Response of Jupiter's Aurora to Plasma Mass Loading Rate Monitored by the Hisaki Satellite During Volcanic Eruptions at Io

Author:

Kimura T.1ORCID,Hiraki Y.2,Tao C.3ORCID,Tsuchiya F.4ORCID,Delamere P. A.5,Yoshioka K.6ORCID,Murakami G.7ORCID,Yamazaki A.7ORCID,Kita H.4ORCID,Badman S. V.8ORCID,Fukazawa K.9,Yoshikawa I.6ORCID,Fujimoto M.710

Affiliation:

1. Nishina Center for Accelerator-Based Science; RIKEN; Wako Saitama Japan

2. Advanced Knowledge Laboratory, Inc.; Shinjuku Japan

3. National Institute of Information and Communications Technology; Tokyo Japan

4. Planetary Plasma and Atmospheric Research Center; Tohoku University; Sendai Japan

5. Geophysical Institute; University of Alaska Fairbanks; Fairbanks AK USA

6. Department of Complexity Science and Engineering; University of Tokyo; Kashiwa Japan

7. Institute of Space and Astronautical Science; Japan Aerospace Exploration Agency; Sagamihara Japan

8. Department of Physics; Lancaster University; Lancaster UK

9. Academic Center for Computing and Media Studies; Kyoto University; Kyoto Japan

10. Earth-Life Science Institute; Tokyo Institute of Technology; Tokyo Japan

Funder

Japan Society for the Promotion of Science

MAEDI

International Space Science Institute (ISSI)

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference80 articles.

1. 1. Transport of mass, momentum and energy in planetary magnetodisc regions;Achilleos;Space Science Reviews,2014

2. Weakening of Jupiter's main auroral emission during January 2014;Badman;Geophysical Research Letters,2016

3. The ionization source near Io from Galileo wake data;Bagenal;Geophysical Research Letters,1997

4. The magnetosphere of Jupiter: Coupling the equator to the poles;Bagenal;Journal of Atmospheric and Solar: Terrestrial Physics,2007

5. Flow of mass and energy in the magnetospheres of Jupiter and Saturn;Bagenal;Journal of Geophysical Research,2011

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