Evidence for the presence of quasi‐two‐dimensional nearly incompressible fluctuations in the solar wind
- 1 December 1990
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 95 (A12) , 20673-20683
- https://doi.org/10.1029/ja095ia12p20673
Abstract
No abstract availableKeywords
This publication has 54 references indexed in Scilit:
- Observations of field-aligned density fluctuations in the inner solar windThe Astrophysical Journal, 1990
- Cosmic-ray pitch-angle scattering in isotropic turbulenceThe Astrophysical Journal, 1988
- Pitch angle distributions of solar energetic particles and the local scattering properties of the interplanetary mediumThe Astrophysical Journal, 1986
- MHD processes in the outer heliosphereSpace Science Reviews, 1984
- Radial evolution of power spectra of interplanetary Alfvénic turbulenceJournal of Geophysical Research, 1982
- Interplanetary Alfvénic fluctuations: A stochastic modelJournal of Geophysical Research, 1981
- On the polarization state of hydromagnetic fluctuations in the solar windJournal of Geophysical Research, 1981
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971
- Collisionless Heating of the Solar-Wind Plasma. II. Application of the Theory of Plasma Heating by Hydromagnetic WavesThe Astrophysical Journal, 1969
- Micro-scale structures in the interplanetary mediumSolar Physics, 1968