Study of magnetospheric dynamics using energetic solar particles

Details Study of magnetospheric dynamics using energetic solar particles Study of magnetospheric dynamics using energetic solar particles

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ssrv...17..391m&link_type=abstract

(IAU, IUGG, URSI, IUPAP, COSPAR, and SCOSTEP, International Solar-Terrestrial Physics Symposium, Sao Paulo, Brazil, June 17-24,

Physics

1

Earth Magnetosphere, Geomagnetism, Particle Trajectories, Solar Corpuscular Radiation, Distribution Functions, Energy Spectra, Geomagnetic Tail, Magnetic Storms, Magnetically Trapped Particles, Particle Diffusion, Solar Protons

Scientific paper

The present work (1) shows the importance of the single-particle approximation (trajectories in a reference field) in forming the basis of an understanding of the quiet-time penetration of cosmic rays into the magnetosphere, (2) considers 'steady dynamics' such as wave-particle interaction and field line reconnection, which is believed to exist nearly all the time, and (3) reviews the work which has been done in the more complex and less understood field of 'impulsive dynamics' such as geomagnetic storms and substorms. At present, the interpretation of energetic particle measurements yields results consistent with other types of measurements.

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