Results 111 to 120 of about 17,759 (228)
Unlike Earth, Mars lacks a global intrinsic magnetic field but has regional crustal magnetic fields concentrated in its southern hemisphere. This unique configuration leads to distinctive interactions with the solar wind.
Yangjun Chen +8 more
doaj +1 more source
Statistics of the Interplanetary Magnetic Field from 0.1 to 30 au. II. Dynamical Variability
The interplanetary magnetic field (IMF) governs the coupling between the solar wind and planetary magnetospheres through a series of complex interactions.
Jiutong Zhao +10 more
doaj +1 more source
Three-dimensional Global Hybrid Simulation of Magnetosheath Jets at Mercury
Plasma high-speed jets are common in Earth’s magnetosheath, and they significantly perturb the magnetosheath and affect the magnetosphere. The space environment of Mercury, characterized by the bow shock, magnetosheath, and magnetosphere, shares many ...
Jin Guo +10 more
doaj +1 more source
Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets [PDF]
A computational model for the determination of the detailed plasma and magnetic field properties of the global interaction of the solar wind with nonmagnetic terrestrial planetary obstacles is described.
Spreiter, J. R., Stahara, S. S.
core +1 more source
Plasma Environment, Radiation, Structure, and Evolution of the Uranian System (PERSEUS): A Dedicated Orbiter Mission Concept to Study Space Physics at Uranus. [PDF]
Cohen IJ +13 more
europepmc +1 more source
Electron Acceleration in Magnetic Islands in Quasi-parallel Shocks
We report new theories and simulations for electron acceleration in magnetic islands generated by magnetic reconnection in the shock turbulence in a quasi-parallel shock, using a 2 and 1/2 dimensional particle-in-cell simulation. When an island is moving,
N. Bessho +6 more
doaj +1 more source
To understand the ion injection for diffusive shock acceleration in space and astrophysical shock waves, such as in planetary bow shocks and supernova remnant shocks, ion heating and acceleration in high-Alfvén-Mach-number ( M _A ) quasi-parallel shock ...
N. Bessho +5 more
doaj +1 more source
Particles accelerated by shocks in the heliosphere [PDF]
The populations of energetic ions accelerated by shocks in the heliosphere are reviewed briefly.
Lee, Martin A.
core +1 more source
Double Beam Instability for the Mercury Upstream Waves
Mercury shock-upstream region is plasma physically of great interest, as the solar wind plasma may encounter two ion beams, forming a double-beam plasma system. Properties of the double-beam instability are studied semianalytically using the magnetoionic
Y. Narita +3 more
doaj +1 more source

