QUESTION01
01-1 Well, I really like it. I hope people use it!
Bruce Chapman, Jet Propulsion Laboratory, bruce.chapman@jpl.nasa.gov
01-2 I love it !!!!!!
01-3 its simply awesome!
victor taylor
01-4 "Two thumbs up, way up..."
Siskel and Ebert, You have new mail.
01-5 I was thinking that it might be nicer if instead of clicking on the number of the question, that the clickable thing was the question itself?
bruce chapman, JPL
01-6 This is the finest site on the web. Especially for a earth imagery freak like me. Thank you, thank you, thank you.
Rob Blomquist, robb@accessone.com
01-7 If this is where technology is taking us, it's great. I only wish I have more time to "surf the net". Faouzi
Faouzi Amar, University of Texas at Arlington, amar@uta.edu
01-8 How about just underlining the word response ?
Tony Freeman, JPL
01-9 There does not seem to be an easy way of thanking somebody for his/her answer other than merely adding an answer and hope that the person you wish to thank will glance at other answers (or obviously, use electronic mail, but that's outside Mosaic or Netscape). Am I wrong ?
Yves Moisan, Universite de Sherbrooke, ymoisan@magellan.geo.usherb.ca
01-10 A modest suggestion for a wonderfully constructed web site: would it be possible to web-ize the 381K document about the scientists and their proposals I. INTRODUCTION i.e., break it up into smaller documents? The navigation is set up just fine, but it is all internal (within this one big file). This will cause memory overload for many users. Thanks -- I really like the level of detail being provided! 1/29/95
01-11 I don't always see a name/address for a question response. Is this because the person was lazy and didn't fill out the id info? How about automatically getting their email address at least? 1/30/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
01-12 in reply to 1-10, I will try to break the mission overview document into smaller sections, so that it does not take so long to load it. in reply to 1-11, yes, it was because the person for whatever reason elected to not say who they were. unfortunately, there is no way to get someones email address automatically. 1/30/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
01-13 also with respect to 1-10, if you want to put a link to a location within the imaging radar home page, be sure to put in the whole path, for instance, introduction is how the above link should read. (don't forget the / as the top directory) 1/30/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
01-14 I found a pretty decent glossary for many of the radar and satellite acronyms at Syracuse University's radar education project. tom pringle/emerald imagery 2/ 1/95
01-15 Actually, what you have put a link to above, is from the Paul Rosen, jpl, par@parsar.jpl.nasa.gov QUESTION09
09-1 The Gatineau receiving station should have a list of orbital elements and insertion times for each phase since launch. I know that the Alaska SAR Facility in Fairbanks has such a list because they gave me a printout last fall to update JPL's EOSMENU ground coverage software. Unfortunately, the list is under piles of paper somewhere on my desk. Give me time to "search" and I can probably help you, otherwise if you need the information soon, contact the Gatineau station, or ASF.
John Crawford, JPL Ocean Sciences, jpc@chukchi.jpl.nasa.gov
QUESTION08
08-1 NASA has asked the Committee on Earth Studies (CES) of the National Research Council Space Studies Board for a scientific assessment of SAR data for Mission to Planet Earth. The CES held its first workshop on this subject in Irvine California from January 9th to 13th. Based on the results of this workshop, they will advise NASA as to the value of a third flight of SIR-C/X-SAR relative to other proposed mission concepts. A decision whether to refly should be made sometime this spring.
Diane Evans, JPL
QUESTION11
11-1 I would like to see a clickable map that would let me zoon in on image files pertaining to my area of interest (Oregon). This would be more convenient than long document lists, some of which are hard to pinpoint from the name alone. With WebMap 1.01, it is easy to convert arbitrary polygonal regions into URL's.
Tom Pringle, Emerald Imagery,
11-2 When I have a chance (sometime in the next month) I will be implementing a clickable map or the world for the picture gallery. At the Eros Data center (go to science and applications, how to get data), there is a clickable map of the world, where you can view the survey data from SIR-C.
bruce chapman, Jet Propulsion Laboratory, bruce.chapman@jpl.nasa.gov
11-3 We have made a few changes to the bulletin board recently. Now, the whole question is clickable. Also, the date of any entry is now listed at the end. The box to click on to submit a question is now also at the top of the page. 1/26/95
bruce chapman, Jet Propulsion Laboratory, bruce.chapman@jpl.nasa.gov
11-4 I would like to see a 3D RADAR image of the Santa Clairita Valey. It would include Valencia,Saugus & Canyon Country. 1/29/95
Henry Armstrong, A.C.C.S. LABS, hca3@smartdocs.com
11-5 We have an image of the LA area that comes down from San Francisco. Some of this image is at the picture gallery, I am not sure if it goes as far north as Santa Clarita . However, I do not think that we have any 3-d data from this area, so unfortunately, at this time I can not put a 3-d image on-line. In order to get 3-d imagery, we currently have to use either airsar/topsar data (which is a NASA/JPL airborne sensor), or by using repeat passes over the same area by SIR-C, J-ERS-1, or ERS-1. This kind of data is not available for a large percentage of the Earth. 1/30/95
bruce chapman, jet propulsion laboratory, bruce.chapman@jpl.nasa.gov
11-6 is there a way for me to find out if a new response has come in since i last looked at a question/response? the best would be if netscape would "un-red" the question in the main list if a new response came in... thanks 2/ 2/95
Tom Farr, JPL
11-7 Reponse to 11-6: We are thinking of adding the date of the last response after the number of responses in the BB. Forcing netscape (or any other browser) to "un-red" a hotlink based on a users local BB history file (that would need to be created) is a bit more complicated than we want to get into at this time. 2/13/95
Sharon Okonek, JPL, sharon.okonek@jpl.nasa.gov
11-8 This is an 'issue' for me too. Basically, we have a sorted database with three fields: questions, responses, and date submitted. Using standard html form yoga and a modest cgi script, responses could be compiled automatically as a database sorted by date and linked to the appropriate question. Then, responses not previously seen by particular individuals would show as blue and likely clustered near the top. It might be fun to see a response and guess what the question was!

This would be groundbreaking work but well worth it -- Ric Ford of MacWeek has been looking at this home page on and off with a view to featuring it in a future column. 2/18/95

tom@emerald
QUESTION03
03-1 This "Submit a Response" box is pretty. I'd rather it scrolled down like a notepad weird on my Mac. It just goes and goes to the right and I can't see what I just wrote.
Tom Pringle, Emerald Imagery, tingalsb@oregon.uoregon.edu
03-2 Unfortunately, that is a property of the forms. 1/26/95
bruce chapman, Jet Propulsion Laboratory, bruce.chapman@jpl.nasa.gov
03-3 Solution A: Stub in the following html code to JPL home page after

Enter your question or comment in this box: Solution B: Mac Netscape users can View>Source... to open Simple Text, start writing at bottom, then paste into comment box. 1/27/95

anonymous
03-4 In 03-3, the stub-in code got taken too literally as html, not text. Intended change just sets columns to 110, which makes text box appropriate for an average screen and drops it to its own line. The larger box is easier to work in. 1/27/95
anonymous
03-5 I think this is what was meant above: I took the liberty of editing this out, as I found it confusing. basically, this person put in a response box of 110 columns. We have changed the size of the response box to 80 characters (bc)
03-6 It might be nice to have a cancel or edit option at the point where the user sees how a given question or response is going to look. Here's an easy workaround (surf your own hard drive): view the current page as source. This opens the SimpleText editor. Select All and Cut. This gives a blank slate. Write out the question or response. Save As anything.html to the desktop. Back in Netscape, Open File and double click on your new .html document. View the document just as it will appear on the JPL home page. Save changes as needed. Copy and paste into the 'Submit Comments box and submit! 2/ 1/95
03-7 I changed the width of the text area from 60 to 80 chars. Hope this helps. 2/ 2/95
Sharon Okonek, JPL, sharon.okonek@jpl.nasa.gov
QUESTION10
10-1 The SIR-C Project has created an Educational CD-ROM called the SIR-CED. This CD contains radar images and tutorials that allow students to learn about the uses of radar. There is a detailed write up on the CD-ROM on the "radar remote sensing education" section of the Imaging Radar Home Page. This section describes the CD-ROM and gives information regarding ordering copies for use in the classroom. Also mentioned in this section is the type of computer equipment needed to display the images from the CD. 1/26/95
Shannon L. McConnell, SIR-C Project
10-2 I have been using the SIR-CED disk since this last summer with high school students and I have developed a unit around the Pennsylvannia image. The week-long computer lab exploration uses the Radar Image and Landsat and digital photographs to show students the problems of Coal Mining and the problem of Acid Mine Waste. Write me for details- BOX 163 Lincoln, VA 22078 (PS Once I'm comfortable on the net I will link and have e-mail) 3/ 8/95
William M. Seebeck , Chantilly High School, Fairfax County Schools,VA, none yet
QUESTION13
13-1 Eventually all SIR-C data will be made available through the EROS Data Center in Sioux Falls, SD. It's going to take a while before the interferometric data (which was acquired experimentally) is released. We (JPL) have an airborne interferometric SAR system which is now operational called TOPSAR. It can generate high resolution topo-data over areas of ~10x10km. Some limited amounts of TOPSAR data have been released. For further info on TOPSAR or TOPSAR data send an e-mail to: radar.queries@jpl.nasa.gov 1/26/95
Tony Freeman, JPL
QUESTION04
04-1 I think this is a really good idea. There are a zillion directions to go off in for 5-channel enhancements -- it would be fun to see what others can come up with since nobody has time to explore them all. To be helpful, enhancement goals, software used, and enhancement steps taken need to be articulated and perhaps edited for consistency. I propose that JPL create a contest (with prizes of course) to see who is the most inventive and skillful at extracting information or making an educational point from radar imaging data. This would consist of posting, say, all channels of some scene at 200K x 5 = 1 meg, setting an enhancement objective, a time frame, a panel of judges, and incentives (CD-ROMs of radar data?). Many of us could productively waste time on this at work because our screens would look okay. 1/28/95
Tom Pringle, Emerald Imagery, tingalsb@oregon.uroegon.edu
04-2 I think this is a great Idea! I spoke with Tony Freeman about it and he agreed. We will try to put a contest like this together. I will be a bit busy for a couple of weeks on other things, but I will try to organize something by the end of March. By the way, we actually have 13 channels of data when we collect all channels (X-band 1 channel, L-band 4 channels, C-band 4 channels) so we will put all of them on-line, and then let the users have their hand at making some nice looking images! I will announce it at whats new, and at the bulletin board. 1/30/95
bruce chapman, Jet Propulsion Laboratory, bruce.chapman@jpl.nasa.gov
04-3 correction (see question 20) . I will put 7 channels of data on-line. (maybe only 6 if I can not get the corresponding x-band data.) 2/ 1/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
04-4 I think the grand prize should be a ride on the Shuttle (provided the winner has the 'right stuff.') Or at least on the TOPSAR DC-8. Not just some CD-ROM. 2/ 1/95
QUESTION15
15-1 Yes, this works. Sort of. JPL has set up the whole nine yards to be underlined so it is hard to tell that the Eros link does work in the original question. While it is not my place to offer design changes to JPL's most excellent home page, bulletin board users who want to see a little less underling in their question could submit it so that only the first word is the link to the responces. From question 15, viewed as source, it is clear that inserting a terminator (/A, sandwiched by 'less than' and 'greater than' symbols) where the underlining should stop is enough. Then the links within their question would show up better. Note that this is only necessary in submitted questions; in submitted responses where links would be more common, they show up fine. 1/28/95
15-2 We really like this idea of putting in links within the questions. We will probably change the format so that the whole question is not underlined, so that it is more clear where a link is... 1/30/95
bruce chapman, Jet propulsion laboratory, bruce.chapman@jpl.nasa.gov
15-3 as shown in the response to question 1-10, if you put in a link to something within the imaging radar home page, don't forget that you have to specify the path, including the top "/", or it won't link correctly. If it is a link outside of the imaging radar home page, then you don't have to worry about that. 1/30/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
15-4 I would like to inclose small graphics as well as links in my responses . However, "Submit a Response" does not seem to accept pasted graphics. Can JPL give us a stable directory path to a folder where we might ftp our images with Fetch, then cite in question or response links? Or would you rather we did these links to our own home pages?

I see where someone has done an end run around the name-affiliation-email paperwork by creating a single paste 'send mail' trigger link in question 22. Can you set things up so all email addresses are provided like this automatically? 2/ 1/95

15-5 Well, I'm not sure. I am not sure if the link in 22 was manually input. It might only be a netscape feature. It may be possible if the netscape software can handle it... 2/ 1/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
15-6 So far as linking in graphics at the bulletin board, this is certainly an interesting idea... 2/ 1/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
15-7 After talking it over, we have decided not to enable linking small graphics into the bulletin board with the img src html command, as then we start having to worry about the amount of disk space that we would have to allocate for this (once it is in a question, we have to keep the image as long as we keep the message). And then there is the problem of inappropriate images. As it is, you can put a link to an image, you just have to click. If you have an image that you would like everyone to see, then send me an email, and we can possibly put it into the
user contribution section for everyone to see. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
15-8 How do you feel about bb users submitting html tables? Like with images, , File sizes stay small with tables; as with images, poor judgement might be exhibited. tom @ emerald

Imaging Radars
AIRSAR SIR-C
SIR-B X-SAR

3/26/95
QUESTION14
14-1 Tom, a very interesting problem. I wonder if the ion-rich river water would be too much of a conductor to allow radar depth mapping, though it should pick up sandbars and shoals. At $500M a pop for shuttle flight, that's going to make a pretty expensive load of soyburgers by the time it gets out here to Oregon. First tell us why an ordinary color Walmart camcorder flown down the river weekly in the belly of the company plane doesn't make something that the captain can look ahead with on his VCR. Your response is probably, this works fine, but it's not high tech enough for us at Marine Equipment plus it doesn't show enough river depth. Okay, here's what you do. Run the video frame-by-frame through an enhancement cycle in Adobe Photoshop, then do a PCA analysis in DIMPLE, under-tinting a supervised classification to draw out the features, and over-vectoring with river charts and DEM GIS data. Dollars will get you donuts that the best channel will pop right out in vivid color. Now drive the VCR frame-by-frame with your GPS satellite downlink to barge river position, so the captain only sees the next mile or two. Or better yet, set the barge up as a Web site, pilot it remotely with a clickable map, and forget the video. 1/28/95
14-2 Interesting problem and response #1 is a neat partial solution. It is true that the radar waves will not penetrate significantly into the water, while short visible wavelengths, like blue and green, will. Silt, etc. in the water would limit this unpredictably, though. 1/30/95
Tom Farr, Jet Propulsion Lab, tom.farr@jpl.nasa.gov
14-3 Fellas, that was a pretty "slick" solution. As far as "high tech" goes, the cam-corder option is cute, but no cigar. Not that it isn't high tech enuf either. Seems like you boys and your tax-payer paid for toys have no real inderstanding of how to apply this technology in the real world where there is a budget you have to meet. I have NEVER run the video through "an enhancement cycle", probably a spin cycle, BUT I WOULD NEVER BE CAUGHT DEAD IN AN ENHANCEMENT CYCLE. Most body shops would NEVER under-tint either. And if you continue to use language like PCA, DIMPLE and DEM GIS, I will have to report you. 1/30/95
14-4 unfortunately, some of the responses to this question were accidentally deleted. 2/ 2/95
bruce chapman
14-5 One deleted response suggested (1) using a blue filter and panchromatic film on auto-exposure cameras, so as not to waste emulsion grains on non-penetrating wavelengths, (2) sizing sediment particles and measuring adsorption with a spectrophotometer, so as to rationally find a penetration window, (3) having idled Navy anti-submarine planes tow sonar devices, reconstructing empty river from cross sections. Barge people needed water depth beyond 9' provided by Coast Guard. 2/ 6/95
QUESTION20
20-1 This is one of the areas that responses were accidentally deleted. I will just restate here that there are really just 9 channels that are recorded by sirc/X-SAR. Each quad pol frequency takes 10 bytes per pixel (see the decompression software manual for more details). Also, H and V just refer to the transmit and receive polarization of each channel. 2/ 2/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
20-2 To amplify Bruce's response for those too lazy to read the manual- the two sir-c bands (L and C) and the 3 AIRSAR bands are often collected in a "polarimetric" mode. This is done by transmitting H and V and receiving all four of the possible combinations (HH, VV, HV, VH), sometimes called "quad-pol". A few years ago, we realized that if we carefully recorded the phase as well as the more traditional amplitude of the returned waves, we could combine the four linear polarizations into any other polarization: eg. linear at 45 deg., circular, elliptical, etc. The term we coined was "polarimetry". We also came up with a way to compress all this information into a minimal number (10) of bytes per pixel. Thus, one needs special decompression software to view the compressed polarimetric data. Not all SIR-C data are polarimetric- it depends on the mode. Finally, X-SAR data are only VV polarization, although they are distributed as 16-bits per pixel to maximize dynamic range. They can be scaled to bytes for viewing, which Bruce has done for the various images on the home page. 2/ 2/95
Tom Farr, JPL
20-3 I recall that the deleted response to Question 20 stated that SIR-C/XSAR basically had 7 channels (not 9) because of setting HV=VH, thus LHH, LHV=LVH, LVV; CHH, CHV=CVH, CVV; XVV. These channels require 22 bytes per pixel (10 each for L and C coherence matrices plus 2 for X) in the 9 channel perspective, but seemingly only 8 + 8 + 2 = 18 bytes if reduced (bytes having real and imaginary parts.

The deleted response also discussed a mix-up with the AIRSAR data, stating it had 13 channels. AIRSAR collected polarization data for P, L, C bands and had no XSAR. Thus, it seems there should be 9 or 12 channels, depending on whether JPL set PVH=PHV, LHV=LVH, and CHV=CVH. Here there should be 30 bytes per pixel of data (10 each for the Stokes matrices) in 12 channel mode but seemingly only 24 if reduced.

2/ 5/95

20-4

The fact of the matter is, any elliptical polarization state can be represented by linear combinations of left and right circular polarizations, these in turn being expandable as superpositions of orthogonal plane polarizations. Are we not back to square one? Would researchers using radar data be likely to have a priori motivation to view any particular elliptical polarization? If isotropy is found during image enhancement, at that point, it might be physically instructive to back-synthesize the polarization that optimally gives rise to the effect. 2/ 5/95

20-5 I don't understand why scaling would be used for data reduction from 16-bits to 8-bits. Uniform compression generally severely and unnecessarily truncates the image. Better to adaptively compress, taking instruction from the histogram, compressing where the data is sparsest, that is, non-uniformly strech the contrast. The following operatations don't commute : 8-bit gsRGB to 4-bit index to contrast stretch versus 8-bit gsRGB to contrast stretch to 4-bit indexed. The first histogram is badly "combed out." 2/ 5/95
20-6 Is not JPL is exhibiting a little of the 'not invented here syndrome'? Polarimetry was invented a century ago; devices to measure components (including chirality) experimentally are described in late ninteenth century optics texts. Radio astronomers have been taking phase measurements for decades in their synthetic aperature radars, while infra-red astronomers like Kemp have been using polarized emitters (white dwarfs) and crossed crystal detectors since 1969. These are both remote sensing endeavors. I see where JPL (Radio Science 29#6, pp.1409-1420, Dec 1994) also 'discovered' that Maxwell's equations are invariant under improper Lorentz transformations (a result published in 1896)! What's next -- JPL taking credit for discovering abelian gauge theories? 2/ 5/95
20-7 Just to further clarify 20-3, the radar instrument for sirc collects HH, HV,VH, and VV data. Prior to processing that data into images, we have stored 4 channels of data per frequency. When we process the data into images, we can store the data into two different formats : SLC (single look complex) or MLC (multi-look complex). The SLC data stores the 4 channels of complex data, but compresses the 4 complex values per pixel to just 10 bytes. The MLC data is averaged down, calibrated, HV=VH, and converts the data to a common map projection, in addition to being compressed to 10 nytes per pixel. The format that the data is stored is determined by the investigator, but most investigators prefer MLC because the files are smaller, the data is calibrated and converted to an easy map projection, and because it still has the phase information between the polarization channels that permits polarization synthesis. It can't, however, be used for interferometry, because the absolute phase for each channel is lost. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
20-8 in answer to question 20-6, please remember that jpl is a big place (5,000 engineers and scientists), and that "JPL" does not really do anything, it is the individuals here taking the initiative to study various problems that do the work. Obviously, no one here can take the credit for inventing polarimetry. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION19
19-1 response is missing 2/ 2/95
bruce chapman
19-2 Here's an off-the-wall idea on how to bring the XSAR date up to snuff so that the SIR-C/XSAR data set better resembles AIRSAR. There could be many benefits to this in software and data processing simplicity. XSAR only collected XVV amplitude, not XHH nor phase. Idea zero is to set XHH = XVV. Idea one is to assign every pixel a constant phase of zero. Idea two is to assign instead a random phase, with the thought that this will wash out during statistical processing. Now the X band data mimics the others in a way that does no real damage post-processing. Garbage initially but tape is cheap. 2/ 5/95
19-3 The latest version of the sir-C/airsar conversion software now converts x-SAR data to sirc "MLD" format data. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
19-4 Actually, I as looking at my code, and I do not know what the conversion is for xsar data from unsigned integers to sigma0 - does anyone out there know how to get sigma0 from the unsigned integer values? 2/10/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION17
17-1 the responses to this question were accidentally deleted. We are planning on upgrading the Macsigma0 software, and are encouraging software developers to incorporate the sirc data formats into their software packages. 2/ 2/95
bruce chapman
QUESTION16
16-1 The responses to this question were accidentally deleted. IDL is a commercial software package from Research systems, inc. We will be having a link to their home page soon (when it becomes available). 2/ 2/95
bruce chapman
16-2 Research Systems has used written a fairly comprehensive image-processing application called ENVI in IDL. It has the similar capabilities for AIRSAR (with upgrades promised for SIR-C) that JPL theoretically offered in MacSigma0, including local Lee standard deviation convolution filtering, ability to read Stokes matrices, synthesize polarizations, and display polarization signatures. You can get this for a Power Mac in a bizarre Unix interface for only $4,475 (June 30, 1994 price). Or you could implement the radar part alone in Mathematica ($178 ed) in a couple of hours...... tom pringle/emerald imagery 2/ 5/95
16-3 Observe that MacMultiView 5.1 costs $668 from JPL/NASA (at Cosmic) and only runs on System 6. MacSigma0, according due a deleted response, will adsorb the functionality of MMV 5.1 in a version due out summer of 1995. It currently costs $234 from JPL/NASA (at Cosmic). We already bought this software once with taxes -- now here's an opportunity to buy it again! 2/ 5/95
16-4 the upgraded Macsigma0 will be on the post-flight sir-c education cd-rom. You will not have to buy it again. 2/ 6/95
16-5 Research Systems is a good source. I have a copy of IDL downloaded off the net and compiled on a SUN. Now I use ENVI running on Xterm from my PC to load, view and process the data. Give them a call or send a note: (303) 786-9900 or maybe : bill@rsinc.com 2/14/95
16-6 Hi, Bill. I am new to this area. I am an environemtal engineer. Radar image can be veruseful for environmental assessemnt. I have download a image file (105k) using Zmodern Binary. My question now is what software I should use to open the binary file. My Email Address is Zhang@FreeNet.Calgary.ab.ca. (Tel:403-299-4625) Thank you! 3/ 1/95
Allan Zhang, Golder Associates Ltd, Zhang@FreeNet.Calgary.ab.ca
QUESTION12
12-1 the responses to this question were accidentally deleted. what I stated before, was that at 25 meter resolution, we would have about 200 billion pixels of the land mass of the Earth. if SIR-C imaged the entire Earth, the data volume would be between 0.2 to 4 Terabytes. This is not an inconceivable amount of data, and in fact, we have imaged 99% of the surface of Venus with radar, which has a larger land mass area than Earth. See the Magellan data at this home page. 2/ 2/95
bruce chapman
QUESTION18
18-1 The best place to start looking is at the Planetary Data System. Try: http://stardust.jpl.nasa.gov/pds_home.html There are links to many other sources of data. Viking did not use radar to map mars, however there have been some low-resolution maps made using earth-bound radars. 2/ 2/95
Tom Farr, JPL
18-2 There is a Mars Atlas that was done based on Viking data. It's a NASA publication. I don't have the SP number handy but I'm sure you can look it up in any list of NASA publications. 2/ 6/95
Jay Trimble, JPL, jtrimble@jpljpt.jpl.nasa.gov
18-3 There is a www site with an on-line atlas of Mars obtained from the Viking orbiters. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
18-4 You might want to check out the VistaPro CDROM. IT has the complete DEM data set for Mars and a great landscape rendering program. For both Mac and Windows. You can buy it from Educorp in San Diego. Contact me for for more information. 303-258-3779 3/27/95
James Perdue, Rocky Mtn Digital Peeks, rmdp@csn.org
QUESTION25
25-1 As I discuss in a response to question 20, for quad pol data we can save the processed images in two different formats: single look complex (SLC) or multilook complex (MLC). The SLC data saves the four complex values per pixel that define the scattering matrix, and is compressed to 10 bytes per pixel. with this data, all four received channels of data are stored. With MLC data, cross-products of the symmetrized stokes matrix are saved. The symmetrized stokes matrix has HV=VH. Also, the data is converted to what we call the "ground range" projection, which is just a map projection on the ground. the SLC data is in the natural "Slant range" projection, which is a projection that is caused by the manner that the radar operates, and is somewhat peculiar. Also, the MLC data is averaged (multilooked) so that each pixel is either 12.5 or 25 meter spacing. This reduces the file size. The MLC data preserves the phase between the polarization channels, and so polarization synthesis is possible (i.e. can synthesize ANY polarization, like right circular). MLC data can not be used for interferometry, as the absolute phase is lost, so in that case, SLC data is required. The data format for any given image is requested by the investigator that has requested the data processing. 2/ 6/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
25-2 Just a further comment : you might want to look at a description of the data formats where I talk about some of this more completely. 2/ 7/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION22
22-1 without a solid surface to reflect radar waves, it would be difficult to interpret the data. You would need to have a high power transmitter, even if it was orbiting jupiter. I am not aware of any attempts to detect Jupiter from ground based radar antennas, but I would not be surprised if someone had attempted it 2/ 6/95
22-2 I believe he is asking about the dielectric constant of the Jovian atmosphere as a function of depth. Radar penetration, based on the 9000 watt Shuttle instrument, seems nil by the time the dielecric constant reaches 3 or 4., which is why water at 87 isn't seen at depth. I would not be surprised if detailed models of Jupiter exist, along the lines of model stellar atmospheres, because there was a lot of interest once in how close Jupiter came to being a binary companion of the sun. Thus, the interpretation of radar data is its comparison to reflectance predicted by the model. The tricky part is how to refine the model if it doesn't agree with the data.. Interferometric data could conceivably be used to probe the depth of turbulent structures. While isotropy is present, It seems that polarized radar is at too long a wavelength to detect it. 2/18/95
22-3 Some of the earliest planetary radar astronomy work was ground based and signals were bounced off the planets. I have not checked the literature, but I know that Venus was probed this way early on, so maybe someone studied Jupiter. try look at the older radar astronomy literature. Also, due to the nature and chemical composition of the Jovian atmosphere, the penetration in to the atmosphere may be very frequency dependent due to absorption by various molecular species. More fun! 3/ 9/95
Sam Gasster, Then Aerospace Corporation, gasster@aero.org
QUESTION26
26-1 The Science team members and their activities are listed here. This document will indicate what the members of the science team are studying. In addition, you can respond to our outreach program, and we will try to either process data for you, or send you data that has already been processed. There is a picture of ubar from SRL-1. Eventually, all the precision data products will be available at the Eros data center, but the procedures for that are still being worked out. Also, it will take us years to process all the data from the two missions. However, most of the data from flight one is now available at the Eros data center, there is a link to that location here 2/ 7/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION27
27-1 There is not yet an AIRSAR home page, but soon there will be. I will be sure to announce it when it is on-line, and to put links to it. 2/ 9/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION28
28-1 I assume that you have gotten the data from the Eros data center, and have downloaded on of the .IMG image segments. This file is what photoshop would call in the "raw" format. So, open photoshop, pull down the file menu, select "open as", change the file format to "raw", enter the name of the file. The next window will ask about the dimensions of the file : enter the height and width of the image (this is given at the page that you retrieved the .IMG file. It will be 2000 in width, as all of the segments are 2000 in width.) There is no header in this file. photoshop should then be able to open the file and display it. write back if this does not work... 2/ 9/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
28-2 In Photoshop, after Open, click show all files. Locate .img file and double click. There is no need to enter width and height -- Photoshop knows these already. This is a grayscale so there are no issues with band interleaving.

For NIH-Image 1.57 freeware , select Import rather than Open. Choose Custom and edit to width and height (e.g., 2000 x 1266) and the file will open. tom@emerald 2/19/95

QUESTION32
32-1 1 - we currently have the SIR-C/X-SAR science team members listed, with their research interests and addresses, but we have not had time to add more than that yet...

2 - Because the Sample data sets are so large, it is not very feasible at this time to put the data on-line.

3 - We have put a SAR reference list on-line, though it is admittedly not complete, it is the best that we have right now.

2/15/95

bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
32-2 Nice job on expanding the SAR reference list -- last time I looked it only had one entry! I wonder if some of the key papers could be put online, or at least the abstracts, or links if the journals are ftp sites -- one hopes that some of the papers are still around, electronically speaking, and wouldn't have to be OCRd in. I'm at a large research university and frankly, no one has ever heard of some of these journals. 3/19/95
QUESTION31
31-1 The captions to the images at the jplinfo site unfortunately do not include datatake id and segment number. However, if you wish to request a precision data product from areas corresponding to these images, just indicate the lat/lon, and that it is an area shown in an image at the jplinfo site, and we will look up the rest. 2/15/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION34
34-1 You might want to look at the response to question 8. There, Diane Evans replies to this question. The SIR-C Survey data is already on CD-ROM, for information, click here. In a few months, we should be distributing the SIR-C post flight education CD-ROM. This cd-rom will have some images from sirc. There is currently no plans to distribute other images or data by cd-rom, though some commercial companies have expressed an interest in some. I will let everyone know here at the imaging radar home page. 2/16/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
34-2 Since Diane's response, there has been a lot of activity involved in definition of what a third flight of SIR-C/X-SAR could do. One of the options being explored is to add a boom about 30 m long with a C-band and maybe an X-band antenna on it. This would allow single-pass interferometry to be accomplished which could be used to produce a digital topographic map of the entire earth (between 60 deg N and S latitudes) at about 80 m horizontal resolution. As Diane said, decisions will be made in the next month or two whether this will be pursued. 2/17/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
34-3 In one month I will publish a CD-ROM called "Earth Exploratorium". It contains 12000 visual images for SRL-1 and over 40 SIR-C/X-SAR images in a very unique navigational interface with lots of search capabilities. For more info, send e-mail to rmdp@csn.org. Newt Perdue, Rocky Mountain Digital Peeks 303-258-3779, only $39. 3/27/95
QUESTION33
33-1 You're not very specific on your "project", but Lidars have mostly been used as altimeters (see refs below). also, there was some work a while back on looking at the reflectance and fluorescence of the ground with a CO2 laser. sorry, i don't have the refs for that handy. Bufton, J.L., J.B. Garvin, J.F. Cavanaugh, L. Ramos-Izquierdo, T. Clem, W.B. Krabill, 1991, Airborne LIDAR for profiling of surface topography, Optical Eng., v. 30, p. 72-78. Harding, D.J., J.L. Bufton, J.J. Frawley, 1994a, Laser altimetry of terrestrial topography: Vertical accuracy as a function of surface slope, roughness, and cloud cover, in press, IEEE Trans. Geosci. Rem. Sens. 2/17/95
Tom Farr, JPL
QUESTION36
36-1 Put in a link to current versions of Netscape and Mosaic. I don't see a further need to support obsolete browsers. 2/18/95
36-2 You should be able to configure the font selection of your browser yourself. The fixed (a.k.a. monospaced) font is the one you'd want to change. Look under Preferences... If it's not there, then there's nothing you can do except get a newer browser (I'm pretty sure recent Mac Mosaics support font selection...) 3/21/95
QUESTION37
37-1 Would this not require platform-dependent compressions of each file to get beyond .gif? 2/18/95
37-2 Most of the images are smaller than 400K. I try to keep the images as small as possible and still retain their information content. 2/20/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION38
38-1

There are two options that readily come to mind using JPL developed software (some commercial software companies now have software to read AIRSAR format data).

1. get the sir-c data decompression and conversion software. the conversion software can convert the AIRSAR data to sirc format, and then the decompression software can synthesize any polarization.

2. There is a program called Macsigma0 that can read and display and allows simple analysis of AIRSAR data. We will be coming out with a new version of this software soon also. I will keep visitors to the imaging radar home page updated as to the status of this.

2/21/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION35
35-1 the .IMG survey image files are just raw byte image files. In this case, the .IMG does not refer to ERDAS' Imagine image format, which also has a .IMG extension. Most any image processing program can read the survey images as raw bytes, using the dimension information associated with the survey product. 2/21/95
Tom Farr, tom.farr@jpl.nasa.gov
35-2 If you are working with ERDAS-IMAGINE software you can import this king of format in the import-expot option using the "generic bynary data" option. You only need to know the number of lines, samples and header bytes, and you can know all this information from the header of your images. 3/25/95
Alvaro Marquez, Complutense University, Madrid, Spain, anguita@eucmvx.sim.ucm.es
QUESTION39
39-1 Good idea! We've been thinking about doing that and will get such a list posted sometime this week. The list will contain the DT number, site name, scene center GMT and scene center latitude and longitude, along with some other information. This list can be used in conjunction with the posted survey data to get a "preview" of the precision processed scene. Keep your eyes out for this posting! 2/27/95
ellen o'leary, jpl, ellen.oleary@jpl.nasa.gov
QUESTION40
40-1

I got the following information from the EROS Data center SIR-C survey image home page at this location:

IMDISP: This software is a general-purpose image display program. It supports EGA, VGA and numerous super-VGA display boards. This program is available and free to have a copy. For further information, contact Mike Martin at (818)306- 6038 (JPLDPS::MMA.RTIN on SPAN)

I think his email address is mmartin@jplpds.jpl.nasa.gov

Maybe someone else knows where to get this software on-line?

3/ 2/95
Bruce Chapman, jpl, bruce.chapman@jpl.nasa.gov
40-2 I just recently discovered that this program for PC type computers is on the pre-flight SIR-C education CD-ROM 3/14/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
QUESTION41
41-1 You must use ftp, not telnet, to kahn in order to get the raven s/w. Then login as guest and enter the password. Next, cd over to pub/raven. Note, RAVEN for IDL 3.6 will be available this week. 3/ 6/95
Sharon Okonek, JPL, sharon.okonek@jpl.nasa.gov
41-2 In addition to response 41-1, I should mention that in order to obtain RAVEN and any other SIR-C software, you must join our Outreach program. This will involve signing a license agreement (amongst some other things). For more info, go to the outreach info page available through the JPL Imaging Radar Home Page. 3/ 6/95
Sharon Okonek, JPL
41-3 Ellen O'Leary's exact email address is Ellen.F.O'Leary@ccmail.jpl.nasa.gov JPL has an X.500 Information Service where you can look up the address of JPL employees and contractors. To querry this database, finger employee-name@jpl.nasa.gov. Since Ellen is the only O'Leary on lab, you could also send email to the infoserver address, where it would be forwarded to the proper location. In this case, you could send email to oleary@jpl.nasa.gov. 3/13/95
Tim Fogarty, JPL, fogarty@sir-c.jpl.nasa.gov
QUESTION43
43-1 first response. see if it works. 3/ 6/95
sharon , jpl, sharon@jpl
43-2 Second response. 3/ 6/95
43-3 Terminal Doppler Weather Radar: TDWR
All of these have TDWR data:

Aviation Weather Development Lab
oratory (AWDL) was established by the Federal Aviation Administration (FAA) to support weather projects in the evolving U.S. National Airspace System. Vast amounts of data from new weather sensing systems such as Next Generation Weather Radars ...
--- [760] http://http.rap.ucar.edu/awdl.html (7K)

Stormscale Research and Applications Division (SRAD)
Mike Eilts, Manager (405) 366-0414 . Personnel as of 4 October 1994-- . Mike Eilts, Manager (405) 366-0414 . Kelly Lynn, Secretary (405) 366-0402 . Susan Cobb, Graphics Consultant . Subdivision information: . Scientific Advisory Panel ...
--- [651] http://www.nssl.uoknor.edu/srad/srad.html (3K)

MIT Radar Data Archive
This document describes the field programs in which the MIT radars have participated over the last twenty years. . Contents: . Introduction . Field Program Objectives . Storage Media . Radar Platforms . Processing and Software . ...
--- [646] http://graupel.mit.edu/Inventory.html (39K)

NSSL/SWAT Home Page
SWAT . Mission Statement . The mission of the Severe Weather Warning Applications and Technology Transfer (SWAT) team is to develop severe weather warning applications and transfer them to users to enhance their capability to warn of severe ...
--- [630] http://www.nssl.uoknor.edu/srad/swat.html (3K)

Gallery: Gust fronts et als.
Gust fronts, thin lines, microbursts, sea breezes (updated 10/27/94) . A gust front in New Mexico: reflectivity and velocity (44K, 54K) . A crisp, clear gust front from a distant (off scope) MCS to the east topped the Sandia Mountains and at --- [625] look here too

Other Weather Radar Web Sites
Other interesting Web Pages on Weather Radar: . The University of Wisconsin puts out a US IR/Radar Composite image (usually ~ 32K) and movie (usually ~850K). A higher resolution image may be found at NASA/MSFC. You can also find current refs at --- MIT


brought to you by tom @ emerald

3/29/95

43-4
For ASR9:

MIT Radar Data Archive
This document describes the field programs in which the MIT radars have participated over the last twenty years. . Contents: . Introduction . Field Program Objectives . Storage Media . Radar Platforms . Processing and Software . ...
--- [767] http://graupel.mit.edu/Inventory.html (39K)

3/29/95
QUESTION44
44-1 i'd like these too! In the interim, what might we expect from these if they were all done, in terms of ground resolution (=file size) and current coverage? 3/ 9/95
tom@emerald
44-2 I have put a couple of data sets from our airborne TOPSAR instrument online. This is a 2-antenna system that produces 10 m or 20 m pixels with about 1 m height error. In addition, a C-band VV polarization image is produced and the new processor also outputs an incidence angle map and an image representing correlation, related to error. The data come in strips about 15 km wide by a few 10s of km long. Newer data have ascii headers giving all sorts of information about the file. Older data have a terse header file associated with the data files. To get the data, anonymous ftp to fringe.jpl.nasa.gov and look in the topsar area. I hope to have more data sets and more documentation by this summer. 3/10/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
44-3 Thanks, Tom, this worked fine. I was able to log on easily as described and open both the impressive grayscale Death Valley allulvial fan CVV image (the file called dv_fans164cvv) and the digital elevation model (called dv_fans_164demi2), on the Mac using Adobe Photoshop, setting raw format at 640 x 2842 pixel width x height for both. On the DEM, since it is 16 bits per pixel, raw format should be set for two channels, with interleaved checked. This gives a Photoshop multichannel document, with channel 1 needing a double tweak with 'Levels' and channel 2 having finer detail. 3/15/95
tom pringle, emerald imagery, tingalsb@oregon.uoregon.edu
44-4 The DEM format raises some unfamiliar issues for the folks out there, namely how to display all of it. The precision of the topographic data necessitated more that the usual 8 bits (0 to 255 after rescaling): 11 bits were needed in the Death Valley scene. Computer hardware is such that two bytes (16 bits) were needed to contain the 11 bits of data dynamic range (0 to 2048). JPL, at the anonymous ftp fringe.jpl.nasa.gov site, essentially put the leading 3 digits in one byte and the trailing 8 digits in the second byte. This downloads as a Word text document with the two bytes together as one number, but opens in imaging programs as a two separate channels, the leading digits being in channel 1.

There is some potential for real confusion here for people used to 24-bit color monitors. It seems like 24 bits is more than enough to hold 11 bits. However, that 24 = 3 x 8, and no single 8 is large enough to display 11, i.e., the separate RGB screen phosphors are only set to display 256 levels each.

Of course, rounding off to the leading 8 digits and displaying as a grayscale 'byte image' is one possiblility. This is a waste of good data -- why send the instrumentation up there and not make use of it? Another option few people will exercise is staring at the array of 640 x 2842 numbers in Word. For other purposes, such as computing slopes or aspects from the DEM, one could do the calculations on the 11-bit numbers in a spreadsheet, then round off to 8 bits after finishing, obtaining some value in enhanced accuracy from the extra bits.

Let's not despair. Here's a easy way (but not necessarily the ultimate way) to display all 11 bits at once using color to supplement the limitations of 8 bit channels. Procede as in 44-3. Then, in the Channels palette, duplicate the trailing bit channel, split, and merge as L.a.b., with leading bits in channel a. This gives a knock-your-socks-off color image explicitly displaying the full resolution of the data, with color trends indicating the broader contour intervals of the leading bits.

I will try to put a small piece of the resulting image into the Lost and Found folder at the ftp site; otherwise, email it to Bruce for inclusion on the home page at his discretion.

tom pringle emerald imagery email:tingalsb@oregon.uoregon.edu 3/15/95

44-5 Another neat way to view the data in color is to place the CVV ground image in L of L.a.b. or B of HSB (Hue, Saturation, Brightness) color modes and the DEM data in the other two channels. This gives the radar image of the ground over-tinted with colored contour bands. The fine-structure DEM is very dramatic when viewed in a palette of ten steps of green. Since the channels are all 640 x 2842, there are no co-registration issues. To reduce file size for rapid color experimentation, co-crop the full 3-channel image and split the channels.

Of course, what Tom Farr really wants us to do with these files is use the digital elevation map to draw a 2-D surface in perspective, then drape the CVV radar image over it. If the DEM has delicately colored contour bands (so as not interfere with the image), an overall 'airplane window' effect is achieved, with a subtle guide to actual elevation to facilitate interpretation of the alluvial fans. Photoshop and the like can only prep the DEM as a DXF file for export to high-end programs such as Strata 3-D. A more affordable solution that has many other imaging uses is macGIS ($30 in the educational version). I am not aware of any freeware up to the task. Again, I'm willing to donate the final file but there is no way to post it to the TOPSAR folder at this time.

tom @ emerald imagery 3/15/95

44-6 I'm impressed with what Tom Pringle has accomplished with Photoshop and the DEMs! I was never able to get Photoshop to ingest the 16-bit topo data, but with his hints, I'll try again. A program I've used on the Mac that accepts 16-bit data is the free program NIH Image. It of course scales the image to 8 bits for display, but retains the transformation, so you can find out what the height of that mountain, etc., is. It allows color tables to be manipulated, etc., but is far less powerful than Photoshop in terms of overlays and color images. I indeed like to overlay images onto topography for perspective views, but there are many other ways to use the DEMs for earth science applications. One that I'm involved in now is the fitting of 3-dimensional equations to landforms, such as alluvial fans (the shallow cones of gravel coming off the mountains in the death valley image). See the Transactions of the Amer. Geophys. Union (Eos), v. 73, p. 553-558 for some details. Other applications are mentioned in an article on TOPSAT (a spaceborne interferometer on the drawing boards) that should be coming out soon in the same newsletter. 3/20/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
44-7

Tom, that's a new one to me, about What year is your TAGU (Eos) article and did you mean by newletter that it is an electronic journal or list server? Your point is a valid one: for accurate equation-fitting of alluvial fans (and other landforms), the data need not be visualized, so 16 bit data is no problem. However, my first impulse would be just display the hypsometric layered tint (24 = 8 x 3) and stop with that because the ground scale of the data pixels falls short of topographic variation significant to physical processes, at least in the case of the Death Valley alluvial fans. I'm not sure I understand the advantage of analytic equations: the data is rasterized from day one, so why not just calculate from it directly as a GIS layer? OK, Ok, I'll look at the paper....tom @ emerald 3/26/95

QUESTION42
42-1 Pam Logan, of the China Exploration and Research Society, is one person looking at the data. You can contact her at pamlogan@alumni.caltech.edu. The World Monument Fund has some people working on this, too. 3/ 7/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
42-2 I'm a student that is new at the net. I would like some help on how to surf the net. Thanks 3/15/95
QUESTION29
29-1 Remote Sensing Bookmarks

Remote Sensing Sites

JPL Imaging Radar Bulletin Board
Internet GIS and Remote Sensing Sites
Center for Remote Sensing: Rutgers
Glossary of satellite acronyms
EROS Data Center
AVIRIS Satellite Program
AVHRR Pathfinder
Thematic Mapper
Landsat
Landsat: GLIS ordering

Imaging Radar

JPL Imaging Radar Home Page
SIR-C Data Example

NASA JPL FTP sites
NASA Shuttle Astro-2
APL Wave Processor Home Page
Science:Geography
Geoscience Maps
North America
GOES Weather Satelite
NOHRSC Snow
Weather Info
Gap Analysis
National Geophysical Data Center
California Enviro: CERES

Canada

NAIS
Geo Index
BC Servers

Remote Sensing Data and Information
Mapping-DBMS Interface
Global Earthquake Report
GISnet BBS WWW Home Page

USGS, USFWS, BLM, USFS

NASA Mission to Planet Earth
Global Change Data Center
Goddard Space Flight Center
Office of Satellite Data Processing
USGS DEMs
USGS GLIS ordering
USFWS
BLM: NSDI MetaData Sites
National Biological Service
US Army FLOOD

Other Planets

Planetary Images
Mars Atlas
Multiresolution - Astronomical Apps

Imaging Software

MultiSpec
NIH Image software
NIH-image: FFT
Image3.1.1 NCSA software
graphics software site
graphic utilities: selective!

3/15/95

submitted by tom @ emerald imager
29-2 Now the $64,000 question is how to edit, collate, remove repetitions, and reorganize largish lists of bookmarks. Netscape 1.1b1, according to MacWeek, has an automatic dead link finder but its location escapes me. Basically, exported bookmarks need to drop into a flatfile database with sorting of URLs and drag-and-drop re-ordering, then be recoverable as bookmarks in the new arrangement. I got this going, more or less, using 'replace' many times in Word and Word tables, via Works, but it is too much of a hack. Maybe someone has a freeware solution out there. It would be best if Netscape dealt with it internally. tom @ emerald 3/19/95
QUESTION45
45-1 Could I suggest you post an announcement on the Educator's BB, with your e-mail address so that students/educators can contact you directly to request a disk containing the material you have developed? By the way, it sounds great! 3/16/95
Tony Freeman, JPL
45-2 Tony, I have tried several times to send a comment to the Educators BB but it will not accept it. Any ideas whats up ?? 3/21/95
Bill
45-3 Since you now have a post to the education bulletin board (response to question 2), I assume that this is no longer a problem...perhaps the net was slow at the time, and it was taking awhile to post? 3/21/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
45-4 Bruce: I have had NO LUCK in posting a Question. True, the response worked OK but I am unable to type and send the offer for the PA Lab as a statement in the send question box. I wonder if that is why there are so few remarkes on the Educator BB ? Can you type my stuff in it for me ? 3/23/95
Bill again
45-5 can you tell me what browser you are using? I just posted a message from my Mac with netscape with no problem...

in the meantime, what do you want me to post ? 3/24/95

bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
45-6 Bruce, I am using EI Net at the moment, just because my hotlist includes this page. (We have Mosaic, MacWeb & Netscape as well) If you could type my offer #45 onto the Education Bulletin Board, I would appreciate it. I will try Netscap next. Thanx. Bill S. 3/27/95
QUESTION24
24-1 There is often very little correlation between the like-polarized (HH and VV) channels and the cross-polarized (HV or VH) channels in polarimetric radar measurments. The correlation between HH and VV can be anywhere between 0 and 1 and often carries a great deal of information about the physics of the scattering which produced the measurements. An additional complication is that the phase difference between HH and VV (whicha re actually complex values) also carries a lot of information.I can send you some materials on this if you send me your street address via e-mail. Tony Freeman, tony.freeman@jpl.nasa.gov 3/16/95
Tony Freeman, JPL
24-2 Thank you, Tony. I still have a long-winded question for the technical bulletin board about the raw SIR-C data set and its subsequent digestion. I have been puzzling over questions and responses of #20 and #25, and now #24.

The radar home page documentation seems to rely on an easy-to-read JPL analysis published in Radio Science, vol. 22, page 529. 1987, to whose notation and diagrams I refer below.

As I understand it, the Shuttle instrument basically collects as primary data the scattering matrix parameters, which relate transmitted and received polarization vectors by a 2x2 complex matrix. This matrix needs to be invertible from considerations of time-reversal invariance of the electromagnetic interaction, so its determinant is not zero. Sequential scattering is carried by matrix multiplication. In short, the set of all possible scattering matrices forms the non-compact Lie group Gl(2,C), an 8-dimensional real manifold.

The JPL article states that an overall phase can be neglected, leaving 7 parameters. This is tantamount to quotienting by the set of all unitary diagonal matrices, a normal subgroup, i.e., GL(2,C)/U(1). The article goes on to cite a principle of reciprocity developed in an unpublished1965 Dutch doctoral dissertation which sets off-diagonal elements equal, leaving 5 parameters. Now symmetric complex matrices (cv. self-adjoint) lack group closure: the product of two symmetric matrices is not in general symmetric (because transpose reverses order and multiplication is not commutative). Yet sequential scattering is a fact of life, so the 1965 proposal may be invalid. This reciprocity principle is a source of confusion in # 20 and #25.

Removing all scalar matrices from the scattering matrix yields GL(2,C)/GL(1,C) = SL(2,C)/Z(2) = SO(3,1) of dimension 6, or passing to maximal compact simple subgroups, SU(2)/Z(2)=SO(3). We now see the double cover explains the origin of the double angles in the Poincare sphere representation of the ellipticity diagram used in your polarization signatures. Many physicists would assume this group from the get-go, invoking general unitarity principles for scattering matrices, the need for the inverse matrix to be the adjoint, conservation of the energy-momentum 4-vector, etc.

Now a circularly polarized electromagnetic field carries angular momentum. Pictorally, the electric field vector rotates about a cylinder whose axis is the direction of translation. In modern terms, the photon is a massless spin 1 gauge boson transforming under integral representations of the proper Lorentz group SO(3,1). Plane polararized light is at the other extreme (zero spin), while ellipitcally polarized light is intermediate. In the Poincare sphere, the angular momentum must in effect be the projection of the elliptical polarization vector on the z axis. Note equatorial polarizations (plane-polarized) have no z-component, as expected.

It os instructive to consider orbits of symmetries that conserve angular momentum, namely the subgoup SO(2) = U(1) of the rotation group SO(3). The action rotates the Poincare sphere on its axis, fixing left and right circular polarizations, taking elliptical polarizations onto their latitude lines, and stabilizing (inter-converting) plane polarizations. This suggests parameterizing polarization signatures by a longitude.

If only magnitude (not sign) is of interest, inversions (reflections that reverse spatial orientation) identify north and south poles, corresponding latitude lines and antipodal equitorial points, reducing the Poincare sphere to RP(2), the real projective plane. Involutions provide a useful eignespace decomposition. The overall symmetry is expanded to the O(2) subgroup of O(3). More generally, Maxwell's equations are invariant under the full Lorentx group O(3,1)=[Z(2) x Z(2)] x' SO(3,1).

So the data seems subject to very substantial symmetry reduction. Is it not far better for JPL to crunch the data once and for all than to send out huge unreduced CD-ROMs and explain group theory to a thousand end users? The polarization signatures (currently imaged as a quasi-Mercator surface or as level curves on the Poincare sphere) positively glow with redundant symmetry. Where are our friends, the spherical harmonics? Is there not an even and odd decompostion of isotropy and anisotropy? Eigenbases of roughness vectors? Higher order terms that drop? I guess I am asking for a planned features list of your forthcoming software, macSigma 0.

Notice that both AIRSAR and SIR-C/XSAR provide us initially with undisplayable images, that is, virtual images whose pixels are Stokes matrices. While I don't have a personal issue with formal manipulations of mulit-dimensional arrays of matrices, image enhancement and scientific interpretation would be greatly facilitated by having monitor-displayable byte images. The real question is, how many real byte image channels will be needed to display all the information, assuming symmetry effects, under-utilized dynamic range, and intra- and inter- band statistical correlation can be removed? And how can these channels be chosen so that they retain physical interpretability?

Sorry to be so long-winded! 3/19/95

Dr.T, Emerald Imagery, tingalsb@OREGON.UOREGON.EDU
24-3 In regards to 24-2, the limitation of the classical correlation coefficient is that it only addresses linear correlation. In other words, two variables with perfect parabolic correlation could have zero linear correlation. In the history of statistics, linear correlation was over-emphasized because that was already a handful with adding machines. [Of course, linear terms arise as the first term in the MacLaurin series expansion of whatever the functional dependence was.] Today, what with Mathematica on every desktop, all mannner of complicated relationships are considered in determining the inter-dependence of independence of two variables.

To say, for example, LVV isn't correlated [linearly predictable] from LHH is not to say there isn't some other simple relation between them. This might be adduced from theoretical grounds or empirically from the scatter diagram. I must respectfully disagree with decoupling the analysis of phase and amplitude correlations. [This procedure already wreaks havoc with real variables, where the sign serves as 'phase.' All the arithmetic operations needed to calculate correlation, such as subtraction, norms, and division, hold for complex numbers. If we would look in a sufficiently obscure statistics journal, we would find statistics was long ago extended to the case of correlation of complex [or quaternionic, 'phase' a point on 3-sphere] variables. Correlation is inherently a geometric concept.

I am not sure how much we are going to learn about the physics producing the scattering event. This is because If the radar pixels are, say, 25 meters square, there are only 9 per acre. A lot of different things can go on across this ground scale. Aren't we learning instead about the superpositioning of a large number of possibly unrelated radar reflection events that produced the final composite signal? I couldn't find very many images to test on the bulletin board. However, the Weddel Sea used LHV and LHH as R and G. These images may have gone through many stages of non-linear tweaking. As posted, the correlation coefficient is indeed low. The scatter plot shows even better that the case is hopeless.

Next, I looked at the AIRSAR Death Valley Images for the L, C, and P radar bands. I did the principal components in Dimple, finding little inter-band linear correlation as these things go:

L,C,P Inter-Band Correlation
Component Variance
PCA 1 79.0%
PCA 2 17.6%
PCA 3 2.7%

The table needs a modern browser to display its excesses. tom @ emerald 3/26/95
QUESTION48
48-1 When I just tried it, (Friday 3pm california time), it ranged from 10 seconds to download a browse image, to a couple of minutes to download the same file. When it takes a long time, I recommend trying again later, the EROS data center server is probably overloaded with requests. 3/17/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
48-2 I suspect that the CD-ROM is being automatically loaded and this takes time. There are over 50 CD-ROMS, so they are not all on line I suspect. 3/27/95
QUESTION30
30-1 check http://images.jsc.nasa.gov/html/earth.htm for listings of hand-held photography from the second flight, by lat, lon, or frame number. Unfortunately, they don't list the pix by MET, so it'll be hard to cross-reference to the radar images... 3/23/95
Tom Farr, JPL, tom.farr@jpl.nasa.gov
QUESTION50
50-1 I unfortunately do not have a reference for you about Lee and Frost filtering, but the slant to ground range conversion may be done by simple geometry. In the azimuth direction, no correction is necessary unless you want to resample the pixel spacing in that direction. In the range direction, the ground range pixel spacing is the slant range pixel spacing divided by the sine of the incidence angle. The tricky part is the resampling to the ground range projection, I am not sure about which interpolation to use, you might want to experiment with several... 3/24/95
Bruce Chapman, jpl, bruce.chapman@jpl.nasa.gov
50-2 Here is a freeware Lee filter, actually something better, a script for local Lee sigma filtering (an adaptive filter that replaces a bad pixel with the local mean if it is a user-specified number of local standard deviations from the local mean). An enclosed even better variation replaces the bad pixel under the same circumstances with the local gaussian blur instead of the local mean.

Never heard of a Frost filter -- what is it supposed to do; does it have another name? tom @ emerald

!local Lee filter as Dimple IOL script images x "whatever" input ; localmean "so" temp ; lmsqd "po" temp ; lsdinitial "io" temp ; mlsdsqd "YP" temp ; lsd "uu" temp ; final "Lee filtered" output ; operations localmean = filter x (1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 ) / 25 ; lmsqd = localmean * localmean; lsdinitial = x * x; mlsdsqd = filter lsdinitial (1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 ) / 25 ; lsd = sqrt( mlsdsqd - lmsqd ); final = If (x > 1.5 * lsd) then localmean; Else x ; endif ; !local Lee gaussian blur as Dimple IOl script images x "whatever" input ; localmean "so" temp ; lmsqd "po" temp ; lsdinitial "io" temp ; mlsdsqd "YP" temp ; lsd "uu" temp ; gauss "pp" temp ; final "Lee filtered" output ; operations localmean = filter x (1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 ) / 25 ; gauss = filter x (1,1,2,1,1,1,2,4,2,1,2,4,8,4,2,1,2,4,2,1,1,1,2,1,1) / 52 ; lmsqd = localmean * localmean; lsdinitial = x * x; mlsdsqd = filter lsdinitial (1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 ) / 25 ; lsd = sqrt( mlsdsqd - lmsqd ); final = If (x > 1.5 * lsd) then gauss ; Else x ; endif ; 3/25/95

50-3 I second the idea that the optimal resampling protocol is tricky., especially if contemplated at the level of intact scattering matrices. For amplitude data, could you explain briefly the 'several' interpolations' already considered? How would we verify that one method worked better than another? My first impulse is to fit a polynomial surface to the slant pixels and then use a parabolic-cylindrical change of variables to incorporate the cosecant multiplication. tom @ emerald 3/26/95
QUESTION47
47-1 I've never heard of it, can you tell us what it is? 3/24/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
47-2 Totally obscure. Not posted anywhere on Web.

tom @ emerald
3/29/95

47-3 I'm not sure if this is what you're looking for but try this: RASSP E&F Home Page at rassp.scra.org on the web also www.ee.gatech.edu/research/DSP/ 4/ 1/95
Michele Estebon, estebon@uhhacb.uhh.hawaii.edu
QUESTION46
46-1 I've never heard of it, what is it? 3/24/95
bruce chapman, jpl, bruce.chapman@jpl.nasa.gov
46-2 Nothing on Web. What is a radar board? Try a Internet white pages search for Tom McKewan.

tom@emerald 3/29/95

46-3 Lawrence Livermore National Labs (LLNL) Location: http://www-atp.llnl.gov:80/ I'm not sure if they have any info on this page about it, but the webmaster should be able to lead you in the right direction. 4/ 3/95
Andy R. Mattice, D.M. Industries, logan5@hti.net
46-4 Thank you for your responses ! I did manage to find out some more information regarding the MIR radar board, from the LLNL. By the way this MIR board is the $10 radar. I have several projects that I would like to work on. Most of them are hokey, but they would be useful devices So far, I have not found a source for these boards. Any help would be greatly appreciated. Thank you. 4/ 4/95
Brett Scott, Just a regular guy, blscott@scottnet.com
QUESTION52
52-1 Yes, indeed. Are you doing custom fly-overs and for what price per mile of swath? Is the data's dynamic range 8-bit? What's your ground resolution at 800 meter height? I would find it more useful to have the radar image registered with a color infra-red photo, even if it's older, than a cartographic map, if I can't have both. Why x-band and are you limited to this? Post some sample radar imagery for us -- forget email, where is your home page anyway? tom@tingalsb.oregon.urogen.edu 3/29/95
QUESTION55
55-1 The image you refer to, P-44758, is a detail of the interferogram derived from 2 passes of X-SAR data (April and October, 1994). The fringe patterns that you see have three likely sources: 1) Topography 2) Small-scale (cm) changes in the position of surface features along the radar line of sight in the six-month interval (i.e. the deformation you asked about) and 3) Differential rotations of the phase of the radar echoes in the two data sets due to differences in atmospheric water vapor abundance along the radar signals' path. To isolate effect number 2 from the others, one must first remove the topographic effect using a DEM (not trivial, but not too dificult, either), and second, gain an understanding of effect number 3 (very difficult). The atmospheric effect was not recognized originally on the analogous SIR-C "displacement" map (P-44753), but detailed comparisons with GPS data show that this can be a real problem. Bottom line is, the fringes in the X-SAR image are not merely a simple function of surface displacements, and should not be interpreted as such. 4/ 3/95
Jeff Plaut, SIR-C Experiment Scientist, JPL, plaut@jpl.nasa.gov