This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian Sun

This page was created on 14-Dec-2009 10:51 by JianSun

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Version Date Modified Size Author Changes ... Change note
186 18-Apr-2021 19:09 44 KB Jian Sun to previous
185 30-Jun-2011 16:36 45 KB Jian Sun to previous | to last
184 11-Apr-2011 10:53 45 KB JianSun to previous | to last
183 11-Apr-2011 10:52 45 KB JianSun to previous | to last
182 04-Apr-2011 15:19 43 KB JianSun to previous | to last
181 04-Apr-2011 15:17 43 KB JianSun to previous | to last

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EisCoreStudy...nobody
EisCoreStudy

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At line 19 changed 2 lines
--- point to a quiet region with an X-ray bright point near disk centre\\
--- run IUU_SLOT_136x400_Q65 (ID # 292) for context\\
-- point to a quiet region with an X-ray bright point near disk centre\\
-- run IUU_SLOT_136x400_Q65 (ID # 292) for context\\
At line 22 changed one line
- run SK_QS_34x168c (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\\
At line 24 changed one line
--- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to track evolution of magnetic fields in the photosphere\\
-- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to track evolution of magnetic fields in the photosphere\\
At line 34 changed 10 lines
- 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)\\
-- 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)\\
At line 48 changed 3 lines
- 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\\
-- 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\\
At line 60 changed 8 lines
- 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__\\
-- 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__\\
At line 77 changed 5 lines
- 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__\\
-- 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__\\
At line 92 changed 9 lines
- 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__\\
-- 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__\\
At line 110 changed 4 lines
- 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\\
-- 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 123 changed one line
- point to a generic quiet Sun region (solar tracking). Two study sequences:\\
-- point to a generic quiet Sun region (solar tracking). Two study sequences:\\
At line 126 changed 5 lines
&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)\\
&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)\\
At line 140 changed 7 lines
- 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\\
-- 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\\
At line 158 changed 6 lines
- 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\\
-- 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\\
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop