2001AIP conference proceedingsRequires access

The project for the determination of Stark broadening parameters within the modified semiempirical approach: Ag II

D. Tankosić

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Abstract

Investigations of the Stark line broadening parameters are important for a number of problems in laboratory and astrophysical plasma research. We use a modified semiempirical approach in order to complete a set of the Stark broadening data. Here we present the Stark broadening data for 6 Ag II spectral lines calculated within the modified semiempirical approach.

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Investigations of the Stark line broadening parameters are important for a number of problems in laboratory and astrophysical plasma research. We use a modified semiempirical approach in order to complete a set of the Stark broadening data. Here we present the Stark broadening data for 6 Ag II spectral lines calculated within the modified semiempirical approach.

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Available abstract

Investigations of the Stark line broadening parameters are important for a number of problems in laboratory and astrophysical plasma research. We use a modified semiempirical approach in order to complete a set of the Stark broadening data. Here we present the Stark broadening data for 6 Ag II spectral lines calculated within the modified semiempirical approach.

Key concepts: Stark effect, Plasma, Doppler broadening, Spectral line, Atomic physics, Homogeneous broadening, Line (geometry), Plasma diagnostics

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