Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink
MSc (Mathematics) === Department of Mathematics and Applied Mathematics === The unsteady hydromagnetic chemically reacting mixed convection MHD ow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink is investigated numerically. The original p...
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ndltd-netd.ac.za-oai-union.ndltd.org-univen-oai-univendspace.univen.ac.za-11602-11242020-05-07T03:17:25Z Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink Machaba, Mashudu Innocent Shateyi, Stanford Netshiozwi, N. J. Magnetohydrodynamics (MHD) Chemically reacting Mixed convection Stretching sheet Porous medium Thermal radiation Heat source/sink 538.6 Magnetohydrodynamics Fluid dynamics Dynamo theory (Cosmic physics) Plasma dynamics MSc (Mathematics) Department of Mathematics and Applied Mathematics The unsteady hydromagnetic chemically reacting mixed convection MHD ow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink is investigated numerically. The original partial di erential equations are converted into ordinary di erential equations by using similarity transformation. The governing non-linear partial di erential equations of Momentum, Energy, and Concentration are considered in this study. The e ects of various physical parameters on the velocity, temperature, and species concentration have been discussed. The parameters include the Prandtl number (Pr), Magnetic parameter (M), the Schmidt number (Sc), Unsteady parameter (A), buoyancy forces ratio parameter (N), Chemical reaction (K), Radiation parameter (Nr), Eckert number (Ec), local heat source/sink parameter (Q) and buoyancy parameter due to temperature ( ). The coe cient of Skin friction and Heat transfer are investigated. The coupled non-linear partial di erential equations governing the ow eld have been solved numerically using the Spectral Relaxation Method (SRM). The results that are obtained in this study are then presented in tabular forms and on graphs and the observations are discussed. NRF 2018 2018-06-05T17:21:48Z 2018-06-05T17:21:48Z 2018-05-18 Dissertation http://hdl.handle.net/11602/1124 en University of Venda 1 online resource (ix, 72 leaves : illustrations) |
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Magnetohydrodynamics (MHD) Chemically reacting Mixed convection Stretching sheet Porous medium Thermal radiation Heat source/sink 538.6 Magnetohydrodynamics Fluid dynamics Dynamo theory (Cosmic physics) Plasma dynamics |
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Magnetohydrodynamics (MHD) Chemically reacting Mixed convection Stretching sheet Porous medium Thermal radiation Heat source/sink 538.6 Magnetohydrodynamics Fluid dynamics Dynamo theory (Cosmic physics) Plasma dynamics Machaba, Mashudu Innocent Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
description |
MSc (Mathematics) === Department of Mathematics and Applied Mathematics === The unsteady hydromagnetic chemically reacting mixed convection MHD
ow over a
permeable stretching sheet embedded in a porous medium with thermal radiation and
heat source/sink is investigated numerically. The original partial di erential equations
are converted into ordinary di erential equations by using similarity transformation. The
governing non-linear partial di erential equations of Momentum, Energy, and Concentration
are considered in this study. The e ects of various physical parameters on the
velocity, temperature, and species concentration have been discussed. The parameters
include the Prandtl number (Pr), Magnetic parameter (M), the Schmidt number (Sc),
Unsteady parameter (A), buoyancy forces ratio parameter (N), Chemical reaction (K),
Radiation parameter (Nr), Eckert number (Ec), local heat source/sink parameter (Q)
and buoyancy parameter due to temperature ( ). The coe cient of Skin friction and
Heat transfer are investigated. The coupled non-linear partial di erential equations governing
the
ow eld have been solved numerically using the Spectral Relaxation Method
(SRM). The results that are obtained in this study are then presented in tabular forms
and on graphs and the observations are discussed. === NRF |
author2 |
Shateyi, Stanford |
author_facet |
Shateyi, Stanford Machaba, Mashudu Innocent |
author |
Machaba, Mashudu Innocent |
author_sort |
Machaba, Mashudu Innocent |
title |
Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
title_short |
Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
title_full |
Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
title_fullStr |
Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
title_full_unstemmed |
Unsteady hydromagnetic chemically reacting mixed convection MHD flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
title_sort |
unsteady hydromagnetic chemically reacting mixed convection mhd flow over a permeable stretching sheet embedded in a porous medium with thermal radiation and heat source/sink |
publishDate |
2018 |
url |
http://hdl.handle.net/11602/1124 |
work_keys_str_mv |
AT machabamashuduinnocent unsteadyhydromagneticchemicallyreactingmixedconvectionmhdflowoverapermeablestretchingsheetembeddedinaporousmediumwiththermalradiationandheatsourcesink |
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1719314320608722944 |