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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
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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

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At line 174 changed one line
-- target: equatorial or low-latitude coronal hole within ± 40%%sup o %% latitude; Polar CH extensions also possible if within ± 40%%sup 3 %%; observe with CH at central meridian\\
-- target: equatorial or low-latitude coronal hole within ± 40%%sup 0%% latitude; Polar CH extensions also possible if within ± 40%%sup 0%%; observe with CH at central meridian\\
At line 192 changed 11 lines
- run studies in the order: three times (a) - n times (b) – three times (a)\\
  - a) Study: quiet_sun_slot (#210); 40x512 slot image as context\\
  - three images should be taken before and after program b)\\
  - b) Study: KM-qs-study-low (#315)\\
  - run in areas of quiet Sun, also plage or moderately active regions possible\\
  - slit should at least be partially on the disk\\
  - avoid large, well developed ARs and coronal holes \\
  - study for small-scale short-term variation of QS structures in cool EIS lines.\\
  - repeat n times to fit into available data volume; at least for 30 min\\
  - EXPOSURE: 20s, RASTER: Scanning, 4 steps, SLIT: 2", STEP: 2", FOV: 10"x464"\\
  - if n = 30 for (b), data volume is 70 Mbits; run (b) for longer if volume available\\
-- run studies in the order: three times (a) - n times (b) – three times (a)\\
  -- a) Study: quiet_sun_slot (#210); 40x512 slot image as context\\
  -- three images should be taken before and after program b)\\
  -- b) Study: KM-qs-study-low (#315)\\
  -- run in areas of quiet Sun, also plage or moderately active regions possible\\
  -- slit should at least be partially on the disk\\
  -- avoid large, well developed ARs and coronal holes \\
  -- study for small-scale short-term variation of QS structures in cool EIS lines.\\
  -- repeat n times to fit into available data volume; at least for 30 min\\
  -- EXPOSURE: 20s, RASTER: Scanning, 4 steps, SLIT: 2", STEP: 2", FOV: 10"x464"\\
  -- if n = 30 for (b), data volume is 70 Mbits; run (b) for longer if volume available\\
At line 224 changed one line
- __Run if suitable quiescent filament is available on disc__\\
-- __Run if suitable quiescent filament is available on disc__\\
At line 230 removed one line
At line 232 changed 4 lines
run dhb_polar_scan_Q90 (ID #294); \\
check with proposers for pointing details\\
__run for small closed structures at CH boundaries or inside on-disc CHs__\\
__------------------------------------------------------------------------------------------------------EIS CORE HOP 80: Polar Coronal Hole Observation – Gabriel ([alan.gabriel@ias.u-psud.fr|mailto:alan.gabriel@ias.u-psud.fr]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])__\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run dhb_polar_scan_Q90 (ID #294); \\
-- check with proposers for pointing details\\
-- __run for small closed structures at CH boundaries or inside on-disc CHs__\\
}}
%%
\\
----
!EIS CORE HOP 80: Polar Coronal Hole Observation – Gabriel ([alan.gabriel@ias.u-psud.fr|mailto:alan.gabriel@ias.u-psud.fr]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])\\
\\
!EIS CORE HOP 130: Multi-temperature Full Disk Slot Scans - Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]), Brooks ([dhbrooks@ssd5.nrl.navy.mil|mailto:dhbrooks@ssd5.nrl.navy.mil])\\
\\
!EIS CORE HOP 146: Solar Wind Source Regions During Solar Minimum Conditions – Kuen Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]), Mariska ([mariska@nrl.navy.mil|mailto:mariska@nrl.navy.mil])\\
At line 237 changed one line
__EIS CORE HOP 130: Multi-temperature Full Disk Slot Scans - Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]), Brooks ([dhbrooks@ssd5.nrl.navy.mil|mailto:dhbrooks@ssd5.nrl.navy.mil]) __\\
!EIS CORE HOP 137: Evolution of Network Boundary Elements: Possible Connections to the Corona – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
----
!!! B. Active Region, Flare, CME\\
%%information
{{Useful AR context studies for before/after main AR observation are: PRY_slot_context_v3 or PRY_slot_contextLITE}}
%%
At line 239 changed 8 lines
__EIS CORE HOP 146: Solar Wind Source Regions During Solar Minimum Conditions – Kuen Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]), Mariska ([mariska@nrl.navy.mil|mailto:mariska@nrl.navy.mil])__\\
\\
__EIS CORE HOP 137: Evolution of Network Boundary Elements: Possible Connections to the Corona – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])__\\
__------------------------------------------------------------------------------------------------------B. Active Region, Flare, CME__\\
__Useful AR context studies for before/after main AR observation are: __\\
__PRY_slot_context_v3 or PRY_slot_contextLITE__\\
\\
__1. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska __\\
!1. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska\\
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop