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Matem. Mod., 2002, Volume 14, Number 10, Pages 95–104 (Mi mm542)  

This article is cited in 2 scientific papers (total in 2 papers)

Traveling contrast structures in various hydromagnetic dynamo models

A. P. Petrov

Peoples Friendship University of Russia

Abstract: Two models are analysed describing the propagation of the large-scale magnetic fields in galaxies. The specific patterns are considered known as magnetic fronts. The speed of the front has been derived in the principal asymptotic term.

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Received: 28.05.2001

Citation: A. P. Petrov, “Traveling contrast structures in various hydromagnetic dynamo models”, Matem. Mod., 14:10 (2002), 95–104

Citation in format AMSBIB
\Bibitem{Pet02}
\by A.~P.~Petrov
\paper Traveling contrast structures in various hydromagnetic dynamo models
\jour Matem. Mod.
\yr 2002
\vol 14
\issue 10
\pages 95--104
\mathnet{http://mi.mathnet.ru/mm542}
\mathscinet{http://www.ams.org/mathscinet-getitem?mr=1989784}
\zmath{https://zbmath.org/?q=an:1015.85003}


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    Citing articles on Google Scholar: Russian citations, English citations
    Related articles on Google Scholar: Russian articles, English articles

    This publication is cited in the following articles:
    1. Mikhailov E.A., “Wavefronts of the Magnetic Field in Galaxies: Asymptotic and Numerical Approaches”, Magnetohydrodynamics, 52:1-2 (2016), 117–124  isi  elib
    2. Andreasyan R.R., Mikhailov E.A., Andreasyan H.R., “Structure and Features of the Galactic Magnetic-Field Reversals Formation”, Astron. Rep., 64:3 (2020), 189–198  crossref  isi  scopus
  • Математическое моделирование
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