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Whistler Mode Quasiperiodic Emissions: Contrasting Van Allen Probes and DEMETER Occurrence Rates
Journal article   Peer reviewed

Whistler Mode Quasiperiodic Emissions: Contrasting Van Allen Probes and DEMETER Occurrence Rates

F. Němec, O. Santolík, G. B. Hospodarsky, M. Hajoš, A. G. Demekhov, W. S. Kurth, M. Parrot and D. P. Hartley
Journal of geophysical research. Space physics, Vol.125(4), e2020JA027918
04/2020
DOI: 10.1029/2020JA027918

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Abstract

Quasiperiodic emissions are magnetospheric whistler mode waves at frequencies between about 0.5 and 4 kHz which exhibit a nearly periodic time modulation of the wave intensity. We use large data sets of events observed by the Van Allen Probes in the equatorial region at larger radial distances and by the low‐altitude DEMETER spacecraft. While Van Allen Probes observe the events at all local times and longitudes, DEMETER observations are limited nearly exclusively to the daytime and significantly less frequent at the longitudes of the South Atlantic Anomaly. Further, while the events observed by Van Allen Probes are smoothly distributed over seasons with only mild maxima in spring/autumn, DEMETER occurrence rate has a single pronounced minimum in July. The apparent inconsistency is explained by considering a nondipolar Earth's magnetic field and significant background wave intensities which in these cases prevent the quasiperiodic events from being identified in DEMETER data. Key Points Van Allen Probes observe the quasiperiodic events at all local times and longitudes, but more often during spring and autumn seasons DEMETER observes the events nearly exclusively during the day, with a significant longitudinal variation and minimum occurrence in July The difference is explained by nondipolar Earth's magnetic field and by background wave intensities complicating DEMETER observations
 DEMETER QP emissions quasiperiodic emissions RBSP

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