2024-10-02T01:11:47.000Z 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 Hosoi Brooks Cruz (RCO) 332 HOP 332 AR 12635 w/IRIS and EIS Active Region PEN PEN 12635 16 20170214_103248 460 488 450 16 70 300 2 1 1 2 0 21 2025 150 1 646.774 276.244 47.55 101.44 2017-02-14T10:32:48.000Z 2017-02-14T10:42:16.000Z 646.774 276.244 Active region jet studies with Hinode and IRIS Faster Full-Res, 16x61", ROI 2, repeat, w/context Request to SOT HOP Number 0332 SOT participation is optional, but two possibilities are the following: 1) If a well-developed sunspot penumbra is included in the IRIS and; EIS rasters, run a repeated dynamics mode raster (full resolution, no summing, 2.4 sec integration), with FOV approx. 20 x 60 or 20 x 80 arcseconds, wide enough to cover all of the inner penumbra and most of the outer penumbra on one side of the spot. An East-West ROI offset may be used to place the SP raster as desired on the penumbra. This should run at least 2 hours, telemetry permitting. 2) Run repeated fast maps covering the central portion of the IRIS and; EIS rasters, with cadence of 10-20 minutes, similar to HOP 306.;;Request to SOT HOP Number 0332 SOT participation is optional, but two possibilities are the following: 1) If a well-developed sunspot penumbra is included in the IRIS and; EIS rasters, run a repeated dynamics mode raster (full resolution, no summing, 2.4 sec integration), with FOV approx. 20 x 60 or 20 x 80 arcseconds, wide enough to cover all of the inner penumbra and most of the outer penumbra on one side of the spot. An East-West ROI offset may be used to place the SP raster as desired on the penumbra. This should run at least 2 hours, telemetry permitting. 2) Run repeated fast maps covering the central portion of the IRIS and; EIS rasters, with cadence of 10-20 minutes, similar to HOP 306.;;Request to SOT HOP Number 0332 SOT participation is optional, but two possibilities are the following: 1) If a well-developed sunspot penumbra is included in the IRIS and; EIS rasters, run a repeated dynamics mode raster (full resolution, no summing, 2.4 sec integration), with FOV approx. 20 x 60 or 20 x 80 arcseconds, wide enough to cover all of the inner penumbra and most of the outer penumbra on one side of the spot. An East-West ROI offset may be used to place the SP raster as desired on the penumbra. This should run at least 2 hours, telemetry permitting. 2) Run repeated fast maps covering the central portion of the IRIS and; EIS rasters, with cadence of 10-20 minutes, similar to HOP 306. ivo://sot.lmsal.com/VOEvent#2017-02-14T10:32:00Z