Force-free foliations

Geoffrey Compère, Samuel E. Gralla, and Alexandru Lupsasca
Phys. Rev. D 94, 124012 – Published 8 December 2016

Abstract

Electromagnetic field configurations with vanishing Lorentz force density are known as force-free and appear in terrestrial, space, and astrophysical plasmas. We explore a general method for finding such configurations based on formulating equations for the field lines rather than the field itself. The basic object becomes a foliation of spacetime or, in the stationary axisymmetric case, of the half-plane. We use this approach to find some new stationary and axisymmetric solutions, one of which could represent a rotating plasma vortex near a magnetic null point.

  • Figure
  • Received 7 October 2016

DOI:https://doi.org/10.1103/PhysRevD.94.124012

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsPlasma Physics

Authors & Affiliations

Geoffrey Compère1,*, Samuel E. Gralla2,†, and Alexandru Lupsasca3,‡

  • 1Université Libre de Bruxelles and International Solvay Institutes Brussels, CP 231 B-1050, Belgium
  • 2Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
  • 3Center for the Fundamental Laws of Nature, Harvard University, Cambridge, Massachusetts 02138, USA

  • *gcompere@ulb.ac.be
  • sgralla@email.arizona.edu
  • lupsasca@fas.harvard.edu

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Issue

Vol. 94, Iss. 12 — 15 December 2016

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