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Cosmic rays propagating in the Galaxy may excite a streaming instability whentheir motion is super-alfvenic, thereby producing the conditions for their owndiffusion. We present the results of a self-consistent solution of thetransport equation where diffusion occurs because of the self-generatedturbulence together with a preexisting turbulence injected, for instance, bysupernova explosions and cascading to smaller scales. All chemicals areincluded in our calculations, so that we are able to show the secondary toprimary ratios in addition to the spectra of the individual elements. Allpredictions appear to be in good agreement with observations.

Self-generated magnetic turbulence and the propagation of galactic cosmic rays