English

Characterizing magnetic reconnection regions using Gaussian mixture models on particle velocity distributions

Plasma Physics 2020-02-05 v1 Solar and Stellar Astrophysics Space Physics

Abstract

We present a method based on unsupervised machine learning to identify regions of interest using particle velocity distributions as a signature pattern. An automatic density estimation technique is applied to particle distributions provided by PIC simulations to study magnetic reconnection. The key components of the method involve: i) a Gaussian mixture model determining the presence of a given number of subpopulations within an overall population, and ii) a model selection technique with Bayesian Information Criterion to estimate the appropriate number of subpopulations. Thus, this method identifies automatically the presence of complex distributions, such as beams or other non-Maxwellian features, and can be used as a detection algorithm able to identify reconnection regions. The approach is demonstrated for specific double Harris sheet simulations but it can in principle be applied to any other type of simulation and observational data on the particle distribution function.

Keywords

Cite

@article{arxiv.1910.10012,
  title  = {Characterizing magnetic reconnection regions using Gaussian mixture models on particle velocity distributions},
  author = {Romain Dupuis and Martin V. Goldman and David L. Newman and Jorge Amaya and Giovanni Lapenta},
  journal= {arXiv preprint arXiv:1910.10012},
  year   = {2020}
}

Comments

20 pages, 8 figures