@Article{CiCP-7-1118,
author = {Taha Sochi},
title = {Emissivity: A Program for Atomic Transition Calculations},
journal = {Communications in Computational Physics},
year = {2010},
volume = {7},
number = {5},
pages = {1118--1130},
abstract = {<p style="text-align: justify;">In this article we report the release of a new program for calculating emissivity
and other physical parameters in atomic transition processes. The program, which
can be downloaded with its documentation and a sample of input and output files
from www.scienceware.net/id1.html, passed various rigorous tests and was used
alongside R-matrix and Autostructure codes 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 line list. 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.</p>},
issn = {1991-7120},
doi = {https://doi.org/10.4208/cicp.2009.09.125},
url = {http://global-sci.org/intro/article_detail/cicp/7667.html}
}