Observation

Observation Details

Overview

Where

Groups: Mode, FOV, # spectra in map

Data Links

2018-09-11 14:20:06-17:13:40

HOP 206 N Pole

Polar Panorama Map for understanding Polar Reversal in Cycle 24

x,y:	-19",873"
Max FOV:	321"x162"
Target:	N Pole
Nearby Events

6302A Continuum Intensity	321"x162"	1019 spectra
6302A Longitudinal Flux Density	321"x162"	1019 spectra
6302A Transverse Flux Density	321"x162"	1019 spectra
6302A Velocity 6301.5A	321"x162"	1019 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly

SOTSP: HOP 206 N Pole

2018-09-11T14:20:06 to 2018-09-11T17:13:40

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=-19 ycen=873

Instrument: SOTSP

HOP/JOP: 206

Description: abstract of observational proposal 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 ? SP FoV 320? x 164?, Pixel size: 0.32?/pix, Binning: 2x2, Single side mode Exposure: 4.8 sec (6 Cycles), JPEG Quality: Q75, Data rate: 600Mbits/map Note: margin factor SP 0x0c5 --- 1.3

abstract of observational proposal 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 ? SP FoV 320? x 164?, Pixel size: 0.32?/pix, Binning: 2x2, Single side mode Exposure: 4.8 sec (6 Cycles), JPEG Quality: Q75, Data rate: 600Mbits/map Note: margin factor SP 0x0c5 --- 1.3

Annotations:

Chief Observer

Cruz (RCO)