Relevant bibliographies by topics / Non-axisymmetric oscillations

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  1. Journal articles

Academic literature on the topic 'Non-axisymmetric oscillations'

Author: Grafiati
Published: 6 September 2023

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Journal articles on the topic "Non-axisymmetric oscillations"

1

Sanz, A., and J. Lopez Diez. "Non-axisymmetric oscillations of liquid bridges." Journal of Fluid Mechanics 205, no. -1 (1989): 503. http://dx.doi.org/10.1017/s0022112089002120.

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2

Sotani, Hajime, and Kostas D. Kokkotas. "Non-axisymmetric Torsional Oscillations of Relativistic Stars." Journal of Physics: Conference Series 314 (September 22, 2011): 012081. http://dx.doi.org/10.1088/1742-6596/314/1/012081.

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3

Dymova, M. V., and M. S. Ruderman. "Non-Axisymmetric Oscillations of Thin Prominence Fibrils." Solar Physics 229, no. 1 (2005): 79–94. http://dx.doi.org/10.1007/s11207-005-5002-x.

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4

Lyubimov, D. V., T. P. Lyubimova, and S. V. Shklyaev. "Non-axisymmetric oscillations of a hemispherical drop." Fluid Dynamics 39, no. 6 (2004): 851–62. http://dx.doi.org/10.1007/s10697-004-0002-3.

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5

Lyubimov, D. V., T. P. Lyubimova, and S. V. Shklyaev. "Non-axisymmetric oscillations of a hemispherical drop." Fluid Dynamics 39, no. 6 (2004): 851–62. http://dx.doi.org/10.1007/s10697-005-0021-8.

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6

Khudainazarov, Sh, B. Donayev, and J. Yarashov. "Non-stationary oscillations of high-rise axisymmetric structures." IOP Conference Series: Materials Science and Engineering 883 (July 21, 2020): 012195. http://dx.doi.org/10.1088/1757-899x/883/1/012195.

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7

Ruderman, Michael S. "Non-axisymmetric oscillations of thin twisted magnetic tubes." Proceedings of the International Astronomical Union 3, S247 (2007): 344–50. http://dx.doi.org/10.1017/s1743921308015068.

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AbstractIn this paper we study non-axisymmetric oscillations of thin twisted magnetic tubes taking the density variation along the tube into account. We use the approximation of the zero-beta plasma. The magnetic field outside the tube is straight and homogeneous, however it is twisted inside the tube. We assume that the azimuthal component of the magnetic field is proportional to the distance from the tube axis, and that the tube is only weakly twisted, i.e. the ratio of the azimuthal and axial components of the magnetic field is small. Using the asymptotic analysis we show that the eigenmode
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8

Narayanan, A. Satya. "Non-Radial Oscillations in an Axisymmetric MHD Incompressible Fluid." International Astronomical Union Colloquium 179 (2000): 361–64. http://dx.doi.org/10.1017/s0252921100064836.

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AbstractIt is well known from Helioseismology that the Sun exhibits oscillations on a global scale, most of which are non-radial in nature. These oscillations help us to get a clear picture of the internal structure of the Sun as has been demonstrated by the theoretical and observational (such as GONG) studies. In this study we formulate the linearised equations of motion for non-radial oscillations by perturbing the MHD equilibrium solution for an axisymmetric incompressible fluid. The fluid motion and the magnetic field are expressed as scalarsU,V,PandT, respectively. In deriving the exact s
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9

Bohdan, A. V., O. N. Petryschev, Yu I. Yakymenko Yakymenko, and Yu Yu Yanovskaya. "Non-axisymmetric radial vibrations of thin piezoelectric disks." Electronics and Communications 16, no. 3 (2011): 195–99. http://dx.doi.org/10.20535/2312-1807.2011.16.3.266783.

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10

Lee, Umin, and Hideyuki Saio. "Angular-Momemtum Transfer by Nonradial Oscillations in Massive Main-Sequence Stars." International Astronomical Union Colloquium 137 (1993): 287–89. http://dx.doi.org/10.1017/s0252921100017942.

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Angular mementum distribution is one of the most important factors for stellar structutre and evolution. Among other mechanisms, angular momentum is transfered by non-axisymmetric oscillations (nonradial oscillations). In this mechanism the angular momentum is carried mainly by the Reynolds stress, which is proportional to the product between radial and azimuthal components of oscillation velocity; i.e., (Φ direction is the direction of rotation velocity). In the linear oscillation analysis, the phase difference between and is with A finite value of δ, which arises from excitation or damping o
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