Three-Dimensional Morphology of Interfaces Driven by Rayleigh-Taylor or Richtmyer-Meshkov instability

Details Three-Dimensional Morphology of Interfaces Driven by Rayleigh-Taylor or Richtmyer-Meshkov instability Three-Dimensional Morphology of Interfaces Driven by Rayleigh-Taylor or Richtmyer-Meshkov instability

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..169t&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

After a presentation of the Rayleigh-Taylor instability, and its role in
the type II supernovae, I present original analytical work on the linear
phase of the IRT for compressible fluids, for constant or time variable
accelerations, and on the three-dimensional non-linear phase of the IRT
single modes. Comparisons with numerical simulations are discussed.

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