Second harmonic poloidal waves observed by Van Allen Probes in the dusk‐midnight sector
Autor: | Kyungguk Min, R. J. Cohen, J. W. Manweiler, Aleksandr Ukhorskiy, A. Rualdo Soto-Chavez, Brian A. Larsen, J. Singer Howard, Seth G. Claudepierre, Kazue Takahashi, Harlan E. Spence |
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Rok vydání: | 2017 |
Předmět: |
Physics
Geomagnetic storm 010504 meteorology & atmospheric sciences Resonance Geophysics 01 natural sciences Computational physics Magnetic field Amplitude Space and Planetary Science Physics::Space Physics 0103 physical sciences Harmonic Wavenumber Van Allen Probes 010303 astronomy & astrophysics Ring current 0105 earth and related environmental sciences |
Zdroj: | Journal of Geophysical Research: Space Physics. 122:3013-3039 |
ISSN: | 2169-9402 2169-9380 |
DOI: | 10.1002/2016ja023770 |
Popis: | This paper presents observations of ultralow-frequency (ULF) waves from Van Allen Probes. The event that generated the ULF waves occurred 2 days after a minor geomagnetic storm during a geomagnetically quiet time. Narrowband pulsations with a frequency of about 7 mHz with moderate amplitudes were registered in the premidnight sector when Probe A was passing through an enhanced density region near geosynchronous orbit. Probe B, which passed through the region earlier, did not detect the narrowband pulsations but only broadband noise. Despite the single-spacecraft measurements, we were able to determine various wave properties. We find that (1) the observed waves are a second harmonic poloidal mode propagating westward with an azimuthal wave number estimated to be ∼100; (2) the magnetic field fluctuations have a finite compressional component due to small but finite plasma beta (∼0.1); (3) the energetic proton fluxes in the energy ranging from above 10 keV to about 100 keV exhibit pulsations with the same frequency as the poloidal mode and energy-dependent phase delays relative to the azimuthal component of the electric field, providing evidence for drift-bounce resonance; and (4) the second harmonic poloidal mode may have been excited via the drift-bounce resonance mechanism with free energy fed by the inward radial gradient of ∼80 keV protons. We show that the wave active region is where the plume overlaps the outer edge of ring current and suggest that this region can have a wide longitudinal extent near geosynchronous orbit. |
Databáze: | OpenAIRE |
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