Academic literature on the topic 'Meridional shape'

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Journal articles on the topic "Meridional shape"

1

Wang, Yan, Quanlin Dong, and Yulian Zhang. "Meridional shape design and the internal flow investigation of centrifugal impeller." Proceedings of the Institution of Mechanical Engineers, Part C: Journal of Mechanical Engineering Science 231, no. 23 (2016): 4319–30. http://dx.doi.org/10.1177/0954406216667407.

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This paper describes an inverse design method for calculating the shape of meridional plane of centrifugal impeller. This design method permits the shroud and hub contours to be indirectly calculated by medial axis contour and constraint equations. The design process is computationally inexpensive and can conveniently modify the shroud and hub shapes as the design’s demand. Based on this design method, new constraint equations are used for a new shape design of meridional plane that lead to a uniform velocity distribution in the inlet of impeller. Numerical simulations are employed to investig
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2

Ragen, Sarah, Kyle C. Armour, LuAnne Thompson, Andrew Shao, and David Darr. "The Role of Atlantic Basin Geometry in Meridional Overturning Circulation." Journal of Physical Oceanography 52, no. 3 (2022): 475–92. http://dx.doi.org/10.1175/jpo-d-21-0036.1.

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Abstract We present idealized simulations to explore how the shape of eastern and western continental boundaries along the Atlantic Ocean influences the Atlantic meridional overturning circulation (AMOC). We use a state-of-the art ocean–sea ice model (MOM6 and SIS2) with idealized, zonally symmetric surface forcing and a range of idealized continental configurations with a large, Pacific-like basin and a small, Atlantic-like basin. We perform simulations with five coastline geometries along the Atlantic-like basin that range from coastlines that are straight to coastlines that are shaped like
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3

Miyauchi, Sunao, Hironori Horiguchi, Jun-ichirou Fukutomi, and Akihiro Takahashi. "K-1102 Optimization of Meridional Shape Design of Pump Impeller." Proceedings of the JSME annual meeting II.01.1 (2001): 25–26. http://dx.doi.org/10.1299/jsmemecjo.ii.01.1.0_25.

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4

Chen, Xin, Linlin Cao, Peng Yan, Peng Wu, and Dazhuan Wu. "Effect of meridional shape on performance of axial-flow fan." Journal of Mechanical Science and Technology 31, no. 11 (2017): 5141–51. http://dx.doi.org/10.1007/s12206-017-1008-1.

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5

Talon, Suzanne, Georges Michaud, and Alain Vincent. "On meridional Circulation in Stars." Symposium - International Astronomical Union 198 (2000): 498–99. http://dx.doi.org/10.1017/s0074180900167154.

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Even though the existence of meridional currents in stars has been known for quite a long time (Eddington 1925, Vogt 1925), its exact structure as well as its influence on stellar evolution is still unclear. Some authors concentrated on finding the exact shape of meridional circulation in a rotating star, while others tried to model its effect on the chemical distribution in the interior. In all studies performed so far however, meridional circulation is considered in an asymptotic regime in which the advection of entropy by the meridional currents is supposed to balance exactly the source ter
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6

Miyauchi, Sunao, Hironori Horiguchi, Jun-ichirou Fukutomi, and Akihiro Takahashi. "Optimization of Meridional Flow Channel Design of Pump Impeller." International Journal of Rotating Machinery 10, no. 2 (2004): 115–19. http://dx.doi.org/10.1155/s1023621x04000120.

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The meridional flow channel design of a pump impeller affects its performance. However, since so many design parameters exist, a new design method is proposed in which a meridional and blade-to-blade flow channel is designed by the parallel use of the circulation distribution provided by the designer. Thus, an optimization method was used to design an axis-symmetrical meridional flow channel from the circulation distribution. In addition, the inverse design method proposed by Zangeneh et al. (1996) was employed to design a three-dimensional blade-to-blade flow channel from the circulation dist
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7

Kim, Sung, Young-Seok Choi, Kyoung-Yong Lee, and Jun-Ho Kim. "Design Optimization of Mixed-flow Pump in a Fixed Meridional Shape." International Journal of Fluid Machinery and Systems 4, no. 1 (2011): 14–24. http://dx.doi.org/10.5293/ijfms.2011.4.1.014.

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8

Kvasha, Yu A., and N. A. Zinevych. "On the effect of the meridional contour shape on the power characteristics of a centrifugal compressor wheel." Technical mechanics 2020, no. 3 (2020): 12–17. http://dx.doi.org/10.15407/itm2020.03.012.

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This work is concerned with the development of approaches to the optimal aerodynamic design of centrifugal compressor wheels, which is due to the use of centrifugal stages in compressors of modern aircraft gas turbine engines and power plants. The aim of this work is a computational study of the effect of the meridional contour shape of a centrifugal compressor wheel on its power characteristics. The basic method is a numerical simulation of 3D turbulent gas flows in centrifugal wheels on the basis of the complete averaged Navier¬–Stokes equations and a two-parameter turbulence model. The comp
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9

Lutsko, Nicholas J., and Isaac M. Held. "The Response of an Idealized Atmosphere to Orographic Forcing: Zonal versus Meridional Propagation." Journal of the Atmospheric Sciences 73, no. 9 (2016): 3701–18. http://dx.doi.org/10.1175/jas-d-16-0021.1.

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Abstract A dry atmospheric general circulation model is forced with large-scale, Gaussian orography in an attempt to isolate a regime in which the model responds linearly to orographic forcing and then to study the departures from linearity as the orography is increased in amplitude. In contrast to previous results, which emphasized the meridional propagation of orographically forced stationary waves, using the standard Held–Suarez (H–S) control climate, it is found that the linear regime is characterized by a meridionally trapped, zonally propagating wave. Meridionally trapped waves of this k
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10

Biggs, James D. "Meridional Compression of Radio Pulsar Beams." International Astronomical Union Colloquium 128 (1992): 22–25. http://dx.doi.org/10.1017/s0002731600154691.

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AbstractWe have studied the radio pulsar emission beam assuming a) a magnetic dipole field geometry and b) that the beam geometry is defined by the field lines that are not contained within the light cylinder. In general, the beam is compressed in the meridional direction. When the magnetic and rotation axes are aligned the beam is circular and as, the angle between these axes increases, the ratio of meridional to longitudinal dimension decreases monotonically to the minimum value 0.62 when the axes are orthogonal. This beam shape is thus consistent with that inferred from the study of circula
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