Characteristics of Asymmetric Coronal Hole Motions over Five Solar Cycles
Barbara A Emery1, Sarah E Gibson2, Ian McDonald Hewins3, Thomas A Kuchar4, David F Webb4 and Robert McFadden5, (1)National Center for Atmospheric Research, Boulder, CO, United States, (2)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (3)ISR, Boston College at HAO/NCAR, Boulder, CO, United States, (4)Boston College, ISR, Chestnut Hill, MA, United States, (5)High Altitude Observatory, Boulder, CO, United States
