Steady state and dynamical structure of a cosmic‐ray‐modified termination shock
- 1 November 1993
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 98 (A11) , 19005-19025
- https://doi.org/10.1029/93ja01948
Abstract
No abstract availableKeywords
This publication has 40 references indexed in Scilit:
- The stability of cosmic-ray-dominated shocks - A secondary instabilityThe Astrophysical Journal, 1993
- Cosmic-ray-modified supernova remnant shocksThe Astrophysical Journal, 1992
- Propagation of a large Forbush decrease in cosmic‐ray intensity past the Earth, Pioneer 11 at 34 AU, and Pioneer 10 at 53 AUGeophysical Research Letters, 1992
- Constraints on the acceleration of anomalous cosmic raysThe Astrophysical Journal, 1992
- The plasma physics of shock accelerationSpace Science Reviews, 1991
- Forbush decreases and particle acceleration in the outer heliosphereGeophysical Research Letters, 1990
- Frequency drift of 3-kHz interplanetary radio emissions: evidence of Fermi accelerated trapped radiation in a small heliosphere?Nature, 1990
- Detection of a radio emission at 3 kHz in the outer heliosphereNature, 1984
- An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmasReports on Progress in Physics, 1983
- Solar wind and interplanetary magnetic fieldReviews of Geophysics, 1967