The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment

The diurnal atmospheric boundary layer evolution of the <sup>222</sup>Rn decaying family is studied using a state-of-the-art large-eddy simulation model. In particular, a diurnal cycle observed during the Wangara experiment is successfully simulated together with the effect of diurnal va...

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Main Authors: S. Galmarini, S. Basu, J.-F. Vinuesa
Format: Article
Language:English
Published: Copernicus Publications 2007-09-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/7/5003/2007/acp-7-5003-2007.pdf
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spelling doaj-b9960466ebf14af6844ae3b73fe462b12020-11-24T21:35:28ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242007-09-0171850035019The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experimentS. GalmariniS. BasuJ.-F. VinuesaThe diurnal atmospheric boundary layer evolution of the <sup>222</sup>Rn decaying family is studied using a state-of-the-art large-eddy simulation model. In particular, a diurnal cycle observed during the Wangara experiment is successfully simulated together with the effect of diurnal varying turbulent characteristics on radioactive compounds initially in a secular equilibrium. This study allows us to clearly analyze and identify the boundary layer processes driving the behaviour of <sup>222</sup>Rn and its progeny concentrations. An activity disequilibrium is observed in the nocturnal boundary layer due to the proximity of the radon source and the trapping of fresh <sup>222</sup>Rn close to the surface induced by the weak vertical transport. During the morning transition, the secular equilibrium is fast restored by the vigorous turbulent mixing. The evolution of <sup>222</sup>Rn and its progeny concentrations in the unsteady growing convective boundary layer depends on the strength of entrainment events. http://www.atmos-chem-phys.net/7/5003/2007/acp-7-5003-2007.pdf
collection DOAJ
language English
format Article
sources DOAJ
author S. Galmarini
S. Basu
J.-F. Vinuesa
spellingShingle S. Galmarini
S. Basu
J.-F. Vinuesa
The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
Atmospheric Chemistry and Physics
author_facet S. Galmarini
S. Basu
J.-F. Vinuesa
author_sort S. Galmarini
title The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
title_short The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
title_full The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
title_fullStr The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
title_full_unstemmed The diurnal evolution of ²²²Rn and its progeny in the atmospheric boundary layer during the Wangara experiment
title_sort diurnal evolution of ²²²rn and its progeny in the atmospheric boundary layer during the wangara experiment
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2007-09-01
description The diurnal atmospheric boundary layer evolution of the <sup>222</sup>Rn decaying family is studied using a state-of-the-art large-eddy simulation model. In particular, a diurnal cycle observed during the Wangara experiment is successfully simulated together with the effect of diurnal varying turbulent characteristics on radioactive compounds initially in a secular equilibrium. This study allows us to clearly analyze and identify the boundary layer processes driving the behaviour of <sup>222</sup>Rn and its progeny concentrations. An activity disequilibrium is observed in the nocturnal boundary layer due to the proximity of the radon source and the trapping of fresh <sup>222</sup>Rn close to the surface induced by the weak vertical transport. During the morning transition, the secular equilibrium is fast restored by the vigorous turbulent mixing. The evolution of <sup>222</sup>Rn and its progeny concentrations in the unsteady growing convective boundary layer depends on the strength of entrainment events.
url http://www.atmos-chem-phys.net/7/5003/2007/acp-7-5003-2007.pdf
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