Formation of the Y Feature at the Venusian Cloud Top by Planetary‐Scale Waves and the Mean Circulation: Analysis of Venus Express VMC Images

Author:

Nara Y.1ORCID,Imamura T.1ORCID,Murakami S.2ORCID,Kouyama T.3ORCID,Ogohara K.4ORCID,Yamada M.5,Takagi M.6ORCID,Kashimura H.7ORCID,Sato N.8

Affiliation:

1. Department of Complexity Science and Engineering, Graduate School of Frontier SciencesThe University of Tokyo Kashiwa Chiba Japan

2. Institute of Space and Astronautical ScienceJapan Aerospace Exploration Agency Sagamihara Kanagawa Japan

3. National Institute of Advanced Industrial Science and Technology Koto‐ku Tokyo Japan

4. Department of Electronic System Engineering, School of EngineeringThe University of Shiga Prefecture Hikone Shiga Japan

5. Planetary Exploration Research CenterChiba Institute of Technology Narashino Chiba Japan

6. Faculty of ScienceKyoto Sangyo University Kyoto Japan

7. Center for Planetary Science/Department of Planetology, Graduate School of ScienceKobe University Kobe Hyogo Japan

8. Natural Science DivisionTokyo Gakugei University Koganei Tokyo Japan

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference43 articles.

1. Study of retrograde rotation, in 4 days, of exterior cloud layer of Venus;Boyer C.;Icarus,1969

2. Planetary‐scale waves in the Venus atmosphere;Covey C.;Journal of the Atmospheric Sciences,1982

3. Temporal variability of ultraviolet cloud features in the Venus stratosphere;Del Genio A. D.;Icarus,1982

4. Planetary‐scale waves and the cyclic nature of cloud top dynamics on Venus;Del Genio A. D.;Journal of the Atmospheric Sciences,1990

5. Ultraviolet contrasts and the absorbers near the Venus cloud tops;Esposito L. W.;Journal of Geophysical Research,1980

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