<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJFD</journal-id><journal-title-group><journal-title>Open Journal of Fluid Dynamics</journal-title></journal-title-group><issn pub-type="epub">2165-3852</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojfd.2012.24017</article-id><article-id pub-id-type="publisher-id">OJFD-25721</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Dufour Effects on Unsteady Hydromagnetic Radiative Fluid Flow past a Vertical Plate through Porous Medium
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>agdish</surname><given-names>Prakash</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Avula</surname><given-names>Golla Vijaya Kumar</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Desu</surname><given-names>Bhanumathi</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sibyala</surname><given-names>Vijaya Kumar Varma</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff3"><addr-line>Department of Mathematics, S.V. University, Tirupati, India</addr-line></aff><aff id="aff2"><addr-line>Department of Mathematics, Sree Vidyanikethan Engineering College</addr-line></aff><aff id="aff1"><addr-line>Department of Mathematics, University of Botswana, Gaborone, Botswana</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>prakashj@mopipi.ub.bw(AP)</email>;<email>agvijaykumar1729@gmail.com(AGVK)</email>;<email>svijayakumarvarma@yahoo.co.in(SVKV)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>13</day><month>12</month><year>2012</year></pub-date><volume>02</volume><issue>04</issue><fpage>159</fpage><lpage>171</lpage><history><date date-type="received"><day>July</day>	<month>23,</month>	<year>2012</year></date><date date-type="rev-recd"><day>September</day>	<month>1,</month>	<year>2012</year>	</date><date date-type="accepted"><day>September</day>	<month>9,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p><html>
 <head></head>
 
  The objective of the present study is to investigate diffusion-thermo (Dufour effect) and radiation effects on unsteady MHD free convection flow past an impulsively started infinite vertical plate with variable temperature and uniform mass diffusion in the presence of transverse applied magnetic field through porous medium. At time t &gt; 0, the plate is given an impulsive motion with constant velocity 
  <img style="border-bottom:medium none;border-left:medium none;border-top:medium none;border-right:medium none;" src="http://chart.googleapis.com/chart?cht=tx&amp;chl=%5Cmu%20_%7Bo%7D" /> in the vertical upward direction against to the gravitational field. At the same time the plate temperature is raised linearly with time t and the level of concentration near the plate is raised to 
  <img style="border-bottom:medium none;border-left:medium none;border-top:medium none;border-right:medium none;" src="http://chart.googleapis.com/chart?cht=tx&amp;chl=%5Cdot%7BC%7Bw%7D%7D" />. A magnetic field of uniform strength 
  <img style="border-bottom:medium none;border-left:medium none;border-top:medium none;border-right:medium none;" src="http://chart.googleapis.com/chart?cht=tx&amp;chl=B%7Bo%7D" /> is applied normal to the direction to the flow. The dimen- sionless governing equations are solved in closed form by Laplace-transform technique. The effect of flow parameters on velocity, temperature, concentration, the rate of heat transfer and the rate of mass transfer are shown through graphs.
 
</html></p></abstract><kwd-group><kwd>MHD; Heat and Mass Transfer; Diffusion-Thermo (Dufour Number); Vertical Plate; Porous Medium</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In nature, there exist flows which are caused not only by the temperature differences but also the concentration differences. These mass transfer differences do affect the rate of heat transfer. In industries, many transport processes exist in which heat and mass transfer takes place simultaneously as a result of combined buoyancy effect in the presence of thermal radiation. Hence, radiative heat and mass transfer play an important role in manufacturing industries for the design of fins, steel rolling, nuclear power plants, gas turbines and various propulsion device for aircraft, missiles, satellites, combustion and furnace design, materials processing, energy utilization, temperature measurements, remote sensing for astronomy and space exploration, food processing and cryogenic engineering, as well as numerous agricultural, health and military applications. If the temperature of surrounding fluid is rather high, radiation effects play an important role and this situation does exist in space technology. In such cases, one has to take into account the combined effect of thermal radiation and mass diffusion.</p><p>Boundary layer flow on moving horizontal surfaces was studied by Sakiadis [<xref ref-type="bibr" rid="scirp.25721-ref1">1</xref>]. The effects of transversely applied magnetic field on the flow of an electrically conducting fluid past an impulsively started isothermal vertical plate were studied by Soundalgekar et al. [<xref ref-type="bibr" rid="scirp.25721-ref2">2</xref>]. MHD effects on impulsively started vertical infinite plate with variable temperature in the presence of transverse applied magnetic field were studied by Soundalgekar et al. [<xref ref-type="bibr" rid="scirp.25721-ref3">3</xref>]. The dimensionless governing equations were solved using Laplace transform technique. Kumari and Nath [<xref ref-type="bibr" rid="scirp.25721-ref4">4</xref>] studied the development of the asymmetric flow of a viscous electrically conducting fluid in the forward stagnation point of a two-dimensional body and over a stretching surface with an applied magnetic field. The governing equations were solved using Laplace transform technique.</p><p>England and Emery [<xref ref-type="bibr" rid="scirp.25721-ref5">5</xref>] studied the thermal radiation effects of an optically thin gray gas bounded by a stationary vertical plate. Soundalgekar and Takhar [<xref ref-type="bibr" rid="scirp.25721-ref6">6</xref>] considered the radiation free convection flow of an optically thin gray gas past a semi-infinite vertical plate. Radiation effects on mixed convection along isothermal vertical plate were studied by Hossain and Takhar [<xref ref-type="bibr" rid="scirp.25721-ref7">7</xref>]. In all above studies, the stationary vertical plate is considered. Raptis and Perdikis [<xref ref-type="bibr" rid="scirp.25721-ref8">8</xref>] studied the effects of thermal radiation and free convection flow past a moving vertical plate. The governing equations were solved analytically. Das et al. [<xref ref-type="bibr" rid="scirp.25721-ref9">9</xref>] analyzed radiation effects on flow past an impulsively started infinite isothermal vertical plate. The governing equations were solved by the Laplace transform technique. Muthucumaraswamy et al. [<xref ref-type="bibr" rid="scirp.25721-ref10">10</xref>] and Rajesh and Varma [<xref ref-type="bibr" rid="scirp.25721-ref11">11</xref>] studied radiation and mass transfer effects on exponentially accelerated isothermal vertical plate. Recently, Kumar and Varma [<xref ref-type="bibr" rid="scirp.25721-ref12">12</xref>] studied thermal radiation and mass transfer effects on MHD flow past an impulsively started exponentially accelerated vertical plate with variable temperature and mass diffusion.</p><p>Free convection flows that occurs in nature and in engineering practice is very large and has been extensively considered by many authors. When heat and mass transfer occurs simultaneously between the fluxes the driving potentials are more intricate in nature. An energy flux is generated not only by temperature gradients but by composition gradients as well. Temperature gradients can also create mass fluxes and this is the Soret or Thermal-diffusion effect. Generally, the thermal-diffusion and diffusion-thermo effects of smaller order magnitude than the effects prescribed by Fourier’s or Fick’s laws and are often neglected in heat and mass transfer processes. Due to the importance of thermal-diffusion and diffusionthermo effects for the fluids with very light molecular weight as well as medium molecular weight many investtigators have studied and reported results for these flows and the contributors such as Eckert and Drake [<xref ref-type="bibr" rid="scirp.25721-ref13">13</xref>], Dursunkaya and Worek [<xref ref-type="bibr" rid="scirp.25721-ref14">14</xref>], Anghel et al. [<xref ref-type="bibr" rid="scirp.25721-ref15">15</xref>], Postenlnicu [<xref ref-type="bibr" rid="scirp.25721-ref16">16</xref>] are worth mentioning. Alam and Rahman [<xref ref-type="bibr" rid="scirp.25721-ref17">17</xref>] studied the Dufour and soret effects on steady MHD free convective heat and mass transfer flow past a vertical porous plate embedded in a porous medium. Alam et al. [<xref ref-type="bibr" rid="scirp.25721-ref18">18</xref>] investigated the Dufour and Soret effects on unsteady free convection and mass transfer flow past an impulsively started infinite vertical plate embedded in a porous medium under the influence of transverse magnetic field.</p><p>In this paper, it is proposed to study diffusion-thermo and radiation effects on MHD free convection flow past an impulsively started infinite vertical plate with variable temperature through porous medium in the presence of transverse applied magnetic field. The dimensionless governing equations are solved using Laplace transform technique. And the solutions are expressed in terms of exponential and complementary error functions.</p></sec><sec id="s2"><title>2. Mathematical Formulation</title><p>Diffusion-thermo and radiation effects on unsteady MHD free convection of flow of a viscous incompressible, electrically, conducting, radiating fluid past an impulsively started infinite vertical plate with variable temperature and uniform mass diffusion in the presence of transverse applied magnetic field through porous medium have been studied. The <img src="7-2320017\edd20f7b-3eee-434c-b258-9c2a8a91faf6.jpg" />-axis is taken along the plate in vertical upward direction and <img src="7-2320017\fa44730d-59d9-4108-941c-3c7c8946269f.jpg" />-axis is taken normal to it in the direction of applied transverse magnetic field. Initially, it is assumed that the plate and surrounding fluid are at the same temperature and concentration in stationary condition for all the points in entire flow region<img src="7-2320017\49fc60ed-30f4-4795-b32e-c0b8abc3acad.jpg" />. At time<img src="7-2320017\242cc177-622f-4d0c-968b-38f34958e4c9.jpg" />, the plate is given an impulsive motion with constant velocity<img src="7-2320017\11c97d85-45c1-497c-9370-e02e67966d44.jpg" />. At the same time, the plate temperature is raised linearly with time t and the concentration levels near the plate are raised to<img src="7-2320017\d8529409-64aa-4699-9211-d1072a2712b2.jpg" />. A magnetic field of uniform strength <img src="7-2320017\ad4f8f5d-f5db-4754-8b00-7f8fec6f871e.jpg" /> is assumed to be applied normal to the flow. For free convection flow, it is also assumed that1) The induced magnetic field is assumed to be negligible as the magnetic Reynolds number of the flow is taken to be very small.</p><p>2) The viscous dissipation is neglected in the energy equation.</p><p>3) The effects of variation in density <img src="7-2320017\a5764f55-c8f6-40a7-b578-a3a502ee18bc.jpg" />&#160;with temperature and species concentration are considered only on the body force term, in accordance with usual Boussinesq approximation.</p><p>4) The fluid considered here is gray, absorbing/emitting radiation but a non-scattering medium.</p><p>5) Since the flow of the fluid is assumed to be in the direction of <img src="7-2320017\5e227e36-7a96-4726-81e6-26fbf4d3bd87.jpg" />axis, so the physical quantities are functions of the space co-ordinate <img src="7-2320017\31dd3b32-75da-44c8-8864-e6e6318898e9.jpg" /> and <img src="7-2320017\a5d2f0f7-5575-4e73-952d-1a578736d677.jpg" />&#160;only.</p><p>Then by usual Boussinesq’s approximation, the flow is governed by the following equations.</p><disp-formula id="scirp.25721-formula132349"><label>(1)</label><graphic position="anchor" xlink:href="7-2320017\5cfc97a8-8679-445b-9ba3-773f12eb31cc.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132350"><label>(2)</label><graphic position="anchor" xlink:href="7-2320017\5107601c-ba22-4ace-9243-93090e883147.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132351"><label>(3)</label><graphic position="anchor" xlink:href="7-2320017\969185f9-95df-41da-a3fe-81347a4a3292.jpg"  xlink:type="simple"/></disp-formula><p>with the following initial and boundary conditions</p><disp-formula id="scirp.25721-formula132352"><label>(4)</label><graphic position="anchor" xlink:href="7-2320017\66777b0c-aab9-44ec-85ea-c147d54cbf4e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="7-2320017\10c977de-39c8-4146-96de-92661c20d9c1.jpg" /> The local radiant for the case of an optically thin gray gas is expressed by</p><disp-formula id="scirp.25721-formula132353"><label>(5)</label><graphic position="anchor" xlink:href="7-2320017\51181584-64f9-4ec7-993d-c65231df87f7.jpg"  xlink:type="simple"/></disp-formula><p>It is assumed that the temperature differences within the flow are sufficiently small and that <img src="7-2320017\5a92810b-abb6-436d-92d5-d48d1afb2af5.jpg" /> may be expressed as a linear function of the temperature. This is obtained by expanding <img src="7-2320017\b061566a-3065-4871-a874-7fbd7b7736e9.jpg" /> in a Taylor series about <img src="7-2320017\8fe06ed2-d257-45d2-9f4a-690de52a012c.jpg" />and neglecting the higher order terms, thus we get</p><disp-formula id="scirp.25721-formula132354"><label>(6)</label><graphic position="anchor" xlink:href="7-2320017\134a3026-c460-41c3-b859-46322e9dd4ce.jpg"  xlink:type="simple"/></disp-formula><p>From Equations (5) and (6), Equation (2) reduces to</p><disp-formula id="scirp.25721-formula132355"><label>(7)</label><graphic position="anchor" xlink:href="7-2320017\6b1288c8-1d62-43bc-b359-669f592e5a9c.jpg"  xlink:type="simple"/></disp-formula><p>On introducing the following non-dimensional quantities</p><disp-formula id="scirp.25721-formula132356"><label>(8)</label><graphic position="anchor" xlink:href="7-2320017\8d8d400d-6147-4466-a529-7d40791e0a23.jpg"  xlink:type="simple"/></disp-formula><p>We get the following governing equations which are dimensionless</p><disp-formula id="scirp.25721-formula132357"><label>(9)</label><graphic position="anchor" xlink:href="7-2320017\09f6cffa-8dc4-4750-add9-7180785e50ad.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132358"><label>(10)</label><graphic position="anchor" xlink:href="7-2320017\a4a0f3db-a620-469c-be6d-5db83a6310f1.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132359"><label>(11)</label><graphic position="anchor" xlink:href="7-2320017\292927c1-a527-4cc8-b30a-92efb128b9e7.jpg"  xlink:type="simple"/></disp-formula><p>The initial and boundary conditions in dimensionless form are as follows:</p><disp-formula id="scirp.25721-formula132360"><label>(12)</label><graphic position="anchor" xlink:href="7-2320017\8c2b33aa-950f-46d6-8ba5-1a777113cea4.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Solution of the Problem</title><p>The appeared physical parameters are defined in the nomenclature. The dimensionless governing equations from (9) to (11), subject to the boundary conditions (12) are solved by usual Laplace transform technique and the solutions are expressed in terms of exponential and complementary error functions.</p><disp-formula id="scirp.25721-formula132361"><label>(13)</label><graphic position="anchor" xlink:href="7-2320017\7e45ae11-7c2b-452a-b095-151cf12adfd4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132362"><label>(14)</label><graphic position="anchor" xlink:href="7-2320017\f82c9ec2-5699-4887-9afd-2e57f7d54af3.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.25721-formula132363"><label>(15)</label><graphic position="anchor" xlink:href="7-2320017\e43b37bf-44e3-4ece-95c7-22fea0281a2d.jpg"  xlink:type="simple"/></disp-formula><p><img src="7-2320017\610baa56-7e98-4959-b635-7ee3e86b3abf.jpg" />,</p><p><img src="7-2320017\b41bae3f-fdd6-45d1-a3e5-dc027e331c22.jpg" /></p><p><img src="7-2320017\44e8ca2d-c44b-4881-add5-a90bde7e0fbd.jpg" /></p></sec><sec id="s4"><title>4. Nusselt Number</title><p>From temperature field, now we study Nusselt number (rate of change of heat transfer) which is given in nondimensional form as</p><disp-formula id="scirp.25721-formula132364"><label>(16)</label><graphic position="anchor" xlink:href="7-2320017\8c1c2a9c-3dc5-4003-bb4c-363d528093b3.jpg"  xlink:type="simple"/></disp-formula><p>From Equations (14) and (16), we get Nusselt number as follows:</p><p><img src="7-2320017\081fade6-0d98-4010-b7e8-7b8e125270dc.jpg" /></p></sec><sec id="s5"><title>5. Sherwood Number</title><p>From concentration field, now we study Sherwood number (rate of change of mass transfer) which is given in non-dimensional form as</p><disp-formula id="scirp.25721-formula132365"><label>(17)</label><graphic position="anchor" xlink:href="7-2320017\b06761eb-e7e4-433a-b339-9ef298af5e5a.jpg"  xlink:type="simple"/></disp-formula><p>From Equations (13) and (17), we get Sherwood number as follows:</p><p><img src="7-2320017\669e1f6a-1560-40f3-b592-7909327bd06d.jpg" /></p></sec><sec id="s6"><title>6. Results and Discussions</title><p>In order to get a clear insight of the physical problem the velocity, temperature, concentration, the rate of heat transfer and the rate of mass transfer have been discussed by assigning numerical values to the parameters like radiation parameter (R), magnetic parameter (M), Schmidt parameter (Sc), Prandtl number (Pr), Dufour number (Du), thermal Grashof number (Gr), mass Grashof number (Gm) and time t from Figures 1-13 for the cases of cooling (Gr &gt; 0, Gm &gt;0) and heating (Gr &lt; 0, Gm &lt; 0) of plate. The heating and cooling takes place by setting up free convection currents due to temperature and concentration gradient.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> depicts the effect of magnetic field parameter on the fluid velocity and we observed that an increase in magnetic field parameter the velocity decreases in case of cooling of the plate while it increases in case of heating. Figures 2-4 show the effects of R, Du, Gr and Gm on the velocity field u. From these figures, it is observed that the velocity u increases as the radiation parameter R or Dufour number Du or thermal Grashof number Gr or mass Grashof number Gm increases in case of cooling of the plate and a reverse effect is noticed in the case of heating. The velocity profiles for different values of Schmidt number are shown in <xref ref-type="fig" rid="fig5">Figure 5</xref>. From this it is seen that the velocity decreases with increasing values of Schmidt number in the case of cooling of the plate but increases in the case of heating of the plate. <xref ref-type="fig" rid="fig6">Figure 6</xref> reveals the velocity variation with time t for the cases of both cooling and heating. From this we observed that the velocity increases as time t increases for the case of cooling and the trend is just reversed for the case of heating of the plate. The effect of permeability parameter k on the velocity field is shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>. It is seen from this figure that the velocity increases with increase of permeability parameter k in both cases of cooling and heating of the plate.</p><p>The influence of various flow parameters on the fluid temperature are illustrated in Figures 8-10. <xref ref-type="fig" rid="fig8">Figure 8</xref> depicts that the effects of the Dufour number on the fluid temperature. It can be clear seen from this figure that the diffusion thermal effects slightly affect the fluid temperature. As the values of Dufour number increase, the fluid temperature is also increases. The effect of thermal radiation R on the temperature field is illustrated in <xref ref-type="fig" rid="fig9">Figure 9</xref>. It is obvious that the radiation parameter restricts the fluid temperature. Therefore, using radiation we can control the fluid temperature. In <xref ref-type="fig" rid="fig1">Figure 1</xref>0, we depict the</p><p>effects of Prandtl number Pr on the temperature field. It is observed that an increase in the Prandtl number leads to decrease in the fluid temperature. It is due to the fact that thermal conductivity of the fluid decreases with increasing Pr, resulting a decrease in thermal boundary layer thickness.</p><p>The concentration profiles for different values of Schmidt number (Sc) and time t are presented in <xref ref-type="fig" rid="fig1">Figure 1</xref>1. From this figure it is seen that the concentration decreases with increase in Sc while it increases with time t. <xref ref-type="fig" rid="fig1">Figure 1</xref>2 reveals the rate of heat transfer coefficient in terms of Nusselt number for different values of radiation parameter R, Prandtl number Pr and Dufour number Dr respectively. It is observed that Nusselt number increases with increasing values of R or Pr but decreases as Du increases. Finally, from <xref ref-type="fig" rid="fig1">Figure 1</xref>3 it is seen that Sherwood number increases with increase of Sc.</p></sec><sec id="s7"><title>REFERENCES</title></sec><sec id="s8"><title>Nomenclature</title><p><img src="7-2320017\e8cd7f70-2a36-471c-921e-0829d5f2fd77.jpg" />&#160;&#160;&#160; Absorption coefficient</p><p><img src="7-2320017\87dcaff2-cda7-43d6-8534-84f40e96b57e.jpg" />&#160;&#160;&#160; External magnetic field</p><p><img src="7-2320017\3610b545-ca14-414e-89c5-c5a33cf1ed0f.jpg" />&#160;&#160;&#160; Species concentration</p><p><img src="7-2320017\7646fb01-804a-4259-a555-8579d13e29f7.jpg" />&#160;&#160; Concentration of the plate</p><p><img src="7-2320017\df09b747-3d7b-46fe-8b75-0ad60cd53f65.jpg" />&#160;&#160; Concentration of the fluid far away from the plate</p><p><img src="7-2320017\446ba5bb-6fa7-4b4f-9103-fa11d1e0df55.jpg" />&#160;&#160;&#160;&#160;&#160;Dimensionless concentration</p><p><img src="7-2320017\3648e00a-1628-4691-9e5e-bf8662a55b3e.jpg" />&#160;&#160; Specific heat at constant pressure</p><p><img src="7-2320017\7221fe56-58f3-4dc9-8e21-617ac8029fa3.jpg" />&#160;&#160;&#160; Concentration susceptibility</p><p><img src="7-2320017\ebaecf28-e2c2-4f09-a6e6-6441f93b9418.jpg" />&#160;&#160;&#160;&#160; Acceleration due to gravity</p><p><img src="7-2320017\f2cae640-c1d1-4e3b-ac64-075128d01255.jpg" />&#160;&#160;&#160; Thermal Grashof number</p><p><img src="7-2320017\c30b72b2-2f6d-471d-bb6d-8899e12d2b12.jpg" />&#160;&#160; &#160;Mass Grashof number</p><p><img src="7-2320017\06aff5a9-3bb7-45a6-8c90-7830d0b76d53.jpg" />&#160;&#160; &#160;Magnetic field parameter</p><p><img src="7-2320017\cb44a5b6-7c5f-495d-b684-d6ecdc57eae8.jpg" />&#160;&#160;&#160; Nusselt number</p><p><img src="7-2320017\6ad21447-7b62-46e8-84c0-50e139a3f7a8.jpg" />&#160;&#160; &#160; Prandtl number</p><p><img src="7-2320017\bb898b20-14d3-4197-b02d-e9f4932f3582.jpg" />&#160;&#160; &#160; Radiative heat flux in the y-direction</p><p><img src="7-2320017\91af44d7-5018-4abe-8550-c8423ffb9cf5.jpg" />&#160;&#160;&#160; Coefficient of mass diffusivity</p><p><img src="7-2320017\ac89a1ad-1a74-4b9b-ac17-ad85630283ab.jpg" /> &#160;&#160;&#160; Radiative parameter</p><p><img src="7-2320017\e0146c89-ce18-422d-988c-b1ac3ba8d8f6.jpg" />&#160;&#160; &#160; Schmidt number</p><p><img src="7-2320017\8a03c305-904d-4cce-bc3c-2b91cf59e284.jpg" />&#160;&#160;&#160; Temperature of the fluid near the plate</p><p><img src="7-2320017\e26d46c8-2577-4707-a27f-e8eaf98deac7.jpg" />&#160;&#160;&#160; Temperature of the plate</p><p><img src="7-2320017\abe51cba-6509-4e16-8c07-6a1cede893c8.jpg" />&#160;&#160;&#160; Temperature of the fluid far away from the plate</p><p><img src="7-2320017\9fd67375-9d7f-4662-a879-57e9de05b897.jpg" />&#160;&#160;&#160;&#160; Time</p><p><img src="7-2320017\e3072a8c-199a-459c-b655-0ab737c2a4a5.jpg" />&#160; &#160; &#160; Dimensionless time</p><p><img src="7-2320017\544ac332-75b0-4228-b5d8-171e366eecd5.jpg" />&#160;&#160; &#160; Velocity of the fluid in the <img src="7-2320017\9e0fe091-a1a3-42c8-9f44-7c5511041df0.jpg" />-direction</p><p><img src="7-2320017\7ef593e6-2ddb-414d-a9d5-5a8ba72f2174.jpg" />&#160;&#160;&#160; Velocity of the plate</p><p><img src="7-2320017\4b95ae2c-0847-48a4-bc41-e830c02c4d25.jpg" />&#160;&#160;&#160;&#160; Dimensionless velocity</p><p><img src="7-2320017\df353aeb-50fa-427d-b092-84f636e0c49a.jpg" />&#160;&#160;&#160; Co-ordinate axis normal to the plate</p><p><img src="7-2320017\d63c658b-34eb-49e5-8239-89fd207b439a.jpg" />&#160;&#160;&#160; Dimensionless co-ordinate axis normal to the plate</p></sec><sec id="s9"><title>Greek Symbols</title><p><img src="7-2320017\ebe176f1-607e-4a3c-adb5-3c49915a542a.jpg" />&#160;&#160;&#160; Thermal conductivity of the fluid</p><p><img src="7-2320017\c6e00491-cd72-4d32-b031-4fb1695e3e54.jpg" />&#160;&#160; Thermal diffusivity</p><p><img src="7-2320017\f2233594-7aec-4f4a-9d3f-9b8b86b03789.jpg" />&#160;&#160; Volumetric coefficient of thermal expansion</p><p><img src="7-2320017\f9ae9366-c765-4698-885e-5e35adf62ad6.jpg" />&#160; Volumetric coefficient of expansion with concentration</p><p>μ&#160;&#160;&#160;&#160;&#160;&#160;&#160;Coefficient of viscosity</p><p>ν&#160;&#160;&#160;&#160;&#160;&#160;&#160; Kinematic viscosity</p><p>r&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; Density of the fluid</p><p>ρ&#160;&#160;&#160;&#160;&#160;&#160;&#160; Electric conductivity</p><p>σ&#160;&#160;&#160;&#160;&#160;&#160;&#160; Dimensionless temperature</p><p>erf&#160;&#160;&#160;&#160;&#160; Error function</p><p>erfc&#160;&#160;&#160;&#160; Complementary error function</p></sec><sec id="s10"><title>Subscripts</title><p><img src="7-2320017\f57b5f20-221e-4148-997d-e8508fee8ec9.jpg" />&#160;&#160;&#160;&#160; Conditions on the wall</p><p><img src="7-2320017\0e63e3e4-304f-4804-802a-21feddcc495d.jpg" />&#160;&#160;&#160;&#160;&#160; Free stream conditions</p></sec><sec id="s11"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.25721-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">B. C. Sakiadis, “Boundary Layer Behavior on Continuous Solid Surfaces: II. Boundary Layer on a Continuous Solid Flat Surfaces,” AIChE Journal, Vol. 7, No. 2, 1961, pp. 221-225. doi:10.1002/aic.690070211</mixed-citation></ref><ref id="scirp.25721-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">V. M. Soundalgekar, S. K. Gupta and N. S. Birajdar, “Ef- fects of Mass Transfer and Free Convection Currents on MHD Stokes Problem for a Vertical Plate,” Nuclear En- gineering and Design, Vol. 53, No. 3, 1979, pp. 339-346.</mixed-citation></ref><ref id="scirp.25721-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">V. M. Soundalgekar, M. R. Patil and M. D. Jahagirdar, “MHD Stokes Problem for a Vertical Plate with Variable Temperature,” Nuclear Engineering and Design, Vol. 64, No. 1, 1981, pp. 39-42. 
doi:10.1016/0029-5493(81)90030-3</mixed-citation></ref><ref id="scirp.25721-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">M. Kumari and G. Nath, “Development of Two Dimensional Boundary Layer with an Applied Magnetic Field Due to an Impulsive Motion,” Indian Journal of Pure and Applied Mathematics, Vol. 30, No. 7, 1999, pp. 695-708.</mixed-citation></ref><ref id="scirp.25721-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">W. G. England and A. F. Emery, “Thermal Radiation Effects on the Laminar Free Convection Boundary Layer of an Absorbing Gas,” Journal of Heat Transfer, Vol. 91, No. 1, 1969, pp. 37-44. doi:10.1115/1.3580116</mixed-citation></ref><ref id="scirp.25721-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">V. M. Soundalgekar and H. S. Takhar, “Radiation Effects on Free Convection Flow past a Semi-Infinite Vertical Plate,” Modeling, Measurement and Control, Vol. 51, 1993, pp. 31-40.</mixed-citation></ref><ref id="scirp.25721-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">M. A. Hossain and H. S. Takhar, “Radiation Effect on Mixed Convection along a Vertical Plate with Uniform Surface Temperature,” Heat and Mass Transfer, Vol. 31, No. 4, 1996, pp. 243-248. doi:10.1007/BF02328616</mixed-citation></ref><ref id="scirp.25721-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">A. Raptis and C. Perdikis, “Radiation and Free Convection Flow past a Moving Plate,” International Journal of Applied Mechanics and Engineering, Vol. 4, No. 4, 1999, pp. 817-821.</mixed-citation></ref><ref id="scirp.25721-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">U. N. Das, R. K. Deka and V. M. Soundalgekar, “Radiation Effects on Flow past an Impulsively Started Vertical Infinite Plate,” Journal of Theoretical Mechanics, Vol. 1, 1996, pp. 111-115.</mixed-citation></ref><ref id="scirp.25721-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">R. Muthucumaraswamy, K. E. Sathappan, and R. Natarajan, “Mass Transfer Effects on Exponentially Accelerated Isothermal Vertical Plate,” International Journal of Applied Mathematics and Mechanics, Vol. 4, No. 6, 2004, pp. 19-25.</mixed-citation></ref><ref id="scirp.25721-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">V. Rajesh and S. V. K. Varma, “Radiation and Mass Transfer Effects on MHD Free Convection Flow past an Exponentially Accelerated Vertical Plate with Variable Temperature,” ARPN Journal of Engineering and Applied Sciences, Vol. 4, No. 6, 2009, pp. 20-26.</mixed-citation></ref><ref id="scirp.25721-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">A. G. Vijaya Kumar and S. V. K. Varma, “Thermal Radiation and Mass Transfer Effects on MHD Flow past an Impulsively Started Exponentially Accelerated Vertical Plate with Variable Temperature and Mass Diffusion,” Far East Journal of Applied Mathematics, Vol. 55, No. 2 2011, pp. 93-115.</mixed-citation></ref><ref id="scirp.25721-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">E. R. G. Eckert and R. M. Drake, “Analysis of Heat and Mass Transfer,” McGraw-Hill, New York, 1972.</mixed-citation></ref><ref id="scirp.25721-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Z. Dursunkaya and W. M. Worek, “Diffusion-Thermo and Thermal-Diffusion Effects in Transient and Steady Natural Convection from Vertical Surface, International Journal of Heat Mass Transfer, Vol. 35, No. 8, 1992, pp. 2060-2065. doi:10.1016/0017-9310(92)90208-A</mixed-citation></ref><ref id="scirp.25721-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">M. Anghel, H. S. Takhar and I. Pop, “Dufour and Soret Effects on Free Convection Boundary Layer over a Vertical Surface Embedded in a Porous Medium,” Mathematics, Vol. 11, No. 4, 2000, pp. 11-21.</mixed-citation></ref><ref id="scirp.25721-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">A. Postelnicu, “Influence of a Magnetic Field on Heat and Mass Transfer by Natural Convection from Vertical Surfaces in Porous Media Considering Soret and Dofour Effects,” International Journal of Hear and Mass Transfer, 47, No. 6-7, 2004, pp. 1467-1472.</mixed-citation></ref><ref id="scirp.25721-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">M. S. Alam, M. M. Rahman and M. A. Smad, “Dufour and Soret Effects on Unsteady MHD Free Convection and Mass Transfer Flow past a Vertical Porous Plate in a Porous Medium,” Nonlinear Analysis: Modelling and Control, Vol. 11, No. 3, 2005, pp. 217-226.</mixed-citation></ref><ref id="scirp.25721-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">M. S. Alam and M. M. Rahman, “Dufour and Soret Effects on MHD Free Convection Heat and Mass Transfer Flow past a Vertical Flat Plate Embedded in a Porous Medium,” Journal of Navel Architecture and Marine Engineering, Vol. 2, No. 1, 2005, pp. 55-65.</mixed-citation></ref></ref-list></back></article>