Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2018-09-05 11:34:37-14:28:11
HOP 206 N-pole
Polar Panorama Map for understanding Polar Reversal in Cycle 24
x,y:-17",850"
Max FOV:319"x162"
Target:North pole
Nearby Events
6302A Continuum Intensity319"x162"1015 spectra
6302A Longitudinal Flux Density319"x162"1015 spectra
6302A Transverse Flux Density319"x162"1015 spectra
6302A Velocity 6301.5A319"x162"1015 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 17 MB
SOTSP: HOP 206 N-pole
2018-09-05T11:34:37 to 2018-09-05T14:28:11
Science Goal: Polar Panorama Map for understanding Polar Reversal in Cycle 24
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: North pole
xcen=-17 ycen=850
Instrument: SOTSP
HOP/JOP: 206
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
Related Links
Cites: HOP 206 N-pole     
Timeline: gif use
See also
Datasets
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 319,162 images: 1015 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 319,162 images: 1015 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 319,162 images: 1015 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 319,162 images: 1015 JavaScript Landing Page
Time Series (SP Datacubes)
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