Shock waves data for minerals

Details Shock waves data for minerals Shock waves data for minerals

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9613350a&link_type=abstract

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Computer Science

Sound

Hugoniot Equation Of State, Minerals, Phase Transformations, Planetary Composition, Planetary Geology, Shock Heating, Shock Wave Propagation, Shock Waves, Acoustic Velocity, Meteorite Collisions, Shock Loads, Tables (Data), Wave Equations

Scientific paper

Shock compression of the materials of planetary interiors yields data which upon comparison with density-pressure and density-sound velocity profiles constrain internal composition and temperature. Other important applications of shock wave data and related properties are found in the impact mechanics of terrestrial planets and solid satellites. Shock wave equation of state, shock-induced dynamic yielding and phase transitions, and shock temperature are discussed. In regions where a substantial phase change in the material does not occur, the relationship between the particle velocity, Up, and the shock velocity, Us, is given by Us = C0 + S Up, where C0 is the shock velocity at infinitesimally small particle velocity, or the ambient pressure bulk sound velocity. Numerical values for the shock wave equation of state for minerals and related materials of the solar system are provided.

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