Results 31 to 40 of about 20,122 (200)
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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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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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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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.
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Modeling of the Jovian Magnetosphere [PDF]
Annales Geophysicae, 2005 This paper presents a global model of the Jovian magnetosphere which is valid not only in the equatorial plane and near the planet, as most of the existing models are, but also at high latitudes and in the outer regions of the magnetosphere. The model
I. I. Alexeev, E. S. Belenkaya
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A statistical study of the global structure of the ring current [PDF]
, 2004 [1] In this paper we derive the average configuration of the ring current as a function of the state of the magnetosphere as indicated by the Dst index.
Hughes, W. J. +3 more
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Recirculation of plasmasphere material during idealized magnetic storms
Frontiers in Physics, 2023 The fate of flux tube material once it is eroded from of the plasmasphere through a dayside plume remains unknown. The eroded plasmasphere material can be either swept away by the solar wind and lost from Earth’s system, or recirculated into the inner ...
Christian-Andrew Bagby-Wright +4 more
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