2024-09-24T22:21:26.000Z 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 Bando Sakao Katsukawa 62 HOP62 thermal structure of corona Active Region CORE: Thermal distributions and evolutions of coronal structures AR 10980 6 20080105_110705 30 49 52 6 51 2000 2 2 1 2 0 22 2028 1000 1 -437.573 -62.612 317 162.304 2008-01-05T11:07:05.000Z 2008-01-05T12:10:18.000Z -437.573 -62.612 CORE: Thermal distributions and evolutions of coronal structures Fast Map, Full FOV No specific request for SOT. Scientific Objectives: XRT has the capability for thermal studies using multi-filter observation sequences. Some multi-filter observations have been performed to-date, but the XRT Team would like to perform some coordinated observations with EIS and SOT. The primary science objective is study the thermal distribution and evolution of loop structures in active regions as well as XBPs, and cooler coronal structures, as seen by XRT and EIS rasters. (For example, some initial results by Reeves et al. directly show the spatial and thermal distribution of cooling plasma throughout coherent post-flare loop structures.);;No specific request for SOT. Scientific Objectives: XRT has the capability for thermal studies using multi-filter observation sequences. Some multi-filter observations have been performed to-date, but the XRT Team would like to perform some coordinated observations with EIS and SOT. The primary science objective is study the thermal distribution and evolution of loop structures in active regions as well as XBPs, and cooler coronal structures, as seen by XRT and EIS rasters. (For example, some initial results by Reeves et al. directly show the spatial and thermal distribution of cooling plasma throughout coherent post-flare loop structures.) ivo://sot.lmsal.com/VOEvent#2008-01-05T11:07:00Z