SOTSP: HOP 81 (S-pole)
2018-09-06T10:51:00 to 2018-09-06T13:50:00
Science Goal: CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: South Pole
xcen=-18 ycen=-976
Instrument: SOT
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.
