The evolution of slab fluctuations in the presence of pressure‐balanced magnetic structures and velocity shears
- 1 October 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (A10) , 23691-23704
- https://doi.org/10.1029/98ja02195
Abstract
No abstract availableKeywords
This publication has 42 references indexed in Scilit:
- Cross‐helicity and residual energy in solar wind turbulence: Radial evolution and latitudinal dependence in the region from 1 to 5 AUJournal of Geophysical Research, 1998
- Dominant two‐dimensional solar wind turbulence with implications for cosmic ray transportJournal of Geophysical Research, 1996
- A model for the three‐dimensional magnetic field correlation spectra of low‐frequency solar wind fluctuations during Alfvénic periodsJournal of Geophysical Research, 1995
- Self-similar decay of three-dimensional homogeneous turbulence with hyperviscosityPhysical Review E, 1995
- Origin of low cross‐helicity regions in the inner solar windJournal of Geophysical Research, 1991
- Interplanetary Alfvénic fluctuations: A stochastic modelJournal of Geophysical Research, 1981
- Alfvén wave refraction by interplanetary inhomogeneitiesJournal of Geophysical Research, 1973
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971
- Magnetic and thermal pressures in the solar windSolar Physics, 1970
- Turbulence, Viscosity, and Dissipation in the Solar-Wind PlasmaThe Astrophysical Journal, 1968