On the role of plasma parameters and the Kelvin-Helmholtz instability in a viscous interaction of solar wind streams
- 1 September 1984
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 32 (9) , 1169-1178
- https://doi.org/10.1016/0032-0633(84)90142-9
Abstract
No abstract availableKeywords
This publication has 24 references indexed in Scilit:
- Coronal streamers in the solar wind at 1 AUJournal of Geophysical Research, 1981
- The solar origins of solar wind interstream flows: Near‐equatorial coronal streamersJournal of Geophysical Research, 1981
- Solar wind helium and hydrogen structure near the heliospheric current sheet: A signal of coronal streamers at 1 AUJournal of Geophysical Research, 1981
- Fine‐scale characteristics of interplanetary sector boundariesJournal of Geophysical Research, 1981
- Magnetic fields, plasmas, and coronal holes: The inner solar systemSpace Science Reviews, 1979
- Coronal magnetic fieldsSolar Physics, 1978
- Solar wind stream evolution at large heliocentric distances: Experimental demonstration and the test of a modelJournal of Geophysical Research, 1976
- Columnar content measurements of the solar-wind turbulence near the sunThe Astrophysical Journal, 1975
- Kelvin-Helmholtz instability of anisotropic plasma in a magnetic fieldJournal of Plasma Physics, 1975
- Magnetic fields and the structure of the solar coronaSolar Physics, 1969