Conductive Heating of the Solar Wind. I.

摘要: The hydrodynamic equations for the solar corona with no external heat source beyond a thin shell are solved case of fast expansion. is assumed to be approximately 10 per cent ionized helium, and Chapman value unihibited thermal conductivity can used everywhere. integrated, from earth sun, on an IBM 7090 computer, power series expansion in neighborhood singularity at r/sub c/, where kT(r/sub c/) = mu/sup 2/(r/sub c/). It found that conduction naturally supplies sufficient heating accelerate particles observed wind flux near earth, if inner coronal densities accepted values, base temperature 2 x 10/sup 6/ deg K. stabilization effects associated viscosity magnetic field examined. (auth)