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- W2030543338 endingPage "2015" @default.
- W2030543338 startingPage "2015" @default.
- W2030543338 abstract "Even though Huygens has not detected acoustic signatures of Titanian lightning, electric discharge processes are thought to be very plausible in Titan’s thick atmosphere dominated by nitrogen and methane. When correlated with electromagnetic signatures, thunder will very likely confirm the occurrence of lightning, both during a probe’s descent and/or once it has landed. The presentation has two parts. In the first part, the mechanisms of Titanian thunder generation are discussed, in the context of the most up‐to‐date predictions of lightning on Titan, as well as relevant Cassini‐Huygens data. In the second part, the propagation of thunder in Titan’s troposphere is addressed. Here, the structure, composition, and ambient conditions of the satellite’s atmosphere will be presented and accounted for. Current Titan lightning models predict cloud‐to‐ground discharge channels of ∼20 km. Long‐range Titanian thunder simulations are developed based on the far‐field superposition of approximately 7000 N‐waves arising from 3‐m “elementary” sources. Two lightning geometries will be considered: linear and tortuous. (Tortuous channels are synthesized as a Gaussian distribution in the orientations of the 7000 elementary sources.) For illustrative purposes, to show the effects of atmospheric filtering, the thunder waveform described above will also be propagated in Venus’ atmosphere." @default.
- W2030543338 created "2016-06-24" @default.
- W2030543338 creator A5063040139 @default.
- W2030543338 date "2010-03-01" @default.
- W2030543338 modified "2023-10-18" @default.
- W2030543338 title "The characteristics of thunder on Titan." @default.
- W2030543338 doi "https://doi.org/10.1121/1.3385245" @default.
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