The evolution of solar wind strahl with heliospheric distance

Field‐aligned beams of suprathermal electrons, known as “strahl,” are a frequently observed constituent of solar wind plasma. However, the formation and interplanetary evolution of the strahl electron populations has yet to be fully understood. As strahl electrons travel away from the Sun, they move...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2017-04, Vol.122 (4), p.3858-3874
Hauptverfasser:	Graham, G. A., Rae, I. J., Owen, C. J., Walsh, A. P., Arridge, C. S., Gilbert, L., Lewis, G. R., Jones, G. H., Forsyth, C., Coates, A. J., Waite, J. H.
Format:	Artikel
Sprache:	eng
Schlagworte:	Adiabatic flow cassini Cassini mission Earth orbits Electron beams electrons Evolution Field strength Flyby missions interplanetary Magnetic fields Pitch (inclination) Saturn Scattering Solar physics Solar wind Spacecraft suprathermal wave‐particle
Online-Zugang:	Volltext
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