Session Details
[P-CG21]Planetary atmosphere, ionosphere and magnetosphere
Thu. May 26, 2016 3:30 PM - 4:45 PM JST
Thu. May 26, 2016 6:30 AM - 7:45 AM UTC
Thu. May 26, 2016 6:30 AM - 7:45 AM UTC
Poster Hall International Exhibition Hall HALL6_1
Convener:*Takeshi Imamura(Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science), Yukihiro Takahashi(Department of Cosmosciences, Graduate School of Science, Hokkaido University), Yoshiyuki O. Takahashi(Graduate School of Science, Kobe University), Keiichiro Fukazawa(Academic Center for Computing and Media Studies, Kyoto University), Hiromu Nakagawa(Planetary Atmosphere Physics Laboratory, Department of Geophysics, Graduate School of Science, Tohoku University)
Studies of planetary atmospheres, ionospheres and magnetospheres are presented and discussed in this session. Results of ground-based observations, plans of spacecraft missions, and theoretical studies are welcome.
[PCG21-P01]Elucidation, this is the engine of Super-Rotation caught by Venus Express/ESA
*Hirofumi Mase1 (1.none)
[PCG21-P02]A plan to study the Venus’ haze based on SOIR/Venus Express and AKATSUKI
*Seiko Takagi1, Arnaud Mahieux2, Valérie Wilquet2, Séverine Robert2, Rachel Drummond2, Ann Carine Vandaele2, Naomoto Iwagami3 (1.Tokai University, Research and Information Center, 2.Belgian Institute for Space Aeronomy, 3.Department of Earth and Planetary Science, the University of Tokyo)
[PCG21-P03]Near-Infrared spectro-polarimetry of Venusian upper cloud structuer
*Takayuki Enomoto1, Takehiko Satoh2, Koji Kawabata3, Hiroshi Akitaya3, Ryosuke Itoh3 (1.Grad.Univ.Advanced Studies, 2.ISAS, 3.Hiroshima Univ.)
[PCG21-P04]Development of Fiber IFU for Venus Cloud Tops
*Manabu Yamada1, Masato Kagitani3, Atsushi Yamazaki2 (1.Planetary Exploration Research Center, Chiba Institute of Technology, 2.Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, 3.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University)
[PCG21-P05]Venus upper atmosphere as observed by Hisaki: Dayglow and ion tail
*Kei Masunaga1, Kanako Seki1, Naoki Terada2, Fuminori Tsuchiya3, Tomoki Kimura4, Kazuo Yoshioka1, Go Murakami5, Atsushi Yamazaki5, Chihiro Tao6, Ichiro Yoshikawa7 (1.Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, 2.Department of Geophysics, Graduate School of Science, Tohoku University, 3.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 4.Nishina Center for Accelerator Based Sciecne, RIKEN, 5.Institute of Space and Astronoutical Science, Japan Aerospace Exploration Agency, 6.National Institute of Information and Communications Technology, 7.Department of Complexity Science and Engineering, University of Tokyo)
[PCG21-P06]Monitoring Observations of Millimeter-Wave Band Spectral Lines of Carbon Monoxide in the Middle Atmospheres of Venus with the SPART Telescope
*Daiki Haraguchi1, Kazunori Morimae1, Naruaki Tanekura1, Kosuke Saito1, Yuji Nishida1, Kazutoshi Ohnishi1, Hiroyuki Maezawa1, Kazuyuki Handa, Tomio Kanzawa, Masaaki Oya, Jun Maekawa, Hiroyuki Iwashita, Masao Saito, Hideo Sagawa, Munetoshi Tokumaru, Akira Mizuno (1.Osaka Prefecture University)
[PCG21-P07]Development of 1.9-THz-band Waveguide-type Hot-electron Bolometer Mixer Employing Superconducting NbTiN Microbridge
*Hiroyuki Maezawa1, Kosuke Saito1, Yuji Nishida1, Tatsuya Soma2, Osamu Oguchi2, Satoshi Yamamoto2 (1.Department of Physical Science, Osaka Prefecture University, 2.The faculty of science, University of Tokyo)
[PCG21-P08]Measurements of the Venusian mesospheric wind and temperature profiles using mid-IR heterodyne spectrometer MILAHI
*Kosuke Takami1, Hiromu Nakagawa1, Hideo Sagawa2, Shohei Aoki3, Yasumasa Kasaba1, Isao Murata1, Shigeto Watanabe4, Makoto Taguchi5, Takeshi Imamura6 (1.Graduate School of Science, Tohoku University, 2.Faculty of Science, Kyoto Sangyo University, 3.Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di AstroFisica, 4.Department of Cosmosciences, Hokkaido University, 5.Rikkyo University, 6.Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science)
[PCG21-P09]Radiative transfer model combined with multiple scattering in planetary atmosphere: implication for a potential biomarker
*Shun Ishihara1, Masayuki Umemura1, Yu Komatsu1 (1.University of Tsukuba)
[PCG21-P10]Ion acceleration by magnetic reconnection in the dayside ionospheres of unmagnetized planets
Hitoshi Sakamoto1, *Naoki Terada1, Hiromu Nakagawa1, Yasumasa Kasaba1 (1.Graduate School of Science, Tohoku University)
[PCG21-P11]Solar wind conditions on the escape of oxygen from Mars
*Junji Miyazawa1, Shigeto Watanabe1 (1.Planetary and Space Group Department of Cosmosciences Hokkaido University)
[PCG21-P12]Study of the solar wind influence on the Jovian inner magnetosphere using an ionospheric potential solver
*Koichiro Terada1, Naoki Terada1, Yasumasa Kasaba1, Hajime Kita2, Chihiro Tao3, Aoi Nakamizo3, Akimasa Yoshikawa4, Shinichi Ohtani5, Fuminori Tsuchiya2, Masato Kagitani2, Takeshi Sakanoi2, Go Murakami6, Kazuo Yoshioka7, Tomoki Kimura8, Atsushi Yamazaki6, Ichiro Yoshikawa9 (1.Dep. Geophysics Graduate School of Science Tohoku University, 2.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 3.Applied Electromagnetic Research Institute, National Institute of Information and Communications Technology, 4.Department of Earth and Planetary Sciences, Faculty of Science, Kyushu University, / International Center for Space Weather Science and Education, Kyushu University, 5.The Johns Hopkins University Applied Physics Laboratory, 6.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 7.Department of Earth & Planetary Science, Graduate School of Science, The University of Tokyo, 8.Nishina-Center for Accelerator Based Science, RIKEN, 9.The University of Tokyo)
[PCG21-P13]Study on dynamics of Jovian atmosphere by a colorimetric observation of surface structures
*Kazuto Iwasaki1, Hidehiko Suzuki1, Isshi Tabe2, Sumito Hirota3 (1.Meiji Univ., 2.Association of Lunar and Planetary Observers of Japan, 3.Kawasaki municipal science museum)
[PCG21-P14]Derivation of the vertical distribution of Jovian decametric
S-burst sources based on ground-based observations
for verification of the Jovian ionospheric Alfven resonator model
*Yuasa Sasaki1, Atsushi Kumamoto1, Yuto Katoh1, Hiroaki Misawa1 (1.Department of Geophysics, Graduate School of Science, Tohoku University)
[PCG21-P15]Observation of Jupiter's synchrotron radiation in the magnetospheric variation period
*Hiroaki Misawa1, Fuminori Tsuchiya1, Shinya Satoh1, Hajime Kita1, Mamoru Sekido2, Kazuhiro Takefuji2, Eiji Kawai2, Tetsuro Kondo2, Shingo Hasegawa2 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.National Institute of Information and Communications Technology)
[PCG21-P16]Estimation of dawn-to-dusk electric field in the Jovian inner magnetosphere from emission asymmetry in the Io plasma torus
*Ryo Arakawa1, Go Murakami2, Hiroaki Misawa1, Fuminori Tsuchiya1, Hajime Kita1 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
[PCG21-P17]North-south asymmetry of Saturn's auroral radio emissions: The seasonal variation of their fluxes
*Ayumu Sasaki1, Yasumasa Kasaba1, Tomoki Kimura2, Chihiro Tao3, Laurent Lamy4, Baptiste Cecconi4 (1.Dep. Geophysics Graduate School of Science Tohoku University, 2.Nishina-Center for Accelerator Based Science, RIKEN, 3.Space Weather and Environment Informatics Laboratory Applied Electromagnetic Research Institute, 4.LESIA, Observatoire de Paris)
[PCG21-P18][OI]630.0nm emission in the Enceladus torus obtained with Haleakala T60/Vispec
*Hiromu Ono1, Takeshi Sakanoi1, Masato Kagitani1 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University)
[PCG21-P19]Test-particle simulation of elastic collisions between magnetospheric 500eV-50keV electrons and neutral H2O molecules originated from Enceladus
*Hiroyasu Tadokoro1, Yuto Katoh2 (1.Musashino University, 2.Tohoku University)