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  • [3] A.D. Erlykin and A.W. Wolfendale: “A search for ‘structure’ in the energy spectra of cosmic ray protons and He-nuclei above 104 GeV”, Astroparticle Physics, Vol. 10, (1999), pp. 69–81; “Supernova remnants and the origin of the cosmic radiation: I. SNR acceleration models and their predictions”, Journal of Physics G, Vol. 27, (2001) pp. 941–958; “Supernova remnants and the origin of the cosmic radiation: II. Spectral variations in space and time”, Journal of Physics G, Vol. 27, (2001), pp. 959–976; “Supernova remnants and the origin of the cosmic radiation: III. Spectral differences for different nuclei”, Journal of Physics G, Vol. 27, (2001), pp. 1709–1721. http://dx.doi.org/10.1016/S0927-6505(98)00040-1

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  • [10] G.T. Zatzepin and V.A. Kuzmin: “Upper limit of the spectrum of cosmic rays”, Journal of Experimental and Theoretical Physics Letters, Vol. 4, (1966), pp. 78–80.

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