Vertical distribution of mercury, CO, ozone, and aerosol scattering coefficient in the Pacific Northwest during the spring 2006 INTEX-B campaign

被引:37
作者
Swartzendruber, P. C. [1 ]
Chand, D. [1 ]
Jaffe, D. A. [1 ]
Smith, J. [3 ]
Reidmiller, D. [1 ]
Gratz, L. [2 ]
Keeler, J. [2 ]
Strode, S. [1 ]
Jaegle, L. [1 ]
Talbot, R. [4 ]
机构
[1] Univ Washington, Dept Atmospher Sci, Seattle, WA 98195 USA
[2] Univ Michigan, Air Qual Lab, Ann Arbor, MI 48109 USA
[3] Univ Washington, Interdisciplinary Arts & Sci, Bothell, WA 98011 USA
[4] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA
关键词
D O I
10.1029/2007JD009579
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
In the spring of 2006, we measured the vertical distribution of gaseous elemental mercury (GEM), CO, ozone, and aerosol scattering coefficient in the Pacific Northwest concurrent with NASA's INTEX-B campaign. Seven profiles from the surface to 6 km were conducted from 12 April to 8 May along with one flight in the Seattle-Tacoma boundary layer. Ozone had a bimodal distribution with the lower mode occurring primarily in the mixed layer and the higher mode occurring in the free troposphere. In the free troposphere, the mixing ratios (1 - sigma) of GEM, CO, ozone, and aerosol scattering coefficient were 1.52 (0.165) ng/m(3), 142 (14.9) ppbv, 78 (7.7) ppbv, and 3.0 (1.8) Mm(-1), respectively. GEM and CO were correlated in the high ozone mode (r(2) = 0.30) but were uncorrelated in the lower mode (r(2) = 0.05). Three flights observed enhancements of GEM and CO with good correlations and with regression slopes (0.0067 (+/- 0.0027) ng/m(3)/ppbv by ordinary least squares regression and 0.0097 (+/- 0.0018) ng/m(3)/ppbv by reduced major axis regression) slightly higher than previous observations of enhancements due to Asian industrial long-range transport (LRT). The influence of Asian LRT is supported by back trajectories and a global chemical transport model. In the Seattle-Tacoma boundary layer flight, CO was uncorrelated with GEM, which reflects relatively weaker local GEM sources. On three flights, pockets of air were observed with strong inverse GEM-ozone and ozone-CO correlations (in contrast to all data), which is evidence of upper tropospheric/lower stratospheric (UTLS) influence. An extrapolation of the GEM-CO and GEM-ozone slopes suggests the UTLS can be depleted of GEM.
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