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Plenary session: Eruptive processes
Thursday, 5 September 2019
11:20 - 13:00
Ito Hall
Chair: Takaaki Yokoyama, University of Tokyo
11:20 - 11:40 Reconnection Microjets in Solar Coronal Loops.
11:40 - 12:00 Evolution of Transient Inverse FIP Composition in a Solar Flare.
12:00 - 12:30 Space weather and high-energy phenomena.
12:30 - 13:00 Predictability of Solar Flares Based on Satellite Observations and Magnetohydrodynamic Instability Models.
- Reconnection Microjets in Solar Coronal Loops
- Patrick Antolin, University of St Andrews, United Kingdom
- Paolo Pagano, University of St Andrews, United Kingdom
- Paola Testa, Harvard-Smithsonian Center for Astrophysics, United States
- Antonino Petralia, INAF-Osservatorio Astronomico di Palermo, Italy
- Fabio Reale, INAF-Osservatorio Astronomico di Palermo & Universita di Palermo, Italy
- Evolution of Transient Inverse FIP Composition in a Solar Flare
- Deborah Baker, MSSL/UCL, United Kingdom
- Lidia van Driel-Gesztelyi, MSSL/UCL, United Kingdom
- David H. Brooks, George Mason University, United States
- Gherardo Valori, MSSL/UCL, United Kingdom
- Alexander W. James, MSSL/UCL, United Kingdom
- J. Martin Laming, Naval Research Laboratory, United States
- David M. Long, MSSL/UCL, United Kingdom
- Pascal Demoulin, LESIA/Observatoire de Paris, France
- Lucie M. Green, MSSL/UCL
- Sarah A. Matthews, MSSL/UCL, United Kingdom
- Katalin Olah, Konkoly Observatory, Hungary
- Zsolt Kovari, Konkoly Observatory, Hungary
- Space weather and high-energy phenomena
- Miho Janvier, Institut d'Astrophysique Spatiale, France
- Predictability of Solar Flares Based on Satellite Observations and Magnetohydrodynamic Instability Models
- Kanya Kusano, ISEE, Nagoya University, Japan
- Yumi Bamba, ISEE & IAR, Nagoya University, Japan
- Tomoya Iju, NAOJ, Japan
- Satoshi Inoue, ISEE, Nagoya University, Japan