An effective calculation method in theory of non-LTE stellar atmospheres - linearization separation technique.

Details An effective calculation method in theory of non-LTE stellar atmospheres - linearization separation technique. An effective calculation method in theory of non-LTE stellar atmospheres - linearization separation technique.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ppmto..13..152w&link_type=abstract

Publ. Purple Mt. Obs., Vol. 13, No. 2, p. 152 - 161

Computer Science

Stellar Atmospheres: Non-Lte Analysis

Scientific paper

This paper introduces a new calculation method of non-LTE stellar atmospheres. This method is based on the combination of the advantages of the complete linearization method by Auer and Mihalas (1969) and the separated-iteration technique. First, the equation of radiative transfer and constraints are linearized respectively, then the linearized equation of the radiative transfer and the linearized constraints are solved, separately. It overcomes the disadvantages of requiring the simultaneous solution of the corresponding equations by the complete linearization. The applicability of this method by calculating a small sample of H-He atmospheres and H line formations is demonstrated.

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