The role of the helicity spectrum function in turbulent dynamo theory
DOI10.1080/03091928208209016zbMath0509.76106OpenAlexW2093787260WikidataQ114640678 ScholiaQ114640678MaRDI QIDQ4749516
M. R. E. Proctor, Henry Keith Moffatt
Publication date: 1982
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091928208209016
dynamo theoryalpha-effectfirst-order smoothing approximationmean electromotive forcehelical inertia waveshelicity spectrum functionRaedler effectreflectional symmetric and asymmetric ingredients
General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Isotropic turbulence; homogeneous turbulence (76F05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Geo-electricity and geomagnetism (86A25)
Related Items (2)
Cites Work
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- On the theory of stationary random processes
- A convection-driven dynamo I. The weak field case
- Diffusion of passive-scalar and magnetic fields by helical turbulence
- The mean electromotive force generated by turbulence in the limit of perfect conductivity
- An approach to a dynamic theory of dynamo action in a rotating conducting fluid
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