And bear in mind that it seems that these storms are transient - there aren't any permanent ones like the GRS on Jupiter. So duplicating them in a Celestia texture isn't particularly realistic, since they may well disappear in the space of a few days or weeks. Also not that most of those storms are actually quite small.
I am not complaning for nothing.I know that infrared provide more detail and so on,but I was surprised because we have real color pictures from Voyager,Hubble and even real color images from Cassini??s Jupiter rendesvouz.
AFAIK none of the raw images from Cassini's Jupiter have been released yet (unless I missed them. I haven't seen them anywhere myself). Quite how many of the thousands of images it took during that flyby were taken using red/green/blue filters is unknown.
Based in this,we can say that Titan??s texture are only a high resolution albedo map,i.e,we don??t know any real feature of this moon?
The surface texture? It's not even very high resolution - the atmosphere still seems to be sufficiently hazy to blur the views through the IR filter that we've seen of the surface so far. That effectively reduces the resolution quite considerably, so that at most all we've seen of Titan's surface - beyond the small snippet taken by Huygens - is very blurry and fuzzy looking. Even the supposedly high resolution views that have been published don't show much:
http://saturn.jpl.nasa.gov/multimedia/i ... ageID=1161
I've only seen one high resolution shot of the surface from cassini, and that's here: url=http://saturn.jpl.nasa.gov/multimedia/images/image-details.cfm?imageID=1165
But generally, I'd call the surface textures we have so far "
low resolution albedo maps". Better than nothing, but we certainly haven't seen Titan's surface at the sort of resolution that we've seen say, Dione's.
The radar has had more luck penetrating, but the problem is that what we've seen from that is so far largely incomprehensible. I think the radar images need to be processed a lot more before we can make much sense of that.
http://saturn.jpl.nasa.gov/multimedia/i ... ageID=1177
http://saturn.jpl.nasa.gov/multimedia/i ... ageID=1176
http://saturn.jpl.nasa.gov/multimedia/i ... ageID=1171
http://saturn.jpl.nasa.gov/multimedia/i ... ageID=1167