Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179..177b&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 2, May 1991, p. 177-188.
Astronomy and Astrophysics
Astrophysics
High Temperature Gases, Hypersonic Flow, Magnetohydrodynamic Waves, Optical Thickness, Shock Waves, Asymptotic Methods, Differential Equations
Scientific paper
The present study examines the structure of a hydromagnetic shock wave which is so strong that downstream of the shock the gas radiates thermally. The general differential approximation for radiation is invoked and the solution is compared with that in a paper by Bestman (1990) for an optically thick gas. The radiative flux was found to play a dominant role in the solution, and the shock structure for the general differential approximation is broadened by radiation far more than the case of optically thick gas.
No associations
LandOfFree
Hydromagnetic shock structure in high temperature hypersonic flow does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Hydromagnetic shock structure in high temperature hypersonic flow, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydromagnetic shock structure in high temperature hypersonic flow will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1036083