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[en] It is proposed that the decrease in cosmic ray secondary to primary abundances with increasing energy is a natural consequence of the decreasing efficiency of cosmic ray scattering by plasma instabilities. The low streaming velocities that can result might also account for a possible truncation of the pathlength distribution. An idealized model equation is used to illustrate some (eventually) observable consequences of this mechanism
Source
CEA, 75 - Paris (France); International Union of Pure and Applied Physics; 415 p; ISBN 2-7272-0067-6; 
; 1982; v. 9 p. 215-217; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981
; 1982; v. 9 p. 215-217; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981