Jokinen T, Sipilä M, Kontkanen J, Vakkari V, Tisler P, Duplissy E-M, Junninen H, Kangasluoma J, Manninen H E, Petäjä T, Kulmala M, Worsnop D R, Kirkby J, Virkkula A, Kerminen V-M
INAR-Institute for Atmospheric and Earth System Research, P.O. Box 64, 00014 University of Helsinki, Finland.
Finnish Meteorological Institute, Erik Palménin aukio 1, 00560 Helsinki, Finland.
Sci Adv. 2018 Nov 28;4(11):eaat9744. doi: 10.1126/sciadv.aat9744. eCollection 2018 Nov.
Formation of new aerosol particles from trace gases is a major source of cloud condensation nuclei (CCN) in the global atmosphere, with potentially large effects on cloud optical properties and Earth's radiative balance. Controlled laboratory experiments have resolved, in detail, the different nucleation pathways likely responsible for atmospheric new particle formation, yet very little is known from field studies about the molecular steps and compounds involved in different regions of the atmosphere. The scarcity of primary particle sources makes secondary aerosol formation particularly important in the Antarctic atmosphere. Here, we report on the observation of ion-induced nucleation of sulfuric acid and ammonia-a process experimentally investigated by the CERN CLOUD experiment-as a major source of secondary aerosol particles over coastal Antarctica. We further show that measured high sulfuric acid concentrations, exceeding 10 molecules cm, are sufficient to explain the observed new particle growth rates. Our findings show that ion-induced nucleation is the dominant particle formation mechanism, implying that galactic cosmic radiation plays a key role in new particle formation in the pristine Antarctic atmosphere.
由痕量气体形成新的气溶胶粒子是全球大气中云凝结核(CCN)的主要来源,可能对云的光学特性和地球辐射平衡产生重大影响。受控实验室实验已经详细解析了可能导致大气中形成新粒子的不同成核途径,但实地研究对大气不同区域所涉及的分子步骤和化合物了解甚少。初级粒子源的稀缺使得二次气溶胶的形成在南极大气中尤为重要。在此,我们报告了对硫酸和氨的离子诱导成核的观测结果——欧洲核子研究组织的CLOUD实验对该过程进行了实验研究——这是南极沿海地区二次气溶胶粒子的主要来源。我们进一步表明,测得的高硫酸浓度超过每立方厘米10个分子,足以解释观测到的新粒子生长速率。我们的研究结果表明,离子诱导成核是主要的粒子形成机制,这意味着银河宇宙辐射在原始南极大气的新粒子形成中起着关键作用。