2024-09-24T22:21:29.000Z 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 SOTSP Narukage Ichimoto Tarbell 2 HOP 2 + spicules Spicule and Jets, N Pole CORE: Polar Region Observation Campaign PC, SPI 10 20070924_132006 110 132 128 10 72 281 16 2 1 1 0 142 2026 281 1 -5.459 927.452 44.539 162.304 2007-09-24T13:20:06.000Z 2007-09-24T14:21:22.000Z -5.459 927.452 CORE: Polar Region Observation Campaign 281 slits (one hour), 16 cyles, I scaled HOP 2 Programs: all fixed pointing at (0, 920) 24 Sep 12:14 - 15:59 Spicule observations in Mg b line with TRACE at 13:00 and 14:38 for about 40 minutes Request to SOT HOP Number 0002 G-band and Ca-H at high cadence full resolution with vector magnetograms. ??????4.8 x 4 seconds integration time needed in SP to increase the SNR a factor of 2 on the limb Time evolution of granular structures are ~ 1 min. 80"x120" maps will take 4 hours in total 5 positions (North, South, East, West, disc center) with no active regions. West limb have been only once observed and East limb never !!! At least high resolution G-band maps (1x1) to identify magnetic features. Scientific Objectives: ??????Objective: To characterize the temperature, dynamics and statistical distribution of polar coronal jets recently observed by XRT.;;HOP 2 Programs: all fixed pointing at (0, 920) 24 Sep 12:14 - 15:59 Spicule observations in Mg b line with TRACE at 13:00 and 14:38 for about 40 minutes Request to SOT HOP Number 0002 G-band and Ca-H at high cadence full resolution with vector magnetograms. ??????4.8 x 4 seconds integration time needed in SP to increase the SNR a factor of 2 on the limb Time evolution of granular structures are ~ 1 min. 80"x120" maps will take 4 hours in total 5 positions (North, South, East, West, disc center) with no active regions. West limb have been only once observed and East limb never !!! At least high resolution G-band maps (1x1) to identify magnetic features. Scientific Objectives: ??????Objective: To characterize the temperature, dynamics and statistical distribution of polar coronal jets recently observed by XRT. ivo://sot.lmsal.com/VOEvent#2007-09-24T13:20:00Z