Abstract
A self-consistent time-dependent cosmic ray-hydrodynamic model is used in spherical symmetry to solve the standard cosmic ray transport equation for combined anomalous and galactic proton transport, and the one-fluid equations for the solar wind/pickup ion fluid including the dynamic effects of cosmic rays. The model calculates the evolution of a single global merged interaction region including its interaction with the heliospheric termination shock, and the consequent effect on cosmic ray modulation. A series of such regions is also simulated to study their combined contribution on the cosmic-ray modulation cycle.
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