RAPOC: The Rosseland and Planck opacity converter
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Published:2022-10-29
Issue:2
Volume:55
Page:521-539
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ISSN:0922-6435
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Container-title:Experimental Astronomy
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language:en
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Short-container-title:Exp Astron
Author:
Mugnai Lorenzo V.ORCID, Modirrousta-Galian DariusORCID
Abstract
Abstract (Rosseland and Planck Opacity Converter) is a Python 3 code that calculates Rosseland and Planck mean opacities (RPMs) from wavelength-dependent opacities for a given temperature, pressure, and wavelength range. In addition to being user-friendly and rapid, can interpolate between discrete data points, making it flexible and widely applicable to the astrophysical and Earth-sciences fields, as well as in engineering. uses ExoMol, DACE, or any user defined input data, provided that it is in a readable format. In this paper, we present the code and compare its calculated Rosseland and Planck mean opacities with other values in the literature. is open-source and available on Pypi and GitHub.
Funder
Agenzia Spaziale Italiana Università degli Studi di Roma La Sapienza
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
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