CAWSES II One-Day Workshop: CME/ICME and Solar Wind
October 20, 2010 @Kwasan Observatory, Kyoto University
主催: 京都大学理学研究科附属天文台/京都大学宇宙総合学研究ユニット
共催: 名古屋大学太陽地球環境研究所
The solar wind and coronal mass ejections (CMEs) are intrinsically three-dimensional (3-D) structures. However, until recently, only in situ measurements at a few points in space (Earth, Mars, Venus, Ulysses) and limited remote-sensing observations (limited to the 15% closest to the Sun) allowed us to learn about these two complex phenomena. Recently, the development of 3-D numerical models, the construction of larger scintillation arrays and the launch of new spacecraft (Coriolis, Hinode, STEREO and SDO) have allowed scientists to investigate in deeper details the 3-D structure of the solar wind and of coronal mass ejections. The workshop of the task group 3 of CAWSESII on October 20, 2010 in Kwasan Observatory, Kyoto University, Kyoto, Japan provided a forum to present the latest advancement in our understanding of CMEs and the solar wind. About 30 scientists participated, from the field of solar and heliospheric physics, focusing on observations, theory and numerical simulations.
Program
10:30 – 12:00 chair: Asai
10:30 – 10:45 K. Shibata: CAWSES II (presentation)
10:45 – 11:45 B. Jackson: ICMEs in the Solar Wind (presentation)
11:45 – 12:15 N. Lugaz: CME-CME Interaction and its Detection with SECCHI (presentation)
13:30 – 15:00 chair: Kusano
13:30 – 13:55 D. Tripathi: Do flux-Ropes form before or during CMEs Eruptions? (presentation)
13:55 – 14:15 A. Asai: Moreton Wave and EIT Wave observed by STEREO and SDO (presentation)
14:15 – 14:30 H. Tamazawa: Modeling of Flare Shock wave in the Corona (presentation)
14:30 – 14:45 Y. Zhang: Prominence Eruption Occurred on 2010 June 20 - A Multi-Wavelength Observation (presentation)
14:45 – 15:00 H. Isobe: Prominence/Filament Oscillation as a possible Diagnostic Tool of their Stability (presentation)
15:30 – 17:30 chair: Singh
15:30 – 15:55 N. Savani: Morphology of CMEs in the inner Heliosphere (presentation)
15:55 – 16:15 K. Kusano: Data Driven Modeling of Solar Flares and CMEs (presentation)
16:15 – 16:25 R. Kataoka: MHD Modeling of the Solar Wind (presentation)
16:25 – 16:35 D. Shiota: MHD modeling for Formation Process of CMEs (presentation)
16:35 – 16:45 T. Matsumoto: The Solar Wind as the Background of CME Propagation (presentation)
List of Participant
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Workshop Photo
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Posted by Noé Lugaz and Ayumi Asai
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