Possible Effects at Voyager 1 and Voyager 2 of Solar Events

Recent Voyager observations are analyzed in the context of the propagation of solar events to the outer heliosphere. The three-dimensional HAFv2 model results show that solar events can asymmetrically propagate to the outer heliosphere. Both longitudinal and latitudinal asymmetries may be important. We compare the preliminary HAFv2 model results with in-situ solar wind plasma, interplanetary magnetic field, and energetic particle observations from Voyager. We also compare the HAFv2 predictions with those from other models.