Scaling Theory for Cross-Field Transport of Cosmic Rays in Turbulent Fields

The transport of charged particles (e.g., cosmic rays) in astrophysically relevant, turbulent magnetic fields (like they exist, e.g., in the solar wind) is investigated. Generic theoretical models-using concepts and insights developed recently in the context of magnetic confinement fusion research-a...

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Veröffentlicht in:	The Astrophysical journal 2010-03, Vol.711 (2), p.997-1007
Hauptverfasser:	Hauff, T, Jenko, F, Shalchi, A, Schlickeiser, R
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CHARGED PARTICLES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COMPUTERIZED SIMULATION CONFINEMENT COSMIC RADIATION Earth, ocean, space Exact sciences and technology IONIZING RADIATIONS MAGNETIC CONFINEMENT MAGNETIC FIELDS ORBITS PLASMA CONFINEMENT RADIATIONS SCALING LAWS SCATTERING SIMULATION SOLAR ACTIVITY SOLAR WIND STELLAR ACTIVITY STELLAR WINDS TURBULENCE
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