<?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">WJM</journal-id><journal-title-group><journal-title>World Journal of Mechanics</journal-title></journal-title-group><issn pub-type="epub">2160-049X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjm.2011.16034</article-id><article-id pub-id-type="publisher-id">WJM-9105</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Convection of Radiating Gas in a Vertical Channel through Porous Media
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>rinal</surname><given-names>Jana</given-names></name><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sovan</surname><given-names>Lal Maji</given-names></name></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sanatan</surname><given-names>Das</given-names></name></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rabindranath</surname><given-names>Jana</given-names></name></contrib></contrib-group><author-notes><corresp id="cor1">* E-mail:<email>jana261171@yahoo.co.in(RJ)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>26</day><month>12</month><year>2011</year></pub-date><volume>01</volume><issue>06</issue><fpage>275</fpage><lpage>282</lpage><history><date date-type="received"><day>September</day>	<month>12,</month>	<year>2011</year></date><date date-type="rev-recd"><day>October</day>	<month>10,</month>	<year>2011</year>	</date><date date-type="accepted"><day>October</day>	<month>31,</month>	<year>2011</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 free convection flow of radiating gas between two vertical thermally conducting walls through porous medium in the presence of a uniform gravitational field has been studied. Closed form solutions for the velocity and temperature have been obtained in the optically thin limit case when the wall temperatures are varying linearly with the vertical distance. It is observed that the fluid velocity increases and the temperature difference between the walls and the fluid decreases with an increase in the radiation parameter. It is also observed that both the fluid velocity and temperature in the flow field increase with an increase in the porosity parameter. It is found that the fluid velocity decreases while the temperature increases with an increase in the thermal conductance of the walls. Further, it is found that radiation causes to decrease the rate of heat transfer to the fluid, thereby reducing the effect of natural convection.
 
</p></abstract><kwd-group><kwd>Radiation</kwd><kwd> Porous Medium</kwd><kwd> Heat Transfer and Thermal Conductance</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In recent years, free convection flow of viscous fluids through porous medium has attracted the attention of a number of researchers in view of its wide application to geophysics, astrophysics, meteorology, aerodynamics, boundary layer control and so on. In addition, convective flow through a porous medium has the application in the field of chemical engineering for filtration and purification processes. In petroleum technology, to study the movement of natural gas oil and water through oil channels/reservoirs and in the field of agriculture engineering to study the underground resources, the channel flows through porous medium have numerous engineering and geophysical applications. However, these studies are confined to normal temperatures of the surrounding medium. If the temperature of the 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 effects of radiation and free convection. Channels are frequently used in various applications in designing ventilating and heating of buildings, cooling electronic components, drying several types of agriculture products grain and food, and packed bed thermal storage. Convective flows in channels driven by temperature differences at bounding walls have been studied and reported extensively in literature. Radiative convective flows are frequently encountered in many scientific and environmental processes such as astrophysical flows, water evaporation from open reservoirs, heating and cooling of chambers and solar power technology. Several researchers have investigated convective flow in porous medium such as Nield and Bejan [<xref ref-type="bibr" rid="scirp.9105-ref1">1</xref>], Sparrow and Cess [<xref ref-type="bibr" rid="scirp.9105-ref2">2</xref>], Burmeister [<xref ref-type="bibr" rid="scirp.9105-ref3">3</xref>], Bejan [<xref ref-type="bibr" rid="scirp.9105-ref4">4</xref>], Kaviany [<xref ref-type="bibr" rid="scirp.9105-ref5">5</xref>] and Vafai [<xref ref-type="bibr" rid="scirp.9105-ref6">6</xref>]. Raptis [7,8] has studied the effect of radiation on free convection flow through a porous medium. The natural convection cooling of vertical rectangular channels in air considering radiation and wall conduction has been studied by Hall et al. [<xref ref-type="bibr" rid="scirp.9105-ref9">9</xref>]. Al-Nimr and Haddad [<xref ref-type="bibr" rid="scirp.9105-ref10">10</xref>] have described the fully developed free convection in open-ended vertical channels partially filled with porous material. Thermal dispersion-radiation effects on non-Darcy natural convection in a fluid saturated porous medium have been investigated by Mohammadein and El-Amin [<xref ref-type="bibr" rid="scirp.9105-ref11">11</xref>]. The effect of wall conductances on free convection between asymmetrically heated vertical plates has been studied by Kim et al. [<xref ref-type="bibr" rid="scirp.9105-ref12">12</xref>]. Greif et al. [<xref ref-type="bibr" rid="scirp.9105-ref13">13</xref>] have made an analysis on the laminar convection of a radiating gas in a vertical channel. Effect of wall conductances on convective magnetohydrodynamic channel flow has been investigated by Yu and Yang [<xref ref-type="bibr" rid="scirp.9105-ref14">14</xref>]. Gupta and Gupta [<xref ref-type="bibr" rid="scirp.9105-ref15">15</xref>] have studied the radiation effect on hydromagnetic convection in a vertical channel. Datta and Jana [<xref ref-type="bibr" rid="scirp.9105-ref16">16</xref>] have studied the effect of wall conductances on hydromagnetic convection of a radiation gas in a vertical channel. Makinde and Mhone [<xref ref-type="bibr" rid="scirp.9105-ref17">17</xref>] investigated the effect of thermal radiation on MHD oscillatory flow in a channel filled with saturated porous medium and non-uniform wall temperatures. Narahari [<xref ref-type="bibr" rid="scirp.9105-ref18">18</xref>] has investiagted the effects of thermal radiation and free convection currents on the unsteady Couette flow between two vertical parallel plates with constant heat flux at one boundary.</p><p>In this paper, we have studied the fully developed free convection flow of radiating gas between two vertical thermally conducting walls embedded in porous medium. The governing equations are solved analytically. The effects of the permeability of the porous medium and the influences of radiation parameter and thermal wall conductances on velocity filed and temperature distribution are investigated and analyzed with the help of their graphical representations. It is observed that the fluid velocity <img src="2-490060\39990fea-34a9-4e3b-bbda-9d988a99ee33.jpg" /> increases whereas the temperature distribution <img src="2-490060\5485e4b9-5a9d-456b-ad75-c2525fa520cf.jpg" /> decreases with an increase in the radiation parameter F. It is also observed that both the fluid velocity <img src="2-490060\17cd2e26-9022-4fa7-bdd3-d1da46325d16.jpg" /> and temperature <img src="2-490060\c752b2da-583a-47f0-8f0f-226a9adbb4ff.jpg" /> in the flow field increase with an increase in the porosity parameter<img src="2-490060\426cfbc9-4b7f-4639-91ba-a477e88c4f25.jpg" />. It is found that the fluid velocity decreases while the temperature increases with an increase in the thermal conductance<img src="2-490060\d23fd6c2-44ce-4627-847b-39dcc3d75339.jpg" />. Further, it is found that radiation causes to decrease the rate of heat transport to the fluid thereby reducing the effect of natural convection. The rate of flow increases with an increase in either radiation parameter F or Rayleigh number</p></sec><sec id="s2"><title>2. Formulation of the Problem and Its Solutions</title><p>Consider a fully developed flow of a viscous incompressible fluid flow in a vertical channel embedded in porous medium. The distance between the channel walls is 2L. Employ a Cartesian coordinates system with zaxis vertically upwards along the direction of flow and y-axis perpendicular to it. The origin of the axes is such that the channel walls are at positions <img src="2-490060\a151f1bd-df39-4c0a-abb0-9126b0622cc7.jpg" /> and <img src="2-490060\a8318116-8f65-469f-92ca-65778195407d.jpg" />(see <xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>For the fully developed laminar flow in porous medium, the velocity and the temperature field have only a vertical component and all of the physical variables except temperature and pressure are functions of y. The temperature inside the fluid can be written as</p><disp-formula id="scirp.9105-formula59418"><label>(1)</label><graphic position="anchor" xlink:href="2-490060\8be8245b-2253-4092-981f-bc7420285a21.jpg"  xlink:type="simple"/></disp-formula><p>where N is the vertical temperature gradient.</p><p>On the use of (1), the momentum and energy equations are simplified to the following form</p><disp-formula id="scirp.9105-formula59419"><label>(2)</label><graphic position="anchor" xlink:href="2-490060\ea52259a-6d7f-498e-a178-b33550026fef.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.9105-formula59420"><label>(3)</label><graphic position="anchor" xlink:href="2-490060\aa8c0ce1-82c0-4767-9706-f200b3bce371.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.9105-formula59421"><label>(4)</label><graphic position="anchor" xlink:href="2-490060\602ab2f8-a4af-487c-83ea-e25a55bdd4fc.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="2-490060\40eb72a9-9414-4a86-b1f5-b55b5c61229d.jpg" />, v is the kinematic coefficient of fluid viscosity, g the acceleration due to gravity, k permeability of the porous medium and <img src="2-490060\1e0481b9-662b-45fe-8edd-43b6d66b9b3e.jpg" /> the thermal conductivity.</p><p>In the optically thin limit, the fluid does not absorb its own emitted radiation. This means that there is no selfabsorption but the fluid does absorb radiation emitted by the boundaries. Cogley et al. [<xref ref-type="bibr" rid="scirp.9105-ref19">19</xref>] showed that in the optically thin limit for a non-grey gas near equilibrium, the following relation holds</p><disp-formula id="scirp.9105-formula59422"><label>(5)</label><graphic position="anchor" xlink:href="2-490060\0f72ecad-7941-4ceb-9949-5b17a7cf7485.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="2-490060\8dcd0ff0-cc6a-4f9b-8347-e912285fb1c0.jpg" />, is the absorption coefficient, <img src="2-490060\d026eb83-7181-4c59-b7e3-e13f38a9891b.jpg" />is the Planck function and the subscript w refers to values at the wall. Further simplifications can be made concerning the spectral properties of radiating gases ([<xref ref-type="bibr" rid="scirp.9105-ref20">20</xref>]) but are not necessary for our investigation.</p><p>On the use of (5), Equation (4) becomes</p><disp-formula id="scirp.9105-formula59423"><label>(6)</label><graphic position="anchor" xlink:href="2-490060\c2906b16-2fc9-4196-9efb-41950a6f86fe.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.9105-formula59424"><label>(7)</label><graphic position="anchor" xlink:href="2-490060\85cb3656-a119-4624-bbda-d7825b6dcb01.jpg"  xlink:type="simple"/></disp-formula><p>Subscript “0” indicates that all quantities have been evaluated at the entrance temperature <img src="2-490060\f5ee54d4-dffd-4223-b204-b57f1142f1a7.jpg" /> which is the temperature of the wall at<img src="2-490060\1fdcab0e-3f17-43f9-8794-de6b2504b6c3.jpg" />.</p><p>Integrating Equation (3) we get</p><disp-formula id="scirp.9105-formula59425"><label>(8)</label><graphic position="anchor" xlink:href="2-490060\0887b560-4604-4014-8437-d48aa1bbb0a6.jpg"  xlink:type="simple"/></disp-formula><p>On use of (8), Equation (2) becomes</p><disp-formula id="scirp.9105-formula59426"><label>(9)</label><graphic position="anchor" xlink:href="2-490060\59b533ba-c50a-409b-905d-53d46bb2046d.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.9105-formula59427"><label>(10)</label><graphic position="anchor" xlink:href="2-490060\998e4fff-8066-40f8-8a36-bd3ed128b61c.jpg"  xlink:type="simple"/></disp-formula><p>Introducing the non-dimensional variables</p><disp-formula id="scirp.9105-formula59428"><label>(11)</label><graphic position="anchor" xlink:href="2-490060\aed4653c-f413-4f74-8cd5-96edd1cbe30d.jpg"  xlink:type="simple"/></disp-formula><p>and on using (11), Equations (9) and (6) become</p><disp-formula id="scirp.9105-formula59429"><label>(12)</label><graphic position="anchor" xlink:href="2-490060\145ef180-f117-48a0-b8f7-5fb3313a0ca4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.9105-formula59430"><label>(13)</label><graphic position="anchor" xlink:href="2-490060\31e9cb58-8b51-4848-8c04-88562c887925.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="2-490060\e28908d6-280a-46be-a082-69496dba802d.jpg" /> is the porosity parameter, <img src="2-490060\0d6319c3-1663-499c-bf39-5e69d062bcb5.jpg" /></p><p>is the Rayleigh number and <img src="2-490060\05937476-32b9-47fc-bb73-14f9859d5bd8.jpg" /> is the radiation parameter.</p><p>The dimensionless velocity and the temperature boundary conditions are</p><p><img src="2-490060\3382020f-7bd4-4a48-9635-5cca5e79ab9a.jpg" /></p><disp-formula id="scirp.9105-formula59431"><label>(14)</label><graphic position="anchor" xlink:href="2-490060\03db4005-501f-432f-bb8b-8091a07b21b1.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="2-490060\9fd2a9f3-3e3a-4fc9-bef4-23fb5d0a7ed1.jpg" /> is the thermal conductance ratio.</p><p>Eliminating <img src="2-490060\e33cf688-b7e3-4220-b2ba-23c46c823921.jpg" /> from (12) and (13), we obtain</p><disp-formula id="scirp.9105-formula59432"><label>(15)</label><graphic position="anchor" xlink:href="2-490060\290bf889-6197-4bf7-b437-dac327c267ce.jpg"  xlink:type="simple"/></disp-formula><p>The solution of <img src="2-490060\b2a06f7b-d6e5-496f-84c9-d6e625913f92.jpg" /> satisfying the boundary conditions (14) is easily obtained. Achieving<img src="2-490060\625f488b-478e-488c-8036-40408b05aef0.jpg" />, one can determine <img src="2-490060\171e2573-c5f9-4051-a7e5-74934603f12d.jpg" /> from (12) using the boundary conditions (14).</p><p>The solutions for <img src="2-490060\2a596288-5b76-4c9d-ab4e-c5d6d8362ae4.jpg" /> and <img src="2-490060\d1803f90-cb3f-4c9e-ad5c-89a6974dac59.jpg" /> subject to the boundary conditions (14) are</p><p><img src="2-490060\0c56e65c-a881-4d6c-84a9-61817bd07de8.jpg" />(16)</p><p><img src="2-490060\3a288498-15cf-4ece-af53-14ca4f0fb662.jpg" />(17)</p><p>where</p><p><img src="2-490060\fa6dfce2-9276-4032-9064-74423c288214.jpg" /></p><p><img src="2-490060\21b48d03-a203-4057-959d-0024096f4001.jpg" /></p><p><img src="2-490060\82cebb4d-5643-4b35-b3d2-dbd0062c7d04.jpg" /></p><disp-formula id="scirp.9105-formula59433"><label>(18)</label><graphic position="anchor" xlink:href="2-490060\3d91ebc2-f9e8-4196-b468-0e93b230c5dd.jpg"  xlink:type="simple"/></disp-formula><p><img src="2-490060\e9ce2abe-9dcc-4866-928e-8ea45c2e5880.jpg" /></p><disp-formula id="scirp.9105-formula59434"><label>(19)</label><graphic position="anchor" xlink:href="2-490060\ab04ccd2-b5e1-4a5b-93ea-ff2f5bd9ac09.jpg"  xlink:type="simple"/></disp-formula><p>It is observed from the Equations (16) and (17) that the velocity and temperature depend on the parameters<img src="2-490060\909c59f3-fe4a-4aef-9d66-871e713d882f.jpg" />, F, <img src="2-490060\864665e0-1318-4423-a3d7-da6948a037d4.jpg" />and<img src="2-490060\235878db-054f-4d11-b9fc-74ac8ba78e6c.jpg" />.</p><p>Case-I: Constant wall temperature (<img src="2-490060\536c6e83-b61f-46fd-bbd5-398e2e24b29d.jpg" />).</p><p>The temperature distribution <img src="2-490060\8639a331-3531-4b31-bfa0-f46fb4c65b73.jpg" /> and velocity <img src="2-490060\7cc3a387-086c-4403-8e82-0041ee9fab40.jpg" /> for constant wall temperature are given by</p><disp-formula id="scirp.9105-formula59435"><label>(20)</label><graphic position="anchor" xlink:href="2-490060\664366b4-cd18-4539-94c5-2461de7e1701.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.9105-formula59436"><label>(21)</label><graphic position="anchor" xlink:href="2-490060\96137284-9387-4436-ac21-09688f0e9e48.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="2-490060\885f9e7a-9766-4197-ba2c-43294af4f325.jpg" /> and <img src="2-490060\49e201c8-9db1-48b8-8c1d-d52ae6703123.jpg" /> are given by (19).</p><p>Case-II: Thermally insulated walls (<img src="2-490060\29006469-d4b3-4feb-a282-6eb1dd7e9769.jpg" />).</p><p>The temperature distribution <img src="2-490060\d9db9796-fdbe-4a12-bc5a-1bc849495151.jpg" /> and velocity <img src="2-490060\f8bf5e80-abb1-4f81-a436-e0cbe96e3182.jpg" /> for thermally insulated walls are given by</p><disp-formula id="scirp.9105-formula59437"><label>(22)</label><graphic position="anchor" xlink:href="2-490060\22aa4fb6-894c-4851-b1b8-73a8c665b685.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.9105-formula59438"><label>(23)</label><graphic position="anchor" xlink:href="2-490060\3099d671-6953-41c7-b61e-7a7d82723197.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="2-490060\8c6ab853-90df-4b72-8b20-e15f459ef032.jpg" /> and <img src="2-490060\2c3cb297-c741-4b08-a10e-fd4fafd7e72d.jpg" /> are given by (19).</p></sec><sec id="s3"><title>3. Results and Discussion</title><p>To study the effects of radiation and porosity of the porous medium on the velocity field <img src="2-490060\efeb86fa-d6e2-46d8-b225-4684da3bc91c.jpg" /> and temperature distribution<img src="2-490060\0e51e1f9-5bba-44f5-a39c-133c0311f4e0.jpg" />, we have presented the non-dimensional velocity <img src="2-490060\e9640c56-daca-41da-913b-b6606514708c.jpg" /> and the temperature <img src="2-490060\342e6e61-80d0-4a10-830d-2360fdd10127.jpg" /> against <img src="2-490060\537f8b85-b60f-40a2-a272-7ffc776cea12.jpg" /> for various values of radiation parameter F, Rayleigh number<img src="2-490060\a1c3b668-9acb-4854-87ef-ab4821224499.jpg" />, porosity parameter <img src="2-490060\e6468342-8fd3-4fd8-bf34-6f919fd07839.jpg" /> and the thermal conductance parameter <img src="2-490060\fd70d7c9-dc19-4a24-802c-ecaabb841813.jpg" /> in Figures 2-9. It is observed from <xref ref-type="fig" rid="fig2">Figure 2</xref> that the velocity <img src="2-490060\86e46978-833c-4d6e-a5dc-97a4e82741bf.jpg" /> increases with an increase in radiation parameter F. Increasing the radiation parameter F produces significant increase in the thermal condition of the fluid. This increase in the fluid temperature induces more flow causing the velocity of the fluid there to increase. <xref ref-type="fig" rid="fig3">Figure 3</xref> shows that the velocity at any point in the flow region decreases with an increase in Rayleigh number<img src="2-490060\4c98d999-eaa3-4393-ba5f-acd1860818ed.jpg" />. The Rayleigh number is viewed as the ratio of buoyancy forces and the product of thermal and momentum diffusivities. Increasing value of Rayleigh number opposes the natural convection and hence the fluid velocity decreases. It is observed from <xref ref-type="fig" rid="fig4">Figure 4</xref> that the velocity <img src="2-490060\959b8e34-25f8-4cd1-9665-fb0e3dc4a76b.jpg" /> increases with an increase in porosity parameter<img src="2-490060\cabdbcd1-8cd2-4bf5-a3e3-736abc440397.jpg" />. Porosity is a measure of the void (or empty) spaces in a porous medium and is a fraction of the volume of voids over the total volume. Porosity influences the convection flow and so the fluid velocity increases. It is seen from <xref ref-type="fig" rid="fig5">Figure 5</xref> that the velocity decreases with an</p><p>increase in thermal conductance parameter<img src="2-490060\a22205d4-7f3d-495c-967b-325bef526849.jpg" />. Figures 6 and 7 reveal that the temperature <img src="2-490060\5b3f244c-fd75-4a89-a31a-1655a104a935.jpg" /> decreases with an increase in either radiation parameter F or Rayleigh number<img src="2-490060\6c20b723-c672-43f7-9b49-e8eccab3f85b.jpg" />. Radiation tends to increase the rate of heat transport to the fluid. Thus the effect of radiation reduces the influence of natural convection by causing a reduction in the temperature difference between the fluid and the channel walls. The increase in radiation parameter F means the release of heat energy from the flow region and so the fluid temperature significantly decreases. It is found from Figures 8 and 9 that the temperature <img src="2-490060\5aad2070-d1b0-47fd-8937-33ba6b8f54ad.jpg" /> increases with an increase in either porosity parameter <img src="2-490060\8150f6ee-778a-4dc7-a09b-d39557449966.jpg" /> or thermal conductance parameter<img src="2-490060\750fb665-8227-4a4e-a69a-e50428d4d3a5.jpg" />.</p><p>The non-dimensional shear stress at the right wall <img src="2-490060\c4cb19bd-a01a-4ffc-a4d0-de31f6dec36b.jpg" /> of the channel is given by</p><disp-formula id="scirp.9105-formula59439"><label>(24)</label><graphic position="anchor" xlink:href="2-490060\3c880cfd-ce56-42fa-ba3b-44963ee6c7bb.jpg"  xlink:type="simple"/></disp-formula><p>Numerical values of non-dimensional shear stress <img src="2-490060\879b4b70-45dd-4ed0-9cd7-14d39daf5095.jpg" /> at the right wall <img src="2-490060\1f0558d6-9606-4ca2-939f-8852bf0ffa8b.jpg" /> of the channel are plotted against F for different values of Ra, <img src="2-490060\03a5b63b-519a-4ec0-848d-0b7bdc7a259b.jpg" />and <img src="2-490060\df2939b5-b30c-4ce4-983f-18e495c3443e.jpg" /> in Figures 10-12. It is observed from <xref ref-type="fig" rid="fig1">Figure 1</xref>0 that for fixed values of F the magnitude of the shear stress <img src="2-490060\252b12ff-fbfd-4958-adfd-0b0afca68b16.jpg" /> at the right wall decreases with an increase in Rayleigh number Ra. <xref ref-type="fig" rid="fig1">Figure 1</xref>1 reveals that the magnitude of <img src="2-490060\6710d61c-6c43-4772-8b76-635c55c35205.jpg" /> increases with an increase in porosity parameter<img src="2-490060\9fb6c291-2efe-4c1b-ac2e-d50f50fdb2b5.jpg" />. On the other hand, it is seen from <xref ref-type="fig" rid="fig1">Figure 1</xref>2 that for fixed values of F, the magnitude of <img src="2-490060\78a490c8-3edc-41fc-a9d6-d54c51bd6395.jpg" /> decreases with an decrease in<img src="2-490060\315f917d-396d-4e50-95e7-0b3edbf9490d.jpg" />.</p><p>The rate of heat transfer across the channel’s wall is given as</p><disp-formula id="scirp.9105-formula59440"><label>(25)</label><graphic position="anchor" xlink:href="2-490060\3176ad27-31cd-412b-b8fc-848177e373fd.jpg"  xlink:type="simple"/></disp-formula><p>Numerical values of the rate of heat transfer <img src="2-490060\41a9fd47-4d47-4201-b544-f151a107d036.jpg" /> are shown graphically against F for different values of<img src="2-490060\50d920da-d820-46c2-9ea5-eca4db7d5af4.jpg" />, <img src="2-490060\6f575fdf-adf4-46ed-b067-7e620cad47fa.jpg" />and <img src="2-490060\4d043034-fb9d-4ff3-ae2d-17b37c2e5500.jpg" /> in Figures 13-15. It is observed from <xref ref-type="fig" rid="fig1">Figure 1</xref>3 that for fixed values of F, the rate of heat transfer <img src="2-490060\305b427e-cd62-4772-b54d-7825c89bf713.jpg" /> decreases with an increase in Rayleigh number<img src="2-490060\563a66ca-81dc-4275-acd9-fd3ad58731a2.jpg" />. <xref ref-type="fig" rid="fig1">Figure 1</xref>4 reveals that the <img src="2-490060\9ea8c72f-fc61-476e-8a9f-ac7d418a7ddb.jpg" /> increases with an increase in porosity parameter<img src="2-490060\ed416531-0af0-4516-9ff7-98663c1703b0.jpg" />. On the other hand, it is seen from <xref ref-type="fig" rid="fig1">Figure 1</xref>5 that for fixed values of F, <img src="2-490060\f1216947-6f99-40cb-a424-8f131440cde9.jpg" />decreases with an decrease in<img src="2-490060\86432f22-b1f4-4460-b0ea-a6fe6b8242da.jpg" />.</p><p>The non-dimensional flow rate is given by</p><disp-formula id="scirp.9105-formula59441"><label>(26)</label><graphic position="anchor" xlink:href="2-490060\9fc990f5-1e71-4b1c-ac5f-1850271b79b0.jpg"  xlink:type="simple"/></disp-formula><p>The non-dimensional flow rate, W has been plotted against F for different values of<img src="2-490060\3021e31f-bc7a-471f-8633-8f4ce5364c6f.jpg" />, <img src="2-490060\99866c14-4c38-4f49-adae-2a9346522a79.jpg" />and <img src="2-490060\c493c3b2-973c-424b-b713-33801388611f.jpg" /> in Figures 16 - 18. It is observed from <xref ref-type="fig" rid="fig1">Figure 1</xref>6 that for fixed values of F, the flow rate W decreases with an increase in Rayleigh number<img src="2-490060\38f0be6e-5371-401c-8a56-cc3e85f93f98.jpg" />. <xref ref-type="fig" rid="fig1">Figure 1</xref>7 reveals that flow rate W increases with an increase in porosity parameter<img src="2-490060\cb1e34e2-f854-4e35-ac4c-0ef39d3e35ab.jpg" />. On the other hand, it is seen from <xref ref-type="fig" rid="fig1">Figure 1</xref>8 that for fixed values of F, W decreases with an decrease in<img src="2-490060\5b838421-c6a7-4f11-877c-cc9fd9a5c43a.jpg" />.</p></sec><sec id="s4"><title>4. Conclusions</title><p>The fully developed free convection flow of a radiating gas between two vertical thermally conducting walls embedded in porous medium has been studied. The effects of the permeability of the porous medium and the influences of radiation parameter and thermal wall conductances on velocity and temperature fields are investigated and analyzed with the help of their graphical representa-</p><p>tions. It is observed that the fluid velocity <img src="2-490060\27b88768-f42a-491f-836a-911b8e88f546.jpg" /> increases and the temperature distribution <img src="2-490060\43fefb92-747c-4c6d-b73a-2d4e8c924065.jpg" /> decreases with an increase in the radiation parameter F. It is also observed that both the fluid velocity and temperature in the flow field increase with an increase in the porosity parameter<img src="2-490060\21d5ac84-7dbe-4350-a7fe-861a6f7130df.jpg" />. It is found that the fluid velocity decreases while the temperature increases with an increase in the thermal conductance of the walls<img src="2-490060\a81a767b-1658-4787-bbc6-0845e2bffcae.jpg" />. Further, it is found that radiation causes to decrease the rate of heat transfer to the fluid thereby reducing the effect of natural convection. The rate of flow increases with an increase in either F or Rayleigh number<img src="2-490060\1bc92793-0f67-4e55-9c28-9d4adc38117e.jpg" />.</p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.9105-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">D.A. Nield and A.Bejan, “Convection in Porous Media,” Springer, Berlin, Heidelberg, New York, 1971. </mixed-citation></ref><ref id="scirp.9105-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">E. M. Sparrrow and R. D. Cess, “Radiation Heat Transfer,” Hemispherer Publication Corp., Washington DC, 1978.</mixed-citation></ref><ref id="scirp.9105-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">L. C. Burmeister, “Convective Heat Transfer,” Wiley, New York, 1983.</mixed-citation></ref><ref id="scirp.9105-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">A. Bejan, “Convection Heat Transfer,” Wiley, New York, 1994.</mixed-citation></ref><ref id="scirp.9105-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">M. Kavinay, “Principles of Heat Transfer in porous Me- dia,” Springer-Verlay, New York, 1995.</mixed-citation></ref><ref id="scirp.9105-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">K. Vafai, “Handbook of Porous Media,” 2nd Edition, Taylor and Francis, New York, 2005.  
doi:10.1201/9780415876384</mixed-citation></ref><ref id="scirp.9105-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">A. Raptis, “Radiation and Free Convection Flow through a Porous Medium,” International Communications in Heat and Mass Transfer, Vol. 25, No. 2, 1998, pp. 289- 295. doi:10.1016/S0735-1933(98)00016-5</mixed-citation></ref><ref id="scirp.9105-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">A. Raptis, “Radiation and Flow through a Porous Me- dium,” Journal of Porous Media, Vol. 4, No. 3, 2001, pp. 271-273.</mixed-citation></ref><ref id="scirp.9105-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">D. Hall, G. C. Vliet and T. L. Bergman, “Natural Convec- tion Cooling of Vertical Rectangular Channels in Air Con- sidering Radiation and Wall Conduction,” Journlaof Electronic Packaging, Vol. 121, No. 2, 1999, pp. 75-84.  
doi:10.1115/1.2792671</mixed-citation></ref><ref id="scirp.9105-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">M. A. Al-Nimr and O. H. Haddad, “Fully Developed Free Convection in Open-Ended Vertical Channels Partially Fil- led with Porous Material,” Journal of Porous Media, Vol. 2, No. 2, 1999, pp. 179-189.</mixed-citation></ref><ref id="scirp.9105-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">A. A. Mohammadein and M. F. El-Amin, “Thermal Dis- persion-Radiation Effects on Non-Darcy Natural Convec- tion in a Fluid Saturated Porous Medium,” Transport in Porous Medium, Vol. 40, No. 2, 2000, pp. 153-163.  
doi:10.1023/A:1006654309980</mixed-citation></ref><ref id="scirp.9105-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">S. H. Kim, N. K. Anand and W. Aung, “Effect of Wall Conduction on Free Convection between Asymmetrically Heated Vertical Plates, Uniform Wall Heat Flux,” International Communications in Heat and Mass Transfer, Vol. 33, No. 5, 1990, pp. 1013-1023.  
doi:10.1016/0017-9310(90)90082-6</mixed-citation></ref><ref id="scirp.9105-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">R. Greif, I. S. Habib and J. C. Lin, “Laminar Convection of a Radiating Gas in a Vertical Channel,” Journal of Fluid Mechanics, Vol. 46, No. 3, 1971, pp. 513-520.  
doi:10.1017/S0022112071000673</mixed-citation></ref><ref id="scirp.9105-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">C. P. Yu and K. K. Yang, “Effect of Wall Conductances on Convective Magnetohydrodynamic Channel Flow,” Ap- plied Scietific Research, Vol. 20, No. 1, 1969, pp. 16-23.  
doi:10.1007/BF00382379</mixed-citation></ref><ref id="scirp.9105-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">N. Datta and R. N Jana, “Effect of Wall Conductances on Hydromagnetic Convection of a Radiation Gas in a Ver- tical Channel,” International Communications in Heat and Mass Transfer, Vol. 19, No. 9, 1974, pp. 1015-1019. doi:10.1016/0017-9310(76)90184-8</mixed-citation></ref><ref id="scirp.9105-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">P. S. Gupta and A. S. Gupta, “Radiation Effect on Hydro- magnetic Convection in a Vertical Channel,” International Communications in Heat and Mass Transfer, Vol. 17, No. 12, 1973, pp. 1437-1442.  
doi:10.1016/0017-9310(74)90053-2</mixed-citation></ref><ref id="scirp.9105-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">O. D. Makinde and P. Y. Mhone, “Heat Transfer to MHD Oscillatory Flow in a Channel Filled with Porous Me- dium,” Romanian Journal of Physics, Vol. 50, No. 9-10, 2005, pp. 931-938.</mixed-citation></ref><ref id="scirp.9105-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">M. Narahari, “Effects of Thermal Radiation and Free Con- vection Currents on the Unsteady Couette Flow between Two Vertical Parallel Plates with Constant Heat Flux at One Boundary,” WSEAS Transactions on Heat and Mass Transfer, Vol. 1, No. 5, 2010, pp. 21-30.</mixed-citation></ref><ref id="scirp.9105-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">A. C. Cogley, W. C. Vincenti and S. E. Gilles, “Differen- tial Approximation for Radiative Transfer in a Non-Grey Gas near Equilibrium,” AIAA Journal, Vol. 6, No. 3, 1968, pp. 551-553. doi:10.2514/3.4538</mixed-citation></ref><ref id="scirp.9105-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">C. L. Tien, “Thermal Radiation Properties of Gases,” Advan- ces in Heat Transfer, Vol. 5, 1968, pp. 253-324.</mixed-citation></ref></ref-list></back></article>