SOT: Ca H 30 sec, G band and Na D mgram 2 min
2007-07-03T01:30:00 to 2007-07-03T10:37:30
Science Goal: Micro-Flares and Evolution in AR 10961
Program: CaH 30sec, Gband NaIV 2min, 4Kx2K, 2x2
Target: Active Region 10961
xcen=273 ycen=-231
Instrument: SOT
HOP/JOP: 0
Description:
Daily Note and User Entry: SOT: Follow AR 10961 as long as possible. Programs for Micro-Flares,
Request to SOT: Observation of Ca H spicules. The sequence that was run previously is used. Widest FOV in the NS direction is desired.
Scientific Objectives: To understand the origin of non-thermal line broadening in coronal emission lines
Other Instruments: Norikura: High dispersion spectra of Fe X6374 and Fe XIV5303 are obtained. High-acuracy Doppler velocity and line width are given. Independent Fe XIV 5303 imaging observations provide high-cadence imaging and Doppler informaiton. Bi-products: andlt
This is the most important for EIS team.andgt
: By the simultaneous observations with Norikura Solar Observatory, EIS line width of instrumental origin is absolutely calibrated. In EIS bandpass there are Fe X lines in the short wavelength band and Fe XIV lines in the long wavelength band. These are calibrated with Fe X 6374 and Fe XIV 5303 emission lines. Norikura Solar Observatory is going to support this campaign observation with a high priority.
