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OH in the tropical upper troposphere and its relationships to solar radiation and reactive nitrogen
Authors:R S Gao  K H Rosenlof  D W Fahey  P O Wennberg  E J Hintsa  T F Hanisco
Institution:1. Chemical Sciences Division, Earth System Research Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, 80305, USA
2. Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, 80309, USA
3. Divisions of Geological and Planetary Sciences and Engineering and Applied Science, California Institute of Technology, Pasadena, CA, 91125, USA
4. Global Monitoring Division, Earth System Research Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, 80305, USA
5. Goddard Space Flight Center, National Aeronautics and Space Administration, Greenbelt, MD, USA
Abstract:In situ measurements of OH], HO2] (square brackets denote species concentrations), and other chemical species were made in the tropical upper troposphere (TUT). OH] showed a robust correlation with solar zenith angle. Beyond this dependence, however, OH] did not correlate to its primary source, the product of O3] and H2O] (O3]?H2O]), or its sink NOy]. This suggests that OH] is heavily buffered in the TUT. One important exception to this result is found in regions with very low O3], NO], and NOy]. Under these conditions, OH] is highly suppressed, pointing to the critical role of NO in sustaining OH in the TUT and the possibility of low OH] over the western Pacific warm pool due to strong marine convections bringing NO-poor air to the TUT. In contrast to OH], HOx] (OH] + HO2]) correlated reasonably well with O3]?H2O]/NOy], suggesting that O3]?H2O] and NOy] are the significant source and sink, respectively, of HOx].
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