搜索结果: 1-8 共查到“天体物理学 Reconnection”相关记录8条 . 查询时间(0.066 秒)
Theory of magnetic reconnection in solar and astrophysical plasmas
Theory magnetic reconnection solar astrophysical plasmas
2012/2/23
Magnetic reconnection is a fundamental process in a plasma that facilitates the release of energy stored in the magnetic field by permitting a change in the magnetic topology. In this article we prese...
Particle Acceleration by Magnetic Reconnection in AGNs and in the IGM
Particle Acceleration Magnetic Reconnection AGNs IGM
2011/10/9
There is no single mechanism by which fast particles are accelerated in astrophysical environments, and it is now recognized that the data require a rich variety of different mechanisms operating unde...
A Generalized Flux Function for Three-dimensional Magnetic Reconnection
Generalized Flux Function Three-dimensional Magnetic Reconnection
2011/10/18
The definition and measurement of magnetic reconnection in three-dimensional magnetic fields with multiple reconnection sites is a challenging problem, particularly in fields lacking null points. We p...
The Internal-Collision-Induced Magnetic Reconnection and Turbulence (ICMART) Model of Gamma-Ray Bursts
gamma-rays burst general gamma-ray bursts individual GRB 080916C magnetic reconnection turbulence
2010/11/11
The recent Fermi observation of GRB 080916C shows that the bright photosphere emission associated with a putative fireball is missing, which suggests that the central engine likely launches a Poynting...
A Reconnection Switch to Trigger Gamma-Ray Burst Jet Dissipation
accretion discs black hole physics galaxies jets gamma rays bursts MHD
2010/11/12
Prompt gamma-ray burst (GRB) emission requires some mechanism to dissipate an ultrarelativistic
jet. Internal shocks or some form of electromagnetic dissipation are candidate mechanisms.
New Insights into Dissipation in the Electron Layer During Magnetic Reconnection
New Insights Magnetic Reconnection Electron Layer
2010/3/8
Detailed comparisons are reported between laboratory observations of electron-scale dissipation layers near a reconnecting X-line and direct two-dimensional full-particle simulations. Many experimenta...
Ultra-high-energy cosmic ray acceleration by magnetic reconnection in newborn pulsars
newborn pulsars cosmic ray magnetic reconnection
2009/6/4
Ultra-high-energy cosmic ray acceleration by magnetic reconnection in newborn pulsars。
Fast reconnection of magnetic fields in turbulent fluids。