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《Chinese Journal of Geophysics》 1990-03
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NUMERICAL STUDY ON PROPERTIES OF TWO-FLUID FIVE-MOMENT SOLAR WIND PLASMAS

WANG JING-FANG JIANG XIN-YING XIONG DONG-HUI(Department of space physics, Wuhan University)  
The variation with radial distance of partl;le density streaming velocity, temperature (T), heat flux (q) and excess (ζ) of non-Maxwellian tail particles in the electron and proton steady solar wind is numerically investigated by using spherically symmetric time-dependent five-moment fluid equations. The effects ofζ 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 ζ can reduce the gap between observations and computations of Te/TP and qe/qp.
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