A recalculation of the line emissivities for the strongest UV and extreme-UV lines in the 400-2800 A wavelength range

Details A recalculation of the line emissivities for the strongest UV and extreme-UV lines in the 400-2800 A wavelength range A recalculation of the line emissivities for the strongest UV and extreme-UV lines in the 400-2800 A wavelength range

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...264..173d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 264, no. 1, p. 173-176.

Astronomy and Astrophysics

Astrophysics

16

Emissivity, Line Spectra, Stellar Atmospheres, Stellar Coronas, Ultraviolet Spectra, Abundance, Atomic Excitations, Emission Spectra, Oscillator Strengths, Photosphere

Scientific paper

Using the most recent atomic data we re-calculate line emissivities for the strongest transitions in the 400-2800 A region. These line emissivities may be used to construct emission measure curves for either observed ultraviolet/extreme ultraviolet solar features or ultraviolet observations of stellar sources. The new tables contain several lines not in the original Raymond and Doyle tables.

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