Time profile of solar energetic particles fit using a mean free path considering the radial dependence of both magnetic field strength and fluctuations

The radially dependent mean free path of solar energetic particles was calculated by considering the radially dependent magnetic field fluctuation, its correlation length and the variation of magnetic field strength along an Archimedean interplanetary magnetic field. A longer mean free path can be d...

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Veröffentlicht in:	Earth, planets, and space planets, and space, 2002-01, Vol.54 (6), p.727-732
1. Verfasser:	SAKAI, Takasuke
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Deceleration Earth, ocean, space Energetic particles Exact sciences and technology Field strength Interplanetary magnetic field Magnetic fields Mathematical analysis Mean free path Particle radiation, solar wind Pitch (inclination) Solar energetic particles Solar physics Solar system Transport equations
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