Atmospheric particulate matter plays an important role in the Earth's radiative balance. Over the past two decades, it has been established that a portion of particulate matter, black carbon, absorbs significant amounts of light and exerts a warming e ect rivalling that of anthropogenic carbon dioxide 1,2 . Most climate models treat black carbon as the sole light-absorbing carbonaceous particulate. However, some organic aerosols, dubbed brown carbon and mainly associated with biomass burning emissions 3-6 , also absorbs light 7 . Unlike black carbon, whose light absorption properties are well understood 8 , brown carbon comprises a wide range of poorly characterized compounds that exhibit highly variable absorptivities, with reported values spanning two orders of magnitude 3-6,9,10 . Here we present smog chamber experiments to characterize the e ective absorptivity of organic aerosol from biomass burning under a range of conditions. We show that brown carbon in emissions from biomass burning is associated mostly with organic compounds of extremely low volatility 11 . In addition, we find that the e ective absorptivity of organic aerosol in biomass burning emissions can be parameterized as a function of the ratio of black carbon to organic aerosol, indicating that aerosol absorptivity depends largely on burn conditions, not fuel type. We conclude that brown carbon from biomass burning can be an important factor in aerosol radiative forcing.Black carbon (BC) in atmospheric particulate matter is an important global warming agent (potentially second only to CO 2 ) with estimates of its direct radiative forcing (DRF) ranging between 0.17 and 1.48 W m −2 (ref. 2). The large uncertainty in BC DRF stems partly from the mismatch between BC light absorption (hence its DRF) estimated by climate models and that retrieved using remote sensing, with models usually reporting smaller values 2 . Open biomass burning contributes one-third of the global BC budget. Biomass burning is also a major source of organic aerosol (OA), contributing two-thirds of the global primary OA budget 2,12 , which most climate models treat as purely scattering. The cooling due to this scattering offsets the warming by BC from biomass burning, resulting in negative net DRF for biomass burning emissions 13 . However, there is a growing body of evidence that biomass burning OA contains substantial amounts of light-absorbing brown carbon 3-6 (BrC), which can shift the net biomass burning DRF to positive values 14 . Neglecting absorption by biomass burning OA might lead to misattribution of observed atmospheric particulate matter absorption to BC, contributing to the discrepancy between models and observations. There are substantial uncertainties in quantifying the effect of BrC. A major obstacle is the very high variability in reported light absorption properties of biomass burning OA, often attributed to fuel type and burn conditions 4,6 , which complicates their treatment in climate models.In this study, we show that the least volatile fraction (extreme...

Experiments were conducted to investigate light absorption of organic aerosol (OA) in fresh and photo-chemically aged biomass-burning emissions. The experiments considered residential hardwood fuel (oak) and fuels commonly consumed in wild-land and prescribed fires in the United States (pocosin pine and gallberry). Photo-chemical aging was performed in an environmental chamber. We constrained the effective light-absorption properties of the OA using conservative limiting assumptions, and found that both primary organic aerosol (POA) in the fresh emissions and secondary organic aerosol (SOA) produced by photo-chemical aging contain brown carbon, and absorb light to a significant extent. This work presents the first direct evidence that SOA produced in aged biomass-burning emissions is absorptive. For the investigated fuels, SOA is less absorptive than POA in the long visible, but exhibits stronger wavelength-dependence and is more absorptive in the short visible and near-UV. Light absorption by SOA in biomass-burning emissions might be an important contributor to the global radiative forcing budget

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Most chemical transport models assume instantaneous equilibrium to represent gas-particle partitioning of semivolatile organic aerosol. This approach has been challenged by recent studies suggesting that secondary organic aerosol (SOA) cannot reach equilibrium within atmospheric time scales. The emergent hypothesis is that gas-particle partitioning rates are limited by diffusion within the condensed phase, which is thought to be "glassy." Here, we investigate the equilibration time scales of SOA formed from α-pinene ozonolysis by measuring the dynamic response to a modest step-change in temperature. Upon heating, equilibrium is disturbed, and the particles evaporate to restore equilibrium at the new temperature, which is attained when evaporation ceases. The SOA was formed at 10 °C and then heated to near room temperature (30 °C) so that the phase state (viscosity) of the condensed-phase after heating is similar to how it would be in the atmosphere. Experiments were performed in both a thermodenuder, with SOA loading of 350 μg/m(3), and in a smog chamber, with SOA loading of 2-12 μg/m(3). Both experiments show, contrary to previous findings, that the SOA achieves equilibrium with dynamic responses consistent with a mass accommodation coefficient of order 0.1. For typical atmospheric conditions, this translates into equilibration time scales on the order of minutes to tens of minutes, supporting the use of equilibrium partitioning in chemical transport models.