Physics – Fluid Dynamics
Scientist
Physics
Fluid Dynamics
Scientist
Korea Astronomy and Space Science Institute, 61-1, Hwaam-dong, Yuseong-gu, Daejeon, 305-348 Korea, Republic of Hee University, Yongin, Republic of Korea;
School of Space Research, Kyung Hee University, 446-701 yongin-si Gyeonggi-do, Republic of Korea;
Heliophysics, NASA / GSFC, Greenbelt, MD, USA;
School of Space Research, Kyunghee Univ., Yong-in Si, Republic of Korea;
School of space research, Kyunghee University, Yongin, Republic of Korea;
School of Spaece Research, Kyung Hee University, Yongin, Republic of Korea;
School of Space Research, Kyung Hee University, Yongin-si, Republic of Korea;
Korea Astronomy and Space Science Institute, 61-1 Whaamdong, Yooseong, Daejeon, 305-348 Korea, Republic of Astronomy and Space Science Institute, Whaam-Dong, Youseong-Gu, Daejeon, 305-348 Korea, Republic of Hee University, Republic of Korea
Kyunghee University, Republic of Korea
School of Space Research, Kyung Hee University, Korea, Republic of
Kyunghee University, Korea, Republic of
Kyunghee university, Kyunghee university Department of Astronomy and Space Science, 1 Seocheon-dong, Giheung-gu, Yongin-si Gyeonggi-do 446-701, KOREA, Yongin-si, 446-701, Korea, Republic of
Korea Astronomy Observatory, whaamdong, Yooseong, Taejeon, 305-348 Korea, Republic of Astronomy and Space Science Institute, Republic of Korea
Big Bear Solar Observatory / NJIT, 40386 North Shore Lane, Big Bear City, CA 92314, USA; Korea Astronomy Observatory, 61-1 Whaamdong, Yooseong-gu, Taejeon, 305-348 Korea, Republic of Astronomical Observatory, 36-1 Whamdong, Yuseong-ku, Taejon, 305-348 Korea, Republic of Hee University, Department of Astronomy and Space Science, Kyungki-do, Yongin- shi, 446-701, Korea, Republic of
Department of Astronomy and Space Scienc
A Statistical Study for Two Classes of CMEs
An Imaging Spectroscopic Study of Active Region EUV Bright Points by Hinode/EIS
An Observational Study of the Relationship between CMEs and Flares
Comparison of Asymmetric and Ice-cream Cone Models for Halo Coronal Mass Ejections
Comparison of CME radial velocities from a flux rope model and an ice cream cone model
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