2007-08-12T23:11:07.000Z http://sot.lmsal.com Ed DeLuca SAO http://hea-www.harvard.edu MS 58, 60 Garden St, Cambridge, MA 02138 +1-617-496-7725 edeluca@cfa.harvard.edu Hinode XRT Sterling Matsumoto Takuma 12,29 0 null G-band Monitoring of CCD 0 -1000000000 -1000000000 0 0 2007-08-09T11:16:54.000Z 2007-08-10T05:59:54.000Z -1000000000 -1000000000 Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs, IHY FILAMENT OBSERVING CAMPAIGN: Activity in Filaments and Filament Cavities CCD_Monitor_During_Bakeout_4_strips Tim File-OBS_DEC: Monitor CCD with G-band; Daily Note: none; Request to XRT HOP Number 0012: 2. ?@ ; ; ; ; ;Monitor around the jets 3.?@ ; ; ; ; ;Monitor around the Ellerman bomb; Other Instruments: ; Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: none; Request to XRT HOP Number 0029: ; Other Instruments: Other Instruments (with campaign points of contact): -------------------------------------------------- SOHO/CDS and SOHO/EIT (Terry Kucera); SOHO/UVCS (Kuen Ko, John Raymond); SMEI (David Webb); STEREO/SECCHI (Simon Plunkett, James Mcateer); TRACE (Kathy Reeves); MLSO (Joan Burkepile); HELIO (Sara Martin); COMP (Steve Tomczyk) ; Scientific Objectives: Goals: To study filaments, filament channels, and filament cavities in order to (a) understand the time dependent, three dimensional density, temperature, and magnetic structure of filaments and filament channels and cavities (b) study how filaments form (c) study filament activation in the chromosphere and CMEs in the corona to better understand how this process works and how it is related to CMEs. In addition, if the observed structures erupt we will (d) study the evolution of the cavity during eruption, and (e) map the EUV signatures into the coronal structures as represented by the coronagraphs, with the goal of understanding more clearly the structure and manifestations of CMEs in the low corona.