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| Main Authors: | , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2508.03573 |
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| _version_ | 1866911274965663744 |
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| author | Moore, Nicholas J. Smith, Stefan G. Llewellyn |
| author_facet | Moore, Nicholas J. Smith, Stefan G. Llewellyn |
| contents | We consider a variant of the kinematic dynamo problem. Rather than prescribing a velocity field and searching for high-growth magnetic fields via an eigenvalue problem, we treat the seed magnetic-field structure as given and ask which velocity field maximally enhances its instantaneous growth. We show this second problem has an elegant formulation in terms of variational calculus. Upon simultaneously constraining the velocity's kinetic energy and enstrophy, the Euler-Lagrange equation leads to a forced Helmholtz partial differential equation (PDE) for the optimal velocity field. For the special case of fixed kinetic energy and unconstrained enstrophy, the optimal velocity field everywhere opposes the divergence-free projection of the Lorentz force. In the more general setting, the optimal velocity field can be found through numerical solution of the forced Helmholtz PDE. We construct 2.5-dimensional numerical examples to support the theoretical findings. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_03573 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Optimal velocity fields for instantaneous magnetic field growth Moore, Nicholas J. Smith, Stefan G. Llewellyn Fluid Dynamics We consider a variant of the kinematic dynamo problem. Rather than prescribing a velocity field and searching for high-growth magnetic fields via an eigenvalue problem, we treat the seed magnetic-field structure as given and ask which velocity field maximally enhances its instantaneous growth. We show this second problem has an elegant formulation in terms of variational calculus. Upon simultaneously constraining the velocity's kinetic energy and enstrophy, the Euler-Lagrange equation leads to a forced Helmholtz partial differential equation (PDE) for the optimal velocity field. For the special case of fixed kinetic energy and unconstrained enstrophy, the optimal velocity field everywhere opposes the divergence-free projection of the Lorentz force. In the more general setting, the optimal velocity field can be found through numerical solution of the forced Helmholtz PDE. We construct 2.5-dimensional numerical examples to support the theoretical findings. |
| title | Optimal velocity fields for instantaneous magnetic field growth |
| topic | Fluid Dynamics |
| url | https://arxiv.org/abs/2508.03573 |