Affiliation:
1. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China
2. Colleage of Earth and Planetary Science University of Chinese Academy of Sciences Beijing China
3. Space and Atmospheric Physics Group Department of Physics Imperial College London London UK
4. Key Laboratory of Space Weather National Center for Space Weather China Meteorological Administration Beijing China
5. Max Planck Institute for Solar System Research Goettingen German
Abstract
AbstractBoundary dynamics are crucial for the transport of energy, mass, and momentum in geospace. The recently discovered plasmapause surface wave (PSW) plays a key role in the inner magnetosphere dynamics. However, a comprehensive investigation of spatial variations of the PSW remains absent. In this study, we elucidate the spatial characteristics of a PSW through observations from multiple spacecrafts in the magnetosphere. Following the initiation of the PSW, quasi‐periodic injections of energetic ions, rather than electrons, are suggested to serve as energy source of the PSW. Based on the distinct wave and particle signatures, we categorize the PSW into four regions: seed region, growth region, stabilization region and decay region, spanning from nightside to afternoon plasmapause. These findings advance our understanding of universal boundary dynamics and contribute to a deeper comprehension of the pivotal roles of surface waves in the energy couplings within the magnetosphere‐plasmasphere‐ionosphere system.
Funder
National Natural Science Foundation of China
National Key Research and Development Program of China
Youth Innovation Promotion Association of the Chinese Academy of Sciences
Publisher
American Geophysical Union (AGU)
Cited by
1 articles.
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