2013-01-18T19:16:53.000Z 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 Sterling Shine (RCO) 141 Sun center programs disk center, Quiet Sun DC, QS DC, QS 8 7 0 112 112 2009-10-06T19:00:32.000Z 2009-10-06T22:55:43.000Z 7 0 Velocity flows in quiet sun magnetic loop footpoints Na IVDG and G/Ca 100"x100", 2x2, slow Sun center programs: HOP 141, velocity flows HOP 136, TESIS HOP 135, H alpha and 5250 Request to SOT HOP Number 0136 AR on disk: Standard AR program, coordinate SP magnetograms to be taken during or near the TESIS joint observing program. AR at the limb: CaII and H-alpha observations to define the chromospheric boundary and identify any prominence material. Cadence of 1-10 minutes for the duration of the observation period (~4hrs) would be sufficient. Large XBP: NFI magnetograms during the TESIS coordination Disk Center: No request Request to SOT HOP Number 0141 Instrument Observable Priority Resolution FOV Cadence SOT/NFI NaD1 dopplergram 1 0.16" ???~ 0.16" 12.80" ???~ 81.92" 15 s NaD1 Stokes I,V 2 SOT/BFI Ca IIH intensity 2 0.11" ???~ 0.11" 19.17" ???~ 88.91" 15 s SOT/SP Fe I full Stokes 1 0.16" ???~ 0.16" 41" ???~ 4.8" 58 s ivo://sot.lmsal.com/VOEvent#2009-10-06T19:00:00Z