Observation and origin of non-thermal hard X-rays from Jupiter-Reference-Cited by-同舟云学术

Observation and origin of non-thermal hard X-rays from Jupiter

Published:2022-02-10 Issue:4 Volume:6 Page:442-448
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Mori Kaya^ORCID,Hailey Charles,Bridges Gabriel,Mandel Shifra^ORCID,Garvin Amani,Grefenstette Brian,Dunn William^ORCID,Hord Benjamin J.^ORCID,Branduardi-Raymont Graziella,Clarke John,Jackman Caitriona^ORCID,Nynka Melania,Ray Licia^ORCID

Funder

NASA | NASA’s Goddard Space Flight Center | Astrophysics Science Division

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01594-8.pdf

Reference45 articles.

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3. Millan, R. M., Lin, R. P., Smith, D. M., Lorentzen, K. R. & McCarthy, M. P. X-ray observations of MeV electron precipitation with a balloon-borne germanium spectrometer. Geophys. Res. Lett. 29, 2194 (2002).

4. Foat, J. E. et al. First detection of a terrestrial MeV X-ray burst. Geophys. Res. Lett. 25, 4109–4112 (1998).

5. Branduardi-Raymont, G. et al. A study of Jupiter’s aurorae with XMM-Newton. Astron. Astrophys. 463, 761–774 (2007).

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