Magnetic Reconnection in Astrophysical and

By E. Zweibel, M. Yamada. 2009

496 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/7c705dea7d4ec8b3a5ddfc42823bd54a9c21c465

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In Astronomy and Astrophysics

Citations in the corpus

Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers (2010, unknown): “dtd" [ ]> Magnetic reconnection is a process by which oppositely directed magnetic field lines passing through a plasma undergo dramatic rearrangement, converting magnetic potential into kinetic energy and hea”
Three-dimensional magnetic reconnection regimes: a review (2011, background): “onnection in 3D. This review is by necessity limited and misses a number of important facets of reconnection research. Complementary reviews include those by Priest and Forbes (2000); Biskamp (2000); Zweibel and Yamada (2009); Yamada et al. (2010). In Section 2 we introduce some key measures and fea”
Magnetic Fields in Galaxies (2010, background): “Classical reconnection rates in the interstellar medium are very low, but a number of mechanisms have been proposed to accelerate the reconnection rate (Zweibel & Yamada 2009).”
The physics of gamma-ray bursts & relativistic jets (2014, background): “[651–655,650,656,657,387,658,659]) — see [660] for a more complete discussion of the extensive literature.”
Non-thermal particle acceleration in collisionless relativistic electron-proton reconnection (2016, background): “Magnetic reconnection is a basic plasma process often leading to the violent release of magnetic energy through rapid rear- rangement of magnetic field geometry (e.g., Biskamp 2005; Zweibel & Yamada 2009; Yamada et al. 2010).”
A Reconnection Switch to Trigger gamma-Ray Burst Jet Dissipation (2010, background): “[For a review, see Kirk, Melrose & Priest (1994), Kulsrud (2005) and Zweibel & Yamada (2009).]”
The Astrophysics of Ultrahigh-Energy Cosmic Rays (2011, background): “In a plasma, a local reconfiguration of the magnetic field topology (or reconnection) happens when the plasma conductivity is not high enough to support the current associated with a magnetic field structure (see Zweibel & Yamada 2009 for a review).”