Some Macroscopic Properties of Shock Waves in the Heliosphere
- 18 March 2013
- book chapter
- Published by Wiley in Geophysical Monograph Series
- Vol. 34, 37-58
- https://doi.org/10.1029/gm034p0037
Abstract
No abstract availableKeywords
This publication has 24 references indexed in Scilit:
- Self-similar solutions for the interaction regions of colliding windsThe Astrophysical Journal, 1983
- Self-similar solutions for the interaction of stellar ejecta with an external mediumThe Astrophysical Journal, 1982
- Self-similar magnetohydrodynamics. I - The gamma = 4/3 polytrope and the coronal transientThe Astrophysical Journal, 1982
- Self-Similar Solutions as Intermediate AsymptoticsAnnual Review of Fluid Mechanics, 1972
- Composition and dynamics of the solar wind plasmaReviews of Geophysics, 1970
- The structure of the solar plasma flow generated by solar flaresPlanetary and Space Science, 1967
- Shock waves in the interplanetary mediumPlanetary and Space Science, 1966
- The SI+-SI− pair and interplanetary forward-reverse shock ensemblesPlanetary and Space Science, 1965
- Sudden Expansion of the Corona Following a Large Solar Flare and the Attendant Magnetic Field and Cosmic-Ray Effects.The Astrophysical Journal, 1961
- Analytic Solutions for the Blast-Wave Problem with an Atmosphere of Varying Density.The Astrophysical Journal, 1957