Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

The coalescence instability in collisionless plasmas

Journal Article · · Physics of Fluids B; (United States)
DOI:https://doi.org/10.1063/1.860392· OSTI ID:7259096
 [1]
  1. Department of Physics and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California 90024-1547 (United States)

The process whereby magnetic island structures tend to merge into larger units is known as magnetic island coalescence. This coalescence process is investigated for the case of a collisionless plasma by means of two-dimensional particle simulations. The pairwise merging of a preformed island chain leads to a gentle redistribution of the density and current density profiles. The linear growth rates substantially exceed the magnetohydrodynamic (MHD) values for {rho}/{lambda}{ge}0.1, where {rho} is the asymptotic ion gyroradius and {lambda} is the current sheet half-thickness. The nonlinear evolution of the collisionless tearing instability in a long system is found to lead to a much more violent coalescence process resulting in the formation of a vacuum X region. This stage is characterized by enhanced growth rates for the long-wavelength modes that exceed the maximum linear tearing growth rate, super-Alfvenic flows away from the reconnection X line, substantial bulk heating in the parallel direction, and the formation of energetic particle tails in the direction of the inductive electric field.

OSTI ID:
7259096
Journal Information:
Physics of Fluids B; (United States), Journal Name: Physics of Fluids B; (United States) Vol. 4:10; ISSN 0899-8221; ISSN PFBPE
Country of Publication:
United States
Language:
English