This page (revision-5) was last changed on 07-Dec-2016 14:14 by David R Williams

This page was created on 13-Sep-2007 16:37 by PeterYoung

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Version Date Modified Size Author Changes ... Change note
5 07-Dec-2016 14:14 2 KB David R Williams to previous Added a disclaimer that the exact studies are no longer appropriate, but that the spirit of the discussion is still very valid
4 16-Jul-2008 05:55 2 KB David R Williams to previous | to last
3 16-Jul-2008 04:35 1 KB David R Williams to previous | to last
2 16-Jul-2008 04:17 1 KB David R Williams to previous | to last
1 13-Sep-2007 16:37 1 KB PeterYoung to last

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%%information The following section %%
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
%%warning The following section %%(color:#5555ff;)in blue%% was written prior to Hinode changing from X-band to S-band telemetry. Therefore, please bear in mind that these studies are unlikely to be able to run at this time.
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%%(background-color:#ffcc33;)This is a list of some studies that I've either designed or used that I think are generally useful.
However, the discussion of the scientific __type__ of observation is still valid, and many new studies have been designed to have a lower volume for the new telemetry situation. For example, {{PRY_footpoints_v2}} has been succeeded by {{PRY_footpoints_lite}}. See [Study4LowDataVolume] for some more examples of lower-volume studies, though.
%%
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%%(color:#5555ff;)This is a list of some studies that I've either designed or used that I think are generally useful.
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A high cadence (4mins) raster covering 40x120 arcsec^2 with many diagnostic lines, and a 10s exposure time. It is a good diagnostic study for studying flaring activity in active regions.
A high cadence (4mins) raster covering 40x120 arcsec%%sup 2%% with many diagnostic lines, and a 10s exposure time. It is a good diagnostic study for studying flaring activity in active regions.
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This page (revision-5) was last changed on 07-Dec-2016 14:14 by David R WilliamsTop