Fullydeveloped flow and heat transfer
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Yuwen Zhang (Talk  contribs) (→Fullydeveloped flow and heat transfer in tubes of noncircular cross section) 

(22 intermediate revisions not shown)  
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==Constant Wall Heat Flux==  ==Constant Wall Heat Flux==  
  In this  +  In this article, we consider the case of fully developed laminar flow and constant properties in a circular tube with a fully developed temperature and concentration profiles. We first consider the case of constant heat rate per unit surface area for steady, laminar, fully developed flow. The energy equation in a circular tube, by neglecting axial heat conduction and viscous dissipation terms, is: 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(1)}}  {{EquationRef(1)}}  
}  }  
  For a fully developed flow with constant wall heat flux, eq. (  +  For a fully developed flow with constant wall heat flux, the following relationship (see eq. (18) in [[basics of internal forced convection]]) 
+  <center>  
+  <math>\frac{\partial T}{\partial x}=\frac{dT_{w}}{dx}=\frac{dT_{m}}{dx}</math>  
+  </center>  
+  can be substituted into the eq. (1) to obtain  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(3)}}  {{EquationRef(3)}}  
}  }  
  Integrating eq. (  +  Integrating eq. (2) twice and applying the boundary conditions in eq. (3) to get the temperature distribution gives us 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(4)}}  {{EquationRef(4)}}  
}  }  
+  
Using the definition of mean temperature presented in the last section with the above profile for temperature, and assuming constant properties:  Using the definition of mean temperature presented in the last section with the above profile for temperature, and assuming constant properties:  
<center><math>{{T}_{m}}=\frac{\int_{A}^{{}}{uTdA}}{\int_{A}^{{}}{udA}}=\frac{2\int_{0}^{{{r}_{o}}}{\pi ruTdr}}{\pi r_{o}^{2}{{u}_{m}}}</math></center>  <center><math>{{T}_{m}}=\frac{\int_{A}^{{}}{uTdA}}{\int_{A}^{{}}{udA}}=\frac{2\int_{0}^{{{r}_{o}}}{\pi ruTdr}}{\pi r_{o}^{2}{{u}_{m}}}</math></center>  
  Substituting eq. (  +  Substituting eq. (4) into the above expression yields: 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(5)}}  {{EquationRef(5)}}  
}  }  
  The heat flux at the wall can be obtained using the above relation for  +  The heat flux at the wall can be obtained using the above relation for ''T<sub>m</sub>'' 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(6)}}  {{EquationRef(6)}}  
}  }  
  The heat flux at the wall can also be calculated using eq. (  +  The heat flux at the wall can also be calculated using eq. (4) for the temperature profile and Fourier’s law of heat conduction 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(7)}}  {{EquationRef(7)}}  
}  }  
  Combining eqs. (  +  Combining eqs. (6) and (7) and solving for the heat transfer coefficient, ''h'', yields 
  h = 4.  +  <center><math>\begin{matrix}{} & h=4.364k/D \\\end{matrix}</math> 
+  </center>  
or in terms of the Nusselt number,  or in terms of the Nusselt number,  
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 width="100%" <center>   width="100%" <center>  
  <math>Nu=4.364</math>  +  <math>\begin{matrix}{}\\\end{matrix}Nu=4.364</math> 
</center>  </center>  
{{EquationRef(8)}}  {{EquationRef(8)}}  
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==Constant Surface Temperature==  ==Constant Surface Temperature==  
  We begin with the energy eq. (  +  We begin with the energy equation (eq. (29) in [[basics of internal forced convection]]) 
+  <center>  
+  <math>u\frac{\partial T}{\partial x}=\alpha \left[ \frac{1}{r}\frac{\partial \left( r\partial T/\partial r \right)}{\partial r}+\frac{\partial ^{2}T}{\partial x^{2}} \right]+\frac{\mu }{\rho c_{p}}\left( \frac{\partial u}{\partial r} \right)^{2}</math>  
+  </center>  
+  and neglect the effects of axial heat conduction and viscous dissipation. We already showed that for a fully developed flow and temperature profile with constant surface temperature  
  <math>\frac{\partial T}{\partial x}=\frac{{{T}_{w}}T}{{{T}_{w}}{{T}_{m}}}\frac{d{{T}_{m}}}{dx}</math>  +  <center><math>\frac{\partial T}{\partial x}=\frac{{{T}_{w}}T}{{{T}_{w}}{{T}_{m}}}\frac{d{{T}_{m}}}{dx}</math></center> 
  The energy equation and boundary conditions, using the fully developed velocity profile  +  The energy equation and boundary conditions, using the fully developed velocity profile (equation 24 in [[basics of internal forced convection]]) 
+  <center>  
+  <math>u=2u_{m}\left( 1\frac{r^{2}}{r_{o}^{2}} \right)</math>  
+  </center>  
+  and the above equation, are  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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{{EquationRef(9)}}  {{EquationRef(9)}}  
}  }  
  +  { class="wikitable" border="0"  
+    
+   width="100%" <center>  
<math>\begin{align}  <math>\begin{align}  
& r={{r}_{o}},\quad \quad T={{T}_{w}} \\  & r={{r}_{o}},\quad \quad T={{T}_{w}} \\  
& r=0,\quad \quad \frac{\partial T}{\partial r}=0\quad \text{or}\quad T=\text{finite} \\  & r=0,\quad \quad \frac{\partial T}{\partial r}=0\quad \text{or}\quad T=\text{finite} \\  
\end{align}</math>  \end{align}</math>  
  +  </center>  
  The above equation and boundary conditions have been solved by various techniques in literatures, including separation of variables and infinite series. For additional detailed information the reader should refer to Burmeister  +  {{EquationRef(10)}} 
  The solution for eqs. (  +  } 
+  
+  The above equation and boundary conditions have been solved by various techniques in literatures, including separation of variables and infinite series. For additional detailed information the reader should refer to <ref name="B1993">Burmeister, L.C., 1993, Convective Heat Transfer, 2nd ed., John Wiley & Sons, Hoboken, NJ.</ref><ref>Faghri, A., Zhang, Y., and Howell, J. R., 2010, Advanced Heat and Mass Transfer, Global Digital Press, Columbia, MO.</ref><ref name="K1987">Kakaç, S., Shah, R., Aung, W., 1987, Handbook of SinglePhase Convective Heat Transfer, John Wiley, New York.</ref><ref name="K2005">Kays, W.M., Crawford, M.E., and Weigand, B., 2005, Convective Heat Transfer, 4th ed., McGrawHill, New York, NY</ref><ref name="B2004">Bejan, A., 2004, Convection Heat Transfer, 3rd ed., John Wiley & Sons, Hoboken, NJ. </ref>.  
+  
+  The solution for eqs. (9) and (10) in the form of an infinite series for the temperature and Nusselt number is <ref name="K1987"/>:  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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<math>\frac{T{{T}_{w}}}{{{T}_{in}}{{T}_{w}}}=\sum\limits_{m=0}^{\infty }{{{C}_{2m}}{{\left( \frac{r}{{{r}_{o}}} \right)}^{2m}}}</math>  <math>\frac{T{{T}_{w}}}{{{T}_{in}}{{T}_{w}}}=\sum\limits_{m=0}^{\infty }{{{C}_{2m}}{{\left( \frac{r}{{{r}_{o}}} \right)}^{2m}}}</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(11)}} 
}  }  
where  where  
  <math>\begin{align}  +  <center><math>\begin{align} 
& {{c}_{o}}=1,\quad \quad {{c}_{2}}=\frac{1}{4}\lambda _{0}^{2}=1.828397,\quad \quad {{c}_{2m}}=\frac{\lambda _{0}^{2}}{{{\left( 2m \right)}^{2}}}\left( {{c}_{2m4}}{{c}_{2m2}} \right) \\  & {{c}_{o}}=1,\quad \quad {{c}_{2}}=\frac{1}{4}\lambda _{0}^{2}=1.828397,\quad \quad {{c}_{2m}}=\frac{\lambda _{0}^{2}}{{{\left( 2m \right)}^{2}}}\left( {{c}_{2m4}}{{c}_{2m2}} \right) \\  
& {{\lambda }_{0}}=2.704364 \\  & {{\lambda }_{0}}=2.704364 \\  
  \end{align}</math>  +  \end{align}</math></center> 
The Nusselt number corresponding to the above temperature distribution is  The Nusselt number corresponding to the above temperature distribution is  
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<math>\text{Nu}=\frac{1}{2}{{\lambda }^{2}}=3.657</math>  <math>\text{Nu}=\frac{1}{2}{{\lambda }^{2}}=3.657</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(12)}} 
}  }  
+  
The temperature slope for constant wall heat flux at the wall is higher than the temperature slope for constant surface temperature. This effect has resulted in a 16 percent increase in Nusselt number for constant wall flux versus constant wall temperature for a fully developed flow and temperature profile.  The temperature slope for constant wall heat flux at the wall is higher than the temperature slope for constant surface temperature. This effect has resulted in a 16 percent increase in Nusselt number for constant wall flux versus constant wall temperature for a fully developed flow and temperature profile.  
The two cases of constant wall temperature and constant wall heat flux are special cases of a more general exponential heat flux boundary condition:  The two cases of constant wall temperature and constant wall heat flux are special cases of a more general exponential heat flux boundary condition:  
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<math>{{{q}''}_{w}}=A\exp \left( \frac{1}{2}n{{x}^{+}} \right)</math>  <math>{{{q}''}_{w}}=A\exp \left( \frac{1}{2}n{{x}^{+}} \right)</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(13)}} 
}  }  
  where ''A'' and ''n'' are both constants and n can be assumed to be either a positive or negative value, and  +  where ''A'' and ''n'' are both constants and ''n'' can be assumed to be either a positive or negative value, and 
  <math>{{x}^{+}}=\frac{x/{{r}_{o}}}{\operatorname{Re}\Pr }.</math>  +  <math>{{x}^{+}}=\frac{x/{{r}_{o}}}{\operatorname{Re}\Pr }.</math> ''n'' = 0 corresponds to constant heat flux at the wall and ''n'' = –14.63 corresponds to constant wall temperature. 
  n = 0 corresponds to constant heat flux at the wall and n = –14.63 corresponds to constant wall temperature.  +  
  Shah and London  +  Shah and London <ref name="SL1978">Shah, R. K.; London, A. L., 1978, “Laminar Flow Convection in Ducts,” Advances in Heat Transfer, Supplement 1, Irvine, T. F. and Harnett, J.P., Eds., Academic Press, San Diego, CA.</ref> developed the following correlation, which fits the exact solution of eq. (13) within 3 percent for –51.36 < ''n'' < 100. 
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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<math>\begin{align}& Nu=4.3573+0.0424n2.8368\times {{10}^{4}}{{n}^{2}}+3.6250\times {{10}^{6}}{{n}^{3}} \\ & 7.6497\times {{10}^{8}}{{n}^{4}}+9.1222\times {{10}^{10}}{{n}^{5}}3.8446\times {{10}^{12}}{{n}^{6}} \\ \end{align}</math>  <math>\begin{align}& Nu=4.3573+0.0424n2.8368\times {{10}^{4}}{{n}^{2}}+3.6250\times {{10}^{6}}{{n}^{3}} \\ & 7.6497\times {{10}^{8}}{{n}^{4}}+9.1222\times {{10}^{10}}{{n}^{5}}3.8446\times {{10}^{12}}{{n}^{6}} \\ \end{align}</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(14)}} 
}  }  
==Fullydeveloped fluid flow and heat transfer in an annulus==  ==Fullydeveloped fluid flow and heat transfer in an annulus==  
  +  [[Image:Fig5.6.jpgthumb400 pxalt=v Flow and heat transfer in an annulus.]]  
  +  
  [[Image:Fig5.6.jpgthumb400 pxalt=v   +  
+  The problem of fluid flow and heat transfer in an annulus (see figure to the right) is also of considerable interest in various applications, including heat exchangers and heat pipes, due to an increase and flexibility in the heating and cooling of surface area.  
+  
+  We present the result below for the case in which both the inner wall (radius ''r<sub>i</sub>'') and outer wall (radius ''r<sub>o</sub>'') are kept at a constant heat flux for various values of ''K'' = ''r<sub>i</sub>''/''r<sub>o</sub>''. ''K'' = 0 corresponds to conventional circular tubes, and ''K'' =1 corresponds to flow between two parallel planes.  
The momentum and energy equations, as well as the boundary conditions for steady, laminar, fully developed flow and temperature profile, by neglecting radial conduction of the wall, axial heat conduction in the fluid, and viscous dissipation, and assuming constant properties, are  The momentum and energy equations, as well as the boundary conditions for steady, laminar, fully developed flow and temperature profile, by neglecting radial conduction of the wall, axial heat conduction in the fluid, and viscous dissipation, and assuming constant properties, are  
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<math>\frac{dp}{dx}=\frac{\mu }{r}\frac{d}{dr}\left( r\frac{du}{dr} \right)</math>  <math>\frac{dp}{dx}=\frac{\mu }{r}\frac{d}{dr}\left( r\frac{du}{dr} \right)</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(15)}} 
}  }  
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<math>u\frac{d{{T}_{m}}}{dx}=\alpha \left[ \frac{1}{r}\left( \frac{\partial }{\partial r}\frac{\partial T}{\partial r} \right) \right]</math>  <math>u\frac{d{{T}_{m}}}{dx}=\alpha \left[ \frac{1}{r}\left( \frac{\partial }{\partial r}\frac{\partial T}{\partial r} \right) \right]</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(16)}} 
}  }  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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<math>r={{r}_{i}},\quad \quad u=0,\quad \quad k{{\left. \frac{\partial T}{\partial r} \right}_{r={{r}_{i}}}}={{q}_{i}}^{\prime \prime }</math>  <math>r={{r}_{i}},\quad \quad u=0,\quad \quad k{{\left. \frac{\partial T}{\partial r} \right}_{r={{r}_{i}}}}={{q}_{i}}^{\prime \prime }</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(17)}} 
}  }  
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<math>r={{r}_{o}},\quad \quad u=0,\quad \quad k{{\left. \frac{\partial T}{\partial r} \right}_{r={{r}_{o}}}}={{q}_{o}}^{\prime \prime }</math>  <math>r={{r}_{o}},\quad \quad u=0,\quad \quad k{{\left. \frac{\partial T}{\partial r} \right}_{r={{r}_{o}}}}={{q}_{o}}^{\prime \prime }</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(18)}} 
}  }  
where<math>{{q}_{i}}^{\prime \prime }</math>and<math>{{q}_{o}}^{\prime \prime }</math>are the inner and outer wall heat fluxes, respectively.  where<math>{{q}_{i}}^{\prime \prime }</math>and<math>{{q}_{o}}^{\prime \prime }</math>are the inner and outer wall heat fluxes, respectively.  
  The velocity profile can be obtained by integrating eq. (  +  
+  The velocity profile can be obtained by integrating eq. (15) twice and applying no slip boundary conditions at both the inner and outer walls.  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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<math>\frac{u}{{{u}_{m}}}=\frac{2}{A}\left[ 1{{\left( \frac{r}{{{r}_{o}}} \right)}^{2}}+B\ln \frac{r}{{{r}_{o}}} \right]</math>  <math>\frac{u}{{{u}_{m}}}=\frac{2}{A}\left[ 1{{\left( \frac{r}{{{r}_{o}}} \right)}^{2}}+B\ln \frac{r}{{{r}_{o}}} \right]</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(19)}} 
}  }  
where  where  
  <math>A=1+{{K}^{2}}B,\quad \quad B=\frac{{{K}^{2}}1}{\ln K},\quad \quad {{u}_{m}}=\frac{\int_{{{r}_{i}}}^{{{r}_{o}}}{urdr}}{\left( {{r}_{o}}^{2}{{r}_{i}}^{2} \right)}</math>  +  <center><math>A=1+{{K}^{2}}B,\quad \quad B=\frac{{{K}^{2}}1}{\ln K},\quad \quad {{u}_{m}}=\frac{\int_{{{r}_{i}}}^{{{r}_{o}}}{urdr}}{\left( {{r}_{o}}^{2}{{r}_{i}}^{2} \right)}</math></center> 
The local heat transfer coefficients and Nusselt numbers are  The local heat transfer coefficients and Nusselt numbers are  
  <math>\begin{align}  +  <center><math>\begin{align} 
& {{h}_{i}}=\frac{{{q}_{i}}^{\prime \prime }}{{{T}_{i}}{{T}_{m}}},\text{ }{{h}_{o}}=\frac{{{q}_{o}}^{\prime \prime }}{{{T}_{o}}{{T}_{m}}} \\  & {{h}_{i}}=\frac{{{q}_{i}}^{\prime \prime }}{{{T}_{i}}{{T}_{m}}},\text{ }{{h}_{o}}=\frac{{{q}_{o}}^{\prime \prime }}{{{T}_{o}}{{T}_{m}}} \\  
& N{{u}_{i}}=\frac{{{h}_{i}}{{D}_{h}}}{k},\text{ }N{{u}_{o}}=\frac{{{h}_{o}}{{D}_{h}}}{k} \\  & N{{u}_{i}}=\frac{{{h}_{i}}{{D}_{h}}}{k},\text{ }N{{u}_{o}}=\frac{{{h}_{o}}{{D}_{h}}}{k} \\  
  \end{align}</math>  +  \end{align}</math></center> 
+  
+  where the hydraulic diameter, ''D<sub>h</sub>'' = 2(''r<sub>o</sub>'' – ''r<sub>i</sub>'').  
+  
+  The energy equation can also be solved using the velocity profile given by eq. (17) in a similar manner as presented for a circular tube, except that it can involve lengthy algebra.  
+  Since the energy equation is linear and homogeneous, the principle of superposition was used to obtain the solution of the above problem as a sum of two problems. One problem is the outer wall heated uniformly and the inner wall insulated. The second problem is the inner wall heated uniformly and the outer wall insulated. The principle of superposition can be applied to linear homogeneous differential equations as long as the summation of the governing equations and boundary conditions for each subset problem will add to the original problem. Kakaç and Yucel <ref name="KY1974">Kakaç, S., and Yucel, O., 1974, Laminar Flow Heat Transfer in an Annulus with Simultaneous Development of Velocity and Temperature Fields, Technical and Scientific Council of Turkey, TUBITAK, ISITEK No. 19, Ankara, Turkey. </ref> performed a numerical solution for fully developed velocity and temperature profile. The following table shows the inner and outer wall Nusselt number for various ''K'' values obtained by Kakaç and Yucel <ref name="KY1974"/>.  
  +  The inner and outer wall Nusselt numbers, based on the average wall heat flux ratio, can be calculated from the results in the following table using the following equations:  
  +  
  +  
  The inner and outer wall Nusselt numbers, based on the average wall heat flux ratio, can be calculated from the results in  +  
{ class="wikitable" border="0"  { class="wikitable" border="0"  
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<math>N{{u}_{i}}=\frac{N{{u}_{ii}}}{1\left( {{{{q}''}}_{o}}/{{{{q}''}}_{i}} \right){{\theta }_{i}}^{*}}</math>  <math>N{{u}_{i}}=\frac{N{{u}_{ii}}}{1\left( {{{{q}''}}_{o}}/{{{{q}''}}_{i}} \right){{\theta }_{i}}^{*}}</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(20)}} 
}  }  
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<math>N{{u}_{o}}=\frac{N{{u}_{oo}}}{1\left( {{{{q}''}}_{i}}/{{{{q}''}}_{o}} \right){{\theta }_{o}}^{*}}</math>  <math>N{{u}_{o}}=\frac{N{{u}_{oo}}}{1\left( {{{{q}''}}_{i}}/{{{{q}''}}_{o}} \right){{\theta }_{o}}^{*}}</math>  
</center>  </center>  
  {{EquationRef(  +  {{EquationRef(21)}} 
}  }  
  where  +  where ''Nu<sub>ii</sub>'' is defined as the inner wall Nusselt number when the inner tube is heated and outer wall is insulated. Similarly, Nu<sub>oo</sub> is the outer tube Nusselt number when the outer wall is heated and inner tube is insulated. 
  <math>\theta _{i}^{*}</math>and<math>\theta _{o}^{*}</math>are defined as influence coefficients and are a function of K only for laminar flow.  +  <math>\theta _{i}^{*}</math>and<math>\theta _{o}^{*}</math>are defined as influence coefficients and are a function of ''K'' only for laminar flow. 
+  
<center>  <center>  
<div style="display:inline;">  <div style="display:inline;">  
  '''Table  +  '''Table''' Nusselt number for fully developed flow and temperature profile with constant wall heat flux in an annulus, ''K'' = ''r<sub>i</sub>'' /''r<sub>o</sub>'' 
{ class="wikitable" border="1"  { class="wikitable" border="1"  
 align="center" style="background:#f0f0f0;" width="10%"  ''K''   align="center" style="background:#f0f0f0;" width="10%"  ''K''  
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</div></center>  </div></center>  
+  ==Fullydeveloped flow and heat transfer in tubes of noncircular cross section==  
+  The fluid and heat transfer solution for tubes of noncircular cross section with a fully developed flow and temperature profile can be obtained by solving the energy equation for the particular geometry. The results for some of the more conventional geometries obtained by Shah and London <ref name="shah1974">Shah, R. K.; London, A. L., 1974, “Thermal Boundary Conditions and Some Solutions for Laminar Duct Flow Forced Convection,” ASME J. Heat Transfer Vol. 96, pp. 159165.</ref> are presented in the following table. There are three different boundary conditions in this table; “H1” which refers to the circumferentially constant wall temperature and the axial constant wall heat flux boundary condition, “H2” is for both axially and circumferentially constant heat flux at the wall, and “T” represents a constant wall temperature boundary condition. For the case of a symmetrically heated straight duct having no corners and a constant peripheral curvature, e.g. parallel planes and circular pipe, H<sub>1</sub> and H<sub>2</sub> boundary conditions are the same.  
+  <center>'''Table''' Solutions for Nusselt Number and Friction Coefficient for fully developed laminar flow and temperature profile for various geometries</center>  
+  [[Image:table5.2.jpgthumbcenter800pxalt=Solutions for Nusselt Number and Friction Coefficient for fully developed laminar flow and temperature profile for various geometries.]]  
  ==  +  ==References== 
  +  {{Reflist}}  
  +  
  {{  + 
Current revision as of 07:18, 27 July 2010
Contents 
Constant Wall Heat Flux
In this article, we consider the case of fully developed laminar flow and constant properties in a circular tube with a fully developed temperature and concentration profiles. We first consider the case of constant heat rate per unit surface area for steady, laminar, fully developed flow. The energy equation in a circular tube, by neglecting axial heat conduction and viscous dissipation terms, is:

For a fully developed flow with constant wall heat flux, the following relationship (see eq. (18) in basics of internal forced convection)
can be substituted into the eq. (1) to obtain

The boundary conditions are

Integrating eq. (2) twice and applying the boundary conditions in eq. (3) to get the temperature distribution gives us

Using the definition of mean temperature presented in the last section with the above profile for temperature, and assuming constant properties:
Substituting eq. (4) into the above expression yields:

The heat flux at the wall can be obtained using the above relation for T_{m}

The heat flux at the wall can also be calculated using eq. (4) for the temperature profile and Fourier’s law of heat conduction

Combining eqs. (6) and (7) and solving for the heat transfer coefficient, h, yields
or in terms of the Nusselt number,

Constant Surface Temperature
We begin with the energy equation (eq. (29) in basics of internal forced convection)
and neglect the effects of axial heat conduction and viscous dissipation. We already showed that for a fully developed flow and temperature profile with constant surface temperature
The energy equation and boundary conditions, using the fully developed velocity profile (equation 24 in basics of internal forced convection)
and the above equation, are


The above equation and boundary conditions have been solved by various techniques in literatures, including separation of variables and infinite series. For additional detailed information the reader should refer to ^{[1]}^{[2]}^{[3]}^{[4]}^{[5]}.
The solution for eqs. (9) and (10) in the form of an infinite series for the temperature and Nusselt number is ^{[3]}:

where
The Nusselt number corresponding to the above temperature distribution is

The temperature slope for constant wall heat flux at the wall is higher than the temperature slope for constant surface temperature. This effect has resulted in a 16 percent increase in Nusselt number for constant wall flux versus constant wall temperature for a fully developed flow and temperature profile. The two cases of constant wall temperature and constant wall heat flux are special cases of a more general exponential heat flux boundary condition:

where A and n are both constants and n can be assumed to be either a positive or negative value, and n = 0 corresponds to constant heat flux at the wall and n = –14.63 corresponds to constant wall temperature.
Shah and London ^{[6]} developed the following correlation, which fits the exact solution of eq. (13) within 3 percent for –51.36 < n < 100.

Fullydeveloped fluid flow and heat transfer in an annulus
The problem of fluid flow and heat transfer in an annulus (see figure to the right) is also of considerable interest in various applications, including heat exchangers and heat pipes, due to an increase and flexibility in the heating and cooling of surface area.
We present the result below for the case in which both the inner wall (radius r_{i}) and outer wall (radius r_{o}) are kept at a constant heat flux for various values of K = r_{i}/r_{o}. K = 0 corresponds to conventional circular tubes, and K =1 corresponds to flow between two parallel planes.
The momentum and energy equations, as well as the boundary conditions for steady, laminar, fully developed flow and temperature profile, by neglecting radial conduction of the wall, axial heat conduction in the fluid, and viscous dissipation, and assuming constant properties, are




whereandare the inner and outer wall heat fluxes, respectively.
The velocity profile can be obtained by integrating eq. (15) twice and applying no slip boundary conditions at both the inner and outer walls.

where
The local heat transfer coefficients and Nusselt numbers are
where the hydraulic diameter, D_{h} = 2(r_{o} – r_{i}).
The energy equation can also be solved using the velocity profile given by eq. (17) in a similar manner as presented for a circular tube, except that it can involve lengthy algebra. Since the energy equation is linear and homogeneous, the principle of superposition was used to obtain the solution of the above problem as a sum of two problems. One problem is the outer wall heated uniformly and the inner wall insulated. The second problem is the inner wall heated uniformly and the outer wall insulated. The principle of superposition can be applied to linear homogeneous differential equations as long as the summation of the governing equations and boundary conditions for each subset problem will add to the original problem. Kakaç and Yucel ^{[7]} performed a numerical solution for fully developed velocity and temperature profile. The following table shows the inner and outer wall Nusselt number for various K values obtained by Kakaç and Yucel ^{[7]}.
The inner and outer wall Nusselt numbers, based on the average wall heat flux ratio, can be calculated from the results in the following table using the following equations:


where Nu_{ii} is defined as the inner wall Nusselt number when the inner tube is heated and outer wall is insulated. Similarly, Nu_{oo} is the outer tube Nusselt number when the outer wall is heated and inner tube is insulated. andare defined as influence coefficients and are a function of K only for laminar flow.
Table Nusselt number for fully developed flow and temperature profile with constant wall heat flux in an annulus, K = r_{i} /r_{o}
K  Nu_{ii}  Nu_{oo}  θ_{i}*  θ_{o}* 
0  ∞  4.364  ∞  0 
0.10  11.900  4.834  1.3835  0.0562 
0.25  7.735  4.904  0.7932  0.1250 
0.50  6.181  5.036  0.5288  0.2160 
1.00  5.384  5.384  0.3460  0.3460 
Fullydeveloped flow and heat transfer in tubes of noncircular cross section
The fluid and heat transfer solution for tubes of noncircular cross section with a fully developed flow and temperature profile can be obtained by solving the energy equation for the particular geometry. The results for some of the more conventional geometries obtained by Shah and London ^{[8]} are presented in the following table. There are three different boundary conditions in this table; “H1” which refers to the circumferentially constant wall temperature and the axial constant wall heat flux boundary condition, “H2” is for both axially and circumferentially constant heat flux at the wall, and “T” represents a constant wall temperature boundary condition. For the case of a symmetrically heated straight duct having no corners and a constant peripheral curvature, e.g. parallel planes and circular pipe, H_{1} and H_{2} boundary conditions are the same.
References
 ↑ Burmeister, L.C., 1993, Convective Heat Transfer, 2nd ed., John Wiley & Sons, Hoboken, NJ.
 ↑ Faghri, A., Zhang, Y., and Howell, J. R., 2010, Advanced Heat and Mass Transfer, Global Digital Press, Columbia, MO.
 ↑ ^{3.0} ^{3.1} Kakaç, S., Shah, R., Aung, W., 1987, Handbook of SinglePhase Convective Heat Transfer, John Wiley, New York.
 ↑ Kays, W.M., Crawford, M.E., and Weigand, B., 2005, Convective Heat Transfer, 4th ed., McGrawHill, New York, NY
 ↑ Bejan, A., 2004, Convection Heat Transfer, 3rd ed., John Wiley & Sons, Hoboken, NJ.
 ↑ Shah, R. K.; London, A. L., 1978, “Laminar Flow Convection in Ducts,” Advances in Heat Transfer, Supplement 1, Irvine, T. F. and Harnett, J.P., Eds., Academic Press, San Diego, CA.
 ↑ ^{7.0} ^{7.1} Kakaç, S., and Yucel, O., 1974, Laminar Flow Heat Transfer in an Annulus with Simultaneous Development of Velocity and Temperature Fields, Technical and Scientific Council of Turkey, TUBITAK, ISITEK No. 19, Ankara, Turkey.
 ↑ Shah, R. K.; London, A. L., 1974, “Thermal Boundary Conditions and Some Solutions for Laminar Duct Flow Forced Convection,” ASME J. Heat Transfer Vol. 96, pp. 159165.