Three-year of observations of Jupiter's aurora and Io plasma torus variabilities by earth orbiting extreme-ultraviolet spectroscope HISAKI

F. Tsuchiya, K. Yoshioka, T. Kimura, G. Murakami, C. Tao, H. Kita, I. Yoshikawa, A. Yamazaki, Y. Kasaba

Research output: Contribution to journalConference article

1 Citation (Scopus)

Abstract

Extreme Ultraviolet spectrograph, EXCEED, on-board the HISAKI satellite is designed for observing tenuous gas and plasma around planets in the solar system. It enables us to obtain continuous and long-term data set and find time variability in the planetary magnetosphere and ionosphere with time scales of several hours to months. Here, we introduce new findings of Jupiter's UV aurora and plasma emissions from the Io plasma torus obtained from the HISAKI observation.

Original languageEnglish
Article number012069
JournalJournal of Physics: Conference Series
Volume869
Issue number1
DOIs
Publication statusPublished - 2017 Jul 11
EventInternational Conference Frontiers in Theoretical and Applied Physics, FTAPS 2017 - Sharjah, United Arab Emirates
Duration: 2017 Feb 222017 Feb 25

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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