Abstract
Particle-in-cell simulations are used to investigate the formation of magnetic fields in plasmas with perpendicular electron density and temperature gradients. For system sizes comparable to the ion skin depth , it is shown that , consistent with the Biermann battery effect. However, for large , it is found that the Weibel instability (due to electron temperature anisotropy) supersedes the Biermann battery as the main producer of . The Weibel-produced fields saturate at a finite amplitude (plasma ), independent of . The magnetic energy spectra below the electron Larmor radius scale are well fitted by the power law with slope , as predicted by Schekochihin et al. [Astrophys. J. Suppl. Ser. 182, 310 (2009)].
- Received 15 August 2013
DOI:https://doi.org/10.1103/PhysRevLett.112.175001
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