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Spectroscopic diagnostics in the VUV for solar and stellar plasmas

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Summary

The VUV emission spectra from the solar atmosphere and stellar atmospheres have been intensively studied during the past 25 years with several major space programs. In this review we discuss the spectroscopic diagnostic techniques used to study astrophysical plasmas, the atomic processes involved, the recent observations and the plans for future space missions.

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  1. Department of Applied Mathematics and Theoretical Physics, Cambridge University, UK

    H. E. Mason

  2. Arcetri Astrophysical Observatory, Florence, Italy

    B. C. Monsignori Fossi

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Mason, H.E., Monsignori Fossi, B.C. Spectroscopic diagnostics in the VUV for solar and stellar plasmas. The Astron Astrophys Rev 6, 123–179 (1994). https://doi.org/10.1007/BF01208253

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