Revealing the source of Jupiter’s x-ray auroral flares

Author:

Yao Zhonghua12ORCID,Dunn William R.345,Woodfield Emma E.6ORCID,Clark George7ORCID,Mauk Barry H.7ORCID,Ebert Robert W.89,Grodent Denis10ORCID,Bonfond Bertrand10ORCID,Pan Dongxiao1ORCID,Rae I. Jonathan11ORCID,Ni Binbin1213ORCID,Guo Ruilong10ORCID,Branduardi-Raymont Graziella3ORCID,Wibisono Affelia D.35ORCID,Rodriguez Pedro14ORCID,Kotsiaros Stavros15ORCID,Ness Jan-Uwe14ORCID,Allegrini Frederic89ORCID,Kurth William S.16ORCID,Gladstone G. Randall89ORCID,Kraft Ralph4ORCID,Sulaiman Ali H.16ORCID,Manners Harry17ORCID,Desai Ravindra T.17ORCID,Bolton Scott J.8ORCID

Affiliation:

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

2. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China.

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

4. Harvard-Smithsonian Center for Astrophysics, Smithsonian Astrophysical Observatory, Cambridge, MA, USA.

5. The Centre for Planetary Science at UCL/Birkbeck, Gower Street, London WC1E 6BT, UK.

6. British Antarctic Survey, Cambridge, UK.

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

8. Space Science and Engineering Division, Southwest Research Institute, San Antonio, TX, USA.

9. Department of Physics and Astronomy, University of Texas at San Antonio, San Antonio, TX, USA.

10. Laboratoire de Physique Atmosphérique et Planétaire, STAR institute, Université de Liège, Liège, Belgium.

11. Northumbria University, Newcastle upon Tyne, UK.

12. Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, Hubei, China.

13. CAS Center for Excellence in Comparative Planetology, Hefei, Anhui, China.

14. European Space Agency (ESA), European Space Astronomy Centre (ESAC), Camino Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Madrid, Spain.

15. NASA Goddard Space Flight Center, Greenbelt, MD, USA.

16. Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA.

17. Blackett Laboratory, Imperial College London, London, UK.

Abstract

Jupiter’s unique x-ray aurora is driven by the same processes as Earth’s: Heavy ion scattering by electromagnetic waves.

Funder

Natural Environment Research Council

Science and Technology Facilities Council

Royal Society

National Natural Science Foundation of China

SAO fellowship to Harvard-Smithsonian Centre for Astrophysics and by European Space Agency

Strategic Priority Research Program of Chinese Academy of Sciences

B-type Strategic Priority Program of the Chinese Academy of Sciences

The pre-research projects on Civil Aerospace Technologies

IGGCAS

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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