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The Xray-EUV spectrum of optically thin plasmas

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Abstract

The new observations of the Extreme Ultraviolet Explorer Spectrometers on EUVE and the future high resolution observation by Coronal Diagnostic Spectrometer (CDS) and SUMER on SOHO have suggested the revision of the Xray-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 Xray-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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Authors and Affiliations

  1. Astrophysical Observatory of Arcetri, Florence, Italy

    B. C. Monsignori Fossi

  2. Department of Astronomy and Space Science, University of Florence, Italy

    M. Landini

Authors
  1. B. C. Monsignori Fossi
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  2. M. Landini
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Monsignori Fossi, B.C., Landini, M. The Xray-EUV spectrum of optically thin plasmas. Sol Phys 152, 81–86 (1994). https://doi.org/10.1007/BF01473187

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  • DOI: https://doi.org/10.1007/BF01473187

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