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Artigos de revistas sobre o tema "Magneto-acoustic"

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Autor: Grafiati

Publicado: 25 de maio de 2024

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1

AMMARI, HABIB, YVES CAPDEBOSCQ, HYEONBAE KANG e ANASTASIA KOZHEMYAK. "Mathematical models and reconstruction methods in magneto-acoustic imaging". European Journal of Applied Mathematics 20, n.º 3 (junho de 2009): 303–17. http://dx.doi.org/10.1017/s0956792509007888.

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In this paper, we provide the mathematical basis for three different magneto-acoustic imaging approaches (vibration potential tomography, magneto-acoustic tomography with magnetic induction and magneto-acoustic current imaging) and propose new algorithms for solving the inverse problem for each of them.

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2

Roth, Bradley J. "Magneto-Acoustic Imaging in Biology". Applied Sciences 13, n.º 6 (18 de março de 2023): 3877. http://dx.doi.org/10.3390/app13063877.

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This review examines the use of magneto-acoustic methods to measure electrical conductivity. It focuses on two techniques developed in the last two decades: Magneto-Acoustic Tomography with Magnetic Induction (MAT-MI) and Magneto-Acousto-Electrical Tomography (MAET). These developments have the potential to change the way medical doctors image biological tissue.

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3

Qu, Min, Srivalleesha Mallidi, Mohammad Mehrmohammadi, Ryan Truby, Kimberly Homan, Pratixa Joshi, Yun-Sheng Chen, Konstantin Sokolov e Stanislav Emelianov. "Magneto-photo-acoustic imaging". Biomedical Optics Express 2, n.º 2 (21 de janeiro de 2011): 385. http://dx.doi.org/10.1364/boe.2.000385.

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4

Li, Jinxing, Tianlong Li, Tailin Xu, Melek Kiristi, Wenjuan Liu, Zhiguang Wu e Joseph Wang. "Magneto–Acoustic Hybrid Nanomotor". Nano Letters 15, n.º 7 (19 de junho de 2015): 4814–21. http://dx.doi.org/10.1021/acs.nanolett.5b01945.

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5

Guyot, M., e V. Cagan. "The magneto‐acoustic emission (invited)". Journal of Applied Physics 73, n.º 10 (15 de maio de 1993): 5348–53. http://dx.doi.org/10.1063/1.353728.

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6

Drummond James, E. "5402786 Magneto-acoustic resonance imaging". Magnetic Resonance Imaging 13, n.º 6 (janeiro de 1995): XXIV—XXV. http://dx.doi.org/10.1016/0730-725x(95)96707-i.

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7

Khantadze, A. G., G. V. Jandieri, A. Ishimaru, T. D. Kaladze e Zh M. Diasamidze. "Electromagnetic oscillations of the Earth's upper atmosphere (review)". Annales Geophysicae 28, n.º 7 (1 de julho de 2010): 1387–99. http://dx.doi.org/10.5194/angeo-28-1387-2010.

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Abstract. A complete theory of low-frequency MHD oscillations of the Earth's weakly ionized ionosphere is formulated. Peculiarities of excitation and propagation of electromagnetic acoustic-gravity, MHD and planetary waves are considered in the Earth's ionosphere. The general dispersion equation is derived for the magneto-acoustic, magneto-gravity and electromagnetic planetary waves in the ionospheric E- and F-regions. The action of the geomagnetic field on the propagation of acoustic-gravity waves is elucidated. The nature of the existence of the comparatively new large-scale electromagnetic planetary branches is emphasized.

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8

Zharkov, S., S. Shelyag, V. Fedun, R. Erdélyi e M. J. Thompson. "Photospheric high-frequency acoustic power excess in sunspot umbra: signature of magneto-acoustic modes". Annales Geophysicae 31, n.º 8 (6 de agosto de 2013): 1357–64. http://dx.doi.org/10.5194/angeo-31-1357-2013.

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Abstract. We present observational evidence for the presence of MHD (magnetohydrodynamic) waves in the solar photosphere deduced from SOHO/MDI (Solar and Heliospheric Observatory/Michelson Doppler Imager) Dopplergram velocity observations. The magneto-acoustic perturbations are observed as acoustic power enhancement in the sunspot umbra at high-frequency bands in the velocity component perpendicular to the magnetic field. We use numerical modelling of wave propagation through localised non-uniform magnetic field concentration along with the same filtering procedure as applied to the observations to identify the observed waves. Guided by the results of the numerical simulations we classify the observed oscillations as magneto-acoustic waves excited by the trapped sub-photospheric acoustic waves. We consider the potential application of the presented method as a diagnostic tool for magnetohelioseismology.

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9

Adamashvili, G. T., e A. A. Maradudin. "Nonlinear magneto-acoustic waves in ferromagnets". Journal of Applied Physics 79, n.º 8 (1996): 5727. http://dx.doi.org/10.1063/1.362232.

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10

Sytcheva, A., U. Löw, S. Yasin, J. Wosnitza, S. Zherlitsyn, T. Goto, P. Wyder e B. Lüthi. "Magneto-Acoustic Faraday Effect in Tb3Ga5O12". Journal of Low Temperature Physics 159, n.º 1-2 (6 de janeiro de 2010): 126–29. http://dx.doi.org/10.1007/s10909-009-0082-x.

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11

Alkahby, H. Y. "The dissipation of magneto-acoustic waves". Computers & Mathematics with Applications 27, n.º 5 (março de 1994): 9–15. http://dx.doi.org/10.1016/0898-1221(94)90072-8.

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12

Szabados, O., R. Baki, Zs, Csincsi, J. Molnar, Á. Pámer, P. Szabó e G. Por. "Magneto-acoustic investigation on steel samples". IOP Conference Series: Materials Science and Engineering 903 (26 de agosto de 2020): 012040. http://dx.doi.org/10.1088/1757-899x/903/1/012040.

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13

Rao, N. N. "Magnetoacoustic modes in a magnetized dusty plasma". Journal of Plasma Physics 53, n.º 3 (junho de 1995): 317–34. http://dx.doi.org/10.1017/s0022377800018237.

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The existence of various types of (fast) magnetoacoustic modes in different frequency regimes in a magnetized dusty plasma consisting of electrons, ions and dust particles is investigated. The analysis is carried out using an effective two-fluid MHD-like model which allows for the non-frozen motion of the component fluids. For frequencies much smaller than the dust particle gyro- frequency, we obtain a magnetoacoustic mode that is a generalization of the usual compressional fast hydromagnetic wave in an electron—ion plasma. In the higher-frequency regimes, we show the existence of two new types of modes called ‘Dust-magnetoacoustic waves’. Both modes are accompanied by compressional magnetic field and plasma number density perturbations, and are the electromagnetic generalizations of the dust-acoustic waves in an unmagnetized dusty plasma with thermal electrons and ions. For a two- component plasma, all three modes degenerate into the same fast magneto- acoustic wave found in the usual electron—ion plasmas. We also obtain another novel type of magneto-acoustic mode called a ‘dust—ion-magneto- acoustic wave’, which is an electromagnetic generalization of the dust—ion- acoustic wave. The dispersion relations as well as the frequency regimes for the existence of the various modes are explicitly obtained. An alternative derivation of the relevant governing equations using an approach similar to that employed in so-called ‘electron magnetohydrodynamics’ (EMHD) is also presented.

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14

Xu, Mingran, Kei Yamamoto, Jorge Puebla, Korbinian Baumgaertl, Bivas Rana, Katsuya Miura, Hiromasa Takahashi, Dirk Grundler, Sadamichi Maekawa e Yoshichika Otani. "Nonreciprocal surface acoustic wave propagation via magneto-rotation coupling". Science Advances 6, n.º 32 (agosto de 2020): eabb1724. http://dx.doi.org/10.1126/sciadv.abb1724.

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A fundamental form of magnon-phonon interaction is an intrinsic property of magnetic materials, the “magnetoelastic coupling.” This form of interaction has been the basis for describing magnetostrictive materials and their applications, where strain induces changes of internal magnetic fields. Different from the magnetoelastic coupling, more than 40 years ago, it was proposed that surface acoustic waves may induce surface magnons via rotational motion of the lattice in anisotropic magnets. However, a signature of this magnon-phonon coupling mechanism, termed magneto-rotation coupling, has been elusive. Here, we report the first observation and theoretical framework of the magneto-rotation coupling in a perpendicularly anisotropic film Ta/CoFeB(1.6 nanometers)/MgO, which consequently induces nonreciprocal acoustic wave attenuation with an unprecedented ratio of up to 100% rectification at a theoretically predicted optimized condition. Our work not only experimentally demonstrates a fundamentally new path for investigating magnon-phonon coupling but also justifies the feasibility of the magneto-rotation coupling application.

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15

TAKATA, Masaaki, Yoshiki NAGASAKI, Kazuhiko HAYAKAWA, Masaaki OKUBO e Hiroyuki YAMASAKI. "Magneto-Acoustic Instability in Disk CCMHD Generator". IEEJ Transactions on Power and Energy 117, n.º 12 (1997): 1584–92. http://dx.doi.org/10.1541/ieejpes1990.117.12_1584.

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16

Vavra, Kevin C., George Yu, Mira Josowicz e Jií Janata. "Magnetic quartz crystal microbalance: Magneto-acoustic parameters". Journal of Applied Physics 110, n.º 1 (julho de 2011): 013905. http://dx.doi.org/10.1063/1.3602998.

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17

Aliroteh, M. S., G. Scott e A. Arbabian. "Frequency‐modulated magneto‐acoustic detection and imaging". Electronics Letters 50, n.º 11 (maio de 2014): 790–92. http://dx.doi.org/10.1049/el.2014.0997.

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18

Ozhogin, V., A. Kiselev, V. Moshkin, V. Preobrazhenskii e V. Shumilov. "Photo‐magneto‐acoustic effect in hematite (abstract)". Journal of Applied Physics 73, n.º 10 (15 de maio de 1993): 6177. http://dx.doi.org/10.1063/1.352687.

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19

Cramer, N. F. "Magneto-acoustic surface waves on current sheets". Journal of Plasma Physics 51, n.º 2 (abril de 1994): 221–32. http://dx.doi.org/10.1017/s0022377800017530.

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The theory of linear magneto-acoustic surface waves is investigated for current sheets across which the magnetic field has an arbitrary change of direction: in the first place discontinuously, and in the second place via a narrow transition region in which the magnetic field rotates with constant amplitude, so that the gas pressure remains constant. It is found that the effect of non-zero pressure is to eliminate the surface wave for certain angles of propagation and to allow the existence of an additional, slower, surface wave for other angles of propagation. The resonance damping of the surface waves when the current sheet is of small non-zero width is considered, and it is found that Alfvénresonance damping always occurs, as well as (for high β and certain angles of propagation) compressive- or cusp-resonance damping.

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20

Yasin, S., A. V. Andreev, A. Sytcheva, J. Wosnitza e S. Zherlitsyn. "Magneto-Acoustic Properties of UCuGe Single Crystal". Journal of Low Temperature Physics 159, n.º 1-2 (31 de dezembro de 2009): 105–8. http://dx.doi.org/10.1007/s10909-009-0088-4.

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21

Ajabshirizadeh, A., E. Tavabi e S. Koutchmy. "Magneto-acoustic wave oscillations in solar spicules". Astrophysics and Space Science 319, n.º 1 (28 de novembro de 2008): 31–35. http://dx.doi.org/10.1007/s10509-008-9951-z.

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22

Campos, L. M. B. C. "On two-dimensional magneto-acoustic-gravity waves". Advances in Space Research 11, n.º 1 (janeiro de 1991): 237–45. http://dx.doi.org/10.1016/0273-1177(91)90116-2.

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23

Goto, Terutaka, Takashi Suzuki, Yohichi Ohe, Tadao Fujimura, Shinichi Sakatsume, Yoshichika \barOnuki e Takemi Komatsubara. "Magneto-Acoustic Effect of CeCu6at Low Temperatures". Journal of the Physical Society of Japan 57, n.º 8 (15 de agosto de 1988): 2612–15. http://dx.doi.org/10.1143/jpsj.57.2612.

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24

Almansouri, Abdullah Saud, Khaled Nabil Salama e Jurgen Kosel. "Magneto-Acoustic Resonator for Aquatic Animal Tracking". IEEE Transactions on Magnetics 55, n.º 2 (fevereiro de 2019): 1–4. http://dx.doi.org/10.1109/tmag.2018.2861980.

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25

Shunqi, Zhang, Xiaoqing Zhou, Yin Tao e Liu Zhipeng. "Magneto-acoustic imaging by continuous-wave excitation". Medical & Biological Engineering & Computing 55, n.º 4 (1 de julho de 2016): 595–607. http://dx.doi.org/10.1007/s11517-016-1538-1.

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26

Велев, Борис, Иван Иванов e Владимир Каменов. "Автоматизированная система комплексного неразрушающего контроля структуры и механических свойств материалов машиностроения". Дефектоскопия 3 (março de 2021): 17–25. http://dx.doi.org/10.31857/s0130308221030027.

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An automated system with two optimized modular devices is presented — MULTITEST-MC010 for research of ferromagnetic materials with the methods for measuring magnetic noise and magneto acoustic emission of Barkhausen and MULTITEST — CD010 for research of mechanical engineering materials with the methods of velocity measurement of longitudinal waves C and attenuation coefficient δof ultrasound. The main approaches and principles for the automated data processing of complex non-destructive testing are presented, as well as the setup of the modular devices of the automated system. For approbation of the system the influence of the heat treatment (hardness) in structural steel 40X on the non-destructive information parameters of the magnetic noise and the magneto acoustic emission — magnetic noise voltage EBN and voltage of the magneto acoustic emission EMAE was studied. The mechanical properties in foundry cast iron samples with complex measurement of the information parameters , C, by simultaneous use of the two modular devices of the system were also studied. The possibility for the complex application of these parameters for non-destructive testing of the mechanical properties after heat treatment in structural steel 40X and the tensile strength in cast iron specimens has been proven.

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27

Liu, Yang, Jing Li, Heming Chen, Yan Cai, Tianyu Sheng, Peng Wang, Zhiyong Li, Fang Yang e Ning Gu. "Magnet-activatable nanoliposomes as intracellular bubble microreactors to enhance drug delivery efficacy and burst cancer cells". Nanoscale 11, n.º 40 (2019): 18854–65. http://dx.doi.org/10.1039/c9nr07021d.

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28

Qu, Zhuohang, Rongguo Zhao e Jianbiao Wen. "Numerical simulation of structure design of magnetoelectric composite ultrasonic levitation device based on multi-physical field coupling". Journal of Physics: Conference Series 2230, n.º 1 (1 de março de 2022): 012023. http://dx.doi.org/10.1088/1742-6596/2230/1/012023.

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Abstract Aiming at the coupling simulation problem that ignores the acoustic structure boundary in the traditional acoustic suspension simulation, based on the magnetostrictive effect, the piezoelectric effect, and the acoustic-structure coupling model, this paper uses a magnetoelectric structure composed of the magnetostrictive material Terfenol-D and the piezoelectric ceramic PZT-5H. The composite material is used as, and the magneto-electric-acoustic fully coupled model of the magneto-electric composite material is established and compared with the one-way coupling model; The particle levitation of magnetoelectric composite materials in the multi-field coupling environment of the magnetic field, electric field, sound field, and displacement field was simulated and calculated; the influence of different widths of magneto-electric composite materials and the size of the resonant cavity on the effect of acoustic levitation was analyzed, and the best results were obtained. The geometric parameters required for optimal suspension are analyzed; the sound pressure output performance of the overall magnetoelectric composite ultrasonic suspension device under the optimal size and the judgment of the suspension position is analyzed, and I displayed the good suspension of the simulated particles in the sound field visually. The research results show that the difference in the amplitude output of the transducer will affect the sound pressure output performance of the transducer, and there is a large error in the one-way coupling; the magnetoelectric composite material can be used as an ultrasonic transducer to achieve acoustic suspension, and suspended particles It shows a good acoustic levitation effect in the simulation. The fully coupled simulation of ultrasonic transducers and the research on such ultrasonic transducers can open new ideas for the research and development of new ultrasonic transducers in the future.

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29

Ryutova, Margarita. "Generation of Plasma Flows and Filamentation of Magnetic Fields in the Solar Atmosphere". International Astronomical Union Colloquium 141 (1993): 549–53. http://dx.doi.org/10.1017/s0252921100029821.

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AbstractNonlinear effects in dynamics of solar magnetic fields which, in particular, determine the evolution of solar magnetic structures and their lifetimes, are discussed. By some analogy with the effects of acoustic streaming in usual hydrodynamics the general definition of these effects as “magneto acoustic streaming” is proposed.

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30

Khomenko, Elena, e Oleg Kochukhov. "Simulations of magneto-hydrodynamic waves in atmospheres of roAp stars". Proceedings of the International Astronomical Union 4, S259 (novembro de 2008): 409–10. http://dx.doi.org/10.1017/s1743921309030907.

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AbstractWe report 2D time-dependent non-linear magneto-hydrodynamical simulations of waves in the atmospheres of roAp stars. We explore a grid of simulations in a wide parameter space. The aim of our study is to understand the influence of the atmosphere and the magnetic field on the propagation and reflection properties of magneto-acoustic waves, formation of shocks and node layers.

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31

Sabri, S., S. Poedts e H. Ebadi. "Plasma heating by magnetoacoustic wave propagation in the vicinity of a 2.5D magnetic null-point". Astronomy & Astrophysics 623 (março de 2019): A81. http://dx.doi.org/10.1051/0004-6361/201834286.

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Context. Magnetohydrodynamic (MHD) waves have significant potential as a plasma heating mechanism. Finding a suitable wave dissipation mechanism is a very tough task, given the many observational constraints on the models, and this has resulted in the development of an important research community in solar physics. The magnetic field structure has an important role in the solar corona heating. Here, we investigate in detail current sheet mode generation via magnetic reconnection and mode conversion releases some of the free magnetic energy and produces heating. In addition, energy conversion is discussed completely. Moreover, nonlinear effects on density variations and, in turn, mode conversion are pursued. Aims. In order to assess the role of magnetoacoustic waves in plasma heating, we have modeled in detail a fast magneto-acoustic wave pulse near a magnetic null-point in a finite plasma-β. The behavior of the propagation and dissipation of the fast magneto-acoustic wave is investigated in the inhomogeneous magnetically structured solar corona. Particular attention is given to the dissipation of waves and coronal heating and energy transfer in the solar corona, focusing on the energy transfer resulting from the interaction of fast magneto-acoustic waves with 2.5D magnetic null-points. Methods. The shock−capturing Godunov−type PLUTO code was used to solve the ideal MHD set of equations in the context of wave-plasma energy transfer. Results. It is shown that magneto-acoustic waves could be a viable candidate to contribute significantly to the heating of the solar corona and maintain the solar corona at a temperature of a few million degrees. The temperature is not constant in the corona. Coronal heating occurs near magnetic null points. It is found that magnetic reconnection, phase mixing and mode conversion contribute to the heating. Moreover, nonlinear fast and slow magnetoacoustic waves are decoupled except in β = 1 layer.

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32

Jain, M. K., S. Schmidt, C. Mungle, K. Loiselle e C. A. Grimes. "Measurement of temperature and liquid viscosity using wireless magneto-acoustic/magneto-optical sensors". IEEE Transactions on Magnetics 37, n.º 4 (julho de 2001): 2767–69. http://dx.doi.org/10.1109/20.951301.

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33

Narayanan, A. Satya, C. Kathiravan e R. Ramesh. "Alfvén waves in a gravitational field with flows". Proceedings of the International Astronomical Union 4, S257 (setembro de 2008): 563–68. http://dx.doi.org/10.1017/s174392130902986x.

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AbstractThe gravitational stratification effect on magnetohydrodynamic waves at a single interface in the solar atmosphere has been studied in the penumbral region of the sunspot recently. The existence of slow and fast magneto acoustic gravity waves and their characteristics has been discussed. The effect of flows on magneto acoustic gravity surface waves leads to modes called flow modes or v-modes. The present geometry is that of a plasma slab moving with uniform velocity surrounded by a plasma of different density. As is applicable to the corona, we assume that the plasma β to be small. The dispersion characteristics change significantly with a change in the value of G (gravity) and uniform flow.

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34

Henderson, Hunter B., Orlando Rios, Gerard M. Ludtka e Michele V. Manuel. "Investigation and Analytical Description of Acoustic Production by Magneto-Acoustic Mixing Technology". Metallurgical and Materials Transactions B 46, n.º 5 (7 de maio de 2015): 2020–27. http://dx.doi.org/10.1007/s11663-015-0359-1.

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35

Wu, Wei, Robert Sych, Jie Chen e Jiang-Tao Su. "Magneto-acoustic waves in magnetic twisted flux tubes". Research in Astronomy and Astrophysics 21, n.º 5 (1 de junho de 2021): 126. http://dx.doi.org/10.1088/1674-4527/21/5/126.

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36

Goldberg, Z., e A. Goldberg. "Goldberg’s Number for Magneto-Acoustic Finite Amplitude Waves". Acoustical Physics 67, n.º 6 (novembro de 2021): 582–83. http://dx.doi.org/10.1134/s1063771021330010.

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37

Latcham, O. S., Y. I. Gusieva, A. V. Shytov, O. Y. Gorobets e V. V. Kruglyak. "Controlling acoustic waves using magneto-elastic Fano resonances". Applied Physics Letters 115, n.º 8 (19 de agosto de 2019): 082403. http://dx.doi.org/10.1063/1.5115387.

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Islam, M. R., e B. C. Towe. "Bioelectric current image reconstruction from magneto-acoustic measurements". IEEE Transactions on Medical Imaging 7, n.º 4 (dezembro de 1988): 386–91. http://dx.doi.org/10.1109/42.14523.

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39

Mushtaq, A. "Ion acoustic solitary waves in magneto-rotating plasmas". Journal of Physics A: Mathematical and Theoretical 43, n.º 31 (6 de julho de 2010): 315501. http://dx.doi.org/10.1088/1751-8113/43/31/315501.

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40

Obregon, M. A., e Yu A. Stepanyants. "Oblique magneto-acoustic solitons in a rotating plasma". Physics Letters A 249, n.º 4 (dezembro de 1998): 315–23. http://dx.doi.org/10.1016/s0375-9601(98)00735-x.

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41

Nogaret, A., L. Eaves, P. C. Main, M. Henini, D. K. Maude, J. C. Portal, E. Molinari e S. P. Beaumont. "Magneto-acoustic phonon antiresonances in Wannier–Stark superlattices". Solid-State Electronics 42, n.º 7-8 (julho de 1998): 1489–93. http://dx.doi.org/10.1016/s0038-1101(98)00055-0.

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42

Mendoza-Briceño, César A., Miguel H. Ibáñez e Valery M. Nakariakov. "Nonlinear magneto-acoustic waves in the solar atmosphere". Dynamics of Atmospheres and Oceans 34, n.º 2-4 (outubro de 2001): 399–409. http://dx.doi.org/10.1016/s0377-0265(01)00077-x.

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43

Aburdzhaniya, G. D., V. P. Lakhin e A. B. Mikhailovskii. "Nonlinear regular structures of drift magneto-acoustic waves". Journal of Plasma Physics 38, n.º 3 (dezembro de 1987): 373–86. http://dx.doi.org/10.1017/s0022377800012666.

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Nonlinear regular structures in a magnetized plasma connected with drift magneto-acoustic waves (DMA) are investigated theoretically. Three-dimensional nonlinear equations of weakly dispersive DMA waves are obtained. These equations contain both the scalar nonlinearity and the vector one, and generalize the two-dimensional Kadomtsev–Petviashvili (KP) equation. The existence is shown of regular stationary structures due to the scalar nonlinearity: one-dimensional solitons, two-dimensional rational solitons, chains of solitons and so-called ‘crosses’. The stability of one-dimensional DMA solitons is investigated. It is shown that soliton stability depends on the sign of the wave dispersion as in the case of systems described by the KP-type equation.

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44

Wang, Jing-xiu. "On the propagation of magneto-acoustic-gravity waves". Chinese Astronomy and Astrophysics 10, n.º 4 (dezembro de 1986): 291–97. http://dx.doi.org/10.1016/0275-1062(86)90019-6.

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45

Buttle, D. J. "Barkhausen and magneto-acoustic emission from ferromagnetic materials". NDT & E International 24, n.º 1 (fevereiro de 1991): 48. http://dx.doi.org/10.1016/0963-8695(91)90796-6.

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Bigot, Lionel. "Theory of Magneto-Acoustic Modes in roAp Stars". International Astronomical Union Colloquium 193 (2004): 445–52. http://dx.doi.org/10.1017/s0252921100011118.

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AbstractIn this review I present the effects of a strong magnetic field on the pulsations of rapidly oscillating Ap stars. I show how the field affects the observables, such as the frequencies and eigenvectors, and the selection of modes.

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Hussain, S., N. Akhtar e H. Hasnain. "Ion acoustic shocks in magneto rotating Lorentzian plasmas". Physics of Plasmas 21, n.º 12 (dezembro de 2014): 122120. http://dx.doi.org/10.1063/1.4905060.

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Matsui, Hiroshi, Terutaka Goto, Tadao Fujimura, Takemi Komatsubara, Yosikazu Isikawa e Kiyoo Sato. "Magneto-Acoustic Effect of Heavy Fermion Compound CeInCu2". Journal of the Physical Society of Japan 59, n.º 10 (15 de outubro de 1990): 3451–54. http://dx.doi.org/10.1143/jpsj.59.3451.

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Hanna, S. M., e G. P. Murphy. "Magneto‐acoustic Bragg diffraction of magnetostatic waves (abstract)". Journal of Applied Physics 67, n.º 9 (maio de 1990): 5505. http://dx.doi.org/10.1063/1.345865.

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Stenflo, L., P. K. Shukla e N. L. Tsintsadze. "Solitary magneto-acoustic waves in partially ionized plasmas". Physics Letters A 191, n.º 1-2 (agosto de 1994): 159–61. http://dx.doi.org/10.1016/0375-9601(94)90576-2.

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