This page (revision-76) was last changed on 07-Dec-2016 14:14 by BriazWearl

This page was created on 25-Jun-2008 06:03 by David R Williams

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At line 36 changed one line
On most orbits, Hinode passes over the South Atlantic Anomaly (SAA), where high-energy particles penetrate lower into the magnetosphere. During such passes, significantly more ''cosmic rays'' are observed on the EIS detector images. These passes are calculated at the same time as other orbital events (such as Eclipse Season NGT events, when appropriate), and times vary each day. Such passes normally last approximately 10 to 20 minutes (although they can be calculated to last for as little as 30 seconds).
On most orbits[8], Hinode passes over the South Atlantic Anomaly (SAA), where high-energy particles penetrate lower into the magnetosphere. During such passes, significantly more ''cosmic rays'' are observed on the EIS detector images. These passes are calculated at the same time as other orbital events (such as Eclipse Season NGT events, when appropriate), and times vary each day. Such passes normally last approximately 10 to 20 minutes (although they can be calculated to last for as little as 30 seconds).
At line 82 added 2 lines
[|#8]: Hinode's orbital period is 98.5 minutes
This page (revision-76) was last changed on 07-Dec-2016 14:14 by BriazWearlTop