Identification of Jupiter’s magnetic equator through H3+ ionospheric emission-Reference-Cited by-同舟云学术

Identification of Jupiter’s magnetic equator through H3+ ionospheric emission

Published:2018-07-23 Issue:10 Volume:2 Page:773-777
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Stallard Tom S.^ORCID,Burrell Angeline G.^ORCID,Melin Henrik,Fletcher Leigh N.,Miller Steve,Moore Luke,O’Donoghue James^ORCID,Connerney John E. P.,Satoh Takehiko,Johnson Rosie E.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-018-0523-z.pdf

Reference23 articles.

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2. Smith, E. J. et al. Jupiter’s magnetic field, magnetosphere, and interaction with the solar wind—Pioneer 11. Science 188, 451–455 (1975).

3. Connerney, J. E. P. The magnetic field of Jupiter—a generalized inverse approach. J. Geophys. Res. 86, 7679–7693 (1981).

4. Connerney, J. E. P., Acuña, M. H., Ness, N. F. & Satoh, T. New models of Jupiter’s magnetic field constrained by the Io flux tube footprint. J. Geophys. Res. 103, 11929–11940 (1998).

5. Connerney, J. E. P. Treatise on Geophysics Vol. 10 (eds Schubert, G. & Spohn, T.) (Elsevier, Oxford, 2007).

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