The nebular shock wave model for chondrule formation - One-dimensional calculations

Details The nebular shock wave model for chondrule formation - One-dimensional calculations The nebular shock wave model for chondrule formation - One-dimensional calculations

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106..179h&link_type=abstract

Icarus, vol. 106, p. 179

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51

Shock Waves, Nebulae, Chondrule, Solar Corona, Interplanetary Dust, Meteorites, Gas Dynamics, Grain Size, Mach Number

Scientific paper

Numerical simulations are conducted for the interactions of a 1D, radiative, gasdynamic shock wave with a solar nebula dust cloud that is dimensionally finite in the direction parallel to shock propagation. Time-step computations are conducted for energy and momentum transfer to the shock-heated gas as it penetrates the dust cloud, in conjunction with computations of the grain heating due to molecular collisions and radiation from shocked gas and surrounding dust grains.

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