Solar EUV, XUV and soft X-ray telescope facilities

Details Solar EUV, XUV and soft X-ray telescope facilities Solar EUV, XUV and soft X-ray telescope facilities

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sao..rept.....w&link_type=abstract

Final Report, 1 May 1977 - 31 Dec. 1981 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Extreme Ultraviolet Radiation, Solar Radiation, Spectroheliographs, Ultraviolet Telescopes, X Ray Telescopes, Chromosphere, Drawings, Mass Flow, Solar Flares, Solar Magnetic Field, Spatial Resolution

Scientific paper

Facility class, high resolution instrumentation can enable maximum spatial, spectral and temporal resolutions and provide understanding of the complex physical conditions in the outer solar atmosphere and the mechanisms responsible for these conditions. The scientific rationale for facility class instruments operating in the EUV, XUV, and soft X ray spectral ranges are discussed. Possible configurations for these facilities and priorities for their development are considered.

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