Stormtime Energetics: Energy Transport Across the Magnetopause in a Global MHD Simulation
Frontiers in Astronomy and Space Sciences, 2021 Coupling between the solar wind and magnetosphere can be expressed in terms of energy transfer through the separating boundary known as the magnetopause.
Austin Brenner +5 more
doaj +1 more source
Dynamics of the Innermost Accretion Flows Around Compact Objects: Magnetosphere-Disc Interface, Global Oscillations and Instabilities [PDF]
, 2012 We study global non-axisymmetric oscillation modes and instabilities in magnetosphere- disc systems, as expected in neutron star X-ray binaries and possibly also in accreting black hole systems.
Abramowicz +58 more
core +1 more source
PARTICLES, NEUTRINO AND PHOTONS IN THE MAGNETOSPHERE OF A COLLAPSING STAR
Odessa Astronomical Publications, 2014 The formation of the stellar magnetosphere during the gravitational collapse is discussed. Primary protons and electrons accelerate in the star’s magnetosphere during its gravitational collapse.
V. G. Kryvdyk
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Propeller outflows from an MRI disc [PDF]
, 2013 We present the results of axisymmetric simulations of MRI-driven accretion onto a rapidly rotating, magnetized star accreting in the propeller regime.
Koldoba, Alexander V. +4 more
core +1 more source
Solar-Terrestrial Physics, 2022 In this paper, we study parameters of geomagnetic pulsations in the 1–4 mHz frequency range (Pc5/Pi3) in the magnetotail, utilizing data obtained by Cluster satellites at different levels of fluctuations in the interplanetary magnetic field (IMF) and the
Yagova N. V. +2 more
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ULF Waves Modulating and Acting as Mass Spectrometer for Dayside Ionospheric Outflow Ions
Geophysical Research Letters, 2019 Ionospheric outflow has been shown to be a dominant ion source of Earth's magnetosphere. However, most studies in the literature are about ionospheric outflow injected into the nightside magnetosphere.
Z.‐Y. Liu +11 more
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Magnetosphere-Ionosphere Coupling: Implications of Non-Equilibrium Conditions
Frontiers in Astronomy and Space Sciences, 2022 The response times of the coupled magnetosphere-ionosphere-thermosphere system are, on average, greater than the autocorrelation timescales of solar wind forcing. This means that the system is rarely, if ever, in equilibrium.
Mike Lockwood, Stan W. H. Cowley
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Pulsar Magnetosphere : A General Relativistic Treatment
, 2004 A fully general relativistic description of the pulsar magnetosphere is provided. To be more concrete, a study of the pulsar magnetosphere is performed in the context of general relativistic magnetohydrodynamics (MHD) employing the so-called Grad ...
Kim, Hongsu +3 more
core +4 more sources
Geophysical Monograph Series, Page i-xiv., 2020 This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.
Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions
Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
wiley +1 more source
Energy Transport by Kelvin-Helmholtz Instability at the Magnetopause
Fluids, 2019 By means of the formation of vortices in the nonlinear phase, the Kelvin Helmholtz instability is able to redistribute the flux of energy of the solar wind that flows parallel to the magnetopause. The energy transport associated with the Kelvin Helmholtz
Francesco Palermo
doaj +1 more source