Abstract
Over oceans and in coastal regions, methane sulfonic acid (MSA) is present in substantial concentrations in aerosols and in the gas phase. We present an investigation into the effect of MSA on sulfuric acid- and dimethyl amine (DMA)-based cluster formation rates. From systematic conformational scans and well-tested ab initio methods, we optimise the structures of all MSAx (H2SO4)yDMAz clusters where x +y ≤3 and z≤2. The resulting thermodynamic data are used in the Atmospheric Cluster Dynamics Code, and the effect of MSA is evaluated by comparing ternary MSA-H2SO4-DMA cluster formation rates to binary H2SO4-DMA cluster formation rates. Within the range of atmospherically relevant MSA concentrations, we find that MSA may increase cluster formation rates by up to 1 order of magnitude, although typically, the increase will be less than 300% at 258 K, less than 100% at 278K and less than 15% at 298 K. The results are rationalised by a detailed analysis of the main growth paths of the clusters. We find that MSA-enhanced clustering involves clusters containing one MSA molecule, while clusters containing more than one MSA molecule do not contribute significantly to the growth.
| Original language | Undefined/Unknown |
|---|---|
| Journal | Atmospheric Chemistry and Physics |
| Volume | 14 |
| Issue number | 22 |
| Pages (from-to) | 12023-12030 |
| Number of pages | 8 |
| ISSN | 1680-7316 |
| DOIs | |
| Publication status | Published - 2014 |