Thermal Doppler Broadening of Spectral Emissions in Space and Astrophysical Plasmas
Authors: G. Livadiotis
2018 The Astrophysical Journal Supplement Series23925.
Provider: AAS Journals
Caption: Figure 6.
Voigt differential profiles plotted for positive attractive potential (oscillation-type) ﹩{\rm{\Phi }}(r)/m=k\cdot {r}^{b}﹩ with b = 5, and for various kappa indices (κ = 1.55, 1.7, 2.5, 20) and convolution ratios S (0.4, 1, 3).