Abstract

Abstract. Satellite observations show that the enormous solar proton events (SPEs) in October–November 2003 had significant effects on the composition of the stratosphere and mesosphere in the polar regions. After the October–November 2003 SPEs and in early 2004, significant enhancements of NOx(=NO+NO2) in the upper stratosphere and lower mesosphere in the Northern Hemisphere were observed by several satellite instruments. Here we present global full chemistry calculations performed with the CLaMS model to study the impact of mesospheric NOx intrusions on Arctic polar ozone loss processes in the stratosphere. Several model simulations are preformed with different upper boundary conditions for NOx at 2000 K potential temperature (≈50 km altitude). In our study we focus on the impact of the non-local production of NOx, which means the downward transport of enhanced NOx from the mesosphere to the stratosphere. The local production of NOx in the stratosphere is neglected. Our findings show that intrusions of mesospheric air into the stratosphere, transporting high burdens of NOx, affect the composition of the Arctic polar region down to about 400 K (≈17–18 km). We compare our simulated NOx and O3 mixing ratios with satellite observations by ACE-FTS and MIPAS processed at IMK/IAA and derive an upper limit for the ozone loss caused by enhanced mesospheric NOx. Our findings show that in the Arctic polar vortex (equivalent lat.>70° N) the accumulated column ozone loss between 350–2000 K potential temperature (≈14–50 km altitude) caused by the SPEs in October–November 2003 in the stratosphere is up to 3.3 DU with an upper limit of 5.5 DU until end of November. Further, we found that about 10 DU, but in any case lower than 18 DU, accumulated ozone loss additionally occurred until end of March 2004 caused by the transport of mesospheric NOx-rich air in early 2004. The solar-proton-produced NOx above 55 km due to the SPEs of October–November 2003 had a negligibly small impact on ozone loss processes through the end of November in the lower stratosphere (350–700 K≈14–27 km). The mesospheric NOx intrusions in early 2004 yielded a lower stratospheric ozone loss of about 3.5 DU, and clearly lower than 6.5 DU through the end of March. Overall, the non-local production of NOx is an additional variability in the existing variations of the ozone loss observed in the Arctic.

Highlights

  • During periods of solar disturbances solar events can affect the concentration of constituents in the middle atmosphere

  • To compare our simulated NOx mixing ratios with satellite observations conducted by MIPAS and Atmospheric Chemistry Experiment (ACE)-FTS (V2.2) the model results were interpolated to the locations of the observations

  • Upper boundary conditions were taken from the results of a long-term simulation conducted with KASIMA, where increased NOx concentration in the mesosphere was derived from MIPAS measurements www.atmos-chem-phys.net/8/5279/2008/

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Summary

Introduction

During periods of solar disturbances solar events can affect the concentration of constituents in the middle atmosphere. The temperatures in the lower stratosphere were unusually high and temperatures in the middle and upper stratosphere were unusually low during and after February 2004 These dynamic disturbances supported the downward transport of NOx leading to the NOx enhancements in the upper stratosphere in early 2004. In addition to this downward transport of NOx in the lower stratosphere, dynamic disturbances of the vortex yielded enhanced meridional transport of NOx-rich and O3-rich air masses from the subtropics into the polar regions in the lower stratosphere This effect was discussed by Konopka et al (2007a) for the winter 2002/2003. They found that the enhanced meridional transport of NOx caused ozone loss that can outweigh the halogen-induced ozone loss processes occurring in winter and early spring in the Arctic lower and middle stratosphere. LopezPuertas et al, 2005b) due to the local production of NOx are not considered

The model study
Model results
NOx mixing ratios
O3 mixing ratios
Ozone loss
Findings
Summary and conclusions
Full Text
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