2024-09-17T21:07:23.354447Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin ATC, 3251 Hanover St., Palo Alto, CA 94306 null null HINODE SOTSP Arikawa Narukage Nitta (RCO) 393 HOP 393 (equatorial 336) Bright Points BP BP 2 20200627_142635 300 333 183 2 40 2000 2 1 1 0 2 21 2009 948 0.948 -28.183 -73.229 300.516 162.304 2020-06-27T14:26:35.000Z 2020-06-27T15:26:57.000Z -28.183 -73.229 Observe bright points near disk center to monitor solar cycle Fast Map, Full FOV 1 side CCD Q75 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.