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Chapter 6 Forced Convection

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Chapter 6 explores the fascinating world of forced convection, a dominant mode of heat and mass transfer driven by external forces, such as fans or pumps, in a fluid flow. This chapter provides a comprehensive and detailed examination of the underlying principles, mathematical models, and practical applications of forced convection. The document covers the governing equations of forced convection, including the Navier-Stokes equations and the continuity equation, essential for understanding fluid flow behavior and heat transfer characteristics. An in-depth analysis of forced convection over various geometries and configurations, including flat plates, cylinders, and tubes, is provided. The chapter offers insights into the effects of flow regimes and boundary conditions on heat transfer rates. Heat transfer correlations and empirical relationships used for engineering calculations are discussed, allowing engineers and researchers to predict and optimize heat transfer performance in forced convection scenarios. The practical applications of forced convection in diverse fields are explored, including cooling of electronic devices, heat exchangers, and heating, ventilation, and air conditioning (HVAC) systems. The chapter also delves into the use of forced convection in industrial processes and renewable energy technologies. Advanced topics, such as turbulent forced convection, enhancement techniques, and numerical simulations, are also addressed, offering a comprehensive understanding of forced convection phenomena and its applications. Researchers, engineers, and students will find this chapter a valuable resource for gaining insights into the complexities of forced convection and for designing efficient heat transfer systems across various industries and engineering disciplines

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Forsberg Heat Transfer
Chapter 6
Forced Convection




Dimensionless Numbers
Experimental data for forced convection
is correlated by three dimensionless
parameters: the Reynolds Number,
the Prandtl number,and the Nusselt Number.
 VL
Reynolds Number = Re =

 = fluid density V = fluid velocity
L = characteristic length of geometry
 = fluid absolute viscosity
 =  /  = fluid kinematic viscosity, so
VL
Reynolds Number = Re =





1

, cp 
Prandtl Number = Pr =
k
cp = fluid specific heat at constant pressure
 = fluid absolute viscosity
k = fluid thermal conductivity
hL
Nusselt Number = Nu =
k
h = convective coefficient
We are looking for h so the convective heat
transfer can be determined. Thus, correlation
of experimental data gives Nu as a function
of Re and Pr : Nu = f (Re, Pr)




Nu = f (Re, Pr)
The functional relationship is often
of the form Nu = C Rea Prb


Fluid velocities for natural convection are much
smaller that those for forced convection. The
Reynolds Number is no longer significant. It is
replaced by the Grashof Number:




2

, g  (Ts − T ) L3
Grashof Number = Gr =
2
g = acceleration of gravity
 = coefficient of thermal expansion of fluid
L = characteristic length of geometry
Ts = surface temperature
T = fluid temperature
 = fluid kinematic viscosity
hL
Nu = = f (Gr, Pr)
k




Forced Convection - External Flow
Flow Over a Flat Plate




3

, There are three flow regions: laminar, transition,
and turbulent. If the plate is short, there might only be
a laminar region on it. The transition region is short, and
often the flow is modeled as only laminar and turbulent;
the "critical length", xc , being the location of the change
from laminar to turbulent.

 = boundary layer thickness




For flow over a flat plate, the Renolds Number at location x is
 u x u x
Re x = =
 
The critical distance is typically the distance where the Reynolds
Number is 5 x 10 5 .
(5 x 105 ) (5 x 105 )
That is, xc = =
 u u
The boundary layer thickness  varies with x. It is usually defined
as the distance from the surface at which the x-component of
velocity, u, is 99% of the free-stream velocity u .
u
At y =  , = 0.99
u




4

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