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,
Gespeichert in:
| 1. Verfasser: | |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
03 August 2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 472, Heft: 2, Pages: 1628-1640 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1981 |
| Online-Zugang: | 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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| Verfasserangaben: | Kiwan Park*, Center for Astronomy, Institute for Theoretical Astrophysics at University of Heidelberg, D-69120 Heidelberg, Germany |
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| 245 | 1 | 0 | |a On the inverse transfer of (non-)helical magnetic energy in a decaying magnetohydrodynamic turbulence |c Kiwan Park*, Center for Astronomy, Institute for Theoretical Astrophysics at University of Heidelberg, D-69120 Heidelberg, Germany |
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| 520 | |a 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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