2007-07-22T21:44:36.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null Hinode SOT Hara Kotoku Sekii, Watanabe and Shine 24 HOP24 filament Filament FIL, QS FIL, QS 12 508 572 111 111 2007-07-21T18:13:41.000Z 2007-07-21T23:39:45.000Z 508 572 filament evolution H lc, CaH, G-b 2Kx2K 2x2, 30s 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. HOP24 filament 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. ivo://sot.lmsal.com/VOEvent#2007-07-21T18:12:40Z