Helium and minor ions in the corona and solar wind - Dynamics and charge states

A theoretical model of the acceleration region of the solar wind with major species (p, alpha, e) and minor ions (e.g., He-3, C, O, Mg, Si) is presented. Observed n(e)-profiles and the equations of continuity and momentum are used to calculate profiles of T, n, and u for all species, as well as char...

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Veröffentlicht in:	Solar physics 1986-02, Vol.103 (2, 19), p.347-383
Hauptverfasser:	Buergi, A., Geiss, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Solar Physics
Online-Zugang:	Volltext
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