Results 61 to 70 of about 59,334 (317)
Solar-Terrestrial Physics, 2019 We have studied the effect of the β solar wind parameter (equal to the ratio of the plasma pressure to the magnetic pressure) on statistical characteristics of the Ap index reflecting the triggering behavior of the activity of Earth’s magnetosphere.
Zotov O.D. +2 more
doaj +1 more source
Frontiers in Astronomy and Space Sciences, 2023 Introduction: During recent years magnetosheath plasma structures called “jets” are identified in spacecraft data as localized regions in the magnetosheath where the dynamic pressure is enhanced compared to the background.
Marius Echim +9 more
doaj +1 more source
MHD Simulations of Magnetospheric Accretion, Ejection and Plasma-field Interaction [PDF]
, 2013 We review recent axisymmetric and three-dimensional (3D) magnetohydrodynamic (MHD) numerical simulations of magnetospheric accretion, plasma-field interaction and outflows from the disk-magnetosphere boundary.
arxiv +1 more source
Kinetic Modeling of Magnetospheres [PDF]
, 2020 This paper presents the state of the art of kinetic modeling techniques for simulating plasma kinetic dynamics in magnetospheres. We describe the critical numerical techniques for enabling large-scale kinetic simulations of magnetospheres: parameter scaling, implicit Particle-in-Cell schemes, and fluid-kinetic coupling.
arxiv +1 more source
The relationship between the magnetosphere and magnetospheric/auroral substorms [PDF]
Annales Geophysicae, 2013 Abstract. On the basis of auroral and polar magnetic substorm studies, the relationship between the solar wind-magnetosphere dynamo (the DD dynamo) current and the substorm dynamo (the UL dynamo) current is studied. The characteristics of both the DD and UL currents reveal why auroral substorms consist of the three distinct phases after the input power
openaire +4 more sources
Frontiers in Astronomy and Space Sciences, 2023 We present a study of the electron magnetohydrodynamics Grad–Shafranov (GS) reconstruction of the electron diffusion region (EDR) of magnetic reconnection.
D. Korovinskiy +6 more
doaj +1 more source
Pulsar Magnetosphere Dynamics [PDF]
arXiv, 2021 With the neutron star rotating under a stationary magnetic field generating unipolar induction, charges are driven to the pulsar surface according to their signs, and are uploaded to the magnetosphere along the magnetic field lines. In the presence of an electron-positron plasma, the pulsar magnetosphere is represented by a unique magnetohydrodynamic ...
arxiv
Dawn–dusk asymmetries in the coupled solar wind–magnetosphere–ionosphere system: a review [PDF]
, 2014 . Dawn–dusk asymmetries are ubiquitous features of the coupled solar-wind–magnetosphere–ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more ...
A. Walsh +10 more
semanticscholar +1 more source
Geophysical Research LettersWe examined rapid variations in the electron zebra stripe patterns, specifically at L = 1.5, over a three‐month duration, using twin Van Allen Probes within Earth's inner magnetosphere. During geomagnetically quiet intervals, these stripes exhibit a peak‐
Megha Pandya +4 more
doaj +1 more source
Earth and Planetary Physics, 2018 We present preliminary results of a new global Magnetohydrodynamics (MHD) simulation model of the Jovian magnetosphere. The model incorporates mass loading from Jupiter's satellite Io, the planet's fast corotation, and electrostatic coupling between its ...
YuXian Wang +4 more
doaj +1 more source