Three-component gas-dynamic model of the interaction of the solar wind with the interstellar medium
- 1 January 1983
- journal article
- Published by Springer Nature in Fluid Dynamics
- Vol. 17 (5) , 754-759
- https://doi.org/10.1007/bf01090158
Abstract
No abstract availableKeywords
This publication has 2 references indexed in Scilit:
- Structure of the region of solar wind?Interstellar medium interaction and its influence on H atoms penetrating the solar windAstrophysics and Space Science, 1979
- Local interstellar mediumNature, 1975