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Marine chromophoric dissolved organic matter (m-CDOM) mediates many vital photochemical processes at the ocean's surface. Isolating m-CDOM within the chemical complexity of marine dissolved organic matter has remained an analytical challenge. The SeaSCAPE campaign, a large-scale mesocosm experiment, provided a unique opportunity to probe the in situ production of m-CDOM across phytoplankton and microbial blooms. Results from mass spectrometry coupled with UV-VIS spectroscopy reveal production of a chemodiverse set of compounds well-correlated with increases in absorbance after a bacterial bloom, indicative of autochthonous m-CDOM production. Notably, many of the absorbing compounds were found to be enriched in nitrogen, which may be essential to chromophore function. From these results, quinoids, porphyrins, flavones, and amide-like compounds were identified via structural analysis and may serve as important photosensitizers in the marine boundary layer. Overall, this study demonstrates a step forward in identifying and characterizing m-CDOM using temporal mesocosm data and integrated UV-VIS spectroscopy and mass spectrometry analyses. 

Water systems often contain complex macromolecular systems that absorb light. In marine environments, these light absorbing components are often at the air–water interface and can participate in the chemistry of the atmosphere in ways that are poorly understood. Understanding the photochemistry and photophysics of these systems represents a major challenge since their composition and structures are not unique. In this study, we present a successful microscopic model of this light absorbing macromolecular species termed “marine derived chromophoric dissolved organic matter” or “m-CDOM” in water. The approach taken involves molecular dynamics simulations in the ground state using on the fly Density Functional Tight-Binding (DFTB) electronic structure theory; Time Dependent DFTB (TD-DFTB) calculations of excited states, and experimental measurements of the optical absorption spectra in aqueous solution. The theoretical hydrated model shows key features seen in the experimental data for a collected m-CDOM sample. As will be discussed, insights from the model are: (i) the low-energy A-band (at 410 nm) is due to the carbon chains combined with the diol- and the oxy-groups present in the structure; (ii) the weak B-band (at 320–360 nm) appears due to the contribution of the ionized speciated form of m-CDOM; and (iii) the higher-energy C-band (at 280 nm) is due to the two fused ring system. Thus, this is a two-speciated formed model. Although a relatively simple system, these calculations represent an important step in understanding light absorbing compounds found in nature and the search for other microscopic models of related materials remains of major interest. 

Abstract. Size distributions of particles formed from sulfuric acid(H2SO4) and water vapor in a photolytic flow reactor (PhoFR) weremeasured with a nanoparticle mobility sizing system. Experiments with addedammonia and dimethylamine were also performed. H2SO4(g) wassynthesized from HONO, sulfur dioxide and water vapor, initiating OHoxidation by HONO photolysis. Experiments were performed at 296 K over arange of sulfuric acid production levels and for 16 % to 82 % relativehumidity. Measured distributions generally had a large-particle mode thatwas roughly lognormal; mean diameters ranged from 3 to 12 nm and widths(lnσ) were ∼0.3. Particle formation conditions werestable over many months. Addition of single-digit pmol mol−1 mixing ratios ofdimethylamine led to very large increases in particle number density.Particles produced with ammonia, even at 2000 pmol mol−1, showed that NH3is a much less effective nucleator than dimethylamine. A two-dimensionalsimulation of particle formation in PhoFR is also presented that starts withgas-phase photolytic production of H2SO4, followed by kineticformation of molecular clusters and their decomposition, which is determined by theirthermodynamics. Comparisons with model predictions of the experimentalresult's dependency on HONO and water vapor concentrations yieldphenomenological cluster thermodynamics and help delineate the effects ofpotential contaminants. The added-base simulations and experimental resultsprovide support for previously published dimethylamine–H2SO4cluster thermodynamics and provide a phenomenological set ofammonia–sulfuric acid thermodynamics. 

Marine aerosols strongly influence climate through their interactions with solar radiation and clouds. However, significant questions remain regarding the influences of biological activity and seawater chemistry on the flux, chemical composition, and climate-relevant properties of marine aerosols and gases. Wave channels, a traditional tool of physical oceanography, have been adapted for large-scale ocean-atmosphere mesocosm experiments in the laboratory. These experiments enable the study of aerosols under controlled conditions which isolate the marine system from atmospheric anthropogenic and terrestrial influences. Here, we present an overview of the 2019 Sea Spray Chemistry and Particle Evolution (SeaSCAPE) study, which was conducted in an 11 800 L wave channel which was modified to facilitate atmospheric measurements. The SeaSCAPE campaign sought to determine the influence of biological activity in seawater on the production of primary sea spray aerosols, volatile organic compounds (VOCs), and secondary marine aerosols. Notably, the SeaSCAPE experiment also focused on understanding how photooxidative aging processes transform the composition of marine aerosols. In addition to a broad range of aerosol, gas, and seawater measurements, we present key results which highlight the experimental capabilities during the campaign, including the phytoplankton bloom dynamics, VOC production, and the effects of photochemical aging on aerosol production, morphology, and chemical composition. Additionally, we discuss the modifications made to the wave channel to improve aerosol production and reduce background contamination, as well as subsequent characterization experiments. The SeaSCAPE experiment provides unique insight into the connections between marine biology, atmospheric chemistry, and climate-relevant aerosol properties, and demonstrates how an ocean-atmosphere-interaction facility can be used to isolate and study reactions in the marine atmosphere in the laboratory under more controlled conditions.