Session Details
[P-PS02_28PO1]Mars
Mon. Apr 28, 2014 6:15 PM - 7:30 PM JST
Mon. Apr 28, 2014 9:15 AM - 10:30 AM UTC
Mon. Apr 28, 2014 9:15 AM - 10:30 AM UTC
Poster 3F_3
Convener:*Satoh Takehiko(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Masaki Ishiwatari(Department of Cosmosciences, Graduate school of Science, Hokkaido University), Ayako Matsuoka Ayako(Research Division for Space Plasma, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Yoshiyuki O. Takahashi(Center for Planetary Science), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Hideaki Miyamoto(The University Museum, The University of Tokyo)
The study on Mars has greatly been advanced due to new data from modern missions as well as to new results from theoretical and numerical works. Morphology and variable phenomena, seen on the surface, in the atmosphere and its surrounding plasma, all indicate that Mars is still an active planet.After the successful launch of Japan's new EPSILON rocket (September 2013), possibilities of small planetary missions are becoming more realistic (Mars is the most important target object, of course). In this session, current researches on Mars, including the latest results from missions, as well as future mission plans are discussed.
[PPS02-P01]Interannual analyses of the meridional distributions of Martian dust and clouds obtained by MRO-MCS
*Katsuyuki NOGUCHI1, Kaori IMAE1, Mai KAWANISHI1 (1.Nara Women's University)
[PPS02-P02]Implementing Martian dust lifting scheme into DCPAM, and a diagnosis experiment of surface dust flux
*Hirotaka OGIHARA1, Yoshiyuki O. TAKAHASHI2, Masaki ISHIWATARI1, Masatsugu ODAKA1, Yoshi-yuki HAYASHI3 (1.Department of Cosmosciences, Graduate school of Science, Hokkaido University, 2.Graduate School of Science, Kobe University, 3.Department of Earth and Planetary Sciences, Graduate School of Science, Kobe University)
[PPS02-P03]Assessment of Mars surface environment for MELOS1 lander using Planetary General circulation model DCPAM
*Masatsugu ODAKA1, Ko-ichiro SUGIYAMA2, Yoshiyuki O. TAKAHASHI3, Seiya NISHIZAWA4, Yoshi-yuki HAYASHI5, George HASHIMOTO6 (1.Department of Cosmosciences, Hokkaido University, 2.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3.Center for Planetary Science, 4.RIKEN Advanced Institute for Computational Science, 5.Department of Earth and Planetary Sciences, Graduate School of Science, Kobe University, 6.Department of Earth Sciences, Okayama University)
[PPS02-P04]Estimation of Martian atmospheric composition change caused by CO2 condensation and its application to radio occultation
*Sayaka IKEDA1, Katsuyuki NOGUCHI1, Takeshi KURODA2, Martin PAETZOLD3 (1.Nara Women's University, 2.Tohoku University, 3.University of Cologne)
[PPS02-P05]Equation of state of (Fe,Ni)3S phase - Implications for Mars internal structure
Shunsuke AKAGI1, *Takeshi SAKAI1, Naohisa HIRAO2 (1.Geodynamics Research Center, Ehime University, 2.Japan Synchrotron Radiation Research Institute)
