2024-09-04T00:31:13.841319Z 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 Hosoi Yasuda DeRosa 336 HOP336 cycle 25 BPs (N hemi) Bright Points BP BP 2 20171016_100538 462 495 480 2 20 2047 6 1 1 0 1 21 2019 1972 0.9633610161211529 -20.343 544.818 312.562 81.152 2017-10-16T10:05:38.000Z 2017-10-16T12:59:21.000Z -20.343 544.818 Cycle 25 Bright Points Normal 320"x82", 1 side, 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. Hinode SP measurements will give us high resolution vector field data, and IRIS will show the chromospheric spectral signature of the bright points.