Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2014-09-09 11:14:37-14:04:47
Polar Panorama Map for understanding Polar Reversal in Cycle 24
Polar Panorama Map for understanding Polar Reversal in Cycle 24
x,y:-14",891"
Max FOV:267"x162"
Target:N Pole
Nearby Events
6302A Continuum Intensity267"x162"850 spectra
6302A Longitudinal Flux Density267"x162"850 spectra
6302A Transverse Flux Density267"x162"850 spectra
6302A Velocity 6301.5A267"x162"850 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 13 MB
SOTSP: Polar Panorama Map for understanding Polar Reversal in Cycle 24
2014-09-09T11:14:37 to 2014-09-09T14:04:47
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=891
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: 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: 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: 59
Chief Observer
Cruz(RCO)
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 267,162 images: 850 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 267,162 images: 850 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 267,162 images: 850 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 267,162 images: 850 JavaScript Landing Page
Time Series (SP Datacubes)