The T21 Mission Description document is now online (http://saturn.jpl.nasa.gov/multimedia/products/pdfs/20061212_titan_mission_description.pdf).
More SAR coming up!
Emily
What's with this "XXX not available for Titan-21" stuff? Seems like less and less effort is put into these flyby descriptions, as it is now only a single page or so of new information is present per flyby. The rest is pretty much copy-paste stuff.
Also, as edstrick pointed out, it would have really been nice to also include science plans for the periapsis passes, at least listing what targets and instruments will be used.
This is one of the few, decent trailing hemisphere passes of the mission for RADAR. It is a short pass, but should be good enough to understand the geometry of the dunes in northern Belet so we can compared those seen on T8.
In addition to Titan, be on the look for images of Pan (from around 750,000 km) and gibbous Dione from 300,000 km centered around 30 N, 135 W.
Titan images are down. Some clouds visible:
http://saturn.jpl.nasa.gov/multimedia/images/raw/raw-images-details.cfm?feiImageID=92452
some more clouds:
http://saturn.jpl.nasa.gov/multimedia/images/raw/raw-images-details.cfm?feiImageID=92502
they also show up very nicely in the recent VIMS/Radar release.
These aren't in the VIMS/RADAR release. these images were taken yesterday.
I was talking about the mid-latitude clouds in more general terms. They are more pronounced in the VIMS/Radar release.
( my understanding of computer image processing is rather limited, so if this is really dum, or is already being done and I didn't notice, please be gentle )
For areas of Titan where we have both high resolution NA camera images and SAR data, could a mathematical correlation of the differences between the 2 data sets be generated, and then be applied to areas of Titan where we only have the NA camera data or only the SAR data to generate the other for both areas?
I think it isn't possible, but I am clueless as to why.
I assume the radar didn't reveal anything news worthy this time around?
Whoa, hold your horses... Not even a week has passed after the flyby + it's weekend now. No point in rushing things!
"For areas of Titan where we have both high resolution NA camera images and SAR data, could a mathematical correlation of the differences between the 2 data sets be generated, and then be applied to areas of Titan where we only have the NA camera data or only the SAR data to generate the other for both areas?"
That works when the two datasets are well correlated and can work nearly perfectly if one dataset can be mapped onto another dataset by a simple one-for-one function. It doesn't have to be linear or a simple curve or anything. You just need a unique Y value for each unique X value.
In multispectal data, we've done that with rover color images with datablocks missing. If a green data chunk is AWOL, a weighted average of the red and blue channels is a good visual match, but close inspection will show the only colors in the "fudged" part of an image are varying shades and intensities of orangy red through gray through greenish blue.. No yellows or greens, where the real data would be brighter than the average, no purples, where the real data would be darker than the average.
With something like VIMS and radar data, it's essentially impossible. Though you can match up features in the two datasets, actual data values have essentially no correlation and there's no possible "reasonally good" mapping from one dataset to the other. They are truely telling you two essentially independent, different things about the same surface.
An analogy is a red and green checkerboard. a 512 channel imaging spectrometer won't tell you anything more about the red and green squares than a single well selected channel. But pick thermal infrared or millimeter waves, and you might not see the checkerboard at all, but the fiber structure of the particle-board or masonite underneath the paint formnig the red and green squares.
I appreciate the response, that was very helpful.
?? How would they know a cryovolcano was active from RADAR?
Interesting question, volcanopele.
How would materials in motion, like, let's say a rapidly ascending volcanic plume, interact with the radar beam and the mathematical reconstruction needed for us to see the image?
Seems like the doppler component of the signals would be distorted in a characteristic way, but does the SAR radar technique look for such characteristics in the returning signals?
moving cryolava flows would be a hint
I think a waterfall (methanefall) would be a lot harder to determine
Is the sar from T21 another one of those full swaths?
Does anyone know when SAR results will be released? I hope the delay is due to seasonal holidays rather than any problems with the observations?
T21 was a half-swath, UVIS had prime point prior to C/A, RADAR afterward.
not sure why some of it hasn't been released yet.
I think things just got too busy over the holidays, and now everyone's facing the LPSC abstract deadline on January 9. I'm hoping to see something after that.
--Emily
http://photojournal.jpl.nasa.gov/catalog/PIA09111
Wow, they really look like a work of art.
Yeah, baby! This goes right over some of the Tiger Stripes north of the Dancing Monkey feature!
They look like broad darker gray lines bordered by subparallel sl. brighter gray lines in RADAR. I'm guessing it was a wide crack bordered by sharp ridges later buried under a bunch of atmospheric schizzle. Not big channels. (Or maybe big channels buried by schizzle)
Awesome!
-Mike
Wow indeed. I wonder how much we can deduce about topographic wind effects (in fact, topography itself) from this sort of data?
I'm not quite sure how to read topography out of these radar images: when you have parallel light and dark lines, does the lighter line represent the crest of the dune, and the dark line the trough, or vice versa? Or is the light line one side of the dune and the dark side the other?
Whoa! That is one of the more enigmatic radar images I've seen so far. Those features seem way to fine and linear for wind or water... perhaps these are some form of expansion faults in the surface that became further eroded?
What do I know, since it's clear I'm not keeping up with planetary geology terms... "covered in schizzle"?!?!?
<airplane> Excuse me, but does anyone present speak Jive? </airplane>
Watch it bub, or I'll get hummocky on your euphemisms!
OK. I'm not totally satisfied with this but...
I tried to stitch together the T30 RADAR Swath and the T21 RADAR Swath at their intersection point. I think the lines at the far end of the T30 RADAR Swath are the Tiger Stripes of Titan and I tried to match them up where they cross the T21 Tiger Stripes. (The two swaths should intersect)
I'm not super sure I got the line up exactly right, but I think I'm close. There are not a lot of obvious features in the region to help line things up ("Wecome to the Big Bland"). Maybe one of the imagemeisters in UMSF-land can take a better stab at this.
You should be careful about calling these "tiger stripes". That nickname has become so ingrained in the community to refer to the cryovolcanic-tectonic structures in Enceladus' south polar region, that calling these features "tiger stripes" may lead people to think that these features are similar. True, these do have a superficial similarity, but quite frankly, we are not sure how these formed, though they do seem to be tectonic in origin. How about..."Zebra Stripes"?
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