SOT: HOP59 QS evolution
2008-01-24T00:05:50 to 2008-01-24T00:15:10
Science Goal: CORE: Quiet Sun Evolution - A Hinode Heritage Study
Program: Mg IVDG, Ca 82x82"", 2x2, 20s
Target: Quiet Sun
xcen=0 ycen=0
Instrument: SOT
HOP/JOP: 59
Description:
Scientific Objectives: A long, continuous study of the quiet Sun is requested to form a ùeheritageùf 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 180ùh (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.
wavelength: TF Mg I 5172 cadence: 0.45 min fov: 20,20 images: 21 JavaScript Landing Page
