Magnetic reconnection in the era of exascale computing and multiscale experiments
Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which
inevitably gives rise to the accumulation of magnetic energy within stressed regions …
inevitably gives rise to the accumulation of magnetic energy within stressed regions …
Magnetic reconnection
The fundamental physics of magnetic reconnection in laboratory and space plasmas is
reviewed by discussing results from theory, numerical simulations, observations from space …
reviewed by discussing results from theory, numerical simulations, observations from space …
The PLUTO code for adaptive mesh computations in astrophysical fluid dynamics
A Mignone, C Zanni, P Tzeferacos… - The Astrophysical …, 2011 - iopscience.iop.org
We present a description of the adaptive mesh refinement (AMR) implementation of the
PLUTO code for solving the equations of classical and special relativistic …
PLUTO code for solving the equations of classical and special relativistic …
[BOOK][B] Plasma physics: an introduction
R Fitzpatrick - 2022 - taylorfrancis.com
Encompasses the Lectured Works of a Renowned Expert in the Field Plasma Physics: An
Introduction is based on a series of university course lectures by a leading name in the field …
Introduction is based on a series of university course lectures by a leading name in the field …
Magnetic reconnection in astrophysical and laboratory plasmas
EG Zweibel, M Yamada - Annual review of astronomy and …, 2009 - annualreviews.org
Magnetic reconnection is a topological rearrangement of magnetic field that converts
magnetic energy to plasma energy. Astrophysical flares, from the Earth's magnetosphere to …
magnetic energy to plasma energy. Astrophysical flares, from the Earth's magnetosphere to …
The inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence
A Brandenburg - The Astrophysical Journal, 2001 - iopscience.iop.org
A numerical model of isotropic homogeneous turbulence with helical forcing is investigated.
The resulting flow, which is essentially the prototype of the α 2 dynamo of mean field …
The resulting flow, which is essentially the prototype of the α 2 dynamo of mean field …
Phase diagram for magnetic reconnection in heliophysical, astrophysical, and laboratory plasmas
H Ji, W Daughton - Physics of Plasmas, 2011 - pubs.aip.org
Recent progress in understanding the physics of magnetic reconnection is conveniently
summarized in terms of a phase diagram which organizes the essential dynamics for a wide …
summarized in terms of a phase diagram which organizes the essential dynamics for a wide …
Magnetic reconnection and plasma dynamics in two-beam laser-solid interactions
We present measurements of a magnetic reconnection in a plasma created by two laser
beams (1 ns pulse duration, 1× 10 15 W cm-2) focused in close proximity on a planar solid …
beams (1 ns pulse duration, 1× 10 15 W cm-2) focused in close proximity on a planar solid …
MHD turbulence: a biased review
AA Schekochihin - Journal of Plasma Physics, 2022 - cambridge.org
This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …
developments of the last few years in the context of the canonical time line (from Kolmogorov …
A review of the 0.1 reconnection rate problem
A long-standing problem in magnetic reconnection is to explain why it tends to proceed at or
below a normalized rate of 0.1. This article gives a review of observational and numerical …
below a normalized rate of 0.1. This article gives a review of observational and numerical …