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Heat and mass transfers in the context of energy geostructures  89


                   3.5.2 Convection heat transfer coefficient values
                   In the analysis of internal and external flows, the convection heat transfer coefficient,
                   h c , is typically used to express with the relevant temperature variation, ΔT, the heat
                   flux density. In the analysis of seepage flows, the separate terms ρ c pf v rf are used to
                                                                              f
                   equivalently express the convection heat transfer coefficient. Accordingly, the convec-
                   tion heat transfer coefficient depends on (1) the fluid thermophysical properties and
                   (2) the fluid velocity. These factors should be considered in the analysis and design of
                   energy geostructures.
                      The convection heat transfer coefficient may be broken down for convenience
                   into two components as

                                                                                          ð3:7Þ
                                                   h c 5 h c;n 1 h c;f
                   where h c;n is the portion of convection coefficient accounting for the natural convec-
                   tion phenomenon, whereas h c;f is the portion accounting for the forced convection
                   phenomenon.
                      A large number of expressions are available for estimating the natural convection
                   coefficient with reference to airflow over surfaces (Khalifa, 2001a; Khalifa, 2001b).
                   Bourne-Webb et al. (2016) report values of h c;n for heat flow from vertical external
                   surfaces in the range of 1 3 W/(m 2   C) (Khalifa, 2001a) and values for enclosed
                   vertical surfaces in the range of 2 4 W/(m 2   C) (Khalifa, 2001b). EN ISO 6946
                   (2007) suggests a value of 2.5 W/(m 2   C) for horizontal heat from internal surfaces.
                   Various expressions are also available for estimating the forced convection coefficient
                   with reference to airflow over surfaces. A power law theoretically relates the forced
                   convection coefficient h c;f to the airflow velocity v ra . However, Bourne-Webb et al.
                   (2016) suggest that a simple linear relationship is sufficiently accurate for airflows
                   characterised by a velocity lower than approximately v ra 5 5 m/s. Fig. 3.9 highlights
                   the previous fact by reporting correlations for flows over concrete between the
                   forced convection coefficient h c;f and the airflow velocity v ra . A correlation pro-
                   posed by Palyvos (2008), additional correlations that describe a comparable relation-
                   ship between the considered variables (EN ISO 6946, 2007; Lee et al., 2009;
                   ASHRAE, 2012) and experimental data provided by Lee et al. (2009) as well as by
                   Guo et al. (2011) are considered.
                      Different thermophysical properties should be considered for the diverse fluids that
                   characterise convection heat transfer phenomena associated with energy geostructures.
                   The fluid that characterises internal flow problems in pipes is water in the simplest
                   case, but may be a mixture of water and other constituents. The fluid that characterises
                   internal flow problems over a surface of an energy geostructure or external flow pro-
                   blems associated with convection at the ground surface is air. The fluid that charac-
                   terises seepage flow problems occurring underground is water.
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