[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]


%%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 study qs20091216-09 has been replaced by a new study (ie.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 study ar20100329-12 has been replaced by a new study (ie.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 study ar20110209-20 has been replaced by a new study (ie.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
}}
%%

[{TableOfContents}]

\\

%%(text-align:center;font-size:20px;bold;)
!!!Available EIS Core Team Studies
%%

\\

!!A. Quiet Sun\\ 

!qs20091216-01 => Evolution of X-ray bright point

  – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=295] (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\\
}}
%%
%%center
||Study ID||Acronym|| ||
|292|IUU_SLOT_136x400_Q65|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=292]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=292]
|295|SK_QS_34x168c|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=295]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=295]
%%


\\

!qs20091216-02 => 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])\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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) - 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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|210|quiet_sun_slot|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=210]
|278|sta_loop_context_lo|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=278]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=278]
%%


\\

!qs20091216-03 => QS Brightenings

&nbsp; – Bewsher ([d.bewsher@rl.ac.uk|mailto:d.bewsher@rl.ac.uk]), Young \\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|251|tr_bright_lo|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=251]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=251]
%%


\\

!qs20091216-04 => Search for Evidence of Wave Activity in the Solar Corona

&nbsp; – Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk]), Harrison ([richard.harrison@stfc.ac.uk|mailto:richard.harrison@stfc.ac.uk])\\ 

%%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__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|337|rah_line_narrow|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=337]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=337]
%%


\\ 


!qs20091216-05 => X-ray Bright Points Onset

&nbsp; – Brown ([dsbrown@uclan.ac.uk|mailto:dsbrown@uclan.ac.uk]), Bewsher ([dbewsher@uclan.ac.uk|mailto:dbewsher@uclan.ac.uk])\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|285|dob_bp_slit_raster|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=285]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=285]
|284|dob_bp_slot_raster|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=284]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=284]
%%


\\

!qs20091216-06 => Coronal Jets

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra \\ 

%%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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|354|PRY_slot_contextLITE|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|358|IUU_SCAN_STEPS_002|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=358]
%%


\\

!qs20091216-07 => Quiet Sun diagnostics/evolution

&nbsp; – Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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)\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|322|NRL_QSCH_30X400_90s2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=322]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=322]
|378|IUU_SLOT_488x512|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=378]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=378]
|336|HPW019AR_1x400_45s|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=336]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=336]
%%


\\

!qs20091216-08 => Coronal Hole Density Measurement

&nbsp; – Young ([peter.young.ctr.uk@nrl.navy.mil|mailto:peter.young.ctr.uk@nrl.navy.mil]) \\ 

%%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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|249|PRY_slot_context_v2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=249]
|268|PRY_CH_density|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=268]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=268]
%%


\\

!qs20091216-10 => Properties in Solar Wind Source Regions

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]) \\

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- target: equatorial or low-latitude coronal hole within ± 40%%sup o%% latitude; Polar CH extensions also possible if within ± 40%%sup o%%; 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__\\
}}
%%
%%center
||Study ID||Acronym|| ||
|330|YKK_EqCH_02n|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=330]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=330]
|329|YKK_EqCH_02w|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=329]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=329]
|249|PRY_slot_context_v2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=249]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=249]
%%


\\

!qs20091216-11 => Quiet sun dynamics study

&nbsp; – Muglach __\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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)\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|210|quiet_sun_slot|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=210]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=210]
|315|KM-qs-study-low|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=315]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=315]
%%


\\ 

!qs20091216-12 => Filament Evolution

&nbsp; – Green ([lmg@mssl.ucl.ac.uk|mailto:lmg@mssl.ucl.ac.uk])\\ 

%%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__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|254|cme_slot_red_lkh|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=254]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=254]
|255|cme_slit_red_lkh|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=255]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=255]
%%


\\

!qs20091216-13 => Interchange Reconnection at CH Boundaries

&nbsp; – Search for closed/open field interactions at CH boundaries with adjacent activity\\
&nbsp; – Baker ([db2@mssl.ucl.ac.uk|mailto:db2@mssl.ucl.ac.uk]), Van Driel ([lidia.vandriel@obspm.fr|mailto:lidia.vandriel@obspm.fr]) \\

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- run dhb_polar_scan_Q90 (ID #294); \\ 
-- check with proposers for pointing details\\ 
-- __run for small closed structures at CH boundaries or inside on-disc CHs__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|294|dhb_polar_scan_Q90|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=294]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=294]
%%


\\

!!B. EIS HOP Obs.\\ 

!hop-a => EIS CORE HOP 80

Polar Coronal Hole Observation\\

&nbsp; – 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])\\

\\

!hop-b => EIS CORE HOP 130

Multi-temperature Full Disk Slot Scans\\

&nbsp; – 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])\\ 

\\

!hop-c => EIS CORE HOP 146

Solar Wind Source Regions During Solar Minimum Conditions\\

&nbsp; – Kuen Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil]), Mariska ([mariska@nrl.navy.mil|mailto:mariska@nrl.navy.mil])\\ 

\\ 

!hop-d => EIS CORE HOP 137

Evolution of Network Boundary Elements: Possible Connections to the Corona\\

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\ 

\\ 

!hop-e => EIS CORE HOP 131 (ToO)

Helioseismology Observations of Coronal Holes with SOT\\

&nbsp; – 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"\\

\\

!hop-f => EIS CORE HOP 150 (ToO)

Flows during a filament eruption\\

&nbsp; – 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\\

&nbsp; – 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\\

&nbsp; – 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\\ 

%%information
Useful AR context studies for before/after main AR observation are: PRY_slot_context_v3 or PRY_slot_contextLITE
%%

\\ 

!ar20091216-01 => Active Region Studies

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Mariska\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|355|HPW017AR_30x400_30s2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=355]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=355]
|356|HPW018AR300x400_30s2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=356]
|357|HPW019AR_1x400_45s2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=357]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=357]
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|354|PRY_slot_contextLITE|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
%%


\\

!ar20091216-02 => AR dynamics and CME watch

&nbsp; – 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])\\ 

%%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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|354|PRY_slot_contextLITE|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
%%


\\

!ar20091216-03 => Active Region Studies

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil]), Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\

%%roundedCorners-yyyy-E3F0EE-808080
{{
--     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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|356|HPW018AR300x400_30s2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=356]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=356]
|358|IUU_SCAN_STEPS_002|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=358]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=358]
%%


\\ 

!ar20091216-04 => Active Region Abundance Variations

&nbsp; – Ko ([yko@ssd5.nrl.navy.mil|mailto:yko@ssd5.nrl.navy.mil])

%%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\\
}}
%%
%%center
||Study ID||Acronym|| ||
|381|YKK_ARabund01|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=381]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=381]
|354|PRY_slot_contextLITE|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
%%


\\


!ar20091216-05 => Pre-flare activity monitoring

&nbsp; – Wallace ([ajw2@mssl.ucl.ac.uk|mailto:ajw2@mssl.ucl.ac.uk])\\ 

%%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.\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|286|Flare0_slit_AJW|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=286]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=286]
%%


\\

!ar20091216-06 => Search for Active Region outflows

&nbsp; – Culhane ([jlc@mssl.ucl.ac.uk|mailto:jlc@mssl.ucl.ac.uk]), Harra ([lkh@mssl.ucl.ac.uk|mailto:lkh@mssl.ucl.ac.uk])\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
--     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__\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|243|HPW015_DETAILED_MAP|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=243]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=243]
%%


\\

!ar20091216-07 => AR Temperature Diagnostic

&nbsp; – 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: 45s; raster: scanning; slit: 2"; step Size: 2", FOV: 322"X376";\\ 
&nbsp; -- raster duration: 2h13m15s; Data volume: 186 Mbits;\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|377|cam_ar_limb_lite_v2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=377]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=377]
%%


\\

!ar20091216-08 => High cadence observations of AR transient brightenings and microflares

&nbsp; – Mason ([hm11@damtp.cam.ac.uk|mailto:hm11@damtp.cam.ac.uk])\\ 

%%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 \\ 
-- run context study PRY_slot_context_v3 before and after\\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|360|cam_artb_lite_v2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=360]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=360]
%%


\\ 

!ar20091216-09 => CME onsets

&nbsp; – Bewsher ([danielle.bewsher@stfc.ac.uk|mailto:danielle.bewsher@stfc.ac.uk]), Harrison([Richard.Harrison@stfc.ac.uk|mailto:Richard.Harrison@stfc.ac.uk])\\ 

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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\\ 
}}
%%
%%center
||Study ID||Acronym|| ||
|279|cmeo_slit_lo|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=279]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=279]
|280|cmeo_slot_lo|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=280]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=280]
%%

\\

!ar20091216-10 => CORE EIS Flare Study 1

&nbsp; – 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 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\\
}}
%%
%%center
||Study ID||Acronym|| ||
|363|FLR001_flare_study|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=363]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=363]
%%

\\

!ar20091229-11 => CORE EIS Flare Study 2

&nbsp; – Hara ([hara@solar.mtk.nao.ac.jp|mailto:hara@solar.mtk.nao.ac.jp])\\

%%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|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=461]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=461]
%%

\\

!ar20100417-13 => Nanoflare heating of coronal loops

&nbsp; – 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|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|392|nanoflare_sas_v1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=392]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=392]
%%

\\

!ar20100423-14 => Active Region Transient Brightening Lite

&nbsp; – 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\\
-- &nbsp; raster to be centred on AR core or polarity inversion line\\
-- &nbsp; exposure time: 10s; raster scanning; slit: 2"; step size: 2"; FOV: 200" x 400"\\
-- &nbsp; raster duration: 21m09s; data volume: 108 Mbits\\
-- &nbsp; run context study PRY_slot_context_v3 before and after 
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|361|cam_artb_cds_a_lite|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=361]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=361]
%%

\\

!ar20100423-15 => Multi-temperature Observation of Sigmoids

&nbsp; – 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\\
-- &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)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|374|cam_sigmoid_study_v1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=374]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=374]
%%


\\


!ar20100426-16 => Outflows from Small Active Regfions

&nbsp; – 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\\
-- &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\\
}}
%%
%%center
||Study ID||Acronym|| ||
|388|PRY_loop_velocity|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=388]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=388]
%%


\\


!ar20100622-17 => AR Temperatures and Flows Optimized for Eclipse Observing

&nbsp; – Warren ([harry.warren@nrl.navy.mil|mailto:harry.warren@nrl.navy.mil])\\

%%roundedCorners-yyyy-E3F0EE-808080
{{
-- 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 \\
}}
%%
%%center
||Study ID||Acronym|| ||
|420|hpw021_vel_120x512v1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=420]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=420]
%%


\\


!ar20101109-18 => Dynamic events at the limb with EIS and AIA

&nbsp; – 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|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|443|PRY_sit_stare_1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=443]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=443]
%%


\\


!ar20110120-19 => AR Loop footpoint studies using the bright point trigger

&nbsp; – 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\\ 
   &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)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|445|Hunter_loop_fe8|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=445]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=445]
|444|Cool_loop_response|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=444]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=444]
%%


\\


!ar20110404-21 => Search for slow mode oscillations in coronal loops

&nbsp; – 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 \\
&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)\\
}}
%%
%%center
||Study ID||Acronym|| ||
|354|PRY_slot_contextLITE|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=354]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=354]
|459|Hot_loop_osci_1_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=459]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=459]
|460|Hot_loop_osci_2_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=460]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=460]
%%


\\


!ar20110411-22 => Cambridge Diagnostic Study for the Impulsive Phase of Small Flares

&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])\\

%%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|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=458]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=458]
%%


\\


!!D. Synoptic and Other Studies\\ 

!syo20100504-01 => EIS Spectral Atlas Synoptic Programme

&nbsp; – 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\\
-- &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*\\
}}
%%
%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|403|Atlas_30|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=403]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=403]
|404|Atlas_60|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=404]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=404]
%%


\\


!syo20100713-02 => Full CCD Study to Measure Relative Wavelengths

&nbsp; – Warren ([hwarren@nrl.navy.mil|mailto:hwarren@nrl.navy.mil])\\

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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\\
}}
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%%center
||Study ID||Acronym|| ||
|413|HPW020_VEL_FULLs1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=413]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=413]
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\\


!!E. Test and Calibration Studies \\ 

!test-01 => EIS slit calibration

&nbsp; – Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\ 

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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.\\ 
}}
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%%center
||Study ID||Acronym|| ||
|389|CALIB_slit_slot_v2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=389]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=389]
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\\ 

!test-02 => EIS velocity calibration

&nbsp; – Kamio ([kamio@linmpi.mpg.de|mailto:kamio@linmpi.mpg.de])\\ 

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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.\\ 
}}
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%%center
||Study ID||Acronym|| ||
|375|SK_DEEP_5x512_SLIT1|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=375]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=375]
|376|SK_DEEP_5x512_SLIT2|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=376]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=376]
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\\

!test-03 => EIS Slot Deconvolution Test

&nbsp; – Sun ([js2@mssl.ucl.ac.uk|mailto:js2@mssl.ucl.ac.uk])\\ 

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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\\
}}
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%%center
||Study ID||Acronym|| ||
|429|js2_decon_slot_sc_LT|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=429]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=429]
|430|js2_decon_ref_vel_LT|[details|http://solarb.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=430]|[Example fits|http://solarb.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=430]
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\\