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Comment on the paper “Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy, N. Anbuchezhian, K. Srinivasan, K. Chandrasekaran, R. Kandasamy, Meccanica (2013) 48:307–321”

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Abstract

In the above paper a theoretical investigation of MHD convective flow and heat transfer of an incompressible viscous nanofluid past a porous vertical stretching sheet in the presence of variable stream condition is presented. The governing boundary layer equations are transformed by a Lie symmetry group transformation and the ordinary differential equations are solved numerically using Runge–Kutta Gill method.

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Reference

  1. Anbuchezhian N, Srinivasan K, Chandrasekaran K, Kandasamy R (2013) Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy. Meccanica 48:307–321

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  1. School of Engineering, Democritus University of Thrace, 67100, Xanthi, Greece

    Asterios Pantokratoras

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  1. Asterios Pantokratoras
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Correspondence to Asterios Pantokratoras.

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Pantokratoras, A. Comment on the paper “Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy, N. Anbuchezhian, K. Srinivasan, K. Chandrasekaran, R. Kandasamy, Meccanica (2013) 48:307–321”. Meccanica 52, 1985–1987 (2017). https://doi.org/10.1007/s11012-016-0522-z

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  • DOI: https://doi.org/10.1007/s11012-016-0522-z

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