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An analysis of Markovian model microfield methods for stark broadening
Authors:Earl W Smith  Bernard Talin  J Cooper
Institution:National Bureau of Standards, Boulder, CO 80303, U.S.A.;Universite de Provence, Marseille, France;Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, CO 80303, U.S.A.
Abstract:Stark broadening theories which concentrate on the statistics of the plasma electric microfield rather than the dynamics of collisions have come to be known as Model Microfield Methods. In the present paper we present an analysis of Stark broadening problems based on Markovian model microfield statistics. Our derivation permits an easy comparison with traditional Stark broadening theories such as the impact and unified theories; this comparison is used to clarify the physical nature of the approximations employed by Markovian models. The strengths and weaknesses of various models are discussed, emphasizing the kangaroo process of Brissaud and Frisch, and methods are suggested for improving the current model microfield approach.
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