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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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

Incoming links Outgoing links
IRIS30day...nobody
IRIS30day

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Difference between version and

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[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
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Please check the two documents available from the 'Attach' tab (see above).
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An IRIS weekly planning meeting will take place at around 20 UT on Wednesdays. This will allow input to the Hinode weekly meeting which takes place at 01:30 UT on Thursdays.
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__UPDATE__: A procedure for automatically aligning EIS slot images with AIA has been implemented so that the EIS pointing accuracy should now be good to 5" or better (in both X and Y).
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A copy of the IRIS 30 day plan can be obtained by clicking on the 'Attach' tab at the top of this page. This document is accurate as of 17 Jan 2013.
A copy of the IRIS 30 day plan can be obtained by clicking on the 'Attach' tab at the top of this page. %%strike This document is accurate as of 17 Jan 2013/%. This document is out-of-date and will be updated around end-May/early-June. IRIS Technical Note 30, which discusses the 30 day plan, is also provided.
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Science goal: evolution of abundances, outflows, and coronal heating.
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also abundance study -DB if we're running 7 hours per day
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Science goal: sunspot oscillations.
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EIS: tbd.
EIS: assuming that waves are of interest - DRW_Alf_01
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Science goal: flows
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EIS: DHB_006
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Science goal: waves in fan loops (both intensity and Doppler velocity)
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EIS: IUU_SCAN_STEPS_002
EIS: IUU_SCAN_STEPS_002 for intensity oscillations (maybe AIA would do this instead?) or BL_SUMER_EIS
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Science goal:on disk, energy transfer (and dynamics) in QS features such as jets and bright points.
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EIS: medium size raster?
EIS: SK_CH1_55X512 a large continuous raster and then HPW002?
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Science goal: spicules - looking for coronal counterpart of spicules.
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EIS:
EIS:narrow raster - DRW001_HIGH_BRT_V2 (with density sensitive lines)
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Science goal: assuming limb: jet and spicules/plumes
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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"
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Science goal:look at absorption across the temperature range, looking at temperature distribution and strong dynamics.
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!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