Physics – Space Physics
Scientist
Physics
Space Physics
Scientist
Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, 171-8501 Japan University, Tokyo, Japan
University of Tokyo Department of Earth and Planetary Physics-STP Graduate School of Science 7-3-1 Hongo Bunkyo-ku, Tokyo 113, Japan
Rikkyo University, 3-34-1, Nishiikebukuro, Toshima-ku, Tokyo, 171-8501 Japan University, 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo, 171-8501 Japan School of Science, University of Tokyo, Tokyo, Japan
Department of Earth and Planetary Science, University of Tokyo, Tokyo, Japan
Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Tokyo, Japan
The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
Department of Physics, Rikkyo University, Toshima, Tokyo 171-8501, Japan.
Department of Physics, Rikkyo University, Toshima-ku, Tokyo, Japan
Tokyo Univ., Japan
Department Phys., Rikkyo Univ., 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo, 171-8501 Japan University, Toshima, Tokyo, 171-8501 Japan University, 3-34-1 Nishi-Ikebukuro Toshima-ku, Tokyo, 171-8501 Japan of Physics, College of Science, Rikkyo University, Tokyo, Japan
Tokyo Univ., Tokyo, Japan
Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
Rikkyo University, 3-34-1 Nishi-ikebukuro, Toshima-ku, 171-8501 Japan and Planetary Science, University of Tokyo, Tokyo, Japan
Graduate School of Science, The univertsity of Tokyo, Tokyo, Japan
Institute of Space and Astronautical S
A Glimpse of Invisible Cold Ions in the Mid-Night Plasma Sheet: GEOTAIL Observations During Solar Umbra
A new perspective on plasma supply mechanisms to the magnetotail from a statistical comparison of dayside mirroring O+ at low altitudes with lobe/mantle beams
A noise attenuation method for medium-energy electron measurements in the radiation belt
Acceleration and heating of cold ion beams in the plasma sheet boundary layer observed with GEOTAIL
Chapter 3-Processes Leading to Plasma Losses into the High-Latitude Atmosphere
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