Results 31 to 40 of about 637,520 (196)
Erosion of the inner magnetosphere during geomagnetic storms [PDF]
Annales Geophysicae, 1997 Using the empirical magnetic field model dependent on the Dst index and solar wind dynamic pressure, we calculated the behaviour of the contour B = Bs in the equatorial plane of the magnetosphere where Bs is the magnetic field in the subsolar point ...
E. Y. Feshchenko, Y. P. Maltsev
doaj +1 more source
Modeling Inner Magnetospheric Electrodynamics [PDF]
, 2013 We describe a model of inner magnetospheric electrodynamics that couples the Rice Convection Model (RCM) to an equilibrium magnetic field model. The equilibrium model is a modified version of the Hesse-Birn [1993] magnetofriction code, adapted for use in the inner magnetosphere.
F. R. Toffoletto +4 more
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Spatial spreading of magnetospherically reflected chorus elements in the inner magnetosphere [PDF]
Annales Geophysicae, 2013 Abstract. Chorus-type whistler waves are known to be generated in the vicinity of the magnetic equator, in the low-density plasma trough region. These wave packets propagate towards the magnetic poles, deviating from the magnetic field lines, before being eventually reflected at higher latitudes.
H. Breuillard +7 more
openaire +3 more sources
Global 3D MHD Simulations of Waves in Accretion Discs
EPJ Web of Conferences, 2013 We discuss results of the first global 3D MHD simulations of warp and density waves in accretion disks excited by a rotating star with a misaligned dipole magnetic field. A wide range of cases are considered.
Romanova M.M., Lovelace R.V.E.
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Nowcast model for low‐energy electrons in the inner magnetosphere [PDF]
Space Weather, 2015 AbstractWe present the nowcast model for low‐energy (<200 keV) electrons in the inner magnetosphere, which is the version of the Inner Magnetosphere Particle Transport and Acceleration Model (IMPTAM) for electrons. Low‐energy electron fluxes are very important to specify when hazardous satellite surface‐charging phenomena are considered.
Ganushkina, N. Yu. +3 more
openaire +2 more sources
, 2011 In this paper we consider the effect of a self-consistently computed magnetodisc field structure on the magnetosphere-ionosphere coupling current system at Jupiter.
Jonathan D. Nichols (7590554)
core +7 more sources
3D MHD Simulations of Waves Excited in an Accretion Disk by a Rotating Magnetized Star
EPJ Web of Conferences, 2014 We present results of global 3D MHD simulations of warp and density waves in accretion disks excited by a rotating star with a misaligned dipole magnetic field. A wide range of cases are considered.
Lovelace R.V.E., Romanova M.M.
doaj +1 more source
Does Ring Current Heating Generate the Observed O+ Shell?
Geophysical Research Letters, 2020 The Naval Research Laboratory (NRL) Sami3 is Also a Model of the Ionosphere (SAMI3) ionosphere/plasmasphere code is used to examine the effect of ring current heating during a storm. With a ring current heating function added to SAMI3, a cold thermal (
J. Krall, J. D. Huba, M.‐C. Fok
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Two types of ion spectral gaps in the quiet inner magnetosphere: Interball-2 observations and modeling [PDF]
Annales Geophysicae, 2002 We analyse measurements of ion spectral gaps (ISGs) observed by the ION particle spectrometer on board the Interball-2 satellite. The ISG represents a sharp decrease in H+ flux at a particular narrow energy range.
N. Y. Buzulukova +9 more
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Electron cyclotron harmonic waves in Jovian magnetosphere as seen by Juno
Frontiers in Astronomy and Space Sciences, 2023 Electron cyclotron harmonic (ECH) waves along with whistler mode waves are suggested to be responsible for causing the persistent diffuse aurora in Jupiter.
J. Joseph +5 more
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