2021
DOI: 10.1029/2021ja029826
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Nonlinear Signatures of VLF‐Triggered Emissions: A Simulation Study

Abstract: Whistler-mode chorus emissions with rising-tone and falling-tone frequencies have been studied for more than half a century. Chorus emissions are often observed outside the plasmapause in conjunction with magnetospheric substorms (Tsurutani & Smith, 1974). Chorus emissions are essentially nonlinear phenomena induced by finite amplitude waves as evidenced by the triggered emissions from the VLF transmitters, which exhibit the same frequency spectra with varying frequencies (see a review by Omura et al., 1991;Go… Show more

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Cited by 19 publications
(42 citation statements)
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“…By pumping a triggering wave at the equator, Nogi et al. (2020) and Nogi and Omura (2021) have produced the downward frequency chirping and electron hills in the phase space, which is consistent with the theoretical predictions proposed by Nunn (1974) and Omura et al. (2008).…”
Section: Conclusion and Discussionsupporting
confidence: 73%
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“…By pumping a triggering wave at the equator, Nogi et al. (2020) and Nogi and Omura (2021) have produced the downward frequency chirping and electron hills in the phase space, which is consistent with the theoretical predictions proposed by Nunn (1974) and Omura et al. (2008).…”
Section: Conclusion and Discussionsupporting
confidence: 73%
“…This has been further supported by numerical simulations, in which the electron holes (Nunn & Omura, 2015;Tao et al, 2017) or hills (Nunn & Omura, 2012;Nogi & Omura, 2021;Nogi et al, 2020) are formed. By pumping a triggering wave at the equator, Nogi et al (2020) and Nogi and Omura (2021) have produced the downward frequency chirping and electron hills in the phase space, which is consistent with the theoretical predictions proposed by Nunn (1974) and Omura et al (2008). While in our simulation, the waves are self-consistently excited by anisotropic electrons, exhibiting an upward chirping followed by a downward chirping (known as a hooked spectrogram).…”
Section: Conclusion and Discussionmentioning
confidence: 65%
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“…The most intense waves are initially linearly excited with small wave‐normal angles near the magnetic equator by anisotropic electrons injected from the plasma sheet (Artemyev et al., 2016 ; Kennel, 1966 ; LeDocq et al., 1998 ; Li et al., 2010 ; Tsurutani & Smith, 1974 ). Next, nonlinear wave growth takes over, leading to the formation of intense rising tone chorus elements, typically lasting more than 100 ms (Demekhov & Trakhtengerts, 2008 ; Nogi & Omura, 2021 ; Nunn, 1974 ; Omura et al., 2008 ; Tao et al., 2017 , 2021 ). During nonlinear wave growth, the geomagnetic field inhomogeneity controls the formation of an electron hole at cyclotron resonance with the wave (Karpman et al., 1974 ; Nunn, 1974 ) and the resulting resonant current leads to a simultaneous increase of wave amplitude and wave frequency, explaining the observed long rising tone elements (Demekhov et al., 2017 ; Omura et al., 2008 ; Summers et al., 2013 ).…”
Section: Introductionmentioning
confidence: 99%