The primary goal of this study is to derive a better understanding of how land surface processes affect simulated boundary layer meteorological characteristics. The secondary goal is to demonstrate the effects of LULC changes on the temperature, wind transport, PBL height structure and surface flux field. MM5 simulations are performed with NOAH land surface model (LSM) and MRF planetary boundary layer (PBL) scheme. Two sets of MM5 sensitivity tests are designed to utilize different LU datasets: USGS and TFS data. The change of the LULC data modifies the simulated surface heat flux structure and local wind transport. The result demonstrates the benefit of utilizing more precise and updated LU data.
The coupling of NOAH LSM and MRF PBL scheme inside MM5 could not accurately simulate daytime and nighttime wind speeds. The daytime wind speed issue is caused by the inappropriate convective velocity scale which enhances the surface momentum flux. To solve this problem, a more represented surface flux formula was implemented in the MRF PBL scheme. The high bias of nighttime wind speed is hypothesized to be caused by the inadequate parameterizations utilized for the strong stable atmospheric conditions or could be associated with the height of the MM5 lowest model layer. MM5 implicitly assumes that the surface layer parameterizations apply to the whole bottom layer. In reality, the PBL height at nighttime can be lower than 100 m AGL and the formulas used are expected to be valid within the surface layer (~about one tenth of the PBL height). Utilization of accurate formulas may overcome the current shortcomings in nighttime wind prediction. Future research will review the formulas suitable for stable condition, modify the PBL schemes in MM5, and compare the new simulations with available measurements in the Houston areas.