Magnetic Reconnection as the Driver of the Solar Wind [PDF]
We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of the solar corona.
Nour E. Raouafi +18 more
semanticscholar +1 more source
Black Hole Flares: Ejection of Accreted Magnetic Flux through 3D Plasmoid-mediated Reconnection [PDF]
Magnetic reconnection can power bright, rapid flares originating from the inner magnetosphere of accreting black holes. We conduct extremely high-resolution (5376 × 2304 × 2304 cells) general-relativistic magnetohydrodynamics simulations, capturing ...
B. Ripperda +7 more
semanticscholar +1 more source
Magnetic reconnection in the era of exascale computing and multiscale experiments [PDF]
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 explosively through
H. Ji +5 more
semanticscholar +1 more source
Magnetic Reconnection and Associated Particle Acceleration in High-Energy Astrophysics [PDF]
Magnetic reconnection occurs ubiquitously in the universe and is often invoked to explain fast energy release and particle acceleration in high-energy astrophysics.
F. Guo +3 more
semanticscholar +1 more source
Interchange reconnection as the source of the fast solar wind within coronal holes [PDF]
Measurements of fast solar wind streams from the Parker Solar Probe spacecraft provide strong evidence for the interchange reconnection mechanism being responsible for accelerating the fast solar wind.
S. Bale +15 more
semanticscholar +1 more source
First-principles theory of the rate of magnetic reconnection in magnetospheric and solar plasmas [PDF]
The rate of magnetic reconnection is of the utmost importance in a variety of processes because it controls, for example, the rate energy is released in solar flares, the speed of the Dungey convection cycle in Earth’s magnetosphere, and the energy ...
Yi‐Hsin Liu +5 more
semanticscholar +1 more source
A magnetic reconnection model for hot explosions in the cool atmosphere of the Sun [PDF]
Context. Ultraviolet (UV) bursts and Ellerman bombs (EBs) are transient brightenings observed in the low solar atmospheres of emerging flux regions. Magnetic reconnection is believed to be the main mechanism leading to formation of the two activities ...
Lei Ni +4 more
semanticscholar +1 more source
3D turbulent reconnection: Theory, tests, and astrophysical implications [PDF]
Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in magnetized plasmas. It is associated with energy release in regions of magnetic field annihilation, but this is only one facet of this process. Astrophysical fluid
A. Lazarian +6 more
semanticscholar +1 more source
Magnetic Reconnection and Hot Spot Formation in Black Hole Accretion Disks [PDF]
Hot spots, or plasmoids, which form due to magnetic reconnection in current sheets, are conjectured to power frequent X-ray and near-infrared flares from Sgr A*, the black hole in the center of our Galaxy.
B. Ripperda, F. Bacchini, A. Philippov
semanticscholar +1 more source
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic reconnection. The Magnetospheric Multiscale (MMS) mission has recently enabled the detailed examination of such turbulent current structures in Earth’s ...
J. Stawarz +8 more
semanticscholar +1 more source

