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MIC Proposals

 

    Using these capabilities, planning has begun to accommodate many proposed observations concerning surface structures and scattering properties, clouds, polar caps, surface features, and dust rings. The proposed observations will be backed up by a series of ground observations made throughout Japan and coordinated to tie in with the MIC observations. The ground observations will occur in preparation for, just before, and simultaneous with the MIC observations. Ground observations are hoped to provide another way to monitor conditions on Mars during the mission lifetime.

Proposed Observations
Title Investigators
  • Volcanologic Characterization and Research Around Arsia Mons
  • Precise Investigation of Rampart Craters by Low-Angle Images
  • Mapping of Aquifers by Variation in the Onset Diameter of Rampart Craters
  • Global Mapping of the Phase Function of Surface Materials
  • Precise Investigation of Subsurface Layered Structure in Steep Slopes
Kei Kurita
Department of Earth and Planetary Physics, University of Tokyo
Masaru Kono
Department of Earth and Planetary Physics, University of Tokyo
Hirohide Demura
Department of Earth and Planetary Physics, University of Tokyo
  • Seasonal Variation of Martian Clouds
Tokuhide Akabane
Hida Observatory, Kyoto University
Yoshikazu Saito
Kwasan Observatory
Kyosuke Iwasaki
Kyoto Gakuen University
Yasunori Narumi
Kyushu-Tokai University
  • Annual Variation of the Martian South Polar Cap
  • Formation of the North Polar Cap
  • Temporary Stop of Regressions of the North Polar Cap
Kyosuke Iwasaki
Kyoto Gakuen University
Tokuhide Akabane
Hida Observatory, Kyoto University
  • Comparative Study on the Hydrogeomorpholgy of Earth and Mars
Akihiko Kondoh
Chiba University
  • Stereo Mapping of Valles Marineris and Surrounding Regions
Sho Sasaki
Geological Institute, University of Tokyo
Goro Komatsu
Lunar and Planetary Laboratory, University of Arizona
Toshiko Takata
Geological Institute, University of Tokyo
  • Investigation of Time-Variable Atmospheric Circulation Indicated by Aeolian Morphology
  • Surface Properties of Near Polar Cap Regions and the Geological Change Due to Polar Cap Movements
  • Distribution of Subsurface Ice Deposits by Investigation of Fluidizing Rampart Craters and Ancient Polar Wandering
Toshiko Takata
Geological Institute, University of Tokyo
Sho Sasaki
Geological Institute, University of Tokyo
Tsukasa Nakano
Geological Survey of Japan
  • Detection of Phobos and Deimos Dust Rings
Hiroshi Ishimoto
Kobe University
Tadashi Mukai
Kobe University
  • Network of Mars Observations from the Ground
Tokuhide Akabane
Hida Observatory, Kyoto University
Noritaka Tokimasa
Nishi-Harima Astronomical University

It is hoped that MIC's unique capabilities will provide opportunities for new research and new discoveries.