Fast Magnetic Reconnection: "Ideal" Tearing and the Hall Effect
TL;DR: In this article, the authors show how the "ideal" tearing mode critical aspect ratio is modified when Hall effects are taken into account, including more general scaling laws of the growth rates in terms of sheet inverse aspect ratio, and discuss the implications of this generalized triggering aspect ratio for recently developed phase diagrams of magnetic reconnection.
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Abstract: One of the main questions in magnetic reconnection is the origin of triggering behavior with on/off properties that accounts, once it is activated, for the fast magnetic energy conversion to kinetic and thermal energies at the heart of explosive events in astrophysical and laboratory plasmas. Over the past decade progress has been made on the initiation of fast reconnection via the plasmoid instability and what has been called "ideal" tearing, which sets in once current sheets thin to a critical inverse aspect ratio $(a/L)_c$: as shown by Pucci and Velli (2014), at $(a/L)_c \sim S^{-1/3}$ the time scale for the instability to develop becomes of the order of the Alfven time and independent of the Lundquist number (here defined in terms of current sheet length $L$). However, given the large values of $S$ in natural plasmas, this transition might occur for thicknesses of the inner resistive singular layer which are comparable to the ion inertial length $d_i$. When this occurs, Hall currents produce a three-dimensional quadrupole structure of magnetic field, and the dispersive waves introduced by the Hall effect accelerate the instability. Here we present a linear study showing how the "ideal" tearing mode critical aspect ratio is modified when Hall effects are taken into account, including more general scaling laws of the growth rates in terms of sheet inverse aspect ratio: the critical inverse aspect ratio is amended to $a/L \simeq (di/L)^ {0.29} (1/S)^{0.19}$, at which point the instability growth rate becomes Alfvenic and does not depend on either of the (small) parameters $d_i/L, 1/S$. We discuss the implications of this generalized triggering aspect ratio for recently developed phase diagrams of magnetic reconnection.
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Citations
Explosive Magnetotail Activity
M. I. Sitnov,Joachim Birn,B. Ferdousi,Evgeny Gordeev,Yuri V. Khotyaintsev,Viacheslav Merkin,Tetsuo Motoba,Antonius Otto,Evgeny V. Panov,P. L. Pritchett,Fulvia Pucci,Fulvia Pucci,Joachim Raeder,Andrei Runov,V. A. Sergeev,Marco Velli,Xu-Zhi Zhou +16 more
TL;DR: Two mechanisms for the generation of the pre-onset current sheet are discussed, namely magnetic flux addition to the tail lobes, or other high-latitude perturbations, and magnetic flux evacuation from the near-Earth tail associated with dayside reconnection.
Magnetic reconnection in the era of exascale computing and multiscale experiments
TL;DR: In this paper , the authors predict that magnetic reconnection explosively releases stored magnetic energy in astrophysical plasmas, which produces a reconfiguration of the magnetic field, along with high-speed flows, thermal heating and nonthermal particle acceleration.
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Influence of 3D plasmoid dynamics on the transition from collisional to kinetic reconnection
TL;DR: In this paper, a first-principles kinetic simulation with a Fokker-Planck collision operator in 3D was performed, showing that the high-Lundquist number reconnection layers are unstable to the plasmoid instability, leading to a turbulent evolution where the reconnection rate can be independent of the underlying resistivity.
34
•Journal Article
Plasmoid Instability in Forming Current Sheets
Influence of 3D plasmoid dynamics on the transition from collisional to kinetic reconnection
TL;DR: In this paper, the authors used a first-principles kinetic simulation with a Fokker-Planck collision operator in 3D and showed that the high-Lundquist number reconnection layers are unstable to the plasmoid instability, leading to a turbulent evolution where the reconnection rate can be independent of the underlying resistivity.
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Instability of current sheets and formation of plasmoid chains
TL;DR: In this article, current sheets formed in magnetic reconnection events are found to be unstable to high-wavenumber perturbations, and a chain of plasmoid secondary islands is formed, whose number scales as S3∕8.
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Electromagnetic Energy Conversion at Reconnection Fronts
TL;DR: In this paper, the authors used a conjunction between eight spacecraft to show that magnetic energy conversion takes place within fronts of recently reconnected magnetic flux, predominantly at 1-to 10-electron inertial length scale, intense electrical current sheets (tens to hundreds of nanoamperes per square meter).
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Reconnection of Quasi-singular Current Sheets: The "Ideal" Tearing Mode
TL;DR: In this paper, it was shown that the Sweet-Parker current sheet is unstable to a reconnecting instability which grows without bound as the Lundquist number, S tends to infinity, and that an ideal tearing mode takes over before current sheets reach such a thickness.
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