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

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EisCoreStudy...nobody
EisCoreStudy

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At line 44 changed 4 lines
&nbsp; - 1st priority on the high cadence (at least < 60sec).\\
&nbsp; - 2nd priority on the longer coverage (>2-3hrs continuous coverage; \\
&nbsp; - Interuptions by SAAs and S/C nights are OK.)\\
&nbsp; - 3rd priority on the FOV (at least, larger than 100arcsec^2)\\
&nbsp; -- 1st priority on the high cadence (at least < 60sec).\\
&nbsp; -- 2nd priority on the longer coverage (>2-3hrs continuous coverage; \\
&nbsp; -- Interuptions by SAAs and S/C nights are OK.)\\
&nbsp; -- 3rd priority on the FOV (at least, larger than 100arcsec^2)\\
At line 170 changed 12 lines
!10. Properties in Solar Wind Source Regions – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]) Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]) \\
target: equatorial or low-latitude coronal hole within ± 400 latitude; Polar CH extensions also possible if within ± 400; observe with CH at central meridian\\
run a) YKK_EqCH_02n around the centre of the coronal hole\\
run b) YKK_EqCH_02n between the centre and East CH boundary\\
run c) YKK_EqCH_02w at E CH boundary partly covering the 'visible' CH, partly covering adjacent AR or QS to the East\\
run context raster slot_context_q50 covering FOV of the a, b and c rasters\\
default pointing: Sun center X=0", Y=0"; slit field-of-view to cover the solar equator; if CH does not reach latitude zero cover lowest latitude reached\\
if all three studies not possible in time available, run b) followed by c)\\
contact Yuan-Kuen Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]) to agree final pointing\\
__see Core HOP 146; use these original studies for on-disc CHs only__\\
\\
__11. Quiet sun dynamics study – Muglach __\\
!10. Properties in Solar Wind Source Regions – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]) \\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- target: equatorial or low-latitude coronal hole within ± 400 latitude; Polar CH extensions also possible if within ± 400; observe with CH at central meridian\\
-- run a) YKK_EqCH_02n around the centre of the coronal hole\\
-- run b) YKK_EqCH_02n between the centre and East CH boundary\\
-- run c) YKK_EqCH_02w at E CH boundary partly covering the 'visible' CH, partly covering adjacent AR or QS to the East\\
-- run context raster slot_context_q50 covering FOV of the a, b and c rasters\\
-- default pointing: Sun center X=0", Y=0"; slit field-of-view to cover the solar equator; if CH does not reach latitude zero cover lowest latitude reached\\
-- if all three studies not possible in time available, run b) followed by c)\\
-- contact Yuan-Kuen Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]) to agree final pointing\\
-- __see Core HOP 146; use these original studies for on-disc CHs only__\\
}}
%%
\\
!11. Quiet sun dynamics study – Muglach __\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
At line 183 changed 17 lines
- 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\\
Co-observing: - SOT:\\
1) magnetograms in either Fe I or Na I, in 60s cadence (or less if telemetry allows). \\
SOT to run > 15 min before EIS start and at least 15 min after EIS end.\\
2) SP scans of the target regions valuable additions but lower priority than 1.\\
3) BFI images in G-Band can be added; lower priority than 1 and 2.\\
4) XRT: filtergrams in the thinnest filter(s)\\
&nbsp; - a) Study: quiet_sun_slot (#210); 40x512 slot image as context\\
&nbsp; - three images should be taken before and after program b)\\
&nbsp; - b) Study: KM-qs-study-low (#315)\\
&nbsp; - run in areas of quiet Sun, also plage or moderately active regions possible\\
&nbsp; - slit should at least be partially on the disk\\
&nbsp; - avoid large, well developed ARs and coronal holes \\
&nbsp; - study for small-scale short-term variation of QS structures in cool EIS lines.\\
&nbsp; - repeat n times to fit into available data volume; at least for 30 min\\
&nbsp; - EXPOSURE: 20s, RASTER: Scanning, 4 steps, SLIT: 2", STEP: 2", FOV: 10"x464"\\
&nbsp; - if n = 30 for (b), data volume is 70 Mbits; run (b) for longer if volume available\\
Co-observing:\\
&nbsp; - SOT:\\
&nbsp; &nbsp; 1) magnetograms in either Fe I or Na I, in 60s cadence (or less if telemetry allows). \\
&nbsp; &nbsp; SOT to run > 15 min before EIS start and at least 15 min after EIS end.\\
&nbsp; &nbsp; 2) SP scans of the target regions valuable additions but lower priority than 1.\\
&nbsp; &nbsp; 3) BFI images in G-Band can be added; lower priority than 1 and 2.\\
&nbsp; &nbsp; 4) XRT: filtergrams in the thinnest filter(s)\\
}}
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At line 201 changed 3 lines
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At line 205 changed 6 lines
- Observe an on-disc filament\\
- Run \\
- cme_slot_red_lkh for approx 30 min; data vol: 18 Mbit; context\\
- cme_slit_red_lkh to fill available time; 34 min has data vol: 31 Mbit\\
- cme_slot_red_lkh for approx 30 min; data vol: 18 Mbit; context\\
__- Run if suitable quiescent filament is available on disc__\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- Observe an on-disc filament\\
-- Run \\
&nbsp; -- cme_slot_red_lkh for approx 30 min; data vol: 18 Mbit; context\\
&nbsp; -- cme_slit_red_lkh to fill available time; 34 min has data vol: 31 Mbit\\
&nbsp; -- cme_slot_red_lkh for approx 30 min; data vol: 18 Mbit; context\\
- __Run if suitable quiescent filament is available on disc__\\
}}
%%
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This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop