Results 131 to 140 of about 916 (176)

Closed magnetic topology in the Venusian magnetotail and ion escape at Venus. [PDF]

open access: yesNat Commun
Xu S   +13 more
europepmc   +1 more source

The anomalous state of Uranus's magnetosphere during the Voyager 2 flyby. [PDF]

open access: yesNat Astron
Jasinski JM   +9 more
europepmc   +1 more source

Mars's induced magnetosphere can degenerate. [PDF]

open access: yesNature
Zhang Q   +7 more
europepmc   +1 more source

A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]

open access: yesJ Geophys Res Space Phys
Salohub A   +3 more
europepmc   +1 more source

Comparison of a new magnetosphere–magnetosheath model with Interball-1 magnetosheath plasma measurements

Planetary and Space Science, 2005
Abstract We report a testing of the earlier developed in the Institute of Mechanics of the Bulgarian Academy of Sciences numerical data-based 3D model of the system magnetosphere–magnetosheath with real satellite data. The model is a result of a self-consistent solution of two tasks: (i) Chapman–Ferraro problem for an arbitrary 3D magnetopause with ...
G N Zastenker
exaly   +2 more sources

The Magnetosheath

Space Science Reviews, 2005
International ...
Lucek, E. A.   +7 more
openaire   +3 more sources

The Magnetosheath and Magnetotail of Venus

Space Science Reviews, 1991
We describe the observational history and assess the current understanding of the magnetosheath and magnetotail of Venus, stressing recent developments. We make recommendations for research that can be done using existing observations, as well as desirable trajectory and instrumentation characteristics for future spacecraft missions.
John L. Phillips, David J. McComas
openaire   +2 more sources

magnetosheath lion roars

Journal of Geophysical Research, 1976
The characteristics of lion roars, which are intense packets of electromagnetic waves characteristically found in the magnetosheath, are studied. The average frequency of the emissions is 120 Hz, with over 90% occurring between 90 and 160 Hz (which is near one-half the local electron gyrofrequency); over 70% of all emissions last a mere 2 sec or less ...
Edward J. Smith, Bruce T. Tsurutani
openaire   +1 more source

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