English

Where should MMS look for electron diffusion regions?

Space Physics 2016-06-22 v1 Earth and Planetary Astrophysics Plasma Physics

Abstract

A great possible achievement for the MMS mission would be crossing electron diffusion regions (EDR). EDR are regions in proximity of reconnection sites where electrons decouple from field lines, breaking the frozen in condition. Decades of research on reconnection have produced a widely shared map of where EDRs are. We expect reconnection to take place around a so called x-point formed by the intersection of the separatrices dividing inflowing from outflowing plasma. The EDR forms around this x-point as a small electron scale box nested inside a larger ion diffusion region. But this point of view is based on a 2D mentality. We have recently proposed that once the problem is considered in full 3D, secondary reconnection events can form [Lapenta et al., Nature Physics, 11, 690, 2015] in the outflow regions even far downstream from the primary reconnection site. We revisit here this new idea confirming that even using additional indicators of reconnection and even considering longer periods and wider distances the conclusion remains true: secondary reconnection sites form downstream of a reconnection outflow causing a sort of chain reaction of cascading reconnection sites. If we are right, MMS will have an interesting journey even when not crossing necessarily the primary site. The chances are greatly increased that even if missing a primary site during an orbit, MMS could stumble instead on one of these secondary sites.

Keywords

Cite

@article{arxiv.1510.03536,
  title  = {Where should MMS look for electron diffusion regions?},
  author = {G. Lapenta and M. Goldman and D. Newman and S. Markidis},
  journal= {arXiv preprint arXiv:1510.03536},
  year   = {2016}
}

Comments

submitted to the Astronum 2015 Conference Proceedings

R2 v1 2026-06-22T11:18:45.330Z