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New parameterization of sulfuric acid-ammonia-water ternary nucleation rates at tropospheric conditions

机译:对流层条件下硫酸-氨-水三元成核速率的新参数化

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Recently, the classical theory of sulfuric acid-ammonia-water (H2SO4-NH3-H2O) nucleation was reinvestigated by including the effect of stable ammonium bisulfate formation into calculations. The predicted nucleation rates lowered by many orders of magnitude, bringing them close to agreement with the available experiments on H2SO4-NH3-H2O nucleation. However, because of complex thermodynamics involved, the theoretical calculations of nucleation rates are computationally demanding, and sometimes the theory breaks down at specific concentrations and temperatures. Here we present parameterized equations of ternary H2SO4-NH3-H2O nucleation rates, critical cluster sizes, and critical cluster compositions. Our parameterizations reduce the computing time of these values by a factor of 105 compared with the calculations with the full thermodynamic model. Also, our parameterizations provide reliable estimates for ternary nucleation rates in cases when the full theory fails in isolated points of the parameter space. The parameterized nucleation rates are accurate to one order of magnitude in nucleation rate. Because of their computational efficiency, our parameterizations are particularly suitable for large-scale models of atmosphere. They are valid for temperatures above 235 K, sulfuric acid concentrations 5 · 104–109 cm?3, ammonia mixing ratios 0.1–1000 ppt, relative humidities 5%–95%, and nucleation rates over 10?5 cm?3 s?1. At these conditions, no significant nucleation occurs above 295 K.
机译:最近,通过将稳定的硫酸氢铵形成的影响纳入计算中,重新研究了硫酸-氨-水(H2SO4-NH3-H2O)成核的经典理论。预测的成核速率降低了多个数量级,使其与H2SO4-NH3-H2O成核的可用实验接近。然而,由于涉及复杂的热力学,成核速率的理论计算需要计算量,有时该理论在特定的浓度和温度下会失效。在这里,我们介绍三元H2SO4-NH3-H2O成核速率,临界团簇尺寸和临界团簇组成的参数化方程式。与完整热力学模型的计算相比,我们的参数化将这些值的计算时间减少了105倍。同样,当整个理论在参数空间的孤立点中失败时,我们的参数化也可提供三元成核速率的可靠估计。参数化的成核速率精确到成核速率的一个数量级。由于它们的计算效率,我们的参数化特别适合大型大气模型。它们适用于温度超过235 K,硫酸浓度5·104–109 cm?3,氨混合比0.1–1000 ppt,相对湿度5%–95%和成核速率超过10?5 cm?3 s?1的情况。 。在这些条件下,高于295 K不会发生明显的成核。

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