This manuscript presents a general overview of the Florida Atmospheric
Mercury Study (FAMS): its objectives, its spatial design, and its ove
rall methodologies. FAMS was initiated in May 1992 with the goal of de
veloping field collection and laboratory analytical protocols for char
acterizing Hg in rainfall (wet-only and bulk), atmospheric aerosols, a
nd total gaseous Hg (TGM) FAMS now comprises a network of 7 operationa
l stations, with 2 additional stations scheduled to become operational
by the end of 1994. Preliminary results for FAMS, which Hill continue
collecting deposition samples through December 1996, are the subjects
of other manuscripts in this volume (Gill et al., Landing et al., and
Guentzel ct al.). Results to date suggest that regional deposition in
south Florida is driven by large-scale regional or hemispheric proces
ses as apposed to local emission/deposition processes. Deposition is s
easonally variable, with fluxes 4- to 6-fold higher during April-Septe
mber compared with October-March. The seasonal difference is fluxes is
driven both by concentration differences (2- to 3-fold) and differenc
es in rainfall depth.