Coronal Emission Lines with UVCS

Details Coronal Emission Lines with UVCS Coronal Emission Lines with UVCS

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.3702r&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #37.02; Bulletin of the American Astronomical Society, Vol. 28, p.877

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Scientific paper

The Ultraviolet Coronagraph Spectrometer aboard the SOHO satellite has observed the extended solar corona in H I Lyalpha and O VI lines for coronal diagnostics, but other, fainter, lines are also present. We discuss a spectral atlas obtained from emission in equatorial streamers and above solar active regions, pointing out lines which are especially useful for determining the elemental abundances, ionization state, and density of the emitting plasma. This work is supported by NASA under contract NAS5-31250 to the Smithsonian Astrophysical Observatory.

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