Goethe-University of Frankfurt, Institute for Atmospheric and Environmental Sciences, 60438 Frankfurt am Main, Germany.
Nature. 2013 Oct 17;502(7471):359-63. doi: 10.1038/nature12663. Epub 2013 Oct 6.
Nucleation of aerosol particles from trace atmospheric vapours is thought to provide up to half of global cloud condensation nuclei. Aerosols can cause a net cooling of climate by scattering sunlight and by leading to smaller but more numerous cloud droplets, which makes clouds brighter and extends their lifetimes. Atmospheric aerosols derived from human activities are thought to have compensated for a large fraction of the warming caused by greenhouse gases. However, despite its importance for climate, atmospheric nucleation is poorly understood. Recently, it has been shown that sulphuric acid and ammonia cannot explain particle formation rates observed in the lower atmosphere. It is thought that amines may enhance nucleation, but until now there has been no direct evidence for amine ternary nucleation under atmospheric conditions. Here we use the CLOUD (Cosmics Leaving OUtdoor Droplets) chamber at CERN and find that dimethylamine above three parts per trillion by volume can enhance particle formation rates more than 1,000-fold compared with ammonia, sufficient to account for the particle formation rates observed in the atmosphere. Molecular analysis of the clusters reveals that the faster nucleation is explained by a base-stabilization mechanism involving acid-amine pairs, which strongly decrease evaporation. The ion-induced contribution is generally small, reflecting the high stability of sulphuric acid-dimethylamine clusters and indicating that galactic cosmic rays exert only a small influence on their formation, except at low overall formation rates. Our experimental measurements are well reproduced by a dynamical model based on quantum chemical calculations of binding energies of molecular clusters, without any fitted parameters. These results show that, in regions of the atmosphere near amine sources, both amines and sulphur dioxide should be considered when assessing the impact of anthropogenic activities on particle formation.
气溶胶颗粒从痕量大气蒸气中形成被认为提供了全球云凝结核的一半以上。气溶胶通过散射阳光和导致更小但更多数量的云滴,从而导致净冷却气候,这使得云更亮并延长了它们的寿命。人类活动产生的大气气溶胶被认为已经抵消了温室气体引起的大部分变暖。然而,尽管它对气候很重要,但大气成核仍未被很好地理解。最近,已经表明硫酸和氨不能解释在低层大气中观察到的颗粒形成速率。人们认为胺可能会增强成核,但直到现在,在大气条件下还没有直接证据表明胺的三元成核。在这里,我们使用 CERN 的 CLOUD(宇宙离开户外液滴)室,发现体积比为每万亿分之三以上的二甲胺可以使颗粒形成速率比氨提高 1000 多倍,足以解释在大气中观察到的颗粒形成速率。对团簇的分子分析表明,更快的成核是由涉及酸-胺对的碱基稳定机制解释的,该机制强烈降低了蒸发。离子诱导的贡献通常很小,这反映了硫酸-二甲胺团簇的高稳定性,并表明银河宇宙射线对它们的形成只有很小的影响,除非整体形成速率较低。我们的实验测量结果很好地被基于分子簇结合能量子化学计算的动力学模型所重现,而无需任何拟合参数。这些结果表明,在大气中靠近胺源的区域,在评估人为活动对颗粒形成的影响时,应同时考虑胺和二氧化硫。