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.
Reference
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
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Conflict of interest
The authors declare that they have no conflict of interest.
Rights and permissions
About this article
Cite this article
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
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11012-016-0522-z