The expected modulation of galactic CR including the solar wind braking by CR pressure was found in Babayan and Dorman (1977a). As an example, in Fig. 3.7.6 the results of calculations are shown for a relative modulation with the primary spectrum described by Eq. 3.7.7 at Ek ,min = 0.01 GeV, including nonlinear interaction of solar wind with CR, i.e. taking into account the obtained dependence u(r ). Curves 1, 2, 3, 4, 5 were obtained for the rigidities 0.5, 1, 5, 10, and 100 GV, respectively.

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