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Variability of urban surface temperatures and implications for aerodynamic energy exchange in unstable conditions
Author(s) -
Crawford Ben,
Grimmond Sue B.,
Gabey Andrew,
Marconcini Mattia,
Ward Helen C.,
Kent Christoph W.
Publication year - 2018
Publication title -
quarterly journal of the royal meteorological society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.744
H-Index - 143
eISSN - 1477-870X
pISSN - 0035-9009
DOI - 10.1002/qj.3325
Subject(s) - environmental science , sensible heat , eddy covariance , planetary boundary layer , aerodynamics , satellite , atmospheric sciences , spatial variability , meteorology , mathematics , geography , statistics , turbulence , geology , physics , ecosystem , ecology , astronomy , biology , thermodynamics
Sensible heat flux ( Q H ) is a critical driver of surface and boundary layer meteorological processes, especially in urban areas. Aerodynamic resistance methods (ARM) for modelling Q H are promising because, in principle, all that is needed is surface temperature ( T 0 ), air temperature ( T A ) and an aerodynamic resistance term ( r H ). There are significant challenges in urban areas, however, due to uncertainties in satellite‐derived land surface temperatures ( LST ), logistical challenges in obtaining high‐resolution air temperatures, and a limited understanding of spatial and temporal variability of r H and associated variables (e.g. thermal roughness length). This work uses an extensive LST dataset covering 6 years (2011–2016) in central London and a long‐term in situ observation network to analyse the variability of LST and r H variables. Results show that LST is spatially correlated with building and vegetation land cover with coherent thermal structures at length scales less than 500–1,000 m. Additionally, satellite‐observed LST varies with average building height (up to 10% cooler in areas with tall buildings). The r H term and associated variables are observed to vary on daily and seasonal cycles, and findings are used to model Q H using five variations of an ARM‐based approach on a 100 m pixel basis. Modelled Q H is compared to observations from three scintillometer paths and an eddy covariance flux tower. We find generally good agreement between observations and models, although there is uncertainty in all methods (mean absolute error ranges from 58.1–129.3 W/m 2 ) due to the challenges involved in determining high‐resolution meteorological and surface inputs, particularly LST and friction velocity ( u * ). Additional complexity in evaluating modelled Q H arises from anthropogenic heat sources: long‐term tower‐based observations show that T A and the radiometer‐derived T 0 are warmer during working weekdays than non‐working days (up to 0.7 °C) and that there is an observed lag (2–3 hr) between energy consumption and the observed warming and modelled Q H .