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Gotowe bibliografie tematyczne / Ion cyclotron waves

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Gotowa bibliografia na temat „Ion cyclotron waves”

Autor: Grafiati

Data publikacji: 6 września 2023

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Artykuły w czasopismach na temat "Ion cyclotron waves"

1

Haridas, Annex Edappattu, and Rama Shankar Pandey. "Study of Low-Frequency Electromagnetic Ion-Cyclotron Wave for Ring Distribution in Magnetosphere of Saturn." Trends in Sciences 19, no. 22 (2022): 1329. http://dx.doi.org/10.48048/tis.2022.1329.

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Magnetic cyclotron waves were discovered by the Cassini-Huygens spacecraft in Saturn's atmospheric torus’ magnetic layer. They are left-handed and propagate at a minor angle to the ambient magnetic field in most areas because their frequency is close to the frequency of the aqua ions. The ion cyclotron instability caused by Saturn's neutral cloud ions helps explain their formation. They can be classified as n = 2 mode fluctuations because of the ion-ring distribution. We planned the characteristics of these waves in advance of starting this project. Our dispersion growth rates are evaluated using kinetic method analysis as well. The results were calculated and explained for the exemplary values of the magnetosphere parameters suitable for Saturn. Another potential free energy source for ion cyclotrons is temperature anisotropy. Instead of the standard Maxwell distribution, a ring distribution is employed in this study. The focus of this research is EMIC waves’ oblique propagation in the magnetic field, which changes their temperature anisotropy, ion energy density, and propagation angle. The interaction of relativistic particles with ion cyclotron waves is also included in this extension. EMIC wave size decreases with the increasing density of particles, as shown by a numerical study. A comparison of planetary studies based on data from space plasma environments and magnetospheric systems produced these results. HIGHLIGHTS Temperature anisotropy - free energy source for Ion Cyclotron waves EMIC wave size decreases with the increasing density of particles Saturn's neutral cloud ions helps the formation of ion cyclotron instability GRAPHICAL ABSTRACT

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2

Pokhotelov, O. A., L. Stenflo, and P. K. Shukla. "Nonlinear interaction of electrostatic ion-cyclotron and drift waves in plasmas." Journal of Plasma Physics 56, no. 1 (1996): 187–91. http://dx.doi.org/10.1017/s0022377800019176.

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Model equations describing the nonlinear coupling between electrostatic ion-cyclotron and drift waves are derived, taking into account the action of the low-frequency ponderomotive force associated with the ion-cyclotron waves. It is found that this interaction is governed by a pair of equations, which can be used for studying the modulational instability of a constant amplitude ion-cyclotron wave as well as the dynamics of nonlinearly coupled ion-cyclotron and drift waves.

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3

Bharuthram, R., S. V. Singh, S. K. Maharaj, et al. "Do nonlinear waves evolve in a universal manner in dusty and other plasma environments?" Journal of Plasma Physics 80, no. 6 (2014): 825–32. http://dx.doi.org/10.1017/s0022377814000427.

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Using a fluid theory approach, this article provides a comparative study on the evolution of nonlinear waves in dusty plasmas, as well as other plasma environments, viz electron-ion, and electron-positron plasmas. Where applicable, relevance to satellite measurements is pointed out. A range of nonlinear waves from low frequency (ion acoustic and ion cyclotron waves), high frequency (electron acoustic and electron cyclotron waves) in electron-ion plasmas, ultra-low frequency (dust acoustic and dust cyclotron waves) in dusty plasmas and in electron-positron plasmas are discussed. Depending upon the plasma parameters, saw-tooth and bipolar structures are shown to evolve.

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4

Blanco-Cano, X., C. T. Russell, D. E. Huddleston, and R. J. Strangeway. "Ion cyclotron waves near Io." Planetary and Space Science 49, no. 10-11 (2001): 1125–36. http://dx.doi.org/10.1016/s0032-0633(01)00020-4.

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5

Russell, C. T., and D. E. Huddleston. "Ion-cyclotron waves at Io." Advances in Space Research 26, no. 10 (2000): 1505–11. http://dx.doi.org/10.1016/s0273-1177(00)00090-9.

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6

Russell, C. T., H. Y. Wei, M. M. Cowee, F. M. Neubauer, and M. K. Dougherty. "Ion cyclotron waves at Titan." Journal of Geophysical Research: Space Physics 121, no. 3 (2016): 2095–103. http://dx.doi.org/10.1002/2015ja022293.

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7

Narita, Y., E. Marsch, C. Perschke, K. H. Glassmeier, U. Motschmann, and H. Comişel. "Wave–particle resonance condition test for ion-kinetic waves in the solar wind." Annales Geophysicae 34, no. 4 (2016): 393–98. http://dx.doi.org/10.5194/angeo-34-393-2016.

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Abstract. Conditions for the Landau and cyclotron resonances are tested for 543 waves (identified as local peaks in the energy spectra) in the magnetic field fluctuations of the solar wind measured by the Cluster spacecraft on a tetrahedral scale of 100 km. The resonance parameters are evaluated using the frequencies in the plasma rest frame, the parallel components of the wavevectors, the ion cyclotron frequency, and the ion thermal speed. The observed waves show a character of the sideband waves associated with the ion Bernstein mode, and are in a weak agreement with the fundamental electron cyclotron resonance in spite of the ion-kinetic scales. The electron cyclotron resonance is likely taking place in solar wind turbulence near 1 AU (astronomical unit).

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8

Thorne, R. M., and R. B. Horne. "Cyclotron absorption of ion-cyclotron waves at the bi-ion frequency." Geophysical Research Letters 20, no. 4 (1993): 317–20. http://dx.doi.org/10.1029/93gl00089.

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9

Sharma, Shatendra, and Jyotsna Sharma. "Spiraling ion beam driven electrostatic ion cyclotron wave instabilities in collisionless dusty plasma." International Journal of Modern Physics: Conference Series 32 (January 2014): 1460352. http://dx.doi.org/10.1142/s2010194514603524.

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The numerical calculations of the growth rate in long parallel wavelength are made for a spiraling ion beam propagating through a collision less magnetized dusty plasma cylinder that drives electrostatic ion cyclotron waves to instability via cyclotron interaction. It is found that the growth rate of the instability of the electrostatic ion cyclotron waves increase in the long parallel limit with the density ratio of negatively charged dust grains to electrons. The growth rate of the unstable mode has the maximum value for the modes whose Eigen functions peak at the location of the beam and varies as the one-third power of the beam current in both the limits.

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10

Sharma, S. C., and V. K. Tripathi. "Excitation of ion-cyclotron waves by a spiralling ion beam in a plasma cylinder." Journal of Plasma Physics 50, no. 2 (1993): 331–38. http://dx.doi.org/10.1017/s0022377800027112.

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A helical ion beam propagating through a plasma cylinder drives electrostatic ion-cyclotron waves to instability via cyclotron interaction. Higher harmonics of the beam cyclotron frequency can be generated in this way. The growth rate increases with the harmonic number. The efficiency of beam energy transfer to the wave can be of the order of a few per cent.

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