Solutions of the two-fluid solar wind equations - Adiabatic and conduction dominated solutions

Details Solutions of the two-fluid solar wind equations - Adiabatic and conduction dominated solutions Solutions of the two-fluid solar wind equations - Adiabatic and conduction dominated solutions

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...74..169r&link_type=abstract

(ESA and European Physical Society, ESLAB Symposium on Physics of Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-19

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1

Adiabatic Conditions, Solar Wind, Two Fluid Models, Asymptotic Methods, Computational Fluid Dynamics, Electron Energy, Solar Protons

Scientific paper

The equations governing the two-fluid spherically symmetric models of the solar wind have been solved numerically for a wide range of base conditions. As predicted from an asymptotic analysis we find a whole domain of solutions which are asymptotically adiabatic with the proton and electron temperatures tending to equality and varying like r-4/3. In these 4/3 solutions the electron and proton heat conduction is asymptotically negligible and if it is neglected the resulting equations can be integrated analytically and shown to have the 4/3, 4/3 behaviour.

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