English

On the Value of the Reconnection Rate

Plasma Physics 2016-11-08 v1 High Energy Astrophysical Phenomena Solar and Stellar Astrophysics Space Physics

Abstract

Numerical simulations have consistently shown that the reconnection rate in certain collisionless regimes can be fast, on the order of 0.1vABu0.1 v_A B_u, where vAv_A and BuB_u are the Alfv\'en speed and the reconnecting magnetic field upstream of the ion diffusion region. This particular value has been reported in myriad numerical simulations under disparate conditions. However, despite decades of research, the reasons underpinning this specific value remain mysterious. Here, we present an overview of this problem and discuss the conditions under which the "0.1 value" is attained. Furthermore, we explain why this problem should be interpreted in terms of the ion diffusion region length.

Keywords

Cite

@article{arxiv.1609.02998,
  title  = {On the Value of the Reconnection Rate},
  author = {Luca Comisso and Amitava Bhattacharjee},
  journal= {arXiv preprint arXiv:1609.02998},
  year   = {2016}
}

Comments

Manuscript submitted for the JPP Special Issue "Solved and Unsolved Problems in Plasma Physics"