are the components of the crossed tensor of particle diffusion which describe the process of the energy exchange between CR and magnetic field inhomogeneities frozen in the solar wind plasma. In agreement with the general theory the quantities Dap, Dpa (as well as Kax) satisfy the principle of the symmetry of kinetic coefficients. As results from Eq. 2.16.10, the value of the vector of particle density in the momentum space is determined by the expression
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