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EUV Line Intensities of Fe X
Published online by Cambridge University Press: 12 April 2016
Abstract
The 4 configuration, distorted wave calculation of Bhatia & Doschek (1995) (hereafter referred to as BD95), together with the ground transition calculation of Pelan & Berrington (1995) are here used to predict the intensities of the Fe X EUV lines, which are then used to derive electron densities from several solar spectra, including the recent SERTS spectra.
- Type
- XIII. Plasma Diagnostics
- Information
- International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 583 - 587
- Copyright
- Copyright © Kluwer 1996
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