Spectroscopic diagnostics in the VUV for solar and stellar plasmas

Details Spectroscopic diagnostics in the VUV for solar and stellar plasmas Spectroscopic diagnostics in the VUV for solar and stellar plasmas

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26arv...6..123m&link_type=abstract

Astronomy and Astrophysics Review (ISSN 0935-4956), vol. 6 no. 1-2, p. 123-179

Astronomy and Astrophysics

Astronomy

99

Plasmas (Physics), Solar Physics, Solar Spectra, Space Plasmas, Ultraviolet Astronomy, Ultraviolet Spectra, Atomic Energy Levels, Continuous Spectra, Emission Spectra, Extreme Ultraviolet Explorer Satellite, Hubble Space Telescope, Iue, Rosat Mission, Skylab Program, Solar Observatories

Scientific paper

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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