ON THE ORIGIN OF SOLAR WIND TURBULENCE: HELIOS DATA REVISITED
Authors:
- Roland GrappinRGRoland Grappin
- André MangeneyAMAndré Mangeney
- Eckhard MarschEMEckhard Marsch
- 1 January 1989
- book chapter
- Published by Elsevier
- p. 81-86
Abstract
No abstract availableThis publication has 11 references indexed in Scilit:
- Onset and decay of two-dimensional magnetohydrodynamic turbulence with velocity–magnetic field correlationThe Physics of Fluids, 1986
- Growth of correlations in magnetohydrodynamic turbulencePhysical Review A, 1986
- The power spectrum of interplanetary Alfvénic fluctuations: Derivation of the governing equation and its solutionJournal of Geophysical Research, 1984
- Turbulent Generation of Outward-Traveling Interplanetary Alfvénic FluctuationsPhysical Review Letters, 1983
- Radial evolution of power spectra of interplanetary Alfvénic turbulenceJournal of Geophysical Research, 1982
- Statistical properties of low‐frequency magnetic field fluctuations in the solar wind from 0.29 to 1.0 AU during solar minimum conditions: HELIOS 1 and HELIOS 2Journal of Geophysical Research, 1982
- Fully Developed Anisotropic Hydromagnetic Turbulence in Interplanetary SpacePhysical Review Letters, 1980
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971
- Turbulence, Viscosity, and Dissipation in the Solar-Wind PlasmaThe Astrophysical Journal, 1968
- Inertial-Range Spectrum of Hydromagnetic TurbulenceThe Physics of Fluids, 1965