Abstract. Iodine chemistry has noteworthy impacts on the oxidising capacity of the
marine boundary layer (MBL) through the depletion of ozone (O3) and
changes to HOx (OH∕HO2) and NOx (NO∕NO2) ratios.
Hitherto, studies have shown that the reaction of atmospheric O3 with
surface seawater iodide (I−) contributes to the flux of iodine species
into the MBL mainly as hypoiodous acid (HOI) and molecular iodine (I2).
Here, we present the first concomitant observations of iodine oxide (IO),
O3 in the gas phase, and sea surface iodide concentrations. The results
from three field campaigns in the Indian Ocean and the Southern Ocean during
2015–2017 are used to compute reactive iodine fluxes in the MBL.
Observations of atmospheric IO by multi-axis differential
optical absorption spectroscopy (MAX-DOAS) show active iodine chemistry in
this environment, with IO values up to 1 pptv (parts per trillion by volume)
below latitudes of 40∘ S. In order to compute the sea-to-air
iodine flux supporting this chemistry, we compare previously established
global sea surface iodide parameterisations with new region-specific
parameterisations based on the new iodide observations. This study shows
that regional changes in salinity and sea surface temperature play a role in
surface seawater iodide estimation. Sea–air fluxes of HOI and I2,
calculated from the atmospheric ozone and seawater iodide concentrations
(observed and predicted), failed to adequately explain the detected IO in
this region. This discrepancy highlights the need to measure direct fluxes
of inorganic and organic iodine species in the marine environment. Amongst
other potential drivers of reactive iodine chemistry investigated,
chlorophyll a showed a significant correlation with atmospheric IO (R=0.7
above the 99 % significance level) to the north of the polar front. This
correlation might be indicative of a biogenic control on iodine sources in
this region.