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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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At line 1 changed 2 lines
[{ALLOW view jsun,DaveWilliams,eiscorestudy}]
[{ALLOW edit jsun,DaveWilliams}]
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
At line 7 changed 4 lines
The conventions of title: HEADERyymmdd-Index => brief descriptions\\
HEADER: qs (Quite Sun); ar (Active Region); hop (Hinode Operation Plan); test (Test studies)\\
yymmdd: the date when the study is added\\
For example: ar100417-13 => Nanoflare heating of coronal loops
=> The conventions of title: HEADERyyyymmdd-Index => brief descriptions\\
    HEADER: qs (Quite Sun); ar (Active Region); hop (Hinode Operation Plan); test (Test studies)\\
    yyyymmdd: the date when the study is added; For "hop" and "test" header, it may be different\\
  For example: ar20100417-13 => Nanoflare heating of coronal loops\\ \\
=> study qs20091216-09 has been replaced by a new study (ie. syo20100504-01) since 2010-May-04\\
=> study ar20100329-12 has been replaced by a new study (ie. syo20100504-01) since 2010-May-04\\
=> study ar20110209-20 has been replaced by a new study (ie.  ar20110404-21) since 2010-Apr-04
At line 24 changed one line
!!Quiet Sun\\
!!A. Quiet Sun\\
At line 26 changed one line
!qs091216-01 => Evolution of X-ray bright point
!qs20091216-01 => Evolution of X-ray bright point
At line 35 changed one line
-- run [SK_QS_34x168c|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=295] (ID # 295) for BP study; data volume: 2.1 Mbit; dur: 3m 49s\\
-- run [SK_QS_34x168c|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=295] (ID # 295) for BP study; data volume: 2.1 Mbit; dur: 3m 49s\\
At line 42 changed 2 lines
|292|IUU_SLOT_136x400_Q65|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=292]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=292]
|295|SK_QS_34x168c|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=295]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=295]
|292|IUU_SLOT_136x400_Q65|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=292]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=292]
|295|SK_QS_34x168c|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=295]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=295]
At line 49 changed one line
!qs091216-02 => Coronal/TR Doppler & photosphere transverse magnetic features and cancellation events
!qs20091216-02 => Coronal/TR Doppler & photosphere transverse magnetic features and cancellation events
At line 76 changed 2 lines
|210|quiet_sun_slot|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=210]
|278|sta_loop_context_lo|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=278]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=278]
|210|quiet_sun_slot|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=210]
|278|sta_loop_context_lo|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=278]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=278]
At line 83 changed one line
!qs091216-03 => QS Brightenings
!qs20091216-03 => QS Brightenings
At line 101 changed 2 lines
|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]
|251|tr_bright_lo|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=251]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=251]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|251|tr_bright_lo|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=251]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=251]
At line 108 changed one line
!qs091216-04 => Search for Evidence of Wave Activity in the Solar Corona
!qs20091216-04 => Search for Evidence of Wave Activity in the Solar Corona
At line 123 changed one line
|337|rah_line_narrow|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=337]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=337]
|337|rah_line_narrow|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=337]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=337]
At line 130 changed one line
!qs091216-05 => X-ray Bright Points Onset
!qs20091216-05 => X-ray Bright Points Onset
At line 149 changed 3 lines
|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]
|285|dob_bp_slit_raster|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=285]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=285]
|284|dob_bp_slot_raster|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=284]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=284]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|285|dob_bp_slit_raster|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=285]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=285]
|284|dob_bp_slot_raster|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=284]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=284]
At line 157 changed one line
!qs091216-06 => Coronal Jets
!qs20091216-06 => Coronal Jets
At line 171 changed 2 lines
|354|PRY_slot_contextLITE|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|358|IUU_SCAN_STEPS_002|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=358]
|354|PRY_slot_contextLITE|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=354]
|358|IUU_SCAN_STEPS_002|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=358]
At line 178 changed one line
!qs091216-07 => Quiet Sun diagnostics/evolution
!qs20091216-07 => Quiet Sun diagnostics/evolution
At line 196 changed 3 lines
|322|NRL_QSCH_30X400_90s2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=322]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=322]
|378|IUU_SLOT_488x512|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=378]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=378]
|336|HPW019AR_1x400_45s|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=336]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=336]
|322|NRL_QSCH_30X400_90s2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=322]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=322]
|378|IUU_SLOT_488x512|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=378]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=378]
|336|HPW019AR_1x400_45s|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=336]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=336]
At line 204 changed one line
!qs091216-08 => Coronal Hole Density Measurement
!qs20091216-08 => Coronal Hole Density Measurement
At line 223 changed 2 lines
|249|PRY_slot_context_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=249]
|268|PRY_CH_density|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=268]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=268]
|249|PRY_slot_context_v2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=249]
|268|PRY_CH_density|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=268]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=268]
At line 230 changed one line
!qs091216-09 => Eclipse Spectral Atlas
!qs20091216-10 => Properties in Solar Wind Source Regions
At line 232 removed 24 lines
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- obtain reference spectra for general science during Hinode eclipse season\\
-- run PRY_slot_context_v3 (5 Mbits) and Eclipse_raster_v2 (99 Mbits)\\
-- observe any target\\
-- run PRY_slot_context_v3 once\\
-- follow by one run of Eclipse_raster_v2 (total duration: 54mins) \\
-- start PRY_slot_context_v3 10 mins after end of Hinode orbital night\\
-- repeat for consecutive day-time periods depending on available data volume\\
}}
%%
%%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]
%%
\\
!qs091216-10 => Properties in Solar Wind Source Regions
At line 273 changed 3 lines
|330|YKK_EqCH_02n|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=330]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=330]
|329|YKK_EqCH_02w|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=329]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=329]
|249|PRY_slot_context_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=249]
|330|YKK_EqCH_02n|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=330]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=330]
|329|YKK_EqCH_02w|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=329]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=329]
|249|PRY_slot_context_v2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=249]
At line 281 changed one line
!qs091216-11 => Quiet sun dynamics study
!qs20091216-11 => Quiet sun dynamics study
At line 309 changed 2 lines
|210|quiet_sun_slot|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=210]
|315|KM-qs-study-low|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=315]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=315]
|210|quiet_sun_slot|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=210]
|315|KM-qs-study-low|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=315]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=315]
At line 316 changed one line
!qs091216-12 => Filament Evolution
!qs20091216-12 => Filament Evolution
At line 332 changed 2 lines
|254|cme_slot_red_lkh|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=254]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=254]
|255|cme_slit_red_lkh|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=255]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=255]
|254|cme_slot_red_lkh|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=254]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=254]
|255|cme_slit_red_lkh|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=255]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=255]
At line 339 changed one line
!qs091216-13 => Interchange Reconnection at CH Boundaries
!qs20091216-13 => Interchange Reconnection at CH Boundaries
At line 353 changed one line
|294|dhb_polar_scan_Q90|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=294]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=294]
|294|dhb_polar_scan_Q90|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=294]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=294]
At line 359 changed one line
!!EIS HOP Obs.\\
!!B. EIS HOP Obs.\\
At line 361 changed one line
!hop-a => EIS CORE HOP 80:
!hop-a => EIS CORE HOP 80
At line 363 changed one line
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])\\
Polar Coronal Hole Observation\\
At line 344 added 2 lines
  – 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])\\
At line 367 changed one line
!hop-b => EIS CORE HOP 130:
!hop-b => EIS CORE HOP 130
At line 369 changed one line
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])\\
Multi-temperature Full Disk Slot Scans\\
At line 352 added 2 lines
  – 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])\\
At line 373 changed one line
!hop-c => EIS CORE HOP 146:
!hop-c => EIS CORE HOP 146
At line 375 changed one line
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])\\
Solar Wind Source Regions During Solar Minimum Conditions\\
At line 360 added 2 lines
  – 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 379 changed one line
!hop-d => EIS CORE HOP 137:
!hop-d => EIS CORE HOP 137
At line 381 changed one line
Evolution of Network Boundary Elements: Possible Connections to the Corona – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
Evolution of Network Boundary Elements: Possible Connections to the Corona\\
At line 368 added one line
  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
At line 384 changed one line
----
\\
At line 372 added 8 lines
!hop-e => EIS CORE HOP 131 (ToO)
Helioseismology Observations of Coronal Holes with SOT\\
  – Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk]), Zharkov ([sz2@mssl.ucl.ac.uk|mailto:sz2@mssl.ucl.ac.uk]), Sekii ([sekii@solar.mtk.nao.ac.jp|mailto:sekii@solar.mtk.nao.ac.jp])\\
__Note__: ToO is for "Targets of Opportunity"\\
At line 382 added one line
!hop-f => EIS CORE HOP 150 (ToO)
At line 389 changed one line
!!Active Region, Flare, CME\\
Flows during a filament eruption\\
At line 386 added 29 lines
  – Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk]), Culhane ([jlc@mssl.ucl.ac.uk|mailto:jlc@mssl.ucl.ac.uk]), Demoulin, Mandrini, Kliem, Williams\\
__Note__: ToO is for "Targets of Opportunity"\\
\\
!hop-g => EIS CORE HOP 160 (ToO)
Long-term Evolution of AR from Flux Emergence through Decay\\
  – Del Zanna ([GDelZanna@spd.aas.org|mailto:GDelZanna@spd.aas.org]), van Driel-Gesztelyi ([lvdg@mssl.ucl.ac.uk|mailto:lvdg@mssl.ucl.ac.uk])\\
__Note__: ToO is for "Targets of Opportunity"\\
\\
!hop-h => EIS CORE HOP 163 (ToO)
Variations in Line Width Across kG Magnetic Field Patches in Coronal Holes\\
  – Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk]), Tsuneta, Ito, Shiota\\
__Note__: ToO is for "Targets of Opportunity"\\
\\
!!C. Active Region, Flare, CME\\
At line 397 changed one line
!ar091216-01 => Active Region Studies
!ar20091216-01 => Active Region Studies
At line 412 changed 5 lines
|355|HPW017AR_30x400_30s2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=355]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=355]
|356|HPW018AR300x400_30s2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=356]
|357|HPW019AR_1x400_45s2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=357]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=357]
|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]
|354|PRY_slot_contextLITE|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|355|HPW017AR_30x400_30s2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=355]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=355]
|356|HPW018AR300x400_30s2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=356]
|357|HPW019AR_1x400_45s2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=357]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=357]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|354|PRY_slot_contextLITE|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=354]
At line 422 changed one line
!ar091216-02 => AR dynamics and CME watch
!ar20091216-02 => AR dynamics and CME watch
At line 424 changed one line
  – Young, Ugarte-Urra \\
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil]), Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil])\\
At line 435 changed 2 lines
|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]
|354|PRY_slot_contextLITE|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|354|PRY_slot_contextLITE|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=354]
At line 442 changed one line
!ar091216-03 => Active Region Studies
!ar20091216-03 => Active Region Studies
At line 455 changed 2 lines
|356|HPW018AR300x400_30s2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=356]
|358|IUU_SCAN_STEPS_002|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=358]
|356|HPW018AR300x400_30s2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=356]
|358|IUU_SCAN_STEPS_002|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=358]
At line 462 changed one line
!ar091216-04 => Active Region Abundance Variations
!ar20091216-04 => Active Region Abundance Variations
At line 477 changed 2 lines
|381|YKK_ARabund01|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=381]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=381]
|354|PRY_slot_contextLITE|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|381|YKK_ARabund01|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=381]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=381]
|354|PRY_slot_contextLITE|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=354]
At line 485 changed one line
!ar091216-05 => Pre-flare activity monitoring
!ar20091216-05 => Pre-flare activity monitoring
At line 499 changed one line
|286|Flare0_slit_AJW|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=286]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=286]
|286|Flare0_slit_AJW|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=286]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=286]
At line 505 changed one line
!ar091216-06 => Search for Active Region outflows
!ar20091216-06 => Search for Active Region outflows
At line 519 changed one line
|243|HPW015_DETAILED_MAP|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=243]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=243]
|243|HPW015_DETAILED_MAP|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=243]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=243]
At line 525 changed one line
!ar091216-07 => AR Temperature Diagnostic
!ar20091216-07 => AR Temperature Diagnostic
At line 534 changed 2 lines
  -- exposure time: 30s; raster: scanning; slit: 2"; step Size: 2", FOV: 360"X400";\\
  -- raster duration: 1h40m46s \\
  -- exposure time: 45s; raster: scanning; slit: 2"; step Size: 2", FOV: 322"X376";\\
  -- raster duration: 2h13m15s; Data volume: 186 Mbits;\\
At line 540 changed one line
|377|cam_ar_limb_lite_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=377]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=377]
|377|cam_ar_limb_lite_v2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=377]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=377]
At line 546 changed one line
!ar091216-08 => High cadence observations of AR transient brightenings and microflares
!ar20091216-08 => High cadence observations of AR transient brightenings and microflares
At line 582 added one line
-- run context study PRY_slot_context_v3 before and after\\
At line 562 changed one line
|377|cam_ar_limb_lite_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=377]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=377]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|360|cam_artb_lite_v2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=360]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=360]
At line 568 changed one line
!ar091216-09 => CME onsets
!ar20091216-09 => CME onsets
At line 570 changed one line
  – Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison\\
  – Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison([Richard.Harrison@stfc.ac.uk|mailto:Richard.Harrison@stfc.ac.uk])\\
At line 584 changed 2 lines
|279|cmeo_slit_lo|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=279]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=279]
|280|cmeo_slot_lo|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=280]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=280]
|279|cmeo_slit_lo|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=279]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=279]
|280|cmeo_slot_lo|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=280]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=280]
At line 590 changed one line
!ar091216-10 => CORE EIS Flare Study 1
!ar20091216-10 => CORE EIS Flare Study 1
At line 605 changed one line
|363|FLR001_flare_study|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=363]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=363]
|363|FLR001_flare_study|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=363]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=363]
At line 610 changed one line
!ar091229-11 => CORE EIS Flare Study 2
!ar20091229-11 => CORE EIS Flare Study 2
At line 617 changed 3 lines
-- 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\\
-- run HH_Flare+AR_180x152 (ID # 461)\\
-- exposure: 9s; raster: scanning, sparse; slit: 2”; step: 6”; FoV: 180” x 152”;\\
-- raster time: 6m 5s, data volume: 3.6 Mbit (JPEG75), 4.4 Mbit (JPEG85)\\
-- default compression is JPEG75; use JPEG85 for short runs\\
-- centre raster on expected AR flare site; adjust raster repeat for maximum possible runtime within telemetry constrainta\\
At line 625 changed one line
|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]
|461|HH_Flare+AR_180x152|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=461]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=461]
At line 630 changed one line
!ar100329-12 => Full CCD Scans of ARs for Increasing Spectral
!ar20100417-13 => Nanoflare heating of coronal loops
At line 632 changed one line
 Information – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
  – Klimchuk ([james.a.klimchuk@masa.gov|mailto:james.a.klimchuk@masa.gov]), Patsourakos ([spatsurakos@gmail.com|mailto:spatsurakos@gmail.com]), Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
At line 636 changed 4 lines
-- 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\\
-- test theory that coronal loops are bundles of unresolved, impulsively-heated strands by searching for spectral signatures in the wings of hot (~ 5MK) emission lines\\
-- run PRY_slot_context_v3 (4.9 Mbits, 3min 29s), nanoflare_sas_v1 (82.5 Mbits, 31min 24s)\\
-- run sequence: PRY_slot_context_v3, then nanoflare_sas_v1, finally PRY_slot_context_v3\\
-- run nanoflare_sas_v1 multiple times with raster repeats to fill available time\\
-- AR pointing for nanoflare_sas_v1 to be at lower legs of loops\\
-- select inner part of AR; not perimeter “fan” loops\\
-- choose side of AR with legs oriented along line-of-sight to maximize Doppler shift due to field-aligned flows\\
-- prefer ARs near disk center\\
-- for wavelength calibration, position hot loops towards either bottom or top of slit; ensure that the opposite side of the slit observes a quiet Sun region.\\
\\
__NOTE__: for pointing confirmation, please send screen grab from eis_image_tool to all three study authors showing suggested pointing. See [http://tiny.cc/43rcc] for typical pointing examples\\
At line 644 changed 2 lines
|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]
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|392|nanoflare_sas_v1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=392]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=392]
At line 650 changed one line
!ar100417-13 => Nanoflare heating of coronal loops
!ar20100423-14 => Active Region Transient Brightening Lite
At line 652 changed one line
 Information – Klimchuk ([james.a.klimchuk@masa.gov|mailto:james.a.klimchuk@masa.gov]), Patsourakos ([spatsurakos@gmail.com|mailto:spatsurakos@gmail.com]), Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
At line 656 changed 9 lines
-- test theory that coronal loops are bundles of unresolved, impulsively-heated strands by searching for spectral signatures in the wings of hot (~ 5MK) emission lines\\
-- run PRY_slot_context_v3 (4.9 Mbits, 3min 29s), nanoflare_sas_v1 (82.5 Mbits, 31min 24s)\\
-- run sequence: PRY_slot_context_v3, then nanoflare_sas_v1, finally PRY_slot_context_v3\\
-- run nanoflare_sas_v1 multiple times with raster repeats to fill available time\\
-- AR pointing for nanoflare_sas_v1 to be at lower legs of loops\\
-- select inner part of AR; not perimeter “fan” loops\\
-- choose side of AR with legs oriented along line-of-sight to maximize Doppler shift due to field-aligned flows\\
-- prefer ARs near disk center\\
-- for wavelength calibration, position hot loops towards either bottom or top of slit; ensure that the opposite side of the slit observes a quiet Sun region.\\
-- run cam_artb_cds_a_lite\\
-- observe on-disc active region close to disc centre; study AR transient brightening and density structure\\
--   raster to be centred on AR core or polarity inversion line\\
--   exposure time: 10s; raster scanning; slit: 2"; step size: 2"; FOV: 200" x 400"\\
--   raster duration: 21m09s; data volume: 108 Mbits\\
--   run context study PRY_slot_context_v3 before and after
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|361|cam_artb_cds_a_lite|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=361]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=361]
%%
At line 666 changed one line
__NOTE__: for pointing confirmation, please send screen grab from eis_image_tool to all three study authors showing suggested pointing. See [http://tiny.cc/43rcc] for typical pointing examples\\
!ar20100423-15 => Multi-temperature Observation of Sigmoids
  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run cam_sigmoid_study_v1\\
-- observe temperature structure of cooling plasma in sigmoidal structures on newly reconnected flux rope field lines\\
--   select small to medium size ARs; the AR should be in the centre of the raster\\
--   exposure time: 10s; raster scanning; slit: 2"; step size: 2"; FOV: 400" x 400"\\
--   raster duration: 41m33s; data volume: 125 Mbits\\
--   repeat to fill available time slot; minimum of 4 repeats preferred (needs 500 Mbits)\\
At line 671 changed 2 lines
|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]
|392|nanoflare_sas_v1|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=392]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=392]
|374|cam_sigmoid_study_v1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=374]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=374]
At line 679 changed one line
!!Test and Calibration Studies \\
!ar20100426-16 => Outflows from Small Active Regfions
At line 732 added 194 lines
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- observe small ARs simultaneously with QS regions to obtain accurate outflow velocities\\
-- run PRY_loop_velocity\\
--   duration: 4h33m; volume:230 Mbits\\
--   position AR near top or bottom of slit; see example at *[http://tiny.cc/qccji|http://tiny.cc/qccji]*\\
--   ensure that any fan loops visible in 171 Å images are contained within raster\\
--   avoid complex ARs\\
}}
%%
%%center
||Study ID||Acronym|| ||
|388|PRY_loop_velocity|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=388]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=388]
%%
\\
!ar20100622-17 => AR Temperatures and Flows Optimized for Eclipse Observing
  – Warren ([harry.warren@nrl.navy.mil|mailto:harry.warren@nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run hpw021_vel_120x512v1\\
--   duration should allow it to be run between eclipses; can be run multiple times to cover a larger area; avoid SAA.\\
--   target: active region\\
--   full slit is taken; position active region near top or bottom of slit so that there is ample quiet Sun for velocity calibration.\\
--   exposure time: 60s; raster: scanning; slit: 1"; step Size: 2", FOV: 120"x512";\\
--   raster duration:1h4m58s; data volume: 135 Mbits \\
}}
%%
%%center
||Study ID||Acronym|| ||
|420|hpw021_vel_120x512v1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=420]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=420]
%%
\\
!ar20101109-18 => Dynamic events at the limb with EIS and AIA
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- pointing should be above the limb, preferably an active region; quiet Sun or prominence cavity also acceptable\\
-- sequence: first run PRY_slot_context_v3, then PRY_sit_stare_1 (repeat for several hours), then PRY_slot_context_v3\\
-- XRT: high cadence, long duration, Y-coverage: 512”; spatial resolution: 1-2” preferred\\
-- SOT: Ca II and/or H-alpha, with high cadence, long duration preferred over spatial resolution \\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|443|PRY_sit_stare_1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=443]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=443]
%%
\\
!ar20110120-19 => AR Loop footpoint studies using the bright point trigger
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- observe AR on the disc with bright loop footpoints (check AIA 171 image)\\
-- target region near central meridian preferred\\
-- run Hunter_loop_fe8 (ID: 445, 3.1 Mbits, 24min); set response study to be Cool_loop_response\\
   (ID: 444, 268 Mbits, 2hr 52m)\\
-- BP trigger parameters are given in the Hunter_loop_fe8 study description, but change the Xthresh \\
   value to 5000 (instead of 5460)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|445|Hunter_loop_fe8|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=445]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=445]
|444|Cool_loop_response|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=444]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=444]
%%
\\
!ar20110404-21 => Search for slow mode oscillations in coronal loops
  – Wang ([tongjiang.wang@nasa.gov|mailto:tongjiang.wang@nasa.gov]), Mariska ([john.mariska@nrl.navy.mil|mailto:john.mariska@nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- pointing is to a possibly flare-productive active region on the limb.\\
-- for Study A, 1/3 FOV on the disk and 2/3 FOV off the limb.\\
-- for Studies B and and C, the slit center position is set about 30-50 arcsec above the AR on the \\
   limb (close to the AR core)\\
-- run PRY_slot_contextLITE (ID #354); Study A\\
-- run Hot_loop_osci_1_v3 (ID #459); Study B, repeating for up to 5 hrs\\
-- run PRY_slot_contextLITE (ID #354); Study A\\
-- run Hot_loop_osci_2_v3 (ID #460); Study C, repeating for up to 5 hrs\\
-- run PRY_slot_contextLITE (ID #354); Study A\\
-- runs can be done in two parts: A B A as one part and A C A as the second part.\\
-- each sequence above should be run uninterrupted (preferably use chained studies)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|354|PRY_slot_contextLITE|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=354]
|459|Hot_loop_osci_1_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=459]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=459]
|460|Hot_loop_osci_2_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=460]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=460]
%%
\\
!ar20110411-22 => Cambridge Diagnostic Study for the Impulsive Phase of Small Flares
  – DelZanna ([gdelzanna@spd.aas.org|mailto:gdelzanna@spd.aas.org]), Mason ([h.e.mason@damtp.cam.ac.uk|mailto:h.e.mason@damtp.cam.ac.uk])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run on small flare-productive AR as it crosses the disc; avoid X-flare regions\\
-- run a high-cadence (2m 47s), small (60” x 120”), sparse (3”) raster on a small AR; 2” slit; 5s exposure\\
-- point to AR core; on-disc and near CM\\
-- run Cam_flare_diag (ID # 458)\\
-- run continuously for ~ 12 hr; 230 repetitions for 10.7 hr and 590 Mbit\\
-- request XRT: FoV ≥ 384” x 384”; use AEC; 2 x 2 binning acceptable; Filters: at least Al_poly_open and one thick filter\\
-- request SOT/FG: NFI Na I 589.6 shuttered Stokes IV with partial FoV (164” x 164”); 2 x 2 binning; 1 – 3 min or longer cadence\\
-- request SOT/SP: Fast map Stokes IQUV 164” x 164”; run at beginning and possibly at end of SOT/FG sequence\\
}}
%%
%%center
||Study ID||Acronym|| ||
|458|Cam_flare_diag|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=458]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=458]
%%
\\
!!D. Synoptic and Other Studies\\
!syo20100504-01 => EIS Spectral Atlas Synoptic Programme
  – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil]), Warren, Mason, Del Zanna\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run twice each month; in the first and third full weeks of the month\\
-- run PRY_slot_context_v3; Duration: 3min 29s; Data volume: 5 Mbit\\
-- follow with either Atlas_30s (34min, 257 Mbit), or Atlas_60s (65min, 257 Mbit)\\
-- pointing to be specified by email to CO at start of observing week by P. Young\\
-- in absence of specific target, CO is free to choose any solar feature on- or off-disc\\
--   *NOTE: use Atlas_30s only if an AR is forecast to produce M-class or greater flares; use Atlas_60s for all other targets*\\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=353]
|403|Atlas_30|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=403]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=403]
|404|Atlas_60|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=404]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=404]
%%
\\
!syo20100713-02 => Full CCD Study to Measure Relative Wavelengths
  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run HPW020_VEL_FULLs1 (ID # 413)\\
-- full CCD sit-and-stare study; Duration: 45 min; Data volume: 243 Mbits.\\
-- prefer run above limb on AR 11087; EIS pointing: x = R_Sun + 15 arc sec, y = 0\\
}}
%%
%%center
||Study ID||Acronym|| ||
|413|HPW020_VEL_FULLs1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=413]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=413]
%%
\\
!!E. Test and Calibration Studies \\
At line 702 changed one line
|389|CALIB_slit_slot_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=389]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=389]
|389|CALIB_slit_slot_v2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=389]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=389]
At line 727 changed 2 lines
|375|SK_DEEP_5x512_SLIT1|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=375]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=375]
|376|SK_DEEP_5x512_SLIT2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=376]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=376]
|375|SK_DEEP_5x512_SLIT1|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=375]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=375]
|376|SK_DEEP_5x512_SLIT2|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=376]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=376]
%%
At line 976 added 23 lines
\\
!test-03 => EIS Slot Deconvolution Test
  – Sun ([js2@mssl.ucl.ac.uk|mailto:js2@mssl.ucl.ac.uk])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- Develop method to deconvolve EIS slot data\\
-- Two studies:\\
   * js2_decon_slot_sc_LT (ID # 429): data volume: 3.71Mbits; duration: 1m51s\\
   * js2_decon_ref_vel_LT (ID # 430): data volume: 87.87Mbits; duration: 47m37s\\
-- Instructions for planner:\\
   - Run study (ID # 429) first, then consecutively run study (ID # 430), then run study (ID # 429) again.\\
   - It's prefer that the slot study (ID # 429) repeats a few times, \\
     eg. study429 (x6), study430 (x1), study429 (x6) \\
-- Target: \\
   - simple active region; \\
   - FoV to cover AR edge to detect outflows; \\
   - both rasters to have identical pointing\\
-- Run during SAA-free interval preferred\\
}}
At line 1,000 added 5 lines
%%center
||Study ID||Acronym|| ||
|429|js2_decon_slot_sc_LT|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=429]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=429]
|430|js2_decon_ref_vel_LT|[details|https://vsolar.mssl.ucl.ac.uk/SolarB/ShowEisStudy.jsp?study=430]|[Example fits|https://vsolar.mssl.ucl.ac.uk/SolarB/Studies2FitsConn.jsp?study=430]
%%
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop