Full Program »
Plenary session: Eruptive processes
Friday, 6 September 2019
09:30 - 11:00
Ito Hall
Chair: Hyeon K. Park, UNIST
9:30 - 10:00 Laboratory study of ideal MHD instabilities and magnetic reconnection relevant to solar eruptive phenomena.
10:00 - 10:20 How solar eruptions generate X-rays and energetic particles.
10:20 - 10:40 Mapping the Magnetic Field of Flare Coronal Loops.
10:40 - 11:00 Flare-productive Active Regions: Hinode’s View and Beyond.
- Laboratory study of ideal MHD instabilities and magnetic reconnection relevant to solar eruptive phenomena
- Hantao Ji, Princeton University, United States
- How solar eruptions generate X-rays and energetic particles
- Paul Bellan, California Institute of Technology, United States
- Byonghoon Seo, California Institute of Technology, United States
- Ryan Marshall, California Institute of Technology, United States
- Pakorn Wongwaitayakornku, California Institute of Technology, United States
- Magnus Haw, California Institute of Technology, United States
- Mapping the Magnetic Field of Flare Coronal Loops
- David Kuridze, Aberystwyth University, United Kingdom
- Mihalis Mathioudakis, Queen's University Belfast, United Kingdom
- Huw Morgan, Aberystwyth University, United Kingdom
- Ramon Oliver, Universitat de les Illes Balears, Spain
- Flare-productive Active Regions: Hinode’s View and Beyond
- Shin Toriumi, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan
- Haimin Wang, New Jersey Institute of Technology, United States