Nonstationary interaction of supersonic inviscid gas flows

Autor:	Yu. N. Sadkov
Rok vydání:	1997
Předmět:	Physics Computational Mathematics Solar wind Discontinuity (linguistics) Flow (mathematics) Inviscid flow Convergence (routing) Astrophysics::Solar and Stellar Astrophysics Supersonic speed Mechanics Divergence (statistics) Stability (probability) Astrophysics::Galaxy Astrophysics
Zdroj:	Computational Mathematics and Modeling. 8:161-164
ISSN:	1573-837X 1046-283X
DOI:	10.1007/bf02405167
Popis:	We consider the flow of supersonic homogeneous gas past a supersonic spherical source. This problem provides a gas-dynamic model of the interaction of interstellar wind with solar wind, and is thus also of independent interest. It is solved using an explicit through divergence scheme of third-order approximation. The analysis focuses on formation and stability of the structure of discontinuity surfaces and convergence to the stationary solution. The results are compared qualitatively and quantitatively with solutions obtained by other methods.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::8d8561e6935a4cf7deb8876c14382326 https://doi.org/10.1007/bf02405167 Zobrazit plný text záznamu Full text from SpringerLink