Biomass Burning: Major Uncertainties, Advances, and Opportunities
Biomass Burning: Major Uncertainties, Advances, and Opportunities
Abstract:
Domestic and open biomass burning are poorly-understood, major influences on Earth’s atmosphere composed of countless individual fires that (along with their products) are difficult to quantify spatially and temporally. Each fire is a minimally-controlled complex phenomenon producing a diverse suite of gases and aerosols that experience many different atmospheric processing scenarios. New lab, airborne, and space-based observations along with model and algorithm development are significantly improving our knowledge of biomass burning. Several campaigns provided new detailed emissions profiles for previously undersampled fire types; including wildfires, cooking fires, peat fires, and agricultural burning; which may increase in importance with climate change and rising population. Multiple campaigns have better characterized black and brown carbon and used new instruments such as high resolution PTR-TOF-MS and 2D-GC/TOF-MS to improve quantification of semi-volatile precursors to aerosol and ozone. The aerosol evolution and formation of PAN and ozone, within hours after emission, have now been measured extensively. The NASA DC-8 sampled smoke before and after cloud-processing in two campaigns. The DC-8 performed continuous intensive sampling of a wildfire plume from the source in California to Canada probing multi-day aerosol and trace gas aging. Night-time plume chemistry has now been measured in detail. Fire inventories are being compared and improved, as is modeling of mass transfer between phases and sub-grid photochemistry for global models.
