Results 171 to 180 of about 103,405 (350)
Comment on low energy electron measurements in the Jovian magnetosphere [PDF]
R. Grard, S. E. Deforest, E. C. Whipple
openalex +1 more source
Abstract Jupiter's auroral regions have previously been defined by broad‐scale auroral structures, but these are typically obscured by the wide array of temporal variability observed at timescales between minutes and days, making it difficult to understand the underlying magnetospheric biases driving these brightness differences.
Tom S. Stallard +9 more
wiley +1 more source
Current Systems in the Earth's Magnetosphere
N. Ganushkina, M. Liemohn, S. Dubyagin
semanticscholar +1 more source
Jupiter’s magnetosphere and aurorae observed by the Juno spacecraft during its first polar orbits
J. Connerney +21 more
semanticscholar +1 more source
On the role of finite inertia and resistivity in axisymmetric pulsar magnetospheres [PDF]
Y.- M. Wang
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Combined Full Wave and Test Particle Simulations of the Io Footprint in the Jovian Aurora
Abstract It is known that the perturbation of the co‐rotating plasma of Jupiter by Io propagates as Alfvén waves along the magnetic field lines. These waves accelerate electrons, which leads to precipitation and the formation of an auroral footprint on the ionosphere.
W. W. Eshetu +3 more
wiley +1 more source
Laboratory Modelling of Neutron Star Magnetospheres [PDF]
Б. Г. Еремин +4 more
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Large‐Amplitude ExB Plasma Drifts in the High‐Latitude Ionosphere
Abstract We investigate the fastest ExB plasma drifts observed by the Vector Electric Field Instrument double probe experiment on the NASA's Dynamics Explorer‐2 (DE‐2) satellite. In the limited DE‐2 database, we find 507 events where the zonal ExB velocity exceeds 4 km/s, in which for 91 events the velocity exceeds 6 km/s and 16 events where the drifts
H. Laakso, R. Pfaff
wiley +1 more source
Adiabatic Motions of Charged Particles in a Dipole Model of the Magnetosphere
E. W. Hones
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Parametric Dependence of Linear and Nonlinear Growth of Whistler‐Mode Chorus Waves
Abstract We calculated the linear and nonlinear growth rates of whistler‐mode chorus waves with relativistic treatment across different wave frequencies and investigated their dependence on the associated parameters, including background magnetic field strength, cold electron density, and energetic electron temperature.
Tian Zhang +2 more
wiley +1 more source

