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Heat transfer
Conduction
Convection
Radiation
Mass transfer
Condensation
 
Conduction

Conduction is the transfer of heat energy through solids or stationary fluids. Heat is transferred by lattice vibrations and particle collisions.

In solids atoms are bound together by bonds which behave like springs. Atoms that are hot will vibrate more vigorously with these vibrations, and therefore energy, being transferred to neighbouring atoms until equilibrium is reached (i.e. until all the atoms have the same energy/temperature).

 

Energy is also transferred by particle collisions. Hotter molecules move faster than cooler ones, and energy is transferred to the lower energy molecules when they collide. These random collisions continue until equilibrium is reached, when the molecules are moving with the same average velocity. This behaviour is seen in stationary fluids and with the free electrons in metals.

The rate of heat transfer due to conduction is:

Where:

Q
is the heat transfer, in W;
is the thermal conductivity of the material, in W/mK;
A
is the cross sectional area, in m2;
T1-T2
is the temperature difference between the two environments, in K;
t
is the thickness between the two cross sections, in m,


           
                      


The thermal resistance of conduction is given by:




Where:




is the thermal resistance of conduction in m2K/W

Therefore:




It is clear from the above equations that there will be lower heat flow (higher resistance) if the thermal conductivity is lower, the heat path is longer, or the area is lower.

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