Here is a combination of all of Galileo's global color views of the Galileans. I have left out the large Europa mosaic because much of its color data is pulled from other orbits. I have also left out colorized views. Due to inconsistent filter selection, there some variation between images. I posted the Europa set in another thread, but I figured I would add the views of Ganymede and Callisto.
Galileo imagery?
http://apod.nasa.gov/apod/ap960830.html
Great work Ted, thanks for the new wallpaper.
...wow, Ted! Thank you; that's an incredible montage. In particular, Ganymede looks more interesting then I've ever seen it before.
Watch out, though; you forgot to include Io among the Galilean moons, so VP's gonna be torqued...
Actually, I didn't forget....There are so many Io images that I haven't gotten to all of them yet. Here are a few I have processed. (I should mention that the third image is two color (violet/IR), which is why it looks a little off compared to the other images. I am working on trying to formulate a better "synthetic green."
This one is actually from Voyager, showing Europa's night side.
This seems like the right place to mention that Emily has posted an excellent http://www.planetary.org/blog/article/00001264/ of Ted's work on her blog, to mark the inclusion of his wonderful Gallileo images of the Galileans on the Planetary Society's web site.
A question for Emily: When you refer to your "image database," I think you mean something more voluminous than the "space topic" write-ups for each planet, but I'm not sure where on the site to find these images.
TTT
Congrats, Ted; Emily's made you an international star! Well done & well deserved.
TTT -- I probably shouldn't refer to my image database in blog entries -- I mean the internal planetary.org image database that is used to populate our website with pictures. I'm proud of it because when we redesigned our website late in 2005 it's one of the things I demanded -- an image library where we can upload one copy of an image, with caption and credit, and it auomatically produces the three browse sizes we use, and spits out the formatted html code for our pages, and we never lose the files or have to rewrite captions, something we used to do regularly before the redesign. I suppose in a future redesign we ought to make this publicly searchable but, I'm very sorry to say, the idea didn't occur to me when we were doing the redesign.
--Emily
That is a really cool feature. By the way Emily, I really like the description of the kind of work I do (the explanation of the difference between what I do and what scientists do - at least most of the time (you will understand in a month or two)). In trying to portray what an object in space looks like, there are often trade-offs. Planetary objects don't have big gores in the side of them and discolored sections where one or two filters didn't cover. So, for the sake of producing a nice picture, creating convincing gapfill is important. However, if such images were used for science, such methods could lead some unfortunate person to think that they had discovered a truly different region. I will admit that I am MUCH more pliable with what I am willing to do with Galileo images than with other probes, as its coverage is so spotty. Where I draw the line is cloning over gaps with fictional features or features from another region - I always use actual images of the missing region or a gray fill that is roughly keyed to the surrounding albedo features. I realize, however, that those folks who produce maps for renderings to be viewed at any angle really don't have a choice but to clone missing regions.
For Galileo, I have even tried to play around with some of the better Opnavs. Sometimes there is a rotation sequence as Galileo approached a moon (usually Ganymede) which allows one to build up. Here is Ganymede on orbit J0 (after insertion and approaching the G1 encounter).
I have re-reworked the closer I32 global view, and in the process I noticed something - you can see the planetshine - lit hemisphere. I know there are plenty of images showing this in much more detail, but I was mainly taken by the fact that I had worked with this dataset so much and never noticed this. The reason is probably that I was focused on making the image black in all areas off the limb except for the faint plume on the upper right. However, due to glow from the daylit hemisphere, the background is actually brighter than the planetshine on the right side of the image, so I probably destroyed it in earlier versions. I wiped out color in the planetshine area because it was not picked up in all filters, making for a very odd appearance. The first image is my new "regular" version, the second is with the planetshine area enhanced.
Here's a special image of the Jovian moons:
http://sohowww.nascom.nasa.gov/pickoftheweek/old/27mar2009/
Why did you think that this fit in a Galileo imagery thread?
nice!
but Galileo image compression almost always wiped out any subtle details in any jupiter-shine imaging. wahhh!
Having seen what Cassini has done at Saturn I'm becoming surprised there aren't any really nice Jupitershine images of the Galileans (especially Io's Jupiter facing hemisphere). This shouldn't have been very difficult since Jupiter is much brighter than Saturn. Of course the downlink was severely limited but despite this I'm a bit surprised.
It's a shame its going to be at least 30 odd years before we ever get a good look at Jupiter again.
I expect the other things visible in sunlight were much higher priority than any potential earthshine images.
Yes, Cassini has 12 bit A/D converters and although it typically encodes images using an 8 bit lookup table, it's still able to capture the greater dynamic range 12 bit images produce, albeit with only 256 discrete levels.
I don't think Galileo having an 8 bit dynamic range to begin with gives you much to work with if the exposures are set for sunlit surfaces. Maybe some detail could be pulled out from higher phase sunlit surfaces since those inherently use longer exposures for rocky surfaces, otherwise the brightness difference is too great.
This is true and even long exposures might have been a problem due to scattered light unless the phase was relatively high. What I had in mind was something similar to Cassini's images of Iapetus (these are the best known Saturnshine images) of Io's subjovian hemisphere. The reason is that Galileo only obtained relatively low resolution images of this hemisphere. But possibly the flyby geometry was never suitable for this - it's probably time to get some SPICE kernels and start digesting them.
Cassini at Iapetus was moving very slowly, but Galileo at Io was moving very fast, so motion blur was a problem and compensation more difficult. And the long exposure would result in really bad radiation effects on the image.
Phil
True, but Io also receives much more jupitershine being much closer to Jupiter (which in turn receives more sunlight) than Iapetus is to Saturn so that tends to cancel out greater flyby speeds somewhat.
In these images, compression was not the worst problem. It was a horrible amount of noise.
Actually there are a few low-resolution, global, Galileo images of Io's nightside in Jupiter shine, taken to look for condensing frosts. See Simonelli et al. 1998, Galileo Search for SO2-Frost Condensation on Io's Nightside, Icarus 135, 166-174. These are from that paper:
Here is another nice view from Galileo, taken during the E15 orbit.
Beautiful images! Io is really very photogenic object.
Here are some images from beginning of Galileo mission.
False colour? really? I've stretched the saturation to the max in Photoshop on that image, and there's no colour at all, just a slight orange tinge across the entire image.
Since the original mosaic was monochrome, any colour is false! Looks good, though - probably fairly realistic.
Phil
I believe machi is using false colour to mean artifical colour, not spectral imaging that uses combinations of wavelengths that do not approximate what is seen by the human eye.
Full inline quote removed - ADMIN
Right. This is maybe little terminological problem. Color is entirely artificial. How Phil said, for this mosaic multispectral images don't exist.
For comparison, this is multispectral image maked from violet, green and IR images.
A more appropriate phrase would have been 'colourised' rather than 'false colour'. 'false colour' infers that you made the image from multiple filters.
As Jason Perry http://gishbar.blogspot.com/2009/10/galileos-i24-flyby-of-io-look-back_11.html a couple months back over at the Gish Bar Times, we have recently passed the tenth anniversary of Galileo's I24 flyby, that probe's first close-up look at Io. However, many of the images collected during the flyby had at least one of two anomalies, which the team later characterized http://pds-imaging.jpl.nasa.gov/data/go-j_jsa-ssi-4-redr-v1.0/go_0022/document/ai8doc.htm. They were able to create an algorithm to correct the first and simpler of the two anomalies, but were unable to correct the second anomaly. Thus, about a dozen close-in images of Io have been lost. I made an initial attempt at correcting the second anomaly for the example image used in the characterization document, but, although it makes for an interesting exercise in image processing, it's completely useless in its current form for anything resembling scientific analysis...
original:
Impressive!
By the way, I don't think I ever have seen the documentation for the second anomaly. Very interesting!
I posted a short Europa-related blog entry yesterday.
http://planetimages.blogspot.com/2009/12/nice-little-view-of-europa.html
Here are two rough color views from Galileo. Valhalla impact basin on Callisto:
http://www.flickr.com/photos/ugordan/4187936017/
Ganymede mosaic consisting of 4 footprints:
http://www.flickr.com/photos/ugordan/4248059931/
That's the http://photojournal.jpl.nasa.gov/catalog/PIA01610 crater chain at lower right. There exists a fifth footprint that I *think* fits to the lower left one, but there's no overlap to match them and I omitted it here.
What a difference rotating an image can make:
Amazing! I'm not geologist, but I have seen this image many times (in raw form) and now it looks really more understandable to me. Fantastic cliff!
Let's Look at Io from a Different Angle!
or a slightly different take, simulating the view one might have out of a porthole on passing space cruiser . . .
On a related note, look at what made it onto Wikipedia's front page today!
http://en.wikipedia.org/wiki/Callisto_%28moon%29
Rather a coincidence considering the recent blog post by Emily.....
I had this on my blog a few days ago, but I've gotten around to putting together a few mosaics of Europa from 1998 and 1999 by Galileo:
Those are just mind-blowing, Jason.
I never knew that there were features like that on Io...(sorry, couldn't resist! )
Shamelessly stealing volcanopele's http://pirlwww.lpl.arizona.edu/~perry/io_images/c10.htm Io image and running it through CIE XYZ color calculation code based on Galileo's filter wavelengths (R 665, G 559 and V 413 nm):
http://i108.photobucket.com/albums/n15/ugordan/10ISIOGLOC03.png
It's also gamma-corrected (assuming the original composite is straight-up RGB substitution, judging by contrast and terminator line). Io's one of the few moons that doesn't really look bland this way.
Oh wow Gold!
I thought that this one was the correct color and gamma
and have been planing on redoing the color on my map ( i white balanced it )
{ http://celestiamotherlode.net/catalog/show_addon_details.php?addon_id=1110 }
[attachment=22188:21ISCOLOR_01.jpg]
http://pirlwww.lpl.arizona.edu/~perry/io_images/c21.htm
http://pirlwww.lpl.arizona.edu/~perry/io_images/21ISCOLOR_01.png
Really brilliant work here, much appreciated...
color ???? "that is the question " when i did my map i did what i would do in the photo darkroom and balanced for white - then tweeked it for ascetics .I always thought that there was too much green in them
and used the
http://pdsimg.jpl.nasa.gov/data/cassini/cassini_orbiter/coiss_3002/data/images/SE_500K_0_0_SIMP.IMG
the eastern half
[attachment=22189:tx_1_0.jpg]
Wow, yeah, that is WAYYYY too red and dark.
Bjorn has a decent tutorial on Io's color at http://www.mmedia.is/bjj/3dtest/io/index.html .
Another true color approximation that is quite good is at http://photojournal.jpl.nasa.gov/catalog/PIA02308
I'm not confusing anything. Not only is the monitor not as bright, the darkest blacks aren't all that dark. As for the two Phoenix images, yes, I am saying that. One is faithful to the brightness of the reflection, one suppresses it in the name of preserving more interesting parts of the image.
My non technical argument would be that we use monitors to view every day photographs and video (of ordinary subjects) and the images look correct and "as it should be".
So if we replicate the same processing that our normal digital cameras do and apply it to raw image data, the results should in practice be the same as is if the images were originally taken with that camera.
As for the Phoenix image posted, I'm forced to say that the right version does look like a normal digital photo taken on Earth. Therefore, it's as real as any photo viewed on a PC screen. But this is just my opinion of course.
But more technically speaking, the left Phoenix image is NOT faithful to image reflexion values unless you forced your monitor to display also with a linear response!
If the monitor is sRGB, it will apply gamma to that image, resulting in a non-linear display. So the right version has the correct linear response.
My biggest issue at this point seems to be that the way my images look in Photoshop CS4 looks quite a bit different when displayed in a browser. In Photoshop, the display looks non-linear, with my image not washed out by any stretch of the imagination, but the terminator region is quite as dark as my images appear in a browser.
So I would like to find a way to make the images that I make in photoshop show up the exact same way in a browser (even on the same computer).
hmm, that doesn't seem to work, but then again, Firefox has always been a bit odd for a while in the way it handles color.
I'll give you a good example. Compare the thumbnail version of 10ISIOGLOC03 on http://pirlwww.lpl.arizona.edu/~perry/io_images/c10.htm with the full size version at http://pirlwww.lpl.arizona.edu/~perry/io_images/10ISIOGLOC03.png . On my browser, I like the way the thumbnail looks because it looks exactly the same way in Photoshop, and that is how I prefer it to appear. But in the full-size version, the terminator is way too dark.
And converting to a different profile (or using JPEG rather than PNG) didn't seem to work.
Hmm. I'm stuck with a laptop right now with lousy contrast so can't make out any differences in the way the terminator appears, though the thumbnail image does seem to appear slightly more greenish compared to the full res. It could be the two have different embedded profiles. Do you generate both in Photoshop or?
I think there was a thread somewhere here about browser issues with color profiles, maybe one of the images is stuck with a profile (even though it's sRGB and FF can't handle it properly or something) instead of bare data.
Edit: yeah, I can see the difference in Photoshop if I resize the thumbnail. When opening the JPG thumbnail it says there's no embedded profile, but when opening the full PNG it says nothing.
oops i posted the wrong link
-- i am going to have to check the README i made an make sure it is correct - gives the correct reference to the orig.
http://astrogeology.usgs.gov/Projects/JupiterSatellites/io/Io_SSI-only_color_merge_SIMP0.cub.gz
http://astrogeology.usgs.gov/Projects/JupiterSatellites/io.html
the 3 band isis cub file
ran "explode" on it then exported each to tiff( gdal) and recombined R,G,B in Nip2
then in gimp cleaned the seams ( that is normal for me - i dislike seams )
the old colors of io , i think have to much green and a bit to much yellow
then AFTER i did the map i came across this
http://pirlwww.lpl.arizona.edu/~perry/io_images/c21.htm
i do need to lighten it up and add back in some of the yellow
Regarding image color profiles and the Web:
My personal opinion is to disable any color corrections in Photoshop and if really needed always specify sRGB for saved files.
What you should correct is your monitor or graphics board (sometimes the only option for laptops) using the sliders normally present on the control panel. These are hardware adjustments and will bet you correct display for everything.
Forcing color space correction on browser or on a program basis is always inconsistent. Here's a nice link about color profiles with interactive examples : http://www.gballard.net/psd/go_live_page_profile/embeddedJPEGprofiles.html
well there is
AdobeRGB1998.icc
HP5000_UVDuraImageGlossMaxQ.icc
sRGB.icm
on my system and i have everything set to sRGB.icm
pick one and calibrate EVERYTHING to it
printer , monitor , photoshop, gimp, Firefox ,( IE 8 ??? ) do not about that one
Perhaps this digression should be extracted into a different thread instead of contaminating this (unrelated) one?
An 8-footprint, roughly natural color Galileo mosaic of crescent Jupiter, taken on September 10th, 1997:
http://www.flickr.com/photos/ugordan/4942095653/
There's also a contrast-enhanced version http://farm5.static.flickr.com/4077/4942699784_dc89893e1a_o.png for those so inclined.
Nice. I have a http://planetimages.blogspot.com/2009/09/despite-its-antenna-problems-galileo.html about that data set that I posted last year.
Little animation experiment with two Jupiter's images from Galileo.
Darkening at right side is caused by rotation of Jupiter between time
when these two images were taken.
http://www.youtube.com/watch?v=IqKwWB8xKHg
Wow...
When doing these morphed animations, are you using Sqirlz Morph (that you discussed http://www.unmannedspaceflight.com/index.php?showtopic=4550&view=findpost&p=166265) or the MSU Frame Rate Conversion Filter (discussed by Ian R http://www.unmannedspaceflight.com/index.php?showtopic=6705&view=findpost&p=166494) or both, depending on the scene and number of frames?
I've been experimenting with the MSU stuff and it works very well for the Voyager 1 Jupiter approach movie (one exception: I need to cut away a few frames at the start of the tweened animation file to avoid 'jumps' in the cloud motion). In contrast, it does not work well for a Cassini animation of Saturn where the time between frames varies a lot and where I sometimes need to interpolate between two adjacent frames before assemling everything into one big tweened animation. I suspect in the Saturn case Sqirlz Morph is the way to go.
Normally I'm using Sqirlz Morph, because of big differences between used images.
I think, that MSU Frame Rate Conversion Filter is usable only for small differences.
Sqirlz M. is usable nearly every time (if images contains enough corresponding details),
but it's time consuming process for every pair of input images.
Cross-eye 3D view of 11 km high Tohil Montes and Radegast Patera (dark lava lake).
Resolution is approx. 150 m/pix. Color from lower resolution images from orbit C21 observations.
BTW, Radegast Patera has almost same diameter as Endeavour crater.
that is very cool, Machi!!
That's gotta be the most dramatic view of Europa that I've seen. Very nice.
Yeah, you won't find topography like that on Europa.
Unless it's Europa in Philovision.
Phil
It's my fault, I forgot "Ionian" before Tohil, which is btw correctly Tohil Mons (mountain), not Tohil Montes (mountains), but I still think, that Montes would be more appropriate for such complex structure.
Now, more stereoscopic images (BW and color anaglyphs + enhanced cross eye version) of Ionian Tohil Mons and Radegast Patera are available on my http://my-favourite-universe.blogspot.com/2011/08/vysoke-stity-ionske.html.
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