2024-09-24T22:21:30.000Z 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 Bando Frank 20 EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating Active Region EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating MFL 12 20070820_112043 34 53 56 12 6 690 6 2 1 1 0 22 2039 690 1 64.718 -232.795 109.365 162.304 2007-08-20T11:20:43.000Z 2007-08-20T12:19:16.000Z 64.718 -232.795 EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating Normal map 100 arcsec Daily Note and User Entry: HOP20: solar microflares and supergranular network dynamics (SOT/XRT/EIS) (07:00 - 13:30 UT) EIS sensitivity monitoring EIS: Target of opportunity observations of coronal hole on disk. XRT: CCD Bakeout plus test X-ray images SOT: Support HOP 20 07:00-13:30 UT; Request to SOT: SOT: We plan (if possible) to run in time a sequence of 3exposures:2using the BFI imager and 1 using the NBIimager.The reason is to cover evolution of the photosphere with its magnetic concentration signatures (G-band), evolution of the longitudinal component of the magnetic field vector inthe photosphere, and evolution of chromosphere (CaIIH)witha reasonable temporal resolution (???`10s per image,???@???`30s???@per???@sequence???@of 3 selected channels).???@ ???@and;#8226;BFI: G-band and CaIIH channels, ???@ ;FOV:109???hx109???h(1k x1kmode, binning 2 x 2 pxs), ; ;3bit JPEG compression, cadence:???`10s per filtergram, ; ;telemetry needed: 300kbps, nocompensation of the solar rotation ;and;#8226;NFI: FeI630.25nm longitudinal magnetograms,other parameters as in ; ;case of BFI ;and;#8226;SP:none; Scientific Objectives: This proposal merges together attempts to observe two kinds of solarstructures and;#8211; solar micro flares and super granular network and;#8211; which are planned tobe investigated toaddress common openquestions on the irrelevance for the heating and dynamics of the solar corona.; Other Instruments: DOT SoHO/CDS/MDI/EIT JOP 189: 3-17 Aug 2007 7:00 - 13:30 UT TRACE RHESSI;;Daily Note and User Entry: HOP20: solar microflares and supergranular network dynamics (SOT/XRT/EIS) (07:00 - 13:30 UT) EIS sensitivity monitoring EIS: Target of opportunity observations of coronal hole on disk. XRT: CCD Bakeout plus test X-ray images SOT: Support HOP 20 07:00-13:30 UT; Request to SOT: SOT: We plan (if possible) to run in time a sequence of 3exposures:2using the BFI imager and 1 using the NBIimager.The reason is to cover evolution of the photosphere with its magnetic concentration signatures (G-band), evolution of the longitudinal component of the magnetic field vector inthe photosphere, and evolution of chromosphere (CaIIH)witha reasonable temporal resolution (???`10s per image,???@???`30s???@per???@sequence???@of 3 selected channels).???@ ???@and;#8226;BFI: G-band and CaIIH channels, ???@ ;FOV:109???hx109???h(1k x1kmode, binning 2 x 2 pxs), ; ;3bit JPEG compression, cadence:???`10s per filtergram, ; ;telemetry needed: 300kbps, nocompensation of the solar rotation ;and;#8226;NFI: FeI630.25nm longitudinal magnetograms,other parameters as in ; ;case of BFI ;and;#8226;SP:none; Scientific Objectives: This proposal merges together attempts to observe two kinds of solarstructures and;#8211; solar micro flares and super granular network and;#8211; which are planned tobe investigated toaddress common openquestions on the irrelevance for the heating and dynamics of the solar corona.; Other Instruments: DOT SoHO/CDS/MDI/EIT JOP 189: 3-17 Aug 2007 7:00 - 13:30 UT TRACE RHESSI ivo://sot.lmsal.com/VOEvent#2007-08-20T11:20:00Z