Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-10-26
Astronomy and Astrophysics
Astrophysics
23 pages, no figures. Submitted to Computer Physics Communications. Code available at http://www.iagusp.usp.br/~alexsilv/popra
Scientific paper
10.1016/S0010-4655(01)00149-7
We describe a Fortran 90 program to calculate population ratios of atomic levels. The program solves the equations of statistical equilibrium considering all possible bound-bound processes: spontaneous, collisional or radiation induced (the later either directly or by fluorescence). There is no limit on the number of levels or in the number of processes that may be taken into account. The program may find a wide range of applicability in astronomical problems, such as interpreting fine-structure absorption lines or collisionally excited emission lines (such as coronal emission lines) in the spectra of several objects, and also in calculating the cooling rates due to collisional excitation.
Silva A. I.
Viegas M. M. S.
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