How Jupiter’s unusual magnetospheric topology structures its aurora

Author:

Zhang Binzheng123ORCID,Delamere Peter A.4ORCID,Yao Zhonghua5ORCID,Bonfond Bertrand6ORCID,Lin D.3ORCID,Sorathia Kareem A.7ORCID,Brambles Oliver J.8,Lotko William39ORCID,Garretson Jeff S.7,Merkin Viacheslav G.7ORCID,Grodent Denis6ORCID,Dunn William R.10,Lyon John G.711ORCID

Affiliation:

1. Department of Earth Sciences, The University of Hong Kong, Hong Kong SAR, China.

2. Laboratory for Space Research, The University of Hong Kong, Hong Kong SAR, China.

3. High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA.

4. Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USA.

5. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.

6. LPAP, Space sciences, Technologies and Astrophysics Research (STAR), Institute Université de Liége (ULiége), Liége, Belgium.

7. Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA.

8. O.J. Brambles Consulting, Preston, UK.

9. Thayer School of Engineering, Dartmouth College, Hanover, NH, USA.

10. Mullard Space Science Laboratory, University College London, Dorking, UK.

11. Gamera Consulting, Hanover, NH, USA.

Abstract

Jupiter’s slow dayside magnetic merging and fast rotation produce an unusual magnetic topology that can explain its polar aurora.

Funder

National Aeronautics and Space Administration

Research Grant Council

PRODEX

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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