Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2018-09-06 13:50:05-16:43:38
HOP 81 (S-pole)
CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle
x,y:-17",-969"
Max FOV:323"x162"
Target:South Pole
Nearby Events
6302A Continuum Intensity323"x162"1021 spectra
6302A Longitudinal Flux Density323"x162"1021 spectra
6302A Transverse Flux Density323"x162"1021 spectra
6302A Velocity 6301.5A323"x162"1021 spectra
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SP Cubes 15 MB
SOTSP: HOP 81 (S-pole)
2018-09-06T13:50:05 to 2018-09-06T16:43:38
Science Goal: CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: South Pole
xcen=-17 ycen=-969
Instrument: SOTSP
HOP/JOP: 81
Description: To understand the fast solar wind, the relationship between photospheric magnetic fields and coronal structures in the polar coronal hole is very essential. During the polarity reversal, the opposite polarity magnetic field invade the polar region. At the time, the relationship between coronal activities/structures and photospheric magnetic field is very interesting for understanding the solar wind.

Annotations:
Hits: 41
Chief Observer
Muhamad --> Cruz (RCO)
Related Links
Cites: HOP 81 (S-pole)     
Timeline: gif use
See also
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 323,162 images: 1021 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 323,162 images: 1021 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 323,162 images: 1021 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 323,162 images: 1021 JavaScript Landing Page
Time Series (SP Datacubes)
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