Spatial structure of flare‐associated perturbations in the solar wind simulated by a two‐dimensional numerical MHD model
- 1 February 1981
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 86 (A2) , 525-534
- https://doi.org/10.1029/ja086ia02p00525
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- Numerical study of an explosion in a non-homogeneous medium with and without magnetic fieldsComputers & Fluids, 1979
- Dynamic MHD modeling of the solar wind disturbances during the August 1972 eventsJournal of Geophysical Research, 1978
- Energetic properties of interplanetary plasma at the earth's orbit following the August 4, 1972 flareSolar Physics, 1977
- MHD solution of interplanetary disturbances generated by simulated velocity perturbationsJournal of Geophysical Research, 1976
- Interplanetary disturbances caused by the August 1972 solar flares as observed by Pioneer 9Journal of Geophysical Research, 1976
- Interplanetary shock waves: Recent developmentsSpace Science Reviews, 1975
- Simulation of driven flare-associated disturbances in the solar windJournal of Geophysical Research, 1973
- Two-dimensional simulation of flare-associated disturbances in the solar windJournal of Geophysical Research, 1971
- Effects of solar flare duration on a double shock pair at 1 AUJournal of Geophysical Research, 1969
- A detached shock calculation by second-order finite differencesJournal of Computational Physics, 1967