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• W2897641331 abstract "Abstract We report narrow band‐filtered imaging observations of the Jovian H 3 + 3.4‐μm emission using the IRCS (infrared camera and spectrograph) on the Subaru telescope taken on 25 May 2016. Approximately 1 hr of data was taken at intervals of 45–110 s, with high spatial resolution (~0.2 arcsec) using adaptive optics. In the northern polar region, we found bright patch‐like emissions on the poleward side of the main oval. One of them had a pulsation period of ~10 min. We utilized an H 3 + emission model to investigate the response time of the H 3 + emission to abrupt and periodic variations of the precipitating electron flux. The model showed that the H 3 + emission could pulsate with this timescale due to a modulated flux of the precipitating electrons in the kilo‐electron‐volt to tens of kilo‐electron‐volt energy range." @default.
• W2897641331 created "2018-10-26" @default.
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• W2897641331 date "2018-11-05" @default.
• W2897641331 modified "2023-10-17" @default.
• W2897641331 title "Pulsation Characteristics of Jovian Infrared Northern Aurora Observed by the Subaru IRCS with Adaptive Optics" @default.
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• W2897641331 doi "https://doi.org/10.1029/2018gl079411" @default.
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