Waves, structures, and the appearance of two‐component turbulence in the solar wind
- 1 October 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (A10) , 23705-23715
- https://doi.org/10.1029/98ja02194
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- The evolution of slab fluctuations in the presence of pressure‐balanced magnetic structures and velocity shearsJournal of Geophysical Research, 1998
- Anisotropy in Hall MHD turbulence due to a mean magnetic fieldJournal of Plasma Physics, 1997
- 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
- Nonlinear evolution of a large‐amplitude circularly polarized Alfvén wave: Low betaJournal of Geophysical Research, 1994
- Proton and electron mean free paths: The Palmer consensus revisitedThe Astrophysical Journal, 1994
- MHD TURBULENCE: THEORY/SIMULATIONSPublished by Elsevier ,1992
- Evidence for the presence of quasi‐two‐dimensional nearly incompressible fluctuations in the solar windJournal of Geophysical Research, 1990
- An interplanetary magnetic field ensemble at 1 AUJournal of Geophysical Research, 1986
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971