The soft X-ray polychromator for the Solar Maximum Mission

Details The soft X-ray polychromator for the Solar Maximum Mission The soft X-ray polychromator for the Solar Maximum Mission

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...65...53a&link_type=abstract

Solar Physics, vol. 65, Feb. 1980, p. 53-71. Research supported by the Science Research Council of England;

Physics

171

Abundance, Line Spectra, Solar Maximum Mission, Solar Temperature, Solar X-Rays, X Ray Spectra, Helium Ions, Hydrogen Ions, Plasma Diagnostics, Solar Flares, Spectrometers

Scientific paper

The paper considers the soft X-ray polychromator (XRP) operating in the 1.4-22.4 A range of the soft X-ray spectrum which includes many emission lines important for the diagnosis of plasmas in the 1.5-50 million deg temperature range. The flat crystal scanning spectrometer provides for a channel polychromatic mapping of flares and active regions in the resonance lines of O VIII, Ne IX, and Mg XI; in its spectral scanning mode it covers essentially the entire 1.4-22.5 A region.

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