The time development of a blast wave with shock-heated electrons

Details The time development of a blast wave with shock-heated electrons The time development of a blast wave with shock-heated electrons

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..833e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 283, Aug. 15, 1984, p. 833-841. Previously announced in STAR as N84-17529.

Computer Science

Numerical Analysis

9

Numerical Analysis, Pressure Effects, Shock Heating, Shock Waves, Supernovae, Adiabatic Conditions, Density Distribution, Electron Energy, Energy Conservation, Temperature Effects

Scientific paper

Accurate approximations are presented for the time development of both edge conditions and internal structures of a blast wave with shock heated electrons, and equal ion and electron temperatures at the shock. The cases considered evolve in cavities with power law ambient densities (including the uniform ambient density case) and have negligible external pressure. Account is taken of possible saturation of the thermal conduction flux. The structures evolve smoothly to the adiabatic structures.

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