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相关论文: Evolution of the Relativistic Plasmoid-Chain in th…

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In this paper, the temporal evolution of 3-dimensional relativistic current sheets in Poynting-dominated plasma is studied for the first time. Over the past few decades, a lot of efforts have been conducted on studying the evolution of…

高能天体物理现象 · 物理学 2018-03-14 Makoto Takamoto

The dynamics of a plasmoid chain is studied with three dimensional Particle-in-Cell simulations. The evolution of the system with and without a uniform guide field, whose strength is 1/3 the asymptotic magnetic field, is investigated. The…

等离子体物理 · 物理学 2015-06-16 Stefano Markidis , Pierre Henri , Giovanni Lapenta , Andrey Divin , Martin Goldman , David Newman , Erwin Laure

The formation of plasmoid chains is explored for the first time within the context of the Taylor problem, in which magnetic reconnection is driven by a small amplitude boundary perturbation in a tearing-stable slab plasma equilibrium.…

等离子体物理 · 物理学 2015-02-20 Luca Comisso , Daniela Grasso , François L. Waelbroeck

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

A conceptual model of resistive magnetic reconnection via a stochastic plasmoid chain is proposed. The global reconnection rate is shown to be independent of the Lundquist number. The distribution of fluxes in the plasmoids is shown to be…

太阳与恒星天体物理 · 物理学 2015-05-19 D. A. Uzdensky , N. F. Loureiro , A. A. Schekochihin

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

Plasmoids, quasi-spherical regions of plasma containing magnetic fields and high-energy particles, are a self-consistent by-product of the reconnection process in the relativistic regime. Recent two-dimensional particle-in-cell (PIC)…

高能天体物理现象 · 物理学 2018-01-24 M. Petropoulou , I. M. Christie , L. Sironi , D. Giannios

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

While relativistic magnetic reconnection in pair plasmas has emerged in recent years as a candidate for the origin of radiation from extreme astrophysical environments, the corresponding subrelativistic pair plasma regime has remained less…

等离子体物理 · 物理学 2025-12-16 Adam Robbins , Anatoly Spitkovsky

A numerical study of magnetic reconnection in the large-Lundquist-number ($S$), plasmoid-dominated regime is carried out for $S$ up to $10^7$. The theoretical model of Uzdensky {\it et al.} [Phys. Rev. Lett. {\bf 105}, 235002 (2010)] is…

太阳与恒星天体物理 · 物理学 2015-05-30 N. F. Loureiro , R. Samtaney , A. A. Schekochihin , D. A. Uzdensky

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

In flare-relevant current sheets, tearing instability may trigger explosive reconnection and plasmoid formation. We explore how the thermal and tearing modes reinforce each other in the fragmentation of a current sheet in the solar corona…

太阳与恒星天体物理 · 物理学 2022-10-05 Samrat Sen , Rony Keppens

For realistic values of Lundquist number in tokamak plasmas, the 1/1 magnetic island leads to the formation of secondary thin current sheet, which breaks up into a chain of small magnetic islands, called plasmoids. The role of plasmoid…

等离子体物理 · 物理学 2019-06-26 A. Ali , P. Zhu

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

Magnetic reconnection is a ubiquitous phenomenon for magnetized plasmas and leads to the rapid reconfiguration of magnetic field lines. During reconnection events, plasma is heated and accelerated until the magnetic field lines enclose and…

高能天体物理现象 · 物理学 2023-11-15 Jesse Vos , Hector Olivares , Benoit Cerutti , Monika Moscibrodzka

A fundamental problem of forced magnetic reconnection has been solved taking into account the plasmoid instability of thin reconnecting current sheets. In this problem, the reconnection is driven by a small amplitude boundary perturbation…

等离子体物理 · 物理学 2015-04-22 Luca Comisso , Daniela Grasso , François L. Waelbroeck

Tearing instability, also known as plasmoid instability, is an effective mechanism to speed up magnetic reconnection process, working in a wide range of magnetized plasma systems with different spatial scales, ionization degrees, and…

太阳与恒星天体物理 · 物理学 2026-02-24 Zehao Tang

We study the compression driven magnetic reconnection in the relativistic electron-positron plasma. Making use of a 2.5D particle-in-cell code, we simulated compression of a magnetized plasma layer containing a current sheet within it. We…

天体物理学 · 物理学 2009-11-13 Yuri Lyubarsky , Michael Liverts

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
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