A numerical study of the evolution of the solar wind from Ulysses to Voyager 2
- 1 February 2000
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 105 (A2) , 2337-2344
- https://doi.org/10.1029/1999ja900436
Abstract
No abstract availableKeywords
This publication has 24 references indexed in Scilit:
- The Piecewise Parabolic Method (PPM) for gas-dynamical simulationsPublished by Elsevier ,2004
- Properties of the interstellar gas inside the heliosphereSpace Science Reviews, 1996
- A Simple Riemann Solver and High-Order Godunov Schemes for Hyperbolic Systems of Conservation LawsJournal of Computational Physics, 1995
- Detection of Interstellar Pick-Up Hydrogen in the Solar SystemScience, 1993
- Stream dynamics between 1 AU and 2 AU: A comparison of observations and theoryJournal of Geophysical Research, 1985
- Voyager observations of solar wind proton temperature: 1‐10AUGeophysical Research Letters, 1982
- Dynamic MHD modeling of solar wind corotating stream interaction regions observed by Pioneer 10 and 11Journal of Geophysical Research, 1978
- Effects of stream-associated fluctuations upon the radial variation of average solar wind parametersJournal of Geophysical Research, 1977
- Solar wind stream evolution at large heliocentric distances: Experimental demonstration and the test of a modelJournal of Geophysical Research, 1976
- Interaction of the solar wind with the neutral component of the interstellar gasJournal of Geophysical Research, 1972