Physics – Condensed Matter – Superconductivity
Scientist
Physics
Condensed Matter
Superconductivity
Scientist
ISAS / JAXA
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
ISAS, Japan
ISAS, Kanagawa, Japan
International Research Centre for Japanese Studies, 610-1192, Kyoto, Japan
The Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara, Kanagawa 229-8510, Japan
Institute of Space and Astronautical Science, Sagamihara, Japan
IFREE, JAMSTEC, Yokohama, Japan; of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Onagawa Magnetic Observatory, Sendai, Japan
Onagawa Magnetic Observatory; Tohoku University, Sendai, Japan
Tohoku Institute of Technology, 35-1 Yagiyama Kasumi-cho, Taihaku-ku, Sendai, Miyagi 982-8577, Japan
Institute of Geophysics, ETH Zurich, Zurich, Switzerland
Department of Chemistry and Biotechnology, University of Tokyo, Rm. 164, General Research Building, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba, 277-8561 Japan of Physics, Tohoku University, Sendai 980, Japan
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
The Institute of Space and Astronautical Science Institute of Space and Astronautical Science
Korea Astronomy and Space Science Institute, Daejeon, Korea
Tohoku Institute of Technology, Taihaku-ku, Sendai, 982-8577, Japan
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510 JAPAN
ISAS / JAXA, University of Tokyo
Inst. of Space and Astronautical Science, Sagamihara, Japan
Tohoku Institute of Technology, Sendai 982-8577, Japan
Information and Communication Engineering, Tohoku Institute of Technology, Sendai, Miyagi 982-8577, Japan
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 Japan
Institute of Space and Astronautical Science, J
(C II) 158 micron and (O I) 63 micron observations of the Galactic center regions
155 Micron Continuum Emission from the Galactic Plane near L = 50 Degrees Observed by IRTS
20cm survey of the AKARI NEP (White+, 2010)
3-D numerical simulations of a growing planet with the core formation by the impact
4.7-micron spectroscopy of NGC 1068 in search of absorption by gaseous CO in the molecular torus
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