2007-07-31T18:25:49.000Z 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 XRT Kamio Lundquist 0 G-band Monitoring of CCD 17 178.368 0.584 528.415 528.415 2007-07-30T08:40:44.000Z 2007-07-30T23:52:59.000Z 178.368 0.584 IHY FILAMENT OBSERVING CAMPAIGN: Activity in Filaments and Filament Cavities CCD_Monitor_During_Bakeout Tim File-OBS_DEC: Monitor CCD with G-band; Daily Note: none; Request to XRT HOP Number 0029: XRT (Hinode/XRT -- campaign contact: Kathy Reeves): --- XRT observations will be of the form of basic main observation loop over a target-focused FOV, with less frequent context observations including full-disk images. Main Loop: Filters: Al/poly (8-16 sec exposure), Ti/Poly (16-23 sec exposure) Cadence: ~1.5 min for whole loop FOV: 768""x384"" Context Observations: Al/poly (2048x2048, 2x2 binned), 5 thin Be (768""x384"" 23 sec) every ~30 minutes For both types of observations, cadences will be reduced as required to protect the CCD if there is an active region on the disk during the observations.; 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. ivo://sot.lmsal.com/VOEvent#2007-07-30T11:01:54Z