First systematic identification of triple-mode Auroral Kilometric Radiation using Arase polarization data
Year: 2025
Type: article
Abstract: Auroral kilometric radiation (AKR), a fundamental plasma emission in Earth's magnetosphere, exhibits three characteristic modes: the right-handed extraordinary (R-X), left-handed ordinary (L-O) and left-handed extraordinary (L-X) modes. The role of AKR in magnetosphere−ionosphere−atmosphere coupling depends sensitively on its wave mode. While previous studies have primarily focused on the dominant R-X mode, we present the first systematic identification of all three modes using a practical polarization analysis method based on Arase satellite observations. This method employs a spin-axis-relative Ratio: when the satellite's spin axis aligns with the background magnetic field, a positive (negative) Ratio indicates the right-handed (left-handed) polarization, with reversal under anti-parallel conditions. Combined polarization-frequency analysis reveals that R-X, L-O, and L-X modes can exist in both dayside and nightside regions, with power spectral densities up to 10^-6 \rmmV^2\rmm^-2\rmHz^-1 . This study resolves long-standing ambiguities in AKR mode classification and has implications for understanding AKR-induced electron dynamics.
Source: Earth and Planetary Physics
DOI: 10.26464/epp2026004
Authors: He YiHua, Li SanGuang, Yang HongMing, Zhang Sai, Jin YuYue, Liu Si, Gao ZhongLei, Xiao FuLiang, He ZhaoGuo, Tang JiaWen, Li Ping
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $2,324
OpenAlex ID: W4414212598
