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Either there's an interplanetary "hot rodder" or there's some
co-orbiting debris floating alongside Cassini. http://saturn.jpl.nasa.gov/multimedi...eiImageID=8552 |
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Bob Carlson wrote:
wrote in message . .. http://saturn.jpl.nasa.gov/multimedia/images/raw/raw-images-details.cfm?feiImageID=8552 Interesting! When you click on the full-res version of the photo the "blob" looks like an arrowhead or a windows-like pointer. Also, I wonder what would be cause of the luminescence in the streak? Bob Carlson Remember that you're looking at a .jpg image, which (as I understand it) has been subjected to some sort of lossy compression. The original, uncompressed image may well look different. This includes the apparent shape of Mimas, which would present roughly a half-moon appearance with its terminator at about the same angle as Saturn's. Mimas's big crater would not have been visible in this picture, so we can't blame the strange shape of the terminator on it. There are actually *two* streaks in the image -- if you put a ruler up to one of them, the other doesn't lie in the same line. These are caused by cosmic rays or other charged particles impinging on the camera's CCD detector during the exposure or during readout. They deposit some of their energy into the CCD by ionizing some of the silicon atoms. The electrons thus liberated look no different from the electrons liberated by the light that hits the chip during the exposure. This happens all the time -- you can see lots of little white dots all over Saturn -- it's just that these two happened to come in almost parallel to the chip's surface (at "grazing incidence") and left long trails as a result. -- Bill Owen |
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![]() -- Bill Owen, Cassini optical navigation team Thanks for the good info. Pardon my dumbness in this area but could the speed of the cosmic ray be determined by using a very short exposure time? And why would the cosmic ray only affect the ccd during the exposure? I thought cosmic rays would penetrate to the ccd at all times regardless of exposure time. Bob Carlson |
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Bob Carlson wrote:
-- Bill Owen, Cassini optical navigation team Thanks for the good info. Pardon my dumbness in this area but could the speed of the cosmic ray be determined by using a very short exposure time? And why would the cosmic ray only affect the ccd during the exposure? I thought cosmic rays would penetrate to the ccd at all times regardless of exposure time. Bob Carlson Cosmic rays (and other charged particles ... remember, Cassini is inside Saturn's magnetosphere) are continually impinging on the CCDs. But the accumulated charge is flushed out immediately before each exposure begins (just like any CCD camera on a ground telescope), so whatever happens before that is gone. During readout, the picture is slowly moved up the chip into a "serial register", and any cosmic rays which hit the remaining part of the picture will also get recorded. You do see more CR hits at the bottom of a Cassini image than at the top. But after the readout is completed, the numbers are (more or less) safely tucked away in the solid state recorder, and cosmic ray effects there are much rarer. Meanwhile, the CCD itself continues accumulating hits until it gets cleared again before the next picture. As for determining the speed, no, this is not the kind of instrument you'd want to use for that. -- Bill |
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