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Global MHD modeling of resonant ULF waves: Simulations with and without a plasmasphere
- Source :
- Journal of Geophysical Research. Space Physics
- Publication Year :
- 2016
- Publisher :
- John Wiley and Sons Inc., 2016.
-
Abstract
- We investigate the plasmaspheric influence on the resonant mode coupling of magnetospheric ultralow frequency (ULF) waves using the Lyon‐Fedder‐Mobarry (LFM) global magnetohydrodynamic (MHD) model. We present results from two different versions of the model, both driven by the same solar wind conditions: one version that contains a plasmasphere (the LFM coupled to the Rice Convection Model, where the Gallagher plasmasphere model is also included) and another that does not (the stand‐alone LFM). We find that the inclusion of a cold, dense plasmasphere has a significant impact on the nature of the simulated ULF waves. For example, the inclusion of a plasmasphere leads to a deeper (more earthward) penetration of the compressional (azimuthal) electric field fluctuations, due to a shift in the location of the wave turning points. Consequently, the locations where the compressional electric field oscillations resonantly couple their energy into local toroidal mode field line resonances also shift earthward. We also find, in both simulations, that higher‐frequency compressional (azimuthal) electric field oscillations penetrate deeper than lower frequency oscillations. In addition, the compressional wave mode structure in the simulations is consistent with a radial standing wave oscillation pattern, characteristic of a resonant waveguide. The incorporation of a plasmasphere into the LFM global MHD model represents an advance in the state of the art in regard to ULF wave modeling with such simulations. We offer a brief discussion of the implications for radiation belt modeling techniques that use the electric and magnetic field outputs from global MHD simulations to drive particle dynamics.<br />Key Points Magnetosphere responds as a resonant waveguide to ULF fluctuations in solar wind dynamic pressureInclusion of a plasmasphere has a substantial impact on the nature of the simulated ULF wavesInclusion of a plasmasphere leads to a deeper penetration of azimuthal electric field oscillations
- Subjects :
- 010504 meteorology & atmospheric sciences
Field line
Plasmasphere
Magnetosphere: Inner
waveguide
01 natural sciences
7. Clean energy
Solar Wind/Magnetosphere Interactions
Standing wave
resonant ULF wave coupling
Polar CaP Phenomena
plasmasphere
Electric field
0103 physical sciences
MHD waves and instabilities
Magnetospheric Physics
field line resonance
010303 astronomy & astrophysics
Numerical Modeling
Research Articles
0105 earth and related environmental sciences
Physics
Magnetospheric Physics (SMP)
MHD waves and turbulence
global MHD simulation
Geophysics
Plasma and MHD instabilities
Computational physics
Magnetic field
Interplanetary Physics
Solar wind
Inner Magnetosphere Coupling: Recent Advances
13. Climate action
Space and Planetary Science
Physics::Space Physics
Space Plasma Physics
Planetary Sciences: Comets and Small Bodies
radiation belts
Magnetohydrodynamics
Longitudinal wave
Research Article
Subjects
Details
- Language :
- English
- ISSN :
- 21699402 and 21699380
- Volume :
- 121
- Issue :
- 1
- Database :
- OpenAIRE
- Journal :
- Journal of Geophysical Research. Space Physics
- Accession number :
- edsair.doi.dedup.....4cd3054edcdfe46d2855e9ddf1054120