2010
DOI: 10.1063/1.3460344
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The parametric decay of Alfvén waves into shear Alfvén waves and dust lower hybrid waves

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Cited by 13 publications
(4 citation statements)
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“…The past studies assumed that all the physical quantities depend only on one spatial coordinate parallel to the ambient magnetic field while it was also suggested that obliquely propagating waves excited by the beam instabilities can play important roles in the nonlinear evolution of the system. Moreover, the presence of charged dust particles also modifies the scenario of the Alfven waves [23][24][25][26][27][28] by enhancing their frequency, modifying the dispersion relation, and showing a damping effect due to dust charge fluctuation dynamics. Jatenco-Pereira et al [29] showed the sensible modification of the dispersion relation of Alfvén waves in the presence of dust and superthermal particles.…”
Section: Introductionmentioning
confidence: 99%
“…The past studies assumed that all the physical quantities depend only on one spatial coordinate parallel to the ambient magnetic field while it was also suggested that obliquely propagating waves excited by the beam instabilities can play important roles in the nonlinear evolution of the system. Moreover, the presence of charged dust particles also modifies the scenario of the Alfven waves [23][24][25][26][27][28] by enhancing their frequency, modifying the dispersion relation, and showing a damping effect due to dust charge fluctuation dynamics. Jatenco-Pereira et al [29] showed the sensible modification of the dispersion relation of Alfvén waves in the presence of dust and superthermal particles.…”
Section: Introductionmentioning
confidence: 99%
“…The spin effects of electrons are important for the following reasons: It is a useful diagnostic technique for the measurement of plasma number density more precisely as compared to the conventional techniques; to measure the width of Doppler broadening of resonance line for plasmas more accurately because this provides the information on the spectrum of particle velocity perpendicular to B 0 ; to calculate the magnetic fields associated with the propagation of electromagnetic or hydromagnetic waves, e.g., Whistlers, Alfv en and Shock, waves excited in plasmas. 22 The nonlinear parametric instabilities [23][24][25][26][27][28] have attained a great interest during last numerous decades and were carefully investigated over wave-wave interactions in plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…Numerous recent papers (e.g. [4]) have thus failed in this respect. Here, our purpose is therefore to present the correct growth rates in forms that are much simpler than those of previous papers [5] and which accordingly can be significantly more useful for specific cases.…”
Section: Introductionmentioning
confidence: 99%