Nonlinear Fast Magnetoacoustic Wave Propagation in the Neighbourhood of a 2D magnetic X-point: Oscillatory Reconnection
arXiv:0901.1781 · doi:10.1051/0004-6361:200810465
Abstract
This paper extends the models of Craig & McClymont (1991) and McLaughlin & Hood (2004) to include finite and nonlinear effects. We investigate the nature of nonlinear fast magnetoacoustic waves about a 2D magnetic X-point. We solve the compressible and resistive MHD equations using a Lagrangian remap, shock capturing code (Arber et al. 2001) and consider an initial condition in (a natural variable of the system). We observe the formation of both fast and slow oblique magnetic shocks. The nonlinear wave deforms the X-point into a 'cusp-like' point which in turn collapses to a current sheet. The system then evolves through a series of horizontal and vertical current sheets, with associated changes in connectivity, i.e. the system exhibits oscillatory reconnection. Our final state is non-potential (but in force balance) due to asymmetric heating from the shocks. Larger amplitudes in our initial condition correspond to larger values of the final current density left in the system. The inclusion of nonlinear terms introduces several new features to the system that were absent from the linear regime.
14 pages, 16 figures
References in corpus (8)
- MHD wave propagation in the neighbourhood of a two-dimensional null point
- Current amplification and magnetic reconnection at a 3D null point. I - Physical characteristics
- A new view of quiet-Sun topology from Hinode/SOT
- MHD mode coupling in the neighbourhood of a 2D null point
- Magnetohydrodynamics wave propagation in the neighbourhood of two dipoles
- MHD Wave Propagation in the Neighbourhood of Two Null Points
- 3D MHD Coronal Oscillations About a Magnetic Null Point: Application of WKB Theory
- A New Look at Mode Conversion in a Stratified Isothermal Atmosphere
Cited by in corpus (22)
- Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
- Persistent Doppler shift oscillations observed with HINODE/EIS in the solar corona: spectroscopic signatures of Alfvenic waves and recurring upflows
- Quasi-periodic pulsations in solar and stellar flares: an overview of recent results
- Above-the-loop-top Oscillation and Quasi-periodic Coronal Wave Generation in Solar Flares
- Quasi-periodic Slipping Magnetic Reconnection During an X-class Solar Flare Observed by the Solar Dynamics Observatory and Interface Region Imaging Spectrograph
- Three-dimensional oscillatory magnetic reconnection
- Generation of quasi-periodic waves and flows in the solar atmosphere by oscillatory reconnection
- On the Periodicity of Oscillatory Reconnection
- A blueprint of state-of-the-art techniques for detecting quasi-periodic pulsations in solar and stellar flares
- A Compact Source for Quasi-Periodic Pulsation in an M-class Solar Flare
- A case-study of multi-temperature coronal jets for emerging flux MHD models
- Magnetoacoustic Waves in a Stratified Atmosphere with a Magnetic Null Point
- Abnormal oscillation modes in a waning light bridge
- The relationship between hard X-ray pulse timings and the locations of footpoint sources during solar flares
- Linear and nonlinear MHD mode coupling of the fast magnetoacoustic wave about a 3D magnetic null point
- Reciprocatory magnetic reconnection in a coronal bright point
- The formation and dissipation of current sheets and shocks due to compressive waves in a stratified atmosphere containing a magnetic null
- A Theoretical Model of Pinching Current Sheet in Low-beta Plasmas
- Phase Mixing of Alfvén Waves Near a 2D Magnetic Null Point
- The behaviour of magnetoacoustic waves in the neighbourhood of a two-dimensional null point: initially cylindrically-symmetric perturbations
- Relativistic magnetic reconnection at X-type neutral points
- 3D WKB solution for fast magnetoacoustic wave behaviour around an X-line