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Uspekhi Fizicheskikh Nauk, 2015, Volume 185, Number 6, Pages 643–648
DOI: https://doi.org/10.3367/UFNr.0185.201506h.0643 (Mi ufn5261) 		 
This article is cited in 23 scientific papers (total in 23 papers)

CONFERENCES AND SYMPOSIA. 75th ANNIVERSARY OF IZMIRAN

Problems of magnetic dynamo

D. D. Sokoloffab

a Lomonosov Moscow State University, Faculty of Physics
b N V Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Troitsk, Moscow
Full-text PDF (169 kB) Citations (23)
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DOI: https://doi.org/10.3367/UFNr.0185.201506h.0643
Abstract: In what is famously known as the solar activity cycle, every 11 years a wave from a quasistationary magnetic field propagates in the solar convective zone from the middle latitudes equatorwards, driven by the dynamo jointly produced by differential rotation and mirror-asymmetric convection. Similar processes occur in other celestial bodies and can to some extent be reproduced in the lab environment. This paper reviews the current status of and future trends in the study of the dynamo phenomenon.
Funding agency Grant number
Russian Foundation for Basic Research 15-02-01407
This work was supported by RFBR project No. 15-02-01407.
Received: March 20, 2015
Accepted: February 25, 2015
English version:
Physics–Uspekhi, 2015, Volume 58, Issue 6, Pages 601–605
DOI: https://doi.org/10.3367/UFNe.0185.201506h.0643
Bibliographic databases:
Document Type: Article
PACS: 07.55.Db, 41.20.-q, 91.25.-r, 96.12.Hg, 96.60.Hv
Language: Russian
Citation: D. D. Sokoloff, “Problems of magnetic dynamo”, UFN, 185:6 (2015), 643–648; Phys. Usp., 58:6 (2015), 601–605
Citation in format AMSBIB
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  • https://www.mathnet.ru/eng/ufn/v185/i6/p643
    CONFERENCES AND SYMPOSIA
    This publication is cited in the following 23 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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