A three‐dimensional model of corotating streams in the solar wind, 1. Theoretical foundations
- 1 December 1978
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 83 (A12) , 5563-5572
- https://doi.org/10.1029/ja083ia12p05563
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Numerical solution of the interaction of a shock wave with a laminar boundary layerPublished by Springer Nature ,2008
- Solar wind stream interfacesJournal of Geophysical Research, 1978
- Effects of stream-associated fluctuations upon the radial variation of average solar wind parametersJournal of Geophysical Research, 1977
- MHD solution of interplanetary disturbances generated by simulated velocity perturbationsJournal of Geophysical Research, 1976
- Solar wind stream evolution at large heliocentric distances: Experimental demonstration and the test of a modelJournal of Geophysical Research, 1976
- Three-dimensional interplanetary stream magnetism and energetic particle motionJournal of Geophysical Research, 1976
- Solar wind structure at large heliocentric distances: An interpretation of Pioneer 10 observationsJournal of Geophysical Research, 1976
- Numerical studies of azimuthal modulations of the solar wind with magnetic fieldsSolar Physics, 1973
- Nonlinear model of high-speed solar wind streamsPublished by American Geophysical Union (AGU) ,1973
- Compressions and rarefactions in the solar wind: Vela 3Journal of Geophysical Research, 1972