<?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">AJCM</journal-id><journal-title-group><journal-title>American Journal of Computational Mathematics</journal-title></journal-title-group><issn pub-type="epub">2161-1203</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ajcm.2016.61001</article-id><article-id pub-id-type="publisher-id">AJCM-63661</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>
 
 
  Effects of Rayleigh Number on MHD Heat Transfer and Fluid Flow in Two-Dimensional Open Square Cavity with Heat Generation
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>heikh</surname><given-names>Anwar Hossain</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mohammad</surname><given-names>Abdul Alim</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Satrajit</surname><given-names>Kumar Saha</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Narail Government Victoria College, Narail, Bangladesh</addr-line></aff><aff id="aff3"><addr-line>Department of Mathematics, Jahangirnagar University, Dhaka, Bangladesh</addr-line></aff><aff id="aff2"><addr-line>Department of Mathematics, Bangladesh University of Engineering &amp;amp; Technology, Dhaka, Bangladesh</addr-line></aff><pub-date pub-type="epub"><day>23</day><month>02</month><year>2016</year></pub-date><volume>06</volume><issue>01</issue><fpage>1</fpage><lpage>16</lpage><history><date date-type="received"><day>1</day>	<month>December</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>20</month>	<year>February</year>	</date><date date-type="accepted"><day>23</day>	<month>February</month>	<year>2016</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>
 
 
  The present work is devoted to investigating heat transfer and fluid flow in a two dimensional square open cavity containing a heated circular cylinder at the centre. A constant heat flux is set at the left sidewall; high and low temperatures are fixed at the bottom and top walls of the cavity respectively. The right side of the cavity is open. Galerkin Weighted Residual Finite Element Analysis is used to visualize the heat transfer and fluid flow solving two-dimensional governing mass, momentum and energy equations for steady state, heat transfer and fluid flow in presence of magnetic field in side an open square cavity. A uniformly heated circular cylinder is placed at the centre of the cavity as a heat source. To find the effects of Rayleigh number (Ra) on the thermal fields and fluid flow in presence of magnetic field and a heated circular cylinder as heat source by visualization and line graphs is the objective of this study. Numerical results are presented in graphical and tabular form. The study is conducted for different values of Rayleigh number, some fixed Hartmann numbers (Ha) and heat flux (q). In the conclusion it has been observed that the temperature 
  field and fluid flow pattern are functions of the parameters Rayleigh number and Hartmann number.
 
</p></abstract><kwd-group><kwd>Natural Convection</kwd><kwd> Rayleigh Number</kwd><kwd> Hartmann Number</kwd><kwd> MHD</kwd><kwd> Heated Cylinder</kwd><kwd> Open Cavity</kwd><kwd> Heat Flux</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The convective heat transfer and the natural convection flow with the presence of magnetic field of the fluid are of great importance in scientific and engineering research, because these types of complicated geometries have applications in engineering and industrial fields. This type of problems of heat transfer attracted very attention of researchers since its numerous uses in the areas of energy conservations, cooling of electrical and electronic equipments, design of solar collectors, heat transfer devices etc. Recently many research work have been done in this field which influence the convection flow nature. It is difficult to solve the natural convection problem in complicated geometry like it. MHD acceleration can use to develop supersonic air craft technology.</p><p>The numerical study on MHD natural convection heat transfer and fluid flow in a two-dimensional square open cavity containing a heated circular cylinder has been done. The left vertical wall is kept at A constant heat flux is set at the left vertical wall, different high and low temperature are set at bottom and top walls of the cavity and remaining side wall is open. Two dimensional Naviar Stoke’s equations with energy equation are used to govern the problem and Galerkin’s Weighted Residual Finite Element Method is used to solve the problem. In the result it is observed that all isotherm lines are concentrated at right lower corner of the cavity and the heat transfer rate is suppressed in suppressed of Rayleigh number in the cavity when Hartmann number is fixed. Recirculations are created in the flow field. Recirculation region is increasing with increasing Rayleigh number (Ra). It is a good agreement with the existing Heat Transfer Theory.</p><p>The terms magneto hydrodynamic, hydrodynamics, magneto gas dynamics and magneto aerodynamics all are the branches of fluid dynamics that deals with the motion of electrically conducting fluids in presence of electric and magnetic fields. The influence of the magnetic field on the boundary layer is exerted only through induced forces within the boundary layer itself, with no additional effects arising from free stream pressure gradient.</p>Literature Review<p>Chan and Tien [<xref ref-type="bibr" rid="scirp.63661-ref1">1</xref>] investigated shallow open cavities and made a comparison study using a square cavity in an enlarged computational domain. They considered a square open cavity having an isothermal vertical side facing the opening and two adjoining adiabatic horizontal sides. They found that satisfactory heat transfer results could be obtained, especially at high Rayleigh numbers. Mohammad [<xref ref-type="bibr" rid="scirp.63661-ref2">2</xref>] studied inclined open square cavities. He considered a restricted computational domain. The rate of change of both velocity components were set to zero at the opening plane which were different from that of Chan and Tien [<xref ref-type="bibr" rid="scirp.63661-ref1">1</xref>] . He found that heat transfer was not sensitive to inclination angle and the flow was unstable at high Rayleigh numbers and small inclination angles.</p><p>Ostrach [<xref ref-type="bibr" rid="scirp.63661-ref3">3</xref>] , Davis [<xref ref-type="bibr" rid="scirp.63661-ref4">4</xref>] , Hossain and Wilson [<xref ref-type="bibr" rid="scirp.63661-ref5">5</xref>] , Hossain et al. [<xref ref-type="bibr" rid="scirp.63661-ref6">6</xref>] and Sarris et al. [<xref ref-type="bibr" rid="scirp.63661-ref7">7</xref>] studied MHD natural convection in a laterally and volumetrically heated square cavity. Their results show that the effect of increasing Hartmann number was not found to be straight forward connected with the resulting flow patterns. Roy and Basak [<xref ref-type="bibr" rid="scirp.63661-ref8">8</xref>] analyzed natural convection flows in a square cavity with non-uniformly heated wall(s). S. Pervin and R. Nasrin [<xref ref-type="bibr" rid="scirp.63661-ref9">9</xref>] , (2011) studied MHD free convection heat transfer for different values of Rayleigh numbers Ra and Hartmann numbers Ha in a rectangular enclosure. They found that the flow pattern and temperature distributions are dependent on the used parameters. Sheikh Anwar Hossain and Alim [<xref ref-type="bibr" rid="scirp.63661-ref10">10</xref>] studied Effects of Natural Convection from an open square cavity containing a heated circular cylinder. S. Saha [<xref ref-type="bibr" rid="scirp.63661-ref11">11</xref>] studied thermo-magnetic convection and heat transfer of paramagnetic fluid in an open square cavity with different boundary conditions. His results show the Effects of Magnetic Rayleigh number, Prandtl number on the flow pattern and isotherm as well as on the heat absorption graphically. He found that the heat transfer rate is suppressed in decreased of the Magnetic Rayleigh number. Hossain, S. A. et al. [<xref ref-type="bibr" rid="scirp.63661-ref12">12</xref>] , (2015) studied MHD free convection heat transfer in an open square cavity containing a heated circular cylinder. In the result they found that heat transfer rate is increased in decreased Hartmann number.</p><p>The study related to heat absorption or rejection in the confined rectangular enclosures has been well discussed in the literature C. Taylor and P. Hood [<xref ref-type="bibr" rid="scirp.63661-ref13">13</xref>] , Chandrasekhar [<xref ref-type="bibr" rid="scirp.63661-ref14">14</xref>] , Dechaumphai [<xref ref-type="bibr" rid="scirp.63661-ref15">15</xref>] . It is observed that comparatively a little work has been done in the case of open square cavities. It might be the difficult on using the boundary conditions at the open side.</p></sec><sec id="s2"><title>2. Two-Dimensional Model</title><p>The two-dimensional diagram of the system considered in the present study is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. The model</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Physical diagram of the problem</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x6.png"/></fig><p>consists of an open square cavity with sides of length L. A heated circular cylinder of diameter D is located at the center of the cavity. The two-dimensional Cartesian co-ordinate system with origin at the lower left corner of the computational domain is considered here. A constant heat flux q is considered at the left vertical wall of the cavity. The bottom wall is kept high temperature T<sub>h</sub> and top wall is kept at low temperature T<sub>c</sub>. The remaining right side wall is open. The temperature at the cylinder T<sub>h</sub><sub>1</sub> is less than that of the bottom wall. A magnetic force of strength B<sub>0</sub> is applied horizontally normal to the side walls.</p></sec><sec id="s3"><title>3. Mathematical Model</title><p>The two-dimensional Naviar-Stoke’s equations together with the energy equation are used to govern the MHD natural convection heat transfer and fluid flow. In this case the flow is considered as steady, laminar, incompressible, two-dimensional and with buoyancy force. To relate the density changes to temperature changes in the fluid properties the Boussinesq approximation is used to here. The following system of differential equations can govern the steady MHD natural convection.</p><disp-formula id="scirp.63661-formula1"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x7.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63661-formula2"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x8.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63661-formula3"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x9.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63661-formula4"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x10.png"  xlink:type="simple"/></disp-formula><sec id="s3_1"><title>3.1. Boundary Conditions</title><p>At Bottom wall: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x12.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x11.png" xlink:type="simple"/></inline-formula>(say); <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x13.png" xlink:type="simple"/></inline-formula></p><p>At Top wall:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x14.png" xlink:type="simple"/></inline-formula>; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x15.png" xlink:type="simple"/></inline-formula></p><p>At the Left wall: u = v = 0, and heat flux q = 150 w/m<sup>2</sup>, 200 w/m<sup>2</sup>, p = 0.</p><p>At the right and open side: Convective Boundary Condition (CBC), pressure p = 0, u = v.</p><p>At the circular cylinder:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x16.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x17.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.63661-formula5"><graphic  xlink:href="http://html.scirp.org/file/1-1100491x18.png"  xlink:type="simple"/></disp-formula><p>In this work x and y denote the distances measured along the bottom and vertical wall respectively from the origin; u and v denote the velocity components in the x and y direction respectively; T represents the temperature in Kelvin scale; g and a denote the kinematic viscosity and the thermal diffusivity respectively; p denotes the pressure and r is the density of the fluid in the cavity.</p></sec><sec id="s3_2"><title>3.2. Governing Equations in Non-Dimensional Form</title><p>The governing equations are nondimensionalized using the following scales.</p></sec><sec id="s3_3"><title>3.3. Non-Dimensional Scales</title><disp-formula id="scirp.63661-formula6"><graphic  xlink:href="http://html.scirp.org/file/1-1100491x19.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63661-formula7"><graphic  xlink:href="http://html.scirp.org/file/1-1100491x20.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3_4"><title>3.4. Non-Dimensional Governing Equations</title><p>Continuity equation:</p><disp-formula id="scirp.63661-formula8"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x21.png"  xlink:type="simple"/></disp-formula><p>Momentum equations:</p><disp-formula id="scirp.63661-formula9"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x22.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63661-formula10"><label>, (7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x23.png"  xlink:type="simple"/></disp-formula><p>Energy equation:</p><disp-formula id="scirp.63661-formula11"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1100491x24.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x25.png" xlink:type="simple"/></inline-formula> is Prandtl number, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x26.png" xlink:type="simple"/></inline-formula>is Rayleigh number and</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x27.png" xlink:type="simple"/></inline-formula>is Hartmann number, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x28.png" xlink:type="simple"/></inline-formula></p></sec><sec id="s3_5"><title>3.5. Boundary Conditions</title><p>At Bottom wall:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x29.png" xlink:type="simple"/></inline-formula>.At Top wall: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x30.png" xlink:type="simple"/></inline-formula></p><p>At the left wall: U = V = 0; Heat Flux q = 125 w/m<sup>2</sup>, 150 w/m<sup>2</sup>, 200 w/m<sup>2</sup>, p = 0</p><p>At the right and open side: Convective Boundary Condition (CBC), p = 0.</p><p>The Nusselt number for natural convection is a function of the Grashof number only. We can obtain the local</p><p>Nusselt number Nu from the temperature field by applying the function<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1100491x31.png" xlink:type="simple"/></inline-formula>.</p><p>The overall or average Nusselt number was calculated by integrating the temperature gradient over the heated wall as follows:</p><disp-formula id="scirp.63661-formula12"><graphic  xlink:href="http://html.scirp.org/file/1-1100491x32.png"  xlink:type="simple"/></disp-formula><p>Here Pr is a nondimensional heat transfer characteristic in the flow field of natural convection. Here Pr = 0.73.</p></sec></sec><sec id="s4"><title>4. Numerical Technique</title><p>The updated version of the software on Finite Element Method as numerical technique based on the Galerkin weighted residual method of finite element method is used in this study. This technique is well described by Tailor and Hood [<xref ref-type="bibr" rid="scirp.63661-ref13">13</xref>] and Dechaumphai [<xref ref-type="bibr" rid="scirp.63661-ref15">15</xref>] . In this case the solution domain is discretized into finite element meshes, which are composed of non-uniform triangular elements. Then the non-dimensional nonlinear governing partial differential equations (i.e. mass, momentum and energy equations) are transferred into a system of integral equations by applying the Galerkin weighted residual technique. To obtain the nonlinear algebraic equations Gauss’s quadrature method is used for integration over each term of these differential equations. Then these obtained nonlinear algebraic equations are modified by setting boundary conditions. Then Newton’s Method is used to transfer the nonlinear algebraic equations into linear algebraic equations. Finally, triangular factorization method is used to solve these linear equations numerically by Finite Element Method. Then numerical solution is converted into graphical solution in terms of isotherms, streamlines and line graphs. To get this results we have defined a program with boundary conditions and values of different parameters in the Finite Element Method. Then run these programs for each set of value. We accept only the convergent solutions. We shifted these graphical results from program to word file and graphical results of line graphs are presented into tabular form.</p></sec><sec id="s5"><title>5. Results and Graphical Discussion</title><p>Computer simulation of Finite Element Method is used to perform the analysis of laminar natural convection heat transfer and fluid flow in an open square cavity with a heated circular cylinder. Effects of various Rayleigh number (Ra) with some fixed Hartmann number (Ha) and Heat flux q are studied on heat transfer and flow inside the cavity by visualizations and line Graphs. The visualizations describe the temperature distributions and flow fields by isotherms and streamlines for different parameters. The values of Ra and Ha in this study vary from 5 &#215; 10<sup>4</sup> to 5 &#215; 10<sup>6</sup> and 25 to 150 respectively while Pr = 0.73 &amp; heat flux q = 125, 150, 200. The results are also presented in the tabular form.</p><p>The flow with all Ra in this work have been affected by the buoyancy force. Figures from <xref ref-type="fig" rid="fig2">Figure 2</xref>(a), <xref ref-type="fig" rid="fig3">Figure 3</xref>(a), <xref ref-type="fig" rid="fig4">Figure 4</xref>(a), <xref ref-type="fig" rid="fig5">Figure 5</xref>(a), <xref ref-type="fig" rid="fig6">Figure 6</xref>(a), <xref ref-type="fig" rid="fig7">Figure 7</xref>(a) and <xref ref-type="fig" rid="fig8">Figure 8</xref>(a) illustrate temperature field in the flow region and in figures from <xref ref-type="fig" rid="fig2">Figure 2</xref>(b), <xref ref-type="fig" rid="fig3">Figure 3</xref>(b), <xref ref-type="fig" rid="fig4">Figure 4</xref>(b), <xref ref-type="fig" rid="fig5">Figure 5</xref>(b), <xref ref-type="fig" rid="fig6">Figure 6</xref>(b), <xref ref-type="fig" rid="fig7">Figure 7</xref>(b) and <xref ref-type="fig" rid="fig8">Figure 8</xref>(b) illustrate streamlines in the flow field. The highest temperature regions remain at the lower half of the open side of the cavity in all figures excepts for Ra = 5 &#215; 10<sup>6</sup> in <xref ref-type="fig" rid="fig7">Figure 7</xref>(a). The isothermal lines are nonlinear for all Ra used in this work and occupied more than right half of the region in the cavity. The all most all isothermal lines are concentrated at the right lower corner of the cavity. The area of isothermal lines and recirculations are increasing with increasing Ra in the same Ha.</p><p><xref ref-type="fig" rid="fig2">Figure 2</xref> Shows the effects of Ra = 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, on isotherms as well as on streamlines for the present configuration at Ha = 75, q = 200. <xref ref-type="fig" rid="fig2">Figure 2</xref>(a) shows the highest temperature remains at the lower part of the cavity. In <xref ref-type="fig" rid="fig2">Figure 2</xref>(b) recirculations are formed around the cylinder. The recirculation region is increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows the effects for Ra = 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup> on isotherms as well as on streamlines for the present configuration at Ha = 25, q = 125. In this case all most all isothermal lines are concentrated at the right lower corner of the cavity. <xref ref-type="fig" rid="fig3">Figure 3</xref>(a) shows the highest temperature at the lower part of the open side. In <xref ref-type="fig" rid="fig3">Figure 3</xref>(b) recirculations are formed around the cylinder and one small vortex is formed above the cylinder in the cavity for Ra = 5 &#215; 10<sup>6</sup>. The recirculations region are increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup>.</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows the effects of Ra = 10<sup>4</sup>, 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup> on isotherms as well as on streamlines for the present configuration at Ha = 25, q = 150. In <xref ref-type="fig" rid="fig4">Figure 4</xref>(b) recirculations are formed around the cylinder at every Ra in the cavity. The recirculations region are increased for Ra = 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>. In <xref ref-type="fig" rid="fig4">Figure 4</xref>(a) all most all the isothermal lines are concentrated at the lower right corner of the cavity.</p><p><xref ref-type="fig" rid="fig5">Figure 5</xref> shows the effects for Ra = 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup> on isotherms as well as on streamlines for the present configuration at Ha = 75, q = 125. In <xref ref-type="fig" rid="fig5">Figure 5</xref>(b) recirculations are formed around the cylinder for every Ra. The recirculations regionare increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup>. The isothermal lines are concentrated at the lower right corner of the cavity. One small vortex is formed above the cylinder for Ra = 5 &#215; 10<sup>6</sup>. <xref ref-type="fig" rid="fig6">Figure 6</xref> shows the effects of Ra = 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup> on isotherms as well as on streamlines for the present configuration at Ha = 100, q = 125. In <xref ref-type="fig" rid="fig6">Figure 6</xref>(b) recirculations are formed around the cylinder at every Ra and one small vortex is formed above the cylinder for Ra = 5 &#215; 10<sup>6</sup>. The recirculations region are increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup>. All most all isothermal lines are concentrated at the lower right corner of the cavity for every</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Streamlines (a) &amp; isotherms (b) for various Ra and Ha = 75, Pr = 0.73, q = 200 in the cavity</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x33.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> (a) Isotherms &amp; (b) streamlines in the cavity for various Ra and Ha = 25, q = 125</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x34.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> (a) Isotherms and (b) streamlines for various Ra while Ha = 25 &amp; heat flux =150</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x35.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> (a) Isotherms and (b) streamlines for various Ra while Ha = 75 &amp; heat flux q =150</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x36.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> (a) Isotherms and (b) streamlines for Ra= 10<sup>5</sup>, …, 5 &#215; 10<sup>6</sup> while Ha = 100 &amp; heat flux q = 125</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x37.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> (a) Isotherms and (b) Streamlines for Ra = 10<sup>5</sup>, … , 5 &#215; 10<sup>6</sup> while Ha =125 &amp; Heat flux =125</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x38.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> (a) Isotherms and (b) streamlines for Ra= 5 &#215; 10<sup>4</sup>, … , 10<sup>6</sup> while Ha =100 &amp; heat flux = 250</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x39.png"/></fig><p>Ra.</p><p><xref ref-type="fig" rid="fig7">Figure 7</xref> shows the effects of Ra = 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup> at Ha = 125 and heat flux q = 125. The isotherm lines are concentrated at right lower corner of the cavity for every Ra and the isotherm lines are located in the right half of the cavity. Here recirculations are formed around the cylinder for every Ha. One small vortex is formed above the cylinder for Ra = 5 &#215; 10<sup>6</sup>. The recirculations region are increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, 5 &#215; 10<sup>6</sup>. The isothermal lines are concentrated at the lower right corner of the cavity for every Ra. Here the highest temperature remains at upper half of the open side for Ra = 5 &#215; 10<sup>6</sup> and Ha = 125.</p><p><xref ref-type="fig" rid="fig8">Figure 8</xref> Show the effects for Ra = 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup> on isotherms as well as on streamlines for the present configuration at Ha = 100, q = 250. Here isotherm lines concentrate at lower right corner of the cavity for every Ra. Here recirculations are formed around the cylinder for every Ra. The recirculation regions are increased for Ra = 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>. <xref ref-type="table" rid="table1">Table 1</xref> shows the amount of heat transferred at the top wall, cylinder and open side of the cavity respectively for various Rayleigh numbers Ra.</p><p>The various Raleigh numbers and magnetic force affect the heat flux along the sides of the cavity. These are observed in figures from <xref ref-type="fig" rid="fig9">Figure 9</xref> and <xref ref-type="fig" rid="fig1">Figure 1</xref>0 that Raleigh number affect on heat flux proportionately. That is heat flux is maximum when Ra is maximum at the top wall and open side. That is if Ra rises then heat flux increases at the open side and upper side of the cavity. But <xref ref-type="fig" rid="fig1">Figure 1</xref>1 shows that the heat transfer at the cylinder is increasing for Ra = 5 &#215; 10<sup>4</sup> to 5 &#215; 10<sup>5</sup> and decreasing for Ra = 10<sup>6</sup> to 5 &#215; 10<sup>6</sup>.</p><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Line graph of heat flux at upper wall for Ra = 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup> &amp; Ha = 80, q = 125</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x40.png"/></fig><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Line graph of heat flux at the open side for Ha = 80, Ra = 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>, 10<sup>6</sup>, q = 125, Pr = 0.73</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x41.png"/></fig><fig id="fig11"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>1</label><caption><title> Line graph of heat flux at the cylinder for Ha = 80, Ra = 5 &#215; 10<sup>4</sup>, 10<sup>5</sup>, 5 &#215; 10<sup>5</sup>,. 5 &#215; 10<sup>6</sup>, q = 125</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1100491x42.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Heat transfer at the top wall, cylinder and open side respectively for various Ra while Ha = 80 and q = 125</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Ra</th><th align="center" valign="middle" >Heat Flux at Top Wall</th><th align="center" valign="middle" >Heat Flux at the Cylinder</th><th align="center" valign="middle" >Heat Flux at Open Side</th></tr></thead><tr><td align="center" valign="middle" >5 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6000</td><td align="center" valign="middle" >28,000</td><td align="center" valign="middle" >200,000</td></tr><tr><td align="center" valign="middle" >10<sup>5</sup></td><td align="center" valign="middle" >9500</td><td align="center" valign="middle" >30,700</td><td align="center" valign="middle" >200,000</td></tr><tr><td align="center" valign="middle" >5 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >35,500</td><td align="center" valign="middle" >42,000</td><td align="center" valign="middle" >220,000</td></tr><tr><td align="center" valign="middle" >10<sup>6</sup></td><td align="center" valign="middle" >60,000</td><td align="center" valign="middle" >40,000</td><td align="center" valign="middle" >320,000</td></tr><tr><td align="center" valign="middle" >5 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >140,000</td><td align="center" valign="middle" >26,500</td><td align="center" valign="middle" >1,100,000</td></tr></tbody></table></table-wrap></sec><sec id="s6"><title>6. Conclusions</title><p>The numerical study on MHD natural convection heat transfer and fluid flow in a two-dimensional square open cavity containing a heated circular cylinder has been done.</p><p>The flow with all Ra in this work has been affected by the buoyancy force. Temperature fields are illustrated in the flow region.</p><p>The high temperature region remains at the lower half of the open side for all Ra except for Ra = 5 &#215; 10<sup>6</sup> in <xref ref-type="fig" rid="fig7">Figure 7</xref>(a).</p><p>The isothermal lines are nonlinear for all Ra used in this work and they occupied more than right half region of the cavity.</p><p>The significant findings of this work are that for all cases of Ha and Ra the isothermal lines concentrated to the right lower corner of the cavity and there are recirculations around the cylinder and one small vortex has been created above the cylinder in the cavity for highest Ra.</p><p>The heat transfer is increasing with increasing Ra at top wall and open side of the cavity.</p><p>The recirculation region is increasing with increasing Ra.</p><p>The result of this work is a good agreement with the existing heat transfer theory.</p></sec><sec id="s7"><title>Cite this paper</title><p>Sheikh AnwarHossain,Mohammad AbdulAlim,Satrajit KumarSaha, (2016) Effects of Rayleigh Number on MHD Heat Transfer and Fluid Flow in Two-Dimensional Open Square Cavity with Heat Generation. American Journal of Computational Mathematics,06,1-16. doi: 10.4236/ajcm.2016.61001</p></sec><sec id="s8"><title>Nomenclature</title></sec></body><back><ref-list><title>References</title><ref id="scirp.63661-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Chan, Y.L. and Tien, C.L. (1985) A Numerical Study of Two-Dimensional Laminar Natural Convection in Shallow Open Cavities. International Journal Heat Mass Transfer, 28, 603-612. http://dx.doi.org/10.1016/0017-9310(85)90182-6</mixed-citation></ref><ref id="scirp.63661-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Mohamad, A. (1995) Natural Convection in Open Cavities and Slots. Numerical Heat Transfer, 27, 705-716. http://dx.doi.org/10.1080/10407789508913727</mixed-citation></ref><ref id="scirp.63661-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Ostrach, S. (1988) Natural Convection in Enclosures. ASME Journal of Heat Transfer, 110, 1175-1190. http://dx.doi.org/10.1115/1.3250619</mixed-citation></ref><ref id="scirp.63661-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Davis, S.H. (1967) Convection in a Box: Linear Theory. Journal of Fluid Machanics, 30, 465-478. http://dx.doi.org/10.1017/S0022112067001545</mixed-citation></ref><ref id="scirp.63661-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Hossain, M.A. and Wilson, M. (2002) Natural Convection Flow in a Fluid-Saturated Porous Medium Enclosed by Non-Isothermal Walls with Heat Generation. International Journal of Thermal Sciences, 41, 447-454. http://dx.doi.org/10.1016/S1290-0729(02)01337-6</mixed-citation></ref><ref id="scirp.63661-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Hossain, M.A., Hafiz, M.S. and Rees, D.A.S. (2005) Buoyancy and Thermocapillary Driven Convection Flow of an Electrically Conducting Fluid in an Enclosure with Heat Generation. International Journal of Thermal Sciences, 44, 676-684. http://dx.doi.org/10.1016/j.ijthermalsci.2004.11.005</mixed-citation></ref><ref id="scirp.63661-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Sarris, I.E., Kakarantzas, S.C., Grecos, A.P. and Vlachos, N.S. (2005) MHD Natural Convection in a Laterally and Volumetrically Heated Square Cavity. International Journal of Heat and Mass Transfer, 48, 3443-3453.</mixed-citation></ref><ref id="scirp.63661-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Roy, S. and Basak, T. (2005) Finite Element Analysis of Natural Convection Flows in a Square Cavity with Non-Uniformly Heated Wall(s). International Journal of Engineering Science, 43, 668-680.  http://dx.doi.org/10.1016/j.ijengsci.2005.01.002</mixed-citation></ref><ref id="scirp.63661-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Parvin, S. and Nasrin, R. (2011) Analysis of the Flow and Heat Transfer Characteristics for MHD Free Convection in an Enclosure with a Heated Obstacle. Nonlinear Analysis, Modeling and Control, 16, 89-99.</mixed-citation></ref><ref id="scirp.63661-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Hossain, S.A. and Alim, M.A. (2012) Effects of Natural Convection from an Open Square Cavity Containing a Heated Circular Cylinder. BJSIR, Dhaka, 47, 19-28.</mixed-citation></ref><ref id="scirp.63661-ref11"><label>11</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Saha</surname><given-names> S. </given-names></name>,<etal>et al</etal>. (<year>2013</year>)<article-title>Effect of MHD and Heat Generation on Natural Convection Flow in an Open Square Cavity under Microgravity Condition</article-title><source> Engineering Computations</source><volume> 30</volume>,<fpage> 5</fpage>-<lpage>20</lpage>.<pub-id pub-id-type="doi"></pub-id></mixed-citation></ref><ref id="scirp.63661-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Hossain, S.A., Alim, M.A. and Saha, S.K. (2015) A Finite Element Analysis on MHD Free Convection Flow in Open Square Cavity Containing Heated Circular Cylinder. American Journal of Computational Mathematics, 5, 41-54. http://dx.doi.org/10.4236/ajcm.2015.51003</mixed-citation></ref><ref id="scirp.63661-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Taylor, C. and Hood, P. Int. J. of Computational Fluids, 1, 73-89.</mixed-citation></ref><ref id="scirp.63661-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Chandrasekhor, S. (1961) Hydrodynamics and Hydromagnetic Stablity. Oxford Clanderon Press, London, 9-79.</mixed-citation></ref><ref id="scirp.63661-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Dechaumphai, P. (1999) Finite Element Method in Engineering. 2nd Edition, Chulalongkorn University Press, Bangkok.</mixed-citation></ref></ref-list></back></article>