Cross‐helicity and residual energy in solar wind turbulence: Radial evolution and latitudinal dependence in the region from 1 to 5 AU
Open Access
- 1 April 1998
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (A4) , 6521-6529
- https://doi.org/10.1029/97ja03029
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- On the “inward” component of the Alfvénic turbulence in the solar windJournal of Geophysical Research, 1997
- Implications of fluctuations in the distribution functions of interstellar pick‐up ions for the scattering of low rigidity particlesGeophysical Research Letters, 1997
- Properties of magnetohydrodynamic turbulence in the solar wind as observed by Ulysses at high heliographic latitudesGeophysical Research Letters, 1995
- Alfvén waves, alpha particles, and pickup ions in the solar windGeophysical Research Letters, 1995
- Observations of evolving turbulence in the polar solar windGeophysical Research Letters, 1995
- Magnetohydrodynamic Turbulence in the Solar WindAnnual Review of Astronomy and Astrophysics, 1995
- Ulysses at 50° south: constant immersion in the high‐speed solar windGeophysical Research Letters, 1994
- Origin of low cross‐helicity regions in the inner solar windJournal of Geophysical Research, 1991
- Radial variation of interplanetary Alfvénic fluctuations: Pioneer 10 and 11 observations between 1 and 5 AUJournal of Geophysical Research, 1986
- Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar windJournal of Geophysical Research, 1982