A model of solar wind fluctuations with two components: Alfvén waves and convective structures
- 1 February 1993
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 98 (A2) , 1257-1276
- https://doi.org/10.1029/92ja01947
Abstract
No abstract availableKeywords
This publication has 52 references indexed in Scilit:
- Magnetohydrodynamic simulation of the radial evolution and stream structure of solar-wind turbulencePhysical Review Letters, 1991
- Transfer equations for spectral densities of inhomogeneous MHD turbulenceJournal of Plasma Physics, 1990
- The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimumGeophysical Research Letters, 1990
- Turbulent cascade of incompressible unidirectional Alfvén waves in the interplanetary mediumPhysical Review Letters, 1989
- Dynamics of correlation functions with Elsässer variables for inhomogeneous MHD turbulenceJournal of Plasma Physics, 1989
- Nonlinear alfvénic fluctuations in uniform magnetic background fieldsGeophysical & Astrophysical Fluid Dynamics, 1988
- Anisotropy in MHD turbulence due to a mean magnetic fieldJournal of Plasma Physics, 1983
- Major Disruptions, Inverse Cascades, and the Strauss EquationsPhysica Scripta, 1982
- Fully Developed Anisotropic Hydromagnetic Turbulence in Interplanetary SpacePhysical Review Letters, 1980
- Turbulence, Viscosity, and Dissipation in the Solar-Wind PlasmaThe Astrophysical Journal, 1968