2025-02-22T16:41:58-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query 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: => 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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Main Author: | |
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Format: | Article |
Language: | English |
Published: |
Головна астрономічна обсерваторія НАН України
2005
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Series: | Кинематика и физика небесных тел |
Subjects: | |
Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/79632 |
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