English

Electromagnetic Energy Conversion in Downstream Fronts from 3D Kinetic Reconnection

Plasma Physics 2015-06-18 v1 Earth and Planetary Astrophysics Solar and Stellar Astrophysics Space Physics

Abstract

The electromagnetic energy equation is analyzed term by term in a 3D simulation of kinetic reconnection previously reported by \citet{vapirev2013formation}. The evolution presents the usual 2D-like topological structures caused by an initial perturbation independent of the third dimension. However, downstream of the reconnection site, where the jetting plasma encounters the yet unperturbed pre-existing plasma, a downstream front (DF) is formed and made unstable by the strong density gradient and the unfavorable local acceleration field. The energy exchange between plasma and fields is most intense at the instability, reaching several pW/m3pW/m^3, alternating between load (energy going from fields to particles) and generator (energy going from particles to fields) regions. Energy exchange is instead purely that of a load at the reconnection site itself in a region focused around the x-line and elongated along the separatrix surfaces. Poynting fluxes are generated at all energy exchange regions and travel away from the reconnection site transporting an energy signal of the order of about S103W/m2\mathbf S \approx 10^{-3} W/m^2.

Keywords

Cite

@article{arxiv.1402.0082,
  title  = {Electromagnetic Energy Conversion in Downstream Fronts from 3D Kinetic Reconnection},
  author = {Giovanni Lapenta and Martin Goldman and David Newman and Stefano Markidis and Andrey Divin},
  journal= {arXiv preprint arXiv:1402.0082},
  year   = {2015}
}

Comments

Based on an invited talk presented at the APS-DPP2013 meeting in Denver. To appear on Phys. Plasmas

R2 v1 2026-06-22T02:59:05.537Z