2009
DOI: 10.1016/j.jastp.2009.03.023
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Plasmaspheric hiss overview and relation to chorus

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Cited by 38 publications
(46 citation statements)
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“…Recent ray trace modeling has shown that hiss originates from a subset of chorus emissions that avoid Landau damping during propagation from the equatorial source region to higher latitude. Such waves also propagate to lower L where they enter and are trapped within the plasmasphere, where the discrete chorus emissions merge together to form incoherent hiss (Bortnik et al 2008b(Bortnik et al , 2009a. The unexpected association between hiss and chorus has been confirmed by simultaneous observations on two THEMIS spacecraft ) and differences in the statistical MLT distribution of the two emissions has been explained by 3D ray tracing (Chen et al 2009b).…”
Section: Fig 2 Spectrogram Of Waves Observed On Combined Release Andmentioning
confidence: 87%
“…Recent ray trace modeling has shown that hiss originates from a subset of chorus emissions that avoid Landau damping during propagation from the equatorial source region to higher latitude. Such waves also propagate to lower L where they enter and are trapped within the plasmasphere, where the discrete chorus emissions merge together to form incoherent hiss (Bortnik et al 2008b(Bortnik et al , 2009a. The unexpected association between hiss and chorus has been confirmed by simultaneous observations on two THEMIS spacecraft ) and differences in the statistical MLT distribution of the two emissions has been explained by 3D ray tracing (Chen et al 2009b).…”
Section: Fig 2 Spectrogram Of Waves Observed On Combined Release Andmentioning
confidence: 87%
“…For reviews of hiss observations, see Hayakawa and Sazhin [1992], Bortnik et al [2009], and the introduction to Tsurutani et al [2015]. These waves are characteristically broadband, spanning several kHz.…”
Section: Introductionmentioning
confidence: 99%
“…Although a variety of electromagnetic "hisses" have been observed with ground-based instruments and reported in the literature starting in the late 1950s [e.g., Ellis, 1959] (see reviews by Hayakawa and Sazhin [1992] and Bortnik et al [2009a]), it is important to distinguish PH as an emission that is only observed in space; that is, it was discovered and observed with the first high-altitude spacecraft [Dunckel and Helliwell, 1969;Russell et al, 1969] and named "plasmaspheric hiss" in large part due to its in situ measurement within the plasmasphere . This distinction is necessary because the PH observed in space is fairly well ordered, whereas the hiss observed at a given point on the ground is a superposition of electromagnetic wave energy that arrives from different sources on the ground and in space.…”
Section: Introductionmentioning
confidence: 99%