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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Bibliographic Details
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
Description
Summary: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.
ISSN:1680-7316
1680-7324