Role of electron physics in the development of turbulent magnetic reconnection in collisionless plasmas

By William S. Daughton, V. Roytershteyn, Homa Karimabadi, L. Yin, B. Albright, B. Bergen, K. Bowers. 2011

545 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a4951abd82770ec36918a83aa238dfa6802fecaa

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. L. Sironi
2. L. Comisso
3. A. Spitkovsky
4. D. Giannios
5. M. Petropoulou
6. J. Arons
7. A. Beloborodov
8. U. Keshet

In Nuclear and High Energy Physics

1. L. Sironi
2. L. Comisso
3. A. Spitkovsky
4. D. Giannios
5. M. Petropoulou
6. J. Arons
7. A. Beloborodov
8. U. Keshet

Citations in the corpus

• The Interplay of Magnetically Dominated Turbulence and Magnetic Reconnection in Producing Nonthermal Particles (2019, background): “4), as highly elongated layers cannot be stable against the plasmoid instability, also in 3D geometry (e.g. Daughton et al. 2011; Sironi & Spitkovsky 2014; Guo et al. 2015; Huang & Bhattacharjee 2016; Ebrahimi 2017; Werner & Uzdensky 2017; Baalrud et al. 2018; Stanier et al. 2019).”
• PARTICLE ACCELERATION AND PLASMA DYNAMICS DURING MAGNETIC RECONNECTION IN THE MAGNETICALLY DOMINATED REGIME (2015, unknown): “…and compared with 2D simulations in a number of non-relativistic studies (Liu et al. 2013; Daughton et al. 2014), which showed only modest differences between 2D and 3D simulations although strong 3D effects emerge as the tearing mode develops over a range of oblique angles (Daughton et al. 2011).”