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
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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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How Do Ultra‐Low Frequency Waves Access the Inner Magnetosphere During Geomagnetic Storms?
Geophysical Research Letters, 2019 Wave‐particle interactions play a key role in radiation belt dynamics. Traditionally, ultra‐low frequency (ULF) wave‐particle interaction is parameterized statistically by a small number of controlling factors for given solar wind driving conditions or ...
I. J. Rae +9 more
semanticscholar +1 more source
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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Analysis of plasma waves observed in the inner Saturn magnetosphere [PDF]
Annales Geophysicae, 2008 Plasma waves observed in the Saturn magnetosphere provide an indication of the plasma population present in the rotationally dominated inner magnetosphere.
J. D. Menietti +5 more
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Observational evidence of the drift-mirror plasma instability in Earth's inner magnetosphere
Physics of Plasmas, 2019 We report on evidence for the generation of an ultra-low frequency plasma wave by the drift-mirror plasma instability in the dynamic plasma environment of Earth's inner magnetosphere.
A. Soto-Chavez +7 more
semanticscholar +1 more source
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