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Detailed Reference Information |
Chen, G., Davis, D., Crawford, J., Nowak, J.B., Eisele, F., Mauldin, R.L., Tanner, D., Buhr, M., Shetter, R., Lefer, B., Arimoto, R., Hogan, A. and Blake, D. (2001). An investigation of South Pole HOx chemistry: Comparison of model results with ISCAT observations. Geophysical Research Letters 28: doi: 10.1029/2001GL013158. issn: 0094-8276. |
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Unexpected high levels of OH and NO were recorded at the South Pole (SP) Atmospheric Research Observatory during the 1998--99 ISCAT field study. Model simulations suggest a major photochemical linkage between observed OH and NO. A detailed comparison of the observations with model predictions revealed good agreement for OH at NO levels between 120 and 380 pptv. However, the model tended to overestimate OH for NO levels 380 pptv. The reasons for these deviations appear not to involve NO directly but rather HOx radical scavenging for the low NO conditions and additional HOx sources for the high NO conditions. Because of the elevated levels of NO and highly activated HOx photochemistry, the SP was found to be a strong net source of surface ozone. It is quite likely that the strong oxidizing environment found at the South Pole extends over the entire polar plateau. ¿ 2001 American Geophysical Union |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Atmospheric Composition and Structure, Atmospheric Composition and Structure, Biosphere/atmosphere interactions, Atmospheric Composition and Structure, Constituent sources and sinks, Atmospheric Composition and Structure, Troposphere—composition and chemistry |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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