Session Details

[P-PS05]Science of Venus: knowing more about the earth's sister planet

Mon. May 23, 2022 9:00 AM - 10:30 AM JST
Mon. May 23, 2022 12:00 AM - 1:30 AM UTC
303 International Conference Hall, Makuhari Messe
convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), convener:Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University), Martha S Gilmore(Wesleyan University), convener:Emmanuel Marcq(Laboratoire Atmospheres, Exploration Spatiale, Institut Pierre-Simon Laplace, Universite de Versailles Saint-Quentin), Chairperson:Martha S Gilmore(Wesleyan University), Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University)
Two Venus orbiting missions, ESA's Venus Express (2006 - 2014) and Japan's Akatsuki (2015 to current in Venus' orbit), have advanced our knowledge mostly about the Venusian atmosphere (dynamics, chemistry and evolution). This strong momentum will further be enhanced by the newly selected 3 Venus missions, NASA's VERITAS and DAVINCI, and ESA's EnVision. We are and will certainly be in a new golden age of the Venus science. Launch dates for the new missions are, of course, still many years ahead but it is never too early to deepen scientific discussion and to clarify what the problems are and how we should answer them.<br/>This session will therefore cover all aspects of science related to Venus, from its interior to the surrounding plasma environment, either by observationally or by theoretically. Implications to the exoplanets are also important objectives of studies of Venus. Contributions by experts and by early-career researchers are all welcome.

[PPS05-06]Periodical variation of the small-scale UV contrast at the cloud top of Venus

Tomoya Suda1, *Takeshi Imamura1 (1.Graduate School of Frontier Sciences, The University of Tokyo)

[PPS05-07]Derivation of vertical profiles of sulfur dioxide in the Venus cloud layer by the Akatsuki radio occultation measurements

*Hinako Onuma1, Katsuyuki Noguchi1, Hiroki Ando2, Takeshi Imamura3, Hideo Sagawa2 (1.Nara Women's University, 2.Kyoto Sangyo University, 3.Tokyo University)
<img src="https://confit-sfs.atlas.jp/customer/jpgu2022/web/ospa2022.png">

[PPS05-08]Short-term and Long-term temperature variations in upper cloud layer of Venus obtained from 10 Venusian-year operation of Akatsuki/LIR★Invited Papers

*Toru Kouyama1, Masataka Imai2, Takeshi Imamura3, Takeshi Horinouchi4, Shin-ya Murakami5, Yeon-Joo Lee6, Makoto Taguchi7 (1.National Institute of Advanced Industrial Science and Technology, 2.Kyoto Sangyo University, 3.University of Tokyo, 4.Hokkaido University, 5.Japan Aerospace Exploration Agency, 6.German Aerospace Center, 7.Rikkyo University)

[PPS05-09]Temperatures at the limb from Akatsuki's LIR camera data★Invited Papers

*Sanjay S Limaye1 (1.University of Wisconsin Madison)

[PPS05-10]Mean winds and planetary-scale waves at the cloud top of Venus from the 6-year observation of Akatsuki/UVI

*Takeshi Horinouchi1, Toru Kouyama2, Masataka Imai3, Yeon Joo Lee4, Shin-ya Murakami5, Shigeto Watanabe6, Manabu Yamada7, Atsushi Yamazaki5 (1.Faculty of Environmental Earth Science, Hokkaido University, 2.AIST, 3.Kyoto Sangyo University, 4.Institute for Basic Science, 5.ISAS, 6.Hokkaido Information University, 7.Chiba Institute of Technology)

Discussion