Fast Cross-Scale Energy Transfer During Turbulent Magnetic Reconnection

被引:9
|
作者
Nakamura, T. K. M. [1 ,2 ]
Hasegawa, H. [3 ]
Genestreti, K. J. [4 ]
Denton, R. E. [5 ]
Phan, T. D. [6 ]
Stawarz, J. E. [7 ]
Nakamura, R. [2 ]
Nystrom, W. D. [8 ]
机构
[1] Karl Franzens Univ Graz, Inst Phys, Graz, Austria
[2] Austrian Acad Sci, Space Res Inst, Graz, Austria
[3] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan
[4] Southwest Res Inst, Durham, NH USA
[5] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[6] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[7] Imperial Coll London, Dept Phys, London, England
[8] Los Alamos Natl Lab, Los Alamos, NM USA
关键词
Diffusion region; energy transfer; kinetic simulation; magnetic island; reconnection; turbulence; EARTHS PLASMA SHEET;
D O I
10.1029/2021GL093524
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Magnetic reconnection is a key fundamental process in collisionless plasmas that explosively converts magnetic energy to plasma kinetic and thermal energies through a change of magnetic field topology in a central electron-scale region called the electron diffusion region (EDR). Past simulations and observations demonstrated that this process causes efficient energy conversion through the formation of multiple macro-scale or micro-scale magnetic islands/flux ropes. However, the coupling of these phenomena on different spatiotemporal scales is still poorly understood. Here, based on a new large-scale fully kinetic simulation with a realistic, initially fluctuating magnetic field, we demonstrate that macro-scale evolution of turbulent reconnection involving merging of macro-scale islands induces repeated, quick formation of new electron-scale islands within the EDR which soon grow to larger scales. This process causes an efficient cross-scale energy transfer from electron- to larger-scales, and leads to strong electron energization within the growing islands.
引用
收藏
页数:8
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