Results 221 to 230 of about 24,725 (253)

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

open access: yesNPJ Microgravity
Slaba TC   +6 more
europepmc   +1 more source

Anomalous transient enhancement of planetary ion escape at Mars. [PDF]

open access: yesNat Commun
Zhang C   +19 more
europepmc   +1 more source

The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission. [PDF]

open access: yesSpace Sci Rev
Walsh BM   +25 more
europepmc   +1 more source

Remote sensing of mercury sodium exospheric patterns in relation to particle precipitation and interplanetary magnetic field. [PDF]

open access: yesSci Rep
Orsini S   +12 more
europepmc   +1 more source

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.   +11 more
openaire   +5 more sources

Callisto in the Magnetosphere of Jupiter

Solar System Research, 2020
The study of the Galilean satellites can help clarify the structure of the magnetospheric magnetic field from observations of their projections along magnetic field lines in the atmosphere/ionosphere of Jupiter, where patches of auroras appear. UV auroras in projections on the ionosphere of Io, Europe and Ganymede occur almost permanently, while the ...
openaire   +2 more sources

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

Home - About - Disclaimer - Privacy