Diagnostics of the Non-Linear Richtmyer-Meshkov Instability

Details Diagnostics of the Non-Linear Richtmyer-Meshkov Instability Diagnostics of the Non-Linear Richtmyer-Meshkov Instability

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.307..251h&link_type=abstract

Astrophysics and Space Science, Volume 307, Issue 1-3, pp. 251-255

Astronomy and Astrophysics

Astrophysics

Richtmyer-Meshkov, Supernovae, Diagnostics, Similarity, Multi-Scale Dynamics

Scientific paper

We study analytically and numerically the evolution of the two-dimensional coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability (RMI) for fluids with a finite density ratio. New diagnostics and scalings are suggested for accurate quantification of RMI dynamics. New similarity features of the late-time instability evolution are observed. The results obtained can serve as benchmarks for high energy density laboratory experiments.

Affiliated with

Also associated with

No associations

Rating

Diagnostics of the Non-Linear Richtmyer-Meshkov Instability 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 Diagnostics of the Non-Linear Richtmyer-Meshkov Instability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diagnostics of the Non-Linear Richtmyer-Meshkov Instability will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1363857