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| Autores principales: | , |
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| Formato: | Preprint |
| Publicado: |
2024
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| Materias: | |
| Acceso en línea: | https://arxiv.org/abs/2406.06256 |
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| _version_ | 1866929380378279936 |
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| author | Kumar, Prince Sharma, Devendra |
| author_facet | Kumar, Prince Sharma, Devendra |
| contents | A numerical simulation of Kelvin-Helmholtz Instability (KHI) in parallel shear flows subjected to external rotation is carried out using a pseudo-spectral technique. The Coriolis force, arising in a rotation frame under the beta plane approximation, tends to suppress the growth of KHI modes. The numerical results show a close qualitative agreement with the analytical results obtained for a step-wise shear flow profile. Experimental evidence demonstrates that particles in a rotating frame experience the Coriolis force, mathematically equivalent to the Lorentz force. Therefore, the Coriolis force affects fluid dynamics in a manner similar to the Lorentz force in magnetized shear flows. This paper exploits the analogy between the magnetic field and rotation to study effects equivalent to a magnetic field on KHI in a rotating frame. Similar to the magnetic field case, the Coriolis force suppresses KHI and tends to form compressed and elongated KH vortex structures. However, the magnetic field and Coriolis force act on different scales, with the latter suppressing long-wavelength mode perturbations. A higher number of vortices are observed in the presence of rotation compared to non-rotating cases |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_06256 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Study on Kelvin Helmholtz shear flows subjected to differential rotation Kumar, Prince Sharma, Devendra Fluid Dynamics Plasma Physics A numerical simulation of Kelvin-Helmholtz Instability (KHI) in parallel shear flows subjected to external rotation is carried out using a pseudo-spectral technique. The Coriolis force, arising in a rotation frame under the beta plane approximation, tends to suppress the growth of KHI modes. The numerical results show a close qualitative agreement with the analytical results obtained for a step-wise shear flow profile. Experimental evidence demonstrates that particles in a rotating frame experience the Coriolis force, mathematically equivalent to the Lorentz force. Therefore, the Coriolis force affects fluid dynamics in a manner similar to the Lorentz force in magnetized shear flows. This paper exploits the analogy between the magnetic field and rotation to study effects equivalent to a magnetic field on KHI in a rotating frame. Similar to the magnetic field case, the Coriolis force suppresses KHI and tends to form compressed and elongated KH vortex structures. However, the magnetic field and Coriolis force act on different scales, with the latter suppressing long-wavelength mode perturbations. A higher number of vortices are observed in the presence of rotation compared to non-rotating cases |
| title | Study on Kelvin Helmholtz shear flows subjected to differential rotation |
| topic | Fluid Dynamics Plasma Physics |
| url | https://arxiv.org/abs/2406.06256 |