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Thermal Doppler Broadening of Spectral Emissions in Space and Astrophysical Plasmas

  • Authors: G. Livadiotis

2018 The Astrophysical Journal Supplement Series 239 25.

  • Provider: AAS Journals

Caption: Figure 9.

Voigt differential profiles plotted for the angular potential ﹩{\rm{\Phi }}(\vartheta )=-{\boldsymbol{\mu }}\cdot {\boldsymbol{B}}=-\mu \,B\cos \vartheta ﹩ with ﹩\beta \equiv \mu \,B/({k}_{{\rm{B}}}T)=0.5﹩, and for various kappa indices (κ = 1.55, 1.7, 2.5, 20) and convolution ratios S (0.4, 1, 3).

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