oscillating sphere
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2021 ◽  
Vol 9 (12) ◽  
pp. 1317
Author(s):  
Huan Wang ◽  
Erzheng Fang ◽  
Mingze Wu ◽  
Lianjin Hong ◽  
Zongru Li

When an underwater target moves in viscous fluid, it may cause the periodic movement of the surrounding fluid and generate ultra-low-frequency (ULF) gravity waves. The initial domain of the gravitational surface wave propagating above the moving target is named circular wave. This article studies the ULF circular wave generated by underwater oscillating sphere, which will provide basis for underwater long-range target detection. Firstly, the circular wave caused by the sphere oscillation in a finite deep fluid is studied based on the theory of linear potential flow. Meanwhile, the multipole expansion theory is established to solve the circular wave field. Secondly, the interface wave generated by the target oscillation in a two-layer fluid are numerically analyzed by comparison with the free surface fluctuation of a single-layer fluid. The results show that the amplitude of the internal interface displacement (AIID) is smaller than that of the free surface (AFSD). When the sphere is in the lower layer, the layering effect of the fluid has significant influences on the AFSD. Finally, the results of the pool experiment verified that the wave generated by the oscillating sphere is the surface gravity wave. Furthermore, the change trend of the test result is consistent with the simulation result.


2021 ◽  
Vol 33 (9) ◽  
pp. 097106
Author(s):  
Samayam Satish ◽  
Justin S. Leontini ◽  
Richard Manasseh ◽  
S. A. Sannasiraj ◽  
V. Sundar

2020 ◽  
Vol 5 (1) ◽  
Author(s):  
Yanzhen He ◽  
Lu Li ◽  
Takashi Taniguchi ◽  
Remco Tuinier ◽  
Tai-Hsi Fan

2020 ◽  
Vol 2020 (0) ◽  
pp. J10214
Author(s):  
Masashi YAMAMOTO ◽  
Kyohei MATSUMOTO ◽  
Hideki SHIMOHARA ◽  
Takashi NOGUCHI ◽  
Katsuya HIRATA

2019 ◽  
Vol 33 (3) ◽  
pp. 283-294
Author(s):  
Katsuya HIRATA ◽  
Tomoya KITAMOTO ◽  
Hajime ONISHI ◽  
Yusuke YAMAOKA ◽  
Hideki SHIMOHARA ◽  
...  

2018 ◽  
Vol 849 ◽  
pp. 834-859 ◽  
Author(s):  
F. Box ◽  
K. Singh ◽  
T. Mullin

We present the results of an experimental and theoretical investigation into the influence of proximate boundaries on the motion of an rotationally oscillating sphere in a viscous fluid. The angular oscillations of the sphere are controlled using the magnetic torque generated by a spatially uniform, oscillatory magnetic field which interacts with a small magnet embedded within the sphere. We study the motion of the sphere in the vicinity of stationary walls that are parallel and perpendicular to the rotational axis of the sphere, and near a second passive sphere that is non-magnetic and free to move. We find that rigid boundaries introduce viscous resistance to motion that acts to suppress the oscillations of the driven sphere. The amount of viscous resistance depends on the orientation of the wall with respect to the axis of rotation of the oscillating sphere. A passive sphere also introduces viscous resistance to motion, but for this case the rotational oscillations of the active sphere establish a standing wave that imparts vorticity to the fluid and induces oscillations of the passive sphere. The standing wave is analogous to the case of an oscillating plate in a viscous fluid; the amplitude of the wave decays exponentially with radial distance from the surface of the oscillating sphere. The standing wave introduces a phase lag between the motion of the active sphere and the response of the passive sphere which increases linearly with separation distance.


2014 ◽  
Vol 14 (6) ◽  
pp. 1914-1922 ◽  
Author(s):  
Stefan Clara ◽  
Hannes Antlinger ◽  
Bernhard Jakoby

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