Session Details
[P-CG31]Status and perspective of future missions and their instruments and technologies for space sciences
Wed. May 27, 2015 6:15 PM - 7:30 PM JST
Wed. May 27, 2015 9:15 AM - 10:30 AM UTC
Wed. May 27, 2015 9:15 AM - 10:30 AM UTC
Convention Hall 2F
Convener:*Masafumi Hirahara(Solar-Terrestrial Environment Laboratory, Nagoya University), Hirotsugu Kojima(Research institute for sustainable humanosphere, Kyoto University), Yukihiro Takahashi(Department of Cosmosciences, Graduate School of Science, Hokkaido University), Makoto Suzuki(Institute for Space and Astronautical Sciences, Japan Aerospace Exploration Agency)
Not only national space agencies but some universities and even companies in the world are now leading a number of space science and exploration missions and also energetically initiating new research activities for satellite and rocket developments and international collaborations in these days because the Earth observations from the space and the space explorations could be achieved much easier than a few decades ago. The deployment to the space, which itself is not purely a scientific purpose but one of methods for better sciences, is vigorously motivating the technical innovation and the educational development. For successful space missions, it is also crucial to research and develop aim-oriented on-board instruments, and the fundamental research and development of observational instrumentation with future perspectives could totally lead space missions in some case. Detailed investigation and evaluation on various on-board instruments are needed during their proposals, selections, and fabrications in order to promote the missions, and inevitably we have to make multi-sided arrangements and evolution at every process and aspect of any type of space missions, independently of their mission sizes. In this session, we focus on these comprehensive research activities in the space missions, including the mission integrations and the individual instrumental developments, and we also call many presentations showing the uniqueness and renovation regarding the mission strategy and methodology, and the status and latest results in the related state-of-the-art researches and developments, which would provide all of researchers and developers with invaluable opportunities for active discussion, information sharing, and collaboration toward the realization of more missions for more fruitful space sciences and explorations in nearer future.
[PCG31-P01]Potential for seismic investigation of Europa using meteorite impacts
*Daisuke TSUJI1, Nicholas TEANBY2 (1.Graduate School of Environmental Studies, Nagoya University, Japan, 2.School of Earth Sciences, University of Bristol, UK)
[PCG31-P02]Development of electric field instrument onboard spacecraft
*Keigo ISHISAKA1, Hirotsugu KOJIMA2, Yasumasa KASABA3, Takumi ABE4 (1.Toyama Prefectural University, 2.RISH, Kyoto University, 3.Tohoku University, 4.ISAS)
[PCG31-P03]Developing of a chip for the interface between plasma wave instruments and plasma particle instruments
*Keisuke ONISHI1, Takahiro ZUSHI1, Hirotsugu KOJIMA2, Yoshifumi SAITO3 (1.Graduate School of Engineering, Kyoto University, 2.Research institute for sustainable humanosphere, Kyoto University, 3.Solar System Science Division, Institute of Space and Astronautical Science, Japan Aerospace Explora)
[PCG31-P04]Improvement of dynamic range of ASIC waveform receiver for plasma wave observations
*Hiroki KOJI1, Mitsunori OZAKI1, Satoshi YAGITANI1, Hirotsugu KOJIMA2, Takahiro ZUSHI2, Akira YOSHIDA1 (1.Graduate School of Natural Science and Technology, Kanazawa University, 2.Research Institute for Sustainable Humanosphere, Kyoto University)
[PCG31-P05]A model calculation of MIA sensor characteristics on board MMO
*Shoichi MIYAZAKI1, Wataru MIYAKE2, Yoshifumi SAITO3, Shoichiro YOKOTA3 (1.Graduate School of Engineering, Tokai University, 2.School of Engineering, Tokai University, 3.ISAS)
[PCG31-P06]Laboratory experiment simulating Martian surface observation with submillimeter-wave polarimetric radiometry
*Taketo ARIMURA1, Satoshi OCHIAI2, Yasuko KASAI2, Kenichi KIKUCHI2, Kazuyuki KITA3 (1.Graduate School of Science and Engineering, Ibaraki University, 2.National Institute of Information and Communications Technology, 3.Faculty of Science, Ibaraki University)