SOT: Synoptic
2007-07-03T11:19:00 to 2007-07-03T11:21:30
Science Goal: Synoptic
Program: Synoptic BFI NFI
Target: Sun Center
xcen=0 ycen=0
Instrument: SOT
HOP/JOP: 10
Description:
Daily Note and User Entry: EIS: Norikura Solar Observatory coronagraph campaign led by EIS CO (2007/07/01 - 2007/07/29)
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.
