The solar wind interacts with Earth's magnetosphere-ionosphere system, driving processes at kinetic, fluid, and global scales. Understanding these multiscale processes is crucial for a comprehensive grasp of solar-wind-magnetosphere interactions. This session focuses on studies using observational data and simulations to explore these interactions across various scales. At the global scale, we examine characteristics of geomagnetic storms and substorms as system responses to solar wind conditions. At the intermediate scale, we investigate phenomena such as convective flows, convective electric fields, electric current systems, Kelvin-Helmholtz (KH) instability in boundary layers, flux transfer events, high-speed jets, ULF waves, and auroral arcs. These phenomena are explored as consequences of various solar wind drivers and cross-region coupling, providing insights into the physical links within global processes. At the kinetic scale, we study kinetic processes and plasma waves to gain insights into energy dissipation mechanisms. We invite contributions that aim to elucidate multiscale dynamic processes governing energy transfer, particle acceleration, energy dissipation, and magnetosphere-ionosphere disturbances. By integrating data from space missions, ground-based observatories, and advanced numerical models, our approach will deepen the understanding of the magnetosphere-ionosphere system's responses to the solar wind, enhancing our ability to predict space weather.
Speakers
- Linggao Kong, Nanjing University, China
- Rajkumar Hajra, University of Science and Technology of China, China
- Shipra Sinha, NASA Goddard Space Flight Centre, United States of America
- Ahmad Lalti, Northumbria University, United Kingdom
- Xiaochao Yang, National Space Science Center, Chinese Academy of Sciences, China
- Senlin Xiong, National Space Science Center, CAS, China
- Niklas Grimmich, TU Braunschweig, Germany
- Su-ping Duan, National Space Science Center of Chinese Academy of Sciences, China
- Kristina Kislyakova, University of Vienna, Austria
- Manu Varghese, National Space Science Center (NSSC), China
- Fei He, Institute of Geology and Geophysics, Chinese Academy of Sciences, China
- Abiyot Workayehu, Helsinki, Finland
- Nozomu Nishitani, Nagoya University, Japan
- Shun-Rong Zhang, Massachusetts Institute of Technology, United States of America
- Yue Deng, University of Texas at Arlington, United States of America
- Bea Gallardo-Lacourt, NASA/CUA, United States of America
- Boyi Wang, Harbin Institute of Technology, Shenzhen, China
- Yunfang Zhong, Wuhan University, China
- Shreedevi Porunakatu Radhakrishna, Institute for Space-Earth Environmental Research, Japan
- Z.H. He, National Space Science Center, Chinese Academy of Sciences, China
- Tonghui Wang, Chinese Academy of Sciences, China
- Xu Wang, University of Chinese Academy of Sciences, China
- Yong Ren, Chinese Academy of Sciences, China
- Kailai Wang, University of Chinese Academy of Sciences, China
- Xiyu Liu, Beihang University, China
- C.-Philippe Escoubet, ESA/ESTEC, Netherlands
- Lei Dai, State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences,, China
- Nigang Liu, Sun Yat-sen University, China
- Timothy Keebler, University of Michigan, United States of America
- Syau-Yun Hsieh, Johns Hopkins University, United States of America
- Yiqun Yu, Beihang University, China
- Minghui Zhu, National Space Science Center, China
- Duan Zhang, National Space Science Center, CAS, China
- Wenhao Chen, Yunnan University, China
- Hyangpyo Kim, Austrian Academy of Sciences, Austria
- Yongcun Zhang, NSSC,CAS, China