Showing 1 - 20 results of 1,786 for search '"Prandtl number"', query time: 0.45s Refine Results
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    On the magnetic prandtl number behavior of accretion disks by Balbus, S, Henri, P

    Published 2008
    “…We investigate the behavior of the magnetic Prandtl number (the ratio of microscopic viscosity to resistivity) for accretion sources. …”
    Journal article
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    Prandtl Number and Viscosity Correlations of Titanium Oxide Nanofluids by Palesa Helen Mlangeni, Zhongjie Huan, Thembelani Sithebe, Vasudeva Rao Veeredhi

    Published 2023-01-01
    “…Many features of nanofluids, such as the Prandtl number and viscosity, are researched as the number of studies conducted in the field of nanofluids increases. …”
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    Article
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    The effects of Prandtl number on black hole accretion flows by Balbus, S, Lesaffre, P

    Published 2008
    “…This dimensionless quantity is known as the magnetic Prandtl number Pm. In general, standard astrophysical accretion disks are characterized by Pm ≪ 1 throughout their radial extent, while low luminosity accretors (e.g. …”
    Journal article
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    Critical magnetic Prandtl number for small-scale dynamo. by Schekochihin, A, Cowley, S, Maron, J, McWilliams, J

    Published 2004
    “…Namely, the dynamo is shut down if the magnetic Prandtl number Pr(m)=Rm/Re is less than some critical value Pr(m,c)< approximately 1 even for Rm for which dynamo exists at Pr(m)> or =1. …”
    Journal article
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    A numerical simulation on high prandtl number liquid bridge by Yang Shuo, Liang Ruquan, He Jicheng

    Published 2015-01-01
    “…The free surface characteristics of high prandtl number liquid bridge with dynamic deformation have been investigated under microgravity based on the Navier-Stokes equations coupled with the energy conservation equation on a staggered grid. …”
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    Article
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    Numerical demonstration of fluctuation dynamo at low magnetic Prandtl numbers. by Iskakov, AB, Schekochihin, A, Cowley, S, McWilliams, J, Proctor, MR

    Published 2007
    “…In the limit Pm<<1, Rmc is about 3 times larger than for the previously well-established dynamo at large and moderate Prandtl numbers: Rmc less than or similar 200 for Re greater than or similar 6000 compared to Rmc approximately 60 for Pm>or=1. …”
    Journal article
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    Fluctuation dynamo and turbulent induction at low magnetic Prandtl numbers by Schekochihin, A, Iskakov, AB, Cowley, S, McWilliams, J, Proctor, M, Yousef, T

    Published 2007
    “…In the limit Pm ≪ 1, Rmc is at most three times larger than for the previously well established dynamo at large and moderate Prandtl numbers: Rmc ≲ 200 for Re ≳ 6000 compared to Rmc ∼ 60 for Pm ≥ 1. …”
    Journal article
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    Fluctuation dynamo and turbulent induction at low magnetic Prandtl numbers by Schekochihin, A, Iskakov, AB, Cowley, S, McWilliams, J, Proctor, M, Yousef, T

    Published 2007
    “…This paper is a detailed report on a programme of simulations used to settle a long-standing issue in the dynamo theory and demonstrate that the fluctuation dynamo exists in the limit of large magnetic Reynolds number Rm&gt;&gt;1 and small magnetic Prandtl number Pm&lt;&lt;1. The dependence of the critical Rm_c vs. the hydrodynamic Reynolds number Re is obtained for 1<re<6700. for="" in="" is="" larger="" limit="" pm="" pm<<1,="" rm_c="" than="" the="" times="" ~3="">1. …”
    Journal article
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    Effects of external environment on thermocapillary convection of high prandtl number fluid by Liang Ruquan, Yan Fuqiang, Li Xiaoyuan, Zhang Shuo, Yang Shuo

    Published 2016-01-01
    “…Numerical simulations have been carried out to investigate the influence of external environment on thermocapillary convection in high Prandtl number (Pr=68) liquid. The geometric model of physical problem is that the the liquid bridge surrounded by ambient air under zero or ground gravity. …”
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    Article
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    The onset of turbulent rotating dynamos at the low magnetic Prandtl number limit by Seshasayanan, K, Dallas, V, Alexakis, A

    Published 2017
    “…We demonstrate that the critical magnetic Reynolds number Rm c for a turbulent nonhelical dynamo in the limit of low magnetic Prandtl number Pm (i.e. Pm=Rm/Re ≪ 1) can be significantly reduced if the flow is subjected to global rotation. …”
    Journal article