Three-Dimensional, Time-Dependent, MHD Model of a Solar Flare-Generated Interplanetary Shock Wave
- 1 January 1986
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Interplanetary disturbances produced by a simulated solar flare and equatorially-fluctuating heliospheric current sheetAstrophysics and Space Science, 1984
- Magnetohydrodynamic modelling of interplanetary disturbances between the Sun and EarthAstrophysics and Space Science, 1984
- Radio-scintillation observations of interplanetary disturbancesAdvances in Space Research, 1984
- Non-planar mhd model for solar flare-generated disturbances in the heliospheric equatorial planeSolar Physics, 1983
- The observation of a coronal transient directed at earthThe Astrophysical Journal, 1982
- A three‐dimensional model of corotating streams in the solar wind: 3. Magnetohydrodynamic streamsJournal of Geophysical Research, 1982
- Meridional flow in the solar wind in the presence of latitudinally dependent boundary conditionsSolar Physics, 1975
- Radio Evidence for the Propagation of Magnetohydrodynamic Waves along Curved Paths in the Solar CoronaPublications of the Astronomical Society of Australia, 1969