The evolution of corotating stream fronts near the ecliptic plane in the inner solar system: 2. Three‐dimensional tilted‐dipole fronts
- 1 April 1991
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 96 (A4) , 5405-5420
- https://doi.org/10.1029/91ja00155
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Solar wind and coronal structure near sunspot minimum: Pioneer and SMM observations from 1985–1987Journal of Geophysical Research, 1990
- Pioneer and Voyager observations of the solar wind at large heliocentric distances and latitudesGeophysical Research Letters, 1989
- A three-dimensional, time-dependent numerical modeling of super-sonic, super-alfvénic MHD flowComputers & Fluids, 1988
- Determination of the solar wind angular momentum flux from the HELIOS data - an observational test of the Weber and Davis theoryThe Astrophysical Journal, 1983
- A three‐dimensional model of corotating streams in the solar wind: 3. Magnetohydrodynamic streamsJournal of Geophysical Research, 1982
- Three-dimensional aspects of interplanetary shock wavesJournal of Geophysical Research, 1976
- Restricted three-dimensional stellar wind modeling. I - Polytropic caseThe Astrophysical Journal, 1975
- Interplanetary stream interfacesJournal of Geophysical Research, 1974
- Compressible-Fluid DynamicsJournal of Applied Mechanics, 1972
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971