SOTSP: HOP59 QS evolution
2008-01-22T11:20:54 to 2008-01-22T12:24:07
Science Goal: CORE: Quiet Sun Evolution - A Hinode Heritage Study
Program: Fast Map, Full FOV
Target: Quiet Sun
xcen=-341 ycen=-1
Instrument: SOTSP
HOP/JOP: 59
Description:
Scientific Objectives: A long, continuous study of the quiet Sun is requested to form a heritage 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.
Scientific Objectives: A long, continuous study of the quiet Sun is requested to form a heritage 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.
wavelength: 6302A Continuum Intensity cadence: 0 min fov: 317,162 images: 1000 JavaScript Landing Page
