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Uspekhi Fizicheskikh Nauk, 2016, Volume 186, Number 6, Pages 577–596
DOI: https://doi.org/10.3367/UFNr.2016.02.037727 (Mi ufn5308) 		 
This article is cited in 8 scientific papers (total in 8 papers)

REVIEWS OF TOPICAL PROBLEMS

Current results on the asymptotics of dynamo models

E. P. Popovaab

a Lomonosov Moscow State University, Faculty of Physics
b Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Full-text PDF (974 kB) Citations (8)
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DOI: https://doi.org/10.3367/UFNr.2016.02.037727
Abstract: Magnetic field generation and evolution models that are capable of describing a large body of observational material are currently available for different celestial bodies. Despite recent decades of great success in numerical magnetic hydrodynamics and in detailed research into some specific problems, asymptotic methods still have to be used to clarify the magnetic field generation mechanism in dynamo theory. In this review, current asymptotic methods are presented together with the results of their application to the simulation of solar, stellar, and galactic magnetic activities.
Funding agency Grant number
Russian Science Foundation 16-17-10097
The work was supported by the Russian Science Foundation grant 16-17-10097.
Received: May 15, 2015
Revised: February 8, 2016
Accepted: February 12, 2016
English version:
Physics–Uspekhi, 2016, Volume 59, Issue 6, Pages 513–530
DOI: https://doi.org/10.3367/UFNe.2016.02.037727
Bibliographic databases:
Document Type: Article
PACS: 52.30.Cv, 96.60.Hv, 96.60.Q-
Language: Russian
Citation: E. P. Popova, “Current results on the asymptotics of dynamo models”, UFN, 186:6 (2016), 577–596; Phys. Usp., 59:6 (2016), 513–530
Citation in format AMSBIB
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    • This publication is cited in the following 8 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    		Успехи физических наук Physics-Uspekhi
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