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Reynolds-averaged turbulence model for magnetohydrodynamic dynamo in a rotating spherical shell

Abstract

Numerical simulation of the magnetic field in a rotating spherical shell was carried out to assess and improve the Reynolds-averaged turbulence model for magnetohydrodynamic flows. In the three-equation model the transport equations for the turbulent energy, its dissipation rate, and the turbulent helicity are solved in addition to the mean magnetic field. The turbulent electromotive force involved in the magnetic field equation is expressed in terms of the {alpha} dynamo and turbulent diffusivity terms. Since the model was improved considering the realizability condition for the turbulent electromotive force, steady state solutions were obtained even in the case of rapidly rotating system such as the Earth. Profiles of the magnetic field, the turbulent energy, and the turbulent helicity as well as their transport equations were examined to check the dynamo mechanism expressed in the model. The dependence on the system rotation and on model constants was examined to assess the model performance.
Authors:
Hamba, Fujihiro [1] 
  1. Institute of Industrial Science, University of Tokyo, Komaba, Meguro-ku, Tokyo 153-8505 (Japan)
Publication Date:
Nov 01, 2004
Product Type:
Journal Article
Resource Relation:
Journal Name: Physics of Plasmas; Journal Volume: 11; Journal Issue: 11; Other Information: DOI: 10.1063/1.1792285; (c) 2004 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); PBD: Nov 2004
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; CHARGED-PARTICLE TRANSPORT; HELICITY; MAGNETOHYDRODYNAMICS; PLASMA; PLASMA SIMULATION; TURBULENCE
OSTI ID:
20619205
Country of Origin:
United States
Language:
English
Other Identifying Numbers:
Journal ID: ISSN 1070-664X; PHPAEN; TRN: US05A0646062710
Submitting Site:
INIS
Size:
page(s) 5316-5327
Announcement Date:
Aug 21, 2005

Citation Formats

Hamba, Fujihiro. Reynolds-averaged turbulence model for magnetohydrodynamic dynamo in a rotating spherical shell. United States: N. p., 2004. Web. doi:10.1063/1.1792285.
Hamba, Fujihiro. Reynolds-averaged turbulence model for magnetohydrodynamic dynamo in a rotating spherical shell. United States. https://doi.org/10.1063/1.1792285
Hamba, Fujihiro. 2004. "Reynolds-averaged turbulence model for magnetohydrodynamic dynamo in a rotating spherical shell." United States. https://doi.org/10.1063/1.1792285.
@misc{etde_20619205,
title = {Reynolds-averaged turbulence model for magnetohydrodynamic dynamo in a rotating spherical shell}
author = {Hamba, Fujihiro}
abstractNote = {Numerical simulation of the magnetic field in a rotating spherical shell was carried out to assess and improve the Reynolds-averaged turbulence model for magnetohydrodynamic flows. In the three-equation model the transport equations for the turbulent energy, its dissipation rate, and the turbulent helicity are solved in addition to the mean magnetic field. The turbulent electromotive force involved in the magnetic field equation is expressed in terms of the {alpha} dynamo and turbulent diffusivity terms. Since the model was improved considering the realizability condition for the turbulent electromotive force, steady state solutions were obtained even in the case of rapidly rotating system such as the Earth. Profiles of the magnetic field, the turbulent energy, and the turbulent helicity as well as their transport equations were examined to check the dynamo mechanism expressed in the model. The dependence on the system rotation and on model constants was examined to assess the model performance.}
doi = {10.1063/1.1792285}
journal = []
issue = {11}
volume = {11}
journal type = {AC}
place = {United States}
year = {2004}
month = {Nov}
}