Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap%26ss.274..293b&link_type=abstract
Astrophysics and Space Science, v. 274, Issue 1/2, p. 293-298 (2000).
Astronomy and Astrophysics
Astrophysics
Scientific paper
For the 1D radial hypersonic flow the development of the configuration with two shocks and contact discontinuity is considered. At small and large moments of time solutions in explicit form are found. As follows from these solutions the contact surface accelerates in time. This acceleration makes possible the Rayleigh-Taylor instability to develop. The 2D numerical investigation of the problem has confirmed the instability of the 1D solution.
Belov Nikolai A.
Myasnikov Artyom V.
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