Suprathermal electron acceleration in magnetic reconnection

By Masahiro Hoshino, T. Mukai, T. Terasawa, I. Shinohara. 2001

322 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/74a58f937ef6a8431fe2842058edfd346a3ed637

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Zenitani
2. Masahiro Hoshino
3. M. Swisdak
4. James Drake
5. Merav Opher
6. Y. Khotyaintsev
7. H. Fu
8. J. Eastwood

In Nuclear and High Energy Physics

1. S. Zenitani
2. Masahiro Hoshino
3. M. Swisdak
4. J. Eastwood
5. Andrey Divin
6. James Drake
7. J. Birn
8. L. Zelenyi

Citations in the corpus

• THE VECTOR DIRECTION OF THE INTERSTELLAR MAGNETIC FIELD OUTSIDE THE HELIOSPHERE (2010, background): “Second, observations and simulations have demonstrated that reconnection can produce both beams of electrons traveling at the electron Alfvén speed (Cattell et al. 2005) and more isotropic populations at relativistic energies (Øieroset et al. 2002; Hoshino et al. 2001; Drake et al. 2006).”
• Particle Acceleration and Magnetic Dissipation in Relativistic Current Sheet of Pair Plasmas (2007, background): “In the geophysical ion-electron contexts, Birn et al. (1997) studied ion acceleration and Hoshino et al. (2001) studied electron acceleration in the magnetic dipole/pileup regions.”
• Dipolarization fronts as a signature of transient reconnection in the magnetotail (2009, methodology): “The main difference between our force-balanced X-line pattern and earlier simulations with the reconnection initiated by the electron tearing mode [ Hoshino et al., 1998, 2001 ] is that the stronger Bzfield in our case allows one to investigate new reconnection regimes with magnetized electrons.”
• ELECTRON ACCELERATION BY MULTI-ISLAND COALESCENCE (2010, background): “…Laboratory, University of California Berkeley 2 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency energization (e.g. Hoshino et al. 2001; Hoshino 2005; Drake et al. 2005; Pritchett 2006; Drake et al. 2006; Karlický & Bárta 2007; Pritchett 2008; Wan et al. 2008;…”
• Intermittent energy dissipation by turbulent reconnection (2017, background): “During reconnection, the magnetic field lines “break” and “reconnect”, and a large amount of energy are released in terms of hard X-rays on the Sun [Masuda et al., 1994] and energetic electrons in the magnetotail [Hoshino et al., 2001; Imada et al., 2007; Huang et al., 2012; Fu et al., 2013].”
• Particle Acceleration in the Magnetotail and Aurora (2012, methodology): “…order to understand the particle acceleration in reconnection, the nonlinear time evolution of a thin current sheet has been studied by many different research groups (e.g., Hoshino et al. 2001; Drake et al. 2003; Pritchett 2008; Oka et al. 2010) using particle-in-cell (PIC) simulations.”