2007-07-31T19:59:36.000Z 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 Kamio Sterling Nakamura and Shine 10 Colonal hole, SP Coronal Hole CH CH 10 943 -4 0 162 2007-07-30T01:50:05.000Z 2007-07-30T04:37:24.000Z 943 -4 Coronal hole magnetic field Fast Map, Full FOV Daily Note and User Entry: Note: The time of the 1st contact (MSP1) is earlier than usual. SOT: Support HOP10 Norikura and HOP24, which observes prominences and filaments at limb. andnbsp; andnbsp; andnbsp; andnbsp; Coalignment program run (N-limb, E-limb, 2hour for each) to run in weekend plan. XRT: Stop X-ray observation (and perform CCD bakeout).; 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#2007-07-30T01:48:00Z