This page (revision-7) was last changed on 07-Dec-2016 14:14 by David R Williams

This page was created on 24-Aug-2009 02:28 by David R Williams

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Version Date Modified Size Author Changes ... Change note
7 07-Dec-2016 14:14 1 KB David R Williams to previous
6 24-Aug-2009 07:02 1 KB David R Williams to previous | to last
5 24-Aug-2009 06:49 1 KB David R Williams to previous | to last
4 24-Aug-2009 06:48 1 KB David R Williams to previous | to last
3 24-Aug-2009 06:45 1 KB David R Williams to previous | to last
2 24-Aug-2009 02:30 612 bytes David R Williams to previous | to last
1 24-Aug-2009 02:28 480 bytes David R Williams to last

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StudiesForRegularProgrammes...nobody
StudiesForRegularProgrammes

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+++ Studies for Regular Programmes
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
!!! Studies for Regular Programmes
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++ About
!! About
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__N.B.__: This page is __not__ a place to add studies that you would like to be regular programmes: it is for COs' reference only.
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+ HOP 79
\\
! HOP 79
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\\
! XRT Synoptics
Purpose: XRT makes a series of full-disc images, which means Hinode repoints at disc centre twice a day.
Study to use: we use this opportunity to make regular measurements of the sensitivity of EIS, using the average quiet Sun as a "standard candle". %%strike On one occasion per day (no more) use the original study, SYNOP001. It's an X-band era study, though, so if you want to run another in the same day, use SYNOP005A. They're both very short.%%
Update: Use SYNOP005A each time: the overhead for SYNOP001 is a little too high.
This page (revision-7) was last changed on 07-Dec-2016 14:14 by David R WilliamsTop