Where are medium-scale solar-wind variations formed?

The locations are discussed where periodic variations in the solar-wind density are formed taking into account the observed antiphase variations in the proton and alpha-particle densities (Viall et al., 2009). Taking into consideration that alpha particles move faster than protons, we can state that...

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Veröffentlicht in:	Geomagnetism and Aeronomy 2014-03, Vol.54 (2), p.162-163
1. Verfasser:	Yermolaev, Yu. I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Earth and Environmental Science Earth Sciences Geophysics/Geodesy Particle physics Protons Solar flares Solar physics
Online-Zugang:	Volltext
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