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相关论文: Self-similar solution of fast magnetic reconnectio…

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We present a new model for time evolution of fast magnetic reconnection in free space, which is characterized by self-similarity. Reconnection triggered by locally enhanced resistivity assumed at the center of the current sheet can…

天体物理学 · 物理学 2009-10-31 S. Nitta , S. Tanuma , K. Shibata , K. Maezawa

This paper investigates Magnetic Reynolds number dependence of the ``self-similar evolution model'' (Nitta et al. 2001) of fast magnetic reconnection. I focused my attention on the flow structure inside and around the reconnection outflow,…

天体物理学 · 物理学 2009-11-13 Shin-ya Nitta

In order to understand the nature of magnetic reconnection in ``free space'' which is free from any influence of external circumstances, I have studied the structure of spontaneous reconnection outflow using a shock tube approximation. The…

天体物理学 · 物理学 2009-11-10 Shin-ya Nitta

In this series of papers we examine magnetic reconnection in a domain where the magnetic field does not vanish and the non-ideal region is localised in space. In a previous paper we presented a technique for obtaining analytical solutions…

天体物理学 · 物理学 2015-05-13 A. L. Wilmot-Smith , G. Hornig , E. R. Priest

This paper analytically investigates a series of two-dimensional MHD reconnection solutions over a wide variation of magnetic Reynolds number ($R_{em}^*$). A new series of solutions explains a continuous transition from Petschek-like fast…

天体物理学 · 物理学 2011-02-11 Shin-ya Nitta

The amplification of magnetic fields in a highly conducting fluid is studied numerically. During growth, the magnetic field is spatially intermittent: it does not uniformly fill the volume, but is concentrated in long thin folded…

混沌动力学 · 物理学 2009-11-10 A. A. Schekochihin , S. C. Cowley , J. L. Maron , J. C. McWilliams

We present a constructive numerical example of fast magnetic reconnection in a three dimensional periodic box. Reconnection is initiated by a strong, localized perturbation to the field lines. The solution is intrinsically three…

等离子体物理 · 物理学 2015-05-18 Bijia Pang , Ue-Li Pen , Ethan T. Vishniac

Fast magnetic reconnection is defined by the topology of the magnetic field lines changing on a timescale that is approximately an order of magnitude longer than the topology-conserving ideal-evolution timescale. Fast reconnection is an…

等离子体物理 · 物理学 2022-05-18 Allen H Boozer

We investigate the large scale evolution of a relativistic magnetic reconnection in an electron-positron pair plasma by a relativistic two-fluid magnetohydrodynamic (MHD) code. We introduce an inter-species friction force as an effective…

高能天体物理现象 · 物理学 2014-11-18 Seiji Zenitani , Michael Hesse , Alex Klimas

We propose an extension of the semi-analytical solutions derived by Lin et al. (1965) describing the two-dimensional homologous collapse of a self-gravitating rotating cloud having uniform density and spheroidal shape, which includes…

天体物理学 · 物理学 2009-11-10 P. Hennebelle

This work presents a 2.5-dimensional simulation study of the instability of current-sheets located in a medium with a strong density variation along the current layer. The initial force-free configuration is observed to undergo a two-stage…

太阳与恒星天体物理 · 物理学 2015-05-13 Lapo Bettarini , Giovanni Lapenta

The fast rates of magnetic reconnection found in both nature and experiments are important to understand theoretically. Recently, it was demonstrated that two-fluid magnetic reconnection remains fast in the strong guide field regime,…

等离子体物理 · 物理学 2015-05-20 A. Stanier , Andrei N. Simakov , L. Chacon , W. Daughton

The efficiency of energy conversion during magnetic reconnection is related to the reconnection rate. While the stable reconnection rate has been studied extensively, its growth between the time of reconnection onset and the peak…

等离子体物理 · 物理学 2022-08-19 D. S. Payne , R. B. Torbert , K. Germaschewski , T. G. Forbes , J. R. Shuster

To systematically stress a rotationally symmetric 3D magnetic null point by advecting the opposite footpoints of the spine axis in opposite directions. This stress eventually concentrates in the vicinity of the null point forming a local…

太阳与恒星天体物理 · 物理学 2015-05-27 K. Galsgaard , D. I. Pontin

Self-organization in continuous systems is associated with dissipative processes. In particular, for magnetized plasmas, it is known as magnetic relaxation, where the magnetic energy is converted into heat and kinetic energy of flow through…

太阳与恒星天体物理 · 物理学 2024-01-23 Satyam Agarwal , Ramit Bhattacharyya , Shangbin Yang

In this paper, we investigate a simple model where two, initially unconnected, flux systems are forced to interact in response to the imposed boundary driving by solving the non-ideal 3D MHD equations numerically. The reconnection rate of…

天体物理学 · 物理学 2007-05-23 K. Galsgaard , C. Parnell

The magnetic flux penetration into the half-space superconductor sample is studied in the flux flow regime in parallel geometry assuming that an external magnetic field increasing with time in accordance with the power law. Assuming that…

超导电性 · 物理学 2015-03-13 N. A. Taylanov

The growth of confined magnetic films with ferromagnetic interactions between nearest-neighbor spins is studied in a stripped $(1+1)-$dimensional rectangular geometry. Magnetic films are grown irreversibly by adding spins at the boundaries…

统计力学 · 物理学 2007-05-23 Julián Candia , Ezequiel V. Albano

Using the in-viscid two-field reduced MHD model, a new analytical theory is developed to unify the Hahm-Kulsrud-Taylor (HKT) linear solution and the Rutherford quasi-linear regime. Adopting a quasi-linear approach, we obtain a closed system…

等离子体物理 · 物理学 2021-05-26 Wenlong Huang , Ping Zhu

The spontaneous evolution of magnetic reconnection in generalized situations (with thermodynamic asymmetry regarding the current sheet and magnetic shear) is investigated using two-dimensional magnetohydrodynamic simulation. We focus on the…

太阳与恒星天体物理 · 物理学 2022-09-14 Shin-ya Nitta , Koji Kondoh
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