2007-07-31T22:03:51.000Z 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 Sterling Sekii, Watanabe and Shine 24 Synoptic Sun Center DC, SYN DC, SYN 19 0 0 223 111 2007-07-26T01:04:00.000Z 2007-07-26T11:35:16.000Z 0 0 Synoptic Synoptic BFI NFI Daily Note and User Entry: EIS: Would like polar coronal hole pointing for co-observing with XRT and SOT. Two programmes are being considered. 1) Slow context raster then fast sit'n'stare slit observations at several positions for short-timescale dynamics. 2) Jet dynamics with 40"" slot sit'n'stare observations EIS will perform MHC software upload toward end of this week. For programme 2 we suggest SOT fast SP maps to observe changes in the photospheric field, and XRT single-filter, high-cadence observations to complement EIS temperature coverage. SOT: Support HOP10 Norikura and HOP24, which observes prominences and filaments at limb. andnbsp; andnbsp; andnbsp; andnbsp; We may try tests for H-alpha dopplergrams, and H-alpha flat field imaging in the quiet sun. SOT: Memory upload operation to load new frame definition tables in FPP memory.; 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#2007-07-26T01:03:30Z