Radial density, velocity and temperature profiles in a multi-species solar wind close to the coronal base: A self-consistent four-species model
We present a multi-species model of the solar wind close to the coronal base. Employing a five-moment approximation, the steady state profiles of densities, velocities as well as temperatures of electrons and three ion species, namely protons, alpha particles and a minor ion population such as oxyge...
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Veröffentlicht in: | Advances in space research 2000, Vol.25 (9), p.1935-1938 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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