Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Licia C Ray"'
Autor:
Dong-Xiao Pan, Zhong-Hua Yao, Rui-Long Guo, Christopher S. Arridge, Licia C. Ray, Yong Zhao, George Clark, I. Jonathan Rae, Anthony T. Y. Lui, Bin-Zheng Zhang, Yong Wei, Xu-Zhi Zhou, Hui-Shan Fu, John E. P. Connerney, Scott J. Bolton
Publikováno v:
The Astrophysical Journal Letters, Vol 969, Iss 2, p L35 (2024)
Magnetic reconnection and current disruption are two key processes in driving energy conversion and dissipation in planetary magnetospheres. At the Earth, the two processes usually occur at different locations: the current disruption process occurs m
Externí odkaz:
https://doaj.org/article/8a018ba3467e499ba9c0ecd3fd15d6ee
Autor:
Japheth N. Yates, Licia C Ray
Publikováno v:
Magnetospheres in the Solar System
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18c7a4268fa974f9feeb02cd3768a933
https://doi.org/10.1002/9781119815624.ch31
https://doi.org/10.1002/9781119815624.ch31
Autor:
A. T. Y. Lui, Barry Mauk, Fran Bagenal, Ruilong Guo, Licia C Ray, Sarah V. Badman, Kazuo Yoshioka, Shengyi Ye, Steve Levin, I. J. Rae, Aikaterini Radioti, Tomoki Kimura, William Dunn, Denis Grodent, Zhonghua Yao, Bertrand Bonfond, William S. Kurth, Benjamin Palmaerts, J. C. Gérard, George Clark, Zuyin Pu, Scott Bolton, Jonathan D. Nichols
Publikováno v:
Geophysical Research Letters. 46:11632-11641
We present simultaneous observations of aurorae at Jupiter from the Hubble Space Telescope and Hisaki, in combination with the in situ measurements of magnetic field, particles, and radio waves from the Juno Spacecraft in the outer magnetosphere, fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b289aab72e94f374c2f50b7996f78d01
https://doi.org/10.1029/2019gl084201
https://doi.org/10.1029/2019gl084201
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:5097-5106
Routine spacecraft encounters with the Saturn current sheet due to the passage of aperiodic waves provide the opportunity to analyze the current sheet structure. The current density is expected to peak where the field strength reaches a minimum if ap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cebb2dc078929f2454282b74a3d9f762
https://doi.org/10.1029/2019ja026767
https://doi.org/10.1029/2019ja026767
Quasi-static potentials have long thought to be one of the significant drivers of the main ultraviolet emission associated with Jupiter’s auroral oval. The magnetic field lines connecting to the auroral zone extend into Jupiter’s middle magnetosp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a477539cb1084826885f76132002a93e
https://doi.org/10.5194/egusphere-egu21-16144
https://doi.org/10.5194/egusphere-egu21-16144
Autor:
Christopher T.S Lorch, Licia C. Ray, Clare E.J. Watt, Robert J. Wilson, Frances Bagenal, Frédéric Allegrini
New insights provided by Juno energetic particle detector measurements indicate signatures of Alfvénic acceleration are more common than previously anticipated. Studies at Earth show that Alfvén waves can substantially accelerate plasma within the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7fe242beb839b62ac7300f716014b0ed
https://doi.org/10.5194/epsc2020-252
https://doi.org/10.5194/epsc2020-252
Autor:
David J. Southwood, Joseph Kinrade, M. Felici, Licia C Ray, Carley Martin, Christopher Lorch, D. A. Constable, Rebecca Gray
Ionospheric outflow is the outward flow of atmospheric plasma, initiated by a loss of equilibrium along the magnetic field. Terrestrial ionospheric outflow presents as a polar wind triggered by the Dungey cycle, which drives much of Earth’s magneto
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8ced5e0369569b0e8d8d517db9cef7e4
https://doi.org/10.5194/epsc2020-369
https://doi.org/10.5194/epsc2020-369
The effects of the solar wind on Saturn’s magnetosphere are poorly constrained as there are no consistent solar wind monitors upstream of the planet. This has limited previous studies of the solar wind’s influence on the Saturnian magnetosphere t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8d990d325278c43f9340479ed2a1dee3
https://doi.org/10.5194/epsc2020-771
https://doi.org/10.5194/epsc2020-771
Ionospheric outflow is the flow of plasma initiated by a loss of equilibrium along a magnetic field line, which induces an ambipolar electric field due to the separation of electrons and ions in a gravitational field and other mass‐dependent source
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9ea320a969e9fc0e1eb0a6a840ce05e
https://doi.org/10.1029/2019JA027727
https://doi.org/10.1029/2019JA027727
Autor:
Chris Lorch, D. A. Constable, Carley Martin, M. Felici, Rebecca Gray, Joe Kinrade, Licia C Ray
Publikováno v:
Journal of Geophysical Research: Space Physics. 125
Ionospheric outflow is driven by an ambipolar electric field induced due to the separation of electrons and ions in a gravitational field when equilibrium along a magnetic field line is lost. A model of ionospheric outflow at Saturn was developed usi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d25c4b27ca361c09f9039f0b7522519
https://doi.org/10.1029/2019ja027728
https://doi.org/10.1029/2019ja027728