activity
19982026
most citedTwo-scale structure of the electron dissipation region during collisionless magnetic reconnection

321 citations · 4.7k across the 94 of their papers we have counts for

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Showing 2015Show all

5 papers · 1 filter

physics.space-ph2015★ 136 cited

Quantifying Gyrotropy in Magnetic Reconnection

M. Swisdak

A new scalar measure of the gyrotropy of a pressure tensor is defined. Previously suggested measures are shown to be incomplete by means of examples for which they give unphysical…

astro-ph.SR2015★ 58 cited

A model of the heliosphere with jets

J. F. Drake, M. Swisdak, M. Opher

An analytic model of the heliosheath (HS) between the termination shock (TS) and the heliopause (HP) is developed in the limit in which the interstellar flow and magnetic field are…

physics.plasm-ph2015

Electron acceleration in three-dimensional magnetic reconnection with a guide field

J. T. Dahlin, J. F. Drake, M. Swisdak

Kinetic simulations of 3D collisionless magnetic reconnection with a guide field show a dramatic enhancement of energetic electron production when compared with 2D systems. In the…

physics.plasm-ph2015★ 32 cited

Fast Magnetic Reconnection Due to Anisotropic Electron Pressure

P. A. Cassak, R. N. Baylor, R. L. Fermo +5

A new regime of fast magnetic reconnection with an out-of-plane (guide) magnetic field is reported in which the key role is played by an electron pressure anisotropy described by t…

astro-ph.SR2015★ 1 cited

Magnetized jets driven by the sun: the structure of the heliosphere revisited

M. Opher, J. F. Drake, B. Zieger +1

The classic accepted view of the heliosphere is a quiescent, comet-like shape aligned in the direction of the Sun's travel through the interstellar medium (ISM) extending for 1000'…