On the Value of the Reconnection Rate
arXiv:1609.02998 · doi:10.1017/S002237781600101X
Abstract
Numerical simulations have consistently shown that the reconnection rate in certain collisionless regimes can be fast, on the order of , where and are the Alfvén speed and the reconnecting magnetic field upstream of the ion diffusion region. This particular value has been reported in myriad numerical simulations under disparate conditions. However, despite decades of research, the reasons underpinning this specific value remain mysterious. Here, we present an overview of this problem and discuss the conditions under which the "0.1 value" is attained. Furthermore, we explain why this problem should be interpreted in terms of the ion diffusion region length.
Manuscript submitted for the JPP Special Issue "Solved and Unsolved Problems in Plasma Physics"
References in corpus (6)
- Instability of current sheets and formation of plasmoid chains
- General Theory of the Plasmoid Instability
- Scaling of magnetic reconnection in relativistic collisionless plasmas
- Extended theory of the Taylor problem in the plasmoid-unstable regime
- Self-regulation of the reconnecting current layer in relativistic pair plasma reconnection
- Rapid Change of Field Line Connectivity and Reconnection in Stochastic Magnetic Fields
Cited by in corpus (34)
- Why does steady-state magnetic reconnection have a maximum local rate of order 0.1?
- A Review of the 0.1 Reconnection Rate Problem
- Plasmoid Instability in Forming Current Sheets
- Magnetic Reconnection as a Mechanism for Energy Extraction from Rotating Black Holes
- First-Principles Theory of the Rate of Magnetic Reconnection in Magnetospheric and Solar Plasmas
- 3D magnetic reconnection and its application to solar flares
- Magnetic Reconnection and Energy Extraction from a Spinning Black Hole with Broken Lorentz Symmetry
- Ion and Electron Acceleration in Fully Kinetic Plasma Turbulence
- TeV neutrinos and hard X-rays from relativistic reconnection in the corona of NGC 1068
- Pitch Angle Anisotropy Controls Particle Acceleration and Cooling in Radiative Relativistic Plasma Turbulence
- A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
- Relativistic Magnetic Reconnection in Astrophysical Plasmas: A Powerful Mechanism of Nonthermal Emission
- Effects of tidal charge on magnetic reconnection and energy extraction from spinning braneworld black hole
- Relativistic Nonthermal Particle Acceleration in Two-Dimensional Collisionless Magnetic Reconnection
- Generation of near-equipartition magnetic fields in turbulent collisionless plasmas
- Extracting energy via magnetic reconnection from Kerr-de Sitter black holes
- Pitch-Angle Anisotropy Imprinted by Relativistic Magnetic Reconnection
- Harvesting energy driven by Comisso-Asenjo process from Kerr-MOG black holes
- Effective resistivity in relativistic collisionless plasmoid-mediated reconnection
- Turbulent model of Crab nebula radiation
- Concurrent Particle Acceleration and Pitch-Angle Anisotropy Driven by Magnetic Reconnection: Ion-Electron Plasmas
- Energy extraction from rotating regular black hole via Comisso-Asenjo mechanism
- Impact of 3D Structure on Magnetic Reconnection
- Resistively controlled primordial magnetic turbulence decay
- Oscillatory reconnection and waves driven by merging magnetic flux ropes in solar flares
- Hall MHD waves: A fundamental departure from their MHD counterparts
- The effects of resistivity on oscillatory reconnection and consequences for solar flare Quasi Periodic Pulsations
- Particle-in-Cell Simulations of Relativistic Magnetic Reconnection with Advanced Maxwell Solver Algorithms
- Hamiltonian formulation of X-point collapse in an extended magnetohydrodynamics framework
- Laboratory study of magnetic reconnection in lunar-relevant mini-magnetospheres
- Magnetic reconnection: an alternative explanation of radio emission in galaxy clusters
- Local extraction of three-dimensional magnetic reconnection X-lines
- Systematic 2.5 D resistive MHD simulations with ambipolar diffusion and Hall effect for fast magnetic reconnection
- Driven Collisionless Reconnection of Force-free Flux Tubes: From Onset to Coalescence