A solar‐wind “trigger” for the outer heliosphere radio emissions and the distance to the terminal shock
- 1 October 1988
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 15 (11) , 1307-1310
- https://doi.org/10.1029/gl015i011p01307
Abstract
No abstract availableThis publication has 19 references indexed in Scilit:
- Formation of a compound stream between 0.85 AU and 6.2 AU and its effects on solar energetic particles and galactic cosmic raysJournal of Geophysical Research, 1986
- The physical properties of the “local fluff”Advances In Space Research, 1986
- The solar wind shock terminationAdvances In Space Research, 1986
- Cosmic ray modulation and turbulent interaction regions near 11 AUJournal of Geophysical Research, 1985
- The solar windSolar Physics, 1985
- Persistence of shocks to large distances in the solar windJournal of Geophysical Research, 1985
- The plasma experiment on the 1977 Voyager MissionSpace Science Reviews, 1977
- Interaction of the interstellar medium with the solar windSpace Science Reviews, 1973
- Interplanetary neutral hydrogen and the radius of the heliospherePlanetary and Space Science, 1968
- Interplanetary Magnetic Fields and Cosmic RaysPhysical Review B, 1955