Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer-Reference-Cited by-同舟云学术

Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer

Published:2019-01-09 Issue:1 Volume:10 Page:
ISSN:2041-1723
Container-title:Nature Communications
language:en
Short-container-title:Nat Commun

Author:

Kashimura Hiroki^ORCID,Sugimoto Norihiko^ORCID,Takagi Masahiro,Matsuda Yoshihisa,Ohfuchi Wataru^ORCID,Enomoto Takeshi^ORCID,Nakajima Kensuke,Ishiwatari Masaki,Sato Takao M.^ORCID,Hashimoto George L.,Satoh Takehiko^ORCID,Takahashi Yoshiyuki O.,Hayashi Yoshi-Yuki^ORCID

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy,General Biochemistry, Genetics and Molecular Biology,General Chemistry

Link

http://www.nature.com/articles/s41467-018-07919-y.pdf

Reference49 articles.

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2. Fukuhara, T. et al. Large stationary gravity wave in the atmosphere of Venus. Nat. Geosci. 10, 85–88 (2017).

3. Limaye, S. S. Venus atmospheric circulation: Known and unknown. J. Geophys. Res. 112, E04S09 (2007).

4. Allen, D. A. & Crawford, J. W. Cloud structure on the dark side of Venus. Nature 307, 222–224 (1984).

5. Crisp, D. et al. The dark side of Venus: near-infrared images and spectra from the Anglo-Australian observatory. Science 253, 1263–1266 (1991).

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