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相关论文: Plasmoid and Kelvin-Helmholtz instabilities in Swe…

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The scaling of plasmoid instability maximum linear growth rate with respect to Lundquist number $S$ in a Sweet-Parker current sheet, $\gamma_{max}\sim S^{1/4}$, indicates that at high $S$, the current sheet will break apart before it…

等离子体物理 · 物理学 2017-12-01 Yi-Min Huang , Luca Comisso , A. Bhattacharjee

The plasmoid instability has revolutionized our understanding of magnetic reconnection in astrophysical environments. By preventing the formation of highly elongated reconnection layers, it is crucial in enabling the rapid energy conversion…

高能天体物理现象 · 物理学 2017-11-30 Luca Comisso , Manasvi Lingam , Yi-Min Huang , Amitava Bhattacharjee

A detailed numerical study of magnetic reconnection in resistive MHD for very large, previously inaccessible, Lundquist numbers ($10^4\le S\le 10^8$) is reported. Large-aspect-ratio Sweet-Parker current sheets are shown to be unstable to…

太阳与恒星天体物理 · 物理学 2015-05-13 R. Samtaney , N. F. Loureiro , D. A. Uzdensky , A. A. Schekochihin , S. C. Cowley

The plasmoid instability in visco-resistive current sheets is analyzed in both the linear and nonlinear regimes. The linear growth rate and the wavenumber are found to scale as $S^{1/4} {\left( {1 + {P_m}} \right)}^{-5/8}$ and $S^{3/8}…

等离子体物理 · 物理学 2016-04-07 Luca Comisso , Daniela Grasso

Our understanding of magnetic reconnection in resistive magnetohydrodynamics has gone through a fundamental change in recent years. The conventional wisdom is that magnetic reconnection mediated by resistivity is slow in laminar high…

等离子体物理 · 物理学 2013-05-21 Yi-Min Huang , A. Bhattacharjee

It has been established that the Sweet-Parker current layer in high Lundquist number reconnection is unstable to the super-Alfv\'enic plasmoid instability. Past two-dimensional magnetohydrodynamic simulations have demonstrated that the…

等离子体物理 · 物理学 2016-02-17 Yi-Min Huang , A. Bhattacharjee

Current sheets formed in magnetic reconnection events are found to be unstable to high-wavenumber perturbations. The instability is very fast: its maximum growth rate scales as S^{1/4} v_A/L, where L is the length of the sheet, v_A the…

天体物理学 · 物理学 2009-11-13 N. F. Loureiro , A. A. Schekochihin , S. C. Cowley

Magnetic reconnection mediated by the hyper-resistive plasmoid instability is studied with both linear analysis and nonlinear simulations. The linear growth rate is found to scale as $S_{H}^{1/6}$ with respect to the hyper-resistive…

等离子体物理 · 物理学 2014-07-24 Yi-Min Huang , A. Bhattacharjee , Terry G. Forbes

Classical MHD reconnection theories, both the stationary Sweet-Parker model and the tearing instability, are known to provide rates which are too slow to explain the observations. However, a recent analysis has shown that there exists a…

高能天体物理现象 · 物理学 2016-06-22 L. Del Zanna , S. Landi , E. Papini , F. Pucci , M. Velli

We investigate the nonlinear formation of plasmoids in 2D low-beta current sheets through the interplay between the Kelvin-Helmholtz instability (KHI) and the lower-hybrid drift instability (LHDI). Using a hybrid kinetic-gyrokinetic…

等离子体物理 · 物理学 2026-01-21 S. Thatikonda , F. N. De Oliveira-Lopes , A. Mustonen , K. Pommois , D. Told , F. Jenko

We investigate analytically and numerically the semi-collisional regime of the plasmoid instability, defined by the inequality $\delta_{SP} \gg \rho_s \gg \delta_{in}$, where $\delta_{SP}$ is the width of a Sweet-Parker current sheet,…

等离子体物理 · 物理学 2018-12-26 Pallavi Bhat , Nuno Loureiro

The plasmoid instability in evolving current sheets has been widely studied due to its effects on the disruption of current sheets, the formation of plasmoids, and the resultant fast magnetic reconnection. In this Letter, we study the role…

等离子体物理 · 物理学 2018-10-24 Chuanfei Dong , Liang Wang , Yi-Min Huang , Luca Comisso , Amitava Bhattacharjee

We investigate, by means of two-dimensional incompressible magnetohydrodynamic (MHD) numerical simulations, the fast collisional magnetic reconnection regime that is supported by the formation of plasmoid chains when the Lundquist number…

太阳与恒星天体物理 · 物理学 2020-02-12 Hubert Baty

A set of reduced Hall magnetohydrodynamic (MHD) equations are used to evaluate the stability of large aspect ratio current sheets to the formation of plasmoids (secondary islands). Reconnection is driven by resistivity in this analysis,…

等离子体物理 · 物理学 2015-05-30 S. D. Baalrud , A. Bhattacharjee , Y. -M. Huang , K. Germaschewski

We investigate the development of tearing-mode instability using the highest-resolution two-dimensional magnetohydrodynamic simulations of reconnecting current sheets performed on a uniform grid, for Lundquist numbers of $10^3 \le S \le 5…

等离子体物理 · 物理学 2026-05-05 G. H. Vicentin , G. Kowal , E. M. de Gouveia Dal Pino , A. Lazarian

Magnetohydrodynamic simulations have shown that a non-unique critical Lundquist number $S_c$ exists, hovering around $S_c \sim 10^4$, above which threshold Sweet-Parker type stationary reconnecting configurations become unstable to a fast…

等离子体物理 · 物理学 2018-06-06 Chen Shi , Marco Velli , Anna Tenerani

We investigate by means of two-dimensional incompressible magnetohydrodynamic (MHD) numerical simulations, the onset phase of the fast collisional magnetic reconnection regime that is supported by the formation of plasmoid chains when the…

太阳与恒星天体物理 · 物理学 2020-07-21 Hubert Baty

We investigate the Kelvin-Helmholtz instability occuring at the interface of a shear flow configuration in 2D compressible magnetohydrodynamics (MHD). The linear growth and the subsequent non-linear saturation of the instability are studied…

天体物理学 · 物理学 2009-10-31 R. Keppens , G. Toth , R. H. J. Westermann , J. P. Goedbloed

We investigate the nonlinear evolution of the $m = 1$ resistive internal kink mode in a two-dimensional (2D) configuration containing a central region of negative current density, also known as the "current hole" setup. The finite-element…

等离子体物理 · 物理学 2020-10-05 Hubert Baty

We perform simulations of the Kelvin-Helmholtz instability using smoothed particle hydrodynamics (SPH). The instability is studied both in the linear and strongly non-linear regimes. The smooth, well-posed initial conditions of Lecoanet et…

天体物理仪器与方法 · 物理学 2019-08-07 Terrence S. Tricco
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