[en] Various injection profiles of solar flare events (gaussian-type, exponential, and step-function-type), characterized by some time tau over which 'effectively' particles are injected, have been convoluted with a solution of the interplanetary cosmic-ray propagation equation for a purely diffusive transport and for the radial dependence of the diffusion coefficient of the form kappa = M(r/rsub(E))sup(β) where rsub(E) = 1 AU. The influence of M, β and tau on the time-intensity- and time-anisotropy-profiles at 1 AU are discussed. (orig.)