Galactic Propagation of Cosmic Rays Below 10 14 eV

[1]  S. V. Bulanov,et al.  The influence of the energy dependence of the diffusion coefficient on the spectrum of the electron component of cosmic rays and the radio background radiation of the galaxy , 1974 .

[2]  J. Osborne,et al.  Origin of energetic cosmic rays. III. One-dimensional diffusion from random sources , 1974 .

[3]  J. Skilling,et al.  On Cosmic Ray Diffusion and Anisotropy , 1974 .

[4]  A. Klimas,et al.  The Fokker-Planck coefficient for pitch-angle scattering of cosmic rays. [considering magnetic field fluctuations , 1973 .

[5]  J. Ormes,et al.  Cosmic Ray Sources: Evidence for Two Acceleration Mechanisms , 1973, Science.

[6]  R. Ramaty,et al.  STATISTICAL DISCRETE-SOURCE MODEL OF LOCAL COSMIC RAYS , 1970 .

[7]  E. Parker,et al.  Cosmic-ray life and the stochastic nature of the galactic magnetic field. , 1969 .

[8]  D. Ter Haar,et al.  On the origin of cosmic rays , 1965 .

[9]  J. Daudin,et al.  Sur les variations diurnes en temps solaire et en temps sidéral des grandes gerbes de l’air , 1956 .

[10]  D. Wentzel.  Cosmic-Ray Propagation in the Galaxy: Collective Effects , 1974 .

[11]  J. Skilling.  Cosmic Rays in the Galaxy: Convection or Diffusion? , 1971 .

[12]  J. Skilling.  The Diffusion of Cosmic Rays , 1970 .

[13]  R. Kulsrud,et al.  The Effect of Wave-Particle Interactions on the Propagation of Cosmic Rays , 1969 .

[14]  D. Wentzel.  Hydromagnetic Waves Excited by Slowly Streaming Cosmic Rays , 1968 .

[15]  N. Sherman.  DIURNAL VARIATIONS IN THE INTENSITY OF COSMIC RAYS UNDERGROUND , 1953 .