Page 187 - Design of Solar Thermal Power Plants
P. 187

172         3. GENERAL DESIGN OF A SOLAR THERMAL POWER PLANT

               Apparently, D ¼ B e F, then, Eq. (3.46) can be reorganized into:
                   2
                  d T fo   dT fo               dT fi
                       þ A     þ BðT fo   T fi ¼ C  þ ES   FðT fi   T a Þ  (3.53)
                                          Þ
                   ds 2     ds                 ds
               Heat losses of parabolic trough collector toward the environment in-
            cludes not only thermal convection with the surrounding air, but also the
            radiation heat exchange with the sky; thus the last column that represents
            heat loss in Eq. (3.53) can be expressed by two terms, one of which takes
            the form of a quadratic term, then Eq. (3.53) can be modified as
               2
              d T fo   dT fo               dT fi                          2
                   þ A     þ BðT fo   T fi Þ¼ C  þ ES   FðT fi   T a Þ  GðT fi   T a Þ
               ds 2     ds                 ds
                                                                        (3.54)
               As a matter of fact, for application-level large-scale parabolic trough
            collectors, inlet temperature T fi and outlet temperature T fo of heat-transfer
            fluid within the collector that have been measured simultaneously do not
            correspond to the two parameters of Eq. (3.54) in time; a time lag rela-
            tionship exists between T fi and T fo , and it is necessary to consider flow
            time s p of heat-transfer fluid from the inlet to the outlet of parabolic trough
            collector. Therefore, the corresponding actual relationship of them in the
            dynamic test model can be expressed as:
                                    T fo ðs þ s p Þ¼ f½T fi ðsފ        (3.55)
            in which s p depends on the length L of parabolic trough collector and
            mean flow rate v of heat-transfer fluid during the test, which can be
            expressed as
                                         s p ¼ L=v                      (3.56)

               However, in order to achieve a concise model expression, in the
            dynamic test model of this section, T fo (s þ s p ) and T fi (s) are no longer
            specially marked; instead, they will be considered during experimental
            data treatment, model identification and thermal performance prediction
            and calculation.

            3.3.3.4 Establishment of Optical Model
               An optical model is established based on S in Eq. (3.54), which aims at
            offering the physical relationship between it and solar DNI G DN and the
            respective mathematical expression. As S is the section absorbed by
            the exterior wall surface of metal tube when solar DNI is perpendicular to
            the aperture of parabolic trough collector, it is a parameter that cannot be
            directly measured; it requires considering influences of parabolic trough
            concentrator reflection and transmission absorption of evacuated tube.
            This section of the model involves a parabolic trough collector truncation
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