Forced 3D Reconnection in an Exponentially Separating Magnetic Field.

We present a solvable scenario for 3D reconnection in a sheared magnetic field. We consider a localized external force that is applied slowly to a flux tube and then maintained, generating an Alfvénic perturbation that spreads along the field lines. Separation of the sheared field lines reduces the scale of the perturbation across the field, enhancing magnetic diffusion. For a fusion-motivated equilibrium with exponential field-line separation, we find a reconnection timescale proportional to S/lnS under magnetohydrodynamics (MHD) and to S^{1/3} for semicollisional electron-only reconnection, where S is the Lundquist number of the perturbed flux tube. We generalize these results to arbitrary magnetic geometries, showing that the semicollisional case is geometry independent. Interestingly, we find that slower field-line separation yields an increased reconnection rate in MHD.

Publication Details

Journal
Apollo (University of Cambridge)
Published
2025-11-11
DOI
https://doi.org/10.17863/cam.122936
Primary Topic
Magnetic confinement fusion research
Type
article
Field-Weighted Citation Impact
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article

Forced 3D Reconnection in an Exponentially Separating Magnetic Field.

Apollo (University of Cambridge)
Magnetic confinement fusion research
article

Forced 3D Reconnection in an Exponentially Separating Magnetic Field.

article en

Abstract

We present a solvable scenario for 3D reconnection in a sheared magnetic field. We consider a localized external force that is applied slowly to a flux tube and then maintained, generating an Alfvénic perturbation that spreads along the field lines. Separation of the sheared field lines reduces the scale of the perturbation across the field, enhancing magnetic diffusion. For a fusion-motivated equilibrium with exponential field-line separation, we find a reconnection timescale proportional to S/lnS under magnetohydrodynamics (MHD) and to S^{1/3} for semicollisional electron-only reconnection, where S is the Lundquist number of the perturbed flux tube. We generalize these results to arbitrary magnetic geometries, showing that the semicollisional case is geometry independent. Interestingly, we find that slower field-line separation yields an increased reconnection rate in MHD.

Apollo (University of Cambridge)
Openalex Percentile: Top 28%
Magnetic confinement fusion research
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