Emissivity: A Program for Atomic Emissivity Calculations
Taha Sochi

TL;DR
This paper introduces a new, efficient software tool for calculating atomic emissivity, aiding astronomical research by generating and comparing theoretical and observational atomic transition data.
Contribution
The paper presents a novel program capable of rapid, resource-efficient atomic emissivity calculations with comprehensive algorithms for analyzing atomic transition lines.
Findings
Program successfully tested and validated.
Enables detailed comparison of theoretical and observational data.
Useful for astronomical atomic line analysis.
Abstract
In this article we report the release of a new program for calculating the emissivity of atomic transitions. The program, which can be obtained with its documentation from our website www.scienceware.net, passed various rigorous tests and was used by the author to generate theoretical data and analyze observational data. It is particularly useful for investigating atomic transition lines in astronomical context as the program is capable of generating a huge amount of theoretical data and comparing it to observational list of lines. A number of atomic transition algorithms and analytical techniques are implemented within the program and can be very useful in various situations. The program can be described as fast and efficient. Moreover, it requires modest computational resources.
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Taxonomy
TopicsAtomic and Molecular Physics · Advanced Frequency and Time Standards · Scientific Measurement and Uncertainty Evaluation
