Impact of geomagnetic excursions on atmospheric chemistry and dynamics

Geomagnetic excursions, i.e. short periods in time with much weaker geomagnetic fields and substantial changes in the position of the geomagnetic pole, occurred repeatedly in the Earth's history, e.g. the Laschamp event about 41 kyr ago. Although the next such excursion is certain to come, litt...

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Main Authors: Suter, I., Zech, R., Anet, J. G., Peter, T.
Format: Text
Language:English
Published: Copernicus 2014
Subjects:
Online Access:https://dx.doi.org/10.21256/zhaw-4654
https://digitalcollection.zhaw.ch/handle/11475/8911
id ftdatacite:10.21256/zhaw-4654
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spelling ftdatacite:10.21256/zhaw-4654 2023-05-15T13:55:24+02:00 Impact of geomagnetic excursions on atmospheric chemistry and dynamics Suter, I. Zech, R. Anet, J. G. Peter, T. 2014 application/pdf https://dx.doi.org/10.21256/zhaw-4654 https://digitalcollection.zhaw.ch/handle/11475/8911 en eng Copernicus Creative Commons Attribution 3.0 Unported https://creativecommons.org/licenses/by/3.0/legalcode cc-by-3.0 CC-BY 500 Naturwissenschaften und Mathematik Text article-journal Journal Article ScholarlyArticle 2014 ftdatacite https://doi.org/10.21256/zhaw-4654 2021-11-05T12:55:41Z Geomagnetic excursions, i.e. short periods in time with much weaker geomagnetic fields and substantial changes in the position of the geomagnetic pole, occurred repeatedly in the Earth's history, e.g. the Laschamp event about 41 kyr ago. Although the next such excursion is certain to come, little is known about the timing and possible consequences for the state of the atmosphere and the ecosystems. Here we use the global chemistry climate model SOCOL-MPIOM to simulate the effects of geomagnetic excursions on atmospheric ionization, chemistry and dynamics. Our simulations show significantly increased concentrations of nitrogen oxides (NOx) in the entire stratosphere, especially over Antarctica (+15%), due to enhanced ionization by galactic cosmic rays. Hydrogen oxides (HOx) are also produced in greater amounts (up to +40%) in the tropical and subtropical lower stratosphere, while their destruction by reactions with enhanced NOx prevails over the poles and in high altitudes (by -5%). Stratospheric ozone concentrations decrease globally above 20 km by 1-2% and at the northern hemispheric tropopause by up to 5% owing to the accelerated NOx-induced destruction. A 5% increase is found in the southern lower stratosphere and troposphere. In response to these changes in ozone and the concomitant changes in atmospheric heating rates, the Arctic vortex intensifies in boreal winter, while the Antarctic vortex weakens in austral winter and spring. Surface wind anomalies show significant intensification of the southern westerlies at their poleward edge during austral winter and a pronounced northward shift in spring. Major impacts on the global climate seem unlikely. Text Antarc* Antarctic Antarctica Arctic Geomagnetic Pole DataCite Metadata Store (German National Library of Science and Technology) Antarctic Arctic Austral The Antarctic
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic 500 Naturwissenschaften und Mathematik
spellingShingle 500 Naturwissenschaften und Mathematik
Suter, I.
Zech, R.
Anet, J. G.
Peter, T.
Impact of geomagnetic excursions on atmospheric chemistry and dynamics
topic_facet 500 Naturwissenschaften und Mathematik
description Geomagnetic excursions, i.e. short periods in time with much weaker geomagnetic fields and substantial changes in the position of the geomagnetic pole, occurred repeatedly in the Earth's history, e.g. the Laschamp event about 41 kyr ago. Although the next such excursion is certain to come, little is known about the timing and possible consequences for the state of the atmosphere and the ecosystems. Here we use the global chemistry climate model SOCOL-MPIOM to simulate the effects of geomagnetic excursions on atmospheric ionization, chemistry and dynamics. Our simulations show significantly increased concentrations of nitrogen oxides (NOx) in the entire stratosphere, especially over Antarctica (+15%), due to enhanced ionization by galactic cosmic rays. Hydrogen oxides (HOx) are also produced in greater amounts (up to +40%) in the tropical and subtropical lower stratosphere, while their destruction by reactions with enhanced NOx prevails over the poles and in high altitudes (by -5%). Stratospheric ozone concentrations decrease globally above 20 km by 1-2% and at the northern hemispheric tropopause by up to 5% owing to the accelerated NOx-induced destruction. A 5% increase is found in the southern lower stratosphere and troposphere. In response to these changes in ozone and the concomitant changes in atmospheric heating rates, the Arctic vortex intensifies in boreal winter, while the Antarctic vortex weakens in austral winter and spring. Surface wind anomalies show significant intensification of the southern westerlies at their poleward edge during austral winter and a pronounced northward shift in spring. Major impacts on the global climate seem unlikely.
format Text
author Suter, I.
Zech, R.
Anet, J. G.
Peter, T.
author_facet Suter, I.
Zech, R.
Anet, J. G.
Peter, T.
author_sort Suter, I.
title Impact of geomagnetic excursions on atmospheric chemistry and dynamics
title_short Impact of geomagnetic excursions on atmospheric chemistry and dynamics
title_full Impact of geomagnetic excursions on atmospheric chemistry and dynamics
title_fullStr Impact of geomagnetic excursions on atmospheric chemistry and dynamics
title_full_unstemmed Impact of geomagnetic excursions on atmospheric chemistry and dynamics
title_sort impact of geomagnetic excursions on atmospheric chemistry and dynamics
publisher Copernicus
publishDate 2014
url https://dx.doi.org/10.21256/zhaw-4654
https://digitalcollection.zhaw.ch/handle/11475/8911
geographic Antarctic
Arctic
Austral
The Antarctic
geographic_facet Antarctic
Arctic
Austral
The Antarctic
genre Antarc*
Antarctic
Antarctica
Arctic
Geomagnetic Pole
genre_facet Antarc*
Antarctic
Antarctica
Arctic
Geomagnetic Pole
op_rights Creative Commons Attribution 3.0 Unported
https://creativecommons.org/licenses/by/3.0/legalcode
cc-by-3.0
op_rightsnorm CC-BY
op_doi https://doi.org/10.21256/zhaw-4654
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