Resistive evolution of the magnetized Kelvin-Helmholtz instability
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Lee, H | ko |
| dc.contributor.author | Kim, T | ko |
| dc.contributor.author | Min, KyoungWook | ko |
| dc.date.accessioned | 2013-02-28T00:33:10Z | - |
| dc.date.available | 2013-02-28T00:33:10Z | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.issued | 1997 | - |
| dc.identifier.citation | NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS, v.20, no.1, pp.121 - 126 | - |
| dc.identifier.issn | 0390-5551 | - |
| dc.identifier.uri | http://hdl.handle.net/10203/71763 | - |
| dc.description.abstract | It is found from the resistive MHD simulation that the most effective momentum transport due to Kelvin-Helmholtz instability is obtained in the small range of magnetic-field intensity when the highly sheared field lines undergo magnetic reconnection in the late stage of the evolution. | - |
| dc.language | English | - |
| dc.publisher | EDITRICE COMPOSITORI BOLOGNA | - |
| dc.title | Resistive evolution of the magnetized Kelvin-Helmholtz instability | - |
| dc.type | Article | - |
| dc.identifier.wosid | A1997XA62400007 | - |
| dc.identifier.scopusid | 2-s2.0-0040600546 | - |
| dc.type.rims | ART | - |
| dc.citation.volume | 20 | - |
| dc.citation.issue | 1 | - |
| dc.citation.beginningpage | 121 | - |
| dc.citation.endingpage | 126 | - |
| dc.citation.publicationname | NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS | - |
| dc.contributor.localauthor | Min, KyoungWook | - |
| dc.contributor.nonIdAuthor | Lee, H | - |
| dc.contributor.nonIdAuthor | Kim, T | - |
| dc.type.journalArticle | Article | - |
| dc.subject.keywordPlus | MAGNETOSPHERIC BOUNDARY | - |
| dc.subject.keywordPlus | DEPENDENCE | - |
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