Accurate determination of the free-free gaunt factor - I. Non-relativistic gaunt factors

77Citations
Citations of this article
21Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Modern spectral synthesis codes need the thermally averaged free-free Gaunt factor defined over a very wide range of parameter space in order to produce an accurate prediction for the spectrum emitted by an ionized plasma. Until now no set of data exists that would meet this need in a fully satisfactory way. We have therefore undertaken to produce a table of very accurate non-relativistic Gaunt factors over a much wider range of parameters than has ever been produced before. We first produced a table of non-averaged Gaunt factors, covering the parameter space 10log εi = -20 to +10 and 10log w = -30 to +25. We then continued to produce a table of thermally averaged Gaunt factors covering the parameter space 10log γ 2 = -6 to +10 and 10log u = -16 to +13. Finally, we produced a table of the frequency integrated Gaunt factor covering the parameter space 10log γ 2 = -6 to +10. All the data presented in this paper are available online.

Cite

CITATION STYLE

APA

van Hoof, P. A. M., Williams, R. J. R., Volk, K., Chatzikos, M., Ferland, G. J., Lykins, M., … Wang, Y. (2014). Accurate determination of the free-free gaunt factor - I. Non-relativistic gaunt factors. Monthly Notices of the Royal Astronomical Society, 444(1), 420–428. https://doi.org/10.1093/mnras/stu1438

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free