Session Details
[P-PS06][EJ] Results of Venus science with Akatsuki in orbit for 1.5 year
Sat. May 20, 2017 10:45 AM - 12:15 PM JST
Sat. May 20, 2017 1:45 AM - 3:15 AM UTC
Sat. May 20, 2017 1:45 AM - 3:15 AM UTC
Convention Hall B International Conference Hall 2F
convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University), Masaru Yamamoto(Research Institute for Applied Mechanics, Kyushu University), Kevin McGouldrick(University of Colorado Boulder), Chairperson:Kevin McGouldrick(University of Colorado Boulder)
This meeting celebrates 1.5 years since Akatsuki's arrival at Venus with all on-board scientific instruments in good health condition. High-quality Venus data are being acquired with such instruments. This session invites papers of scientific results with the data from Akatsuki and other missions, and recent results of theoretical and numerical works. We expect participants of this session will share the latest research results through presentations and discussion.
[PPS06-06]Characteristic features in cloud-top temperature of Venus★Invited papers
*Makoto Taguchi1, Tetsuya Fukuhara1, Toru Kouyama2, Takeshi Imamura3, Takao M. Sato4, Masahiko Futaguchi10, Mao Takamura1, Takeru Yamada1, Naomoto Iwagami5, Makoto Suzuki4, Munetaka Ueno6, Mitsuteru Sato7, George Hashimoto8, Seiko Takagi9, Masato Nakamura4 (1.Rikkyo University, 2.National Institute of Advanced Industrial Science and Technology, 3.The University of Tokyo, 4.Institute of Space and Astronautical Science, 5.Senshu University, 6.Kobe University, 7.Hokkaido University, 8.Okayama University, 9.Tokai University, 10.Toho University)
[PPS06-07]Stationary features at the cloud top of Venus observed in Akatsuki UV images
*Takehiko Kitahara1, Takeshi Imamura1, Atsushi Yamazaki2, Manabu Yamada3, Shigeto Watanabe4 (1.The University of Tokyo, 2.ISAS/JAXA, 3.Chiba Institute of Technology, 4.Hokkaido Information University)
[PPS06-08]Stationary features at the Venus cloud top seen in Akatsuki/IR2 2.02-μm dayside images
*Takao M. Sato1, Shin-ya Murakami1, Takeshi Horinouchi2, Takehiko Satoh1, Javier Peralta1, Takeshi Imamura3 (1.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2.Hokkaido University, 3.The University of Tokyo)
[PPS06-09]Venus Express observations of longitude variations of zonal wind, UV albedo and H2O at Venus cloud top level explained by stationary gravity waves.★Invited papers
*Jean-Loup Bertaux1 (1.Le Laboratoire Atmospheres, Milieux, Observations Spatiales)
[PPS06-10]Effects of topography on Venus' atmospheric general circulation inferred from GCM experiments
*Masaru Yamamoto1, Kohei Ikeda2, Masaaki Takahashi (1.Research Institute for Applied Mechanics, Kyushu University, 2.National Institute for Environmental Studies)