2008-10-18T11:19:48.000Z 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 SOT Arikawa Sterling Ishikawa 91 91 null HOP 91: Nanoflares QS QS Quiet Sun 4 -17 -100 0 0 2008-10-18T18:14:00.000Z 2008-10-18T23:54:00.000Z -17 -100 CORE Quiet sun nanoflares Na MG4 V/I +140, Ca II H, full FOV The quiet Sun is very dynamic. SXT on Yohkoh dicovered continuous and ubiquitous flaring activity above the phostospheric network and in bright points. We intend to perform a statistical studies of the physical properties of these quiet Sun nanoflares (also known as network flares), investigating frequency, brightness, temperature and luminosity distributions, as well as the structure of the photospheric magnetic field at the nanoflaring sites. TOO for quiet Sun near disk center.