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The fraunhofer lines classifications by asymmetry changes inside the profiles in the spectrum of the Sun

The fraunhofer lines classifications by asymmetry changes inside the profiles in the spectrum of... The method of asymmetry change inside Fraunhofer lines profiles is proposed. New digital spectra with high resolution were used. It was shown that asymmetry may change repeatedly by value and a sign inside the spectral line profile. The lines can be classified in three groups on asymmetry changes inside the profiles. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Astrophysical Bulletin Springer Journals

The fraunhofer lines classifications by asymmetry changes inside the profiles in the spectrum of the Sun

Kuli-Zade, D.; Mamedov, S.; Aliyeva, Z.
Astrophysical Bulletin , Volume 72 (3) – Sep 9, 2017
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Publisher
Springer Journals
Copyright
Copyright © 2017 by Pleiades Publishing, Ltd.
Subject
Physics; Astronomy, Astrophysics and Cosmology
ISSN
1990-3413
eISSN
1990-3421
DOI
10.1134/S1990341317030221
Publisher site
See Article on Publisher Site

Abstract

The method of asymmetry change inside Fraunhofer lines profiles is proposed. New digital spectra with high resolution were used. It was shown that asymmetry may change repeatedly by value and a sign inside the spectral line profile. The lines can be classified in three groups on asymmetry changes inside the profiles.

Journal

Astrophysical Bulletin – Springer Journals

Published: Sep 9, 2017

References

  • Solar Flux Atlas from 296 to 1300 nm
    Kurucz, R. L.; Furenlid, I.; Brault, J.; Testerman, L.