2024-11-13T00:33:05.000Z 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 Yoshitake Ishibashi Cruz (RCO) 206 HOP 206 N Pole N Pole LMB LMB 14 20180911_142006 197 218 236 14 26 2046 6 1 1 2 0 141 2012 1014 0.991202 -19.184 872.57 321.438 162.304 2018-09-11T14:20:06.000Z 2018-09-11T17:13:40.000Z -19.184 872.57 Polar Panorama Map for understanding Polar Reversal in Cycle 24 Fast deep mode, 2048 slit position, LIMB ONLY abstract of observational proposal The data obtained by the HOP81 observations show that the longitudinal dependence of polar reversal is large. Especially, the dependence becomes important for understanding the progress of polar reversal when polar reversal is progressing to the final phase. Hence, we propose the special observation for taking the panorama map of magnetic field around Pole. If we want to make the panorama map that covers until 65 degrees latitude, we need to perform the polar observation every 3.5 days during one month. Considering the matters about Hinode operation (flares, satellite operation, etc.), we request to perform the polar observation every 3 days. It means that we need to perform 10 polar observations for one panorama map during one month. request to SOT ? SP FoV 320? x 164?, Pixel size: 0.32?/pix, Binning: 2x2, Single side mode Exposure: 4.8 sec (6 Cycles), JPEG Quality: Q75, Data rate: 600Mbits/map Note: margin factor SP 0x0c5 --- 1.3 ivo://sot.lmsal.com/VOEvent#2018-09-11T14:20:00Z