Development of solar wind shock models with tensor plasma pressure for data analysis

Details Development of solar wind shock models with tensor plasma pressure for data analysis Development of solar wind shock models with tensor plasma pressure for data analysis

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975wusl.rept.....a&link_type=abstract

Final Technical Report, 1 Aug. 1970 - 31 Dec. 1975 Washington Univ., Saint Louis, MO. Dept. of Electrical Engineering.

Physics

Data Processing, Mathematical Models, Plasma Pressure, Plasmas (Physics), Shock Waves, Solar Wind, Pioneer 6 Space Probe, Pioneer 7 Space Probe, Pioneer 8 Space Probe, Pioneer 9 Space Probe, Pressure Effects

Scientific paper

The development of solar wind shock models with tensor plasma pressure and the comparison of some of the shock models with the satellite data from Pioneer 6 through Pioneer 9 are reported. Theoretically, difficulties were found in non-turbulent fluid shock models for tensor pressure plasmas. For microscopic shock theories nonlinear growth caused by plasma instabilities was frequently not clearly demonstrated to lead to the formation of a shock. As a result no clear choice for a shock model for the bow shock or interplanetary tensor pressure shocks emerged.

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