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In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft. [PDF]

Nat Commun
Rabia J, Hue V, Louis CK, André N, Nénon Q, Szalay JR, Prangé R, Lamy L, Zarka P, Collet B, Allegrini F, Ebert RW, Greathouse TK, Bonfond B, Gladstone GR, Sulaiman AH, Kurth WS, Connerney JEP, Louarn P, Penou E, Kamran A, Santos-Costa D, Giles RS, Kammer JA, Versteeg MH, Bolton SJ.   +25 more
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The Pulsar Magnetosphere

Astrophysics and Space Science, 2000
Domains of the pulsar magnetosphere, both within and without the light-cylinder, are studied under varying provisional assumptions. Some of the qualitative features emerging should persist in the ultimate synthesis of a completely self-consistent model.
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Pulsar magnetospheres

Nature Physical Science, 1971
Abstract The energy loss from the neutron star - as inferred from the secular increase in rotation period - is much greater than that emitted in either the radio or the other observed wavelengths. A primary motivation of magnetospheric theory is to trace the mode in which this energy and the associated angular momentum are in fact ...
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Magnetospheric Wind

Science, 1969
An experiment designed to detect the bulk flow of cool plasma within the magnetosphere has been flown on the ATS-1 (Applications Technology Satellite) synchronous satellite. This experiment has yielded evidence for gusts of streaming positive ions in the magnetospheric equatorial plane. This directed ion flow is interpreted as the result of large-scale
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Magnetospheric turbulence and properties of magnetospheric dynamics

Advances in Space Research, 2008
Abstract High level of turbulence is one of the main peculiarities inherent to magnetospheric dynamics. Mechanisms for generation of magnetospheric turbulence are analyzed. The instabilities in the plasma pressure distribution are examined as source of large and medium scale modes in the turbulence spectra.
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Cluster at the Magnetospheric Cusps

Space Science Reviews, 2005
International ...
Cargill, P.J., Lavraud, B., J. Owen, C., Grison, B., Dunlop, M.W., Cornilleau-Wehrlin, N., Escoubet, C.P., Paschmann, G., Phan, T.D., Rezeau, L., Bogdanova, Y., Nykyri, K.   +11 more
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Magnetosphere

ACM SIGGRAPH 2007 posters, 2007
Kumiko Kushiyama, Shinji Sasada, Masashi Yasada, Yuji Suzumura   +3 more
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Magnetospheric Energy Principle for Spherically Symmetric Monopolar Magnetospheres

Physical Review Letters, 2013
A new magnetospheric energy principle is developed for spherically symmetric monopolar magnetospheres with open straight field lines. The principle is based on the self-adjointness of the force operator, which ensures energy conservation in the unperturbed magnetospheric plasma volume. A Neuman-type boundary condition for the perpendicular displacement
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The international magnetospheric study

Acta Astronautica, 1974
Abstract During the past 15 years, the study of the earth's magnetosphere—man's immediate plasma and radiation environment—has undergone a successful stage of discovery and exploration. We have obtained a morphological description of the magnetospheric field, the particle population embedded in it, and its interface with the solar wind, and we have ...
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The solar wind-magnetosphere dynamo and the magnetospheric substorm

Planetary and Space Science, 1975
Abstract In a quiet condition, the solar wind kinetic energy is converted into electrical energy. A small part of this energy is dissipated as heat energy in the polar ionosphere. We identify at least three types of magnetospheric disturbances which are not associated with an increase of the heat production and call them reversible disturbances ...
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