Fig. 2. Velocity v and cosmic rays pressures and as functions of a distance for model 1. Three different positions of the shock are indicated by dotted lines; from each one of them the downstream intergration starts and results in a different profile of the considered quantities. The production efficiency is chosen for each shock as a maximum possible value from the range (0,0.15) still yielding a nonnegative ACR pressure downstream of the shock. It is equal 0.0, 0.01, and 0.06 for the shock at 65, 80, and 95 AU, respectvely.