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Discover the fascinating world of magnetized plasmas through observations, laboratory experiments, and simulations, focusing on reconnection phenomena like solar flares and auroras. Delve into the micro and macro processes, magnetic helicity, plasmoids, and shock waves, and investigate anomalous resistivity and particle acceleration mechanisms. Gain insights into magnetic reconnection mechanisms and self-organization in an active universe. Join us in advancing the understanding of nonequilibrium systems and engineering applications of magnetohydrodynamics and nuclear fusion experiments. Visit the International Workshop on Explosive Phenomena in Magnetized Plasmas for the latest research in reconnection dynamics.
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Explosive Phenomena in Magnetized Plasmas Reconnection A flare : The Sun An aurora: The Earth Observations of the macro features Laboratory experiments and observations Observations of the micro processes A simulation of the Earth's magnetosphere A simulation of a solar flare Theory and simulations • The origin of anomalous resistivity • The particle acceleration mechanism • The role of magnetic helicity • The plasmoid and the shock wave To investigate Solar-B mission(2006） Adaptive optics of Hida Observatory Merging spheromaks and SCOPE mission (2010) Laser experiment To solve the mechanisms of magnetic reconnection • Investigating the nature of the active universe. • Approaching a complete understanding of the nonequilibrium open • system and self-organization. • Establishing the basis of the engineering applications of • magnetohydrodynamics and nuclear fusion experiments.
International Workshop "Explosive Phenomena in Magnetized Plasmas- New Developments in Reconnection Research" 2004 Mar. 17 - 19Yukawa Institute for Theoretical Physics, Kyoto University (Kyoto, Japan) http://www.kwasan.kyoto-u.ac.jp/reconnection2004 Reconnection A flare : The Sun An aurora: The Earth Observations of the micro processes Laboratory experiments and observations Observations of the macro features A simulation of the Earth's magnetosphere A simulation of a solar flare Theory and simulations • The origin of anomalous resistivity • The particle acceleration mechanism • The role of magnetic helicity • The plasmoid and the shock wave To investigate Solar-B mission(2006） Adaptive optics of Hida Observatory Merging spheromaks and SCOPE mission (2010) Laser experiment To solve the mechanisms of magnetic reconnection • Investigating the nature of theactive universe. • Approaching a complete understanding of the nonequilibrium open system and self-organization. • Establishing the basis of the engineering applications of • magnetohydrodynamics and nuclear fusion experiments . Invited/Key Speakers:Parker, E. N., Yamada, M., Kulsrud, R., Scholer, M., Drake, J., Craig, I., Fuselier, S., Tsuneta, S., Sato, T., Omura, Y., Yoshida, Z., Matsumoto, R., Makishima, K.,Takabe, H., Ono, Y., Yoneda, H., Kojima, H., Fujimoto, M., Kusano, K., Shibata, K., Hoshino, M., Ugai, M., Horiuchi, R., Ogino, T., Terasawa T. Scientific Organizing Committee: K. Shibata (chair), T. Terasawa, M. Hoshino, Y. Ono Local Organizing Committee: K. Shibata (chair), S. Mineshige, T. Miyagoshi, S. Tanuma T. Yokoyama Hosts: 21st century COE "Center for Diversity and Universality in Physics"at Kyoto University, Kwasan and Hida Observatories, Yukawa Institute for Theoretical Physics Contact Address : K. Shibata and T. Miyagoshi, Kwasan Observatory, Kyoto University, Yamashina, Kyoto 607-8471, Japan tel: +81-75-581-1235 Email: miyagosi@kwasan.kyoto-u.ac.jp 040226R2
