How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities?
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| Title: | How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities? |
|---|---|
| Authors: | Favier, B.1, Jouve, L.2,3, Edmunds, W.1, Silvers, L. J.4, Proctor, M. R. E.1 |
| Source: | Monthly Notices of the Royal Astronomical Society; Nov2012, Vol. 426 Issue 4, p3349-3359, 11p |
| Database: | Applied Science & Technology Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: aci DbLabel: Applied Science & Technology Source An: 82614698 AccessLevel: 2 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=aci&AN=82614698 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1111/j.1365-2966.2012.21920.x Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 11 StartPage: 3349 Titles: – TitleFull: How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities? Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Favier, B. – PersonEntity: Name: NameFull: Jouve, L. – PersonEntity: Name: NameFull: Edmunds, W. – PersonEntity: Name: NameFull: Silvers, L. J. – PersonEntity: Name: NameFull: Proctor, M. R. E. IsPartOfRelationships: – BibEntity: Dates: – D: 11 M: 11 Text: Nov2012 Type: published Y: 2012 Identifiers: – Type: issn-print Value: 00358711 Numbering: – Type: volume Value: 426 – Type: issue Value: 4 Titles: – TitleFull: Monthly Notices of the Royal Astronomical Society Type: main |
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