2009-04-20T17:17:20.000Z 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 Arikawa Sterling Suematsu 72 72 null HOP 72 Radiative structure of small magnetic elements: faculae, network and inter network in the quiet Sun QS Quiet Sun 7 -535 -6 0 0 2008-08-08T09:30:00.000Z 2008-08-08T09:41:00.000Z -535 -6 Radiative structure of small magnetic elements: faculae, network and inter network in the quiet Sun Fast map, 62"x82", single, 1-side CCD, Q75 Scientific Objectives: The smallest magnetic features in the solar photosphere are the G-band bright points. It is fundamental to study their structure and size, as they are in the resolution limit,and can appear as points or unresolved features (Ishiwawa et al 2007, Berger et al 2004). We intend to study them at maximum spatial resolution in intensity and magnetic field at several wavelengths to determine their dimensional and thermal structure. Observations in G-band (=430.5nm), CaII(=396.9nm), CN(=388.35nm) as well as magnetograms: MgIb(=517.27nm), FeI(=517.27nm) and NaID(=589.6nm are proposed in this document.