Abstract

Abstract. We present altitude-dependent lifetimes of NOx, determined with MIPAS/ENVISAT (the Michelson Interferometer for Passive Atmospheric Sounding/the European Environment Satellite), for the Southern polar region after the solar proton event in October–November 2003. Between 50° S and 90° S and decreasing in altitude they range from about two days at 64 km to about 20 days at 44 km. The lifetimes are controlled by transport, mixing and photochemistry. We infer estimates of dynamical lifetimes by comparison of the observed decay to photochemical lifetimes calculated with the SLIMCAT 3-D Model. Photochemical loss contributes to the observed NOx depletion by 0.1% at 44 km, increasing with altitude to 45% at 64 km. In addition, we show the correlation of modelled ionization rates and observed NOx densities under consideration of the determined lifetimes of NOx, and calculate altitude-dependent effective production rates of NOx due to ionization. For that we compare ionization rates of the AIMOS data base with the MIPAS measurements from 15 October–31 December 2003. We derive effective NOx-production rates to be applied to the AIMOS ionization rates which range from about 0.2 NOx-molecules per ion pair at 44 km to 0.7 NOx-molecules per ion pair at 62 km. These effective production rates are considerably lower than predicted by box model simulations which could hint at an overestimation of the modelled ionization rates.

Highlights

  • Used dataWe describe the data used for this study. Mixing ratios of NO and NO2 are retrieved from spectra of MIPAS (Sect. 2.1) and the 3-D model Atmospheric Ionization Module Osnabruck (AIMOS) is used to get ionization rates (Sect. 2.2)

  • We show the correlation of modelled ioniza- geomagnetic field, forcing precipitation of low energetic partion rates and observed NOx densities under consideration of the determined lifetimes of NOx, and calculate altitudedependent effective production rates of NOx due to ionization

  • We showed a simple method to derive lifetimes of NOx after a solar proton event by means of MIPAS/Environment Satellite (ENVISAT) measurements

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Summary

Used data

We describe the data used for this study. Mixing ratios of NO and NO2 are retrieved from spectra of MIPAS (Sect. 2.1) and the 3-D model AIMOS is used to get ionization rates (Sect. 2.2). We use NOx-data of the nominal measurement mode (Funke et al, 2005a), which covers altitudes from 6–68 km. The standard error of the mean is dependent on the number of geolocations and bigger during the SPE but mostly lower than 10 %. The 24-h zonal means of the NOx number density we use in Sect. The Atmospheric Ionization Module Osnabruck, (AIMOS, Wissing and Kallenrode, 2009) is a 3-D model, which determines the atmospheric ionization caused by protons, electrons, and alpha particles It is based on flux measurements of GOES (Geostationary Operational Environmental Satellite) and POES (Polar Operational Environmental Satellite) covering an energy range of 150 eV to 500 MeV for protons, 4 MeV to 500 MeV for alpha particles, and 150 eV to 2.5 MeV for electrons.

Lifetime of NOx
Dependence of NOx on ion pair production
Comparison with previous model studies
Findings
Conclusions
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