Carboxylic acids in gas and particulate phase above the Atlantic Ocean

被引:144
作者
Baboukas, ED [1 ]
Kanakidou, M [1 ]
Mihalopoulos, N [1 ]
机构
[1] Univ Crete, Dept Chem, Environm Chem Proc Lab, Iraklion 71409, Greece
关键词
D O I
10.1029/1999JD900977
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Mixing ratios of acetic (CH3COOH), formic (HCOOH), pyruvic (CH3COCOOH), and oxalic ((COOH)(2)) acids were measured both in gas and particulate phase in the marine boundary layer, over the Atlantic Ocean from 63 degrees N to 39 degrees S on board of the RN Polarstern in October/November 1996, The average mixing ratios for gas phase CH,COOH, HCOOH, CH3COCOOH, and (COOH)(2) were 291.2 +/- 151.9, 448.7 +/- 182.1, 1.1 +/- 1.0, and 6.1 +/- 5.4 parts per trillion by volume (pptv), respective ly. The partitioning of these acids in the aerosol phase and the size distribution of their particulate form was 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 acids were encountered in the southern hemisphere (springtime) compared to the northern hemisphere (autumn), indicating a possible seasonal variation in their 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 120 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 observed in the marine atmosphere. A local marine source of HCOOH of about 50 Tg/yr on a global scale is required to reasonably simulate the observations in the marine atmosphere.
引用
收藏
页码:14459 / 14471
页数:13
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