SOTSP: HOP 393 (equatorial 336)
2020-06-27T14:22:30 to 2020-06-27T15:27:00
Science Goal: Observe bright points near disk center to monitor solar cycle
Program: Fast Map, Full FOV 1 side CCD Q75
Target: Bright Points
xcen=-22 ycen=-81
Instrument: SOTSP
HOP/JOP: 393
Description:
Small magnetic features and coronal bright points have been shown to indicate the bands of activity associated with the solar cycle. The precise location of these bands is important for predicting the timing of solar minimum and, more generally, the long-term variability of the Sun.
