Abstract:A kinetic theory of triggered VLF whistler emissions is given that is capable of predicting from a small scale numerical implementation the observed emission forms, and frequency-time characteristics. The present paper focuses on the theoretical developments and the explanation of the triggering process, complete with a demonstration of the threshold behavior (sometimes known as the dot-dash anomaly) and the generation of specific falling frequency emissions that compare quite favorably to typical observations… Show more
“…Wellorganized electron beams can be produced by quasimonochromatic whistler wave packets. 5,6 Such a situation takes place in the Earth's magnetosphere in the case of the socalled triggered ELF/VLF emissions. [7][8][9][10] The beams with a step-like distribution function can appear in space plasma conditions even more often than ␦-functions.…”
A new analytical approach to cyclotron instability of electron beams with sharp gradients in velocity space (step-like distribution function) is developed taking into account magnetic field inhomogeneity and nonstationary behavior of the electron beam velocity. Under these conditions, the conventional hydrodynamic instability of such beams is drastically modified and second order resonance effects become important. It is shown that the optimal conditions for the instability occur for nonstationary quasimonochromatic wavelets whose frequency changes in time. The theory developed permits one to estimate the wave amplification and spatio-temporal characteristics of these wavelets.
“…Wellorganized electron beams can be produced by quasimonochromatic whistler wave packets. 5,6 Such a situation takes place in the Earth's magnetosphere in the case of the socalled triggered ELF/VLF emissions. [7][8][9][10] The beams with a step-like distribution function can appear in space plasma conditions even more often than ␦-functions.…”
A new analytical approach to cyclotron instability of electron beams with sharp gradients in velocity space (step-like distribution function) is developed taking into account magnetic field inhomogeneity and nonstationary behavior of the electron beam velocity. Under these conditions, the conventional hydrodynamic instability of such beams is drastically modified and second order resonance effects become important. It is shown that the optimal conditions for the instability occur for nonstationary quasimonochromatic wavelets whose frequency changes in time. The theory developed permits one to estimate the wave amplification and spatio-temporal characteristics of these wavelets.
“…The nonlinear self-consistent interaction of cyclotron resonant energetic electrons with narrow band VLF waves in the Earth's magnetosphere has been used to explain many of the qualitative physical features underlying these types of emissions (Helliwell 1967;Karpman et al 1974;Yoshida et al 1983;Molvig et al 1988;Omura et al 1991;Nunn et al 1997;Trakhtengerts and Rycroft 2000). In spite of tremendous efforts and huge theoretical work published so far; a selfconsistence theory capable of predicting the observed dynamic spectra, threshold behavior and frequency time characteristics has remained elusive.…”
A unique night-time natural electromagnetic disturbances in the VLF/ELF range received during a magnetically quite period at a low latitude Indian ground station, Jammu (geomag. lat. 19°26 N, L = 1.17) has been reported. During the routine observation of VLF waves at Jammu, whistlers and different types of VLF/ELF emissions such as whistlers of varying dispersion confined to a small band limited frequency range, hisslers, pulsing hiss, discrete chorus emissions of rising and falling tones with multiple bands, oscillating tone discrete emission, whistler-triggered hook and discrete chorus risers emissions, etc. have been observed simultaneously during the quiet period on a single night. Such type of unique simultaneous observations has never been reported from any of the low latitude ground stations and this is the first observation of its kind. The results are discussed in the light of recorded features of whistlers and emissions. Generation and propagation mechanism are discussed briefly. Plasma parameters are further derived from the dispersion analysis of nighttime whistlers and emissions recorded simultaneously during magnetically quiet periods.
“…Similar equations have also been exploited repeatedly in subsequent studies on the nonlinear gyroresonant phenomena in the magnetosphere (e.g. Nunn, 1974;Karpman, 1974;Roux and Pellat, 1978;Bell and Inan, 1981;Molvig et al, 1988;Carlson et al, 1990;Shklyar et al, 1992). In essence, the simplified description of the particle dynamics (Dysthe, 1971) reduces to a change of rigorous equations of motion for equations averaged over the Larmor gyration of the particle.…”
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