Presentation Information
[PPS01-13]Volcanic Control of Jupiter's Aurora and Middle Magnetosphere Dynamics Observed by Hisaki/EXCEED
*Chihiro Tao1, Tomoki Kimura2, Fuminori Tsuchiya3, Go Murakami4, Kazuo Yoshioka5, Atsushi Yamazaki4, Sarah V Badman6, Hiroaki Misawa3, Hajime Kita3, Yasumasa Kasaba3, Ichiro Yoshikawa5, Masaki Fujimoto4 (1.National Institute of Information and Communications Technology, 2.Riken, 3.Tohoku University, 4.ISAS/JAXA, 5.University of Tokyo, 6.Lancaster University)
Keywords:
Hisaki,Jupiter,Aurora
Temporal variation of Jupiter's northern aurora during enhanced Io volcanic activity was detected using the EXCEED spectrometer on board the Hisaki Earth-orbiting planetary space telescope. It was found that in association with reported Io volcanic events in early 2015, auroral power and estimated field-aligned currents were enhanced during day of year 40–120. Furthermore, the far ultraviolet color ratio decreased during the event, indicating a decrease of auroral electron mean energy and total acceleration by <30%. During the episode of enhanced Io volcanic activity, Jupiter's magnetosphere contains more source current via increased suprathermal plasma density by up to 42%; therefore, it would have required correspondingly less electron acceleration to maintain the enhanced field-aligned current and corotation enforcement current. Sporadic large enhancements in auroral emission detected more frequently during the active period could have been contributed by non-adiabatic magnetospheric energization.