Iodine has a profound impact on tropospheric chemistry through its role in ozone depletion, particle formation, and impact on the oxidative capacity (see Saiz-Lopez et al., 2012, and references therein). In a previous publication (Gómez Martín et al., 2021), we reported the spatial variability of total iodine (TI) in aerosol by compiling and homogenizing a comprehensive data set of field observations at open ocean, insular, and coastal locations and appending to it previously unpublished measurements, spanning a period of 55 years. The analysis of the latitudinal and longitudinal dependence of TI in aerosol provided for the first time observational evidence from the field showing that the dominant global source of atmospheric iodine to the atmosphere is the reaction between iodide and ozone on the sea-water interface (Carpenter et al., 2013). After uptake on particle surfaces, iodine undergoes a rich aqueous-phase chemistry, which is known to depend on the origin and chemical properties of the aerosol (e.g., acidity ) but still remains poorly understood. Iodine speciation determines whether recycling to the gas phase can proceed through formation of volatile species, which is thought to occur via iodide (I − ), or aerosol becomes essentially an atmospheric iodine sink through accumulation of species assumed to be stable and unreactive, that is, iodate (IO 3 − ; Vogt et al., 1999). However, current aerosol chemical schemes cannot explain the concentrations of I − , IO 3 − , and soluble organic iodine (SOI) observed in field campaigns. Models predict negligible concentrations of I − following recycling to the gas phase and high concentrations of IO 3 − ,