Magnetopause Line Within Geosynchronous Orbit - HD

259 views · Published 8 October 2012 · 7:32 · Indexed 25 October 2026

Channel: maalaea · 2012 · Education

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http://iswa.ccmc.gsfc.nasa.gov/iswa/iSWA.html
http://www.solarmonitor.org/index.php?date=20120911&region=11564
http://wdc.kugi.kyoto-u.ac.jp/kp/index.html

http://irsa.ipac.caltech.edu/IRASdocs/exp.sup/ch3/C.html#1
C.4 Strategy during South Atlantic Anomaly Passage

Survey observations were interrupted for up to l4 minutes during SAA passages even after selection of the least affected orbits. When the telescope entered the SAA during a survey scan its scanning motion was halted and it remained pointing at the same point on the celestial sphere until it emerged from the SAA when the scan was restarted with an overlap. During the SAA passage, "bias boost" was applied to the 60 and 100  µm detectors until about three minutes before exit. The internal reference sources were flashed just before entry and just after exit at the end and beginning of survey scans (Section III.B.3). Some SAA passages required so much time that the telescope would have violated the Earth infrared constraint (Section III.B.4) after SAA passage. In such cases it was necessary to leave a hole in the sky coverage and try to recover it with specially prepared short scans in the preceding or succeeding pair of SOPs. The failure to recover all of these holes contributed to the variable depth of sky coverage.

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