The corotating particle events give us a unique opportunity to probe t
he three-dimensional structures of the heliosphere. This is especially
true if we have observations over a period of extreme stability of th
e CIRs, such as existed over the recent solar minimum. We discuss how
the observations fit into the context of current heliospheric magnetic
field models. The energetic particle signatures of CIRs throughout th
e regions of the heliosphere covered by the deep-space missions are re
viewed. The CIRs accelerate these particles and at the same time modul
ate both the high energy galactic cosmic rays and the anomalous cosmic
rays.