Magnetic-Field Generation and Amplification in an Expanding Plasma

K. M. Schoeffler, N. F. Loureiro, R. A. Fonseca, and L. O. Silva
Phys. Rev. Lett. 112, 175001 – Published 30 April 2014

Abstract

Particle-in-cell simulations are used to investigate the formation of magnetic fields B in plasmas with perpendicular electron density and temperature gradients. For system sizes L comparable to the ion skin depth di, it is shown that Bdi/L, consistent with the Biermann battery effect. However, for large L/di, it is found that the Weibel instability (due to electron temperature anisotropy) supersedes the Biermann battery as the main producer of B. The Weibel-produced fields saturate at a finite amplitude (plasma β100), independent of L. The magnetic energy spectra below the electron Larmor radius scale are well fitted by the power law with slope 16/3, as predicted by Schekochihin et al. [Astrophys. J. Suppl. Ser. 182, 310 (2009)].

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  • Received 15 August 2013

DOI:https://doi.org/10.1103/PhysRevLett.112.175001

© 2014 American Physical Society

Authors & Affiliations

K. M. Schoeffler1, N. F. Loureiro1, R. A. Fonseca1,2, and L. O. Silva1

  • 1Instituto de Plasmas e Fusão Nuclear—Laboratório Associado, Instituto Superior Técnico, Universidade de Lisboa, 1049-001 Lisboa, Portugal
  • 2DCTI/ISCTE—Instituto Universitário de Lisboa, 1649-026 Lisboa, Portugal

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Vol. 112, Iss. 17 — 2 May 2014

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