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Akademický článek

In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements

Autor: Y. Xu, C. S. Arridge, Z. H. Yao, B. Zhang, L. C. Ray, S. V. Badman, W. R. Dunn, R. W. Ebert, J. J. Chen, F. Allegrini, W. S. Kurth, T. S. Qin, J. E. P. Connerney, D. J. McComas, S. J. Bolton, Y. Wei

Publikováno v: Nature Communications, Vol 15, Iss 1, Pp 1-9 (2024)

Abstract The magnetospheric cusp connects the planetary magnetic field to interplanetary space, offering opportunities for charged particles to precipitate to or escape from the planet. Terrestrial cusps are typically found near noon local time, but

Externí odkaz: https://doaj.org/article/d6c7d3de53de4ed68847871fa9b0548b

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Akademický článek

The magnetosheath at high spectral resolution

Autor: K. D. Küntz, D. Koutroumpa, W. R. Dunn, A. Foster, F. S. Porter, D. G. Sibeck, B. Walsh

Publikováno v: Earth and Planetary Physics, Vol 8, Iss 1, Pp 234-246 (2024)

While we eagerly anticipate SMILE’s (Solar wind Magnetosphere Ionosphere Link Explorer) unprecedented X-ray observations of the Earth’s magnetosheath and the initiation of a new era of magnetospheric research, it seems appropriate to look ahead t

Externí odkaz: https://doaj.org/article/832139efd54b4f318d6029b90b596e4a

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Akademický článek

A Survey of Magnetic Field Line Curvature in Jovian Dawn Magnetodisc

Autor: W. D. Gu, Z. H. Yao, Y. Wei, T. S. Qin, B. Z. Zhang, Y. Xu, W. R. Dunn, P. A. Delamere, Y. N. Chen

Publikováno v: Geophysical Research Letters, Vol 51, Iss 1, Pp n/a-n/a (2024)

Abstract The Jovian magnetosphere is highly dynamic, influenced by both solar wind and internal processes associated with the rapid planetary rotation and Io's volcanic activities. Accompanying the mass and energy circulations driven by the magnetosp

Externí odkaz: https://doaj.org/article/06b8ca35a1764dd69eaaa5debec6e4b1

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Akademický článek

On the Relation Between Jupiter's Aurora and the Dawnside Current Sheet

Autor: Y. Xu, Z. H. Yao, B. Zhang, P. A. Delamere, L. C. Ray, W. R. Dunn, S. V. Badman, E. H. Feng, Z. Q. Zheng, S. J. Bolton, D. Grodent, B. Bonfond, Y. Wei

Publikováno v: Geophysical Research Letters, Vol 50, Iss 13, Pp n/a-n/a (2023)

Abstract Jupiter's auroral emission is a spectacular phenomenon that provides insight into energy release processes related to the coupling of its magnetosphere and ionosphere. This energy release is influenced by solar wind conditions. Using joint o

Externí odkaz: https://doaj.org/article/f08b626d32d343fcb90ddf7129a34661

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Jupiter’s equatorial X-ray emissions over two solar cycles

Autor: A D Wibisono, G Branduardi-Raymont, A J Coates, W R Dunn, R J French

Publikováno v: Monthly Notices of the Royal Astronomical Society. 521:5596-5603

Jupiter’s disc is bright in X-rays as H2 molecules in the atmosphere are very effective at scattering solar X-rays. K-shell fluorescence from carbon atoms in atmospheric methane is thought to also provide a minor contribution. XMM–Newton has now

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::279d2440779e425af0d7a300015eb132
https://doi.org/10.1093/mnras/stad905

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