Non-detection at Venus of high-frequency radio signals characteristic of terrestrial lightning

D. A. Gurnett (), P. Zarka, R. Manning, W. S. Kurth, G. B. Hospodarsky, T. F. Averkamp, M. L. Kaiser and W. M. Farrell
Additional contact information
D. A. Gurnett: Department of Physics and Astronomy The University of Iowa
P. Zarka: Observatoire de Paris
R. Manning: Observatoire de Paris
W. S. Kurth: Department of Physics and Astronomy The University of Iowa
G. B. Hospodarsky: Department of Physics and Astronomy The University of Iowa
T. F. Averkamp: Department of Physics and Astronomy The University of Iowa
M. L. Kaiser: NASA/Goddard Space Flight Center
W. M. Farrell: NASA/Goddard Space Flight Center

Nature, 2001, vol. 409, issue 6818, 313-315

Abstract: Abstract The detection1,2 of impulsive low-frequency (10 to 80 kHz) radio signals, and separate very-low-frequency (∼100 Hz) radio ‘whistler’ signals3,4,5 provided the first evidence for lightning in the atmosphere of Venus. Later, a small number of impulsive high-frequency (100 kHz to 5.6 MHz) radio signals, possibly due to lightning, were also detected6. The existence of lightning at Venus has, however, remained controversial7,8,9,10,11,12,13. Here we report the results of a search for high-frequency (0.125 to 16 MHz) radio signals during two close fly-bys of Venus by the Cassini spacecraft. Such signals are characteristic of terrestrial lightning, and are commonly heard on AM (amplitude-modulated) radios during thunderstorms. Although the instrument easily detected signals from terrestrial lightning during a later fly-by of Earth (at a global flash rate estimated to be 70 s-1, which is consistent with the rate expected for terrestrial lightning), no similar signals were detected from Venus. If lightning exists in the venusian atmosphere, it is either extremely rare, or very different from terrestrial lightning.

Date: 2001
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DOI: 10.1038/35053009

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