Abstract
We briefly describe the Pioneer Venus plasma wave instrument and continue with a discussion of wave observations throughout the typical. near‐noon and near‐midnight orbits. This is followed by a detailed comparison of the bow shock turbulence characteristics at earth and at Venus. We then turn to analyze the wave‐particle interactions detected near the dayside ionopause, and we show that the whistler mode Landau damping develops when the B field direction changes so that the Whistler becomes oblique.
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