Scaling theory of three-dimensional magnetic reconnection spreading
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Arencibia, Milton
[1
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Cassak, P. A.
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West Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
West Virginia Univ, Ctr KINETIC Plasma Phys, Morgantown, WV 26506 USAWest Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
Cassak, P. A.
[1
,2
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Shay, M. A.
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Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USAWest Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
Shay, M. A.
[3
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Priest, E. R.
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St Andrews Univ, Dept Math, St Andrews KY16 8QR, Fife, ScotlandWest Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
Priest, E. R.
[4
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[1] West Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
[2] West Virginia Univ, Ctr KINETIC Plasma Phys, Morgantown, WV 26506 USA
[3] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
[4] St Andrews Univ, Dept Math, St Andrews KY16 8QR, Fife, Scotland
We develop a first-principles scaling theory of the spreading of three-dimensional (3D) magnetic reconnection of finite extent in the out of plane direction. This theory addresses systems with or without an out of plane (guide) magnetic field, and with or without Hall physics. The theory reproduces known spreading speeds and directions with and without guide fields, unifying previous knowledge in a single theory. New results include the following: (1) reconnection spreads in a particular direction if an x-line is induced at the interface between reconnecting and non-reconnecting regions, which is controlled by the out of plane gradient of the electric field in the outflow direction. (2) The spreading mechanism for anti-parallel collisionless reconnection is convection, as is known, but for guide field reconnection it is magnetic field bending. We confirm the theory using 3D two-fluid and resistive-magnetohydrodynamics simulations. (3) The theory explains why anti-parallel reconnection in resistive-magnetohydrodynamics does not spread. (4) The simulation domain aspect ratio, associated with the free magnetic energy, influences whether reconnection spreads or convects with a fixed x-line length. (5) We perform a simulation initiating anti-parallel collisionless reconnection with a pressure pulse instead of a magnetic perturbation, finding spreading is unchanged rather than spreading at the magnetosonic speed as previously suggested. The results provide a theoretical framework for understanding spreading beyond systems studied here and are important for applications including two-ribbon solar flares and reconnection in Earth's magnetosphere.