Results 91 to 100 of about 103,965 (278)
Abstract Stable auroral red (SAR) arcs are luminous subauroral emissions produced by the collisional excitation of oxygen atoms during geomagnetically active times. While traditionally attributed to inner magnetospheric electron heating, recent observations and simulations challenge the exclusivity of this mechanism.
Jing Liu +9 more
wiley +1 more source
On the self-consistent model of the axisymmetric radio pulsar magnetosphere
We consider a model of axisymmetric neutron star magnetosphere. In our approach, the current density in the region of open field lines is constant and the returning current flows in a narrow layer along the separatrix.
Beskin, V. S., Malyshkin, L. M.
core +1 more source
Chorus Wave–Driven Electron Dynamics in the Van Allen Belts: From Coherence to Diffusion
Abstract The Van Allen radiation belts contain relativistic electrons trapped by Earth's magnetic field, posing serious risks to spacecraft. Chorus waves are known to accelerate these electrons via resonant interactions, but these interactions are inherently nonlinear and coherent.
Xin Tao +4 more
wiley +1 more source
Solar Wind—Magnetosphere Coupling Functions: Pitfalls, Limitations, and Applications
Solar wind‐magnetosphere coupling functions have now been in use for almost 50 years. In that time, a very large number of formulations have been proposed.
Mike Lockwood
doaj +1 more source
The modulation of SiO maser polarization by Jovian planets
Searching for planets in the atmosphere of AGB stars is difficult, due to confusion with the stellar wind and pulsations. The aim here is to provide a complementary strategy for planet search in such a dense environment.
Alexeev +48 more
core +2 more sources
Knowledge of the ion composition in the near-Earth’s magnetosphere and plasma sheet is essential for the understanding of magnetospheric processes and instabilities.
E. Kronberg +15 more
semanticscholar +1 more source
Abstract This meeting report summarizes outcomes from the AGU Chapman Conference on Particle Precipitation: Drivers, Properties, and Impacts on Atmosphere, Ionosphere, Magnetosphere (AIM) Coupling, held 14–21 February 2025, in Melbourne, Australia. This conference brought together scientists from around the world to identify pressing AIM open science ...
A. W. Breneman +8 more
wiley +1 more source
Explicit IMF By Dependence in Geomagnetic Activity: Modulation of Precipitating Electrons
The most important driver of geomagnetic activity is the north–south ( Bz) component of the interplanetary magnetic field (IMF), which dominates the solar wind‐magnetosphere coupling and all solar wind coupling functions.
L. Holappa, T. Asikainen, K. Mursula
doaj +1 more source
Kinetic-scale magnetic turbulence and finite Larmor radius effects at Mercury
We use a nonstationary generalization of the higher-order structure function technique to investigate statistical properties of the magnetic field fluctuations recorded by MESSENGER spacecraft during its first flyby (01/14/2008) through the near Mercury ...
Alexandrova +89 more
core +1 more source
Abstract A mathematical and numerical framework is developed for modeling Earth's magnetic field and optimizing the trajectory of the whole system using geomagnetic observations. The conventional approach is adopted to model Earth's magnetic field in the source‐free region via the Gauss coefficient, for which the fast dynamical component for the mantle‐
Kuan Li
wiley +1 more source

