Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter
<p>Energetic particle precipitation (EPP) affects the chemistry of the polar middle atmosphere by producing reactive nitrogen (<span class="inline-formula">NO<sub><i>y</i></sub></span>) and hydrogen (<span class="inline-formula">HO&...
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doaj-4f54f2e13c0e466e9510908a47b5105e2020-11-25T00:32:39ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242019-07-01199485949410.5194/acp-19-9485-2019Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winterP. Arsenovic0P. Arsenovic1A. Damiani2E. Rozanov3E. Rozanov4E. Rozanov5B. Funke6A. Stenke7T. Peter8Institute for Atmospheric and Climate Science, ETH, Zürich, Switzerlandnow at: Air Pollution/Environmental Technology, Empa, Dübendorf, SwitzerlandCenter for Environmental Remote Sensing (CEReS), Chiba University, Chiba, JapanInstitute for Atmospheric and Climate Science, ETH, Zürich, SwitzerlandPhysikalisch-Meteorologisches Observatorium Davos – World Radiation Center, Davos, SwitzerlandPushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Kaliningrad, RussiaInstituto Astrofísica Andalucía, Consejo Superior de Investigaciones Científicas, Granada, SpainInstitute for Atmospheric and Climate Science, ETH, Zürich, SwitzerlandInstitute for Atmospheric and Climate Science, ETH, Zürich, Switzerland<p>Energetic particle precipitation (EPP) affects the chemistry of the polar middle atmosphere by producing reactive nitrogen (<span class="inline-formula">NO<sub><i>y</i></sub></span>) and hydrogen (<span class="inline-formula">HO<sub><i>x</i></sub></span>) species, which then catalytically destroy ozone. Recently, there have been major advances in constraining these particle impacts through a parametrization of <span class="inline-formula">NO<sub><i>y</i></sub></span> based on high-quality observations. Here we investigate the effects of low (auroral) and middle (radiation belt) energy range electrons, separately and in combination, on reactive nitrogen and hydrogen species as well as on ozone during Southern Hemisphere winters from 2002 to 2010 using the SOCOL3-MPIOM chemistry-climate model. Our results show that, in the absence of solar proton events, low-energy electrons produce the majority of <span class="inline-formula">NO<sub><i>y</i></sub></span> in the polar mesosphere and stratosphere. In the polar vortex, <span class="inline-formula">NO<sub><i>y</i></sub></span> subsides and affects ozone at lower altitudes, down to 10 hPa. Comparing a year with high electron precipitation with a quiescent period, we found large ozone depletion in the mesosphere; as the anomaly propagates downward, 15 % less ozone is found in the stratosphere during winter, which is confirmed by satellite observations. Only with both low- and middle-energy electrons does our model reproduce the observed stratospheric ozone anomaly.</p>https://www.atmos-chem-phys.net/19/9485/2019/acp-19-9485-2019.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
P. Arsenovic P. Arsenovic A. Damiani E. Rozanov E. Rozanov E. Rozanov B. Funke A. Stenke T. Peter |
spellingShingle |
P. Arsenovic P. Arsenovic A. Damiani E. Rozanov E. Rozanov E. Rozanov B. Funke A. Stenke T. Peter Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter Atmospheric Chemistry and Physics |
author_facet |
P. Arsenovic P. Arsenovic A. Damiani E. Rozanov E. Rozanov E. Rozanov B. Funke A. Stenke T. Peter |
author_sort |
P. Arsenovic |
title |
Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter |
title_short |
Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter |
title_full |
Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter |
title_fullStr |
Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter |
title_full_unstemmed |
Reactive nitrogen (NO<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during Southern Hemisphere winter |
title_sort |
reactive nitrogen (no<sub><i>y</i></sub>) and ozone responses to energetic electron precipitation during southern hemisphere winter |
publisher |
Copernicus Publications |
series |
Atmospheric Chemistry and Physics |
issn |
1680-7316 1680-7324 |
publishDate |
2019-07-01 |
description |
<p>Energetic particle precipitation (EPP) affects the
chemistry of the polar middle atmosphere by producing reactive nitrogen
(<span class="inline-formula">NO<sub><i>y</i></sub></span>) and hydrogen (<span class="inline-formula">HO<sub><i>x</i></sub></span>) species, which then catalytically destroy
ozone. Recently, there have been major advances in constraining these
particle impacts through a parametrization of <span class="inline-formula">NO<sub><i>y</i></sub></span> based on high-quality
observations. Here we investigate the effects of low (auroral) and middle
(radiation belt) energy range electrons, separately and in combination, on
reactive nitrogen and hydrogen species as well as on ozone during Southern
Hemisphere winters from 2002 to 2010 using the SOCOL3-MPIOM chemistry-climate model. Our results show that, in the absence of solar proton events, low-energy electrons produce the majority of <span class="inline-formula">NO<sub><i>y</i></sub></span> in the polar mesosphere
and stratosphere. In the polar vortex, <span class="inline-formula">NO<sub><i>y</i></sub></span> subsides and affects ozone
at lower altitudes, down to 10 hPa. Comparing a year with high electron
precipitation with a quiescent period, we found large ozone depletion in the
mesosphere; as the anomaly propagates downward, 15 % less ozone is found
in the stratosphere during winter, which is confirmed by satellite
observations. Only with both low- and middle-energy electrons does our model
reproduce the observed stratospheric ozone anomaly.</p> |
url |
https://www.atmos-chem-phys.net/19/9485/2019/acp-19-9485-2019.pdf |
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