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Further evidence for lightning on Venus

dc.contributor.authorSingh R.N.; Russell C.T.
dc.date.accessioned2025-05-24T09:56:25Z
dc.description.abstractImpulsive electrical signals at all frequencies recorded by the plasma wave instrument on Pioneer Venus are found to cluster around periapsis. The signals are strongest at 100 Hz and have a secondary peak at 5.4 kHz. These characteristics are consistent with generation by lightning in the Venus atmosphere and the direct propagation of whistler mode signals below the electron gyro frequency and the partial transmission of electromagnetic waves in the presence of electron density inhomogeneities above the electron gyro frequency. The scattering by electron density inhomogeneities may also weaken any correlation with surface topographical features. Thus, the source of these signals may either be intercloud lightning at high altitudes or lightning in volcanic plumes near the ground, despite the large scatter in inferred source locations. Copyright 1986 by the American Geophysical Union.
dc.identifier.doihttps://doi.org/10.1029/GL013i010p01051
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/20978
dc.relation.ispartofseriesGeophysical Research Letters
dc.titleFurther evidence for lightning on Venus

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