2008-10-21T15:27:24.000Z 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 SOT Arikawa Sterling Ishikawa 91 HOP 91: Nanoflares Quiet Sun QS QS 4 -16 -99 327 163 2008-10-18T18:14:31.000Z 2008-10-18T23:34:41.000Z -16 -99 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. ivo://sot.lmsal.com/VOEvent#2008-10-18T18:14:00Z