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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Journal of Astrophys...arrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Journal of Astrophysics and Astronomy
Article . 2000 . Peer-reviewed
License: Springer TDM
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International Astronomical Union Colloquium
Article . 2000 . Peer-reviewed
Data sources: Crossref
https://dx.doi.org/10.1007/bf0...
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Magnetoconvection and the solar dynamo

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2000 English Publisher:Springer Science and Business Media LLCJournal:Journal of Astrophysics and Astronomy, volume 21, pages 307-313 (issn: 0250-6335, eissn: 0973-7758, Copyright policy )
Authors: Å. Nordlund; S. B. F. Dorch; R. F. Stein;

doi: 10.1007/bf02702415 , 10.1017/s0252921100064733

Magnetoconvection and the solar dynamo

Abstract

AbstractWe review current understanding of the interaction of magnetic fields with convective motions in stellar convection zones. Among the most exciting recent results is the discovery that magnetic fields need not primarily be confined to the stable layer below the convection zone; numerical simulations have shown that surprisingly, strong magnetic fields can be maintained in the interior of the convection zone.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
4
Average
Average
Average
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