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

Only authorized users are allowed to rename pages.

Only authorized users are allowed to delete pages.

Page revision history

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

Page References

Incoming links Outgoing links
EisCoreStudy...nobody
EisCoreStudy

Version management

Difference between version and

At line 82 added one line
}}
At line 85 changed 10 lines
__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]) __\\
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:\\
PRY_slot_context_v2 (dur 3 min; vol 3 Mbit) once at start of observation\\
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\\
PRY_slot_context_v2 at end of observations\\
run dob_bp_****_raster for minimum 4h; run both studies on different days\\
request SOT and XRT to observe EIS FoV: 120x160" (dob_bp_slit_raster) or 160x160" (dob_bp_slot_raster)\\
TRACE/CDS involvement desirable; __advise schedule to Brown and Bewsher__\\
!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])\\
%%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:\\
  - PRY_slot_context_v2 (dur 3 min; vol 3 Mbit) once at start of observation\\
  - 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\\
  - PRY_slot_context_v2 at end of observations\\
  - run dob_bp_****_raster for minimum 4h; run both studies on different days\\
  - request SOT and XRT to observe EIS FoV: 120x160" (dob_bp_slit_raster) or 160x160" (dob_bp_slot_raster)\\
  - TRACE/CDS involvement desirable; __advise schedule to Brown and Bewsher__\\
}}
%%
\\
At line 96 changed 14 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\\
!7. Quiet Sun diagnostics/evolution - Ugarte-Urra ([iugarte@ssd5.nrl.navy.mil|mailto:iugarte@ssd5.nrl.navy.mil]) \\
point to a generic quiet Sun region (solar tracking). Two study sequences:\\
a) run NRL_QSCH_30X400_90s2 multiple times (3 at least)\\
b) run IUU_SLOT___488x512__ as context\\
run HPW019AR__1x400_45s (sit-and-stare) for 2 hours\\
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)\\
%%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\\
}}
%%
\\
!7. Quiet Sun diagnostics/evolution - 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:\\
  a) run NRL_QSCH_30X400_90s2 multiple times (3 at least)\\
  b) run IUU_SLOT___488x512__ as context\\
    - run HPW019AR__1x400_45s (sit-and-stare) for 2 hours\\
    - 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 111 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\\
%%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\\
At line 149 added 5 lines
}}
%%
\\
This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop