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I 06                                                CHAPTER 4 PHYSICAL FUNDAMENTALS
                      4.3.1.3 Radiation
                          Heat radiation is electromagnetic radiation that all bodies emit due to
                      their temperature. The wavelength of electromagnetic radiation is be-
                      tween 0.3 and 50 jjim. This mode of heat transfer does not depend on an
                      intermediate agent. When radiation falls on a body, part of the energy is
                      absorbed, part is reflected, and the remainder is transmitted through the
                      body. These components of the incoming radiation are the absorption ra-
                      tio a, reflectance ratio p and transmission ratio r. When a body is in a
                      state of equilibrium, the incoming and outgoing radiation are equal.
                      Hence, a + p + r — 1.
                          A body having good electrical conductivity will absorb the incoming ra-
                      diation on a distance of one wavelength. Now r = 0 and a + p = 1.
                          A planar polished surface reflects heat radiation in a similar manner with
                      which it reflects light. Rough surfaces reflect energy in a diffuse manner; hence
                      radiation is reflected in all directions. A blackbody absorbs all incoming radi-
                      ation and therefore has no reflection. A perfect blackbody does not exist; a
                      near perfect blackbody surface such as soot reflects 5% of the radiation, mak-
                      ing it the standard for an ideal radiator.
                          The radiant emittance of a blackbody is


                                                                       2
                                                                                  4
                      where cr is the Stefan-Boltzmann constant, 11.865 W m~  (MJ/kmol)" .
                          The radiation emitted by a body due to its temperature is defined by the
                      factor e, the emissivity,







                      for a given temperature, angle, and frequency. For approximate calculations
                      the emissivity can be assumed constant over the whole frequency spectrum. In
                      this case the body is classified as a gray body.
                          The net heat transfer between two surfaces according to Eq. (4.159)
                      is proportional to the first or second power of the temperature differ-
                      ence; hence the radiation heat transfer dominates at a high temperature
                      or for large temperature differences. When the temperature difference is
                      small, a heat transfer factor is used similar to that used for convective
                      heat transfer:




             4.3.2 Analogy with the Theory of Electricity
                      Equation (4.154) gives conduction for the one-dimensional case with constant
                      thermal conductivity:
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