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

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

Afiliação

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 em En | MEDLINE | ID: mdl-38105161

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article