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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Version Date Modified Size Author Changes ... Change note
76 07-Dec-2016 14:14 10 KB BriazWearl to previous
75 11-Mar-2015 09:29 10 KB David R Williams to previous | to last
74 22-Jun-2010 16:19 10 KB David R Williams to previous | to last
73 19-May-2010 14:56 10 KB David R Williams to previous | to last
72 12-May-2010 23:12 10 KB David R Williams to previous | to last
71 12-May-2010 21:01 10 KB David R Williams to previous | to last
70 11-May-2010 15:52 10 KB David R Williams to previous | to last
69 11-May-2010 12:31 11 KB David R Williams to previous | to last
68 11-May-2010 12:29 10 KB David R Williams to previous | to last
67 11-May-2010 12:28 10 KB David R Williams to previous | to last
66 11-May-2010 12:28 10 KB David R Williams to previous | to last
65 11-May-2010 12:25 10 KB David R Williams to previous | to last
64 25-Jan-2010 14:31 9 KB David R Williams to previous | to last
63 25-Jan-2010 14:30 9 KB David R Williams to previous | to last
62 25-Jan-2010 14:21 9 KB David R Williams to previous | to last
61 19-May-2009 11:27 9 KB David R Williams to previous | to last

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SbandObservingInfo
SbandObservingInfo

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At line 6 changed 3 lines
!!Practical constraints?
!Time
OP Periods[1]
!!!Practical constraints?
!!Time
!OP[1] Periods
This is the period of time during which an observing programme (''plan'') is defined. e.g. from 10:23 UT on 2008/05/02 to 11:19 UT on 2008/05/04
At line 11 added 2 lines
!Eclipse Season
During eclipse season, the line of sight between the spacecraft and the Sun grazes the Earth's atmosphere, causing attenuation (and ultimately complete absorption) of the light that would otherwise be seen by each of the instruments. This attenuation affects first the EUV and X-ray bands, then later the visible wavelength range.
At line 11 changed one line
!Volume
The duration of night-time is calculated for the visible band, and in the peak of eclipse season (around mid-July [eclipsepeak])
!!Volume
At line 15 changed one line
!Do you have examples of what kind of observations are best suited for EIS?
!!Do you have examples of what kind of observations are best suited for EIS?
At line 19 changed 2 lines
!!Why can my old HOP no longer be run?
!!How is the HOP process different?
!!!Why can my old HOP no longer be run?
!!!How is the HOP process different?
At line 26 changed 2 lines
;__OP__:''__Operation Programme''
;__OP Period__:[1|#1]''Period of time during which an observing programme is defined. e.g. from 10:23 UT on 2008/05/02 to 11:19 UT on 2008/05/04''
;__OP__:[1|#1]''__Operation Programme''
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At line 35 added 2 lines
[#eclipsepeak]: Is this correct? I know it's approximately true, since we start in late April, and come out of eclipse season in early September.
This page (revision-76) was last changed on 07-Dec-2016 14:14 by BriazWearlTop