The Dependence of the Applicability of Spatial Diffusion Equation for Solar Cosmic Rays upon the Magnitude of Time Derivative of Anisotropy

Details The Dependence of the Applicability of Spatial Diffusion Equation for Solar Cosmic Rays upon the Magnitude of Time Derivative of Anisotropy The Dependence of the Applicability of Spatial Diffusion Equation for Solar Cosmic Rays upon the Magnitude of Time Derivative of Anisotropy

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....3..193s&link_type=gif

Proceedings of the 22nd International Cosmic Ray Conference. 11-23 August, 1991. Dublin, Ireland. Under the auspices of the Inte

Physics

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