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SOHO/EIT is operating at a reduced image cadence
At the end of 2010 July, EIT has completed fourteen and a half years of synoptic observations of the low corona. SDO AIA images at much higher resolution and time cadence are now available for all the EIT wavebands, and three other EUV wavelengths as well. The telemetry bandwidth that has been used by EIT will be used by LASCO to improve the cadence of its observations of the fastest CME's. EIT will continue to obtain a couple of "synoptic sets" of images in all four wavelengths per day to track detector behavior, and to maintain the uniform data set.
Originally posted by CLPrime
reply to post by habfan1968
Any static you see on these satellite images is from solar ray bombardment. Each dot is a single particle capture.
Originally posted by spirit_horse
Are you talking about the first 4 pics? It looks like the CCD is washed out possibly from high energy particles from the solar wind or flare, etc. I haven't seen them look like that before, but I don't go there a lot either. I am sure there are a lot of others on ATS that know everything about SOHO and it's compadres...
I did find this about the EIT photos:
SOHO/EIT is operating at a reduced image cadence
At the end of 2010 July, EIT has completed fourteen and a half years of synoptic observations of the low corona. SDO AIA images at much higher resolution and time cadence are now available for all the EIT wavebands, and three other EUV wavelengths as well. The telemetry bandwidth that has been used by EIT will be used by LASCO to improve the cadence of its observations of the fastest CME's. EIT will continue to obtain a couple of "synoptic sets" of images in all four wavelengths per day to track detector behavior, and to maintain the uniform data set.
edit on 2/11/11 by spirit_horse because: Add Info