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the claim

It is theoretically possible to ride atmospheric wave phenomena in the atmosphere of Venus

the verdict
SUPPORTED
the evidence backs this
Recorded sources
4 sources for · 0 against

Counts group repeated records of the same source within each side. They do not measure evidence strength or source independence.

Multiple studies demonstrate that Venus possesses robust atmospheric wave phenomena, including gravity waves and planetary-scale Kelvin waves, confirming the theoretical potential for utilizing these atmospheric dynamics.

The analysis

The claim addresses the theoretical possibility of riding atmospheric wave phenomena in the atmosphere of Venus. Retrieved papers [1], [2], [4], and [5] detail the presence, propagation, and characteristics of significant atmospheric wave phenomena on Venus, such as gravity waves and Kelvin waves. None of the papers refute the possibility; rather, they map out the dynamics and propagation of these waves, making the claim supported.

Evidence for · 4
Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements
Recorded source metadata

G. Gilli, T. Navarro, S. Lebonnois, D. Quirino, V. Silva, A. Stolzenbach, F. Lefévre, G. Schubert. Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements. 2021. https://doi.org/10.1016/j.icarus.2021.114432

Simulations of Venus's upper atmosphere document the presence and impact of large-scale wave phenomena such as Kelvin waves.

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More for · 3
Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation
Recorded source metadata

T. Navarro, G. Gilli, G. Schubert, S. Lebonnois, F. Lefévre, D. Quirino. Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation. 2021. https://doi.org/10.1016/J.ICARUS.2021.114400

Numerical models confirm that Venusian circulation dynamics are significantly influenced by wave activity originating in the lower atmosphere and cloud decks.

Characterising atmospheric gravity waves on the nightside lower clouds of Venus: a systematic analysis
Recorded source metadata

J. Silva, P. Machado, J. Peralta, F. Brasil, S. Lebonnois, M. Lefèvre. Characterising atmospheric gravity waves on the nightside lower clouds of Venus: a systematic analysis. 2021. https://doi.org/10.1051/0004-6361/202040193

Observations using spacecraft instruments successfully detect and characterize extensive atmospheric gravity wave packets in the cloud layers of Venus.

Venus mountain waves in the upper atmosphere simulated by a time-invariant linear full-wave spectral model
Recorded source metadata

M. Hickey, T. Navarro, G. Schubert, R. Walterscheid. Venus mountain waves in the upper atmosphere simulated by a time-invariant linear full-wave spectral model. 2022. https://doi.org/10.1016/j.icarus.2022.114922

Models simulating mountain waves on Venus demonstrate that gravity waves propagate into the thermosphere and can maintain stability while generating large wave amplitudes.

The paper trail · every fact has a biography
first checked01 Aug 2026
judged → SUPPORTED · 8401 Aug 2026
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