9:00 AM - 11:00 AM
[PPS05-P01] A new constraint on HCl abundance at the cloud top of Venus by IRTF/iSHELL observations
★Invited Papers
*Takao M. Sato1, Hideo Sagawa2 (1.Hokkaido Information University, 2.Kyoto Sangyo University)
[E] Poster
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
Mon. May 30, 2022 9:00 AM - 11:00 AM Online Poster Zoom Room (3) (Ch.03)
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:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University), Martha S Gilmore(Wesleyan 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.
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.
9:00 AM - 11:00 AM
*Takao M. Sato1, Hideo Sagawa2 (1.Hokkaido Information University, 2.Kyoto Sangyo University)
9:00 AM - 11:00 AM
*Hamamoto Ko1, Yukihiro Takahashi1, Seiko Takagi1, Makoto Taguchi2, Masataka Imai3 (1.Graduate School of Science, Hokkaido University, 2.Rikkyo University, 3.Kyoto Sangyo University)
9:00 AM - 11:00 AM
*Tatsuro Iwanaka1, Takeshi Imamura1 (1.Graduate School of Science, The University of Tokyo)
9:00 AM - 11:00 AM
*Masataka Imai1, Toru Kouyama2, Takeshi Horinouchi3, Makoto Taguchi4, Masahiro Takagi1 (1.Kyoto Sangyo University, 2.National Institute of Advanced Industrial Science and Technology, 3.Hokkaido University, 4.Rikkyo University)
9:00 AM - 11:00 AM
*Hiroyuki Koyama1, Takeshi Imamura1 (1.The University of Tokyo)
9:00 AM - 11:00 AM
*Takehiko Satoh1, Takao M. Sato2, Takeshi Horinouchi3, Takeshi Imamura4, George HASHIMOTO5 (1.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2.Hokkaido Information University, 3.Hokkaido University, 4.The University of Tokyo, 5.Okayama University)
9:00 AM - 11:00 AM
*Fukuoka Seiki1, Takeshi Imamura1, Hiroki Ando2 (1.Graduate School of Frontier Sciences, The University of Tokyo, 2.kyoto sangyo university)
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