A Collisional Radiative Code for Plasma Modeling

Details A Collisional Radiative Code for Plasma Modeling A Collisional Radiative Code for Plasma Modeling

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprb17075g&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

A collisional radiative model based on the atomic data calculated by the Flexible Atomic Code is presented. The model is capable of including most important atomic processes, such as collisional excitation, ionization, photoionization, radiative and dielectronic recombination. It is also possible to choose a subset of the processes to investigate the effects of the missing ones. The model uses an efficient iterative procedure to solve the statistical balance. The method does not assume the coronal approximation, therefore it can be used to investigate various density effects. The Flexible atomic Code, also developed by the author, is based on the relativistic distorted-wave approximation. Along with the collisional radiative model, they form an integral software package for the spectral modeling of highly ionized ions under a wide range of physical conditions.

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