1992•Unpublished venueRequires access

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

J. G. Doyle, F. P. Keenan

Abstract

Using the most recent atomic data, line emissivities are re-calculated 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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Key concepts: Physics, Extreme ultraviolet, Ultraviolet, Line (geometry), Astrophysics, Wavelength, Ultraviolet astronomy, Emission spectrum