2007-10-24T22:14:31.000Z 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 SOT Arikawa Kamio Lites 0 high cadence field observations Quiet Sun CH, FT CH, FT 5 336 -360 19 88 2007-10-23T19:02:40.000Z 2007-10-23T20:15:02.000Z 336 -360 Field dynamics in CH Mg b Shless IQUV DG, 160x1k, 2x2 Daily Note and User Entry: SOT: --HOP28: Investigation of the quiet sun fine-scale structures ( -2007/10/23) (8 - 11 UT at Sun center; 15 - 17 UT at N limb) --Oslo Spicules, coordinated La Palma, Limb (11 - 14 UT) --Support for HOP 0036 - Coronal heating with EIS and Norikura --Support for HOP 0041 - A search for the roots of Parker's nanoflares --Support for HOP 0011 - Coordinated Campaign Observation with THEMIS. Start from 24 Oct, at 11 UT. --TOO: Xray Bright Point, active region near disk center (needs intermittent andnbsp; andnbsp; andnbsp; andnbsp;coverage for two days), Shimizu --Scattering Polarization in CN, Na D, 7 pointings quiet Sun, 4hours, Frans Snik, Utrecht U. (Core program.) --Quiet Sun network dynamics, disk center, 2 hours, Catherine Fischer, Utrecht U. andnbsp;(Core program.) (XRT could run disk center programs during these periods.) --FPP wavefront reconstruction with focus, active region plage (or disk-center QS), 4 hours, C. Keller, Utrecht U. (Core program.) XRT: - Support for HOP 0011 - Coordinated Campaign Observation with THEMIS - c. Measurements of Magnetic Energy and Helicity Fluxes. andnbsp;Start from 24 Oct, at 11 UT. - Support for HOP 0028 - Investigation of the quiet sun fine-scale structures - Support for HOP 0036 - Coronal heating; Simultaneous observations with EIS and Norikura Coronagraph - Support for HOP 0041 - A search for the roots of Parker's nanoflares - TOO: SOT coordination program: ephemeral active region study with SOT (SOT poc: Lites/Elliot) - Support for Oslo period on La Palma EIS: - Request time to observe on-disc coronal hole (should be near disc centre) either andnbsp; andnbsp;a) if the activity to the east of the CH is significant, andnbsp; andnbsp; andnbsp; to observe interchange reconnection (5.5 hrs) andnbsp; andnbsp;b) if not, to observe jet material fall-back (multiples of 2.5 hours) - HOP 28 (QS fine scale) and Oslo: 15 - 17 UT and 08 - 11 UT - HOP 36 (Norikura) observations above the limb: 22 - 02 UT - HOP 41 (nanoflares): any time, but for several hours- HOP 11 (or HOP 04, andnbsp;mag. helicity and energy flux): 0730 - 1100 UT andnbsp;(EIS will make narrow-slot movies primarily for He II.) Computer Maintainance Note: andnbsp;Computer maintainance is schedule after 15:00 JST. The data distributor ""datastrg1"" will be stopped. CP is required to complete the cmdi tranfer by 15:00 JST. ivo://sot.lmsal.com/VOEvent#2007-10-23T19:00:00Z