对大气中硫酸胺粒子核化的分子理解
João Almeida1, Siegfried Schobesberger, Andreas Kürten
1Goethe-University of Frankfurt, Institute for Atmospheric and Environmental Sciences, 60438 Frankfurt am Main, Germany.
Nature
|October 8, 2013
概括
甲基胺显著增强气溶颗粒的形成,这对于云凝结核至关重要. 这一发现澄清了大气核化过程及其对气候的影响,特别是在胺源附近.
科学领域:
- 大气化学 大气化学
- 气候科学 气候科学
- 气溶物理 气溶物理
背景情况:
- 气溶颗粒对于云形成和气候调节至关重要.
- 目前的模型很难解释观测到的大气核化速率.
- 硫酸和氨单独不会导致颗粒的形成.
研究的目的:
- 研究氨酸在大气核形成中的作用.
- 提供氨基三元核形成的直接证据.
- 量化二甲基胺对粒子形成率的影响.
主要方法:
- 使用了CERN的CLOUD (宇宙在户外留下水滴) 室.
- 经过实验测试的核化速率与不同的二甲基胺度.
- 采用分子分析和量子化学计算用于集群动力学.
主要成果:
- 在 parts-per-trillion 的水平上,二甲基与氨相比,增强了超过 1,000 倍的颗粒形成.
- 涉及酸氨基对的基稳定机制解释了增强的核化.
- 银河系宇宙射线对星团形成的影响最小,除了低速率.
结论:
- 氨基,特别是二甲基胺,是大气核形成的关键驱动因素.
- 酸氨基对稳定了,减少了蒸发,增加了形成速度.
- 人为影响评估必须考虑在排放源附近的氨基和二氧化硫.
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