Abstract
In turbulent fluid motion, a number of ordered or coherent structures can be detected, which may be classified according to their characteristic spatial scales. As is seen from Eq. (3.46), components of fluid motion with larger spatial scales possess longer time scales in general, and they have large influence on various flow aspects. In this sense, the component of turbulent motion that is abstracted through the ensemble averaging procedure often contain important global properties. In reality, the flow structure characterized by the mean velocity gradient governs the production mechanism of turbulent energy or the mechanism of draining energy from large- to small-scale components.
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References
Biskamp, D. (1993), Nonlinear Magnetohydrodynamics (Cambridge U. P., Cambridge).
Braginskii, S. (1964), JETP 20, 1462.
Chen, H. and Montgomery, D. (1987) Plasma Phys. and Controlled Fusion 29, 205.
Cowling, T. G. (1934), Mon. Not. Astron. Soc. 94, 39.
Hamba, F. (1987), J. Phys. Soc. Jpn. 56, 79.
Hamba, F. (1992), Phys. Fluids A 4, 441.
Hoyng, P. (1993), in The Sun: A Laboratory for Astrophysics, edited by J. T. Schmelz and J. C. Brown ( Kluwer, Dordrecht ), p. 99.
Kato, S. and Yoshizawa, A. (1993), Publ. Astron. Soc. Jpn. 45, 103.
Kraichnan, R. H. (1965), Phys. Fluids 8, 1385.
Krause, F. and Rädler, K. -H. (1980), Mean-Field Magnetohydrodynamics and Dynamo Theory ( Pergamon, Oxford).
Melchior, P. (1986), The Physics of the Earth’s Core (Pergamon, Oxford). Miyamoto, K. (1989), Plasma Physics for Controlled Fusion ( The MIT, Cambridge).
Moffatt, H. K. (1978), Magnetic Field Generation in Electrically Conducting Fluids (Cambridge U. P., Cambridge).
Moreau, R. (1990), Magnetohydrodynamics ( Kluwer, Dordrecht).
Nakao, Y. (1997), Publ. Astron. Soc. Jpn. 49, 659.
Pouquet, A., Frisch, U., and Léorat, J. (1976), J. Fluid Mech. 77, 321.
Priest, E. (1982), Solar Magnetohydrodynamics (D. Reidel, Dordrecht).
Roberts, P. H. (1993), in Astrophysical Fluid Dynamics,edited by J. -P.
Zahn and J. Zinn-Justin (Elsevier, Amsterdam), p. 229.
Yoshizawa, A. (1985), Phys. Fluids 28, 3313.
Yoshizawa, A. (1990), Phys. Fluids B 2, 1589.
Yoshizawa, A. (1996), J. Phys. Soc. Jpn. 65, 124.
Yoshizawa, A. and Yokoi, N. (1996), Phys. Plasmas 3, 3604.
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Yoshizawa, A. (1998). Magnetohydrodynamic Turbulence Modeling. In: Hydrodynamic and Magnetohydrodynamic Turbulent Flows. Fluid Mechanics and Its Applications, vol 48. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1810-3_9
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DOI: https://doi.org/10.1007/978-94-017-1810-3_9
Publisher Name: Springer, Dordrecht
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