On the inverse transfer of (non-)helical magnetic energy in a decaying magnetohydrodynamic turbulence
Abstract. In our conventional understanding, large-scale magnetic fields are thought to originate from an inverse cascade in the presence of magnetic helicity,
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
03 August 2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 472, Issue: 2, Pages: 1628-1640 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1981 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx1981 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/472/2/1628/4062205 
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| Author Notes: | Kiwan Park*, Center for Astronomy, Institute for Theoretical Astrophysics at University of Heidelberg, D-69120 Heidelberg, Germany |
| Summary: | Abstract. In our conventional understanding, large-scale magnetic fields are thought to originate from an inverse cascade in the presence of magnetic helicity, |
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| Item Description: | Gesehen am 12.06.2018 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1981 |