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The role of nearby galactic sources, the supernova remnants, in formation ofobserved energy spectrum and anisotropy of high-energy cosmic rays is studied.The list of these sources is made up based on radio, X-ray and gamma-raycatalogues. The distant sources are treated statistically as ensemble ofsources with random positions and ages. The source spectra are defined based onthe modern theory of cosmic ray acceleration in supernova remnants while thepropagation of cosmic rays in the interstellar medium is described in theframeworks of galactic diffusion model. Calculations of anisotropy are made toreproduce the experimental procedure of getting the two-dimensional anisotropy.The detailed comparison of calculations with cosmic ray data is made. Weexplained simultaneously the new cosmic ray data on a fine structure of allparticle spectra around the knee and the amplitude and direction of the dipolecomponent of anisotropy in the wide energy range 1 TeV - 1 EeV. Madeassumptions do not look exotic, and they confirm the modern understanding ofcosmic ray origin.

Spectrum and Anisotropy of Cosmic Rays at TeV-PeV-energies and Contribution of Nearby Sources