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1.8 Principles of heat and fluid flow  15




                  Eq. (1.25) over the entire surface leads to average convection coefficient ( ) h  for the                                 h¯
                  entire surface:
                                                 1
                                              h  =   hdA                         (1.26)
                                                 L  ∫ A s  s                                                                                 h¯=1L∫AshdAs
                     A thermal resistance is also defined for convection heat transfer from Eq. (1.27):

                                             Q    =  ∆T  =  ∆T                   (1.27)
                                                1/ hA  R conv                                                                                  Q˙=∆T1/hA=∆TRconv

                     The convective thermal resistance (R  ) is then:
                                                  conv
                                                     1
                                                R  =                             (1.28)
                                                 conv  hA                                                                                    Rconv=1hA
                     Another important factor in convective heat transfer is friction coefficient (C ),
                                                                                    f
                  the characteristic of the fluid flow, which is:
                                                    τ
                                              C f  =  w                          (1.29)
                                                      2
                                                  ρ u /2                                                                                     Cf=τwρ∞u∞ /2
                                                                                                                                                       2
                                                   ∞∞
                  1.8.2.3  Radiation heat transfer
                  Radiation heat transfer is the energy that is emitted by matter in the form of photons
                  or electromagnetic waves. Radiation can be important even in situations in which
                  there is an intervening medium. An example is the heat  transfer that take place
                  between a living entity with its surrounding.
                     All bodies radiate energy in the form of photons. A photon is the smallest discrete
                  amount of electromagnetic radiation (i.e., one quantum of electromagnetic energy is
                  called a photon). Photons are massless and move in a random direction, with random
                  phase and frequency. The origin of radiation is electromagnetic and is based on the
                  Ampere law, the Faraday law and the Lorentz force. Maxwell analytically showed
                  the existence of electromagnetic wave. Electromagnetic waves transport energy at
                  the speed of light in empty space and are characterized by their frequency (ν) and
                  wavelength (λ) as follow:
                                                    C
                                                 λ =                             (1.30)
                                                    ν                                                                                       λ=Cν
                  where C is the speed of light in the medium.
                     The electromagnetic waves appear in nature for wavelength over an unlimited
                  range. Radiation with wavelength between 0.1 and 100 µm is in form of thermal
                  radiation and is called radiation heat transfer. Thermal radiation includes the entire
                  visible and infrared as well as a portion of ultraviolet radiation.
                     All bodies at a temperature above absolute zero emit radiation in all directions
                  over a wide range of wavelengths. The amount of emitted energy from a surface at a
                  given wavelength depends on the material, condition, and temperature of the body.
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