2024-09-24T22:21:35.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null HINODE SOTSP Hosoi Yasuda DeRosa 336 HOP336 cycle 25 BPs (S hemi) Active Region BP BP 2 20171016_130404 462 495 480 2 20 2047 6 1 1 1 0 21 2019 2031 0.9921836834391793 -21.35 -804.39 321.914 81.152 2017-10-16T13:04:04.000Z 2017-10-16T15:57:48.000Z -21.35 -804.39 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.;;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. ivo://sot.lmsal.com/VOEvent#2017-10-16T13:04:00Z