The September 2010 PIESA/Aerosol Experiments: Difference between revisions
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== The QFED Emissions == | == The QFED Emissions == | ||
In order to further improve the GEOS-5 modeling capabilities and accelerate the transition of NASA satellite information into operational application, an improved biomass burning emissions dataset - Quick Fire Emission Dataset (QFED) was developed. QFED addresses some of the weaknesses of the Global Fire Emissions Database used in the base system configuration. Among the major limitations of the GFED emissions are the low spatial resolution (1x1 degree) and temporal resolution (monthly). | |||
The QFED emissions are based on the 'top-down' approach that uses the fact that the fire radiative power (FRP) at the top of the atmosphere is proportional to the rate of organic/vegetation mass that is burning. On the other hand, the emission of gasses and particulate matter released during burning is proportional to the consumed mass, hence the emissions rates are proportional to the measured FRP. | |||
The FRP needed to calculate the biomass burning emission were derived from the MODIS Thermal Anomalies/Fire products (MOD14, MYD14). The calibration of the QFED emissions was done individually for the MODIS/Terra and MODIS/Aqua data using the emissions factors from Andreae and Merlet. Our first step was to use global monthly mean GFED emissions to find individual global calibration factors for MODIS/Terra and MODIS/Aqua instruments. Using individual calibration factors has an advantage over using a single common factor for the two instruments, because one can account for the differences in the fire strengths at the local time of the satellite overpass, and at the same time provides redundancy in case one of the satellites fails. The derived in this way fire emissions were used in the 'R_ddQFED' experiment (see below). The benefits of this calibration is that the globally the fire emissions are comparable to the commonly used GFED emissions, however they are available daily at 0.25x0.25 degrees horizontal resolution. | |||
Our next objective was to produce more realistic fire emission magnitudes. As in-situ measurements of fire emissions are very limited, we instead relied on the fact that biomass burning can have significant contribution to the total aerosol loadings near active fires and downwind. Thus, one can use AOT magnitude and relate it to the fire emission strength. | |||
Our approach was to find a global scale factor that minimizes the differences between the AOT retrieved by satellites and the modeled AOT which is equal to the sum of AOT due to biomass burning and AOT due to other type of aerosols. We constructed and performed two modeling runs - one with biomass burning (R_ddQFED) and another with no biomass burning (R_mmNOBB). From these two runs we calculated the contribution of the biomass burning to the AOT and found the optimal value of the global scale factor that minimized the difference between the observed AOT and the modeled AOT. As a first approximation the same factor was used to scale the QFED emissions. The derived in this way QFED emissions were used in the R_ddQFED_MISR experiment. | |||
(Overview of the formulation, including results of tuning exercise) | (Overview of the formulation, including results of tuning exercise) | ||