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• W2006183863 abstract "This paper studies the global solar wind between 1 AU and the termination shock, taking into account the highly latitude dependent solar wind at the 1 AU boundary and the ionization of interstellar neutral hydrogen. A system of two-fluid magnetohydrodynamics equations governs the flow of solar wind plasma; the conditions of the solar wind at 1 AU are generated from Ulysses data for the relatively stable state of the wind during the declining phase and solar minimum of the solar cycle. A one-fluid model is used to describe the flow of neutral hydrogen and its condition in the far-field boundary outside the termination shock. Simultaneous solutions are obtained using a high-resolution computational code for the two equation systems coupled by the ionization of neutral hydrogen. The ionization process leads to removal of neutral hydrogen in the heliosphere: a hydrogen cavity forms inside ∼4 AU; the cavity extends on the downwind side to form a long cavity wake. Solutions show how the ionization process and the wind condition at 1 AU boundary affect the spatial variation of the wind speed, temperature, pickup proton, fast Mach number, and plasma β-ratio. The wind properties inside 4 AU are axisymmetrical about the solar rotation axis; this axi-symmetry totally disappears in the outer heliosphere. All wind properties are substantially modified at an increasing heliocentric distance on the upwind side to generate an upwind–downwind asymmetry dictated by the direction of the relative motion between the Sun and the interstellar medium." @default.
• W2006183863 created "2016-06-24" @default.
• W2006183863 creator A5027681010 @default.
• W2006183863 date "2010-03-25" @default.
• W2006183863 modified "2023-09-26" @default.
• W2006183863 title "THE GLOBAL SOLAR WIND BETWEEN 1 AU AND THE TERMINATION SHOCK" @default.
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• W2006183863 doi "https://doi.org/10.1088/0004-637x/713/2/721" @default.
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