Physical consistency in modeling interplanetary magnetohydrodynamic fluctuations

Details Physical consistency in modeling interplanetary magnetohydrodynamic fluctuations Physical consistency in modeling interplanetary magnetohydrodynamic fluctuations

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..64.2591z&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 64, May 21, 1990, p. 2591; Authors' Reply, p. 2592.

Astronomy and Astrophysics

Astronomy

8

Astronomical Models, Interplanetary Magnetic Fields, Magnetohydrodynamic Turbulence, Heliosphere, Magnetohydrodynamic Waves, Solar Wind, Wentzel-Kramer-Brillouin Method

Scientific paper

The validity of the Velli, Grappin and Mangeney (1989) model is evaluated. It is argued that the model is incorrect because it mixes different dynamical models, assumes weak nonlinearities, makes predictions that vary with observations, and violates causality. It is proposed that self-similar behavior in the coronal source region of the magnetohydrodynamic fluctuations cause the Kolmogorov-like spectra.

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