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Alfven waves ambient solar wind angular momentum anisotropic Astrophys Bame basic two-fluid model blast wave Burlaga chromosphere coronal density coronal expansion models coronal temperature coulomb collisions discussion electron and proton electron temperature emission energy flux density energy source energy-per-charge expansion speed flow speed fluid geomagnetic geomagnetic storms Geophys Hartle heat conduction flux helium abundance high-speed plasma streams high-speed streams Hundhausen hydrogen hydrostatic equilibrium implies integration interaction interplanetary magnetic field interplanetary plasma interplanetary shock waves interplanetary space ionization ions km sec-1 magnetic field lines magnetic sectors Ogilvie one-fluid model Parker particle phenomena photospheric physical planetary polarity post-shock predicted pressure produced propagation proton temperature radial region scale shock front solar activity solar corona solar flares Solar Phys solar rotation solar wind disturbances solar wind observations solar wind properties solar wind speed solutions source surface Space Sci spacecraft spectral peak spherically-symmetric steady structure thermal conductivity variations Vela velocity