This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian Sun

This page was created on 14-Dec-2009 10:51 by JianSun

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Version Date Modified Size Author Changes ... Change note
186 18-Apr-2021 19:09 44 KB Jian Sun to previous
185 30-Jun-2011 16:36 45 KB Jian Sun to previous | to last
184 11-Apr-2011 10:53 45 KB JianSun to previous | to last
183 11-Apr-2011 10:52 45 KB JianSun to previous | to last
182 04-Apr-2011 15:19 43 KB JianSun to previous | to last
181 04-Apr-2011 15:17 43 KB JianSun to previous | to last

Page References

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EisCoreStudy...nobody
EisCoreStudy

Version management

Difference between version and

At line 387 removed 40 lines
!ar100329-1 => Full CCD Scans of ARs for Increasing Spectral
 Information – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- study to run nominally once per week subject to pressure from other requests\\
-- *run on any available AR following check with proposer\\
-- *run context study, PRY_slot_context_v3\\
-- *run eclipse_raster_v2; ID: 362; data volume: 100 Mbit\\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|362|Eclipse_raster_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=362]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=362]
%%
\\
!ar091229-01 => CORE EIS Flare Study 2
  – Hara ([hara@solar.mtk.nao.ac.jp|mailto:hara@solar.mtk.nao.ac.jp])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- study used to search for flow structures in flares\\
-- run HH_Flare_180x160_v2 (ID # 390)\\
-- exposure: 8s; raster: scanning, sparse; slit: 2”; step: 5”; FoV: 180” x 160”; raster time: 6m 36s, data volume: 4.7 Mbit\\
-- with compression (JPEG85) study should run at 757 Mbit in 16h 30m\\
-- see [http://www.mssl.ucl.ac.uk/www_solar/eisflarestudy.html] for further details\\
}}
%%
%%center
||Study ID||Acronym|| ||
|390|HH_Flare_180x160_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=390]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=390]
%%
\\
At line 620 removed one line
At line 600 added one line
!ar091229-01 => CORE EIS Flare Study 2
At line 602 added 39 lines
  – Hara ([hara@solar.mtk.nao.ac.jp|mailto:hara@solar.mtk.nao.ac.jp])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- study used to search for flow structures in flares\\
-- run HH_Flare_180x160_v2 (ID # 390)\\
-- exposure: 8s; raster: scanning, sparse; slit: 2”; step: 5”; FoV: 180” x 160”; raster time: 6m 36s, data volume: 4.7 Mbit\\
-- with compression (JPEG85) study should run at 757 Mbit in 16h 30m\\
-- see [http://www.mssl.ucl.ac.uk/www_solar/eisflarestudy.html] for further details\\
}}
%%
%%center
||Study ID||Acronym|| ||
|390|HH_Flare_180x160_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=390]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=390]
%%
\\
!ar100329-01 => Full CCD Scans of ARs for Increasing Spectral
 Information – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- study to run nominally once per week subject to pressure from other requests\\
-- run on any available AR following check with proposer\\
-- run context study, PRY_slot_context_v3\\
-- run eclipse_raster_v2; ID: 362; data volume: 100 Mbit\\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|362|Eclipse_raster_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=362]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=362]
%%
\\
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop