SOTSP: HOP257 (SST-IRIS-Hinode)
2015-09-03T09:12:51 to 2015-09-03T10:01:50
Science Goal: SST-IRIS-Hinode campaign
Program: Fast map, BFI Full FOV, Q65, 1-side CCD
Target: Active Region
xcen=-150 ycen=-448
Instrument: SOTSP
HOP/JOP: 257
Description:
Coordinated observing campaign using the Swedish Solar Telescope on La Palma, IRIS and Hinode is scheduled for September 3 - October 14, 2015. Observers at the SST will be from Oslo and LMSAL for this entire period. The goal is to obtain very high cadence, high spatial resolution observations of the photosphere and chromosphere with CRISP to accompany the IRIS spectra and images of the chromosphere and transition region. CRISP data will allow measurement of line profiles for Doppler shifts and polarization for some magnetic field information above the photosphere. Hinode will contribute precise photospheric fields with SOT/SP, magnetogram evolution with SOT/NFI and coronal images and spectra with XRT and EIS. IRIS and SST will have a number of science goals, listed here in no particular order. Priorities will depend to some extent on how much good data is obtained during the June IRIS/SST campaign. There are a variety of targets: AR sunspot, AR plage, QS, CH, filament on disk, and AR, QS, CH. (Prominence targets are not included because the SST adaptive optics system won?t work above the limb.) For IRIS, the IRIS coordination calendar has the appropriate IRIS OBS to use for each priority. A. Chromospheric Heating in QS/AR/CH: for Hinode, SOT: large FOV SP scans, NFI magnetograms
EIS: EIS study 373
XRT: Al poly filter images at 30s with FOV 384"x384" B. Bombs and flux emergence in AR: for Hinode similar to HOP 268 (not for IRIS) but with NFI magnetograms C. Jets in CH/QS: for Hinode, HOP 243 D. Previously Unresolved Fine structure: for Hinode, HOP 243 E. Penumbral jets: AR sunspot
for Hinode, HOP 250 F. Spicules at the limb: QS or CH limb
for Hinode, HOP 249
Coordinated observing campaign using the Swedish Solar Telescope on La Palma, IRIS and Hinode is scheduled for September 3 - October 14, 2015. Observers at the SST will be from Oslo and LMSAL for this entire period. The goal is to obtain very high cadence, high spatial resolution observations of the photosphere and chromosphere with CRISP to accompany the IRIS spectra and images of the chromosphere and transition region. CRISP data will allow measurement of line profiles for Doppler shifts and polarization for some magnetic field information above the photosphere. Hinode will contribute precise photospheric fields with SOT/SP, magnetogram evolution with SOT/NFI and coronal images and spectra with XRT and EIS. IRIS and SST will have a number of science goals, listed here in no particular order. Priorities will depend to some extent on how much good data is obtained during the June IRIS/SST campaign. There are a variety of targets: AR sunspot, AR plage, QS, CH, filament on disk, and AR, QS, CH. (Prominence targets are not included because the SST adaptive optics system won?t work above the limb.) For IRIS, the IRIS coordination calendar has the appropriate IRIS OBS to use for each priority. A. Chromospheric Heating in QS/AR/CH: for Hinode, SOT: large FOV SP scans, NFI magnetograms
EIS: EIS study 373
XRT: Al poly filter images at 30s with FOV 384"x384" B. Bombs and flux emergence in AR: for Hinode similar to HOP 268 (not for IRIS) but with NFI magnetograms C. Jets in CH/QS: for Hinode, HOP 243 D. Previously Unresolved Fine structure: for Hinode, HOP 243 E. Penumbral jets: AR sunspot
for Hinode, HOP 250 F. Spicules at the limb: QS or CH limb
for Hinode, HOP 249
wavelength: 6302A Continuum Intensity cadence: -1 min fov: 243,122 images: 772 JavaScript Landing Page
