Carboxylic acids in gas and particulate phase above the Atlantic Ocean

Citation
Ed. Baboukas et al., Carboxylic acids in gas and particulate phase above the Atlantic Ocean, J GEO RES-A, 105(D11), 2000, pp. 14459-14471
Citations number
55
Categorie Soggetti
Earth Sciences
Volume
105
Issue
D11
Year of publication
2000
Pages
14459 - 14471
Database
ISI
SICI code
Abstract
Mixing ratios of acetic (CH3COOH), formic (HCOOH), pyruvic (CH3COCOOH), and oxalic ((COOH)(2)) acids were measured both in gas and particulate phase i n the marine boundary layer, over the Atlantic Ocean from 63 degrees N to 3 9 degrees S on board of the RN Polarstern in October/November 1996, The ave rage mixing ratios for gas phase CH,COOH, HCOOH, CH3COCOOH, and (COOH)(2) w ere 291.2 +/- 151.9, 448.7 +/- 182.1, 1.1 +/- 1.0, and 6.1 +/- 5.4 parts pe r trillion by volume (pptv), respective ly. The partitioning of these acids in the aerosol phase and the size distribution of their particulate form w as also investigated. In the fine mode the mean mixing ratios for acetate, formate, pyruvate, and oxalate were 69.7 +/- 47.5, 32.5 +/- 39.4, 1.0 +/- 1 .0, and 5.1 +/- 3.7 pptv, respectively. Elevated levels of all organic acid s were encountered in the southern hemisphere (springtime) compared to the northern hemisphere (autumn), indicating a possible seasonal variation in t heir source strength and/or enhanced photochemical production. The observed distributions of formic and acetic acids have been compared to the results of a global chemistry/transport three-dimensional model. The model results show that acetic acid has mainly secondary photochemical sources (about 12 0 Tg CH3COOH/yr). On the opposite, the known chemical sources of HCOOH are quite weak (20 Tg HCOOH/yr) and insufficient to simulate the HCOOH levels o bserved in the marine atmosphere. A local marine source of HCOOH of about 5 0 Tg/yr on a global scale is required to reasonably simulate the observatio ns in the marine atmosphere.