activity
20032022
most citedWhy does steady-state magnetic reconnection have a maximum local rate of order 0.1?

186 citations · 269 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2022★ 1 cited

Multi-species Ion Acceleration in 3D Magnetic Reconnection with Hybrid-kinetic Simulations

Qile Zhang, Fan Guo, William Daughton +4

Magnetic reconnection drives multi-species particle acceleration broadly in space and astrophysics. We perform the first 3D hybrid simulations (fluid electrons, kinetic ions) that…

physics.plasm-ph2017★ 8 cited

Collisionless Kinetic Theory of Oblique Tearing Instabilities

Scott D. Baalrud, Amitava Bhattacharjee, William Daughton

The linear dispersion relation for collisionless kinetic tearing instabilities is calculated for a Harris equilibrium. In contrast to the conventional 2D geometry, which considers…

physics.plasm-ph2016★ 186 cited

Why does steady-state magnetic reconnection have a maximum local rate of order 0.1?

Yi-Hsin Liu, M. Hesse, F. Guo +4

Simulations suggest collisionless steady-state magnetic reconnection of Harris-type current sheets proceeds with a rate of order 0.1, independent of dissipation mechanism. We argue…

physics.plasm-ph2004★ 74 cited

Influence of the Lower Hybrid Drift Instability on the onset of Magnetic Reconnection

Paolo Ricci, J. U. Brackbill, W. Daughton +1

Two-dimensional and three-dimensional kinetic simulation results reveal the importance of the Lower-Hybrid Drift Instability LHDI to the onset of magnetic reconnection. Both explic…

astro-ph2003

Kinetic simulations of collisionless magnetic reconnection in presence of a guide field

P. Ricci, J. U. Brackbill, W. Daughton +1

The results of kinetic simulations of magnetic reconnection in Harris current sheets are analyzed. A range of guide fields is considered to study reconnection in plasmas characteri…