Correlation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various Wavelengths-Reference-Cited by-同舟云学术

Correlation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various Wavelengths

Published:2022-06 Issue:6 Volume:127 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:JGR Planets

Author:

Narita M.¹^ORCID,Imamura T.²^ORCID,Lee Y. J.³^ORCID,Watanabe S.⁴^ORCID,Yamazaki A.⁵^ORCID,Satoh T.⁵^ORCID,Taguchi M.⁶^ORCID,Sato T. M.⁴,Fukuhara T.⁶^ORCID,Yamada M.⁷^ORCID,Kouyama T.⁸^ORCID,Iwagami N.⁹^ORCID

Affiliation:

1. Department of Mechanical and Industrial Engineering University of Toronto Toronto ON Canada

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

3. Institute of Planetary Research German Aerospace Center (DLR) Berlin Germany

4. Space Information Center Hokkaido Information University Ebetsu Japan

5. Japan Aerospace Exploration Agency Sagamihara Japan

6. College of Science Rikkyo University Tokyo Japan

7. Chiba Institute of Technology Narashino Japan

8. National Institute of Advanced Industrial Science and Technology Tokyo Japan

9. Retired Tokyo 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/10.1029/2022JE007228

Reference65 articles.

1. Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation

2. Images from Galileo of the Venus Cloud Deck

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. Galileo Infrared Imaging Spectroscopy Measurements at Venus

5. Water vapor near Venus cloud tops from VIRTIS-H/Venus express observations 2006–2011

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