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Ion induced nucleation in the atmosphere: Studies of ammonia, sulfuric acid, and water cluster ions.

机译:离子在大气中引起的成核作用:研究氨,硫酸和水簇离子。

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摘要

Current models of homogeneous gas phase nucleation lack thermodynamic data essential to understanding particle growth mechanisms and accurately predicting nucleation rates in the atmosphere. Nucleation model predictions are highly sensitive to the thermodynamics of the initial stages of particle growth, where free energies calculated using classical nucleation theory are expected to be the least accurate. There is strong evidence that H2SO 4, H2O, and NH3 are involved in atmospheric nucleation. These species are also principal components of atmospheric ions, suggesting that they may play important roles in ion-induced nucleation mechanisms. The purpose of this work is to measure thermodynamic parameters for cluster ions composed of NH3, H2SO4, and H2O. Equilibrium constants for the reactions of H2O and NH3 with the cluster ions, H+(H2SO4) s(H2O)w, HSO4(H 2SO4)s(H2O) w, and NH4+(NH3) n(H2SO4)s(H 2O)w, were measured using an ion flow reactor over a range of temperatures, and thermodynamic quantities (Δ H° and ΔS°) were derived from van't Hoff analyses. Ab initio structures were calculated to elucidate trends in ligand bonding. Current experimental results, combined with our previous measurements of H2SO4 bond enthalpies within cluster ions, are used to determine the nucleating ability of these systems for a range of atmospheric conditions. In general, nucleation of the negative cluster ions is predicted to be preferred over nucleation of positive ions in the atmosphere. For temperatures ≤250 K, relative humidities ≥50%, and H2SO4 concentrations ≥107 molecule cm−3 there is no thermodynamic barrier to nucleation of the HSO4(H2SO4) s(H2O)w system. Ammonia typically stabilizes H2SO4 within positive cluster ions due to formation of fully ionic crystalline-like clusters of the type NH 4+(NH4+HSO4)c, c = 1–3. However, nucleation barriers for the NH4+(NH 3)n(H2SO4) s(H2O)w system are strongly dependent on ambient NH3 concentrations, and positive ion nucleation in the atmosphere may actually be inhibited by the presence of low levels of NH3.
机译:当前的均相气相成核模型缺乏了解颗粒生长机理和准确预测大气中成核速率所必需的热力学数据。成核模型预测对粒子生长初始阶段的热力学高度敏感,其中使用经典成核理论计算的自由能预计最不准确。有强有力的证据表明H 2 SO 4 ,H 2 O和NH 3 参与了大气成核。这些物质也是大气离子的主要成分,表明它们可能在离子诱导的成核机制中发挥重要作用。这项工作的目的是测量由NH 3 ,H 2 SO 4 和H 2组成的簇离子的热力学参数 O。 H 2 O和NH 3 与簇离子H + (H 2 的反应的平衡常数SO 4 s (H 2 O) w ,HSO 4 - (H 2 SO 4 s (H 2 O) w 和NH 4 + (NH 3 n (H 2 SO 4 使用离子流反应器在一定范围内测量 s (H 2 O) w 的温度和热力学量(Δ H °和Δ S °)是根据van't Hoff分析得出的。计算了 Ab initio 结构,以阐明配​​体键合的趋势。当前的实验结果,结合我们先前对簇离子中H 2 SO 4 键焓的测量,可用于确定这些系统在一定范围的大气条件下的成核能力。通常,预计在大气中,负簇离子的成核比正离子的成核要好。对于温度≤250K,相对湿度≥50%和H 2 SO 4 浓度≥10 7 分子cm −3 < / super>对HSO 4 -(H 2 SO 4 )成核没有热力学障碍italic> s (H 2 O) w 系统。氨通常会由于形成正离子型NH 4 类型的完全离子晶体状簇而稳定正簇离子中的H 2 SO 4 + (NH 4 + HSO 4 - c = 1-3。但是,NH 4 + (NH 3 n ( H 2 SO 4 s (H 2 O) < sub> w 系统强烈依赖于环境NH 3 的浓度,而大气中正离子的成核作用实际上可能由于低含量的NH 的存在而受到抑制。 3

著录项

  • 作者

    Froyd, Karl David.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Chemistry Physical.; Geophysics.
  • 学位 Ph.D.
  • 年度 2002
  • 页码 p.2854
  • 总页数 312
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 物理化学(理论化学)、化学物理学;
  • 关键词

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