Persistence of shocks to large distances in the solar wind
- 1 May 1985
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 90 (A5) , 3967-3972
- https://doi.org/10.1029/ja090ia05p03967
Abstract
No abstract availableKeywords
This publication has 7 references indexed in Scilit:
- The far reaches of the solar wind - Pioneer 10 and Pioneer 11 plasma resultsThe Astrophysical Journal, 1984
- The forward‐reverse shock pair at large heliocentric distancesJournal of Geophysical Research, 1984
- Shock acceleration of nuclei and electrons in the heliosphere beyond 24 AUThe Astrophysical Journal, 1984
- Dynamical evolution of interplanetary magnetic fields and flows between 0.3 AU and 8.5 AU: EntrainmentGeophysical Research Letters, 1983
- Dynamic MHD modeling of solar wind corotating stream interaction regions observed by Pioneer 10 and 11Journal of Geophysical Research, 1978
- Solar wind stream evolution at large heliocentric distances: Experimental demonstration and the test of a modelJournal of Geophysical Research, 1976
- Evolution of large-scale solar wind structures beyond 1 AUPublished by American Geophysical Union (AGU) ,1973