Results 231 to 240 of about 5,188 (295)

Simulations of the interaction of the solar wind with planetary magnetospheres : from Mercury to Uranus, the part of the planetary rotation

, 2018
Léa Griton
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Field-particle energy transfer during chorus emissions in space. [PDF]

Nature
Liu CM, Zhao BN, Cao JB, Pollock CJ, Russell CT, Liu YY, Xing XN, Linqvist PA, Burch JL.   +8 more
europepmc   +1 more source

Oceanic and ionospheric tidal magnetic fields extracted from global geomagnetic observatory data. [PDF]

Philos Trans A Math Phys Eng Sci
Tyler RH, Trossman DS.
europepmc   +1 more source

Global-scale magnetosphere convection driven by dayside magnetic reconnection. [PDF]

Nat Commun
Dai L, Zhu M, Ren Y, Gonzalez W, Wang C, Sibeck D, Samsonov A, Escoubet P, Tang B, Zhang J, Branduardi-Raymont G.   +10 more
europepmc   +1 more source

Planetary magnetospheres: The double tilt of Uranus [PDF]

Nature, 1986
Torsion de plus de 60° par rapport a l'axe de rotation de l'axe du champ magnetique d'Uranus, decouverte par Voyager ...
F. Bagenal
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Planetary Magnetospheres

2007
The physical interaction of a planetary object with the surrounding plasma varies according to the properties of both the object and the plasma flow in which it is embedded. A planets that has a substantial internal magnetic field is surrounded by a region within the external plasma—a magnetosphere—that extends the planet's influence beyond its surface
Margaret Galland Kivelson, Fran Bagenal
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Plasma Motions in Planetary Magnetospheres

Science, 1991
Before direct exploration by spacecraft, Jupiter was the only planet other than Earth that was known to have a magnetic field, as revealed by its nonthermal radio emissions. The term "magnetosphere" did not exist because there was no clear concept of such an entity.
A. J. Dessler, T. W. Hill
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Planetary Ionospheres and Magnetospheres

2008
We begin this chapter with a detailed review of the ionization and recombination processes in a planetary ionosphere, as exemplified by the ionosphere we know the most about, that of the Earth. We then extend the discussion to the ionospheres of Mars and Venus, and examine atmospheric loss mechanisms.
Eugene F. Milone, William J. F. Wilson
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Reconnection in planetary magnetospheres

Advances in Space Research, 2000
Current sheets in planetary magnetospheres that lie between regions of "oppositely-directed" magnetic field are either magnetopause-like, separating plasmas with different properties, or tail-like, separating plasmas of rather similar properties. The magnetopause current sheets generally have a nearly limitless supply of magnetized plasma that can ...
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Dust in planetary magnetospheres

Advances in Space Research, 1993
Abstract Dust particles immersed in the magnetized plasma environment of planetary magnetospheres collect electrostatic charges. The expected charges are modest and only micron and smaller grains will be significantly perturbed by the resulting electrodynamic forces. These electrodynamic perturbations compete with other processes - radiation pressure,
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