Direct measurements of the net ecosystem exchange (NEE) of gaseous elemental mercury (Hg 0 ) are important to improve our understanding of global Hg cycling and, ultimately, human and wildlife Hg exposure. The lack of long-term, ecosystem-scale measurements causes large uncertainties in Hg 0 flux estimates. It currently remains unclear whether terrestrial ecosystems are net sinks or sources of atmospheric Hg 0 . Here, we show a detailed validation of direct Hg 0 flux measurements based on the eddy covariance technique (Eddy Mercury) using a Lumex RA-915 AM mercury monitor. The flux detection limit derived from a zero-flux experiment in the laboratory was 0.22 ng m −2 h −1 (maximum) with a 50 % cutoff at 0.074 ng m −2 h −1 . We present eddy covariance NEE measurements of Hg 0 over a low-Hg soil (41-75 ng Hg g −1 in the topsoil, referring to a depth of 0-10 cm), conducted in summer 2018 at a managed grassland at the Swiss FluxNet site in Chamau, Switzerland (CH-Cha). The statistical estimate of the Hg 0 flux detection limit under outdoor conditions at the site was 5.9 ng m −2 h −1 (50 % cutoff). We measured a net summertime emission over a period of 34 d with a median Hg 0 flux of 2.5 ng m −2 h −1 (with a −0.6 to 7.4 ng m −2 h −1 range between the 25th and 75th percentiles). We observed a distinct diel cycle with higher median daytime fluxes (8.4 ng m −2 h −1 ) than nighttime fluxes (1.0 ng m −2 h −1 ). Drought stress during the measurement campaign in summer 2018 induced partial stomata closure of vegetation. Partial stomata closure led to a midday depression in CO 2 uptake, which did not recover during the afternoon. The median CO 2 flux was only 24 % of the median CO 2 flux measured during the same period in the previous year (2017). We suggest that partial stomata closure also dampened Hg 0 uptake by vegetation, resulting in a NEE of Hg 0 that was dominated by soil emission. Finally, we provide suggestions to further improve the precision and handling of the "Eddy Mercury" system in order to assure its suitability for long-term NEE measurements of Hg 0 over natural background surfaces with low soil Hg concentrations (< 100 ng g −1 ). With these improvements, Eddy Mercury has the potential to be integrated into global networks of micrometeorological tower sites (FluxNet) and to provide the longterm observations on terrestrial atmosphere Hg 0 exchange necessary to validate regional and global mercury models.