Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2019-09-03 16:01:22-18:54:55
HOP 206 N Pole
Polar Panorama Map for understanding Polar Reversal in Cycle 24
x,y:-21",868"
Max FOV:319"x162"
Target:N Pole
Nearby Events
6302A Continuum Intensity319"x162"1017 spectra
6302A Longitudinal Flux Density319"x162"1017 spectra
6302A Transverse Flux Density319"x162"1017 spectra
6302A Velocity 6301.5A319"x162"1017 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 17 MB
SOTSP: HOP 206 N Pole
2019-09-03T16:01:22 to 2019-09-03T18:54:55
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=-21 ycen=868
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 Note: margin factor FG 0x41c --- 1.3 SP 0x0c5 --- 1.3 Other Instruments: IRIS can support HOP 206 with the following program, at pointings of 0, ?}910: 3600110077 | Very large dense 320-step raster 105.3x175 arcsec FOV 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 Note: margin factor FG 0x41c --- 1.3 SP 0x0c5 --- 1.3 Other Instruments: IRIS can support HOP 206 with the following program, at pointings of 0, ?}910: 3600110077 | Very large dense 320-step raster 105.3x175 arcsec FOV 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.

Annotations:
Hits: 24
Chief Observer
Cruz (RCO)
Related Links
Cites: HOP 206 N Pole     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 319,162 images: 1017 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 319,162 images: 1017 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 319,162 images: 1017 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 319,162 images: 1017 JavaScript Landing Page
Time Series (SP Datacubes)