On the periodicity of linear and nonlinear oscillatory reconnection
arXiv:1811.08831 · doi:10.1051/0004-6361/201834369
Abstract
(Abridged for ArXiv) An injection of energy towards a magnetic null point can drive reversals of current sheet polarity leading to time-dependent Oscillatory Reconnection, which is a possible explanation of how periodic phenomena can be generated when reconnection occurs in the solar atmosphere. However, the details of what controls the period of these oscillations is poorly understood, despite being crucial in assessing whether OR can account for observed periodic behaviour. This paper aims to highlight that different types of reconnection reversal are supported about null points, and that these are distinct from the oscillation on the closed-boundary, linear systems considered in the 1990s. In particular, we explore the features of a nonlinear oscillation local to the null point, and examine the effect of resistivity and perturbation energy on the period, contrasting it to the linear case. It is found that in the linear systems, the inverse Lundquist number dictates the period, provided the perturbation energy is small relative to the inverse Lundquist number defined on the boundary, regardless of the broadband structure of the initial perturbation. However, when the perturbation energy exceeds the threshold required for 'nonlinear' null collapse to occur, a complex oscillation of the magnetic field is produced which is, at best, only weakly-dependent on the resistivity. The resultant periodicity is strongly influenced by the amount of free energy, with more energetic perturbations producing higher-frequency oscillations. Crucially, with regards to typical solar-based and astrophysical-based input energies, we demonstrate that the majority far exceed the threshold for nonlinearity to develop. This substantially alters the properties and periodicity of both null collapse and subsequent OR. Therefore, nonlinear regimes of OR should be considered in solar and astrophysical contexts.
arXiv commentAccepted in A&A, 5 Figures (1 animated)
References in corpus (22)
- Instability of current sheets and formation of plasmoid chains
- Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares
- General Theory of the Plasmoid Instability
- Quasi-periodic pulsations in solar and stellar flares: an overview of recent results
- 3D Null Point Reconnection Regimes
- Nonlinear Fast Magnetoacoustic Wave Propagation in the Neighbourhood of a 2D magnetic X-point: Oscillatory Reconnection
- Review article: MHD wave propagation near coronal null points of magnetic fields
- Three-dimensional oscillatory magnetic reconnection
- Generation of quasi-periodic waves and flows in the solar atmosphere by oscillatory reconnection
- Alfvén Wave Heating of the Solar Chromosphere: 1.5D models
- On the Periodicity of Oscillatory Reconnection
- A quasi-periodic fast-propagating magnetosonic wave associated with the eruption of a magnetic flux rope
- Theory of magnetic reconnection in solar and astrophysical plasmas
- Spatio-temporal dynamics of sources of hard X-ray pulsations in solar flares
- Properties of quasi-periodic pulsations in solar flares from a single active region
- Magnetoacoustic Waves in a Stratified Atmosphere with a Magnetic Null Point
- Nonlinear wave propagation and reconnection at magnetic X-points in the Hall MHD regime
- Relationship of type III radio bursts with quasi-periodic pulsations in a solar flare
- Linear and nonlinear MHD mode coupling of the fast magnetoacoustic wave about a 3D magnetic null point
- Implosive collapse about magnetic null points: A quantitative comparison between 2D and 3D nulls
- 3D Alfven wave behaviour around proper and improper magnetic null points
- Resistively-limited current sheet implosions in planar anti-parallel (1D) and null-point containing (2D) magnetic field geometries
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- Oscillatory Reconnection of a 2D X-point in a hot coronal plasma
- Oscillatory reconnection as a plasma diagnostic in the solar corona
- The formation and dissipation of current sheets and shocks due to compressive waves in a stratified atmosphere containing a magnetic null
- Reconnection generated plasma flows in the quasi-separatrix layer in localised solar corona
- Simulation of Thermal Nonequilibrium Cycles in the Solar Wind
- HEL1OS -- A Hard X-ray Spectrometer on Board Aditya-L1
- The independence of oscillatory reconnection periodicity from the initial pulse