Mirror-mode storms inside stream interaction regions and in the ambient solar wind: A kinetic study

Mirror‐mode structures have been found in the solar wind at various heliocentric distances with different missions. Recently, STEREO has observed mirror‐mode waves present as trains of holes and also as humps in the magnetic field magnitude. In some cases, mirror‐mode trains last for very long perio...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2013-01, Vol.118 (1), p.17-28
Hauptverfasser:	Enríquez-Rivera, O., Blanco-Cano, X., Russell, C. T., Jian, L. K., Luhmann, J. G., Simunac, K. D. C, Galvin, A. B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy kinetic instabilities Kinetics Magnetic fields magnetic holes mirror mode storms mirror mode trains mirror modes Solar physics Storms stream interaction regions Variance analysis
Online-Zugang:	Volltext
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