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Overview Where Groups: Mode, FOV, # spectra in map Data Links
2013-09-09 13:55:04-16:48:38
HOP 206 (Polar Panorama Map)
Polar Panorama Map for understanding Polar Reversal in Cycle 24
x,y:-14",883"
Max FOV:322"x162"
Target:N Pole
Nearby Events
6302A Continuum Intensity322"x162"1022 spectra
6302A Longitudinal Flux Density322"x162"1022 spectra
6302A Transverse Flux Density322"x162"1022 spectra
6302A Velocity 6301.5A322"x162"1022 spectra

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SP Cubes 16 MB
SOTSP: HOP 206 (Polar Panorama Map)
2013-09-09T13:55:04 to 2013-09-09T16:48:38
Science Goal: Polar Panorama Map for understanding Polar Reversal in Cycle 24
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: N Pole
xcen=-14 ycen=883
Instrument: SOTSP
HOP/JOP: 206
Description: Request to SOT HOP Number 0206 ???EBFI G-band: FoV 221"x111", Binning: 2x2, Time resolution: 30 min, JPEG Quality: Q75, Data rate: 9 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 Other Instruments: Scientific Objectives: The data obtained by the HOP81 observations show that the longitudinal dependence of polar reversal is large. Especially, the dependence becomes important for understanding the progress of polar reversal when polar reversal is progressing to the final phase. Hence, we propose the special observation for taking the panorama map of magnetic field around Pole. If we want to make the panorama map that covers until 65 degrees latitude, we need to perform the polar observation every 3.5 days during one month. Considering the matters about Hinode operation (flares, satellite operation, etc.), we request to perform the polar observation every 3 days. It means that we need to perform 10 polar observations for one panorama map during one month.

Request to SOT HOP Number 0206 ???EBFI G-band: FoV 221"x111", Binning: 2x2, Time resolution: 30 min, JPEG Quality: Q75, Data rate: 9 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 Other Instruments: Scientific Objectives: The data obtained by the HOP81 observations show that the longitudinal dependence of polar reversal is large. Especially, the dependence becomes important for understanding the progress of polar reversal when polar reversal is progressing to the final phase. Hence, we propose the special observation for taking the panorama map of magnetic field around Pole. If we want to make the panorama map that covers until 65 degrees latitude, we need to perform the polar observation every 3.5 days during one month. Considering the matters about Hinode operation (flares, satellite operation, etc.), we request to perform the polar observation every 3 days. It means that we need to perform 10 polar observations for one panorama map during one month.

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Chief Observer
Cruz(RCO)
Related Links
Cites: HOP 206 (Polar Panorama Map)     
Timeline: gif use
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wavelength: 6302A Continuum Intensity cadence: -1 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: -1 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: -1 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: -1 min fov: 322,162 images: 1022 JavaScript Landing Page
Time Series (SP Datacubes)