Numerical study on properties of two-fluid five-moment solar wind plasmas.

Details Numerical study on properties of two-fluid five-moment solar wind plasmas. Numerical study on properties of two-fluid five-moment solar wind plasmas.

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acgsn..33..259w&link_type=abstract

Acta Geophys. Sin., Vol. 33, No. 3, p. 259 - 266

Statistics

Computation

Solar Wind: Plasma

Scientific paper

The variation with radial distance of particle density streaming velocity, temperature, heat flux and excess (ξ) of non-Maxwellian tail particles in the electron and proton steady solar wind is numerically investigated bt using spherically symmetric time-dependent five-moment fluid equations. The effects of ξ on the temperature and heat flux of protons are given special attention. The comparison of those plasma properties of the two-fluid solar wind between five-moment and four-moment models indicates that the moment equation of ξ can reduce the gap between observations and computations.

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