Stationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard Akatsuki-Reference-Cited by-同舟云学术

Stationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard Akatsuki

Published:2019-05 Issue:5 Volume:124 Page:1266-1281
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Kitahara Takehiko¹,Imamura Takeshi²^ORCID,Sato Takao M.³⁴^ORCID,Yamazaki Atsushi⁴^ORCID,Lee Yeon Joo²,Yamada Manabu⁵,Watanabe Shigeto³,Taguchi Makoto⁶^ORCID,Fukuhara Tetsuya⁶^ORCID,Kouyama Toru⁷^ORCID,Murakami Shin‐ya⁴^ORCID,Hashimoto George L.⁸^ORCID,Ogohara Kazunori⁹^ORCID,Kashimura Hiroki¹⁰^ORCID,Horinouchi Takeshi¹¹^ORCID,Takagi Masahiro¹²^ORCID

Affiliation:

1. Department of Earth and Planetary Science The University of Tokyo Tokyo Japan

2. Graduate School of Frontier Sciences The University of Tokyo Kashiwa Chiba Japan

3. Space Information Center Hokkaido Information University Ebetsu Hokkaido Japan

4. Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Sagamihara Kanagawa Japan

5. Planetary Exploration Research Center (PERC) Chiba Institute of Technology Narashino Chiba Japan

6. College of Science Rikkyo University Tokyo Japan

7. Artificial Intelligence Research Center National Institute of Advanced Industrial Science and Technology Tokyo Japan

8. Department of Earth Science Okayama University Okayama Japan

9. School of Engineering University of Shiga Prefecture Hikone Shiga Japan

10. Department of Planetology/Center for Planetary Science Kobe University Kobe Hyogo Japan

11. Faculty of Environmental Earth Science Hokkaido University Sapporo Hokkaido Japan

12. Faculty of Science Kyoto Sangyo University Kyoto Japan

Publisher

American Geophysical Union (AGU)

Subject

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

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018JE005842

Reference43 articles.

1. A mechanism for the Venus thermospheric superrotation

2. Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves

3. VEGA 1 and VEGA 2 entry probes: An investigation of local UV absorption (220-400 nm) in the atmosphere of Venus (SO2aerosols, cloud structure)

4. Implications of the VEGA Balloon Results for Venus Atmospheric Dynamics

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