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182 04-Apr-2011 15:19 43 KB JianSun to previous | to last
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[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
[{ALLOW view jsun,eiscorestudy}]
[{ALLOW edit jsun}]
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%%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 study qs20091216-09 has been replaced by a new study (ie.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 study ar20100329-12 has been replaced by a new study (ie.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 study ar20110209-20 has been replaced by a new study (ie.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
}}
%%
[Possible EIS Core Team Studies (2009-Dec-01)|http://docs.google.com/Doc?docid=0AdazsPAS3_6xZGNzZHFiOWhfMTY2ZjQ3cG1oZGQ&hl=en&invite=CIDL2K4H]\\
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[{TableOfContents}]
\\
%%(text-align:center;font-size:20px;bold;)
!!!Available EIS Core Team Studies
%%(text-align:center;font-size:25px;bold;)
Available EIS Core Team Studies
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!!A. Quiet Sun\\
!!!Quiet Sun\\
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!qs20091216-01 => Evolution of X-ray bright point
!1. Evolution of X-ray bright point – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\
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  – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\
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-- 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\\
-- run SK_QS_34x168c (ID # 295) for BP study; data volume: 2.1 Mbit; dur: 3m 49s\\
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-- 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\\
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%%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]
%%
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!qs20091216-02 => Coronal/TR Doppler & photosphere transverse magnetic features and cancellation events
!2. Coronal/TR Doppler & photosphere transverse magnetic features and cancellation events – Yokoyama ([yokoyama.t@eps.s.u-tokyo.ac.jp|mailto:yokoyama.t@eps.s.u-tokyo.ac.jp])\\
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  – Yokoyama ([yokoyama.t@eps.s.u-tokyo.ac.jp|mailto:yokoyama.t@eps.s.u-tokyo.ac.jp])\\
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-- run studies in the order: three times (a) - n times (b) - three times (a)\\
-- run studies in the order: three times (a) - n times (b) \u2013 three times (a)\\
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%%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]
%%
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!qs20091216-03 => QS Brightenings
!3. QS Brightenings – Bewsher ([d.bewsher@rl.ac.uk|mailto:d.bewsher@rl.ac.uk]), Young \\
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  – Bewsher ([d.bewsher@rl.ac.uk|mailto:d.bewsher@rl.ac.uk]), Young \\
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%%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]
%%
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!qs20091216-04 => Search for Evidence of Wave Activity in the Solar Corona
!4. Search for Evidence of Wave Activity in the Solar Corona - Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk]), Harrison ([richard.harrison@stfc.ac.uk|mailto:richard.harrison@stfc.ac.uk])\\
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  – Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk]), Harrison ([richard.harrison@stfc.ac.uk|mailto:richard.harrison@stfc.ac.uk])\\
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%%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]
%%
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!qs20091216-05 => X-ray Bright Points Onset
!5. X-ray Bright Points Onset – Brown ([dsbrown@uclan.ac.uk|mailto:dsbrown@uclan.ac.uk]), Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk])\\
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  – Brown ([dsbrown@uclan.ac.uk|mailto:dsbrown@uclan.ac.uk]), Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk])\\
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%%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]
%%
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!qs20091216-06 => Coronal Jets
!6. Coronal Jets – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra \\
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  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra \\
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%%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]
%%
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!qs20091216-07 => Quiet Sun diagnostics/evolution
!7. Quiet Sun diagnostics/evolution - Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
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  – Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
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%%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]
%%
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!qs20091216-08 => Coronal Hole Density Measurement
!8. Coronal Hole Density Measurement – Young ([peter.young.ctr.uk@nrl.navy.mil|mailto:peter.young.ctr.uk@nrl.navy.mil]) \\
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  – Young ([peter.young.ctr.uk@nrl.navy.mil|mailto:peter.young.ctr.uk@nrl.navy.mil]) \\
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%%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]
%%
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!qs20091216-10 => Properties in Solar Wind Source Regions
!9. Eclipse Spectral Atlas - Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
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  – 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
{{
-- 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\\
}}
%%
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\\
!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]) \\
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-- 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\\
-- 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\\
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%%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]
%%
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!qs20091216-11 => Quiet sun dynamics study
!11. Quiet sun dynamics study – Muglach __\\
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  – Muglach __\\
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%%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]
%%
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!qs20091216-12 => Filament Evolution
!12. Filament Evolution – Green ([lmg@mssl.ucl.ac.uk|mailto:lmg@mssl.ucl.ac.uk])\\
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  – Green ([lmg@mssl.ucl.ac.uk|mailto:lmg@mssl.ucl.ac.uk])\\
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%%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]
%%
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!qs20091216-13 => Interchange Reconnection at CH Boundaries
!13. Interchange Reconnection at CH Boundaries – Baker ([db2@mssl.ucl.ac.uk|mailto:db2@mssl.ucl.ac.uk]), Van Driel ([lidia.vandriel@obspm.fr|mailto:lidia.vandriel@obspm.fr]) search for closed/open field interactions at CH boundaries with adjacent activity\\
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  – Search for closed/open field interactions at CH boundaries with adjacent activity\\
  – Baker ([db2@mssl.ucl.ac.uk|mailto:db2@mssl.ucl.ac.uk]), Van Driel ([lidia.vandriel@obspm.fr|mailto:lidia.vandriel@obspm.fr]) \\
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%%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]
%%
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!!B. EIS HOP Obs.\\
----
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!hop-a => EIS CORE HOP 80
!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])\\
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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])\\
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!hop-b => EIS CORE HOP 130
!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])\\
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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])\\
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!hop-c => EIS CORE HOP 146
!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])\\
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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])\\
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!hop-d => EIS CORE HOP 137
!EIS CORE HOP 137: Evolution of Network Boundary Elements: Possible Connections to the Corona – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
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Evolution of Network Boundary Elements: Possible Connections to the Corona\\
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  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
----
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\\
!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"\\
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!hop-f => EIS CORE HOP 150 (ToO)
!!! B. Active Region, Flare, CME\\
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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\\
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Useful AR context studies for before/after main AR observation are: PRY_slot_context_v3 or PRY_slot_contextLITE
{{Useful AR context studies for before/after main AR observation are: PRY_slot_context_v3 or PRY_slot_contextLITE}}
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!ar20091216-01 => Active Region Studies
!1. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska\\
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  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska\\
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%%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]
%%
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!ar20091216-02 => AR dynamics and CME watch
!2. AR dynamics and CME watch – Young, Ugarte-Urra \\
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  – 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])\\
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%%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]
%%
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!ar20091216-03 => Active Region Studies
!3. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
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  – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
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%%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]
%%
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!ar20091216-04 => Active Region Abundance Variations
!14/12/09: Active Region Abundance Variations - Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil])
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  – Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil])
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%%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]
%%
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!ar20091216-05 => Pre-flare activity monitoring
!4. 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\\
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  – Wallace ([ajw2@mssl.ucl.ac.uk|mailto:ajw2@mssl.ucl.ac.uk])\\
%%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__\\
}}
%%
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\\
!5. Pre-flare activity monitoring - Wallace ([ajw2@mssl.ucl.ac.uk|mailto:ajw2@mssl.ucl.ac.uk])\\
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%%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]
%%
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!ar20091216-06 => Search for Active Region outflows
!6. Search for Active Region outflows – Culhane ([jlc@mssl.ucl.ac.uk|mailto:jlc@mssl.ucl.ac.uk]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])\\
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  – Culhane ([jlc@mssl.ucl.ac.uk|mailto:jlc@mssl.ucl.ac.uk]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])\\
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%%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]
%%
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!ar20091216-07 => AR Temperature Diagnostic
  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
!7. AR Temperature Diagnostic – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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  -- exposure time: 45s; raster: scanning; slit: 2"; step Size: 2", FOV: 322"X376";\\
  -- raster duration: 2h13m15s; Data volume: 186 Mbits;\\
  -- exposure time: 30s; raster: scanning; slit: 2"; step Size: 2", FOV: 360"X400";\\
  -- raster duration: 1h40m46s \\
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%%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]
%%
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!ar20091216-08 => High cadence observations of AR transient brightenings and microflares
!8. High cadence observations of AR transient brightenings and microflares - Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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-- run context study PRY_slot_context_v3 before and after\\
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%%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]
%%
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!ar20091216-09 => CME onsets
!9. CME onsets - Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison\\
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  – Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison([Richard.Harrison@stfc.ac.uk|mailto:Richard.Harrison@stfc.ac.uk])\\
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-- 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\\
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-- 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__\\
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-- algorithm uses difference imaging so minimum durations must be available\\
-- algorithm uses difference imaging so minimum durations __must__ be available\\
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%%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]
%%
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!ar20091216-10 => CORE EIS Flare Study 1
!10. CORE EIS Flare Study – Milligan ([ryan.o.milligan@nasa.gov|mailto:ryan.o.milligan@nasa.gov])\\
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  – Milligan ([ryan.o.milligan@nasa.gov|mailto:ryan.o.milligan@nasa.gov])\\
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-- 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\\
}}
-- run for 2 hr; data volume: 36 Mbit\\
-- target: any AR with significant flare probability\\
}]
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%%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]
%%
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!ar20091229-11 => CORE EIS Flare Study 2
!!!C. Test and Calibration Studies \\
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  – Hara ([hara@solar.mtk.nao.ac.jp|mailto:hara@solar.mtk.nao.ac.jp])\\
!1. EIS slit calibration – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
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-- 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\\
-- Obtain co-spatial data in the 1", 2" and 40" slits for various calibration tests (slit widths, tilt, intensity calibration)\\
-- run CALIB_slit_slot_v1\\
-- study includes three separate rasters; each must be individually pointed\\
-- point off-limb above the quiet Sun at the equator (either limb)\\
-- make two separate adjacent entries of calib_slit_slot_v1 on the timeline\\
-- select Solar-X position 50-60” above limb; same for each of the rasters in both study entries\\
-- select Y position with the YIP input rather than the solar-Y position\\
-- set the YIP entry to 511 for each of the three rasters in first study entry \\
-- for the second study entry, set YIP to 1 for each of the three rasters\\
-- data volume: 54 Mbits.\\
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%%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]
\\
!2. EIS velocity calibration – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\
[{ALLOW view jsun,eiscorestudy}]
[{ALLOW edit jsun}]
[Possible EIS Core Team Studies (2009-Dec-01)|http://docs.google.com/Doc?docid=0AdazsPAS3_6xZGNzZHFiOWhfMTY2ZjQ3cG1oZGQ&hl=en&invite=CIDL2K4H]\\
%%(text-align:center;font-size:25px;bold;)
Available EIS Core Team Studies
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!ar20100417-13 => Nanoflare heating of coronal loops
!!!Quiet Sun\\
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  – 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])\\
!1. Evolution of X-ray bright point – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\
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-- 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\\
-- point to a quiet region with an X-ray bright point near disk centre\\
-- run IUU_SLOT_136x400_Q65 (ID # 292) for context\\
-- data volume: 12.1 Mbit; duration: 15m 41s\\
-- run SK_QS_34x168c (ID # 295) for BP study; data volume: 2.1 Mbit; dur: 3m 49s\\
-- run for 3 hours or longer \\
-- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to track evolution of magnetic fields in the photosphere\\
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%%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]
%%
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!ar20100423-14 => Active Region Transient Brightening Lite
!2. Coronal/TR Doppler & photosphere transverse magnetic features and cancellation events – Yokoyama ([yokoyama.t@eps.s.u-tokyo.ac.jp|mailto:yokoyama.t@eps.s.u-tokyo.ac.jp])\\
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  – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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-- 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
-- QS near the disk centre, if possible, include an XBP in FOV for alignment\\
-- observation structure similar to the Muglach programme\\
-- run studies in the order: three times (a) - n times (b) \u2013 three times (a)\\
-- a) Study: quiet_sun_slot (#210); 40x512 slot image as context; volume: 1.4Mbits, \\
-- duration: 1.5min, rate:16.4kbps\\
-- three images should be taken before and after program b)\\
-- b) Study: sta_loop_context_lo (#278); vol: 23.3Mbits, dur: 34min, rate: 34kbps\\
-- repeat n times to fit into available data volume\\
-- EXPOSURE: 30s, RASTER: 60 steps, SLIT: 2", STEP: 2" FOV: 120"x248"\\
-- __SOT __support: FG/NFI: NaI/IV 2-wavelength filter (mandatory)\\
&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)\\
-- SP: fast mapping, FOV: same as FG/NFI (mandatory)\\
-- FG/BFI: CaII/G-band (lowest priority, can be omitted)\\
-- __XRT __support: FOV: cover the same FOV as SOT Filters: low-temperature filter-pair; Cadence: <5min\\
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%%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]
%%
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!ar20100423-15 => Multi-temperature Observation of Sigmoids
!3. QS Brightenings – Bewsher ([d.bewsher@rl.ac.uk|mailto:d.bewsher@rl.ac.uk]), Young \\
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&nbsp; – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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-- run cam_sigmoid_study_v1\\
-- observe temperature structure of cooling plasma in sigmoidal structures on newly reconnected flux rope field lines\\
-- &nbsp; select small to medium size ARs; the AR should be in the centre of the raster\\
-- &nbsp; exposure time: 10s; raster scanning; slit: 2"; step size: 2"; FOV: 400" x 400"\\
-- &nbsp; raster duration: 41m33s; data volume: 125 Mbits\\
-- &nbsp; repeat to fill available time slot; minimum of 4 repeats preferred (needs 500 Mbits)\\
-- EIS to point at quiet Sun region near disk centre \\
-- run following studies:\\
&nbsp; -- PRY_slot_context_v3 (dur: 3min; vol: 3 Mbit) once at start of observation\\
&nbsp; -- tr_bright_lo (dur: 6min; vol: 1.5 Mbit) repeatedly to fill available time slot\\
&nbsp; -- PRY_slot_context_v3 again, once at end of observation\\
&nbsp; -- run tr_bright_lo for minimum of 4h; longer if possible\\
-- request SOT and XRT to observe EIS FoV: 20” x 144”\\
-- SOHO/CDS involvement desirable; __advise schedule to Bewsher__\\
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%%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]
%%
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!4. Search for Evidence of Wave Activity in the Solar Corona - Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk]), Harrison ([richard.harrison@stfc.ac.uk|mailto:richard.harrison@stfc.ac.uk])\\
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!ar20100426-16 => Outflows from Small Active Regfions
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run__ __rah_line_narrow; duration: 1 h 5 m 20 s; data volume: 24 Mbits\\
-- run for 6 hour min (~ 144Mbits); longer if possible; repeat to fill time slot\\
-- point to the off limb ‘quiet’ solar corona above the equator; solar y = 0; limb should be in the fov; planner should maximise the altitude observable\\
-- request SOT and XRT to observe EIS fov (238 x 256”)\\
-- __CDS involvement essential,__ __advise schedule to Bewsher – note email change__\\
}}
%%
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&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
\\
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!5. X-ray Bright Points Onset – Brown ([dsbrown@uclan.ac.uk|mailto:dsbrown@uclan.ac.uk]), Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk])\\
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-- observe small ARs simultaneously with QS regions to obtain accurate outflow velocities\\
-- run PRY_loop_velocity\\
-- &nbsp; duration: 4h33m; volume:230 Mbits\\
-- &nbsp; position AR near top or bottom of slit; see example at *[http://tiny.cc/qccji|http://tiny.cc/qccji]*\\
-- &nbsp; ensure that any fan loops visible in 171 Å images are contained within raster\\
-- &nbsp; avoid complex ARs\\
-- EIS to point at quiet Sun region near disk centre \\
-- target QS magnetic fragments as seen by SOT with little/no emission in the corona\\
-- run the following studies:\\
&nbsp; -- PRY_slot_context_v2 (dur 3 min; vol 3 Mbit) once at start of observation\\
&nbsp; -- dob_bp_slit_raster (dur 33m 50s; vol 7 Mbit) or dob_bp_slot_raster (dur 2m 13s; vol 7 Mbit); repeat to fill available time slot\\
&nbsp; -- PRY_slot_context_v2 at end of observations\\
&nbsp; -- run dob_bp_****_raster for minimum 4h; run both studies on different days\\
&nbsp; -- request SOT and XRT to observe EIS FoV: 120x160" (dob_bp_slit_raster) or 160x160" (dob_bp_slot_raster)\\
&nbsp; -- TRACE/CDS involvement desirable; __advise schedule to Brown and Bewsher__\\
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%%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]
%%
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!6. Coronal Jets – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra \\
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!ar20100622-17 => AR Temperatures and Flows Optimized for Eclipse Observing
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- measure DEM in jet reconnection region\\
-- run slot_context_lite_v1 before/after IUU_SCAN_STEPS_002 in N- polar CH\\
-- place raster (slit: 368") so that part covers adjacent Quiet Sun\\
-- run for as long as possible outside of eclipse\\
}}
%%
At line 755 changed one line
&nbsp; – Warren ([harry.warren@nrl.navy.mil|mailto:harry.warren@nrl.navy.mil])\\
\\
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!7. Quiet Sun diagnostics/evolution - Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
At line 759 changed 6 lines
-- run hpw021_vel_120x512v1\\
-- &nbsp; duration should allow it to be run between eclipses; can be run multiple times to cover a larger area; avoid SAA.\\
-- &nbsp; target: active region\\
-- &nbsp; full slit is taken; position active region near top or bottom of slit so that there is ample quiet Sun for velocity calibration.\\
-- &nbsp; exposure time: 60s; raster: scanning; slit: 1"; step Size: 2", FOV: 120"x512";\\
-- &nbsp; raster duration:1h4m58s; data volume: 135 Mbits \\
-- point to a generic quiet Sun region (solar tracking). Two study sequences:\\
&nbsp; a) run NRL_QSCH_30X400_90s2 multiple times (3 at least)\\
&nbsp; b) run IUU_SLOT_488x512 as context\\
&nbsp; &nbsp; -- run HPW019AR_1x400_45s (sit-and-stare) for 2 hours\\
&nbsp; &nbsp; -- run IUU_SLOT_488X512 as context\\
-- Note: ideally run sequences one after the other on the same pointing. \\
-- sequences can run independently of each other if needed. \\
-- SOT magnetograms and XRT C_poly or Al_poly observations desirable, matching EIS cadence (1-2 min) in sequence b)\\
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%%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]
%%
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!8. Coronal Hole Density Measurement – Young ([peter.young.ctr.uk@nrl.navy.mil|mailto:peter.young.ctr.uk@nrl.navy.mil]) \\
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!ar20101109-18 => Dynamic events at the limb with EIS and AIA
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- polar or equatorial CH\\
-- select pointing based on EIT 195 images; choose darkest part of CH\\
-- accurate warm pixel removal essential for CH data\\
-- run REGCAL071 and REGCAL072 on the same day; also context study\\
-- study sequence is: REGCAL071; REGCAL072; PRY_slot_context_v2 ;\\
-- PRY_CH_density\\
-- run on mid-latitude extension to N-polar CH\\
Note 1: repeat PRY_CH_density to fill time slot; vol: 20 Mbit; data rate: 5.2 kbps\\
Note 2: for large dark CH areas, stitch two or more repeats of PRY_CH_density\\
}}
%%
At line 778 changed one line
&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
\\
At line 601 added 2 lines
!9. Eclipse Spectral Atlas - Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
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-- 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 \\
-- 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\\
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%%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]
%%
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!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]) \\
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!ar20110120-19 => AR Loop footpoint studies using the bright point trigger
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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\\
-- 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__\\
}}
%%
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&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
\\
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!11. Quiet sun dynamics study – Muglach __\\
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-- 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\\
&nbsp;&nbsp; (ID: 444, 268 Mbits, 2hr 52m)\\
-- BP trigger parameters are given in the Hunter_loop_fe8 study description, but change the Xthresh \\
&nbsp;&nbsp; value to 5000 (instead of 5460)\\
-- run studies in the order: three times (a) - n times (b) – three times (a)\\
&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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%%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]
%%
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\\
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\\
!12. Filament Evolution – Green ([lmg@mssl.ucl.ac.uk|mailto:lmg@mssl.ucl.ac.uk])\\
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%%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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!ar20110404-21 => Search for slow mode oscillations in coronal loops
\\
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&nbsp; – Wang ([tongjiang.wang@nasa.gov|mailto:tongjiang.wang@nasa.gov]), Mariska ([john.mariska@nrl.navy.mil|mailto:john.mariska@nrl.navy.mil])\\
!13. Interchange Reconnection at CH Boundaries – Baker ([db2@mssl.ucl.ac.uk|mailto:db2@mssl.ucl.ac.uk]), Van Driel ([lidia.vandriel@obspm.fr|mailto:lidia.vandriel@obspm.fr]) search for closed/open field interactions at CH boundaries with adjacent activity\\
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-- 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 \\
&nbsp;&nbsp; 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)\\
-- 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__\\
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%%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]
%%
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\\
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----
!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])\\
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!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])\\
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!ar20110411-22 => Cambridge Diagnostic Study for the Impulsive Phase of Small Flares
\\
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&nbsp; – 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])\\
!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])\\
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\\
!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}}
%%
\\
!1. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska\\
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-- 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\\
-- Studies HPW017AR_30x400_30s2, HPW018AR300x400_30s2 and \\
-- HPW019AR_1x400_45s2\\
-- select as appropriate for AR ToO\\
-- use PRY_slot_context_v3 or PRY_slot_contextLITE before/after selected HPW\\
-- check with Harry Warren re ASRC for raster expansion\\
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%%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]
%%
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!2. AR dynamics and CME watch – Young, Ugarte-Urra \\
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!!D. Synoptic and Other Studies\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 40” slot for large FoV, high cadence AR images in a wide Te range to i) examine loop morphology ii) detect CME initiation. \\
-- run either i) PRY_slot_context_v3 (AR dynamics, includes diagnostics) or ii) PRY_slot_contextLITE (488”x488”; 3.5min); (CME watch, low TLM, extended hours)\\
-- repeat to fill available time slot; run for 3 hours, preferably longer\\
}}
%%
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!syo20100504-01 => EIS Spectral Atlas Synoptic Programme
\\
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&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil]), Warren, Mason, Del Zanna\\
!3. Active Region Studies – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
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-- 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\\
-- &nbsp; *NOTE: use Atlas_30s only if an AR is forecast to produce M-class or greater flares; use Atlas_60s for all other targets*\\
-- observe the large dispersing AR near CM\\
-- run a large raster with HPW018\\
-- run a fast scan with IUU_SCAN_STEPS_002 for several hours\\
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%%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]
%%
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\\
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\\
!14/12/09: Active Region Abundance Variations - Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil])
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%%roundedCorners-yyyy-E3F0EE-808080
{{
-- target: young AR of less than 3 days; search for any abundance evolution\\
-- FoV to cover centre of the AR\\
-- run study twice a day; separate runs by ~ 12 hours; run for 7 consecutive days until AR west limb passage or decay - subject to TLM limitations\\
-- run YKK_ARabund01; raster scanning: 2” slit and 3” step; exposure: 45s; FOV: 194"x280; duration: 53 m 19s; Data: DCPM/64Mbit.\\
-- run PRY_slot_contextLITE for context after each raster\\
}}
%%
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!syo20100713-02 => Full CCD Study to Measure Relative Wavelengths
\\
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&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\
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!4. 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\\
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-- 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\\
-- 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: \\
&nbsp; - PRY_footpoints_lite once at beginning of a period \\
&nbsp; - sta_loop_slot_lo at the same pointing\\
&nbsp; - repeat sta_loop_slot_lo to fill available time slot.\\
-- __run on any quiescent AR; advise schedule to de Moortel__\\
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%%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]
%%
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!!E. Test and Calibration Studies \\
!5. Pre-flare activity monitoring - Wallace ([ajw2@mssl.ucl.ac.uk|mailto:ajw2@mssl.ucl.ac.uk])\\
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!test-01 => EIS slit calibration
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- point to a flaring AR to search for features that precede flares\\
&nbsp; -- run Flare0_slit_AJW; (dur: 50m 34s; vol: 2.9 Mbits; size: 180” x 320”)\\
&nbsp; -- scanning raster; slit: 2”; step:2”; exposure: 30s; 89 steps.\\
-- run repeatedly on a flaring AR to fill available time allocation.\\
}}
%%
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&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
\\
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!6. Search for Active Region outflows – Culhane ([jlc@mssl.ucl.ac.uk|mailto:jlc@mssl.ucl.ac.uk]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])\\
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-- Obtain co-spatial data in the 1", 2" and 40" slits for various calibration tests (slit widths, tilt, intensity calibration)\\
-- run CALIB_slit_slot_v2 (ID # 389)\\
-- study includes three separate rasters; each must be individually pointed\\
-- point off-limb above the quiet Sun at the equator (either limb)\\
-- make two separate adjacent entries of calib_slit_slot_v2 on the timeline\\
-- select Solar-X position 50-60” above limb; same for each of the rasters in both study entries\\
-- select Y position with the YIP input rather than the solar-Y position\\
-- set the YIP entry to 511 for each of the three rasters in first study entry \\
-- for the second study entry, set YIP to 1 for each of the three rasters\\
-- data volume: 35 Mbits\\
-- duration: 56m.\\
-- observe AR outflows at opposite boundaries of the large dispersing AR near CM\\
-- run HPW015_DETAILED_MAP_1_45s_200x360 twice; two separate pointings\\
-- total data volume: 662 Mbits; duration: 2 x 2h 44 m or 5h 28 m total\\
-- __check pointing positions with proposers__\\
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%%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]
\\
!7. AR Temperature Diagnostic – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run cam_ar_limb_lite_v2\\
-- target: temperature structure of active regions on the limb\\
&nbsp; -- centre raster at the active region core.\\
&nbsp; -- exposure time: 30s; raster: scanning; slit: 2"; step Size: 2", FOV: 360"X400";\\
&nbsp; -- raster duration: 1h40m46s \\
}}
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\\
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\\
!8. High cadence observations of AR transient brightenings and microflares - Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\
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!test-02 => EIS velocity calibration
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run cam_artb_lite_v2\\
-- run on AR to study transient brightenings and microflares at very high cadence\\
-- raster centre should be at polarity inversion line.\\
-- raster: scanning; slit: 2", step size: 2"; FOV: 40"X120"\\
-- raster duration: 4m32 seconds\\
-- run as many times as possible and at least for 3-4 hours continuous \\
}}
%%
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&nbsp; – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\
\\
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!9. CME onsets - Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison\\
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-- Determine the slit tilt and curvature in full Y height for velocity calibration\\
-- execute raster scans at three positions with 1" and 2" slits\\
-- run ID 375 SK_DEEP_5x512_SLIT1 - the 1" slit study, with Y initial positions\\
&nbsp;&nbsp; #1 YIP=1; #2 YIP=256; #3 YIP=512\\
-- run ID 376 SK_DEEP_10x512_SLIT2 - the 2" slit study, with Y initial positions\\
&nbsp;&nbsp; #4 YIP=1; #5 YIP=256; #6 YIP=512\\
-- six consecutive rasters require total time ~ 60min and data volume ~ 45Mbits\\
-- target: quiet region near disk center (0", 0"); shift EIS FOV ±200" in E-W direction to avoid ARs; do not run if ARs in target area;\\
-- keep the same mirror initial position (MIP) for all rasters.\\
-- algorithm to detect CME-related dimming\\
-- point above limb __at AR if it develops __with part of limb in FoV\\
-- if AR present, centre raster y-direction on the AR; null evaluation in AR absence\\
-- run cmeo_slit_lo; minimum 5 rasters; Duration: 4.2 h; Volume: 13 Mbit __or__\\
-- run cmeo_slot_lo; min duration: 5 h; Volume: 10 Mbit\\
-- algorithm uses difference imaging so minimum durations __must__ be available\\
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%%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]
%%
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\\
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!10. CORE EIS Flare Study – Milligan ([ryan.o.milligan@nasa.gov|mailto:ryan.o.milligan@nasa.gov])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run FLR001_flare_study; \\
-- exposure: 5s; raster: scanning; slit: 2”; step: 2”; FoV: 80” x 120”; raster time: 5m\\
-- run for 2 hr; data volume: 36 Mbit\\
-- target: any AR with significant flare probability\\
}]
%%
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!test-03 => EIS Slot Deconvolution Test
!!!C. Test and Calibration Studies \\
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&nbsp; – Sun ([js2@mssl.ucl.ac.uk|mailto:js2@mssl.ucl.ac.uk])\\
!1. EIS slit calibration – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
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-- Develop method to deconvolve EIS slot data\\
-- Two studies:\\
&nbsp;&nbsp; * js2_decon_slot_sc_LT (ID # 429): data volume: 3.71Mbits; duration: 1m51s\\
&nbsp;&nbsp; * js2_decon_ref_vel_LT (ID # 430): data volume: 87.87Mbits; duration: 47m37s\\
-- Instructions for planner:\\
&nbsp;&nbsp; - Run study (ID # 429) first, then consecutively run study (ID # 430), then run study (ID # 429) again.\\
&nbsp;&nbsp; - It's prefer that the slot study (ID # 429) repeats a few times, \\
&nbsp;&nbsp;&nbsp;&nbsp; eg. study429 (x6), study430 (x1), study429 (x6) \\
-- Target: \\
&nbsp;&nbsp; - simple active region; \\
&nbsp;&nbsp; - FoV to cover AR edge to detect outflows; \\
&nbsp;&nbsp; - both rasters to have identical pointing\\
-- Run during SAA-free interval preferred\\
-- Determine the slit tilt and curvature in full Y height for velocity calibration\\
-- execute raster scans at three positions with 1" and 2" slits\\
-- run ID 375 SK_DEEP_5x512_SLIT1 – the 1" slit study, with Y initial positions\\
#1 YIP=1; #2 YIP=256; #3 YIP=512\\
-- run ID 376 SK_DEEP_10x512_SLIT2 – the 2" slit study, with Y initial positions\\
#4 YIP=1; #5 YIP=256; #6 YIP=512\\
-- six consecutive rasters require total time ~ 60min and data volume ~ 45Mbits\\
-- target: quiet region near disk center (0", 0"); shift EIS FOV ±200" in E-W direction to avoid ARs; do not run if ARs in target area;\\
-- keep the same mirror initial position (MIP) for all rasters.\\
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%%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]
%%
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\\
\\
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop