2008-12-16T10:38:16.000Z 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 Magara 59 59 null HOP59 QS evolution CORE: Quiet Sun Evolution - A Hinode Heritage Study QS Quiet Sun 6 -132 -2 0 0 2008-01-23T10:50:00.000Z 2008-01-24T00:00:00.000Z -132 -2 CORE: Quiet Sun Evolution - A Hinode Heritage Study Fast Map, Full FOV Scientific Objectives: A long, continuous study of the quiet Sun is requested to form a ???eheritage???f data-set that will be suitable for a variety of scientific investigations both for current and future solar researchers. Request to SOT HOP Number 0059 Magnetograms are important for identifying magnetic cancellation/emergence events, while G-band and Ca II are important for identifying release at photospheric/chromospheric heights that can be related to the transition region/coronal emission observed with EIS. NFI Mg I magnetograms should be interspersed with BFI Ca II and G-band images. The BFI focus should be optimised for Ca II. Time cadence does not need to be high, and both NFI and BFI should have a FOV in X of at least 180???h (to match EIS), and have the full field of view in Y. It is important that a regular and consistent mixing of the three filters should be maintained during the 72 hour observation period to obtain a homogeneous data-set.