Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.275..285j&link_type=abstract
Astrophysics and Space Science, v. 275, Issue 3, p. 285-297 (2001).
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
Two theoretical models, spherical and cylindrical, of propagation of shock waves with varying energy in a rotating, magneto-radiative, self-gravitating non-uniform atmosphere have been developed. Subsequently, a comparison between the two models has been drawn with the aid of variation of flow variables with distance graphically. Significant is the difference between two models, when one observes the variations of radial velocity, pressure, mass, radiation flux, magnetic field and energy with distance. Also, the respective influences of radiation flux, magnetic field and rotational velocity on the variations of the flow variables have been studied.
Ganguly Ashok
Jana Mrinal
No associations
LandOfFree
A Comparative study between two models of propagation of spherical and cylindrical shock waves with varying energy in self-gravitating, magneto-radiative non-uniform atmosphere 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 A Comparative study between two models of propagation of spherical and cylindrical shock waves with varying energy in self-gravitating, magneto-radiative non-uniform atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Comparative study between two models of propagation of spherical and cylindrical shock waves with varying energy in self-gravitating, magneto-radiative non-uniform atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1712524