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8
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85034286962
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Recall that the derivation (Ref. 6) of the Strauss equations explicitly excludes the presence of an initial O(1) population of Alfvén waves. However, if they exist, simulations (Refs. 11 and 17) show that evolution proceeds in such a way as to make the Stauss equations an increasingly valid approximation
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Recall that the derivation (Ref. 6) of the Strauss equations explicitly excludes the presence of an initial O(1) population of Alfvén waves. However, if they exist, simulations (Refs. 11 and 17) show that evolution proceeds in such a way as to make the Stauss equations an increasingly valid approximation.
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-
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16
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0007011271
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W. H. Matthaeus, L. W. Klein, S. Ghosh, and M. R. Brown, J. Geophys. Res. 96, 5421 (1991).
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(1991)
J. Geophys. Res.
, vol.96
, pp. 5421
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-
Matthaeus, W.H.1
Klein, L.W.2
Ghosh, S.3
Brown, M.R.4
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18
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0000640106
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W. H. Matthaeus, S. Ghosh, S. Oughton, and D. A. Roberts, J. Geophys. Res. 101, 7619 (1996).
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(1996)
J. Geophys. Res.
, vol.101
, pp. 7619
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Matthaeus, W.H.1
Ghosh, S.2
Oughton, S.3
Roberts, D.A.4
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27
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85034301901
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0. This is usually explained in terms of the Alfvén effect (Ref. 41)
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0. This is usually explained in terms of the Alfvén effect (Ref. 41).
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-
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29
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85034295878
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-
note
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1)2〉, and for isotropic turbulence this is equal to 5E/Ω (Ref. 28). Since we are primarily interested in the scaling properties, and also we cannot invoke isotropy, we have elected to drop the associated numerical factors here.
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31
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85034301541
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Note that the two cases are analogous to the cases considered in Ref. 13, in which the discussion is couched entirely in terms of RMHD
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Note that the two cases are analogous to the cases considered in Ref. 13, in which the discussion is couched entirely in terms of RMHD.
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32
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85034302826
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Pergamon, Oxford, UK
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M. Hossain, P. C. Gray, D. H. Pontius, Jr., W. H. Matthaeus, and S. Oughton, in Proceedings of Solar Wind 8, COSPAR Colloquia Series (Pergamon, Oxford, UK, 1996).
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(1996)
Proceedings of Solar Wind 8, COSPAR Colloquia Series
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Hossain, M.1
Gray, P.C.2
Pontius Jr., D.H.3
Matthaeus, W.H.4
Oughton, S.5
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33
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0001626979
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M. Hossain, P. C. Gray, D. H. Pontius, Jr., W. H. Matthaeus, and S. Oughton, Phys. Fluids 7, 2886 (1995).
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(1995)
Phys. Fluids
, vol.7
, pp. 2886
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Hossain, M.1
Gray, P.C.2
Pontius Jr., D.H.3
Matthaeus, W.H.4
Oughton, S.5
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34
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0004044780
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Nijhoff, Dordrecht, The Netherlands
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M. Lesieur, Turbulence in Fluids (Nijhoff, Dordrecht, The Netherlands, 1990).
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(1990)
Turbulence in Fluids
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-
Lesieur, M.1
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39
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85034280066
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See also Ref. 36 but note that the ICs in their simulations are not isotropic, so that it is difficult to say whether the observed anisotropy is a consequence of the initial data, nonlinear evolution, or perhaps both factors
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See also Ref. 36 but note that the ICs in their simulations are not isotropic, so that it is difficult to say whether the observed anisotropy is a consequence of the initial data, nonlinear evolution, or perhaps both factors,
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