Large stationary gravity wave in the atmosphere of Venus

Tetsuya Fukuhara, Masahiko Futaguchi, Joji Hashimoto, Takeshi Horinouchi, Takeshi Imamura, Naomoto Iwagaimi, Toru Kouyama, Shin Ya Murakami, Masato Nakamura, Kazunori Ogohara, Mitsuteru Sato, Takao M. Sato, Makoto Suzuki, Makoto Taguchi, Seiko Takagi, Munetaka Ueno, Shigeto Watanabe, Manabu Yamada, Atsushi Yamazaki

Research output: Contribution to journalArticle

35 Citations (Scopus)

Abstract

The planet Venus is covered by thick clouds of sulfuric acid that move westwards because the entire upper atmosphere rotates much faster than the planet itself. At the cloud tops, about 65 km in altitude, small-scale features are predominantly carried by the background wind at speeds of approximately 100 m s â '1. In contrast, planetary-scale atmospheric features have been observed to move slightly faster or slower than the background wind, a phenomenon that has been interpreted to reflect the propagation of planetary-scale waves. Here we report the detection of an interhemispheric bow-shaped structure stretching 10,000 km across at the cloud-top level of Venus in middle infrared and ultraviolet images from the Japanese orbiter Akatsuki. Over several days of observation, the bow-shaped structure remained relatively fixed in position above the highland on the slowly rotating surface, despite the background atmospheric super rotation. We suggest that the bow-shaped structure is the result of an atmospheric gravity wave generated in the lower atmosphere by mountain topography that then propagated upwards. Numerical simulations provide preliminary support for this interpretation, but the formation and propagation of a mountain gravity wave remain difficult to reconcile with assumed near-surface conditions on Venus. We suggest that winds in the deep atmosphere may be spatially or temporally more variable than previously thought.

Original languageEnglish
Pages (from-to)85-88
Number of pages4
JournalNature Geoscience
Volume10
Issue number2
DOIs
Publication statusPublished - Feb 1 2017

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standing wave
Venus
gravity wave
atmosphere
planet
atmospheric feature
atmospheric wave
mountain
upper atmosphere
sulfuric acid
topography
simulation

ASJC Scopus subject areas

  • Earth and Planetary Sciences(all)

Cite this

Fukuhara, T., Futaguchi, M., Hashimoto, J., Horinouchi, T., Imamura, T., Iwagaimi, N., ... Yamazaki, A. (2017). Large stationary gravity wave in the atmosphere of Venus. Nature Geoscience, 10(2), 85-88. https://doi.org/10.1038/ngeo2873

Large stationary gravity wave in the atmosphere of Venus. / Fukuhara, Tetsuya; Futaguchi, Masahiko; Hashimoto, Joji; Horinouchi, Takeshi; Imamura, Takeshi; Iwagaimi, Naomoto; Kouyama, Toru; Murakami, Shin Ya; Nakamura, Masato; Ogohara, Kazunori; Sato, Mitsuteru; Sato, Takao M.; Suzuki, Makoto; Taguchi, Makoto; Takagi, Seiko; Ueno, Munetaka; Watanabe, Shigeto; Yamada, Manabu; Yamazaki, Atsushi.

In: Nature Geoscience, Vol. 10, No. 2, 01.02.2017, p. 85-88.

Research output: Contribution to journalArticle

Fukuhara, T, Futaguchi, M, Hashimoto, J, Horinouchi, T, Imamura, T, Iwagaimi, N, Kouyama, T, Murakami, SY, Nakamura, M, Ogohara, K, Sato, M, Sato, TM, Suzuki, M, Taguchi, M, Takagi, S, Ueno, M, Watanabe, S, Yamada, M & Yamazaki, A 2017, 'Large stationary gravity wave in the atmosphere of Venus', Nature Geoscience, vol. 10, no. 2, pp. 85-88. https://doi.org/10.1038/ngeo2873
Fukuhara T, Futaguchi M, Hashimoto J, Horinouchi T, Imamura T, Iwagaimi N et al. Large stationary gravity wave in the atmosphere of Venus. Nature Geoscience. 2017 Feb 1;10(2):85-88. https://doi.org/10.1038/ngeo2873
Fukuhara, Tetsuya ; Futaguchi, Masahiko ; Hashimoto, Joji ; Horinouchi, Takeshi ; Imamura, Takeshi ; Iwagaimi, Naomoto ; Kouyama, Toru ; Murakami, Shin Ya ; Nakamura, Masato ; Ogohara, Kazunori ; Sato, Mitsuteru ; Sato, Takao M. ; Suzuki, Makoto ; Taguchi, Makoto ; Takagi, Seiko ; Ueno, Munetaka ; Watanabe, Shigeto ; Yamada, Manabu ; Yamazaki, Atsushi. / Large stationary gravity wave in the atmosphere of Venus. In: Nature Geoscience. 2017 ; Vol. 10, No. 2. pp. 85-88.
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