Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions
The short-living cosmogenic isotope 7 Be, which is produced by cosmic rays in the atmosphere, is often used as a tracer for atmospheric dynamics, with precise and high-resolution measurements covering the recent decades. The long-living isotope 10 Be, as measured in polar ice cores with an annual re...
Published in: | Geoscientific Model Development |
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2021
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Online Access: | https://doi.org/10.5194/gmd-14-7605-2021 https://gmd.copernicus.org/articles/14/7605/2021/ |
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Copernicus Publications: E-Journals |
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English |
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The short-living cosmogenic isotope 7 Be, which is produced by cosmic rays in the atmosphere, is often used as a tracer for atmospheric dynamics, with precise and high-resolution measurements covering the recent decades. The long-living isotope 10 Be, as measured in polar ice cores with an annual resolution, is a proxy for long-term cosmic-ray variability, whose signal can, however, be distorted by atmospheric transport and deposition that need to be properly modeled to be accounted for. While transport of 7 Be can be modeled with high accuracy using the known meteorological fields, atmospheric transport of 10 Be was typically modeled using case-study-specific simulations or simplified box models based on parameterizations. Thus, there is a need for a realistic model able to simulate atmospheric transport and deposition of beryllium with a focus on polar regions and (inter)annual timescales that is potentially able to operate in a self-consistent mode without the prescribed meteorology. Since measurements of 10 Be are extremely laborious and hence scarce, it is difficult to compare model results directly with measurement data. On the other hand, the two beryllium isotopes are believed to have similar transport and deposition properties, being different only in production and lifetime, and thus the results of 7 Be transport can be generally applied to 10 Be. Here we present a new model, called CCM SOCOL-AERv2-BE, to trace isotopes of 7 Be and 10 Be in the atmosphere based on the chemistry–climate model (CCM) SOCOL (SOlar Climate Ozone Links), which has been improved by including modules for the production, deposition, and transport of 7 Be and 10 Be. Production of the isotopes was modeled for both galactic and solar cosmic rays by applying the CRAC (Cosmic Ray Atmospheric Cascade) model. Transport of 7 Be was modeled without additional gravitational settling due to the submicron size of the background aerosol particles. An interactive deposition scheme was applied including both wet and dry deposition. Modeling was performed using a full nudging to the meteorological fields for the period of 2002–2008 with a spin-up period of 1996–2001. The modeled concentrations of 7 Be in near-ground air were compared with the measured ones at a weekly time resolution in four nearly antipodal high-latitude locations: two in the Northern (Finland and Canada) and two in the Southern (Chile and the Kerguelen Islands) Hemisphere. The model results agree with the measurements in the absolute level within error bars, implying that the production, decay, and lateral deposition are correctly reproduced. The model also correctly reproduces the temporal variability of 7 Be concentrations on annual and sub-annual scales, including the presence and absence of the annual cycle in the Northern and Southern Hemisphere, respectively. We also modeled the production and transport of 7 Be for a major solar energetic particle event (SPE) on 20 January 2005, which appears insufficient to produce a measurable signal but may serve as a reference event for historically known extreme SPEs. Thus, a new full 3D time-dependent model, based on CCM SOCOL, of 7 Be and 10 Be atmospheric production, transport, and deposition has been developed. Comparison with real data on the 7 Be concentration in the near-ground air validates the model and its accuracy. |
format |
Text |
author |
Golubenko, Kseniia Rozanov, Eugene Kovaltsov, Gennady Leppänen, Ari-Pekka Sukhodolov, Timofei Usoskin, Ilya |
spellingShingle |
Golubenko, Kseniia Rozanov, Eugene Kovaltsov, Gennady Leppänen, Ari-Pekka Sukhodolov, Timofei Usoskin, Ilya Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
author_facet |
Golubenko, Kseniia Rozanov, Eugene Kovaltsov, Gennady Leppänen, Ari-Pekka Sukhodolov, Timofei Usoskin, Ilya |
author_sort |
Golubenko, Kseniia |
title |
Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
title_short |
Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
title_full |
Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
title_fullStr |
Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
title_full_unstemmed |
Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions |
title_sort |
application of ccm socol-aerv2-be to cosmogenic beryllium isotopes: description and validation for polar regions |
publishDate |
2021 |
url |
https://doi.org/10.5194/gmd-14-7605-2021 https://gmd.copernicus.org/articles/14/7605/2021/ |
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Canada Kerguelen Kerguelen Islands |
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Canada Kerguelen Kerguelen Islands |
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Kerguelen Islands Northern Finland |
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Kerguelen Islands Northern Finland |
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eISSN: 1991-9603 |
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doi:10.5194/gmd-14-7605-2021 https://gmd.copernicus.org/articles/14/7605/2021/ |
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https://doi.org/10.5194/gmd-14-7605-2021 |
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Geoscientific Model Development |
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7605 |
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7620 |
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ftcopernicus:oai:publications.copernicus.org:gmd93174 2023-05-15T17:02:10+02:00 Application of CCM SOCOL-AERv2-BE to cosmogenic beryllium isotopes: description and validation for polar regions Golubenko, Kseniia Rozanov, Eugene Kovaltsov, Gennady Leppänen, Ari-Pekka Sukhodolov, Timofei Usoskin, Ilya 2021-12-16 application/pdf https://doi.org/10.5194/gmd-14-7605-2021 https://gmd.copernicus.org/articles/14/7605/2021/ eng eng doi:10.5194/gmd-14-7605-2021 https://gmd.copernicus.org/articles/14/7605/2021/ eISSN: 1991-9603 Text 2021 ftcopernicus https://doi.org/10.5194/gmd-14-7605-2021 2021-12-20T17:22:29Z The short-living cosmogenic isotope 7 Be, which is produced by cosmic rays in the atmosphere, is often used as a tracer for atmospheric dynamics, with precise and high-resolution measurements covering the recent decades. The long-living isotope 10 Be, as measured in polar ice cores with an annual resolution, is a proxy for long-term cosmic-ray variability, whose signal can, however, be distorted by atmospheric transport and deposition that need to be properly modeled to be accounted for. While transport of 7 Be can be modeled with high accuracy using the known meteorological fields, atmospheric transport of 10 Be was typically modeled using case-study-specific simulations or simplified box models based on parameterizations. Thus, there is a need for a realistic model able to simulate atmospheric transport and deposition of beryllium with a focus on polar regions and (inter)annual timescales that is potentially able to operate in a self-consistent mode without the prescribed meteorology. Since measurements of 10 Be are extremely laborious and hence scarce, it is difficult to compare model results directly with measurement data. On the other hand, the two beryllium isotopes are believed to have similar transport and deposition properties, being different only in production and lifetime, and thus the results of 7 Be transport can be generally applied to 10 Be. Here we present a new model, called CCM SOCOL-AERv2-BE, to trace isotopes of 7 Be and 10 Be in the atmosphere based on the chemistry–climate model (CCM) SOCOL (SOlar Climate Ozone Links), which has been improved by including modules for the production, deposition, and transport of 7 Be and 10 Be. Production of the isotopes was modeled for both galactic and solar cosmic rays by applying the CRAC (Cosmic Ray Atmospheric Cascade) model. Transport of 7 Be was modeled without additional gravitational settling due to the submicron size of the background aerosol particles. An interactive deposition scheme was applied including both wet and dry deposition. Modeling was performed using a full nudging to the meteorological fields for the period of 2002–2008 with a spin-up period of 1996–2001. The modeled concentrations of 7 Be in near-ground air were compared with the measured ones at a weekly time resolution in four nearly antipodal high-latitude locations: two in the Northern (Finland and Canada) and two in the Southern (Chile and the Kerguelen Islands) Hemisphere. The model results agree with the measurements in the absolute level within error bars, implying that the production, decay, and lateral deposition are correctly reproduced. The model also correctly reproduces the temporal variability of 7 Be concentrations on annual and sub-annual scales, including the presence and absence of the annual cycle in the Northern and Southern Hemisphere, respectively. We also modeled the production and transport of 7 Be for a major solar energetic particle event (SPE) on 20 January 2005, which appears insufficient to produce a measurable signal but may serve as a reference event for historically known extreme SPEs. Thus, a new full 3D time-dependent model, based on CCM SOCOL, of 7 Be and 10 Be atmospheric production, transport, and deposition has been developed. Comparison with real data on the 7 Be concentration in the near-ground air validates the model and its accuracy. Text Kerguelen Islands Northern Finland Copernicus Publications: E-Journals Canada Kerguelen Kerguelen Islands Geoscientific Model Development 14 12 7605 7620 |