When taking a look at some of the Voyager images of Jupiter I noticed something interesting in Voyager 1 image C1638201.IMQ - possible cloud shadows. I haven't seen them before on Jupiter in any spacecraft images. Here is a flat fielded, cleaned up and contrast stretched version of C1638201.IMQ:
Would that 3D process work on those images? Seems like if the shading was shadows, the software might do something, but IIRC, the software was designed for a solid surface, not a cloudscape . . .
Sorry, it's late and I am not sharp enough right now to find the right thread with the info.
Wow - that's neat. Certainly looks like just the tops are reaching a level where they glaciate. What are the clouds made of at that level?
P
One of the best images of Jupiter from Voyager 1. Resolution is 2.65 km/pix.
In this image are very interesting clouds, they looks like flying icebergs.
"Would that 3D process work on those images? Seems like if the shading was shadows, the software might do something, but IIRC, the software was designed for a solid surface, not a cloudscape . . ."
The software doesn't know what the surface is made of. Shape from shading certainly could do something with the clouds that show shadows. The varying shades among the background clouds may create artifacts, but albedo markings do that on solid surfaces as well.
Phil
I'm reviving this old thread because the Juno images have made it rather interesting. Many of the JunoCam images show cloud shadows and elevation differences but in the Voyager images cloud shadows are rare. Here are two more high resolution Voyager 1 images that are interesting when one has seen the Juno images. First narrow angle image C1638155. It has been enhanced and sharpened a bit:
Very interesting; good work as usual!. The effect is certainly close to the threshold of detectability, but I think it's real. I suppose the competing, non-shadow interpretation would be that albedo features happen to place darker features on the anti-sun side of some brighter albedo features. It's hard to refute that with certainty; by definition, the brightest regions in an image will be surrounded by darker regions on all sides. The strength of the shadow interpretation would depend upon the candidate shadows being darker than the regions on the opposite, closer-to-subsolar side of the bright regions.
That applies here, but the margins are certainly tight, often just one pixel showing the darkness.
A real clincher would be if we had images of similar or identical regions ~4 hours apart, with the direction of illumination roughly reversed, and we saw the candidate shadows switch sides. Voyager's trajectory could never provide that sort of imagery because both Voyagers flew past the sunset boundary and were never close to having a favorable view of the sunrise boundary. Ditto for Cassini. And of course, Galileo had to skip a lot of imaging opportunities. So this is one particular investigation that Juno permits for the first time. Although I'd be very, very surprised if these Voyager images weren't showing shadows.
Post #1 in this thread is pretty impressive in its showing of shadows from Voyager. The cloud near the upper boundary looks much like a convective overshooting top on Earth.
I agree, Steve. It's interesting to think of the jovian equivalent of terrestrial weather patterns. Somewhere in that huge atmosphere, there may be cold fronts and/or low pressure centers triggering patterns of thunderstorms. I think we have yet to characterize it all, but these sure look like what you say.
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