Physics – Condensed Matter – Mesoscale and Nanoscale Physics
Scientist
Physics
Condensed Matter
Mesoscale and Nanoscale Physics
Scientist
for the Pierre Auger Collaboration
for The Pierre Auger Observatory Collaboration
Institute for Cosmic Ray Research, University of Tokyo, Tokyo 188-8502, Japan
Tokyo, University, Komaba, Japan
Department of Physics, Konan University, Kobe 658-8501, Japan
ISAS / JAXA, Sagamihara, Japan; University, Kobe, Japan; of Space and Astronautical Science, Kanagawa, Japan
Tokyo, University, Tokyo, Japan
Tokyo, University, Japan
Alaska, University, Fairbanks, AK
Institute of Space and Astronautical Science, Tokyo, Japan
Kavli Institute of Cosmological Physics, Enrico Fermi Institute, Department of Astronomy and Astrophysics, The University of Chicago, 5640 S. Ellis, Chicago, IL60637, USA
Department of Earth and Planetary Sciences, Nagoya University, Nagoya 464-8604, Japan; Institute of Low Temperature Science, Hokkaido University, Sapporo 060-0819, Japan
Nagoya Univ., Toyokawa, Japan
ISAS, Kanagawa, Japan
Department of Earth and Planetary Science, University of Tokyo, Tokyo, Japan
Institute of Space and Astronautical Science, Sagamihara, Japan
Department of Earth and Planetary Sciences, Hokkaido University, Sapporo 060-0810, Japan
Institute of Space and Astronautical Sciences, Sagamihara Kanagawa, Japan
Institute of Space and Astronautical Science, STP, Sagamihara, Kanagawa, Japan
Department of Earth and Planetary Sciences, Hokkaido University, Sapporo 060, Japan
Inst. of Space and Astronautical Science, Sagamihara, Japan
ISAS, Sagamihara Kanagawa 229, Japan
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara Kanagawa 229, Japan
Institute of Space and Astronautical Science Sagamihara 229, Japan
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai Sagamihara 229, Japan
Institute of Space and Astronautical Science, Sagamihar
$μ$SR studies of the frustrated quasi-2d square-lattice spin system Cu(Cl,Br)La(Nb,Ta)$_{2}$O$_{7}$: evolution from spin-gap to antiferromagnetic state
A contribution of stellar flares to the GRXE -- based on MAXI observations --
A Feasibility Study of Robotic Servicing for the Hubble Space Telescope
A filament of energetic particles near the high-latitude dawn magnetopause
A flux rope followed by recurring encounters with traveling compression regions: GEOTAIL observations
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