*Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90024, U.S.A.
**Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.
Abstract:
The subsolar ionopause of Venus is expected to be stable to both the Kelvin-Helmholtz and flute instabilities. However, magnetic profiles obtained in the subsolar region indicate that the surface of the ionopause contains large amplitude corrugations, perhaps incipient flux ropes. A possible mechanism for destabilizing the boundary is suggested by the observation that the ion density does not drop abruptly at the ionopause but continues to decrease smoothly into the magnetosheath.