-
4
-
-
85037223575
-
-
C. Heiles, A. Goodman, C. McKee, and E. Zweibel, Protostars and Planets IV, edited by D. Black and M. Matthews (University of Arizona Press, Tucson, 1993); p. 279;
-
C. Heiles, A. Goodman, C. McKee, and E. Zweibel, Protostars and Planets IV, edited by D. Black and M. Matthews (University of Arizona Press, Tucson, 1993); p. 279;
-
-
-
-
8
-
-
0000750541
-
-
A. Ruzmaikin, J. Feynman, B. Goldstein, and E. Smith, J. Geophys. Res. 100, 3395 (1995).
-
(1995)
J. Geophys. Res.
, vol.100
, pp. 3395
-
-
Ruzmaikin, A.1
Feynman, J.2
Goldstein, B.3
Smith, E.4
-
16
-
-
0029656766
-
-
A. Brandenburg, R. Jennings, A. Nordlund, M. Rieutord, R. Stein, and I. Tuominen, J. Fluid Mech. 306, 325 (1996);
-
(1996)
J. Fluid Mech.
, vol.306
, pp. 325
-
-
Brandenburg, A.1
Jennings, R.2
Nordlund, A.3
Rieutord, M.4
Stein, R.5
Tuominen, I.6
-
23
-
-
85037187110
-
-
see also CNRS-MFGA Workshop, edited by D. Schertzer and E. Falgarone (Paris, 1995) (unpublished)
-
see also CNRS-MFGA Workshop, edited by D. Schertzer and E. Falgarone (Paris, 1995) (unpublished).
-
-
-
-
31
-
-
85037222654
-
-
Note that [Formula Presented] for example when the variation on a third dimension is assumed negligible and all [Formula Presented] components of the vector fields are kept
-
Note that d*≠d, for example when the variation on a third dimension is assumed negligible and all d* components of the vector fields are kept.
-
-
-
-
32
-
-
85037229249
-
-
Such laws do not apply in the case of exact solutions to the MHD equations like Alfvén waves [Formula Presented] which render the nonlinear terms exactly equal to zero (except for the pressure), and cannot be considered within the present framework, since this analysis stems from the existence of a nonzero transfer of energy to small scales
-
Such laws do not apply in the case of exact solutions to the MHD equations like Alfvén waves v=±b, which render the nonlinear terms exactly equal to zero (except for the pressure), and cannot be considered within the present framework, since this analysis stems from the existence of a nonzero transfer of energy to small scales.
-
-
-
-
33
-
-
0007454831
-
-
Cambridge University Press, Cambridge, H. K. Moffatt, A. Tsinober
-
H. Politano, P. L. Sulem, and A. Pouquet, in Topological Fluid Mechanics, edited by H. K. Moffatt and A. Tsinober (Cambridge University Press, Cambridge, 1990);
-
(1990)
Topological Fluid Mechanics
-
-
Politano, H.1
Sulem, P.L.2
Pouquet, A.3
-
34
-
-
0029690493
-
-
M. Meneguzzi, H. Politano, A. Pouquet, and M. Zolver, J. Comput. Phys. 123, 32 (1996).
-
(1996)
J. Comput. Phys.
, vol.123
, pp. 32
-
-
Meneguzzi, M.1
Politano, H.2
Pouquet, A.3
Zolver, M.4
-
36
-
-
85037224995
-
-
Whether the intermittency corrections for higher-order functions are also dependent on the amount of global correlation remains an open, interesting problem
-
Whether the intermittency corrections for higher-order functions are also dependent on the amount of global correlation remains an open, interesting problem.
-
-
-
-
40
-
-
0002894412
-
-
R. Benzi, S. Ciliberto, R. Tripiccione, C. Baudet, F. Massaioli, and S. Succi, Phys. Rev. E 48, R29 (1993).
-
(1993)
Phys. Rev. E
, vol.48
-
-
Benzi, R.1
Ciliberto, S.2
Tripiccione, R.3
Baudet, C.4
Massaioli, F.5
Succi, S.6
-
45
-
-
0000594570
-
-
M. Medvedev, V. Shevchenko, P. Diamond, and P. V. Galinsky, Phys. Plasmas 4, 1257 (1997).
-
(1997)
Phys. Plasmas
, vol.4
, pp. 1257
-
-
Medvedev, M.1
Shevchenko, V.2
Diamond, P.3
Galinsky, P.V.4
|