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2025-02-22T16:41:58-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-79632%22&qt=morelikethis&rows=5
2025-02-22T16:41:58-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-22T16:41:58-05:00 DEBUG: Deserialized SOLR response

Negative magnetic buoyancy and formation of a sunspot belt

Magnetic buoyancy constrains the magnitude of toroidal field excited by the Ω-effect near the bottom of the solar convection zone (SCZ). Therefore, we examined two negative magnetic buoyancy effects: i) macroscopic turbulent diamagnetism (the γ-effect) and ii) magnetic advection caused by vertical i...

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Bibliographic Details
Main Author: Kryvodubskyj, V.N.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
Series:Кинематика и физика небесных тел
Subjects:
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/79632
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