Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2009-08-29 15:52:56-17:00:56
HOP 81 Polar monitoring
CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle
x,y:-10",932"
Max FOV:32"x81"
Target:N Pole
Nearby Events
6302A Continuum Intensity32"x81"1006 spectra
6302A Longitudinal Flux Density32"x81"1006 spectra
6302A Transverse Flux Density32"x81"1006 spectra
6302A Velocity 6301.5A32"x81"1006 spectra

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SOTSP: HOP 81 Polar monitoring
2009-08-29T15:52:56 to 2009-08-29T17:00:56
Science Goal: CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle
Program: Fast map half height 32", Q75, 1-side CCD
Target: N Pole
xcen=-10 ycen=932
Instrument: SOTSP
HOP/JOP: 81
Description: 1: To observe the evolution of the magnetic field distribution around the poles during the solar cycle. 2: To understand the relationship between photospheric magnetic field and the coronal structures (include the solar wind) around the poles. For FSM ???EBFI G-band: FoV 221"x111", Binning: 2x2, Time resolution: 30 min, JPEG Quality: Q75, Data rate: 9 Mbits/h Note: The G-band images are used for mainly co-alignment. Please insert a G-band image when the observation starts. ???ENFI Na I: IVDG mode, FoV: 328???h x 164???h, Binning: 2x2, Time resolution: 5 min, JPEG Quality: Q75, Data rate: 102 Mbits/h ???E SP FoV 320???h x 164???h, Pixel size: 0.32???h/pix, Binning: 2x2, Single side mode Exposure: 4.8 sec (6 Cycles), JPEG Quality: Q75, Data rate: 600Mbits/map

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Hits: 32
Chief Observer
Frank(RCO)
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Cites: HOP 81 Polar monitoring     
Timeline: gif use
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 32,81 images: 1006 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 32,81 images: 1006 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 32,81 images: 1006 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 32,81 images: 1006 JavaScript Landing Page
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