This page (revision-7) was last changed on 07-Dec-2016 14:14 by Peter Young

This page was created on 01-Feb-2013 21:34 by Peter Young

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Page revision history

Version Date Modified Size Author Changes ... Change note
7 07-Dec-2016 14:14 7 KB Peter Young to previous
6 02-May-2013 21:40 7 KB Peter Young to previous | to last
5 23-Apr-2013 08:15 6 KB Louise Harra to previous | to last
4 01-Feb-2013 22:16 5 KB Peter Young to previous | to last
3 01-Feb-2013 22:15 5 KB Peter Young to previous | to last
2 01-Feb-2013 21:38 5 KB Peter Young to previous | to last
1 01-Feb-2013 21:34 5 KB Peter Young to last

Page References

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IRIS30day...nobody
IRIS30day

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Difference between version and

At line 57 added 2 lines
Science goal: evolution of abundances, outflows, and coronal heating.
At line 64 added one line
also abundance study -DB if we're running 7 hours per day
At line 68 added 2 lines
Science goal: sunspot oscillations.
At line 69 changed one line
EIS: tbd.
EIS: assuming that waves are of interest - DRW_Alf_01
At line 80 added 2 lines
Science goal: flows
At line 84 added 2 lines
EIS: DHB_006
At line 88 added 2 lines
Science goal: waves in fan loops (both intensity and Doppler velocity)
At line 83 changed one line
EIS: IUU_SCAN_STEPS_002
EIS: IUU_SCAN_STEPS_002 for intensity oscillations (maybe AIA would do this instead?) or BL_SUMER_EIS
At line 98 added 2 lines
Science goal:on disk, energy transfer (and dynamics) in QS features such as jets and bright points.
At line 91 changed one line
EIS: medium size raster?
EIS: SK_CH1_55X512 a large continuous raster and then HPW002?
At line 108 added 2 lines
Science goal: spicules - looking for coronal counterpart of spicules.
At line 99 changed one line
EIS:
EIS:narrow raster - DRW001_HIGH_BRT_V2 (with density sensitive lines)
At line 118 added 2 lines
Science goal: assuming limb: jet and spicules/plumes
At line 122 added 13 lines
EIS: DRW001_HIGH_BRT_V2 (may need something with bigger step sizes?)
IRIS - possible pointing E-W at limb.
!CH2 - coronal hole properties - 1.5 hours
Science goal: energy transfer in coronal hole - tracking outflow through the atmosphere.
IRIS: deep full wavelength raster.
EIS: quiet raster atlas - DHB_atlas_120M_30"
At line 137 added 2 lines
Science goal:look at absorption across the temperature range, looking at temperature distribution and strong dynamics.
At line 109 changed one line
!PR2 - filament -
EIS: take a full spectrum once. HPW23, then do a sit n stare at limb - PROM_RAST_SMALL_V2
IRIS:
!PR2 - filament - #
Science goal: waves and dynamics in filaments
EIS: sit and stare - BL_SUMER_EIS
IRIS:
This page (revision-7) was last changed on 07-Dec-2016 14:14 by Peter YoungTop