2007-07-04T21:43:42.000Z 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 Arikawa Okamoto Jurcak, Tarbell 0 Ca H 30 sec, G band and Na D mgram 2 min Active Region 10961 AR, MFL, SS AR, MFL, SS 10961 1 397 -230 223 111 2007-07-03T01:30:32.000Z 2007-07-03T20:34:21.000Z 397 -230 Micro-Flares and Evolution in AR 10961 CaH 30sec, Gband NaIV 2min, 4Kx2K, 2x2 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. ivo://sot.lmsal.com/VOEvent#2007-07-03T01:30:00Z