Astrophysics (Index)About

Voigt profile

(mathematical shape that models spectral lines)

The Voigt profile is a model shape of spectral lines, i.e., a model line profile. Its shape described by the Voigt function, which is a convolution combining two distribution functions that model the effects of two types of line broadening: Doppler broadening and pressure broadening. (These, and the result, are termed line broadening functions, or broadening functions, or BFs.) The math offers a means of analyzing a line regarding the two effects, separately and combined.

Voigt-function approximations have been developed because such convolutions are a computational challenge. With today's computing power, the approximations still may be useful for cases where such a model's calculation must be done many times, or for back-of-the-envelope estimates.


(spectrography,lines)
Further reading:
https://en.wikipedia.org/wiki/Voigt_profile
https://www.chemeurope.com/en/encyclopedia/Voigt_profile.html
https://scipython.com/book/chapter-8-scipy/examples/the-voigt-profile/
https://cefrc.princeton.edu/sites/g/files/toruqf1071/files/2018_hanson_plecture6.pdf
https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Stellar_Atmospheres_(Tatum)/10%3A_Line_Profiles/10.04%3A_Combination_of_Profiles

Referenced by pages:
convolution
line shape function

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