2017-10-16T17:47:49.000Z http://sot.lmsal.com Ted Tarbell LMSAL http://lmsal.com 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA, 94304 +1-650-424-2400 tarbell@lmsal.com Hinode SOTSP Hosoi Yasuda DeRosa 336 336 null HOP336 cycle 25 BPs (N hemi) BP BP Bright Points 2 -31 537 0 0 2017-10-16T10:04:00.000Z 2017-10-16T12:59:35.000Z -31 537 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.