Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOTSP: HOP 206 N-pole
2018-09-05T15:00:00 to 2018-09-05T18:05:05
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=-18 ycen=844
Instrument: SOT
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.

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Chief Observer
Muhamad
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contextwavelength: null cadence: fov: null,null images: null