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- W1649291249 abstract "Physical properties such as temperature and electron density of solar plasma and other astrophysical objects can be inferred from EUV and X-ray emission lines observed from space. These lines are emitted when the higher states of an ion are excited by electron impact and then decay by photon emission. Excitation cross sections are required for the spectroscopic analyses of the observations and various approximations have been used to calculate the scattering functions. One of them which has been widely used is a distorted wave approximation. This approximation, along with its applications to solar observations, is discussed. The Bowen fluorescence mechanism and optical depth effects are also discussed. It is concluded that such calculations are reliable for highly charged ions and for high electron temperatures." @default.
- W1649291249 created "2016-06-24" @default.
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- W1649291249 date "2000-01-01" @default.
- W1649291249 modified "2023-09-26" @default.
- W1649291249 title "Distorted Wave Calculations and Applications" @default.
- W1649291249 hasPublicationYear "2000" @default.
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