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Hinode: Waves and turbulence
Tuesday, 3 September 2019
14:00 - 16:00
Ito Hall
Chair: Jorrit Leenaarts, Stockholm University
14:00 - 14:30 EUV spectroscopy of active regions from view point of coronal heating mechanisms.
14:30 - 14:45 The drivers of active region outflows into the slow solar wind.
14:45 - 15:00 IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole.
15:00 - 15:15 Wave heating of the lower solar atmosphere.
15:15 - 15:30 Shock heating energy in an umbra of a sunspot with integral field unit spectroscopy.
15:30 - 16:00 Magnetic Reconnection in the partially ionized low solar atmosphere.
- EUV spectroscopy of active regions from view point of coronal heating mechanisms
- Paola Testa, Harvard-Smithsonian Center for Astrophysics, United States
- The drivers of active region outflows into the slow solar wind
- David Brooks, George Masin University at JAXA, Japan
- Hi-C Science Team Hi-C Science Team
- IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole
- Akiko TEI, Kyoto University, Japan
- Joten OKAMOTO, National Astronomical Observatory of Japan, Japan
- Petr HEINZEL, Astronomical Institute, Academy of Sciences of the Czech Republic, Czech Republic
- Stanislav GUNAR, Astronomical Institute, Academy of Sciences of the Czech Republic, Czech Republic
- Sonja JEJCIC, University of Ljubljana, Slovenia
- Kazunari SHIBATA, Kyoto University, Japan
- Wave heating of the lower solar atmosphere
- Shahin Jafarzadeh, Rosseland Centre for Solar Physics, University of Oslo, Norway
- Sven Wedemeyer, Rosseland Centre for Solar Physics, University of Oslo, Norway
- Mikolaj Szydlarski, Rosseland Centre for Solar Physics, University of Oslo, Norway
- Shock heating energy in an umbra of a sunspot with integral field unit spectroscopy
- Tetsu Anan, National Solar Observatory, United States
- Thomas Schad, National Solar Observatory, United States
- Sarah Jaeggli, National Solar Observatory, United States
- Lucas Tarr, National Solar Observatory, United States
- Magnetic Reconnection in the partially ionized low solar atmosphere
- Lei Ni, Yunnan observatories, Chinese Academy of Sciences, China