I have noticed that the January 1, 2007 Cassini PDS release is already available, see http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/
I haven't downloaded all of the imaging data and I'm just beginning to digest what I already have but there are some beautiful images of Enceladus' plumes and satellite mutual events, images of the G and D rings and interesting images of Saturn's nightside and fairly good Iapetus images.
Radar and VIMS is also available.
All in all a nice 'Christmas gift' .
This release covers the time period from January 1 to March 31, 2006. No RADAR SAR swaths were taken during this period of time. There were three Titan flybys: T10 (ORS covering anti-Saturnian hemisphere), T11 (ORS low-phase inbound over sub-Saturnian hemisphere), and T12 (ORS moderate phase over anti-Saturnian hemisphere). T11 has some good observations, never messed with T10 or T12 too much since it covered the same territory we had seen over and over again without adding to much new information.
Beyond Titan, there is a decent sequence at Enceladus from Rev20 (look for images in the N1516153055 through N1516171418 range). There are also decent Rhea observations during each orbit (Rev20-21-22). rev22 has some decent Rhea saturn-shine images. Finally, Rev21 has a couple of observations of Tethys over Penelope crater.
EDIT: actually, there was a distant SAR look on T12. I'll try to post that within an hour.
EDIT again...: and that isn't available yet. Hopefully it will be up by Monday.
Here's an 8 frame animation showing the late January 2006 "flyby" of Iapetus from this PDS batch. Closest approach was around 880 000 km.
http://m1.freeshare.us/view/?126fs4705368.gif
Three of the frames are natural color RGB composites, the rest are stretched color IR/G/UV processed to match natural color views. Images have been magnified 2x for better visibility.
cool
Not that I can see. It is possible that I was wrong and that there wasn't a distant SAR look on T12, but I could have swore they did.
(pointed here by Emily's post in http://www.unmannedspaceflight.com/index.php?showtopic=3135&pid=83262&st=15&#entry83262)
The April 1, 2007 PDS release is out with new ISS, VIMS and RADAR data.
I have looked at all of the ISS images and updated my summary of Cassini images at http://www.mmedia.is/bjj/misc/css_stuff/images/coiss_overview.html.
I will soon be adding a list of flybys for each satellite near the top of the document ("a summary of the summary").
The ISS release wasn't particularly interesting to me this time. Some highlights:
* Images of Iapetus down to a range of ~600,000 km
* Two targeted flybys of Titan
* Many spectacular satellite mutual events since Cassini was very close to the ring plane
* Interesting images of Hyperion, Janus, Atlas and Pan
* Rhea global color at a range of ~480,000 km
* Many distant high phase images showing Enceladus' plumes
* Saturn star occultations
Incidentally, I ran into a few cases of erroneously formatted numbers in several of the index.tab files that caused some problems when loading these files into an Access database so I'm going 'complain' to the PDS. Example: 1.0524616e-
I suspect 'very small' numbers may get incorrectly formatted, possibly numbers smaller than 0.001 or 0.0001.
I could make the database available if someone can host it, it's too big for me to do so (about 55 MB zipped). It contains all of the information from all of the index.tab files on volumes COISS_1001 to COISS_1009 and COISS_2001-COISS_2023.
Is anyone having luck accessing the PDS site, namely http://pds-imaging.jpl.nasa.gov/? It's broken for me at least since yesterday.
Same thing here. Fortunately I finished downloading the ISS data before this started .
http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/ works fine for me right now.
Some highlights from my perspective are the T13 radar SAR swath (the one that crosses Xanadu) and the distant encounters with Janus and Pan.
Here's Janus, an approximately natural color view and enhanced stretched color to bring out subtle color differences:
http://m1.freeshare.us/view/?130fs699977.png
Unlike Telesto which appears bluish in natural color and very faintly orangish in stretched color, Janus is more like other rocky moons -- Prometheus and Pandora. Magnified 2x.
A few comments:
This is a Microsoft Access database containing two tables, coiss and coiss_revised. Coiss simply combines all of the index.tab files on the Cassini ISS volumes 1001-1009 and 2001-2023 into a single database without any significant modifications, except for the rejection of erroneously formatted numbers (see the list of errors at the end of this message).
The coiss_revised table contains updated values for a few fields. These values are *probably* slightly more accurate (from my experience when doing a cylindrical map of Saturn) than the original values although I cannot completely guarantee this. They are computed from the latest SPICE kernels (CK and SPK). The NORTH_AZIMUTH value is also included as there's no equivalent field in the coiss table. At this time only a few images are included in coiss_revised. I don't know the exact geometric meaning of north_azimuth_clock_angle in the index.tab files but it is totally different from north_azimuth so I added north_azimuth in a separate table. However, I have only determined it for a few images (70 - mostly the ones I used to do a map of Saturn) but plan to do so for all of the images, possibly before the next batch of images gets released 3 months from now.
There are a few simple queries there as well that I decided to include as a simple example of what can be done.
I use this database extensively when searching for interesting and/or specific images, both from within Access and directly from programs I have written. I rarely use the PDS to search for images, I mainly use it to download entire data volumes.
As previously mentioned I found errors in some of the index.tab files. The errors I know of are:
coiss_2017: There are erroneously formatted floating point numbers in rows 1253-1257 in index.tab, columns 2541-2551 (SUB_SPACECRAFT_LATITUDE). I tried 'guessing' the correct values. These are images N1512191594_1.IMG, N1512191728_1.IMG, W1512191728_1.IMG, N1512191860_1.IMG and N1512191993_1.IMG.
coiss_2020: There are erroneously formatted floating point numbers in rows 170-171 in index.tab, columns 2628-2638 (TARGET_SOUTHERNMOST_LATITUDE). I fixed this manually - the fixed values are a guess and the correct value to use is uncertain. These are images N1517273822_1.IMG and N1517273855_1.IMG.
coiss_2021: There are erroneously formatted floating point numbers in rows 1980-1990 and 2648-2649 in index.tab, columns 2541-2551 (SUB_SPACECRAFT_LATITUDE). I fixed this manually - the fixed values are a guess and the correct value to use is uncertain. These are images W1520869299_1.IMG, N1520869388_1.IMG, W1520869388_1.IMG, N1520869616_1.IMG, W1520869616_1.IMG, N1520869705_1.IMG, W1520869705_1.IMG, N1520869934_1.IMG, W1520869934_1.IMG, N1520870023_6.IMG, W1520870023_1.IMG, W1521409807_1.IMG and N1521409944_1.IMG.
coiss_2023: There are erroneously formatted floating point numbers in rows 2785-2788 in index.tab, columns 2616-2626 (TARGET_NORTHERNMOST_LATITUDE). As previously I fixed this by trying to guess the correct values. These are images N1530372696_1.IMG, N1530372841_1.IMG, N1530372986_1.IMG and N1530373131_1.IMG.
There might be more errors.
Is there any sort of search capability in existence for any of the PDS ISS released products ??
For instance... if one wanted to look for NAC images where the boresite intersect was in the B-ring
and the range was under say 10 Rs ??? or where the target was PROMETHEUS and the range was under
1M km ??
my first impression is that the INDEX.TAB files *seem* to have some problems ... but perhaps I've not
gone thru enough documentation .... any pointers on documentation source would also be great !!
Thanks !!
I'd say the best thing to use to search would be Bjorn's database, referenced earlier in this thread. He's already got basic queries on some targets with ranges in there -- they'd be easy enough to modify to get your Prometheus-under-1Mkm search, but I don't know how you'll do the B-ring one.
Bjorn, if you update your database with the tables of info from the latest release I'll gladly host it for you.
--Emily
What tallbear wants to do should be trivial to do in my database, in fact the reason I made the database was that I wanted flexible search capabilities. The Prometheus-related query is trivial (there are similar sample queries I did in the database where the target is different but they illustrate how to do this).
The B ring query is probably easy as well although I should mention that I have not tried something like it (I'm on my laptop at the moment and the database is on my desktop computer so I cannot try it at the moment).
I didn't notice any problems with the INDEX.TAB files except for the ones mentioned in my April 3 message earlier in this thread. The database contains all of the fields/columns from all of the index files.
Cool... I'll try Bjorn's database....read over what it takes to get it up and running....
It's interesting that the Rings Node has really neat search capabilities for Voyager
images... but for Cassini ... it's unmannedspaceflight.com that's forging the way ....
...Thanks ... Great Work ... I'll get in and start nosing around...
The July 1, 2007 PDS Cassini release is starting to appear. The ISS and VIMS stuff is already there:
http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/
So far I have downloaded only about 1500 ISS images and have looked at only a few of them but there's one particularly interesting imaging sequence in this release: The ISS data includes the famous imaging sequence showing Saturn and the rings backlit with the Earth visible as a tiny bright spot. That particular imaging sequence starts in directory data/1536725883_1537013377 on the coiss_2025 volume.
Cool!
I've been wanting to do something to make PDS Cassini images easier to find but this data set is way too big for me to do a complete treatment on it. Instead, I was thinking of producing an index page to all moon images where the moon spans more than N pixels. The thing is I haven't decided what N should be yet. 200? 100? 128? What's a good number? I'd probably use a different number for the major icy sats than for the ringmoons and Lagrange point moons. Any thoughts?
--Emily
Emily,
That would be pretty neat to see an index. From my perspective it sounds like you have some good numbers in mind. In the case for some of my maps I've used images getting down to just over 100-120 pixels, though most are over 200.
What would the diameter be for the middle of the disc to be 1 degree of latitude / pixel. That might be an appropriate figure to work from. My brain can't do the trig to figure it out
Doug
Maybe 115 pixels?
Yeah, it could be 115. 1/sin(0.5 deg).
I sketched my little diagrams and chanted "SOH CAH TOA" and worked it out and yes it came to 114.6 pixels. That sounds like a good plan. I'll put in >114.
I ran that in to Bjorn's database as of March and got the following numbers of images:
Mimas: 422
Enceladus: 623
Tethys: 749
Dione: 884
Rhea: 1584
Hyperion: 677
Iapetus: 2181
Phoebe: 383
These numbers are a little on the highish side...running it down to 200 pixels across, here's what I get:
Mimas: 327
Enceladus: 603
Tethys: 308
Dione: 600
Rhea: 1150
Hyperion: 496
Iapetus: 1061
Phoebe: 227
(Interesting how much of a hit Iapetus and Tethys take, while Enceladus is virtually unchanged!)
...and remember that that's less than 2/3 of the way through the mission. I'm kind of inclined to go with the higher number so as not to have mind-numbing quantities of images where the moons aren't very big, but if someone makes the case that I'll miss out on too many phase angles or mutual events I'll try it with the lower-res ones included.
I should also add that I'm not real excited about downloading 25 volumes and will be more excited about doing this if I can figure out how to use Bjorn's database to write batch files for wget that will only retrieve the files I want...we'll see!
--Emily
Screw it - go for 2 pixels / degree 230 pixels for cash.
Doug
I think it might be a good idea to limit this by resolution and not pixel size. A 115 (or 200) pixel diameter image of Mimas or Enceladus is usually much more interesting than a 115 pixel diameter image of Rhea unless you are interested in photometry. Another way of putting this: Make the size limit in pixels a function of satellite radius.
That's not a bad idea. Got any specific recommendations?
--Emily
Hm, taking Mimas as your 114 px baseline, that comes out to:
Mimas 114
Enceladus 140
Tethys 292
Dione 306
Rhea 417
Titan 1405
Iapetus 392
Assuming I'm not working with ridiculously antiquated figures here...
I now have the information on the just released Cassini images ready for getting added to the Access image database discussed earlier in this thread. That database includes everything up to and including the April 1, 2007 release. The files below add the images released on July 1, 2007.
Transferring the entire database file is an overkill so I prepared two Excel (!) files that can be imported into the database. The files are fairly small (less than 3 MB each). Emily has hosted them on the same server as the database:
http://filicio.us/tpss3/files/23158/cassini_images_index_24.zip
http://filicio.us/tpss3/files/23159/cassini_images_index_25.zip
In Access, do File -> Get External Data -> Import
What follows should be obvious, accept the defaults and when asked "Where would you like to store your data?" choose the table "coiss" in the list that appears next to "In an Existing Table:".
Thanks to Emily for hosting this together with the database.
A little comparison of Cassini's solar eclipse as seen by VIMS and ISS:
Two short time-lapse sequences:
Three frames on the left show the opposition surge on part of the rings. Don't know which part though, probably A or B rings. The surge appears elongated probably because as VIMS was scanning the cube the opposition highlight moved. Also note ring darkening as phase increases.
The 5 frame sequence on the right was taken on 2006-08-18 and spans an hour and a half. Each VIMS scan took more than 10 minutes to read out. Noisy as hell. I removed most of the linear noise but it wasn't perfect and left some residuals as well as cosmic noise hits.
I'm returning to this project after a hiatus. I am now trying to figure out what information will be valuable to include in the browse pages. There is a huge number of fields available in the database. Here is what I am thinking about including; let me know if there are any fields I've missed that you can't live without.
FILE_NAME (e.g. W1481738172_2.IMG)
TARGET_NAME (e.g. DIONE)
TARGET_LIST (listed only if it is not "N/A" or identical to TARGET_NAME -- picks up other bodies that may be in frame, useful for mutual events)
OBSERVATION_ID (e.g. ISS_00BDI_GLOCOL001_PRIME) <-- note you get information on which rev you're on in this one
IMAGE_MID_TIME and IMAGE_MID_TIME_SEC_FRAC (e.g. 12/14/2004 5:30:21.716) -- is this OK or is START_TIME better?
PIXEL_SCALE (e.g. 9.3249958) <-- in km
TARGET_DISTANCE (e.g. 156875.92) <-- in km. this is redundant with the pixel scale but I think it's useful to show both.
PHASE_ANGLE (e.g. 34.258215) <-- in degrees
SUB_SPACECRAFT_LATITUDE and SUB_SPACECRAFT_LONGITUDE (e.g. 11.092879 and 207.90797) <-- I prefer this to the CENTER_LAT and CENTER_LON because I think it makes more sense for images where the entire body is contained somewhere within the FOV.
EXPOSURE_DURATION (e.g. 5600) <--need to state units
INSTRUMENT_MODE_ID (listed only if it's been 2x2 or 4x4 binned, "SUM2" or "SUM4")
INST_CMPRS_TYPE (LOSSY or LOSSLESS)
Some questions:
Can I get away with skipping INSTRUMENT_ID? Whether it's WA or NA will be clear from the file name.
Are EMISSION_ANGLE and INCIDENCE_ANGLE important, or is there enough information contained in PHASE_ANGLE?
--Emily
Instrument_ID isn't important if you are listing both WACs and NACs, and the file name is listed. That field is just useful as a search criteria, e.g. you want to retrieve NACs only.
Emission angle and incidence angle is important if the object more than fills the frame. Emission angle is important if you are looking for useful Titan images.
I just went through the process of creating an index page for Dione, using the 2 pixels per degree (=228 pixel diameter) size cutoff:
http://planetary.org/data/cassini/dioneattempt/
WARNING: to view this page requires you to download about 42 MB of data.
[Note: I didn't bother uploading the full-size images, only the thumbnails, so the images won't link to anything. Also, I didn't yet include all the fields I mentioned in my previous post; I did intend to include the filters and stupidly forgot. Next time around they'll be in there.]
This included more than 500 images, but after seeing the results I don't think it was enough. Cassini has so danged many filters that those 500 images were for a relatively small number of distinct observations (22), most of them on nontargeted flybys; the query did not pull in nearly as many global shots of the moon as I was hoping to get. So I think I will back away and try the 1 pixel per degree cutoff next time.
What do you think of the layout, with one observation per line? I think I will reduce the size of the thumbnails next time. They are currently 256 pixels -- I think I will reduce to 128 or even 100.
I used IMG2PNG to convert these, and did calibration, but the calibration didn't seem to work for the WAC images for some reason.
Comments?
Emily
Wow, this is quite an undertaking you're doing there, Emily! You sure your server is good for all this data?
One parameter that might be nice to add is which way north is (IIRC can be approximated from from the so-called TWIST_ANGLE). I'd use IMAGE_MID_TIME as I think it's more reliable than START_TIME.
What do you mean by WAC calibration not working? 128 pixel thumbs seem about right, anything smaller might make more distant observations look bad.
There are a few more fields I'd include, in approximate order of priority:
FILTER_NAME_1
FILTER_NAME_2
SUB_SOLAR_LATITUDE
SUB_SOLAR_LONGITUDE
INST_CMPRS_RATIO
DECLINATION
TWIST_ANGLE
RIGHT_ASCENSION
The first five are essential in my opinion. Possibly include VOLUME_ID and some of the RINGS_ fields as well.
Note: I'm using the field names from the Access database, not the fields in the INDEX.LBL files (which describe the contents of the INDEX.TAB files from which the database was generated). The field names are usually identical but there are a few exceptions where I broke a field from INDEX.LBL up into two fields, for example the two FILTER_NAME fields (because it seemed more convenient) and the SEC_FRAC fields (because as far as I know the maximum precision of Access dates is one second).
I'd use IMAGE_MID_TIME as you did rather than IMAGE_START_TIME.
The page layout looks fine but it contains a lot of stuff (42 MB) so maybe it should be broken up into several pages, probably by OBSERVATION_ID.
I'll see if I can find out why calibration didn't work for the WA images (it does on my machine when I use my big program from which IMG2PNG was cannibalized).
I like it. Perhaps you could do it with more images, but do it yearly (in other words, separate pages for 2004, 2005, 2006, etc). One thing (not sure if it is just because you are still working), the links to the PNG images don't work.
I've stumbled upon an error in the latest batch, there are two polarized UV NAC frames, N1536539385_1.IMG and N1536539427_1.IMG incorrectly labeled as:
TARGET_DESC = "Tethys"
TARGET_LIST = "N/A"
TARGET_NAME = "TETHYS"
OBSERVATION_ID = "ISS_028TE_TETHYSORS001_CIRS"
When in fact they target Enceladus:
I've reduced the thumbnails to 128 pix and converted them from 16-bit PNG to JPG, and together that brings the page down to 2 MB of data, which is much better!
One thing that bothers me about this page is that there's a lot of redundancy -- it doesn't seem necessary to show thumbnails of all of the images of the same spot taken through different filters. I'm going to do some fiddling and see if I can come up with a different way to present this that has less redundancy, but shows more of the metadata.
Hmmm...
--Emily
Ahh, that explains it. Thanks a lot, pat, I'm always interested in learning in more detail how all these sequences are actually developed and executed at the low level. The shortening of the observation does seem like the most plausible reason. I did notice the one smeared image you mention, but the empty ones must have slipped me as "non-interesting".
Speaking of slew maneuvers, one thing I was always wondering is how much buffer time the cameras use when making mosaics of targets spanning over 1 FOV? Is it a couple of minutes or shorter? How fast can Cassini actually turn around say 180 degrees and steady up at the target pointing?
OK, I've had a slightly different go at it.
http://planetary.org/data/cassini/dioneattempt/index2.html
This is a much improved 726k to download. Note that the links to full-size images still do NOT work.
I used the 1 pix/degree cutoff this time (923 images) and incorporated more metadata, but am only showing one image from each multispectral set. I think I am happy with the number of observations included now -- I think it's more like 44 -- but am not totally happy with the page layout yet. I was hoping to come up with something where I could almost fully automate the generation of the html, but the step of deleting redundant images (something that's really necessary to reduce the amount of data on the browse page) has to be done by hand, and that's time consuming.
Two things I forgot and will include in any future version: I wanted to put the file names in with the metadata, but they're not there (though they are preserved in the URLs, so at least you can see them that way); and I wanted to include the TARGET_LIST field at the end.
EDIT: I added one more thing -- I was curious to see how many of these observations had resulted in products released to Photojournal. Many have, but many have not; and there are also a great many Photojournal releases of images where Dione was smaller than my size cutoff (though many of these were multiple-body images, so the small size made sense). Notes on Photojournal releases are now on the page. Also, the look through Photojournal made me realize that I missed all the opnavs, because these have a target of "SKY" -- I need to modify my query to add in those opnavs. There were 20 or so that were within the size range.
I'm going to start uploading the full-size images now and leave it running overnight -- it's 800 Megs of data!! That's a bit more than I bargained for. Too many 16-bit images.
Comments?
--Emily
Wow, I assumed the reaction wheel figures were high but these are quite substantial indeed. Is the time difference primarily due to different mass distribution along each axis? I can't seem to dig up a schematic showing the orientation of principal axes, but this would suggest the Z axis running along the length of the s/c, parallel with HGA boresight and the X axis being the most inert of them, orthogonal to the plane in which HGA boresight and magnetometer boom lie?
How do these figures change with propellant depletion (if at all)? Optimizing slew maneuvers is no doubt one of the (many) factors in increasing useful observation times...
Thanks. For the Photojournal images, I just searched on Dione, and then I matched the dates and, when date was ambiguous (or, in one case, incorrect), I matched the phase angles and distances. A bit tedious but that's one thing I've been very curious about -- just how many of the "good" images have been released to the public in one way or another? It's not a bad proportion, it turns out, but it's not all of them by any means, and there is a LOT that can be done that hasn't yet been done with color data.
The 16-bit images do have a variety of brightnesses, but I did use IMG2PNG with the "-r" switch and all the Cassini calibration data to calibrate them as I did the format conversion. Clear and green filter images do seem to be pretty reasonable in their brightness, UV ones are pretty dark -- which is more or less what I expect, actually. Remember that Dione is somewhat dark as icy satellites go. Maybe Bjorn can comment on whether the full-size images look like they are supposed to, especially in the UV. I did get errors on every WAC image upon conversion though, so I'm not sure that those are properly calibrated. Of the 900 or so NAC images, IMG2PNG reported errors during the calibration step for about 20 of them.
On the next go-round I'll do Enceladus and we can see how different those look.
--Emily
I was intrigued by some fairly big brightness differences between different filters in Emily's page. For example the UV images turn out much darker than when I throw them through my software. I decided to do a comparison of narrow angle frames N1507738546_2 (RED,CL2), N1507738663_2 (CL1,GRN) and N1507738491_2 (BL1,CL2). Below are simple RGB composites, modified only to resize and register the three filters:
http://m1.freeshare.us/view/?164fs366995.jpghttp://m1.freeshare.us/view/?164fs367198.jpg
The left image uses IMG2PNG converted data, the right one is my calibration result.
I didn't touch the channel balance in the left case, there are a couple of notes about my results:
I do all the calibration steps except dark current removal. In practice this doesn't amount to anything than a slightly brighter background signal in the longer exposed images (blue and especially UV in NAC and violet in WAC case) and is in no way capable of such a drastic difference. If you really kick up the saturation in my image, you'll see the bluish hue likely due to dark current.
Other than that, I use the official calibration "fudge factors" found on COISS_0011 with a slight modification for RED/CL2 filters. Early on I realized the red channel turned out consistently too bright with those factors so I worked out it needed to be multplied by 0.949 to bring it in line with other filters. The official calibration factors might indeed be off since they're quite old as a contact from PDS emailed me, in fact the whole calibration procedure was greatly improved since then. I don't have too much faith in other infrared filter factors either. Such factors weren't even derived for WAC and are missing from the calibration volume.
The color of Dione's surface in the left case suggests to me it shows the total radiance as seen by the instrument. It reminds me of my VIMS experiments without dividing by solar spectrum as sunlight is actually yellowish.
In my calibration procedure the filter transmissivities are divided by integrated solar spectrum and produce reflectance (I hope it's the right term) instead, the intrinsic color of the moon if you will. This is consistent in that it produces gray Mimas, Enceladus and gray non-stained hemispheres of Dione and Tethys. In essence the color they'd appear if shined upon by a big, white light lamp.
I like your page elakdawalla
Reminds me of a http://www.divshare.com/download/1457089-5e2 I did for Themis. Apologies for the file share download, but it's all I have at the moment.
MouseOnMars
It's starting to appear, the ISS volumes COISS_2026 and COISS_2027 are up, but not searchable yet. They can be accessed directly:
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2026/
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2027/
I've done a preliminary browse of the thumbnails to see if anything interesting's up. This is still the time period when Cassini was spending a lot of time on the nightside, seeing unlit rings. The real good Saturn stuff should be appearing in the Jan 1, 2008 release.
In the meantime, here are a few takeouts:
http://i108.photobucket.com/albums/n15/ugordan/Hyperion_RGB_2X.png
Hyperion in natural color, 2x magnified.
http://i108.photobucket.com/albums/n15/ugordan/Iap_RGB_IR3GUV3_Nov_27_2006_2X.png
Iapetus in natural and IR3/GRN/UV3 color, 2x magnified. November 27, 2006.
http://i108.photobucket.com/albums/n15/ugordan/NiceWacshadow.png http://i108.photobucket.com/albums/n15/ugordan/WAC_RGB_normal.png
Couple of Saturn north pole shots. A moon shadow (probably Mimas) visible near the terminator in the left image.
Titan and a lovely shot with Saturn's hazy limb showing through the translucent, unlit rings:
http://i108.photobucket.com/albums/n15/ugordan/W1544657962_1_8bit.png http://i108.photobucket.com/albums/n15/ugordan/Titan_NAC_RGB_N1540316375_1.jpg http://i108.photobucket.com/albums/n15/ugordan/Rings_NAC_RGB_8bit.png
I've been waiting for this!! Thanks for the notice, Gordan.
Bjorn, I'm ready to make the database update whenever you can put the tables together.
--Emily
This also means that some of my favorite SAR swaths, from T19, T20 (HiSAR over Tortola Facula), and T21 will also be released.
The information from this ISS release is now ready for getting added to the Access database described in this thread (see http://www.unmannedspaceflight.com/index.php?showtopic=4076&view=findpost&p=87414). The database includes all of the information from the index.tab files and makes the images much easier to work with.
As before, Emily has hosted them on the same server as the database:
http://filicio.us/tpss3/files/31020/cassini_images_index_26.zip
http://filicio.us/tpss3/files/31032/cassini_images_index_27.zip
These are Excel files that must be added to the Access database as described http://www.unmannedspaceflight.com/index.php?s=&showtopic=4076&view=findpost&p=93903.
The ISS volumes Coiss_2026 and Coiss_2027 are now available from
PDS Planetary Rings Node in zipped form (convenient for downloading).
http://pds-rings.seti.org/archives/
There is an early 'Christmas present' at the PDS: The January 1, 2008 data release (ISS and VIMS) is already there. I have managed to take a quick look at all of the ISS images and post a summary at http://www.mmedia.is/bjj/misc/css_stuff/images/coiss_overview.html . This also includes all of the earlier ISS data volumes.
With the exception of Titan, there are very few interesting satellite images this time, Cassini's orbit was highly inclined. The most interesting ones are probably the ones of Hyperion in coiss_2029\data\1550261798_1550410364 (mentioned by Emily in http://www.unmannedspaceflight.com/index.php?showtopic=3861).
There is heavy emphasis on the rings with lots of various movies including F ring movies, spoke movies etc. plus lots of multispectral coverage showing both the lit side and the unlit side. There are also many interesting images of Saturn, mainly WAC images. These include great images of the south pole obtained at high inclination. There are several images there that I'm going to process when I have the time (probably immediately after Christmas).
Updates to the Cassini image database (see http://www.unmannedspaceflight.com/index.php?showtopic=4076 for further details) are available at the following URLs for volumes coiss_2028, coiss_2029 and coiss_2030 respectively:
http://planetary.s3.amazonaws.com/data/cassini/metadata/index_28.zip
http://planetary.s3.amazonaws.com/data/cassini/metadata/index_29.zip
http://planetary.s3.amazonaws.com/data/cassini/metadata/index_30.zip
Lot of good stuff in this PDS release. Your summary page is very helpful, particularly before the new data becomes searchable on the PDS.
Here's a quick Saturn composite, just part of a sequence of color ring plane crossing Ian Regan animated back in the day:
http://i108.photobucket.com/albums/n15/ugordan/saturn_van.jpg
"....There is heavy emphasis on the rings with lots of various movies including F ring movies, spoke movies etc. plus lots of multispectral coverage ..."
My recollection is that the Voyagers got surprisingly little multispectral coverage of the rings. Imaging sequences concentrated on things like phase and inclination angle, radial structure mapping, etc, followed by the big "spoke movie" from Voyager 2 after the Voyager 1 spoke discovery.
I think I recall that one mision (maybe Voyager 1), got only orange/blue or some such 2-filter moderately high rez color coverage of the rings. I suspect there was no expectation that the rings would have widespread color variation and only minimal effort to check for radial color variations was worth the data-bandwidth.
There is definitely a large body of high phase multispectral ring data from Voyager. I am not sure about data taken on approach.
I've made progress on my massive project to make the better images of the icy satellites more accessible to people. I'm not quite done with it -- I still need to sort out and format pages for Phoebe and the rocks, and have a bunch of introductory and explanatory text to write -- but for those of you who don't need any hand-holding to enjoy PNGified versions of every decent-sized icy satellite image in the PDS, here's the work in progress: http://www.planetary.org/explore/topics/cassini_huygens/data_iss.html. I decided to post it now even though it's not done because I think MESSENGER may keep me too busy this week for me to do any more work on it for a bit.
--Emily
Folks, just a heads up that 3 new ISS DVDs are now available at the PDS, covering a data collection period period of April 1 - June 30, 2007:
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2031
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2032
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2033
Just glancing through the index tables, apart from the usual assortment of Titan flyby imagery, Saturn and rings, there are some nice higher resolution multispectral observations of Dione, Tethys, Rhea and Atlas (highest res imagery throughout the mission) and also lower resolution stuff on Mimas and Iapetus (Cassini's first good look at the trailing side), Enceladus low phase observations, couple of mutuals, etc.
Also, new VIMS data is here:
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/covims_0019/
As usual, Bjorn has created updates to the massive Cassini Image database for this latest release. For those of you who haven't seen it before, Bjorn made a Microsoft Access database containing all the metadata for all the images released by Cassini ISS to the Planetary Data System. This database is great because you can construct really quite complex queries and have it spit out lists of images that you might be interested in -- for instance, you could, if you wanted to, find all images that contain both Saturn and Titan that were taken through a RED filter, or find all images of Atlas with resolutions higher than 5 km/pixel, and so on. I use it to produce lists of files that I can then run wget on to automatically download only the images I'm interested in.
I have now created http://www.planetary.org/explore/topics/cassini_huygens/data_iss_database.html. Enjoy! And don't forget to check out the pages I made that show http://www.planetary.org/explore/topics/cassini_huygens/data_iss.html -- I haven't updated these pages yet with the April 1 release but I'll begin to work on that now that Bjorn's updated the database.
--Emily
It's amazing that Emily has put these pages together for all the main icy satellites. Nice that the images appear to be more directly usable without the need for 16-bit to 8-bit conversion (or at least my viewers are doing this more easily now). I also note the sub-spacecraft lat/lon that are useful in mapping. I wonder how these were obtained since when I browse the headers on the PDS web pages I usually just see the image center point lat/lon. I see these are listed in the more complete list of header definitions on Emily's page. Just FYI, I also like to use the sub solar lat/lon info for mapping. Kudos to Bjorn as well.
Steve
Here's the best icy moons and rocks stuff from the latest release. --Emily
http://www.planetary.org/data/cassini/u08q2icy/
http://www.planetary.org/data/cassini/u08q2rocks/
The ISS images for the July-September 2007 period have hit the PDS even though July 1 is several days away. I haven't had time to look at much yet but know there's a lot of interesting stuff there. The highlights I remember are:
* The only targeted Iapetus flyby
* A 5000 km nontargeted Rhea flyby
* A very nice flyby of Dione (~40,000 km IIRC)
* Lots of nice Tethys images
* Several Titan flybys
Ooh, nice catch, Bjorn. I was checking it myself earlier today and no luck. This is as fresh as it gets
Iapetus!!!! I can't believe it's been long enough since that flyby that the data is on the PDS already. I can't wait to see what you guys produce from that data set.
I'm looking forward to downloading stuff -- but probably can't get to it until this weekend. Bjorn, I'm ready for the database update whenever you get around to it.
--Emily
A taste of Iapetus data, from the Saturn system PR sequence before C/A. RGB color:
http://flickr.com/photos/ugordan/2611785538/
I forgot which star that was to the above right of Iapetus and also apparently another one off the sunlit crescent.
EDIT: Quick regional RGB color on the outbound part and one of the parting shots on the right at 2x:
http://i108.photobucket.com/albums/n15/ugordan/Iap_regional_rgb.jpg http://i108.photobucket.com/albums/n15/ugordan/parting_N1568715677_1.png
The dark stuff truly is remarkably gray on the trailing hemisphere. I'm now wondering whether my plan for redoing the big outbound mosaic in approx. natural color is worth the trouble just to get essentially b/w imagery in the end. There are still odd false color high-res mosaics here and there, though, that weren't released officially.
Ooh! An amuse bouche if I ever tasted one
--Emily
Another tidbit from the release: an approx. natural color ring scan of the left ansa, consisting of 5 NAC RGB segments. This was taken a couple of days (Sep 7 IIRC) before the Iapetus encounter and shows a similar vantage point. There's also the right ansa data at the PDS, but it doesn't show as much interesting stuff (Mimas, Pan and Prometheus).
http://flickr.com/photos/ugordan/2614029786/
I am wondering how can I decode PDS ".img" file on my mac. I have OS 10.5.3 and before, on my old pc, I have found a Gimp plugin to read .IMG files. Gimp 2.4 run on OS 10.5, but, the plugin is not compiled and I don't know how to do . This is for Gimp, but, I imagine that there are other solution .
Doug : you are on a mac, how do you do?
I use a PC
Seriously - I do - img2png on my desktop PC machine.
My MacBookPro is my 'life' machine (Email, calender, presentations, photos etc), my PC desktop is my 'power' machines (storage, PTGui, cold hard data, 3d rendering, Photoshop)
Doug
And now when I am at last ready to start large scale downloading Murphy's law strikes and I cannot access the PDS imaging node. I guess I'm not the only one...
Blerg. I can't access it either.
--Emily
I find that the PDS site is unavailable all too often. I'm not sure if it's a maintenance thing, but weekends usually seem to be iffy. Very annoying.
I just exchanged emails with some folks at the PDS. They know about the problem, has something to do with an expired something-or-other on a server so access isn't currently permitted; they hoped the problem would be resolved some time today.
--Emily
Looks like they need a mission extension as well.
You're just trying to make us jealous. Admit it.
The ISS volumes Coiss_2034, Coiss_2035, Coiss_2036 and Coiss_2037 are now available from PDS Planetary Rings Node in tar.gz form (convenient for downloading, even with a 4:1 compression ratio).
COISS_2034.tar.gz - 1208 MB
COISS_2035.tar.gz - 1026 MB
COISS_2036.tar.gz - 1117 MB
COISS_2037.tar.gz - 167 MB
http://pds-rings.seti.org/archives/
Still waiting for all the RADAR swaths to return.
Björn sent me these last week and I finally posted them: the Excel updates for the latest four volumes for his Access database to all Cassini images. Download from http://www.planetary.org/explore/topics/cassini_huygens/data_iss_database.html.
--Emily
After living with the browse pages I'd made for the Cassini PDS images, I decided I didn't like them, so I am trying out a new design, more like the one I did for the RAC pages. Please check out my new http://planetary.org/data/cassini/enceladus.html and let me know what you think; after a little input I'll go ahead and do these for the rest of the moons. (An example of my old design is http://planetary.org/data/cassini/enceladus/.)
To whet your appetite, here's some plumes from rev 50.
That looks brilliant Emily, a really useful resource I think. I know for a fact I haven't got the imaging skills or tech savvy to make any real practical use of it, but others here - and elsewhere - will, and they'll appreciate all your hard work and effort I'm sure. It is a lot neater and more easily navigable than v1.0. Great seeing all the plumes images in one place, really brings home just how fascinating and important a moon Enceladus is.
Agreed - and nine days until the next sub-50km flyby, featuring amongst other things, some close-ups of the plume vents
Sorry Emily, that came out wrong! I meant use it in the same way that our experts here - ugordan, james, etc - will use it, i.e. making elaborate mosaics and finely colour- and level-balanced images. I don't have the software, experience (or patience!) to create the masterpieces they do. But I will definitely be using it to make simpler RGB composites and to pull details out of images of plumes and surface features, for use in my Outreach talks, and have already started on a couple of images today for use in my astro soc meeting on Monday night...
I'm resurrecting this old thread to announce a new version of the database discussed earlier in the thread. All of the errors I mentioned there have been fixed and the database includes information for all of the ISS images released to the PDS so far (almost 200,000 images).
As earlier Emily has provided hosting for this big file (it's about 85 MB zipped). Further information is available here:
http://planetary.org/explore/topics/cassini_huygens/data_iss_database.html
I just noticed that the January 1, 2008 ISS PDS release is already there. What's more, there is now a compressed (GZ) file available for each volume. This is a very welcome addition - it reduces the amount of data to download and more importantly, download errors now manifest themselves as error messages during decompression. This is very important as I have discovered a few cases where files got corrupt during downloading without any error messages appearing during the download. Because of this I may even gradually redownload everything I have previously downloaded, this time as GZ files.
I haven't downloaded anything yet but now I know this weekend is going to be a 'download weekend' .
*Glub glub glub*
That's the sound of Emily drowning in data. I haven't even wrapped my mind around the last PDS release yet! Not that I'm complaining.
--Emily
Modern webservers do http://en.wikipedia.org/wiki/HTTP_compression, though the speedup may not be apparent.
This turned out to be a more interesting release than I had expected. Because of all of the recent Enceladus flybys in the extended mission I had managed to completely forget that this release includes the first targeted Enceladus flyby in 2008 (it occurred on March 12). The best images are in directory 1584035653_1584189857 on the coiss_2042 volume.
There are also interesting low phase images of Rhea from ~550,000 km where the phase angle drops down to 0.05 degrees. They are in directory 1579255943_1579280127 on the coiss_2041 volume. These are the best low phase Rhea observations so far and nicely reveal the opposition surge:
I would like to note that in the directory http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/ you can find new files (updated January 16) with name xxxxx_MD5.txt. Cryptographic hash function MD5 is commonly used to check the integrity of files, now each Cassini's file is in MD5 expressed as a 32 digit hexadecimal number.
example:
b41fdfd79ca9eb873f86f9e910a66be7 coiss_2001/data/1454725799_1455008789/N1454738788_1.LBL
70d3903a26f05673022d98de4cf53dc3 coiss_2001/data/1454725799_1455008789/N1454725799_1.IMG
4b2321a08362f019afa50915faed31e8 coiss_2001/data/1454725799_1455008789/N1454738788_1.IMG
9b8e12e3469407daa881168233c5c95a coiss_2001/data/1454725799_1455008789/N1454725799_1.LBL
07d2bf79db8a5939f3361c260c3b9794 coiss_2001/data/1454725799_1455008789/N1454745007_1.IMG
53e278ab66c32d87a11c7b7c37e14074 coiss_2001/data/1454725799_1455008789/N1454726579_1.IMG
792848149f521c6d57fdb65a27a7f5a3 coiss_2001/data/1454725799_1455008789/N1454745007_1.LBL
82171afd4c7bcbaa11c4e27be835d3bf coiss_2001/data/1454725799_1455008789/N1454726579_1.LBL
9e785eda0deb16860f07c758aefc17fd coiss_2001/data/1454725799_1455008789/N1454745055_1.IMG
368bc03dc3aef22914d308a44160ea65 coiss_2001/data/1454725799_1455008789/N1454727359_1.IMG
...it's apparently been available since March 18 or so but I got the email from the PDS today. As before, there are now tarred and zipped archives available for all the images. Seems to be a lot of ring movies in there, spoke formation stuff -- are there any exciting moon encounters in this batch?
--Emily
There are a few nontargeted icy satellite flybys but no targeted ones. The most interesting satellite images are great views of Tethys' Ithaca Chasma from ~180,000 km. There are some decent views of Mimas and Enceladus from ~200,000 km and Rhea from ~350,000 km. I haven't checked if there are interesting images of the small 'rocks' yet.
FWIW I don't think these images became available until right at the end of March (I checked every day in the last week of March ).
BTW the images of Tethys I mentioned are in directory data\1588868011_1589091244 on volume coiss_2044.
I should also mention that this release includes some highly spectacular images of Saturn's northern hemisphere. A good example is some of the images in the directory that precedes the one mentioned above.
What's more, the http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_0011_v2/ has been released, although it's still being reviewed.
Looks like it's time to go back to the software and check/refine the calibration procedure with new info...
This is great news - I didn't notice this volume. Now I also need to check my calibration code. Actually it would probably a good idea to compare our calibration results to get rid of possible bugs.
The email from the PDS had this to say about the calibration updates:
Cassini images covering the period from October 1 to December 31, 2008 were released by the PDS three days ago. I havent looked at everything yet but I took a quick look at all of the icy satellite images plus the almost 1000 images of Titan. There is a lot of interesting icy satellite images this time, especially Enceladus with two targeted flybys. The highlights:
105 images of Mimas.
Beautiful Mimas/Prometheus mutual event (directory coiss_2049/data/1603163051_1603326763)
Mimas from approximately ~180,000 km (directory coiss_2049/data/1603527465_1603553855)
599 images of Enceladus.
Targeted flyby of Enceladus on 2008-10-09 (directory coiss_2049/data/1602219901_1602277473)
Targeted flyby of Enceladus on 2008-10-31 (directory coiss_2049/data/1604111692_1604168387)
Enceladus on 2008-12-02 from ~125,000 km (directory coiss_2050/data/1606797017_1607025755)
Enceladus plume images on 2008-12-26 from ~760,000 km (directory coiss_2051/data/1608970573_1609104344)
113 images of Tethys.
Tethys on 2008-10-10 from ~400,000 km with Ithaca Chasma visible (directory coiss_2049/data/1602277538_1602387820)
Hi-res images of Tethys on 2008-11-24 from ~60,000 km (directory coiss_2050/data/1606210264_1606378271)
Tethys on 2008-12-09 from ~250,000 km (directory coiss_2050/data/1607482567_1607567228)
43 images of Dione.
136 images of Rhea.
Low-phase Rhea on 2008-10-05 from ~850,000 km (directory coiss_2049/data/1601659146_1601870393)
Rhea on 2008-11-01 from ~480,000 km, phase ~85° (directory coiss_2049/data/1604264777_1604402429)
880 images of Titan.
In many case there are images in the directories preceding and following the ones listed here.
Cassini images covering the period from January 1 to March 31, 2009 were released by the PDS.
http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/ (coiss_2052 and coiss_2053)
Nontargeted flyby of RHEA on 2009-02-02 (directory
http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2052/data/1612149251_1612261808/ and
http://pds-imaging.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_2052/data/1612261825_1612297448/ )
I'm resurrecting this thread again - updates to the Cassini image database from the past several PDS image releases have been posted at the same URL as before (thanks to Emily / The Planetary Society for hosting this):
http://planetary.org/explore/topics/cassini_huygens/data_iss_database.html
There's further information there, including information on how to import the updates. The updates are Excel files. In short, unzip the updates, open the database in Access, and then do File > Get External Data > Import to import the XLS file just unzipped. Accept the default options, and then, when asked "Where would you like to store your data?" choose the table "coiss" in the list that appears next to "In an Existing Table."
A Cassini data release occurred a few days ago. This release is somewhat unusual as there are absolutely no interesting icy satellite images. However, there are several targeted and nontargeted Titan flybys plus lots and lots of interesting ring images. With equinox approaching (August 2009; this release covers April-June 2009) the focus was on the rings. I have now looked at all of the coiss_2054 images; there are lots of images showing satellite shadows on the rings and some images showing shadows cast by features in the rings themselves. There are also various movies, including F ring movies. The most interesting directories in my opinion:
coiss_2054\data\1617917998_1618066143 : Shadows cast by features at the edge of a gap.
coiss_2054\data\1621652147_1621937939 : The outer edge of the A ring showing Daphnis with shadows of ring features visible at the inner edge of the Keeler gap.
coiss_2054\data\1621957143_1621968573 : Movie: The outer edge of the A ring, shadows from a disturbance are visible when Daphnis passes by. Propeller feature near the outer edge of the Encke gap.
coiss_2055 might be even more interesting since at covers a period closer to equinox but I have yet to take a detailed look at it.
I'm waiting to take a look at these until I can access the volumes through the OPUS search tool at the Rings node; I understand they have to receive copies of the volumes on DVD-ROM from the Imaging Node first (how archaic!) but they should be available there within a week or two.
..delivered by a guy driving an AMC Gremlin and listening to his 8-track player.
I have now also taken a quick look at all of the images in the coiss_2055 volume and as I suspected they are even more interesting than the coiss_2054 images. I can hardly wait for the next release which covers the equinox ring imaging.
The highlights in my opinion are in these directories:
coiss_2055\data\1622711732_1623166344 and coiss_2055\data\1623166377_1623224391 :
Great images of Daphnis, the Keeler gap and shadows cast by features at the edges of the gap.
coiss_2055\data\1624654802_1624836470 and coiss_2055\data\1624836945_1625069379 :
Beautiful Daphnis/Keeler gap images showing ring feature shadows @820,000 km.
Two examples from the the many ring images. Calibrated, cropped and slightly sharpened images:
The database update for the April 1, 2010 ISS PDS release has been posted on the database page at the TPS website:
http://planetary.org/explore/topics/cassini_huygens/data_iss_database.html
(you need to scroll down a bit to find the two relevant files for the April 1, 2010 release)
I forgot to 'announce' this here until now - database updates for the October 1, 2010 and January 1, 2011 data releases were recently posted at http://www.planetary.org/explore/topics/cassini_huygens/data_iss_database.html
The Cassini images for the period April 1 to June 30, 2010 were recently released at the PDS. This release contains *lots* of interesting satellite images, including beautiful closeups of Enceladus' plumes. There are 2 images of Mimas, 227 of Enceladus, 2 of Tethys, 181 of Dione, 13 of Rhea, 2 of Hyperion, 1114 of Titan and 170 images of Iapetus.
This is a quick and dirty false color composite of Enceladus from IR3, GRN and UV3 images obtained on May 18, 2010 at a range of 45,000. It is centered near latitude 0° and longitude 310°. It has been processed to reveal compositional differences:
Nice!
"There are 2 images of Mimas, 227 of Enceladus, 2 of Tethys, 181 of Dione, 13 of Rhea, 2 of Hyperion, 1114 of Titan and 170 images of Iapetus."
And 4 images of Janus, and some of Epimetheus and Pandora .
Two images, second one is Janus in false colors (ir3+grn+uv3 filters), 1.5× magnified, first one is hi-res image of Dione, colorised from lower resolution images
(again ir+grn+uv filters, but notably manually corrected, so it's very artistic interpretation ).
Image of Dione is without detailed information in index tab. So I tried excerpt some information about it.
This image covers small area in Eurotes Chasmata and big crater (at top of the image) has coordinates approx. latitude -24S, longitude 323W.
Horizontal resolution is ~14 m/pix, vertical is much lower. Highest cliffs are more than 1 km height.
Great images, especially the one of Dione which shows a real landscape at this resolution, overall with an alien appearance but there are some features that look a bit similar to terrestrial landscapes.
And regarding Dione, I now see that there are more images of it than I thought. I found the Dione images using a database search with target='DIONE' but for these images Saturn is the target for some reason (and the viewing geometry applies to Saturn) but the target description is 'DIONE' and the target list includes Dione. Weird - and I obviously need to modify my database queries.
By the way I decided to replace the image in the starting message of this thread with a significantly improved version. I discovered that I had forgotten to rotate it so that south was originally up (north is up in the new version). Perhaps more importantly, I have now aligned the color channels much more carefully.
This is getting a bit embarassing, I had to replace the image again because I discovered that the original version really *was* correctly oriented (I forgot to check a "north azimuth" orientation box in the rendering software). Everything should be correct now but if anyone notices any errors please let me know!
I need to do some comprehensive testing to determine which query guarantees that you get every image you are looking for (assuming the metadata contains no errors) but this might work:
SELECT *
FROM coiss
WHERE coiss.TARGET_NAME='MIMAS' Or coiss.TARGET_DESC='MIMAS'
In addition it might be necessary to check whether the target_list contains the string 'MIMAS'.
The challenging thing is that I usually limit my searches by TARGET_DISTANCE in order to get only images that have more than, say, 100 pixels across the disk -- but that doesn't work, sadly, if MIMAS is not the TARGET. With a little trigonometry though, at least for the inner moons, you could at least limit it by the CENTRAL_BODY_DISTANCE (no greater than Mimas' orbital radius plus whatever distance to Mimas you're looking for) to weed out spurious hits where MIMAS is in the TARGET_LIST but is only a speck.
http://ringsnodesearchtool.blogspot.com/2011/04/new-cassini-iss-volumes-coiss2062-and.html:
http://pds-rings.seti.org/search/results/#volumeid=COISS_2062
http://pds-rings.seti.org/search/results/#volumeid=COISS_2063
The database updates for the April 1, 2011 data release (which covers the period from April 1, 2010 to June 30, 2010) are now available at http://www.planetary.org/explore/topics/cassini_huygens/data_iss_database.html
There are lots of interesting satellite images (especially of Enceladus and Dione) in this most recent data release.
A new version of the entire ISS image database is now available here:
http://planetary.org/explore/topics/cassini_huygens/data_iss_database.html
It includes data up to and including the most recent PDS release on October 1, 2011. The entire database was updated instead of posting smaller files containing the latest PDS releases because several recent ISS volumes had errors in the INDEX.TAB files - the subspacecraft longitude was off by 180 degrees. This has now been corrected and the database contains information from the updated and corrected INDEX.TAB files.
I strongly recommend replacing older versions of the database with this one (if you have created any queries you want to keep you should copy them from the old database to the new one before deleting the old one).
The following item was published in the most recent Planetary Exploration Newsletter:
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