Results 81 to 90 of about 940 (176)
Hybrid-Vlasov simulation of soft X-ray emissions at the Earth’s dayside magnetospheric boundaries
Solar wind charge exchange produces emissions in the soft X-ray energy range which can enable the study of near-Earth space regions such as the magnetopause, the magnetosheath and the polar cusps by remote sensing techniques. The Solar wind Magnetosphere
M. Grandin +7 more
doaj +1 more source
Mirror-mode (MM) structures, characterized by intermittent sharp depressions or enhancements of magnetic magnitude, are key plasma-instability-driven phenomena and commonly observed in high- β and temperature-anisotropic space plasmas.
C. Q. Wang +5 more
doaj +1 more source
The Soft X-ray Imager (SXI) on board the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) spacecraft will be able to view the Earth’s magnetosheath in soft X-rays.
Andrew Read
doaj +1 more source
Turbulence properties in the solar wind change with increasing heliospheric distance. Observations from different missions have shown how spectral indices converge toward an f ^−5/3 spectrum in the inertial range as the solar wind reaches 1 au and how ...
Victor Montagud-Camps +10 more
doaj +1 more source
Magnetosheath Jets Over Solar Cycle 24: An Empirical Model. [PDF]
Vuorinen L +3 more
europepmc +1 more source
Jets and Mirror Mode Waves in Earth's Magnetosheath. [PDF]
Blanco-Cano X +3 more
europepmc +1 more source
Plasma acceleration and boundary compression in the magnetosheath of Mars under low-Alfvén-Mach-number solar wind. [PDF]
Qiao F +20 more
europepmc +1 more source
Simultaneous Mars-orbit observations reveal Kelvin-Helmholtz instability-driven bulk atmospheric ion escape. [PDF]
Zhang C +13 more
europepmc +1 more source
Induced magnetosphere of Mars responds fast to interplanetary magnetic field rotation. [PDF]
Lin R +13 more
europepmc +1 more source

