In a series of small-scale field studies, two experiments were carried out on reemission after 1-h HTO deposition phases, one at sunrise (7.00 a.m.) and one at sunset (9.00 p.m.), on two subsequent days. In both cases, wind speeds were extremely low to absolutely calm during the observed 12-h reemission periods. Both sunrise and sunset experiments showed the same reemission rate of 28% h −1 during the first hour of reemission, in spite of the differences of the atmosphere/soil conditions. Time-of-day specific deviations of the reemission rates appeared only during the subsequent hours, leading to total losses of the deposited HTO of 84% during the 12-h day-phase after the sunrise deposition and of 57% during the 12-h nightphase after the sunset deposition. The experimental conditions were used to model the time courses of the reemission rates by the appropriate module of the UFOTRI code, which is characterized by a coupling of HTO reemission to H 2O evaporation and a set of default values, where more detailed information is not available. The comparison shows a rather poor agreement, as neither the high first-hour values nor the subsequent strong reductions can be reproduced. Agreement is improved, however, after modification of the default values. The findings suggest that at least the initial reemission rate should be modeled independently from the H 2O evaporation rate, and the spatial resolution of multilayer soil models should be of the same order of magnitude as the scaling length of the deposition profile, i.e. some 10 −3 m, characterizing the penetration depth of HTO after 1h of deposition and approximating the thickness of the uppermost soil layer that releases tritium during the first hour of the reemission process.
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