<?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.2013.32011</article-id><article-id pub-id-type="publisher-id">OJFD-33643</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>
 
 
  Similarity Solution of the Influence of the Thermal Radiation and Heat Transfer on Steady Compressible Boundary Layer Flow
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>elix</surname><given-names>Ilesanmi Alao</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>Samson</surname><given-names>Babatunde Folarin</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Mathematical Science Department, Federal University of Technology, Akure, Nigeria</addr-line></aff><aff id="aff2"><addr-line>King Fahd University of Petroleum and Mineral, Dhahran, Saudi Arabia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>sanmialao@yahoo.com(SBF)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>06</month><year>2013</year></pub-date><volume>03</volume><issue>02</issue><fpage>82</fpage><lpage>85</lpage><history><date date-type="received"><day>January</day>	<month>25,</month>	<year>2013</year></date><date date-type="rev-recd"><day>February</day>	<month>28,</month>	<year>2013</year>	</date><date date-type="accepted"><day>March</day>	<month>8,</month>	<year>2013</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>
 
 
  This paper determines the influence of the radiation and heat transfer on the compressible boundary layer flow using similarity solutions approach. The Roseland approximation is used to describe the radiative heat flux in the energy equation and the compressible boundary layer equations are transformed using Stewartson transformation. Similarity (invariant) solutions for the governing partial differential equations system are constructed. The shooting method is employed to transform the resulting non-linear boundary value problem into initial value problem, which is solved numerically. The effects of various parameters on the velocity and temperature profiles as well as the Falkner skan exponent and Prandtl number are shown graphically.
   
    
 
</p></abstract><kwd-group><kwd>Radiation; Heat Transfer; Stewartson Transformation; Roseland Approximation</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The analysis of heat transfer through a laminar boundary layer in the flow of a viscous fluid over arbitrary specified surface temperature contributes a very important problem in the field of heat transfer. The prediction of heat transfer under such condition encompasses a wide range of technological applications, such as calculation of heat transfer at the front portion of the projectile, aircraft or other body moving through the atmosphere. Radiative effects have important applications in physics and engineering, and its effects on different flows are very important in space technology and high temperature processes. But very little is known about the effects of radiation on the boundary layer flow. Thermal radiation effects may play an important role in controlling heat transfer in polymer processing industry where the quality of the final product depends on the heat controlling factors to some extent. High temperature plasmas, cooling of nuclear reactors, liquid metal fluids, power generation systems are some important applications of radiative heat transfer from a wall to conductive gray fluids. Although this problem has been successfully studied in the past, to our best knowledge, only little research work has been conducted to investigate the effect of radiation with heat transfer on compressible boundary layer flow. T. C. Chaim [<xref ref-type="bibr" rid="scirp.33643-ref1">1</xref>], discusses the heat transfer in a fluid with variable thermal conductivity over stretching sheet. J. C. Crepeau and R. Clarksean [<xref ref-type="bibr" rid="scirp.33643-ref2">2</xref>], examine the similarity solution of natural convection with internal generation of heat. The effect of radiation on heat transfer problems has been studied by Hossain and Takhar [<xref ref-type="bibr" rid="scirp.33643-ref3">3</xref>]. S. Mukhopadhyay [<xref ref-type="bibr" rid="scirp.33643-ref4">4</xref>], studies the effect of radiation and variable fluid viscosity on flow and heat transfer along a symmetric wedge. The present work deals with the influence of the thermal radiation and heat transfer on steady compressible boundary layer flow.</p></sec><sec id="s2"><title>2. Governing Equations</title><p>We consider a steady, two-dimensional, laminar boundarylayer flow of viscous compressible fluid, given as,</p><disp-formula id="scirp.33643-formula142423"><label>(2.1)</label><graphic position="anchor" xlink:href="8-2320047\a5f84f8d-1dc1-4c7f-9765-1bf2f507c0ea.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142424"><label>(2.2)</label><graphic position="anchor" xlink:href="8-2320047\0ba30651-84b8-4bd0-9ca2-d34232fc833e.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142425"><label>(2.3)</label><graphic position="anchor" xlink:href="8-2320047\aaca0bf6-8caf-438a-9fe0-bc9ef2c3de55.jpg"  xlink:type="simple"/></disp-formula><p>Boundary conditions are:</p><p><img src="8-2320047\0fdcfc11-04d2-4048-825d-749e9ce89055.jpg" />at <img src="8-2320047\5de42c4e-4439-445f-a0e9-73a59b5dfa56.jpg" />&#160;&#160;&#160; &#160;&#160;&#160;&#160;&#160;(2.4)</p><p><img src="8-2320047\7dcd7b01-4a6e-4e62-8aac-cc4603cbd445.jpg" />at <img src="8-2320047\66a5a2ae-0523-4963-aedc-55406e25fa76.jpg" />&#160;&#160;&#160;&#160; &#160;&#160;&#160;&#160;&#160;&#160;(2.5)</p><p>where, <img src="8-2320047\c793737c-497d-4f53-a74b-7ad8478e672d.jpg" />is the constant wall temperature, <img src="8-2320047\b74f571b-45d1-48a8-a277-8600dcca9d67.jpg" />are the Cartesian coordinates with x and y axes along and normal to the surface of the cylinder respectively, <img src="8-2320047\4288a3dc-fc6d-4488-9acb-e116f391c38d.jpg" />are the velocity components along x and y axes, p is the pressure, <img src="8-2320047\5964f2a3-07ff-4cce-8582-7ce21f9bd9ac.jpg" />is the density, k is the thermal conductivity, <img src="8-2320047\1cd93f4d-9521-460c-8b32-1ed260d9b92d.jpg" />is the specific heat at constant pressure, R is the gas constant and the suffix o, refers to some standard state, say<img src="8-2320047\8263311e-112e-455d-938a-0dde3d2e3a6c.jpg" />.</p></sec><sec id="s3"><title>3. Method of Solution</title><p>Stewartson transformation variables of the reduced Equations (2.1)-(2.3) is given as,</p><disp-formula id="scirp.33643-formula142426"><label>(3.1)</label><graphic position="anchor" xlink:href="8-2320047\f5ae83da-50c2-400d-83db-4a00bcfdf3d9.jpg"  xlink:type="simple"/></disp-formula><p>Then,</p><disp-formula id="scirp.33643-formula142427"><label>(3.2)</label><graphic position="anchor" xlink:href="8-2320047\14b2abbe-113b-4abb-a899-416374fbfe64.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142428"><label>(3.3)</label><graphic position="anchor" xlink:href="8-2320047\63610b04-1eb8-4b81-9411-147a3ac8a2e0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142429"><label>(3.4)</label><graphic position="anchor" xlink:href="8-2320047\34899b1b-98dc-49ec-8df0-2674966478b9.jpg"  xlink:type="simple"/></disp-formula><p>see Stewartson [<xref ref-type="bibr" rid="scirp.33643-ref5">5</xref>], with</p><disp-formula id="scirp.33643-formula142430"><label>(3.5)</label><graphic position="anchor" xlink:href="8-2320047\5476277a-f9eb-43ff-b620-64d19514c846.jpg"  xlink:type="simple"/></disp-formula><p>By applying the stewartson transformation variables on Equations (2.1)-(2.6), we obtained</p><disp-formula id="scirp.33643-formula142431"><label>(3.6)</label><graphic position="anchor" xlink:href="8-2320047\6e338ec0-80e9-47d0-b9ba-9a182adad9dd.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142432"><label>(3.7)</label><graphic position="anchor" xlink:href="8-2320047\41d8323d-663d-4d1c-80f8-21854a8d17f8.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="8-2320047\56d00328-b94c-41b5-83ae-06a5b6b2669f.jpg" /> is the stream function, a<sub>1</sub> and a<sub>0</sub> are velocities of sounding main stream.</p><p>The roseland approximation for radiation is given by</p><p><img src="8-2320047\0a61092a-fa0c-481f-9e1a-9ebeab66fcc1.jpg" />(see Mukhopadhyay [<xref ref-type="bibr" rid="scirp.33643-ref4">4</xref>]) <img src="8-2320047\aab93bf2-1e2f-45b7-914b-172b7feb980b.jpg" />is the absorption coefficient and <img src="8-2320047\670bc992-b4dc-483f-a12b-b7f315b118a2.jpg" /> is the Stefan-Boltzman constant. Assuming the temperature within the flow is such that, <img src="8-2320047\69529b8b-1780-4557-8305-231fe087d27f.jpg" />may be expanded in Taylor series about <img src="8-2320047\76193e26-8024-4763-a6c1-bfe8a4e03fce.jpg" />&#160;(free stream temperature) and neglecting the higher orders terms, we have,</p><disp-formula id="scirp.33643-formula142433"><label>(3.8)</label><graphic position="anchor" xlink:href="8-2320047\4849985c-f1d4-462a-9520-0e1cd3e80ae4.jpg"  xlink:type="simple"/></disp-formula><p>replacing <img src="8-2320047\905c0f2b-4052-49a7-abc6-b47ff17731e7.jpg" /> by unity and using roseland approximation on Equations (3.6) and (3.7), gives</p><disp-formula id="scirp.33643-formula142434"><label>(3.9)</label><graphic position="anchor" xlink:href="8-2320047\fac87f99-09bb-4857-8cc4-76e8737af891.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142435"><label>(3.10)</label><graphic position="anchor" xlink:href="8-2320047\8889f471-d017-471d-bbd8-ab685d40a76f.jpg"  xlink:type="simple"/></disp-formula><p>The non dimensionalized form of Equation (3.10) with the transformed boundary conditions using<img src="8-2320047\33340595-1ddb-4c09-a2ee-7b0ff2eca260.jpg" />becomes</p><disp-formula id="scirp.33643-formula142436"><label>(3.11)</label><graphic position="anchor" xlink:href="8-2320047\3f7d3b9a-b59a-4c3c-bf5f-07edfa81a723.jpg"  xlink:type="simple"/></disp-formula><p>With the boundary conditions</p><p><img src="8-2320047\e2d689e2-5a35-49c8-9916-b25e5b4bc953.jpg" />at <img src="8-2320047\c925d4f9-4dea-4181-b0b3-a114b787a7ad.jpg" />&#160; &#160;&#160;&#160;&#160;(3.12)</p><p><img src="8-2320047\7d95641c-ac4e-416e-a7df-82f472433fff.jpg" />at <img src="8-2320047\51c31702-a452-4431-bea4-4002f05dd214.jpg" /> &#160;&#160;(3.13)</p><p>where <img src="8-2320047\eafc7ce2-3288-4427-b1c4-b705c2562b87.jpg" /> (radiative term).</p><p>The similarity variables defined below, are used to transformed Equations (3.9)-(3.13)</p><disp-formula id="scirp.33643-formula142437"><label>(3.14)</label><graphic position="anchor" xlink:href="8-2320047\f3dee76c-39b6-4893-b998-2086e0d55011.jpg"  xlink:type="simple"/></disp-formula><p>The transformations gives the below coupled non linear ordinary differential equations</p><disp-formula id="scirp.33643-formula142438"><label>(3.15)</label><graphic position="anchor" xlink:href="8-2320047\b60e7302-231d-468b-b981-719b1a90fc80.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142439"><label>(3.16)</label><graphic position="anchor" xlink:href="8-2320047\3dd6aa99-6496-4078-a49b-8109da32d595.jpg"  xlink:type="simple"/></disp-formula><p>because of the presence of temperature T, we define the function S relating to the absolute temperature, with Mach number as</p><disp-formula id="scirp.33643-formula142440"><label>(3.17)</label><graphic position="anchor" xlink:href="8-2320047\75355e80-4eb1-455b-906a-e1b1a6e0aac5.jpg"  xlink:type="simple"/></disp-formula><p>where, <img src="8-2320047\06d42310-8eda-49fa-9579-604d89097d31.jpg" />(subsonic flow), <img src="8-2320047\d4a72eb9-84e3-42bd-8d58-6ed852c34683.jpg" />simplifying Equation (3.17) and substituting it into Equations (3.15) and (3.16), we obtained</p><disp-formula id="scirp.33643-formula142441"><label>(3.18)</label><graphic position="anchor" xlink:href="8-2320047\b17ccc31-ff37-4e9e-99b5-60b0a1d8af68.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142442"><label>(3.19)</label><graphic position="anchor" xlink:href="8-2320047\3c9b7f5c-3aa5-43ed-ac0c-f551e4af6d5b.jpg"  xlink:type="simple"/></disp-formula><p>With the boundary conditions,</p><p><img src="8-2320047\b63c259c-6d68-4feb-8581-1df9c73cb10d.jpg" />at <img src="8-2320047\3588a6ad-eff2-4fce-8c63-d3be78ef4863.jpg" />&#160;&#160; (3.20)</p><p><img src="8-2320047\65340ca8-0e0d-4ea8-b15b-1685a73d2032.jpg" />at <img src="8-2320047\64baa700-9a69-4502-abfc-dddf5ed8866a.jpg" />&#160; &#160;&#160;&#160;&#160;&#160;&#160;&#160;(3.21)</p><p>where <img src="8-2320047\f422526c-3eb4-4078-be23-5675d0d2d6cd.jpg" /> and <img src="8-2320047\904eb79f-6c1b-4ed4-a871-cdcb3fc97363.jpg" /></p><p>finally we have Equations (3.18)-(3.21) as</p><disp-formula id="scirp.33643-formula142443"><label>(3.22)</label><graphic position="anchor" xlink:href="8-2320047\3ac51b92-74e6-4553-bc5b-863487545b2a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142444"><label>(3.23)</label><graphic position="anchor" xlink:href="8-2320047\31b5e8c2-df53-4c69-a996-7df87d73cdb1.jpg"  xlink:type="simple"/></disp-formula><p>With boundary conditions,</p><p><img src="8-2320047\abf536dd-209d-4ef4-9d11-c95c8f455591.jpg" />at <img src="8-2320047\207fa05d-7365-4b02-b165-25cc2f9db819.jpg" /> &#160;(3.24)</p><p><img src="8-2320047\ab43eaf2-b7b2-4d58-86d7-20a1493623f8.jpg" />at <img src="8-2320047\1227c25f-a05b-44ba-9f3a-e656f3841c50.jpg" />&#160; &#160;&#160;&#160;&#160;&#160;&#160;&#160;(3.25)</p></sec><sec id="s4"><title>4. Numerical Solution</title><p>Shooting method was employed to transform Equations (3.25)-(3.28) into coupled initial value problems. The approximate solution is constructed using Runge-Kutta fourth order technique. Furthermore, the resulting higher order non-linear coupled differentials are decomposed into systems of first order differential equations given below</p><disp-formula id="scirp.33643-formula142445"><label>(4.1)</label><graphic position="anchor" xlink:href="8-2320047\edb039d2-ac81-43e5-8af8-257a7edd6b7d.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142446"><label>(4.2)</label><graphic position="anchor" xlink:href="8-2320047\34fb4dc8-797b-47f9-9f4d-c533088c45cd.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142447"><label>(4.3)</label><graphic position="anchor" xlink:href="8-2320047\b535be02-e90d-41cb-8ff7-297944d5d8a3.jpg"  xlink:type="simple"/></disp-formula><p>Also</p><disp-formula id="scirp.33643-formula142448"><label>(4.4)</label><graphic position="anchor" xlink:href="8-2320047\b44edea2-3d72-4d76-9c54-749b3f0fa298.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.33643-formula142449"><label>(4.5)</label><graphic position="anchor" xlink:href="8-2320047\6e15e6d4-53bd-4ffe-8eed-905687389ca8.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s5"><title>5. Results</title>Discussion of Results<p>In order to illustrate the results, numerical values were plotted in Figures 1-3). In all cases, we considered the parameters, <img src="8-2320047\a83ef385-e7db-4159-9e6e-9e992b5f7174.jpg" />and<img src="8-2320047\87a2d5da-deaa-4c26-b6d9-47411f7d03df.jpg" />. Others are <img src="8-2320047\3b5e3905-06c3-46b2-8245-002b002fa215.jpg" /> and<img src="8-2320047\6ac6e91d-8128-459b-9ba4-0bee11334386.jpg" />.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> demonstrates the effect of radiative parameter on velocity field, with fixed Falkner skan exponent m, and Prandtl number Pr on both region of the boundary layer flow. It is discovered that, increase in radiation has insignificant effect on the velocity field of the boundary layer. Also, <xref ref-type="fig" rid="fig2">Figure 2</xref> shows the effect of radiation on the velocity field, Radiation has insignificant effect on the fluid flow on the boundary layer.</p><p>Furthermore, <xref ref-type="fig" rid="fig3">Figure 3</xref> shows the effects of the radia-</p><p>tive parameters Q on the temperature field in the presence of some fixed parameter. The temperature <img src="8-2320047\fe749306-edd5-4d18-919b-6f3d69d803b8.jpg" /> decreases as the thermal radiation Q increases. This is in agreement with the physical fact that the thermal boundary layer decreases with increasing Q.</p></sec><sec id="s6"><title>6. Conclusion</title><p>The present study gives the similarity solution with the approximate solution using the shooting method to determine radiative the heat transfer on the boundary layer flow. Our results show that due to radiation, the rate of heat transfer increases. It is found that the effect of thermal radiation is insignificant in the fluid velocity. The flow separation can be controlled in the presence of lower radiation. The temperature of the boundary layer decreases with increasing thermal radiation.</p></sec><sec id="s7"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.33643-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">T. C. Chaim, “Heat Transfer in a Fluid with Variable Thermal Conductivity over Stretching Sheet,” Acta Mechanica, Vol. 129, No. 1-2, 1998, pp. 63-72. 
doi:10.1007/BF01379650</mixed-citation></ref><ref id="scirp.33643-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">J. C. Crepeau and R. Clarksean, “Similarity Solution of Natural Convection with Internal Generation of Heat,” Journal of Heat Transfer, Vol. 119, No. 1, 1997, pp. 183-185. doi:10.1115/1.2824086</mixed-citation></ref><ref id="scirp.33643-ref3"><label>3</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,” International Journal of Heat and Mass Transfer, Vol. 31, No. 4, 1996, pp. 243-248. 
doi:10.1007/BF02328616</mixed-citation></ref><ref id="scirp.33643-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">S. Mukhopadhyay, “Effect of Radiation and Variable Fluid Viscosity on Flow and Heat Transfer along a Symmetric Wedge,” Journal of Applied Fluid Mechanics, Vol. 2, No. 2, 2009, pp. 29-34.</mixed-citation></ref><ref id="scirp.33643-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">K. Stewartson, “Correlated Incompressible and Compressible Boundary Layers,” Proceedings of the Royal Society of London A, Vol. 200, No. 1060, 1949, pp. 84-100.</mixed-citation></ref></ref-list></back></article>