Spatially Asymmetric Increase in Hot Electron Fraction in the Io Plasma Torus During Volcanically Active Period Revealed by Observations by Hisaki/EXCEED From November 2014 to May 2015-Reference-Cited by-同舟云学术

Spatially Asymmetric Increase in Hot Electron Fraction in the Io Plasma Torus During Volcanically Active Period Revealed by Observations by Hisaki/EXCEED From November 2014 to May 2015

Published:2020-02-25 Issue:3 Volume:125 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Hikida R.¹^ORCID,Yoshioka K.²^ORCID,Tsuchiya F.³^ORCID,Kagitani M.³^ORCID,Kimura T.⁴^ORCID,Bagenal F.⁵^ORCID,Schneider N.⁵^ORCID,Murakami G.⁶^ORCID,Yamazaki A.⁶^ORCID,Kita H.⁶^ORCID,Nerney E.⁵,Yoshikawa I.²^ORCID

Affiliation:

1. Department of Earth and Planetary ScienceThe University of Tokyo Bunkyo Japan

2. Department of Complexity Science and EngineeringThe University of Tokyo Bunkyo Japan

3. Planetary Plasma and Atmospheric Research CenterTohoku University Sendai Japan

4. Frontier Research Institute for Interdisciplinary SciencesTohoku University Sendai Japan

5. Laboratory for Atmospheric and Space PhysicsUniversity of Colorado Boulder Boulder CO USA

6. Institute of Space and Astronautical Science (ISAS)Japan Aerospace Exploration Agency (JAXA) Sagamihara Japan

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027100

Reference54 articles.

1. Empirical model of the Io plasma torus: Voyager measurements

2. Flow of mass and energy in the magnetospheres of Jupiter and Saturn

3. Dawn-dusk electric field asymmetry of the Io plasma torus

4. NRL Plasma Formulary. Revision

5. The Response of Jupiter's Magnetosphere to an Outburst on Io

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