The equilibrium state of shock-heated rotating atmosphere under the force of gravitation

DOI10.1007/BF00639722zbMath0673.76083OpenAlexW2055515511MaRDI QIDQ1121111

Onkar Nath

Publication date: 1989

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00639722

zbMATH Keywords

shock wavecylindrical shock wavesconstant shock-strength hypothesisflow of a rotating atmosphereforce of gravitationouter solar atmospheresteady mass motion

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05) Basic methods in fluid mechanics (76M99) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• SIMILARITY FLOWS BEHIND STRONG SHOCK WAVES
• Unnamed Item

This page was built for publication: The equilibrium state of shock-heated rotating atmosphere under the force of gravitation