Middle Atmosphere NOx variations and solar UV VAriability: Examples to study mesospheric/stratospheric coupling and the impact of solar variability on stratospheric ozone
Final Report 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 performed with different upper boundary conditions for NOx at 2000K potential temperature (circa 50 km altitude). In our study we focussed 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 (circa 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 (circa 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 (350-700K circa 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.
Publications
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Model simulations of stratospheric ozone loss caused by enhanced mesospheric NOx during Arctic Winter 2003/2004 Atmospheric chemistry and Physics, Vol. 8.2008, Issue 17. pp. 5279-5293.
Vogel, B., Konopka, P., Grooß, J. U., Müller, R., Funke, M., Lopez-Puertas, M., Reddmann, T., Stiller, G., von Clarmann, T., Riese, M.
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The influence of energetic particles on the chemistry of the middle atmosphere. In: Climate And Weather of the Sun-Earth (CAWSES): Highlights from a priority program, ed.: F.-J. Lübken, (Springer Atmospheric Sciences), 2013, pp 247-273, ISBN 978-94-007-4347-2.
Reddmann, T., Funke, B., Konopka, P., Stiller, G., Versick, S., Vogel, B.
