Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Sagamihara, 229-8510 Japan Astronomy Observatory
Chinese Academy of Sciences, Atomic Energy Institute, Beijing, People's Republic of China
Applied Electromagnetic Res, NICT, Tokyo, Japan; Astronomy Observatory, Taejon 305-348, Korea Institute of Information and Communication Technology, Koganei, Japan
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan
Korea Advanced Institute of Science and Technology Science Research Division, Korea Astronomy Observatory, Daejeon 305-348, Korea Science Research Group, Korea Astronomy Observatory
School of Space Research, Kyung Hee University, Gyeonggi, Korea
Kyung Hee University, Korea, Republic of
National Institute of Information and Communication Technology, 4-2-1 Nukuikitamachi, Koganei, 184-8795, Japan of Space Research, Kyung Hee University, Gyeonggi, South Korea
National Institute of Information and Communications Technology, Tokyo, Japan
National Institute of Information and Communications Technology, Koganei, Tokyo, Japan
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, 229-8510 Japan 4-2-1 Nukui-Kitamachi, Koganei, Tokyo, 184-8795, Japan 61-1 Whaam-dong, Yusong-gu, Taejon, 305-348 Korea, Republic of
NICT, Tokyo, Japan of Space Research, Kyung Hee University, Yongin, Republic of Korea
Kyung-Hee University, Yongin, Republic of Korea
KyungHee Observatory, Department of Astronomy and Space Science, KyungHee University
National Institute of Information and Communications Technology, Koganei, Japan
Korea Astronomy Observatory, Space Sciences Group, KAO, Taejon, 305-348 Korea, Republic of Institute of Information and Communications Technology, Koganei
3-D Model Analyses for Lunar Sodium Exosphere and Tail
A comparison of THEMIS Pi2 observations near the dawn and dusk sectors in the inner magnetosphere
A Numerical Study of the Ionospheric Environment for Different Strengths of the Geomagnetic Main Field
Airglow Observation from STSAT-1
An Improved Dilaton Background in Soft-Wall Model
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