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Title: Collisionless kinetic theory of oblique tearing instabilities

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.5020777· OSTI ID:1429052
 [1];  [2];  [3]
  1. Univ. of Iowa, Iowa City, IA (United States). Dept. of Physics and Astronomy
  2. Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences; Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
  3. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

The linear dispersion relation for collisionless kinetic tearing instabilities is calculated for the Harris equilibrium. In contrast to the conventional 2D geometry, which considers only modes at the center of the current sheet, modes can span the current sheet in 3D. Modes at each resonant surface have a unique angle with respect to the guide field direction. Both kinetic simulations and numerical eigenmode solutions of the linearized Vlasov-Maxwell equations have recently revealed that standard analytic theories vastly overestimate the growth rate of oblique modes. We find that this stabilization is associated with the density-gradient-driven diamagnetic drift. The analytic theories miss this drift stabilization because the inner tearing layer broadens at oblique angles sufficiently far that the assumption of scale separation between the inner and outer regions of boundarylayer theory breaks down. The dispersion relation obtained by numerically solving a single second order differential equation is found to approximately capture the drift stabilization predicted by solutions of the full integro-differential eigenvalue problem. A simple analytic estimate for the stability criterion is provided.

Research Organization:
Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Univ. of Iowa, Iowa City, IA (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Fusion Energy Sciences (FES); National Science Foundation (NSF)
Grant/Contract Number:
SC0016159; AGS-0962698; AC52-06NA25396
OSTI ID:
1429052
Alternate ID(s):
OSTI ID: 1421302; OSTI ID: 1438147; OSTI ID: 1777874
Report Number(s):
LA-UR-18-21045; TRN: US1802606
Journal Information:
Physics of Plasmas, Vol. 25, Issue 2; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 5 works
Citation information provided by
Web of Science

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Cited By (3)

Influence of 3D plasmoid dynamics on the transition from collisional to kinetic reconnection journal July 2019
Relativistic Tearing Mode in Pair Plasmas and Application to Magnetic Giant Flares journal July 2019
The Interplay of Magnetically Dominated Turbulence and Magnetic Reconnection in Producing Nonthermal Particles journal November 2019

Figures / Tables (13)