Fast Magnetic Reconnection: “Ideal” Tearing and the Hall Effect

Journal Article · Thu Aug 10 00:00:00 EDT 2017 · Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/AA7B82· OSTI ID:22875936

Pucci, Fulvia ^[1]; Velli, Marco; Tenerani, Anna ^[2]

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1. Dipartimento di Fisica e Astronomia, Università di Roma Tor Vergata (Italy)
2. Earth, Planetary and Space Sciences, University of California, Los Angeles, CA 90095 (United States)

One of the main questions in magnetic reconnection is the origin of triggering behavior with on/off properties that, once it is activated, accounts for the fast magnetic energy conversion to kinetic and thermal energies at the heart of explosive events in astrophysical and laboratory plasmas. Over the past decade, progress has been made on the initiation of fast reconnection via the plasmoid instability and what has been called “ideal” tearing, which sets in once current sheets thin to a critical inverse aspect ratio (a/L){sub c}. As shown by Pucci and Velli, at (a/L){sub c}∼S{sup −1/3}, the timescale for the instability to develop becomes of the order of the Alfvén time and independent of the Lundquist number (here defined in terms of current sheet length L). However, given the large values of S in natural plasmas, this transition might occur for thicknesses of the inner resistive singular layer that are comparable to the ion inertial length d {sub i}. When this occurs, Hall currents produce a three-dimensional quadrupole structure of the magnetic field, and the dispersive waves introduced by the Hall effect accelerate the instability. Here we present a linear study showing how the “ideal” tearing mode critical aspect ratio is modified when Hall effects are taken into account, including more general scaling laws of the growth rates in terms of sheet inverse aspect ratio: the critical inverse aspect ratio is amended to a/L≃(di/L){sup 0.29}(1/S){sup 0.19}, at which point the instability growth rate becomes Alfvénic and does not depend on either of the (small) parameters d{sub i}/L,1/S. We discuss the implications of this generalized triggering aspect ratio for recently developed phase diagrams of magnetic reconnection.

• OSTI ID: 22875936
• Journal Information: Astrophysical Journal, Vol. 845, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ASPECT RATIO
ASTROPHYSICS
COMPARATIVE EVALUATIONS
ENERGY CONVERSION
HALL EFFECT
INSTABILITY GROWTH RATES
LAYERS
MAGNETIC FIELDS
MAGNETIC RECONNECTION
MAGNETOHYDRODYNAMICS
PHASE DIAGRAMS
PLASMA
QUADRUPOLES
TEARING INSTABILITY
THICKNESS
THREE-DIMENSIONAL CALCULATIONS