Proton and alpha particle fluxes in the solar wind : results of a three-fluid model
In: JGR. Journal of geophysical research. Part A, Space physics, Jg. 97 (1992), Heft 3, S. 3137-3150
academicJournal
- print,
Zugriff:
A three-fluid model for the solar wind, with continuity, momentum, and energy equations for the three species protons, alpha particles, and electrons, including electron heat conduction and a parameterized coronal heat source, is used to study the behavior of the resulting proton and alpha fluxes as a function of coronal energy input and the proton-to-alpha density ratio at the coronal base.
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Proton and alpha particle fluxes in the solar wind : results of a three-fluid model
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Autor/in / Beteiligte Person: | BÜRGI, A |
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Zeitschrift: | JGR. Journal of geophysical research. Part A, Space physics, Jg. 97 (1992), Heft 3, S. 3137-3150 |
Veröffentlichung: | Washington, DC: American Geophysical Union, 1992 |
Medientyp: | academicJournal |
Umfang: | print, |
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