SOTSP: amgnetic field in weak plage
2007-10-24T04:27:25 to 2007-10-24T04:48:38
Science Goal: Wavefront tes with focus
Program: Normal map 40 arcsec half height
Target: Plage
xcen=99 ycen=-249
Instrument: SOTSP
HOP/JOP: 0
Description:
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.
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.
wavelength: 6302A Continuum Intensity cadence: -1 min fov: 40,81 images: 250 JavaScript Landing Page
