The X-ray-EUV spectrum of optically thin plasmas

Details The X-ray-EUV spectrum of optically thin plasmas The X-ray-EUV spectrum of optically thin plasmas

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152...81m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 81-86

Physics

34

Extreme Ultraviolet Radiation, Iron, Line Spectra, Rarefied Plasmas, Solar Corona, Solar X-Rays, Stellar Models, Extreme Ultraviolet Explorer Satellite, Soho Mission

Scientific paper

The new observations of the Extreme Ultraviolet Explorer Spectrometers on Extreme Ultraviolet Explorer (EUVE) and the future high resolution observation by Coronal Diagnostic Spectrometer (CDS) and Solar Ultraviolet Measurement of Emitted Radiation (SUMER) on the Solar and Heliospheric Observatory (SOHO) have suggested the revision of the X-ray-EUV spectral code of the authors (1990) for optically thin plasmas. More accurate atomic data computations are now available and several lines have been added. Work is in progress to update the X-ray-EUV code following the suggestions of the reviewers of the workshop on `Atomic data assessment for SOHO' held in Abingdon (March 1992). Special care is given to the highly ionized iron lines in the EUV spectral region.

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