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Radiative heat transfer due to solar radiation in MHD Sisko nanofluid flow
In the present work, the mathematical model for the solar thermal collectors is considered in the form of a nonlinearly stretching sheet. The radiative heat transfer due to solar radiation in magnetohydrodynamic Sisko nanofluid flow over a stretching sheet in the presence of variable thermal conductivity and a heat source is analyzed effectively. The Sisko fluid has been used as a working fluid in the solar collector. The governing boundary value problem is transformed into a system of nonlinear ordinary differential equations using the similarity transformation technique, which is then solved numerically using the finite difference method combined with the quasilinearization technique. The results shown graphically are discussed for the effects of the thermal conductivity parameter, radiation parameter, and heat source parameter on the flow regime. It is observed that increasing values of radiation parameters imply greater thermal conduction and less thermal radiation, as a result of which the nanofluid temperature in the fluid regime will decrease.
Radiative heat transfer due to solar radiation in MHD Sisko nanofluid flow
In the present work, the mathematical model for the solar thermal collectors is considered in the form of a nonlinearly stretching sheet. The radiative heat transfer due to solar radiation in magnetohydrodynamic Sisko nanofluid flow over a stretching sheet in the presence of variable thermal conductivity and a heat source is analyzed effectively. The Sisko fluid has been used as a working fluid in the solar collector. The governing boundary value problem is transformed into a system of nonlinear ordinary differential equations using the similarity transformation technique, which is then solved numerically using the finite difference method combined with the quasilinearization technique. The results shown graphically are discussed for the effects of the thermal conductivity parameter, radiation parameter, and heat source parameter on the flow regime. It is observed that increasing values of radiation parameters imply greater thermal conduction and less thermal radiation, as a result of which the nanofluid temperature in the fluid regime will decrease.
Radiative heat transfer due to solar radiation in MHD Sisko nanofluid flow
Bisht, Ankita (author) / Bisht, Arvind Singh (author)
Heat Transfer ; 51 ; 7411-7434
2022-12-01
24 pages
Article (Journal)
Electronic Resource
English
On three-dimensional boundary layer flow of Sisko nanofluid with magnetic field effects
| British Library Online Contents | 2016
On three-dimensional boundary layer flow of Sisko nanofluid with magnetic field effects
| British Library Online Contents | 2016