Session Details
[P-PS02]Recent advances of Venus science and coming decades
Thu. Jun 3, 2021 10:45 AM - 12:15 PM JST
Thu. Jun 3, 2021 1:45 AM - 3:15 AM UTC
Thu. Jun 3, 2021 1:45 AM - 3:15 AM UTC
Ch.02 Zoom Room 02
convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Thomas Widemann(Observatoire de Paris), Kevin McGouldrick(University of Colorado Boulder), Hideo Sagawa(Kyoto Sangyo University), Chairperson:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
Akatsuki, Japan's Venus Climate Orbiter, has been operational in the Venus orbit for more than 5 Earth years, advancing our knowledge mostly about the atmospheric dynamics by feature tracking in the high-resolution imagery. Together with 8 years of coverage made by ESA's Venus Express (2006 - 2014), including spectroscopic information plus plasma measurements, we are in another golden age of Venus science decades after the landing missions of the USA and the former USSR in the 1970's. In addition, the Venus community has been eager to realize next generation missions to Venus. This session will cover all aspects of science related to Venus, either by observationally (including future missions) or by theoretically, about the planet itself or its surrounding environment or even implications to the exoplanets. Contributions by experts and by early-career researchers are all welcome.
[PPS02-07]Microphysics Implications of the Venus Bow Wave seen by LIR on Akatsuki
*Kevin McGouldrick1 (1.Laboratory for Atmospheric and Space Physics, University of Colorado Boulder)
[PPS02-08]Barotropic instability and traveling linear features detected in the near-infrared images from Akatsuki
*Takeshi Horinouchi1, Takehiko Satoh2, Choon Wei Vun2, Eliot F. Young3 (1.Faculty of Environmental Earth Science, Hokkaido University, 2.ISAS, 3.Southwest Research Institute)
[PPS02-09]Statistical analysis of the morphology of Venusian clouds
*Tomoya Suda1, Takeshi Imamura1 (1.Graduate School of Frontier Sciences, The University of Tokyo)
<img src="https://confit-sfs.atlas.jp/customer/jpgu2021/web/OSPA.png"><br/>
[PPS02-10]Simulation of sulfuric acid cloud distributions by a Venus GCM for the comparison with observations
*Hiroki Karyu1, Takeshi Kuroda1, Naoki Terada1, Yasumasa Kasaba1, Masaru Yamamoto2, Masaaki Takahashi3, Kohei Ikeda4 (1.Tohoku University, 2.Kyushu University, 3.University of Tokyo, 4.National Institute for Environmental Studies)
[PPS02-11]A development of a broadband radiative transfer model "Mstrn-Venus" for Venus atmosphere
*Miho Sekiguchi1, Reiko Kurihara1, Naohiro Manago2, Masahiro Takagi3, Hideo Sagawa3, Yoshihisa Matsuda4 (1.Tokyo University of Marine Science and Technology, 2.Chiba University, 3.Kyoto Sangyo University, 4.Tokyo Gakugei University)
