Results 81 to 90 of about 67,260 (280)
A Predictive Model of the Position of Plasmapause Based on Lunar Phase and Deep Learning Framework
Abstract The plasmapause position is crucial for understanding magnetospheric dynamics and space weather forecasting. This study pioneers the integration of lunar phase (LP) into plasmapause modeling using two neural network architectures (BP and fully connected neural network) and a large database of 37,869 crossing events from 1977 to 2015.
Yajun Li+11 more
wiley +1 more source
Control of the Jovian Magnetopause by Iogenic Plasma: Initial Results From Global MHD Simulations
The size and variability of Jupiter's magnetosphere are not only determined by upstream conditions but also substantially influenced by internal processes within Jupiter's magnetosphere, specifically the dynamics of the rotation magnetodisc.
Enhao Feng+6 more
doaj +1 more source
Theory of Disk Accretion onto Magnetic Stars
Disk accretion onto magnetic stars occurs in a variety of systems, including accreting neutron stars (with both high and low magnetic fields), white dwarfs, and protostars.
Lai, Dong
core +2 more sources
Are There Magnetars in High Mass X-ray Binaries? The Case of SuperGiant Fast X-Ray Transients [PDF]
In this paper we survey the theory of wind accretion in high mass X-ray binaries hosting a magnetic neutron star and a supergiant companion. We concentrate on the different types of interaction between the inflowing wind matter and the neutron star ...
Bamba A.+10 more
core +1 more source
Abstract Energetic particle deep penetration into low L‐shells (L < 4) impacts the dynamics of the radiation belts and ring current. Previous studies reported that electrons penetrate more frequently, deeply, and faster than protons of similar energies, but underlying mechanisms are unclear.
Rui Chen+4 more
wiley +1 more source
Statistical analysis of plasma turbulence using Cluster II data
The possibility of using different statistical approaches to the description of the turbulent and dynamic processes in the Earth's magnetosphere is represented.
L. V. Kozak, B. A. Petrenko
doaj +1 more source
On the magnetosphere of an accelerated pulsar [PDF]
matches published ...
Samuel E. Gralla, T. Daniel Brennan
openaire +3 more sources
Unveiling the Global Characteristics of Turbulence in the Venusian Space Environment
Abstract Turbulence plays a crucial role in energy transfer from large to small scales in solar wind‐Venus interaction. Observations have identified magnetic field fluctuations and turbulence in the Venusian space environment. However, due to limited observations and simulation resolutions, neither the global characteristics nor the driving mechanisms ...
Tong Dang+8 more
wiley +1 more source
Global explicit particle-in-cell simulations of the nonstationary bow shock and magnetosphere
We carry out two-dimensional global particle-in-cell simulations of the interaction between the solar wind and a dipole field to study the formation of the bow shock and magnetosphere.
Hu, Huidong+6 more
core +1 more source
Electrospherics and magnetospherics [PDF]
In the second part of a two-part article, additional experiments with small spheres of magnetic material are described. Not only are the results interesting in themselves, but also it is hoped that they may serve as analogs for such phenomena as Brownian movement, thermal movement of molecules, crystal formation, bacterial chaining, and others.
openaire +1 more source