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. Author manuscript; available in PMC: 2023 Jan 31.
Published in final edited form as: Int J Wildland Fire. 2022 Jan 31;31(2):193–211. doi: 10.1071/wf20140

Table 3.

Plume rise model differences

Approach Briggs Sofiev PBL500
Type Empirical, analytical Empirical, analytical Statistical
Scheme Plume height is a function of downwind distance, modified for wildfire by Pouliot et al. (2005); plume top is calculated, and the plume bottom is set to be 2/3 of plume top value Energy-balance-based parameterisation (similar to convective cloud formulations) accounting for planetary boundary layer (PBL) height, power law dependence of fire intensity, and stability above the PBL, with four fitted tuneable parameters to match observed plume heights by MISR Observation-based, consistent statistical approximation
Input parameters Area burned, fuel loading, wind speed, duration of fire, heat content, fire location coordinates Fire Radiative Power (FRP), potential temperature as a function of geometric height to derive Brunt–Väisälä frequency, PBL height, fire location coordinates PBL height, fire location coordinates
Output parameters Top and bottom of smoke plume Top of smoke plume Top of smoke plume
Previous comparisons with satellite observations Tendency to underpredict (Raffuse et al. 2012); plume tops are generally higher than Sofiev owing to inherent incompatibility and formulation (designed for stack heights), with fires (Sofiev et al. 2012) Poor to moderate; comparable with or better than a one-dimensional plume rise model (Sofiev et al. 2012; Paugam et al. 2016) Not available
Ease of implementation in CMAQ Currently used Low to moderate Very low
Existing implementation SMOKE, CMAQ, HYSPLIT CMAQ (by Baldassarre et al. 2015) Not currently used