Abstract URSI Meeting Toronto 1999. 
Wave Interactions with Geomagnetically Trapped Particles  

Martin Walt 
Department of Electrical Engineering 
Stanford University, Stanford, California, 94305, U. S. A. 
Tel: (650) 723-2690; Fax:(650) 723-9251; E-mail: walt@nova.stanford.edu 

      Geomagnetically trapped electrons are readily removed from the
radiation belts by pitch angle scattering with plasma waves. Much
theoretical and experimental evidence supports the argument that VLF
whistlers, plasmaspheric hiss, chorus, and ground based transmitters
contribute to this removal. However, there is considerable uncertainty
about which of these wave sources is most important in the various
regions of the magnetosphere. A better knowledge of the wave fields
throughout the magnetosphere is needed for a better assessment of the
overall importance of the electron-wave interaction process. 
The experimental evidence for the scattering of trapped ions by
waves is much less abundant and suggests that pitch angle scattering of
protons is a slow process. Many estimates of proton transport in the
radiation belts neglect pitch angle scattering although it is clear from
theory that such scattering must occur. Recent data bearing on
wave-proton scattering will be presented.

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