Multitemperature analysis of solar X-ray line emission

Details Multitemperature analysis of solar X-ray line emission Multitemperature analysis of solar X-ray line emission

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...67..285s&link_type=abstract

Solar Physics, vol. 67, Sept. 1980, p. 285-309.

Physics

52

Emission Spectra, Solar Spectra, Solar Temperature, Solar X-Rays, Spectrum Analysis, X Ray Spectra, Abundance, Computerized Simulation, High Temperature Plasmas, Line Spectra, Plasma Diagnostics, Solar Maximum Mission, Solar Wind, Stellar Models, Temperature Measurement

Scientific paper

A new method of multitemperature analysis of solar X-ray spectra is proposed and tested. The method, based on a technique developed by Withbroe (1975), is designed to be used in the interpretation of spectra, to be measured by the X-Ray Polychromator on the Solar Maximum Mission. Various tests of the method on simulated temperature models establish its usefulness, generality, and stability. The possibilities of deriving the relative element abundances are analyzed. The results of the present paper extend the possibility of the multitemperature analysis of X-ray spectra as compared with the results of Craig and Brown (1976) and Craig (1977).

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