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Abstract: In this article we report the release of a new program for calculating theemissivity of atomic transitions. The program, which can be obtained with itsdocumentation from our website www.scienceware.net, passed various rigoroustests and was used by the author to generate theoretical data and analyzeobservational data. It is particularly useful for investigating atomictransition lines in astronomical context as the program is capable ofgenerating a huge amount of theoretical data and comparing it to observationallist of lines. A number of atomic transition algorithms and analyticaltechniques are implemented within the program and can be very useful in varioussituations. The program can be described as fast and efficient. Moreover, itrequires modest computational resources.



Autor: Taha Sochi

Fuente: https://arxiv.org/



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