This page (revision-3) was last changed on 02-Feb-2017 13:19 by JianSun

This page was created on 03-Dec-2009 22:30 by JianSun

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Version Date Modified Size Author Changes ... Change note
3 02-Feb-2017 13:19 16 KB JianSun to previous
2 04-Dec-2009 16:38 16 KB JianSun to previous | to last
1 03-Dec-2009 22:30 16 KB JianSun to last

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At line 1 changed 2 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
[{ALLOW view jsun}]
[{ALLOW edit jsun}]
At line 5 removed one line
[Possible EIS Core Team Studies (2009-Dec-01)|http://docs.google.com/Doc?docid=0AdazsPAS3_6xZGNzZHFiOWhfMTY2ZjQ3cG1oZGQ&hl=en&invite=CIDL2K4H]\\
At line 7 removed one line
At line 11 changed 6 lines
- 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\\
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\\
At line 19 changed 9 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) – 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"\\
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"\\
At line 29 changed 6 lines
- 1st priority on the high cadence (at least < 60sec).\\
- 2nd priority on the longer coverage (>2-3hrs continuous coverage; \\
- Interuptions by SAAs and S/C nights are OK.)\\
- 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)\\
1st priority on the high cadence (at least < 60sec).\\
2nd priority on the longer coverage (>2-3hrs continuous coverage; \\
Interuptions by SAAs and S/C nights are OK.)\\
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)\\
This page (revision-3) was last changed on 02-Feb-2017 13:19 by JianSunTop