Turbulence structure over heated surfaces: Numerical solutions

被引:6
作者
Nosov V.V. [1 ]
Lukin V.P. [1 ]
Nosov E.V. [1 ]
Torgaev A.V. [1 ]
机构
[1] V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences, pl. Akademika Zueva 1, Tomsk
关键词
coherent structure; coherent turbulence; inhomogeneously heated surface; Navier–Stokes equations; simulation of coherent structures; thermal diversity; topological soliton; turbulence;
D O I
10.1134/S1024856016030118
中图分类号
学科分类号
摘要
The structure of air turbulent motions inside closed volumes (without exchange of material through the boundary) over inhomogeneously heated underlying surfaces is studied by the numerical solution of boundary problems for hydrodynamics equations (Navier–Stokes). Large solitary vortices (coherent structures, topological solitons) are observed over inhomogeneously heated surfaces. The number of vortices and their internal structure depend on the form and size of heated inhomogenities. In the case of simple forms of heating (homogeneous heating, a round heated spot), a coherent turbulence induced by the decay of coherent vortices is observed inside a closed volume. For complex forms of heating (thermal diversity), the toroidal vortices are noticeably deformed. The vortices can be extended along the surface and have spiral (helix) streamlines. The vortices are noticeably mixed during the evolution, which results in a Kolmogorov (incoherent) turbulence. Experimental data received earlier inside dome rooms of astronomical telescopes confirm our numerical simulation. © 2016, Pleiades Publishing, Ltd.
引用
收藏
页码:234 / 243
页数:9
相关论文
共 36 条
[1]  
Nosov V.V., Grigor'ev V.M., Kovadlo P.G., Lukin V.P., Nosov E.V., Torgaev A.V., Astroclimate of specialized rooms of the Large solar vacuum telescope. Part 1, Atmos. Ocean. Opt., 20, 11, pp. 926-934, (2007)
[2]  
Nosov V.V., Grigor'ev V.M., Kovadlo P.G., Lukin V.P., Nosov E.V., Torgaev A.V., Astroclimate of specialized rooms of the Large solar vacuum telescope. Part 2, Atmos. Ocean. Opt., 21, 3, pp. 180-190, (2008)
[3]  
Nosov V.V., Grigoriev V.M., Kovadlo P.G., Papushev P.G., Torgaev A.V., Astroclimate inside the dome of AZT-14 telescope of Sayan Solar Observatory, Proc. SPIE, 69361R, pp. 1-4, (2007)
[4]  
Nosov V.V., Grigor'ev V.M., Kovadlo P.G., Lukin V.P., Nosov E.V., Torgaev A.V., Coherent structures in turbulent atmosphere. Experiment and Theory, Solnech.-Zemnaya Fiz., 14, pp. 97-113, (2009)
[5]  
Nosov V.V., Lukin V.P., Nosov E.V., Torgaev A.V., Grigoriev V.M., Kovadlo P.G., Coherent structures in turbulent atmosphere, Proc. SPIE, 7296-9, pp. 53-70, (2009)
[6]  
Nosov V.V., Lukin V.P., Nosov E.V., Torgaev A.V., Grigoriev V.M., Kovadlo P.G., Coherent Structures in the Turbulent Atmosphere, Mathematical Models of Non-Linear Phenomena, Processes and Systems: From Molecular Scale to Planetary Atmosphere, Ed. by A.B. Nadycto et al. (Nova Science Publishers, N.Y., 2013), chap., 20, pp. 297-330
[7]  
Nosov V.V., Kovadlo P.G., Lukin V.P., Torgaev A.V., Atmospheric coherent turbulence, Atmos. Ocean. Opt., 26, 3, pp. 201-206, (2013)
[8]  
Nosov V.V., Grigor'ev V.M., Kovadlo P.G., Lukin V.P., Papushev P.G., Torgaev A.V., Results of measurement of astroclimate parameters of the under-dome space of the AXT-33 telescope of the Sayan solar observatory, Institute of Solar-Terrestrial Physics SB RAS, Solnech.-Zemnaya Fiz., 9, pp. 101-102, (2006)
[9]  
Nosov V.V., Lukin V.P., Torgaev A.V., Grigoriev V.M., Kovadlo P.G., Result of measurements of the astroclimate characteristics of astronomical telescopes in the mountain observatories, Proc. SPIE, 7296-11, pp. 82-87, (2009)
[10]  
Nosov V.V., Lukin V.P., Torgaev A.V., Grigoriev V.M., Kovadlo P.G., Astroclimate parameters of the surface layer in the Sayan solar observatory, Proc. SPIE, 7296-12, pp. 87-94, (2009)