A brightening of Jupiter’s auroral 7.8-μm CH4 emission during a solar-wind compression-Reference-Cited by-同舟云学术

A brightening of Jupiter’s auroral 7.8-μm CH4 emission during a solar-wind compression

Published:2019-04-08 Issue:7 Volume:3 Page:607-613
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Sinclair J. A.^ORCID,Orton G. S.,Fernandes J.,Kasaba Y.,Sato T. M.^ORCID,Fujiyoshi T.,Tao C.,Vogt M. F.^ORCID,Grodent D.,Bonfond B.^ORCID,Moses J. I.,Greathouse T. K.,Dunn W.^ORCID,Giles R. S.,Tabataba-Vakili F.,Fletcher L. N.,Irwin P. G. J.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-019-0743-x.pdf

Reference46 articles.

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2. Kim, S. J., Caldwell, J., Rivolo, A. R., Wagener, R. & Orton, G. S. Infrared polar brightening on Jupiter. III. Spectrometry from the Voyager 1 IRIS experiment. Icarus 64, 233–248 (1985).

3. Flasar, F. M. et al. An intense stratospheric jet on Jupiter. Nature 427, 132–135 (2004).

4. Grodent, D., Gérard, J.-C., Clarke, J. T., Gladstone, G. R. & Waite, J. H. A possible auroral signature of a magnetotail reconnection process on Jupiter. J. Geophys. Res. Space 109, A05201 (2004).

5. Nichols, J. D. et al. Response of Jupiter’s auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno. Geophys. Res. Lett. 44, 7643–7652 (2017).

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