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: Peter, T., Zech, Roland, Suter, I., Anet, J. G.
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2014
Subjects:
Online Access:https://dx.doi.org/10.7892/boris.58526
http://boris.unibe.ch/58526/
id ftdatacite:10.7892/boris.58526
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spelling ftdatacite:10.7892/boris.58526 2023-05-15T13:54:54+02:00 Impact of geomagnetic excursions on atmospheric chemistry and dynamics Peter, T. Zech, Roland Suter, I. Anet, J. G. 2014 application/pdf https://dx.doi.org/10.7892/boris.58526 http://boris.unibe.ch/58526/ en eng Copernicus Publications info:eu-repo/semantics/openAccess 910 Geography & travel CreativeWork article 2014 ftdatacite https://doi.org/10.7892/boris.58526 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. Article in Journal/Newspaper Antarc* Antarctic Antarctica Arctic Geomagnetic Pole DataCite Metadata Store (German National Library of Science and Technology) Arctic Antarctic The Antarctic Austral
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic 910 Geography & travel
spellingShingle 910 Geography & travel
Peter, T.
Zech, Roland
Suter, I.
Anet, J. G.
Impact of geomagnetic excursions on atmospheric chemistry and dynamics
topic_facet 910 Geography & travel
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 Article in Journal/Newspaper
author Peter, T.
Zech, Roland
Suter, I.
Anet, J. G.
author_facet Peter, T.
Zech, Roland
Suter, I.
Anet, J. G.
author_sort Peter, T.
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 Publications
publishDate 2014
url https://dx.doi.org/10.7892/boris.58526
http://boris.unibe.ch/58526/
geographic Arctic
Antarctic
The Antarctic
Austral
geographic_facet Arctic
Antarctic
The Antarctic
Austral
genre Antarc*
Antarctic
Antarctica
Arctic
Geomagnetic Pole
genre_facet Antarc*
Antarctic
Antarctica
Arctic
Geomagnetic Pole
op_rights info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.7892/boris.58526
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