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

Only authorized users are allowed to rename pages.

Only authorized users are allowed to delete pages.

Page revision history

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

Incoming links Outgoing links
EisCoreStudy...nobody
EisCoreStudy

Version management

Difference between version and

At line 1 changed 2 lines
[{ALLOW view jsun,eiscorestudy}]
[{ALLOW edit jsun}]
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
At line 4 added 13 lines
%%roundedCorners-yyyy-E3F0EE-808080
{{
=> 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 study qs20091216-09 has been replaced by a new study (ie.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 study ar20100329-12 has been replaced by a new study (ie.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 study ar20110209-20 has been replaced by a new study (ie.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 19 added one line
\\
At line 7 changed 2 lines
%%(text-align:center;font-size:25px;bold;)
Available EIS Core Team Studies
%%(text-align:center;font-size:20px;bold;)
!!!Available EIS Core Team Studies
At line 13 changed one line
!!!A. Quiet Sun\\
!!A. Quiet Sun\\
At line 15 changed one line
!qs091216-01. Evolution of X-ray bright point
!qs20091216-01 => Evolution of X-ray bright point
At line 24 changed one line
-- run SK_QS_34x168c (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 26 changed one line
-- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to track evolution of magnetic fields in the photosphere\\
-- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to track evolution of magnetic fields in the photosphere\\
At line 43 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 added one line
At line 32 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 40 changed one line
-- run studies in the order: three times (a) - n times (b) \u2013 three times (a)\\
-- run studies in the order: three times (a) - n times (b) - three times (a)\\
At line 77 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 added one line
At line 60 changed one line
!qs091216-03. QS Brightenings
!qs20091216-03 => QS Brightenings
At line 102 added 5 lines
%%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]
|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 added one line
At line 79 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 124 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 129 added one line
At line 96 changed one line
!qs091216-05. X-ray Bright Points Onset
!qs20091216-05 => X-ray Bright Points Onset
At line 150 added 6 lines
%%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]
|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 added one line
At line 116 changed one line
!qs091216-06. Coronal Jets
!qs20091216-06 => Coronal Jets
At line 172 added 5 lines
%%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]
|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 added one line
At line 131 changed one line
!qs091216-07. Quiet Sun diagnostics/evolution
!qs20091216-07 => Quiet Sun diagnostics/evolution
At line 197 added 6 lines
%%center
||Study ID||Acronym|| ||
|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 added one line
At line 150 changed one line
!qs091216-08. Coronal Hole Density Measurement
!qs20091216-08 => Coronal Hole Density Measurement
At line 167 changed 17 lines
\\
!qs091216-09. Eclipse Spectral Atlas
  – 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|| ||
|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 added one line
At line 188 changed one line
!qs091216-10. Properties in Solar Wind Source Regions
!qs20091216-10 => Properties in Solar Wind Source Regions
At line 194 changed one line
-- 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\\
-- target: equatorial or low-latitude coronal hole within ± 40%%sup o%% latitude; Polar CH extensions also possible if within ± 40%%sup o%%; observe with CH at central meridian\\
At line 250 added 6 lines
%%center
||Study ID||Acronym|| ||
|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 257 added one line
At line 208 changed one line
!qs091216-11. Quiet sun dynamics study
!qs20091216-11 => Quiet sun dynamics study
At line 286 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 292 added one line
At line 237 changed one line
!qs091216-12. Filament Evolution
!qs20091216-12 => Filament Evolution
At line 309 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 315 added one line
At line 254 changed one line
!qs091216-13. Interchange Reconnection at CH Boundaries
!qs20091216-13 => Interchange Reconnection at CH Boundaries
At line 330 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 335 added one line
At line 269 changed one line
!!! A-1. EIS HOP Obs.\\
!!B. EIS HOP Obs.\\
At line 271 changed one line
!hop-a. EIS CORE HOP 80:
!hop-a => EIS CORE HOP 80
At line 273 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 277 changed one line
!hop-b. EIS CORE HOP 130:
!hop-b => EIS CORE HOP 130
At line 279 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 283 changed one line
!hop-c. EIS CORE HOP 146:
!hop-c => EIS CORE HOP 146
At line 285 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 289 changed one line
!hop-d. EIS CORE HOP 137:
!hop-d => EIS CORE HOP 137
At line 291 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 294 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 298 changed one line
!!! B. Active Region, Flare, CME\\
!hop-f => EIS CORE HOP 150 (ToO)
At line 384 added 31 lines
Flows during a filament eruption\\
  – 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 306 changed one line
!ar091216-01. Active Region Studies
!ar20091216-01 => Active Region Studies
At line 434 added 8 lines
%%center
||Study ID||Acronym|| ||
|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 443 added one line
At line 322 changed one line
!ar091216-02. AR dynamics and CME watch
!ar20091216-02 => AR dynamics and CME watch
At line 324 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 457 added 5 lines
%%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]
|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 463 added one line
At line 336 changed one line
!ar091216-03. Active Region Studies
!ar20091216-03 => Active Region Studies
At line 477 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 483 added one line
At line 350 changed one line
!ar091216-04: Active Region Abundance Variations
!ar20091216-04 => Active Region Abundance Variations
At line 363 changed 19 lines
\\
!ar091216-05. Loop morphology and oscillations
  – de Moortel ([ineke@mcs.st-and.ac.uk|mailto:ineke@mcs.st-and.ac.uk]), Bewsher ([d.bewsher@rl.ac.uk|mailto:d.bewsher@rl.ac.uk]), Young\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- relatively quiescent (non-flaring) coronal loop system either on disk or limb.\\
-- point to loops in the active region.\\
-- run PRY_footpoints_lite (dur: 28min; vol: 55 Mbit), sta_loop_slot_lo (dur: 39min; vol: 22 Mbit).\\
-- study sequence is: \\
  - PRY_footpoints_lite once at beginning of a period \\
  - sta_loop_slot_lo at the same pointing\\
  - repeat sta_loop_slot_lo to fill available time slot.\\
-- __run on any quiescent AR; advise schedule to de Moortel__\\
}}
%%center
||Study ID||Acronym|| ||
|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 505 added one line
At line 387 changed one line
!ar091216-06. Pre-flare activity monitoring
!ar20091216-05 => Pre-flare activity monitoring
At line 521 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 526 added one line
At line 402 changed one line
!ar091216-07. Search for Active Region outflows
!ar20091216-06 => Search for Active Region outflows
At line 541 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 546 added one line
At line 417 changed one line
!ar091216-08. AR Temperature Diagnostic
!ar20091216-07 => AR Temperature Diagnostic
At line 426 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 562 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 567 added one line
At line 433 changed one line
!ar091216-09. 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 585 added 5 lines
%%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]
|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 591 added one line
At line 450 changed one line
!ar091216-10. CME onsets
!ar20091216-09 => CME onsets
At line 452 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 457 changed one line
-- point above limb __at AR if it develops __with part of limb in FoV\\
-- point above limb at AR if it develops with part of limb in FoV\\
At line 459 changed one line
-- run cmeo_slit_lo; minimum 5 rasters; Duration: 4.2 h; Volume: 13 Mbit __or__\\
-- run cmeo_slit_lo; minimum 5 rasters; Duration: 4.2 h; Volume: 13 Mbit or\\
At line 461 changed one line
-- algorithm uses difference imaging so minimum durations __must__ be available\\
-- algorithm uses difference imaging so minimum durations must be available\\
At line 608 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 467 changed one line
!ar091216-11. CORE EIS Flare Study
!ar20091216-10 => CORE EIS Flare Study 1
At line 475 changed 3 lines
-- run for 2 hr; data volume: 36 Mbit\\
-- target: any AR with significant flare probability\\
}]
-- run for as long as possible with available TLM; data volume: 37 Mbit/hr\\
-- target: any AR with significant flare probability\\
-- see [http://www.mssl.ucl.ac.uk/www_solar/eisflarestudy.html] for further details\\
}}
At line 629 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 482 changed one line
!!! C. Test and Calibration Studies \\
!ar20091229-11 => CORE EIS Flare Study 2
At line 484 changed one line
!test-01. EIS slit calibration
  – Hara ([hara@solar.mtk.nao.ac.jp|mailto:hara@solar.mtk.nao.ac.jp])\\
At line 640 added 288 lines
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- study used to search for flow structures in flares\\
-- 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\\
-- see [http://www.mssl.ucl.ac.uk/www_solar/eisflarestudy.html] for further details\\
}}
%%
%%center
||Study ID||Acronym|| ||
|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]
%%
\\
!ar20100417-13 => Nanoflare heating of coronal loops
  – 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])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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\\
}}
%%
%%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]
|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]
%%
\\
!ar20100423-14 => Active Region Transient Brightening Lite
  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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]
%%
\\
!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)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|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]
%%
\\
!ar20100426-16 => Outflows from Small Active Regfions
  – 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 \\
!test-01 => EIS slit calibration
At line 491 changed one line
-- run CALIB_slit_slot_v1\\
-- run CALIB_slit_slot_v2 (ID # 389)\\
At line 494 changed one line
-- make two separate adjacent entries of calib_slit_slot_v1 on the timeline\\
-- make two separate adjacent entries of calib_slit_slot_v2 on the timeline\\
At line 499 changed one line
-- data volume: 54 Mbits.\\
-- data volume: 35 Mbits\\
-- duration: 56m.\\
At line 945 added 4 lines
%%center
||Study ID||Acronym|| ||
|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 950 added one line
At line 505 changed one line
!test-02. EIS velocity calibration
!test-02 => EIS velocity calibration
At line 513 changed one line
-- run ID 375 SK_DEEP_5x512_SLIT1 \u2013 the 1" slit study, with Y initial positions\\
-- run ID 375 SK_DEEP_5x512_SLIT1 - the 1" slit study, with Y initial positions\\
At line 515 changed one line
-- run ID 376 SK_DEEP_10x512_SLIT2 \u2013 the 2" slit study, with Y initial positions\\
-- run ID 376 SK_DEEP_10x512_SLIT2 - the 2" slit study, with Y initial positions\\
At line 970 added 5 lines
%%center
||Study ID||Acronym|| ||
|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 one line
At line 979 added 29 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\\
}}
%%
%%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