Magnetic island merger as a mechanism for inverse magnetic energy transfer

Magnetic energy transfer from small to large scales due to successive magnetic island coalescence is investigated. A solvable analytical model is introduced and shown to correctly capture the evolution of the main quantities of interest, as borne out by direct numerical simulations. Magnetic reconne...

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Bibliographic Details
Main Authors: Zhou, Muni (Author), Bhat, Pallavi (Author), Gomes Loureiro, Nuno F (Author), Uzdensky, Dmitri A. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Nuclear Science and Engineering (Contributor), Massachusetts Institute of Technology. Plasma Science and Fusion Center (Contributor)
Format: Article
Language:English
Published: American Physical Society (APS), 2020-03-25T18:14:07Z.
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Online Access:Get fulltext
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042 |a dc 
100 1 0 |a Zhou, Muni  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Nuclear Science and Engineering  |e contributor 
100 1 0 |a Massachusetts Institute of Technology. Plasma Science and Fusion Center  |e contributor 
700 1 0 |a Bhat, Pallavi  |e author 
700 1 0 |a Gomes Loureiro, Nuno F  |e author 
700 1 0 |a Uzdensky, Dmitri A.  |e author 
700 1 0 |a Zhou, Muni  |e author 
245 0 0 |a Magnetic island merger as a mechanism for inverse magnetic energy transfer 
260 |b American Physical Society (APS),   |c 2020-03-25T18:14:07Z. 
856 |z Get fulltext  |u https://hdl.handle.net/1721.1/124331 
520 |a Magnetic energy transfer from small to large scales due to successive magnetic island coalescence is investigated. A solvable analytical model is introduced and shown to correctly capture the evolution of the main quantities of interest, as borne out by direct numerical simulations. Magnetic reconnection is identified as the key mechanism enabling the inverse transfer, and setting its properties: Magnetic energy decays as [˜ over t][superscript −1], where [˜ over t] is time normalized to the (appropriately defined) reconnection timescale, and the correlation length of the field grows as [˜ over t][superscript 1/2]. The magnetic energy spectrum is self-similar, and evolves as ∝[˜ over t][superscript −3/2]k[superscript −2,] where the k dependence is imparted by the formation of thin current sheets. 
520 |a National Science Foundation (U.S.) (CAREER Award 1654168) 
520 |a National Science Foundation (U.S.) (Award DE-SC0016215) 
520 |a United States. Department of Energy (Award DE-SC0016215) 
546 |a en 
655 7 |a Article 
773 |t 10.1103/PHYSREVRESEARCH.1.012004 
773 |t Physical Review Research