65 pages matching interplanetary space in this book
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4He+ Alfven waves ambient solar wind angular momentum assumed assumption basic two-fluid model blast wave Burlaga chromosphere Class collisions component 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 flare ejecta flow speed fluid geomagnetic Hartle heat conduction flux helium abundance high-speed plasma streams high-speed streams hydrogen hydrostatic equilibrium implies indicated interplanetary magnetic field interplanetary plasma interplanetary shock waves interplanetary space ionization ions km sec-1 magnetic field lines magnetic sectors mass and energy one-fluid model Parker particle phenomena photospheric physical polarity polytropic post-shock predicted pressure produced propagation proton temperature radial ratio region scale shock front shock normal similar solar activity solar corona solar flares solar rotation solar wind disturbances solar wind observations solar wind properties solar wind speed solutions source surface spectral peak spherically-symmetric steady supersonic thermal conductivity variations velocity