DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Multi-fluid and kinetic models of partially ionized magnetic reconnection

Abstract

Magnetic reconnection in partially ionized plasmas is a ubiquitous and important phenomenon in both laboratory and astrophysical systems. Here, simulations of partially ionized magnetic reconnection with well-matched initial conditions are performed using both multi-fluid and fully-kinetic approaches. Despite similar initial conditions, the time-dependent evolution differs between the two models. In multi-fluid models, the reconnection rate locally obeys either a decoupled Sweet–Parker scaling, where neutrals are unimportant, or a fully coupled Sweet–Parker scaling, where neutrals and ions are strongly coupled, depending on the resistivity. In contrast, kinetic models show a faster reconnection rate that is proportional to the fully-coupled, bulk Alfvén speed, $$v^*_A$$. In this work, these differences are interpreted as the result of operating in different collisional regimes. Multi-fluid simulations are found to maintain $$ν_{ni}L/v^*_A$$ ≳1, where $$ν_{ni}$$ is the neutral–ion collision frequency and L is the time-dependent current sheet half-length. This strongly couples neutrals to the reconnection outflow, while kinetic simulations evolve to allow $$ν_{ni}L/v^*_A$$ <1, decoupling neutrals from the reconnection outflow. Differences in the way reconnection is triggered may explain these discrepancies.

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [1]
  1. Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
  2. Harvard and Smithsonian, Cambridge, MA (United States)
Publication Date:
Research Org.:
Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States); Argonne National Laboratory (ANL), Argonne, IL (United States). Argonne Leadership Computing Facility (ALCF)
Sponsoring Org.:
National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); USDOE Office of Science (SC)
OSTI Identifier:
1804609
Alternate Identifier(s):
OSTI ID: 1776994
Grant/Contract Number:  
AC02-09CH11466; H-TIDES NNH15AB29I; S014981-F; 1931388; 80NSSC18K1124; 80NSSC20K0174; NNM07AB07C; AC02-06CH11357; AC0209CH11466.
Resource Type:
Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Volume: 28; Journal Issue: 4; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; Atomic and molecular collisions; Thermodynamic states and processes; Computational fluid dynamics; Energy equations; Charge exchange reactions; Particle-in-cell method; Plasma properties and parameters; Magnetic reconnection; Collisional processes; Partially ionized plasma

Citation Formats

Jara-Almonte, J., Murphy, N. A., and Ji, H. Multi-fluid and kinetic models of partially ionized magnetic reconnection. United States: N. p., 2021. Web. doi:10.1063/5.0039860.
Jara-Almonte, J., Murphy, N. A., & Ji, H. Multi-fluid and kinetic models of partially ionized magnetic reconnection. United States. https://doi.org/10.1063/5.0039860
Jara-Almonte, J., Murphy, N. A., and Ji, H. Tue . "Multi-fluid and kinetic models of partially ionized magnetic reconnection". United States. https://doi.org/10.1063/5.0039860. https://www.osti.gov/servlets/purl/1804609.
@article{osti_1804609,
title = {Multi-fluid and kinetic models of partially ionized magnetic reconnection},
author = {Jara-Almonte, J. and Murphy, N. A. and Ji, H.},
abstractNote = {Magnetic reconnection in partially ionized plasmas is a ubiquitous and important phenomenon in both laboratory and astrophysical systems. Here, simulations of partially ionized magnetic reconnection with well-matched initial conditions are performed using both multi-fluid and fully-kinetic approaches. Despite similar initial conditions, the time-dependent evolution differs between the two models. In multi-fluid models, the reconnection rate locally obeys either a decoupled Sweet–Parker scaling, where neutrals are unimportant, or a fully coupled Sweet–Parker scaling, where neutrals and ions are strongly coupled, depending on the resistivity. In contrast, kinetic models show a faster reconnection rate that is proportional to the fully-coupled, bulk Alfvén speed, $v^*_A$. In this work, these differences are interpreted as the result of operating in different collisional regimes. Multi-fluid simulations are found to maintain $ν_{ni}L/v^*_A$ ≳1, where $ν_{ni}$ is the neutral–ion collision frequency and L is the time-dependent current sheet half-length. This strongly couples neutrals to the reconnection outflow, while kinetic simulations evolve to allow $ν_{ni}L/v^*_A$ <1, decoupling neutrals from the reconnection outflow. Differences in the way reconnection is triggered may explain these discrepancies.},
doi = {10.1063/5.0039860},
journal = {Physics of Plasmas},
number = 4,
volume = 28,
place = {United States},
year = {Tue Apr 13 00:00:00 EDT 2021},
month = {Tue Apr 13 00:00:00 EDT 2021}
}

Works referenced in this record:

Magnetic reconnection in the low solar chromosphere with a more realistic radiative cooling model
journal, April 2018

  • Ni, Lei; Lukin, Vyacheslav S.; Murphy, Nicholas A.
  • Physics of Plasmas, Vol. 25, Issue 4
  • DOI: 10.1063/1.5018351

Interaction of the solar wind with the local interstellar medium
journal, November 1995

  • Pauls, H. L.; Zank, G. P.; Williams, L. L.
  • Journal of Geophysical Research: Space Physics, Vol. 100, Issue A11
  • DOI: 10.1029/95JA02023

A general nonlinear fluid model for reacting plasma-neutral mixtures
journal, July 2012

  • Meier, E. T.; Shumlak, U.
  • Physics of Plasmas, Vol. 19, Issue 7
  • DOI: 10.1063/1.4736975

Magnetic reconnection in a weakly ionized plasma
journal, June 2013

  • Leake, James E.; Lukin, Vyacheslav S.; Linton, Mark G.
  • Physics of Plasmas, Vol. 20, Issue 6
  • DOI: 10.1063/1.4811140

Are iris Bombs Connected to Ellerman Bombs?
journal, June 2016


Prevalence of small-scale jets from the networks of the solar transition region and chromosphere
journal, October 2014


Influence of Coulomb collisions on the structure of reconnection layers
journal, July 2009

  • Daughton, W.; Roytershteyn, V.; Albright, B. J.
  • Physics of Plasmas, Vol. 16, Issue 7
  • DOI: 10.1063/1.3191718

Influence of 3D plasmoid dynamics on the transition from collisional to kinetic reconnection
journal, July 2019

  • Stanier, A.; Daughton, W.; Le, A.
  • Physics of Plasmas, Vol. 26, Issue 7
  • DOI: 10.1063/1.5100737

Multi-Fluid Simulations of Chromospheric Magnetic Reconnection in a Weakly Ionized Reacting Plasma
journal, November 2012


Magnetic Reconnection in Strongly Magnetized Regions of the Low Solar Chromosphere
journal, January 2018

  • Ni, Lei; Lukin, Vyacheslav S.; Murphy, Nicholas A.
  • The Astrophysical Journal, Vol. 852, Issue 2
  • DOI: 10.3847/1538-4357/aa9edb

A binary collision model for plasma simulation with a particle code
journal, November 1977


The SEL macroscopic modeling code
journal, December 2004


Particle-in-cell charged-particle simulations, plus Monte Carlo collisions with neutral atoms, PIC-MCC
journal, April 1991

  • Birdsall, C. K.
  • IEEE Transactions on Plasma Science, Vol. 19, Issue 2
  • DOI: 10.1109/27.106800

The Effect of Wave-Particle Interactions on the Propagation of Cosmic Rays
journal, May 1969

  • Kulsrud, Russell; Pearce, William P.
  • The Astrophysical Journal, Vol. 156
  • DOI: 10.1086/149981

Ultrahigh performance three-dimensional electromagnetic relativistic kinetic plasma simulation
journal, May 2008

  • Bowers, K. J.; Albright, B. J.; Yin, L.
  • Physics of Plasmas, Vol. 15, Issue 5
  • DOI: 10.1063/1.2840133

Magnetic reconnection in partially ionized gases
journal, May 1989

  • Zweibel, Ellen G.
  • The Astrophysical Journal, Vol. 340
  • DOI: 10.1086/167416

Phase diagram for magnetic reconnection in heliophysical, astrophysical, and laboratory plasmas
journal, November 2011

  • Ji, Hantao; Daughton, William
  • Physics of Plasmas, Vol. 18, Issue 11
  • DOI: 10.1063/1.3647505

Magnetic Reconnection in Astrophysical and Laboratory Plasmas
journal, September 2009


Onset of fast Magnetic Reconnection in Partially Ionized Gases
journal, September 2011


Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
journal, December 2007


Laboratory Study of Hall Reconnection in Partially Ionized Plasmas
journal, January 2013


Hot explosions in the cool atmosphere of the Sun
journal, October 2014


Driven magnetic reconnection near the Dreicer limit
journal, May 2010

  • Roytershteyn, V.; Daughton, W.; Dorfman, S.
  • Physics of Plasmas, Vol. 17, Issue 5
  • DOI: 10.1063/1.3399787

Magnetic reconnection
journal, March 2010


Experimental Test of the Sweet-Parker Model of Magnetic Reconnection
journal, April 1998


Solar Hydrogen "bombs"
journal, July 1917

  • Ellerman, Ferdinand
  • The Astrophysical Journal, Vol. 46
  • DOI: 10.1086/142366

Experimental Verification of the Hall Effect during Magnetic Reconnection in a Laboratory Plasma
journal, July 2005


The formation of sharp structures by ambipolar diffusion
journal, June 1994

  • Brandenburg, Axel; Zweibel, Ellen G.
  • The Astrophysical Journal, Vol. 427
  • DOI: 10.1086/187372

Asymmetric Magnetic Reconnection in Weakly Ionized Chromospheric Plasmas
journal, May 2015


Magnetic reconnection in partially ionized plasmas
journal, April 2020

  • Ni, Lei; Ji, Hantao; Murphy, Nicholas A.
  • Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 476, Issue 2236
  • DOI: 10.1098/rspa.2019.0867

Mathematical structure of transport equations for multispecies flows
journal, January 1977


Kinetic Simulations of Magnetic Reconnection in Partially Ionized Plasmas
journal, January 2019