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相关论文: Topological Constraints on the Relaxation of Compl…

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Magnetic field relaxation is determined by both the field's geometry and its topology. For relaxation processes, however, it turns out that its topology is a much more stringent constraint. As quantifier for the topology we use magnetic…

太阳与恒星天体物理 · 物理学 2013-11-18 Simon Candelaresi , Axel Brandenburg

Stability and reconnection of magnetic fields play a fundamental role in natural and man-made plasma. In these applications the field's topology determines the stability of the magnetic field. Here I will describe the importance of one…

太阳与恒星天体物理 · 物理学 2015-06-15 Simon Candelaresi

The energy of the stochastic magnetic field is bounded from below by a topological quantity expressing the degree of linkage of the field lines. When the bound is saturated one can assume that the storage of a certain magnetic energy…

等离子体物理 · 物理学 2007-05-23 F. Spineanu , M. Vlad

Magnetic helicity is an invariant of ideal magnetohydrodynamics (MHD) that encodes information on the topology of magnetic field lines. It has long been appreciated that magnetic topology is an important constraint for the evolution of…

太阳与恒星天体物理 · 物理学 2020-09-25 David MacTaggart , Chris Prior

Magnetic helicity is a conserved quantity of ideal magnetohydrodynamics (MHD) that is related to the topology of the magnetic field, and is widely studied in both laboratory and astrophysical plasmas. When the magnetic field has a…

等离子体物理 · 物理学 2023-07-28 David MacTaggart , Alberto Valli

Astrophysical objects with negligible resistivity are often threaded by large scale magnetic fields. The generation of these fields is somewhat mysterious, since a magnetic field in a perfectly conducting fluid cannot change the flux…

天体物理学 · 物理学 2007-05-23 E. T. Vishniac , A. Lazarian , J. Cho

We study the evolution of turbulent magnetic fields from a topological point of view, invoking commonplace mathematical tools from general topology and dynamical systems theory which connect magnetic field evolution to time reversal…

高能天体物理现象 · 物理学 2021-01-12 Amir Jafari , Ethan Vishniac

We investigate the evolution of field line helicity for magnetic fields that connect two boundaries without null points, with emphasis on localized finite-B magnetic reconnection. Total (relative) magnetic helicity is already recognized as…

等离子体物理 · 物理学 2015-03-11 Alexander J. B. Russell , Anthony R. Yeates , Gunnar Hornig , Antonia L. Wilmot-Smith

Magnetic helicity is conserved under ideal magnetohydrodynamics (MHD) and quasi-conserved even under a resistive process. The standard definition for magnetic helicity cannot be applied directly to an open magnetic field in a volume,…

太阳与恒星天体物理 · 物理学 2020-05-27 Kai E. Yang , Michael S. Wheatland , Stuart A. Gilchrist

Magnetic helicity is a quantity that underpins many theories of magnetic relaxation in electrically conducting fluids, both laminar and turbulent. Although much theoretical effort has been expended on magnetic fields that are everywhere…

等离子体物理 · 物理学 2025-04-18 Sauli Lindberg , David MacTaggart

A topological constraint on the dynamics of a magnetic field in a flux tube arises from the fixed point indices of its field line mapping. This can explain unexpected behaviour in recent resistive-magnetohydrodynamic simulations of magnetic…

等离子体物理 · 物理学 2015-03-19 A. R. Yeates , G. Hornig

The dual symmetry between the electric and magnetic fields underlies Maxwell's electrodynamics. Due to this symmetry one can describe topological properties of an electromagnetic field in free space and obtain the conservation law of…

光学 · 物理学 2015-12-31 E. O. Kamenetskii , M. Berezin , R. Shavit

The final state of turbulent magnetic relaxation in a reversed field pinch is well explained by Taylor's hypothesis. However, recent resistive-magnetohydrodynamic simulations of the relaxation of braided solar coronal loops have led to…

太阳与恒星天体物理 · 物理学 2015-05-19 A. R. Yeates , G. Hornig , A. L. Wilmot-Smith

Magnetic reconnection is a complex mechanism that converts magnetic energy into particle kinetic energy and plasma thermal energy in space and astrophysical plasmas. In addition, magnetic reconnection and turbulence appear to be intimately…

等离子体物理 · 物理学 2021-12-22 Rodrigo A. Miranda , Juan A. Valdivia , Abraham C. -L. Chian , Pablo R. Muñoz

Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which inevitably gives rise to the accumulation of magnetic energy within stressed regions including current sheets. This stored energy is often released…

等离子体物理 · 物理学 2022-02-21 Hantao Ji , William Daughton , Jonathan Jara-Almonte , Ari Le , Adam Stanier , Jongsoo Yoo

Magnetic helicity is a fundamental quantity of magnetohydrodynamics that carries topological information about the magnetic field. By `topological information', we usually refer to the linkage of magnetic field lines. For domains that are…

等离子体物理 · 物理学 2019-09-25 David MacTaggart , Alberto Valli

Twisted magnetic flux ropes are reservoirs of free magnetic energy. In a highly-conducting plasma such as the solar corona, energy release through multiple magnetic reconnections can be modelled as a helicity-conserving relaxation to a…

太阳与恒星天体物理 · 物理学 2023-08-17 Philippa Browning , Mykola Gordovskyy , Alan Hood

We study the relaxation of a topologically non-trivial vortex braid with zero net helicity in a barotropic fluid. The aim is to investigate the extent to which the topology of the vorticity field -- characterized by braided vorticity field…

流体动力学 · 物理学 2021-05-05 Simon Candelaresi , Gunnar Hornig , Benjamin Podger , David Ian Pontin

We revisit the issue of conservation of magnetic helicity and the Woltjer-Taylor relaxation theory in magnetohydrodynamics in the context of weak solutions. We introduce a relaxed system for the ideal MHD system, which decouples the effects…

偏微分方程分析 · 数学 2021-09-21 Daniel Faraco , Sauli Lindberg , László Székelyhidi

Through a direct comparison between numerical simulations in two and three dimensions, we investigate topological effects in reconnection. A simple estimate on increase in reconnection rate in three dimensions by a factor of $\sqrt{2}$,…

太阳与恒星天体物理 · 物理学 2015-06-19 Miljenko Čemeljić , Ruei-Yang Huang
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