Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003

We present altitude-dependent lifetimes of NO<sub>x</sub>, 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&...

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Main Authors: F. Friederich, T. von Clarmann, B. Funke, H. Nieder, J. Orphal, M. Sinnhuber, G. P. Stiller, J. M. Wissing
Format: Article
Language:English
Published: Copernicus Publications 2013-03-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/13/2531/2013/acp-13-2531-2013.pdf
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spelling doaj-7bd2e66d86d3425e9224e6d4b2e6a2b72020-11-24T23:16:53ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242013-03-011352531253910.5194/acp-13-2531-2013Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003F. FriederichT. von ClarmannB. FunkeH. NiederJ. OrphalM. SinnhuberG. P. StillerJ. M. WissingWe present altitude-dependent lifetimes of NO<sub>x</sub>, 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&deg; S and 90&deg; 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 NO<sub>x</sub> depletion by 0.1% at 44 km, increasing with altitude to 45% at 64 km. <br><br> In addition, we show the correlation of modelled ionization rates and observed NO<sub>x</sub> densities under consideration of the determined lifetimes of NO<sub>x</sub>, and calculate altitude-dependent effective production rates of NO<sub>x</sub> 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 NO<sub>x</sub>-production rates to be applied to the AIMOS ionization rates which range from about 0.2 NO<sub>x</sub>-molecules per ion pair at 44 km to 0.7 NO<sub>x</sub>-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.http://www.atmos-chem-phys.net/13/2531/2013/acp-13-2531-2013.pdf
collection DOAJ
language English
format Article
sources DOAJ
author F. Friederich
T. von Clarmann
B. Funke
H. Nieder
J. Orphal
M. Sinnhuber
G. P. Stiller
J. M. Wissing
spellingShingle F. Friederich
T. von Clarmann
B. Funke
H. Nieder
J. Orphal
M. Sinnhuber
G. P. Stiller
J. M. Wissing
Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
Atmospheric Chemistry and Physics
author_facet F. Friederich
T. von Clarmann
B. Funke
H. Nieder
J. Orphal
M. Sinnhuber
G. P. Stiller
J. M. Wissing
author_sort F. Friederich
title Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
title_short Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
title_full Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
title_fullStr Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
title_full_unstemmed Lifetime and production rate of NO<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in October&ndash;November 2003
title_sort lifetime and production rate of no<sub>x</sub> in the upper stratosphere and lower mesosphere in the polar spring/summer after the solar proton event in october&ndash;november 2003
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2013-03-01
description We present altitude-dependent lifetimes of NO<sub>x</sub>, 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&deg; S and 90&deg; 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 NO<sub>x</sub> depletion by 0.1% at 44 km, increasing with altitude to 45% at 64 km. <br><br> In addition, we show the correlation of modelled ionization rates and observed NO<sub>x</sub> densities under consideration of the determined lifetimes of NO<sub>x</sub>, and calculate altitude-dependent effective production rates of NO<sub>x</sub> 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 NO<sub>x</sub>-production rates to be applied to the AIMOS ionization rates which range from about 0.2 NO<sub>x</sub>-molecules per ion pair at 44 km to 0.7 NO<sub>x</sub>-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.
url http://www.atmos-chem-phys.net/13/2531/2013/acp-13-2531-2013.pdf
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