Results 271 to 280 of about 102,442 (313)

Electrostatic solitary wave modeling in lunar wake plasma. [PDF]

Sci Rep
Singh K, Varghese SS, Kourakis I.
europepmc   +1 more source

Juno Observations Set New Constraints on the Electrodynamic Interaction Between Io and Jupiter. [PDF]

J Geophys Res Space Phys
Kotsiaros S, Connerney JEP, Saur J, Kokkalis A, Herceg M, Martos YM, Schlegel S, Jørgensen JL, Bolton SJ.   +8 more
europepmc   +1 more source

Extreme two-phase change of ionospheric electron temperature overshoot during geomagnetic storms. [PDF]

Sci Rep
Smirnov A, Shprits Y, Lühr H, Pignalberi A, Kronberg E, Prol F, Xiong C.   +6 more
europepmc   +1 more source

Validated space radiation exposure predictions from earth to mars during Artemis-I. [PDF]

NPJ Microgravity
Slaba TC, Rahmanian S, George S, Laramore D, Norbury JW, Werneth CM, Zeitlin C.   +6 more
europepmc   +1 more source

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Tail of the magnetosphere

Journal of Geophysical Research, 1965
Tangential stress effects on magnetosphere tail with regard to magnetic field intensity and direction, trapped particle fluxes and low energy cosmic ray cut ...
H. E. Petschek, W. I. Axford, G. L. Siscoe   +2 more
openaire   +2 more sources

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.
Elizaveta Antonova, Elizaveta Antonova
openaire   +2 more sources

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
openaire   +5 more sources

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.
openaire   +2 more sources

A survey of low-energy electrons in the evening sector of the magnetosphere with OGO 1 and OGO 3.

, 1968
Observations of electrons of energy 125 ev to ∼2 kev with the OGO 1 satellite and of electrons of energy 40 ev to ∼2 kev with OGO 3 (by means of modulated Faraday cup detectors) are used to investigate the low-energy electron population in the ...
V. Vasyliūnas
semanticscholar   +1 more source

The Terrestrial Magnetosphere

1998
A magnetosphere is shaped by the interaction between a planetary magnetic field and the solar wind. The magnetopause is a discontinuity separating both fields, forming a cavity in the solar wind. Since the solar wind is a supersonic flow, a standing shock wave, the bow shock, develops in front of the magnetopause.
openaire   +2 more sources