-------------------------------------------------------------------------------------- PLANNING - CURRENT STATUS (2007/08/12 14:30UT) -------------------------------------------------------------------------------------- CONTACT: dot_jop189_hop020 (AT) astro.sk !!!!!!!!!! Campaign coordinators : 03-12/08 : Jan Rybak 13-15/08 : 22-23/08 : Sigrid Stoiser 16-21/08 : 24-31/08 : Astrid Veronig DOT support astronomer: 03-31/08 : Peter Gomory ------------------------------------------------------------------------------ SOHO JOP 189 details DOY 225 Monday August 13 2007 - disk center: (x,y)=(0,0) without tracking (t_start,t_end)=(07:00-13:30) Notes: - CDS/SOHO: no support for JOP189 - MDI FD mode - mags with the highest cadence possible - 11:00-13:30 - same target with HOP026 TRACE : requstedd: 06:46 - 13:35 JOP 189 Sunspot, Active Region 0966, (x,y)=(0, -200) 171 ~ 50s cadence, 1216, 1550, 1600, WL every 10 cycles MDI : requested: FD mags DOT : ------------------------------------------------------------------------------ ------------------------------------------------------------------------------ -------------------------------------------------------------------------------------- OPEN QUESTIONS: - TRACE support for our prime time before Aug 20 ? Yes, if possible. -------------------------------------------------------------------------------------- TARGET(S): - default: disk center (for the case no other target will be provided in time) - limit time for specification of the new target position : 12:00 UT for the next day (on Friday also for Sunday and Monday besides Saturday) - addresses to instrument planners: SOHO : soc AT soc.nascom.nasa.gov CDS : planner AT cdso8.nascom.nasa.gov week 33: Aug 13 - Aug 19 Terry Kucera therese.a.kucera AT nasa.gov week 34: already keyhole MDI : mdi-ops AT mdisas.nascom.nasa.gov TRACE : trace_planner AT lmsal.com, trace_planner AT cheyenne.nascom.nasa.gov DOT : P.Suetterlin AT astro.uu.nl, gomory AT astro.sk HVAR : bvrsnak AT geodet.geof.hr, asv AT igam06ws.uni-graz.at, manuela.temmer AT uni-graz.at KH : baumgartner AT kso.ac.at, otruba AT kso.ac.at, werner.poetzi AT uni-graz.at HINODE: sot_co AT solar.isas.jaxa.jp, eis_co AT solar.isas.jaxa.jp, xrt_co AT solar.isas.jaxa.jp PG : gomory AT astro.sk JR : rybak AT astro.sk -------------------------------------------------------------------------------------- OPTIONAL COOPERATION: 2007/08/10 11:00 - 2007/08/10 18:00 (-41.2/+ 0.2) HOP26, QS Sun-center tracking possible joining with DOT Bloomfiled + Tsuneta -------------------------------------------------------------------------------------- CONFLICTING APPLICATIONS: * Aug 8-18 JOP194 Activity in Filaments and Filament Cavities, CDS/UVCS/EIT/LASCO/TRACE/Hinode-EIS/Hinode-XRT/STEREO/ Hinode-SOT/COMP/HELIO/SOLARC(TBC)/ProMag(TBC)/MWA(TBC)/RHESSI/ PROBA2/GOES/BBSO/ISOON/MLSO,SMEI, POC: Terry Kucera JOP description: http://sohowww.nascom.nasa.gov/soc/JOPs/jop194.txt 27/7: The most important time of day for campaign participation would be 17:00 -- 20:00 UT, the best observing period of Mauna Loa. The full Mauna Loa observing day can run from 16:30 -- 02:30 UT. Scheduling spacecraft supports to these times would help to interleave with the JOP 189, which has its ground-based support focus on Canary islands and in Europe. * Aug 13 CDS atlas - no time available * Aug 12-Sep 09 26m Keyhole - this only decrease the telemetry throughput * Aug 18-Sep 03 34m Keyhole - this will stop SOHO supprt for us In brackets below the finally provided days from HINODE TAC are given: * Aug 09-20 HOP 026 Hinode-SST. Wave transmission in QS + Wave Variations in PEN (09-17) Bloomfield, Tsuneta SST, no TRACE, no EIS, no XRT but EIS doing its core observations only Peter G. will try to make agreement on the target * Aug 21-30 JOP 186 HOP 034 Atmospheric Seismology, Mike Marsh (25-28) SST, TRACE, HINODE-EIS/SOT/XRT Peter G. will try to make agreement on the target http://sohowww.nascom.nasa.gov/soc/JOPs/jop186.txt TRACE: our JOP was the first -> priority for TRACE * Aug 25-31 HOP021 Hinode/CALAS - Families of granules (29-31) Roudier, Berger PdM, EIS, XRT -------------------------------------------------------------------------------------- SOHO: telemetry: lose significant high rate times due to the 34m keyhole (18-31 August) orientation: SOHO is in upside down roll (180 deg) position keyholes: Aug 11-Sep 9 26 m keyhole - start Aug 19-Sep 2 34 m keyhole - start POC : Alex Young: alex.young AT gsfc.nasa.gov MDI : do not see a conflict with supporting your JOP up to 34keyhole !!! MDI wait your pointing for Saturday Aug 18 when HR mode is scheduled in our prime time 11/8: MDI will resume Full Disk Magnetograms and Dopplergrams, Saturday, 11-Aug-2007 ~14:35. We will likely not get all 15 96 minute synoptic Magnetograms every day from 11-Aug through 09-Sep. 10/8: information for week 33: only FD, high rate only on Sat, 18-Aug, 09:53-17:00UT 27/7: MDI will support with HR Filtergrams and Magnetograms when target in the HRFOV. FD Magnetograms and Dopplergrams otherwise. JOP targets will also be specified preferably in the HRFOV. 31/7: HR when requested, high rate telemetry for 07:00-13:30 probable but not sure fopr each day EIT : support until start of the 26m keyhole as goes to bakeout (TRACE will do full mosaics) bakeout: start - 2007/08/26 DSS-24 16:05 - 01:00; bakeout begins by 21:00 UT end - 2007/09/01 bakeout ends from plan at 09:00 UT Aug 9 EIT shutterless #28 (timing TBC) 27/7: EIT will support through Aug 25 (until the beginning of the CCD bakeout) CDS : conflict: the filament/cavity campaign able to support each day during 3-17 August in case of no time conflict with prominence/filament campaigns week33: Thuesday-Sunday each day 10/08: CDS until Aug 19 including but pinting two days in advance 10/08: CDS Realtime data: wrong sign on X,Y positions, rasters unsidedown + left/right W to right, N down 27/7: CDS will support on selected dates, as time allows. 31/7: CDS confimed support from Aug 3 for 07:00-13:30 -------------------------------------------------------------------------------------- TRACE: confirmed support: 20 - 31 August tbd support: 03 - 20 August if no good target for the filaments and prominence campaigns present themselves 03/8: support obtained for morning period! 31/7: TRACE support before Aug 20 possible: send targets each day 27/7: TRACE will only support 20-31 Aug fro sure -------------------------------------------------------------------------------------- HINODE: request for EIS+SOT+XRT for the period mainly during the SOHO keyhole (after Aug 17) - final details - Aug 3 - EIS run details - Jul 17,20 - 1st list of our campain on the Hinode plan for Aug 2007 - Jul 02 - discussion on simplifying and shortening - Jun 22 - sent - May 31 - expected EIS procedure: 1) Run context (~8 UT) 2) Run SNS * N times 3) Stop for ~15 minutes (~9:30 UT) for EIS tables upload - stopped for ~15 minutes) 4) Run SNS * M times 5) run context just before 12 UT 6) Stop at ~12 UT -------------------------------------------------------------------------------------- PLANNING - LOG: -------------------------------------------------------------------------------------- 09/08 - DOT best frame storing suggested/agreed 08/08 - sharing coordination duties, coordination_duties.txt 07/08 - AR10966 with MDI in HR 06/08 - disk center -> AR 10966 EIS is doing core observations when HOP021 and 026 CDS VARDYN_C with 100s full detector allowed also for AR MDI asked for FD on 7/8 and later for HR movet in y to -180" (AR10966) 03/08 - MDI plans for week 32 discussed, EIS studies 196 and 197, specification of order CDS plan for 4,5,6/8, EIS suggestion for HOP026 period 02/08 - target info to CDS,TRACE,MDI,DOT,SOC,POC for 8/3 sent at 07UT 02/08 - EIS informed about including our runs to EIS DB 02/08 - MDI changed FD for HR for Aug 3-5! 01/08 - TRACE confimed support from Aug 3 in case of no conflicts 01/08 - MDI confimed support from Aug 3 (HR from Aug 6) 31/07 - CDS confimed support from Aug 3 31/07 - emails to planners: CDS, MDI, TRACE + email to SOHO POC and SOHO SOC 09/07 - cooperation (no conflicts) with JOP88 - Gary Kilper 02/07 - our program is on the Hinode plan as HOP 020 for 18-31/8/2007 22/06 - simplifying and shortening the Hinode application 18/06 - conflicting Hinode applications with Mike Marsh no conflict with its TRACE camapaign part 31/05 - Hinode application sent to CC and SSCs of SOT,EIT,XRT 25/05 - SOHO Science Planning Working Group - decision made - we are on calendar 23/05 - SOHO JOP 189 number has been given to our proposal 18/05 - TRACE decision made 16/05 - SOHO JOP application, MDI request, TRACE request 05 - CDS request - positive 04 - DOT TAC decision - 3-31/8/2007 01 - DOT TAC application -------------------------------------------------------------------------------------- PLANNING - TODO: -------------------------------------------------------------------------------------- -------------------------------------------------------------------------------------- TEMPORARY NOTES: -------------------------------------------------------------------------------------- > hr_ve_fe_me - high res FOV 1024 (EW) x 500 (NS) pixel (horizontal strip) > (or 620"x310") extract of velocity, continuum filtergram, & magnetogram > > hr_t2_ve_fe_me - HR FOV 700x700 pixel square extract (or 420"x420") of > dopplergrams, continuum filtergrams, & magnetograms, with capability to > track solar rotation. > > hr_m1_context - Full HR FOV magnetograms and 2x2 pixel binned velocities > once per minute, with a Full HR FOV filtergram image every 60 minutes. Right now, SOHO is upside down (roll angle 180 degrees). The MDI HR FOV right now, extends 432 arcseconds south of disk center and 188 arcseconds north of disk center, 320 arcseconds east of disk center and 300 arcseconds west of disk center. When we roll back to 0 degrees sometime in March, during the next Keyhole, the MDI HR FOV will extend 188 arcseconds south of disk center and 432 arcseconds north of disk center, 300 arcseconds east of disk center to 320 arcseconds west of disk center. You can see this difference in the following two images: http://mdisas.nascom.nasa.gov/gif_summary/igram/smdi_igram_fd_20060103_1032.gif http://mdisas.nascom.nasa.gov/gif_summary/igram_fd_2005/smdi_igram_fd_20051114_0000.gif . Most MDI HR campaigns can be positioned anywhere within the HR FOV. Camapigns extraxt from the detextor (1k x 1k pxs) ussually 512 x 512 pxs or 1024 x 512 pxs. Position of the total HR FOV depends on the actual position of the SOHO. (SOHO roll orientation is changing over the year upside-down to compensate a little bit problem with the fixed antenna - http://sohowww.nascom.nasa.gov/pickoftheweek/old/02jul2003/SOHOOrbit.jpg). Right now, SOHO is upside down (roll angle 180 degrees). The MDI HR FOV right now, extends 432 arcseconds south of disk center and 188 arcseconds north of disk center, 320 arcseconds east of disk center and 300 arcseconds west of disk center. When we roll back to 0 degrees sometime in March, during the next Keyhole, the MDI HR FOV will extend 188 arcseconds south of disk center and 432 arcseconds north of disk center, 300 arcseconds east of disk center to 320 arcseconds west of disk center. You can see this difference in the following two images: http://mdisas.nascom.nasa.gov/gif_summary/igram/smdi_igram_fd_20060103_1032.gif http://mdisas.nascom.nasa.gov/gif_summary/igram_fd_2005/smdi_igram_fd_20051114_0000.gif . Most MDI HR campaigns can be positioned anywhere within the HR FOV. Camapigns extraxt from the detextor (1k x 1k pxs) ussually 512 x 512 pxs or 1024 x 512 pxs. Here follow some of them which cover both intensity, magneto and Doppler: hr_ve_fe_me - high res FOV 1024 (EW) x 500 (NS) pixel (horizontal strip (or 620"x310") extract of velocity, continuum filtergram, & magnetogram hr_t_ve_fe_me - same as hr_ve_fe_me except vertical strip extract, 500 (EW) x 1024 (NS) pixels (or 310"x620"), with cability to track solar rotation. Some other are also available - the full list is available at http://mdisas.nascom.nasa.gov/Collaborate . All of the campaigns we have can still be moved to different parts of the FOV within the set FOV position, to get any area you want, ie, disk center, top half of the FOV, bottom half of the FOV, etc. But the center of the FOV depends on the SOHO roll angle (up-down). Nevertheless, it seems to me that the above mentioned ones are quite good for you, as they can cover ARs both on the north and south. Of course they can not cover the ARs farer than ~300 arc seconds from the disk center in the E-W direction.