Observation

Observation Details

SOT: HOP10 prominence

2007-07-23T00:44:30 to 2007-07-23T10:33:30

Science Goal: Joint Observation of the Solar Corona between Hinode EIS and NAOJ Norikura Observatory for nonthermal line broadening in the coronal emission

Program: H-a 2 wave for DG, CaH2Kx2K 2x2, 30s

Target: Prominence

xcen=930 ycen=-99

Instrument: SOT

HOP/JOP: 10

Description: Daily Note and User Entry: SOT: Track AR and observe filament or prominence HOP15 will be tested from 07/18 to 07/22. HOP10 prominence observation. EIS: HOP10 Norikura 4hour per day if whether is fine in Norikura. (Limb fix) XRT: Support HOP10 if possible. Mike Marsh's AR evolution program (coordinated with TRACE) may be run if possible.
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.

Annotations:

Chief Observer

Sekii, Watanabe and Shine