes, the Opera products have a requirement to have an
Speaker 2: accuracy of five millimeters per years and that has been
Speaker 2: validated for places where the data has high quality. There
Speaker 2: are some areas where the InSAR coherence is low due
Speaker 2: to farm plowing fields or flooding or dense vegetation that
Speaker 2: is incoherent in central one seed bend data, and those
Speaker 2: are markets unreliable in the recommended matter that's included with
Speaker 2: the products, and there's no useful velocity measurements in those areas.
Speaker 1: Question seven for the Python demonstration are subsidence and delish
Speaker 1: and equal.
Speaker 2: There's a quite complex relationship between the volume of groundwater
Speaker 2: extracted and the amount of service. Subsidence This is determined
Speaker 2: by the characteristics of the groundwater reservoir, which varies greatly
Speaker 2: in different places, even within the same sedimentary basin, and
Speaker 2: the situation could be especially complex in places where there's
Speaker 2: groundwater reservoirs at different depths. They are not equal, but
Speaker 2: they're closely related it and require some advanced hydrological modeling
Speaker 2: of the ground border reservoir to better understand what the
Speaker 2: the reservoir characteristics and response are.
Speaker 1: Thank you. Question eight is I'm seeing some missing monthly
Speaker 1: data while working with the ASF data. What is the
Speaker 1: reason for this?
Speaker 2: The opera products are only available when the source data
Speaker 2: was acquired. The various satellites, especially Sentinel one, sometimes miss
Speaker 2: a few acquisitions or or change their change their acquisition plans.
Speaker 2: The Sentinel one constellation has had some changes over time.
Speaker 2: Initially they had just one satellite, they Sentinel one A.
Speaker 2: Then they added Sentinel one B, but then the Sentinel
Speaker 2: one B satellite stopped working in December twenty twenty one,
Speaker 2: so then they were back to having only one satellite
Speaker 2: until twenty twenty five when they got Sentinel one C
Speaker 2: in operation and they just I think earlier this month,
Speaker 2: declared Sentinel one d to be operational. So they're now
Speaker 2: back to full operational strength with two Sentinel one satellites.
Speaker 2: But during the especially during the time in the world
Speaker 2: where there was only one Sentinel one satellite, they had
Speaker 2: to reduce their data coverage because if they had less
Speaker 2: half the acquisition capacity, and if they didn't acquire the data,
Speaker 2: then Opera couldn't has no data point.
Speaker 1: Great, thank you. Question nine is when we downloaded that
Speaker 1: disk files, what is the best way to assign the
Speaker 1: reference based on a point or border of the mounting box?
Speaker 1: How is a reference point selected for measurement of displacement?
Speaker 1: Is there any specific point we should select?
Speaker 2: So you want to choose a reference point in a
Speaker 2: place that you know or have good reason to believe
Speaker 2: that the ground surface is not moving or stable. For
Speaker 2: groundwater studies, you typically want to have a point that's
Speaker 2: outside of the sedimentary basin nearby but not in the
Speaker 2: not likely to be affected by the subsidence. And the
Speaker 2: reference point also needs to be coherent in all the
Speaker 2: dates of the ins our time series. So for the
Speaker 2: Sentinel one display some products, you can't choose a point
Speaker 2: in an area where there's dense vegetation that will not
Speaker 2: have a good measurement and being coherent.
Speaker 1: The next question is question ten. What's the difference between
Speaker 1: a line of sight velocity deformation along slope horizontal and
Speaker 1: vertical deformation and how are they estimated using SAR?
Speaker 2: So the fundamental measurement that we get from the InSAR
Speaker 2: is the line of sight velocity. The single a single
Speaker 2: line of sight velocity from one track of data is
Speaker 2: not sufficient to be able to separate horizontal and vertical displacements.
Speaker 2: There are ways to combine two or more line of
Speaker 2: sight displacements to estimate what component of the displacement for
Speaker 2: each point is vertical and what part is horizontal. This
Speaker 2: is what the opera vertical land motion processing we'll be
Speaker 2: doing in the future. The if you only have two
Speaker 2: line of sight directions like you get from the ascending
Speaker 2: and descending sentinel one, then you only the only horizontal
Speaker 2: component that can be estimated is the east west direction.
Speaker 2: You can't estimate the north south component.
Speaker 1: Question eleven is is there any atmospheric correction applied to
Speaker 1: the level three or raw results when analyzing the displacement
Speaker 1: time series? Should we apply corrections like ionosphere delay, solid
Speaker 1: or tides et cetera.
Speaker 2: So the operator displacement products, the raw products that you
Speaker 2: get with from the time series files or do not
Speaker 2: have the atmospheric directions applied, but they do have extra
Speaker 2: layers in the in the file that include the ionospheric
Speaker 2: delay and solid earth tide estimation.
Speaker 1: The UH.
Speaker 2: These effects are really quite small for the c bend
Speaker 2: Sentinel one data, so for most purposes this is doing
Speaker 2: that those two corrections are not necessary. As I mentioned briefly,
Speaker 2: the opera product is providing a separate tropospher delay estimation
Speaker 2: that can be used to estimate and apply a troposfer
Speaker 2: delay correction. And these are much much larger than the
Speaker 2: amosphere or solid earth tide corrections, but requires some a
Speaker 2: little bit of extra work to add to your analysis
Speaker 2: group not covered here, just to.
Speaker 1: Make a point that the simple file that you have
Speaker 1: in your exercise will show a different layers that includes
Speaker 1: what doctor Filling is mentioned and question twelve in the
Speaker 1: displacement portal, there are many pixels over a water body.
Speaker 1: Why why were the pixels not removed by the water mask.
Speaker 2: The AESF displacement portal does include a water mask and
Speaker 2: a mask for areas of low InSAR coherence. There should
Speaker 2: not be pixels over a water body unless unless that
Speaker 2: water body was dried up for some reason. The Tu
Speaker 2: Laari Lake in the Central Valley of California is typically
Speaker 2: dry most of the time, but it did get water
Speaker 2: in it during the very heavy rainfall of the winter
Speaker 2: of twenty twenty three, so in that area we get
Speaker 2: a we had we could see that there was a
Speaker 2: measurements in the time in twenty three, and then during
Speaker 2: twenty twenty three when there was water there there's no measurements.
Speaker 1: Interesting question thirteen. In the time series that you shoot,
Speaker 1: does each point represent deformation with respect to the reference
Speaker 1: data or to the data immediately before. If we have
Speaker 1: deformation in time T times T one, T two, T three,
Speaker 1: the shown deformation in T three is deformation with reference
Speaker 1: to T two or T one. Assuming T one is
Speaker 1: a reference date.
Speaker 2: The time series is with reference to the reference date.
Speaker 2: So when I the opper products are process in these
Speaker 2: mini snacks, so there is a separate reference date for
Speaker 2: each mini stack. But the the Jupiter notebook that I
Speaker 2: had ties together the reference states for each mini stack,
Speaker 2: so that the whole time series is relative to the
Speaker 2: reference date of the first mini snack.
Speaker 1: That's great, And if you again look at the supplemental
Speaker 1: document in today's exercise, you will see that the file
Speaker 1: LIMB convention is explained in there. And then question fourteen,
Speaker 1: when analyzing displacement time series data, should we use unfiltered
Speaker 1: displacement or shortwave displacement?
Speaker 2: For almost every analysis you want to use the unfiltered displacement.
Speaker 2: The short wavelength displacement is just a visualization tool that
Speaker 2: makes it easy to show the displacement over a large
Speaker 2: area without worrying about local reference points, and it's not
Speaker 2: really usable for detailed analysis.
Speaker 1: Next question fifteen, is the displacement time series comparable with
Speaker 1: s PASS derived displacement time series?
Speaker 2: Yes, it's it should be comparable. The OPERA time series
Speaker 2: analysis uses a more sophisticated what we call persistent scatterer
Speaker 2: and distributed scatter analysis to get higher quality measurements, but
Speaker 2: the fundamental result should be similar to s PASS for most.
Speaker 1: So the next question also is like what algorithms? What
Speaker 1: algorithm uses opera to create the time series PSI or
Speaker 1: s BUS.
Speaker 2: The Opera algorithm is what we call it's a phase linking.
Speaker 2: It's called phase linking. It actually uses both persistent scatterer
Speaker 2: PSI InSAR and distributed scatterer in SAR, so it's kind
Speaker 2: of a combination of PSI and s PASS and the
Speaker 2: two measurements are combined into each thirty meter by thirty
Speaker 2: meter pixel.
Speaker 1: Next question is I received this message time series service
Speaker 1: earn no upera ice on burst frame IDs were found
Speaker 1: over the given AOI and the point is given here,
Speaker 1: what should I do? This is twenty nine longitude, which was.
Speaker 2: Yeah, this is outside of North America. There's not going
Speaker 2: to be any opera data outside of North America.
Speaker 1: I think it's not in North America. So question eighteen
Speaker 1: are the velocity maps and average or total for years?
Speaker 2: The calculation that I showed in the notebook is the
Speaker 2: average over the time and of ALE. So I showed
Speaker 2: two different calculations. One was the average velocity from twenty
Speaker 2: nineteen to twenty twenty two, the dry years, and the
Speaker 2: other was the average velocity from twenty twenty two to
Speaker 2: twenty twenty four, which was the wet years. So those
Speaker 2: were the average velocities over those two time intervals. You
Speaker 2: can't you can do other types of analysis. That's what
Speaker 2: the full time series is available for other types of estimation.
Speaker 2: I also showed some maps that were the total or
Speaker 2: cumulative displacement.
Speaker 1: Question nineteen is the velocity map still in line of
Speaker 1: site direction or does the script download both directions and
Speaker 1: decompose the vertical element.
Speaker 2: The script the analysis that I showed in the notebook
Speaker 2: is still in the line of site direction. I only
Speaker 2: have it only used one track of the opera displacement products,
Speaker 2: and that's just one line of sight. There's no decomposition.
Speaker 1: Question twenty is what should be the minimum time being
Speaker 1: able to measure surface displacement for groundwater applications?
Speaker 2: Well, that's going to the minimum time interval is going
Speaker 2: to depend on how fast the groundwater displacements are happening
Speaker 2: in a given area. In the Central Valley, the displacements
Speaker 2: can be up to thirty centimeters per year, so you
Speaker 2: can get a good measurement in just a few months.
Speaker 2: Other places, the displacements are much slower, maybe only a
Speaker 2: centimeter a year, and you might need to have two
Speaker 2: or three years of data to get a good estimate
Speaker 2: of what the rates are if the rates are quite slow.
Speaker 1: Question twenty one, why are these why are there positive
Speaker 1: subsidence points?
Speaker 2: Yes, that's quite a surprising effect there in the twenty
Speaker 2: twenty two to twenty twenty four time interval, because this
Speaker 2: was a time interval where the California received a huge
Speaker 2: amount of rainfall. The groundwater actually was recharged and the
Speaker 2: surface rebounded due to the very large amount of rainfall
Speaker 2: during those two years.
Speaker 1: Thank you. Question twenty two. While excluding the ASF portal,
Speaker 1: in my region, I'm seeing localized pockets of subsidence a
Speaker 1: few hundred meters per yards across. Is it reasonable to
Speaker 1: interpret this as subsidence? What sort of factor should be
Speaker 1: wary of for misinterpreting At fine scales.
Speaker 2: The displacement products are indicating that there's some type of
Speaker 2: ground motion. It's probably a subsidence, but it could be
Speaker 2: some other effect like such as landslides moving or in California,
Speaker 2: we have earthquakes also in Nevada and other places. But
Speaker 2: most of the measurements should be useful. Uh, it's it's
Speaker 2: just a measurement of the surface displacement. It doesn't tell
Speaker 2: you necessarily the cause of that surface displacement. So you
Speaker 2: do have to do some interpretation as to what would
Speaker 2: I actually is causing the displacement. In other places, there's
Speaker 2: some displacement where landfills or former landfills that the material
Speaker 2: keeps compacting with time, and you can see that on
Speaker 2: the on the opera products in urban areas where there's
Speaker 2: large landfills that are been they've been covered over with
Speaker 2: because they stopped using them, but the material keeps compacting
Speaker 2: with time. Mhm H.
Speaker 1: It's interesting. Question twenty three. Land displacement can be caused
Speaker 1: by multiple factors such as erosion to be separate them
Speaker 1: from groundwater subsidence in the dispretas.
Speaker 2: Sold land surface modification by erosion or other. You know,
Speaker 2: construction that that changes the land surface in a major
Speaker 2: way will become incoherent in the InSAR measurements and therefore
Speaker 2: it'll it won't have a valid measurement. So the InSAR
Speaker 2: measurements in the opera displacement products are only in places
Speaker 2: where the surface is not being changed significantly over time
Speaker 2: and major erosion. You can't measure erosion directly with insert.
Speaker 1: Thank you. Question twenty four. Could you provide key references
Speaker 1: documentations that could guide us to produce opera land displacement
Speaker 1: or vertical land motion, et cetera output data sets for
Speaker 1: study area located in Africa, for example.
Speaker 2: Yet the main uh opera algorithm is UH. All the
Speaker 2: software is online at gitab. The main there is a
Speaker 2: paper that's coming out shortly on the whole opera algorithm
Speaker 2: and methodology. It's not yet published, so I can't give
Speaker 2: you that link yet.
Speaker 1: Okay. Question twenty five is there a way to enter
Speaker 1: the codinates of my point of interest directly into the
Speaker 1: opera disc search bar?
Speaker 2: The displacement portal doesn't have that capability at this time.
Speaker 1: In NASA Earth Data, you can do that. You can
Speaker 1: just click on a point and then modify the let
Speaker 1: alone exactly the way you like.
Speaker 2: Ah, yes you can. You can. You can search for
Speaker 2: the opera displacement products, but not in the displacement portal.
Speaker 1: Not in the portal, Yes, thank you. Question twenty six,
Speaker 1: how can operate this time series be quantitatively integrated with
Speaker 1: Grace and Chielda's data to improve groundwor the storage estimation
Speaker 1: considering the different special and physical sensitivities.
Speaker 2: This is important question, but it's really beyond the scope
Speaker 2: of this training that you have to consider the whole
Speaker 2: response of the reservoirs in the areas, and the spatial
Speaker 2: resolution is a major effect that requires some computer modeling
Speaker 2: or data assimilation techniques beyond the scope of this training.
Speaker 2: But people have done this work and there's a number
Speaker 2: of papers on combining INSERT and GRACE and grace follow
Speaker 2: on data with insert to get a better estimation of
Speaker 2: what the local variations in the ground order extraction.
Speaker 1: Question twenty seven is, since OPERA disc uses insert radar
Speaker 1: from satellites, does the radar beam actually penetrate underground and
Speaker 1: see the water table directly?
Speaker 2: Now, the radar beam does not see the water table.
Speaker 2: It penetrates into the ground surface at most a few centimeters.
Speaker 1: In twenty eight, when OPERA data is processed, are there
Speaker 1: different reference points for the North America region or is
Speaker 1: there a unique point? Can we know the location of
Speaker 1: such point?
Speaker 2: The Opera displacement products are are not processed to any
Speaker 2: global reference point for all of North America, and that's
Speaker 2: what the for the future vertical land motion product will
Speaker 2: you be So each each track is basically each frame
Speaker 2: has its own local reference system and you need to
Speaker 2: provide your own reference points and when you do your analysis,
Speaker 2: there's no absolute reference point for the Opera displacement products.
Speaker 1: Question twenty nine for insult, what are some best practices
Speaker 1: if studying groundwater related subsidence in a seismically active area,
Speaker 1: in addition to analyzing both ascending and descending data sets.
Speaker 1: Do you have further recommendations.
Speaker 2: Yeah, Well, earthquakes are our fault motions. Gradual fault motions
Speaker 2: are a concern in most cases that the faults are
Speaker 2: are not in the middle of the groundwater basins, but
Speaker 2: in other places there are. There's an additional effect where
Speaker 2: many times the groundwater reservoirs are actually have an edge
Speaker 2: right at the location of a fall, and you may
Speaker 2: see that there's a bigger ground water variation on one side
Speaker 2: of the fault on the other side of the fault.
Speaker 2: It doesn't mean that the fault itself is moving. It
Speaker 2: just means that the aquifer layers in the groundwater are
Speaker 2: of different thickness on the two sides of the fault.
Speaker 2: We've seen. We saw that very clearly in the area
Speaker 2: of what's called the Santa Clara Valley that include San
Speaker 2: Jose in California. There's a few papers on that.
Speaker 1: Question. Thirty is InSAR measures displacement relative to a reference point,
Speaker 1: but no point is truly stable due to tectonic strain.
Speaker 1: And other factors in a basin with both regional tectonics
Speaker 1: and groundwater pumping. What the minimum temporal baseline is needed
Speaker 1: to separate these signals.
Speaker 2: Yes, the the InSAR measurements are are always relative to
Speaker 2: a reference point. In some cases, you may have a
Speaker 2: GPS station or or g n SS station that you
Speaker 2: can use to get the full absolute three dimensional UH
Speaker 2: displacement time series for that point and use that as
Speaker 2: your stable reference for the InSAR. That's a that's an
Speaker 2: effective way to try to separate the two signals. UH
Speaker 2: different signals, but you would have to do some your
Speaker 2: own analysis of the tectonic signal to see how it
Speaker 2: might be affecting the groundwater. Typically they're they're on different
Speaker 2: spatial scales, So just by looking at the spatial resolute,
Speaker 2: the spatial area a special pattern, you can separate different
Speaker 2: effects by using what when you have a local reference point,
Speaker 2: it's basically saying that that local reference point has zero displacement.
Speaker 2: So if there's some kind of you know, large scale
Speaker 2: plate motion, that that plate motion has already been subtracted
Speaker 2: out because you set that you have that local reference point.
Speaker 1: So next question, let's see if it's relevant. What if
Speaker 1: we want to do groundwater temporal changes as one of
Speaker 1: the environmental factor to demonstrate a casual relationship coursal relationship
Speaker 1: to the lake geo hazard, which data set is the
Speaker 1: best available option place as its own limitations.
Speaker 2: I'm not sure what they mean by the lake gudo hazard,
Speaker 2: but typically the in Sorrow or other just InSAR is
Speaker 2: going to give you the higher spatial resolution that you
Speaker 2: can more easily tie to or local effects. The grace
Speaker 2: data is only going to give you a regional scale
Speaker 2: look at what's happening in the given area.
Speaker 1: Question thirty two is if the area of selection is
Speaker 1: bigger than one frame, does that this Jupiter script music
Speaker 1: them and fix the phrase jump in between?
Speaker 2: No, this Jupiter script only works with one frame. In fact,
Speaker 2: you have to make sure that your area of interest
Speaker 2: fits within frame boundary or it'll it'll stop running.
Speaker 1: Thirty three is pont Opera process Canada even by removing
Speaker 1: wintertime data? Is there a limitation in processing six months
Speaker 1: of data every year?
Speaker 2: It was a decision that they made some years ago.
Speaker 2: I don't know the exact reason, but they decided not
Speaker 2: to process the part of Canada out north of more
Speaker 2: than two hundred meters two hundred kilometers from the border.
Speaker 2: That's just what they decided to do, mostly because of
Speaker 2: the snow cover issues. But so there is a snowcover
Speaker 2: issue in Alaska, and when you look at the displacement
Speaker 2: data in Alaska, you'll see that there's large gaps in
Speaker 2: the time series during the winters when there's snow cover.
Speaker 2: It is possible to do that kind of processing, but NASA,
Speaker 2: the NASA funding wasn't sufficient to do that for the
Speaker 2: large area of northern Canada.
Speaker 1: Thank you. Question thirty four. How can OPERA disc data
Speaker 1: be used at the local scale to assess groundwater level
Speaker 1: variations linked to vegetation eveport transpiration, particularly in comparing water
Speaker 1: use between fast growing and slow growing forestry species.
Speaker 2: So the OPERA displacement products are measured with the whatever
Speaker 2: temper resolution is available from the Centinel one data and
Speaker 2: in the future NISER data Sentinel one. As I mentioned earlier,
Speaker 2: some of the time they've had two satellites, in which
Speaker 2: case they in some places they actually acquired data every
Speaker 2: six days, especially over the West coast of the United States,
Speaker 2: but in other places they acquire data only every twelve days.
Speaker 2: And NISAR will also be twelve days. So the temporal
Speaker 2: resolution is determined by the input data, so you're not
Speaker 2: going to see variations at time intervals less than the
Speaker 2: data acquisition.
Speaker 1: Great, we just have time for a couple of more
Speaker 1: questions and then we'll stop. We're almost at the end
Speaker 1: of the time. What's the cause of the positive effect
Speaker 1: artifacting around bodies of water in the ASF.
Speaker 2: Yes, So this is due to the way that they
Speaker 2: calculate the short wave length filtered version of the placements.
Speaker 2: To calculate a short wavelength displacement, you take a window
Speaker 2: it's about twenty five kilometers across, take the average of
Speaker 2: that window and subtract it from the data, and that
Speaker 2: means that the center of the subsidence ball gets still
Speaker 2: has the subsidence, but then the areas next nearby end
Speaker 2: up having an apparent uplift. That's just due to the
Speaker 2: way the filter was calculated.
Speaker 1: Next question, when calculating the linear recurrence velocity of pixels,
Speaker 1: what is the improvement to accuracy of using a polynomial
Speaker 1: fitting instead, At least over smaller area where computation time
Speaker 1: is not a major concern.
Speaker 2: You can use higher order polynomial fitting, but then you
Speaker 2: may be fitting a noise in the data. There is
Speaker 2: a significant noise in each measurement. This can be reduced
Speaker 2: if you do the tropospheric corrections that I mentioned earlier.
Speaker 2: So you don't want to overfit and stay fitting noise
Speaker 2: in the data. That's why we typically use averages over
Speaker 2: at least a few months.
Speaker 1: Yeah. The last question is it is commonly known that
Speaker 1: Mexico City is sinking due to the compression of the
Speaker 1: clay beneath it. In our exercise, this negative lend displacement
Speaker 1: was surrounded by a ring of positive displacement. Why is this?
Speaker 2: Yeah, this is the same thing that I just described.
Speaker 2: It's due to the way the filter was applied. When
Speaker 2: you do the short wave length filter, it shows up
Speaker 2: as positive around the edges the subsidence in the middle.
Speaker 2: If you look at the unfiltered displacements from Mexico City,
Speaker 2: you will see that there is no uplift around the edges.
Speaker 2: It's only subsidence inside the basin.
Speaker 1: Thank you so much, Eric. We thank Doc right Fielding
Speaker 1: for his presentation and answering all the questions today and
Speaker 1: he's sharing his expertise on this subject. So thank you
Speaker 1: all for attending this webinar series. This is the last
Speaker 1: part of this series and we hope to see you
Speaker 1: in our future training, so please stay updated with our
Speaker 1: SAT listener you'll get information about our upcoming trainings. Also,
Speaker 1: please take a few minutes to complete the survey that
Speaker 1: you receive so that we get feedback from you. And
Speaker 1: we want to thank our set team for their help.
Speaker 1: Our coordinator Natasha Johnson Griffin, our editor Maria Marapito and
Speaker 1: other coordinators Roc Plevins, Salvin Hadsondoy, Shry Morris, and our
Speaker 1: editors Jonathan O'Brien and Sarah Corschel. Also want to thank
Speaker 1: our institutional designer Susan Monthy and my colleagues Sean McCartney
Speaker 1: and Erica Potters for everybody's help. And once again, Doctor Fielding,
Speaker 1: we thank you for your help and time with this
Speaker 1: training and it looks like it generated so many questions
Speaker 1: and people are very interested in this topic. So hopefully
Speaker 1: through the exercise and through the jupitter notebook you can
Speaker 1: explore this data and then, as as we told you earlier,
Speaker 1: the homework is you on fifteenth of May, and we
Speaker 1: hope to see you in our future training.
Speaker 2: Thank you all, Thank you, and you're welcome
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