Bridging the gap between applied meteorology and climate science: a white roof example
Dan Li1*
1 Department of Earth and Environment and Department of Mechanical Engineering, Boston University, Boston, USA
* corresponding author: [email protected]
White roof is a widely-studied urban heat mitigation strategy and frequently incorporated into climate adaptation plans by cities.
Assessing the effects of white roofs on temperature has often been approached from the perspective of applied meteorology.
Here, the white roof problem is reframed to a climate science problem by focusing on the roof surface temperature, incorporating concepts of climate forcing, sensitivity, and feedback, and utilizing a linearized surface energy balance (SEB) model.
Different from the Albedo Cooling Effectiveness (ACE) index used for \textit{quantifying} white roof effects, a new index called Albedo Cooling Sensitivity (
Li et al. (in submission). Bridging the gap between applied meteorology and climate science: a white roof example
https://github.com/DanLi-BU/WRF/tree/WRF_ALBEDO (tag: ALB_final)
Model | Version | Repository Link | Tag | DOI |
---|---|---|---|---|
WRF | 4.2.2 | https://github.com/DanLi-BU/WRF/tree/WRF_ALBEDO | ALB_final |
Fill in detailed info here or link to other documentation to thoroughly walkthrough how to use the contents of this repository to reproduce your experiment. Below is an example.
- Install the software components required to conduct the experiment from contributing modeling software
- Download and install the supporting input data required to conduct the experiment. wrfinput_d03 is for the control run, and wrfinput_d03_alb60 is for the high-albedo run. Do NOT modify URBPARM.TBL when considering high albedo for roofs because modifying URBPARM.TBL will alter the roof albedo for all domains.
- Use the following namelist.input in the
scripts
directory to re-create this experiment:
Script Name | Description | How to Run |
---|---|---|
namelist.input_July |
namelist to run the WRF experiment for July | |
namelist.input_Feb |
namelist to run the WRF experiment for Feb |
- change sf_sfclay_physics and bl_pbl_physics of all three domains to 2 for using MYJ
- change sf_sfclay_physics and bl_pbl_physics of all three domains to 5 for using MYNN
Use the scripts found in the figures
directory to reproduce the figures used in this publication.