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


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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.

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D. Kuli-Zade

Baku State University

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Email: ckulizade@mail.ru
阿塞拜疆, Baku, AZ 1148

S. Mamedov

Shamakhy Astrophysical Observatory

Email: ckulizade@mail.ru
阿塞拜疆, Shamakhi, AZ 5626

Z. Aliyeva

Baku State University

Email: ckulizade@mail.ru
阿塞拜疆, Baku, AZ 1148

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