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Quasi-periodic ELF/VLF emissions with atypical time structure inside the plasmasphere
Some results of observations on board the Van Allen probe A spacecraft of atypical quasi-periodic VLF
electromagnetic emissions inside the plasmasphere are discussed. We study in detail two events (December
6, 2015 and November 24, 2015) of the generation of deeply modulated quasi-periodic VLF emissions (QP)
in the frequency band below 2 kHz, when separate relatively short (on the order of 20 and 60 s) bursts
of hiss without any notable frequency drift repeated with a period of 90 and 240 s. The emissions selected
for analysis were not accompanied by a hydromagnetic compression wave, which indicates the impossibility
of their interpretation in terms of the concept of QP 1 modulated hiss. For the considered events, no clear
periodicity of spectral bursts typical for QP 2 emissions take place. The dynamic spectra analysis makes it
possible to conclude that the cyclotron generation of electromagnetic emissions occurs in the regions of the
electron radiation belts with relatively dense cold plasma. The time course of these emissions can be explained
under the assumption of a periodic modification of the conditions for the reflection of whistler wave incident
on the ionosphere from above. Based on the available data and calculations, it was concluded that it is possible
to interpret the analysed atypical quasi-periodic VLF emissions as a result of the resonant parametric action
of ionospheric infrasonic waves with periods close to the repetition period of spectral bursts in quasi-periodic
emissions.