Other
Scientist
Plasma and Space Science Center, National Cheng-Kung University, Tainan, Taiwan;
Institute of Space, Astrophysical and Plasma Sciences, National Cheng Kung University, Tainan, Taiwan;
Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA of Space, Astrophysical and Plasma sciences, National Cheng Kung University, 1 University Rd., Tainan, 70101, Taiwan; Plasma and Space Science Center, National Cheng Kung University, 1 University Rd., Tainan, 70101, Taiwan
Institute of Space, Astrophysical and Plasma Sciences, National Cheng Kung University, Tainan, 70101, Taiwan; Plasma and Space Science Center, National Cheng Kung University, Tainan, 70101, Taiwan
Plasma and Space Science Center, National Cheng-Kung University, No.1 University Road, Tainan, 70101, Taiwan
Institute of Space, Nation Cheng Kung University Astrophysical and Plasma Sciences, No.1, University Road, Tainan, 70101, Taiwan; Plasma and Space Science Center, Nation Cheng Kung University, No.1, University Road, Tainan, 70101, Taiwan
Massachusetts Institute of Technology, Center for Space Research, Cambridge, MA 02139, USA and Space Science Center, No.1 University Road, Tainan City, 70101, Taiwan
National Cheng Kung University, Plasma and Space Science Center, Tainan, 70101, Taiwan
Plasma and Space Science Center, National Cheng-Kung University, Tainan, Taiwan
Plasma and Space Science Center, National Cheng Kung University, Tainan, Taiwan
Institute of Space, Astrophysical and Plasma Sciences, National Cheng Kung University, Tainan, Taiwan
Department of Chemistry, The University of Hong Kong, Pokfulam Road, Hong Kong.
Analysis of Ionospheric Electron Parameters in Relation to the Geomagnetic Index Dst and Solar F10.7 Flux from RO Data of FORMOSAT-3/COSMIC
Analysis on Ionospheric Electron Densities of Storm Events From FORMOSAT-3/COSMIC Observations
Azimuthal structure of auroral arcs associated with various disturbed magnetic conditions
Azimuthal structure of substorm breakup arcs prior to expansive phase onset using ISUAL/FORMOSAT-2
Behavior of global 630.0 nm midnight brightness
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