2024-09-24T22:22:00.000Z 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 Arikawa Brooks Sekii 126 Tracking AR 11234 (cont) Active Region, Spicule and Jets AR, CHR, JET AR, CHR, JET 11234 11 20110615_090611 291 324 331 11 71 60 1 1 1 2 1 82 2012 1328 44.266666666666666 230.46 -316.419 9.568 81.152 2011-06-15T09:06:11.000Z 2011-06-15T10:10:00.000Z 230.46 -316.419 CORE: Chromospheric Jets Dynamics, 9.6"x82", repeat Tracking AR 11234 and HOP 126 Request to SOT HOP Number 0126 Context programs: SP: fast map large enough to cover the AR, perhaps 123x123 or 164x164 arcsec, avoiding SAA NFI: Program 0x3b4 AR mode case2 (Large), G-band 120min, Na IV 5min, Ca H 5min, during the SP map High-cadence programs: NFI: Program 03bd H-alpha sequence: H-alpha at -2.1A, at -1.28A and -0.87A, 112"x112", 2x2 summed, at 13 s cadence, and Na D IVDG every 5 minutes, same FOV SP : Program 0xed fast raster (dynamics), 4.8"x60" at 1 min cadence The NFI high cadence program should run for the prime observing time in La Palma, 2-3 hours depending on telemetry. The SP high cadence should run for 30 minutes in the middle of this period (avoiding SAA). The context programs should run once before the high cadence observing begins and again once after it ends. The CT should cycle off/on before the start of each of the SP programs.;;Tracking AR 11234 and HOP 126 Request to SOT HOP Number 0126 Context programs: SP: fast map large enough to cover the AR, perhaps 123x123 or 164x164 arcsec, avoiding SAA NFI: Program 0x3b4 AR mode case2 (Large), G-band 120min, Na IV 5min, Ca H 5min, during the SP map High-cadence programs: NFI: Program 03bd H-alpha sequence: H-alpha at -2.1A, at -1.28A and -0.87A, 112"x112", 2x2 summed, at 13 s cadence, and Na D IVDG every 5 minutes, same FOV SP : Program 0xed fast raster (dynamics), 4.8"x60" at 1 min cadence The NFI high cadence program should run for the prime observing time in La Palma, 2-3 hours depending on telemetry. The SP high cadence should run for 30 minutes in the middle of this period (avoiding SAA). The context programs should run once before the high cadence observing begins and again once after it ends. The CT should cycle off/on before the start of each of the SP programs. ivo://sot.lmsal.com/VOEvent#2011-06-15T09:06:00Z