NASA NTRS · 19920036959
Structure and evolution of time-dependent intermediate shocks
Abstract
A quantitative description of time-dependent intermediate shocks is formulated using the Cohen-Kulsrud-Burgers equations. In noncoplanar Riemann problems, time-dependent two-three transition intermediate shocks evolve in time as a localized self-similar structure whose strength decreases as 1/the square root of t, and whose width expands as the square root of t. Time-dependent intermediate shocks offer a way of solving the noncoplanar MHD Riemann problem.
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Wu, C. C., Kennel, C. F.. 1992-01-06. Structure and evolution of time-dependent intermediate shocks. https://ntrs.nasa.gov/citations/19920036959
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