Dynamical model for the distribution of geomagnetically trapped anomalous-component ions

Details Dynamical model for the distribution of geomagnetically trapped anomalous-component ions Dynamical model for the distribution of geomagnetically trapped anomalous-component ions

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....3..629b&link_type=abstract

Proceedings of the 22nd International Cosmic Ray Conference. 11-23 August, 1991. Dublin, Ireland. Under the auspices of the Inte

Physics

Dynamic Models, Energetic Particles, Radiation Belts, Cosmic Rays, Earth Magnetosphere, Oxygen Ions, Particle Energy, Spectral Line Width, Trapped Particles

Scientific paper

Analyses of data gathered by the Space Shuttle TRIS experiment have stimulated study of the anomalous component of the cosmic ray spectrum, as well as of the geomagnetic trapping of its constituent ions. Due to their high-Z/low-energy characteristics, solar particles are also partially ionized and result in a similar trapping of energetic solar particles. Attention is here given to estimates of the anomalous components' spectral shape, lifetime, and L-value distribution.

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