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Title: Multi-scale structures of turbulent magnetic reconnection

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4951025· OSTI ID:22600077
; ; ;  [1];  [2]
  1. Space Research Institute, Austrian Academy of Sciences, Graz 8042 (Austria)
  2. Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

We have analyzed data from a series of 3D fully kinetic simulations of turbulent magnetic reconnection with a guide field. A new concept of the guide filed reconnection process has recently been proposed, in which the secondary tearing instability and the resulting formation of oblique, small scale flux ropes largely disturb the structure of the primary reconnection layer and lead to 3D turbulent features [W. Daughton et al., Nat. Phys. 7, 539 (2011)]. In this paper, we further investigate the multi-scale physics in this turbulent, guide field reconnection process by introducing a wave number band-pass filter (k-BPF) technique in which modes for the small scale (less than ion scale) fluctuations and the background large scale (more than ion scale) variations are separately reconstructed from the wave number domain to the spatial domain in the inverse Fourier transform process. Combining with the Fourier based analyses in the wave number domain, we successfully identify spatial and temporal development of the multi-scale structures in the turbulent reconnection process. When considering a strong guide field, the small scale tearing mode and the resulting flux ropes develop over a specific range of oblique angles mainly along the edge of the primary ion scale flux ropes and reconnection separatrix. The rapid merging of these small scale modes leads to a smooth energy spectrum connecting ion and electron scales. When the guide field is sufficiently weak, the background current sheet is strongly kinked and oblique angles for the small scale modes are widely scattered at the kinked regions. Similar approaches handling both the wave number and spatial domains will be applicable to the data from multipoint, high-resolution spacecraft observations such as the NASA magnetospheric multiscale (MMS) mission.

OSTI ID:
22600077
Journal Information:
Physics of Plasmas, Vol. 23, Issue 5; Other Information: (c) 2016 Author(s); Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
Country of Publication:
United States
Language:
English

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Explosive Magnetotail Activity journal May 2019
Observational Evidence of Large-Scale Multiple Reconnection at the Earth's Dayside Magnetopause journal October 2018
Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail journal November 2018
Oblique Ion-Scale Magnetotail Flux Ropes Generated by Secondary Tearing Modes journal October 2018
MMS Multi‐Point Analysis of FTE Evolution: Physical Characteristics and Dynamics journal July 2019
A Statistical Study of the Force Balance and Structure in the Flux Ropes in Mercury's Magnetotail journal July 2019
MMS Study of the Structure of Ion‐Scale Flux Ropes in the Earth's Cross‐Tail Current Sheet journal June 2019
Electron‐Scale Magnetic Structure Observed Adjacent to an Electron Diffusion Region at the Dayside Magnetopause journal December 2019
Magnetic Reconnection in Three Dimensions: Modeling and Analysis of Electromagnetic Drift Waves in the Adjacent Current Sheet journal December 2019
Diffusion regions and 3D energy mode development in spontaneous reconnection journal July 2019
Diffusion regions and 3D energy mode development in spontaneous reconnection text January 2019
Turbulent mass transfer caused by vortex induced reconnection in collisionless magnetospheric plasmas journal November 2017