Food Preservation by
Application of Heat
Radiation heat transfer is the transfer of heat energy by electromagnetic
radiation. Radiation operates independently of the medium through which it
occurs and depends upon the relative temperatures, geometric arrangements
and surface structures of the materials that are emitting or absorbing heat.
Radiation of wavelength 0.8-400 µm (infrared) is referred to as thermal
radiation or heat rays since electro magnetic radiation with this wavelength is
most readily absorbed and converted to heat energy. The infrared radiation is
used primarily for surface heating as it is transmitted rapidly to the surface. It
is used for dehydration of fruits and vegetables, freeze drying, baking, etc.
Radiation can be significant with small temperature differences as, for
example, in freeze-drying and in cold stores, but it is generally more important
where the temperature differences are greater. Under these circumstances, it is
often the most significant mode of heat transfer, for example in bakers' ovens
and in radiant driers.
The basic formula for radiant-heat transfer is the Stefan-Boltzmann Law
q = A σT
4
(1.3)
Where, T is the absolute temperature (measured from the absolute
zero of temperature at −273°C, and indicated in Bold type) in degrees
Kelvin (K) in the SI system, and (sigma) is the Stefan-Boltzmann constant
= 5.73 × 10
−8
J m
−2
s
−1
K
−4
The absolute temperatures are calculated by the
formula K = (°C+273).
This law gives the radiation emitted by a perfect radiator (a black body as this
is called though it could be a red-hot wire in actuality). A black body gives the
maximum amount of emitted radiation possible at its particular temperature.
Real surfaces at a temperature T do not emit as much energy as predicted by
Eq. (1.3), but it has been found that many emit a constant fraction of it. For
these real bodies, including foods and equipment surfaces, that emit a constant
fraction of the radiation from a black body, the equation can be rewritten
q
= εA σT
4
(1.4)
Where, ε (epsilon) is called the emissivity of the particular body and is a
number between 0 and 1. Bodies obeying this equation are called grey bodies.
Emissivities vary with the temperature T and with the wavelength of the
radiation emitted. For many purposes, it is sufficient to assume that for:
* dull black surfaces (lamp-black or burnt toast, for example), emissivity is
approximately 1;
* surfaces such as paper/painted metal/wood and most foods, emissivities
are about 0.9;
* rough un-polished metal surfaces, emissivities vary from 0.7 to 0.25;
* polished metal surfaces, emissivities are about or below 0.05.
These values apply at the low and moderate temperatures, which are those
encountered in food processing. Just as a black body emits radiation, it also
absorbs it and according to the same law, Eq. (1.3). Again grey bodies absorb
a fraction of the quantity that a black body would absorb, corresponding this
time to their absorptivity α (alpha). For grey bodies it can be shown that α =
ε. The fraction of the incident radiation that is not absorbed is reflected, and
thus, there is a further term used, the reflectivity, which is equal to (1 – α).
The radiant energy transferred between two surfaces depends upon their
temperatures, the geometric arrangement, and their emissivities. For two
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