Coronal Expansion and Solar Wind |
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¹H+ Alfvén speed Alfvén waves ambient solar wind angular momentum anisotropy assumed assumption Astrophys average Bame basic two-fluid model Burlaga chromosphere component configuration coronal density coronal expansion models coronal temperature coulomb collisions discussion electron and proton electron temperature emission energy equation energy source energy-per-charge ergs expansion speed flow speed fluid geomagnetic Geophys Hartle heat conduction flux helium abundance high-speed plasma streams high-speed streams Hundhausen hydrogen implies interplanetary magnetic field interplanetary plasma interplanetary shock waves interplanetary space ionization ions km sec km sec-1 magnetic field lines magnetic force magnetosonic waves mass momentum equation nonradial one-fluid model particle photospheric physical polarity polytropic predicted produced propagation proton temperature protons and electrons r=ro radial ratio region scale sec¹ shock front solar corona solar flares Solar Phys SOLAR RADII solar rotation solar wind observations solar wind properties solar wind speed solutions spacecraft spectral peak spherically-symmetric thermal conductivity variations Vela velocity viscosity