Observational Evidence for Three Time‐Scale Modulations in the Pulsating Aurora

Abstract We report an Arase‐all sky imager (ASI) conjugate event in which the pulsating aurora (PsA) has a one‐to‐one correspondence with chorus bursts. Wavelet analysis displayed three peaks at ∼0.3 Hz, 4 Hz, and >10 Hz, corresponding to the main pulsation, internal modulation, and fast modulation, respectively. These correspond to the old terms of ∼5–15 s pulsations, chorus risers/elements and subelements/subpackets, respectively. Electron “microbursts” correspond to the 4‐Hz peak. The internal and fast modulations are further verified by the analysis based on fast Fourier transform analyses. Moreover, the spatial distributions of the Fourier spectral amplitude show that the internal and fast modulations are well‐structured within auroral patches. The above results indicate a paradigm shift away from quasilinear theory which implicitly assumes diffuse wave generation. The three time‐scale modulations are consistent with coherent chorus which has been theoretically argued to lead to pitch angle transport three orders of magnitude faster.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-08-15
DOI
https://doi.org/10.1029/2024gl108253
Citations
7
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
2.32
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article

Observational Evidence for Three Time‐Scale Modulations in the Pulsating Aurora

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7 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
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article

Observational Evidence for Three Time‐Scale Modulations in the Pulsating Aurora

Rui Chen, Yoshiya Kasahara, Satoko Nakamura, Shoya Matsuda, Iku Shinohara, Yasunobu Ogawa, Xinliang Gao, Shin‐ichiro Oyama, Tomoaki Hori, Quanming Lu, Ayako Matsuoka, Keisuke Hosokawa, B. T. Tsurutani, Yoshizumi Miyoshi
article en
7 citations

Abstract

Abstract We report an Arase‐all sky imager (ASI) conjugate event in which the pulsating aurora (PsA) has a one‐to‐one correspondence with chorus bursts. Wavelet analysis displayed three peaks at ∼0.3 Hz, 4 Hz, and >10 Hz, corresponding to the main pulsation, internal modulation, and fast modulation, respectively. These correspond to the old terms of ∼5–15 s pulsations, chorus risers/elements and subelements/subpackets, respectively. Electron “microbursts” correspond to the 4‐Hz peak. The internal and fast modulations are further verified by the analysis based on fast Fourier transform analyses. Moreover, the spatial distributions of the Fourier spectral amplitude show that the internal and fast modulations are well‐structured within auroral patches. The above results indicate a paradigm shift away from quasilinear theory which implicitly assumes diffuse wave generation. The three time‐scale modulations are consistent with coherent chorus which has been theoretically argued to lead to pitch angle transport three orders of magnitude faster.

Geophysical Research LettersVol. 51(16)
Kanazawa University (JP), Pasadena City College (US), University of Science and Technology of China (CN), University of Electro-Communications (JP), Kyoto University (JP), Japan Aerospace Exploration Agency (JP), National Institute of Polar Research (JP), Center for Excellence in Molecular Cell Science (CN), Institute of Space and Astronautical Science (JP), Nagoya University (JP)
Openalex Percentile: Top 12%
Ionosphere and magnetosphere dynamics
2.32
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