Maya Milliez

Micrometeorological Modeling of Radiative and Convective Effects with a Building-Resolving Code

AbstractIn many micrometeorological studies with computational fluid dynamics, building-resolving models usually assume a neutral atmosphere. Nevertheless, urban radiative transfers play an important role because of their influence on the energy budget. To take into account atmospheric radiation and the thermal effects of the buildings in simulations of atmospheric flow and pollutant dispersion in urban areas, a three-dimensional (3D) atmospheric radiative scheme has been developed in the atmospheric module of the Code_Saturne 3D computational fluid dynamic model. On the basis of the discrete ordinate method, the radiative model solves the radiative transfer equation in a semitransparent medium for complex geometries. The spatial mesh discretization is the same as the one used for the dynamics. This paper describes ongoing work with the development of this model. The radiative scheme was previously validated with idealized cases. Here, results of the full coupling of the radiative and thermal schemes with...

Effect of Atmospheric Stability on the Atmospheric Dispersion Conditions Over a Industrial Site Surrounded by Forests

This work investigates the impact of terrain heterogeneity and stability conditions (stable and unstable) on the local turbulence kinetic energy (TKE) around an industrial site using 36 months of data collected at the experimental site SIRTA (Instrumental Site of Atmospheric Research by Remote Sensin). These measurements show that the normalized TKE (TKE/U2: where U is the wind speed) is highly depended on the upstream complexity of the terrain (presence of forested areas or buildings) whatever the stability conditions (stable, unstable). The highest values of normalized TKE are obtained for unstable thermal stratification for all wind direction sector in the zones located behind the forested areas.

Development of a Building Resolving Atmospheric CFD Code Taking into Account Atmospheric Radiation in Complex Geometries

In order to take into account atmospheric radiation and the thermal effects of the buildings in simulations of atmospheric flow and pollution dispersion in urban areas, we have developed a three-dimensional atmospheric radiative scheme in the atmospheric module of the open-source CFD model Code_Saturne. This paper describes our ongoing work on the development of this model. The radiative scheme has been previously validated with idealized cases and the results of a real case. Here we present results of the full coupling of the radiative and thermal schemes with the 3D dynamical flow model and compare the results with simpler approaches found in the literature.

A New Method for Fast Computation of Three-Dimensional Atmospheric Infrared Radiative Transfer in a Nonscattering Medium, with an Application to Dynamical Simulation of Radiation Fog in a Built Environment

AbstractThe atmospheric radiation field has seen the development of more accurate and faster methods to take into account absorption. Modeling fog formation, where infrared radiation is involved, requires accurate methods to compute cooling rates. Radiative fog appears under clear-sky conditions owing to a significant cooling during the night where absorption and emission are the dominant processes. Thanks to high-performance computing, high-resolution multispectral approaches to solving the radiative transfer equation are often used. Nevertheless, the coupling of three-dimensional radiative transfer with fluid dynamics is very computationally expensive. Radiation increases the computation time by around 50% over the pure computational fluid dynamics simulation. To reduce the time spent in radiation calculations, a new method using analytical absorption functions fitted by Sasamori on Yamamoto’s radiation chart has been developed to compute an equivalent absorption coefficient (spectrally integrated). Onl...

3D Radiative and Convective Modeling of Urban Environment: An Example for the City Center of Toulouse

A three dimensional tool coupling the thermal energy balance of buildings and the modeling of the atmospheric flow in urban areas has been developed. In this work the effects of complexity in real urban geometry on the interaction between airflows and radiation exchanges with different surfaces is tested. The model results are encouraging and give insight into local surface-atmosphere processes, but further and more rigorous testing has to be performed with other datasets.

Comparison Between a Building Resolving Micro-Meteorogical Model and Measurements at SIRTA

This numerical work presents a computational fluid dynamics (CFD) model to simulate wind flow over complex site SIRTA which is located in Palaiseau, 20 km south of Paris (France) in a semi urban environment. The purpose is to study the ability of an atmospheric CFD model (Code_Saturne) to reproduce the micro scale heterogeneities of wind and turbulent kinetic energy (TKE), using a 16 month data set collected at SIRTA site. The forested areas were modeled either according to the classical roughness law or with a drag porosity model, in which trees effects are modeled with additional terms in momentum, TKE and dissipation rate equations. The results obtained in this work show that the drag porosity model represents well the special heterogeneities of the site and gives results much closer to experimental results than the classical roughness law in the sector where the influence of forested areas is predominant.

Poster 8 Radiative transfers in CFD modelling of the urban canopy

Abstract The processes that govern air pollution in the urban canopy highly depend on the shape and spacing of the buildings. The dynamical effects have been extensively studied using CFD techniques, usually assuming a neutral atmosphere and neglecting the thermal effects. Nevertheless, radiative transfers play an important role because of their influence on the urban canopy budget. In order to take into account the radiation budget in simulations of pollution dispersion in urban areas, we have developed a radiative scheme in the atmospheric CFD model Mercure_Saturne .