Bibliografías temáticas / Ion cyclotron waves

Literatura académica sobre el tema "Ion cyclotron waves"

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Publicado: 6 de septiembre de 2023

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Artículos de revistas sobre el tema "Ion cyclotron waves"

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Haridas, Annex Edappattu y Rama Shankar Pandey. "Study of Low-Frequency Electromagnetic Ion-Cyclotron Wave for Ring Distribution in Magnetosphere of Saturn". Trends in Sciences 19, n.º 22 (5 de noviembre de 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 y P. K. Shukla. "Nonlinear interaction of electrostatic ion-cyclotron and drift waves in plasmas". Journal of Plasma Physics 56, n.º 1 (agosto de 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, S. Moolla, I. J. Lazarus, R. V. Reddy y G. S. Lakhina. "Do nonlinear waves evolve in a universal manner in dusty and other plasma environments?" Journal of Plasma Physics 80, n.º 6 (14 de julio de 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 y R. J. Strangeway. "Ion cyclotron waves near Io". Planetary and Space Science 49, n.º 10-11 (agosto de 2001): 1125–36. http://dx.doi.org/10.1016/s0032-0633(01)00020-4.

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Russell, C. T. y D. E. Huddleston. "Ion-cyclotron waves at Io". Advances in Space Research 26, n.º 10 (enero de 2000): 1505–11. http://dx.doi.org/10.1016/s0273-1177(00)00090-9.

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Russell, C. T., H. Y. Wei, M. M. Cowee, F. M. Neubauer y M. K. Dougherty. "Ion cyclotron waves at Titan". Journal of Geophysical Research: Space Physics 121, n.º 3 (marzo de 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 y H. Comişel. "Wave–particle resonance condition test for ion-kinetic waves in the solar wind". Annales Geophysicae 34, n.º 4 (7 de abril de 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. y R. B. Horne. "Cyclotron absorption of ion-cyclotron waves at the bi-ion frequency". Geophysical Research Letters 20, n.º 4 (19 de febrero de 1993): 317–20. http://dx.doi.org/10.1029/93gl00089.

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Sharma, Shatendra y Jyotsna Sharma. "Spiraling ion beam driven electrostatic ion cyclotron wave instabilities in collisionless dusty plasma". International Journal of Modern Physics: Conference Series 32 (enero de 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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Sharma, S. C. y V. K. Tripathi. "Excitation of ion-cyclotron waves by a spiralling ion beam in a plasma cylinder". Journal of Plasma Physics 50, n.º 2 (octubre de 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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Tesis sobre el tema "Ion cyclotron waves"

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Teodorescu, Catalin. "Laboratory investigation of electrostatic ion waves modified by parallel-ion-velocity shear". Morgantown, W. Va. : [West Virginia University Libraries], 2003. http://etd.wvu.edu/templates/showETD.cfm?recnum=2901.

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Thesis (Ph. D.)--West Virginia University, 2003.
Title from document title page. Document formatted into pages; contains xiv, 215 p. : ill. Vita. Includes abstract. Includes bibliographical references (p. 107-113).
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2

Nguyen, Son Thanh Perez Joseph D. "Interactions between electromagnetic ion cyclotron waves and protons in the magnetosphere SCATHA Results /". Auburn, Ala., 2007. http://hdl.handle.net/10415/1380.

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Hannan, Abdul. "Modelling Ion Cyclotron Resonance Heating and Fast Wave Current Drive in Tokamaks". Doctoral thesis, KTH, Fusionsplasmafysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-119930.

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Fast magnetosonic waves in the ion cyclotron range of frequencies have the potential to heat plasma and drive current in a thermonuclear fusion reactor. A code, SELFO-light, has been developed to study the physics of ion cyclotron resonantheating and current drive in thermonuclear fusion reactors. It uses a global full wave solver LION and a new 1D Fokker-Planck solver for the self-consistent calculations of the wave field and the distribution function of ions.In present day tokamak experiments like DIII-D and JET, fast wave damping by ions at higher harmonic cyclotron frequencies is weak compared to future thermonuclear tokamak reactors like DEMO. The strong damping by deuterium, tritium and thermonuclear alpha-particles and the large Doppler width of fast alpha-particles in DEMO makes it difficult to drive the current when harmonic resonance layers of these ionspecies are located at low field side of the magnetic axis. At higher harmonic frequencies the possibility of fast wave current drive diminishes due to the overlapping of alpha-particle harmonic resonance layers. Narrow frequency bands suitable for the fast wave current drive in DEMO have been identified at lower harmonics of the alpha-particles. For these frequencies the effect of formation of high-energy tails in the distribution function of majority and minority ion species on the current drive have been studied. Some of these frequencies are found to provide efficient ion heating in the start up phase of DEMO. The spectrum where efficient current drive can be obtained is restricted due to weak electron damping at lower toroidal mode numbers and strong trapped electron damping at higher toroidal mode numbers. The width of toroidal mode spectra for which efficient current drive can be obtained have been identified, which has important implications for the antenna design.

QC 20130327

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De, Soria-Santacruz Pich Maria. "Controlled precipitation of energetic Van Allen belt protons by electromagnetic ion cyclotron (EMIC) waves : scientific and engineering implications". Thesis, Massachusetts Institute of Technology, 2014. http://hdl.handle.net/1721.1/87127.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Aeronautics and Astronautics, 2014.
This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references (pages 235-247).
The inner Van Allen radiation belt traps highly energetic protons sourced from solar storms, cosmic rays and other processes. These particles can rapidly damage the space systems orbiting the inner region, limiting access to Low Earth Orbit (LEO). Decades of modeling and observations, however, show that naturally generated ULF/VLF waves have the capability of precipitating energetic trapped electrons and protons. This fact suggests that there could be human control over the stable inner belt proton population by artificially transmitting Electromagnetic Ion Cyclotron (EMIC) waves from space-based antennas (named remediation). These waves are naturally generated by equatorial ring current ions in the outer belt region, which explains the absence of EMIC waves at lower altitudes. Consequently, the precipitation of high-energy protons requires artificial generation of EMIC waves into the inner zone. The controlled removal of energetic outer belt electrons by man-made whistler waves has been widely studied, and a space test of a linear antenna for this purpose is in preparation. Contrarily, the interaction between inner belt protons and EMIC waves from in-situ transmitters is an unexplored solution to the radiation environment that should be addressed given its relevance to the scientific and engineering communities. This dissertation focuses on four interconnected research efforts in this direction, which are (1) the radiation of EMIC waves from a space-based antenna, (2) the propagation of these waves in the inner radiation belt, (3) the wave-particle interactions with energetic trapped protons and (4) the feasibility of a mission capable of significantly reducing this hazardous radiation. Our analyses show that a DC rotating coil antenna would be capable of radiating EMIC waves into space. Magnetic dipoles, however, have a very small radiation resistance. Additionally, the interaction between these waves and energetic protons is very inefficient. Our simulations show that, with the current technology, it is not engineeringly feasible to clean up the proton belt using space-based transmitters. A mission scaled down to detectability of the precipitating protons, however, could be launched easily and would allow us to better understand the science and test the technology involved in the concept of remediation.
by Maria de Soria-Santacruz Pich.
Ph. D.
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5

Urbanczyk, Guillaume. "Interaction of High-Power waves with the plasma periphery of WEST & EAST tokamaks". Electronic Thesis or Diss., Université de Lorraine, 2019. http://www.theses.fr/2019LORR0181.

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Cette thèse vise à étudier les interactions entre le plasma et les parois de tokamaks liées aux ondes à la fréquence cyclotronique ionique (FCI), les interactions plasma-métaux étant à éviter absolument car elles sont synonymes de dégradations matérielles de l’enceinte et la libération d’impuretés métalliques dans le plasma dont les performances s’en trouvent grandement réduites. Cette problématique affecte concrètement toute machine visant à chauffer les ions via des ondes à la fréquence FCI, ce qui sera notamment le cas d’ITER. Cette thèse s'inscrit dans une collaboration entre le CEA Cadarache (France) et l’Institut de Physique des Plasmas à Hefei (Chine). Divers travaux expérimentaux ont été effectués sur les tokamaks EAST (Chine) et WEST (France) afin d'identifier les paramètres pertinents pour d'une part optimiser l'efficacité par laquelle les ondes FCI utilisées pour chauffer le plasma doivent être excitées afin de maximiser la quantité de puissance couplée au plasma tout en minimisant les interactions du plasma avec les parois dues à ce type d'ondes et souvent attribuées au concept de gaine radiofréquence au cœur de cette thèse
This thesis aims at studying phenomena by which Ion Cyclotron Resonance Heating (ICRH) induces interactions between the plasma and the walls of tokamaks, the plasma-metal interactions being deleterious not only to prevent vessel materials degradation but also not to affect plasma performance due to the presence of heavy metallic impurity compared to foreseen fuel (namely deuterium and tritium). This problematic basically affects any machine aiming at heating the ions with waves at the ion cyclotron frequency, which in particular will be the case of ITER. This thesis is the result of a collaboration between CEA Cadarache (France) and the Institute of Plasma Physics in Hefei (China). Various experimental work have been carried out on the EAST (China) and WEST (France) tokamaks in order to identify the relevant parameters allowing to optimize the efficiency by which the ICRF waves – used to heat the plasma – must be excited in order to maximize the amount of power coupled, while simultaneously minimizing the plasma interactions with the walls due to this type of waves and the so called radiofrequency sheath excitation
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Kwon, Myeun. "Fast wave ion cyclotron resonance heating experiments on the advanced toroidal facility". Diss., Georgia Institute of Technology, 1990. http://hdl.handle.net/1853/13015.

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Hedin, Johan. "Ion cyclotron resonance heating in toroidal plasmas". Doctoral thesis, KTH, Alfvén Laboratory, 2000. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3073.

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Shepard, Thomas Donavon. "Fast wave ion cyclotron resonance heating experiments on the Alcator C tokamak". Thesis, Massachusetts Institute of Technology, 1988. http://hdl.handle.net/1721.1/14402.

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Johnson, Thomas. "Fast wave heating of cyclotron resonant ions in tokamaks". Doctoral thesis, KTH, Alfvénlaboratoriet, 2004. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3771.

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Chang, Ouliang. "Numerical Simulation of Ion-Cyclotron Turbulence Generated by Artificial Plasma Cloud Release". Thesis, Virginia Tech, 2009. http://hdl.handle.net/10919/34018.

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Possibilities of generating plasma turbulence to provide control of space weather processes have been of particular interest in recent years. Such turbulence can be created by chemical released into a magnetized background plasma. The released plasma clouds are heavy ions which have ring velocity distribution and large free energy to drive the turbulence. An electromagnetic hybrid (fluid electrons and particle ions) model incorporating electron inertia is developed to study the generation and nonlinear evolution of this turbulence. Fourier pseudo-spectral methods are combined with finite difference methods to solve the electron momentum equations. Time integration is accomplished by a 4th-order Runge-Kutta scheme or predicator-corrector method. The numerical results show good agreement with theoretical prediction as well as provide further insights on the nonlinear turbulence evolution. Initially the turbulence lies near harmonics of the ring plasma ion cyclotron frequency and propagates nearly perpendicular to the background magnetic field as predicted by the linear theory. If the amplitude of the turbulence is sufficiently large, the quasi-electrostatic short wavelength ion cyclotron waves evolve nonlinearly into electromagnetic obliquely propagating shear Alfven waves with much longer wavelength. The results indicate that ring densities above a few percent of the background plasma density may produce wave amplitudes large enough for such an evolution to occur. The extraction of energy from the ring plasma may be in the range of 10-15% with a generally slight decrease in the magnitude as the ring density is increased from a few percent to several 10's of percent of the background plasma density. Possibilities to model the effects of nonlinear processes on energy extraction by introducing electron anomalous resistivity are also addressed. Suitability of the nonlinearly generated shear Alfven waves for applications to scattering radiation belt particles is discussed.
Master of Science
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Libros sobre el tema "Ion cyclotron waves"

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Workshop, on the Current-Driven Electrostatic Ion-Cyclotron Instability (1987 Innsbruck Austria). Proceedings of the Workshop on the Current-Driven Electrostatic Ion-Cyclotron Instability: July 9/10, 1987, Innsburck, Austria. Singapore: World Scientific, 1988.

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V, Khazanov G. y United States. National Aeronautics and Space Administration., eds. Lower hybrid oscillations in multicomponent space plasmas subjected to ion cyclotron waves. [Washington, DC: National Aeronautics and Space Administration, 1997.

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United States. National Aeronautics and Space Administration., ed. Studies of electromagnetic ion cyclotron waves using AMPTE/CCE and dynamics explorer: Semi-annual report covering the period from 6/1/93 to 12/1/93. [Washington, DC: National Aeronautics and Space Administration, 1993.

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Imre, Kaya. Wave propagation across ion cyclotron resonance harmonic layers. New York: Courant Institute of Mathematical Sciences, New York University, 1987.

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Studies of electromagnetic ion cyclotron waves using AMPTE/CCE and dynamics explorer: Final report, period of performance 6/1/91 to 8/31/94. [Washington, DC: National Aeronautics and Space Administration, 1994.

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Imre, Kaya y H. Weitzner. Wave Propagation Across Ion Cyclotron Resonance Harmonic Layers. Creative Media Partners, LLC, 2015.

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Imre, Kaya y H. Weitzner. Wave Propagation Across Ion Cyclotron Resonance Harmonic Layers. Creative Media Partners, LLC, 2018.

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Capítulos de libros sobre el tema "Ion cyclotron waves"

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Wei, H. Y., L. K. Jian, C. T. Russell y N. Omidi. "Ion Cyclotron Waves in the Solar Wind". En Low-Frequency Waves in Space Plasmas, 253–67. Hoboken, NJ: John Wiley & Sons, Inc, 2016. http://dx.doi.org/10.1002/9781119055006.ch15.

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Fraser, B. J., T. M. Loto'aniu y H. J. Singer. "Electromagnetic Ion Cyclotron Waves in the Magnetosphere". En Magnetospheric ULF Waves: Synthesis and New Directions, 195–212. Washington, D. C.: American Geophysical Union, 2006. http://dx.doi.org/10.1029/169gm13.

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Walker, A. D. M. "Waves in the Plasmasphere — 3. Ion Cyclotron Whistlers". En Plasma Waves in the Magnetosphere, 249–64. Berlin, Heidelberg: Springer Berlin Heidelberg, 1993. http://dx.doi.org/10.1007/978-3-642-77867-4_12.

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Li, Xing y Shadia R. Habbal. "Ion Cyclotron Waves, Instabilities and Solar Wind Heating". En Physics of the Solar Corona and Transition Region, 485–97. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-017-3429-5_30.

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Delva, Magda, Christian Mazelle y César Bertucci. "Upstream Ion Cyclotron Waves at Venus and Mars". En Space Sciences Series of ISSI, 5–24. New York, NY: Springer US, 2011. http://dx.doi.org/10.1007/978-1-4614-3290-6_2.

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Temerin, M., C. Carlson y J. P. Mcfadden. "The Acceleration of Electrons by Electromagnetic Ion Cyclotron Waves". En Auroral Plasma Dynamics, 155–61. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm080p0155.

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Fraser, B. J., S. K. Morley, R. S. Grew y H. J. Singer. "Classification of Pc1-2 Electromagnetic Ion Cyclotron Waves at Geosynchronous Orbit". En Dynamics of the Earth's Radiation Belts and Inner Magnetosphere, 53–68. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/2012gm001353.

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Khazanov, George V. "Kinetic Theory of Ring Current and Electromagnetic Ion Cyclotron Waves: Applications". En Kinetic Theory of the Inner Magnetospheric Plasma, 491–540. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-6797-8_10.

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Khazanov, George V. "Kinetic Theory of Ring Current and Electromagnetic Ion Cyclotron Waves: Fundamentals". En Kinetic Theory of the Inner Magnetospheric Plasma, 429–89. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-6797-8_9.

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Fraser, B. J. "Observations of Ion Cyclotron Waves Near Synchronous Orbit and on the Ground". En Space Plasma Simulations, 357–74. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5454-0_22.

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Actas de conferencias sobre el tema "Ion cyclotron waves"

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Li, Xing. "Heating in coronal funnels by ion cyclotron waves". En SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP, 2003. http://dx.doi.org/10.1063/1.1618595.

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Merlino, R. L., S. Kim, N. D'Angelo y Gurudas I. Ganguli. "The Effect of Ion Flow Shear on Electrostatic Ion-Cyclotron Waves". En IEEE Conference Record - Abstracts. 2005 IEEE International Conference on Plasma Science. IEEE, 2005. http://dx.doi.org/10.1109/plasma.2005.359504.

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Weitzner, Harold, Lee A. Berry, E. Fred Jaeger y Donald B. Batchelor. "Ion flow driven by waves in the ion cyclotron frequency range". En The thirteenth topical conference on radio frequency power in plasmas. AIP, 1999. http://dx.doi.org/10.1063/1.59696.

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Bilato, R. "Investigation of Mode-Transformed Ion Cyclotron Waves at the Ion-Ion Hybrid Layer". En RADIO FREQUENCY POWER IN PLASMAS: 16th Topical Conference on Radio Frequency Power in Plasmas. AIP, 2005. http://dx.doi.org/10.1063/1.2098210.

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Girka, V. O. y I. V. Pavlenko. "Ion surface cyclotron waves in the planar metallic waveguides". En IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science. IEEE, 1996. http://dx.doi.org/10.1109/plasma.1996.551478.

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Girka, Volodymyr O., Igor O. Girka, Anton V. Klyzhka, Ivan V. Pavlenko, Volodymyr Bobkov y Jean-Marie Noterdaeme. "Surface Ion Cyclotron Waves Propagating Across an External Magnetic Field". En RADIO FREQUENCY POWER IN PLASMAS: Proceedings of the 18th Topical Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3273826.

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Kuley, A., J. Bao, Z. Lin, X. S. Wei y Y. Xiao. "Nonlinear particle simulation of ion cyclotron waves in toroidal geometry". En RADIO FREQUENCY POWER IN PLASMAS: Proceedings of the 21st Topical Conference. EURATOM, 2015. http://dx.doi.org/10.1063/1.4936506.

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Pongkitiwanichakul, Peera, Benjamin D. G. Chandran, Philip A. Isenberg, Bernard J. Vasquez, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet y F. Pantellini. "Resonant Interactions Between Protons and Oblique Alfvén∕Ion-Cyclotron Waves". En TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP, 2010. http://dx.doi.org/10.1063/1.3395966.

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Tejero, E. M., W. E. Amatucci y E. Thomas. "Laboratory study of velocity shear-driven electromagnetic ion cyclotron waves". En 2011 XXXth URSI General Assembly and Scientific Symposium. IEEE, 2011. http://dx.doi.org/10.1109/ursigass.2011.6051087.

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Swanson, D. G. y Suwon Cho. "Mode conversion of lower hybrid waves at high ion cyclotron harmonics". En AIP Conference Proceedings Volume 129. AIP, 1985. http://dx.doi.org/10.1063/1.35258.

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Informes sobre el tema "Ion cyclotron waves"

1

Chang, C. Control of energetic ion confinement by ion cyclotron range of frequency waves. Office of Scientific and Technical Information (OSTI), febrero de 1990. http://dx.doi.org/10.2172/5089627.

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2

Jaeger, E. F., D. B. Batchelor y H. Weitzner. Global ion cyclotron waves in a perpendicularly stratified, one-dimensional warm plasma. Office of Scientific and Technical Information (OSTI), abril de 1987. http://dx.doi.org/10.2172/6566744.

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3

Masayuki Ono. Cold Electronstatic Ion Cyclotron Waves for Preionization and IBW Launching in LHD. Office of Scientific and Technical Information (OSTI), abril de 1999. http://dx.doi.org/10.2172/6260.

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4

Kim, Eun y J. R. Johnson. Comment on "Mode Conversion of Waves In The Ion-Cyclotron Frequency Range in Magnetospheric Plasmas". Office of Scientific and Technical Information (OSTI), febrero de 2014. http://dx.doi.org/10.2172/1128922.

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5

Perkins, F. W., R. B. White, P. T. Bonoli y V. S. Chan. Generation of Plasma Rotation in a Tokamak by Ion-Cyclotron Absorption of Fast Alfven Waves. Office of Scientific and Technical Information (OSTI), noviembre de 2000. http://dx.doi.org/10.2172/768762.

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6

Ono, Masayuki. Investigation of electrostatic waves in the ion cyclotron range of frequencies in L-4 and ACT-1. Office of Scientific and Technical Information (OSTI), mayo de 1993. http://dx.doi.org/10.2172/10160802.

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7

Ono, Masayuki. Investigation of electrostatic waves in the ion cyclotron range of frequencies in L-4 and ACT-1. Office of Scientific and Technical Information (OSTI), mayo de 1993. http://dx.doi.org/10.2172/6483928.

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8

Fruchtman, A., K. Riedel, H. Weitzner y D. B. Batchelor. Strong cyclotron damping of electron cyclotron waves in nearly parallel stratified plasmas. Office of Scientific and Technical Information (OSTI), septiembre de 1986. http://dx.doi.org/10.2172/7242112.

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9

Ram, Abhay K., Paul T. Bonoli y John C. Wright. Propagation And Damping Of High Harmonic Fast Waves And Electron Cyclotron Waves In The Nstx-U-Device. Office of Scientific and Technical Information (OSTI), marzo de 2014. http://dx.doi.org/10.2172/1464084.

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10

Ram, Abhay, Paul Bonoli y John C. Wright. Propagation And Damping Of High Harmonic Fast Waves And Electron Cyclotron Waves In The Nstx-U-Device. Office of Scientific and Technical Information (OSTI), marzo de 2014. http://dx.doi.org/10.2172/1464085.

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