Modes of Heat Transfer
OBJECTIVES:
-- To study different modes of heat transfer.
-- To determine rate of heat transfer in food and
non-food materials
Why study heat transfer?
-- to examine how foods are heated and cooled
-- to calculate the rate of heating and cooling
-- to design new heat transfer equipment
-- to assess the performance of existing heat
exchange equipment
-- Energy transfer at a molecular level
-- No physical movement of the material
-- Heating/Cooling of the solid material
The rate of heat flux (rate of heat transfer per
unit area) in a solid object is proportional to the temperature gradient, this
can be stated mathematically as,

We
may remove the proportionality by using a constant 'k', to obtain, Fourier’s Law

where
qx = rate of heat
transfer in the x direction by conduction, W
k = thermal conductivity, W/mC
A = area (normal to x-direction) through which heat flows, m2
T = temperature, C
x = length, variable, m
SIGN CONVENTION
Temperature Distance


Thermal Conductivity,
k unit: W/mC
Water: k = 0.597 W/mC
Air : k
= 0.0251 W/mC
Insulating
materials: k = 0.035 - 0.173 W/mC
For foods
k = 0.25 mc
+ 0.155 mp + 0.16 mf + 0.135 ma + 0.58 mm
Where m is mass
fraction and subscripts c: carbohydrate, p: protein, f: fat, a: ash, m:
moisture.
CONVECTION
Fluid flow over a solid body --
heat transfer between a solid and a fluid.

Newton’s Law of Cooling:
q = h A (Tp-Ta)
where: h is convective heat transfer coefficient
(W/m2C), A is area (m2), Tp is plate surface
temperature (°C),
Ta is
surrounding fluid temperature (°C).
Forced
Convection - artificially
induced fluid flow
Free
(Natural) Convection -- caused due
to density differences
Fluid condition h (W/m2C)
Air, free
convection 5-25
Air,
forced convection 10-200
Water,
free convection 20-100
Water,
forced convection 50-10,000
Boiling
water 3,000-100,000
Condensing
water vapor 5,000-100,000
RADIATION
Heat transfer between two surfaces by emission and later absorption of electromagnetic radiation

n
requires no physical
medium
n
Stefen-Boltzmann
Equation:
q
= A s e (T24
– T14)
where s =
Stefen-Boltzmann's constant, 5.669x10-8 W/m2K4
e = emissivity,
(varies from 0 to 1) dimensionless
A = area, m2
T1 =
temperature of surface 1, Absolute
T2 =
temperature of surface 2, Absolute