Theoretical Overview
The basic equations used to study heat transfer are:
q = UADT
where U is the overall heat transfer coefficient; A is the area over which heat transfer occurs; T is the temperature; and q is the heat transferred.
Nu = hD/k
Nu a Re
Nu a Pr
where h is the local heat transfer coefficient; D is the diameter; k is the thermal conductivity; Re is the Reynolds Number; Pr is the Prandtl Number; and Nu is the Nusselt Number.
Re = uD/v
where u is the velocity of the fluid; and v is the kinematic viscosity.
Pr = v/a
where a is the thermal diffusivity.
The diffusive-convective equation is an energy balance of the heat transferred in and out of the system.
rCpV(¶T/¶t) = k(¶2T/¶x2)+ Q
where r is the density of the fluid; Cp is the heat capacity of the fluid; V is the volume of the fluid; (¶T/¶t) is the change in temperature with respect to time; (¶2T/¶x2) is the change of temperature with respect to position; Q is the rate of heat generation in the system.
What
is Unsteady State Heat Transfer |
Unsteady State Heat
Transfer Experiment |
Examples of Unsteady State Heat Transfer | |
Applications
in Industry
| Definitions
| References