Why chorus waves are the dominant driver for diffuse auroral precipitation.

Gao, Xinliang; Ma, Jiuqi; Shao, Tong; Chen, Rui; Ke, Yangguang; Lu, Quanming

Gao, Xinliang; Ma, Jiuqi; Shao, Tong; Chen, Rui; Ke, Yangguang; Lu, Quanming.

Afiliación

Gao X; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China.
Ma J; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China.
Shao T; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China.
Chen R; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China.
Ke Y; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China.
Lu Q; Deep Space Exploration Laboratory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China; CAS Center for Excellence in Comparative Planetology, Hefei 230026, China. Electronic address: qmlu@ustc.edu.cn.

Sci Bull (Beijing) ; 69(5): 597-600, 2024 Mar 15.

Article en En | MEDLINE | ID: mdl-38105161

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Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Sci Bull (Beijing) Año: 2024 Tipo del documento: Article País de afiliación: China

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