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Turkyilmazoglu M (2011) Wall stretching in magnetohydrodynamics rotating flows in inertial and rotating frames. AIAA J Thermophys Heat Transfer 25(4):606–613 15. Turkyilmazoglu M (2011) Thermal radiation effects on the time-dependent MHD permeable flow having variable viscosity. Int J Thermal Sci 50(1):88–96 16. Turkyilmazoglu M (2012) Effects of uniform radial electric field on the MHD heat and fluid flow due to a rotating disk. Int J Eng Sci 51:233–240 17. Turkyilmazoglu M (2012) Three dimensional MHD stagnation flow due to a stretchable rotating disk.

34 [3, 4, 6, 15–25] (Fig. 3). 1. They result from a solution of Eqs. 2 lg(Reω ) Fig. 3 Local Nusselt numbers on a rotating disk [1]. ; 2— Tw ≈ const. 3–10—calculations, Eq. 4). 0187 [26]. 34 [6]. 1 Constant K1 according to the exact solution of Eqs. 1981 K1 ¼ Àh0f¼0 : ð3:5Þ For Tw = const. , the exponent in Eq. 30) for laminar flow is the same: n* = 0. g. 1). For non-isothermal disks and smaller values of the Pr number, there are no experimental data in literature that would enable validation of the constant K1.

Inzhenerno-Fizicheskiy Zhurnal 7(1):3–11 (in Russian) 80. Kapinos VM (1965) Heat transfer from a disc rotating in a housing with a radial flow of coolant. J Eng Phys Thermophys 8(1):35–38 81. Kapinos VM (1965) Heat transfer of a disk rotating in a housing. Izvestiya vuzov. Aviatsyonnaya Tekhnika 2:76–86 (in Russian) 82. Goldstein S (1935) On the resistance to the rotation of a disc immersed in a fluid. Proc Cambridge Phil Soc 31:232–241 83. Johnson MC (1980) Turbulent heat transfer to a rotating disk: a review and extension of Dorfman.

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101 glorious ways to cook chicken

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