Sulfate particles form when sulfuric acid (H₂SO₄) molecules cluster together and grow large enough to become stable, a process called nucleation. Extensive chamber experiments, most notably the Cosmics Leaving Outdoor Droplets (CLOUD) campaigns (Dias et al. 2017), have mapped how nucleation behaves under typical tropospheric conditions (Dunne et al., 2016).
Far fewer experiments have reproduced stratospheric conditions, where two differences likely matter. Water vapor is one of the two components of nucleation, and the stratosphere is extremely dry. Cosmic rays also produce ions at these altitudes, and those ions can stabilize newly formed clusters.
Models reflect this gap. Compared with the limited chamber studies run at stratospheric conditions, commonly used nucleation schemes overestimate new particle formation by 3–4 orders of magnitude (Yu et al., 2023). The same schemes overestimate background particle concentrations relative to in situ data by a smaller factor of 2–4 (Yu et al., 2023).
Chamber experiments on H₂SO₄ nucleation at low humidity, low temperature, and low pressure, run both with and without ions, will constrain these rates directly. Nucleation is one of several uncertainties in aerosol microphysics, but it sets the number of particles formed per unit of injected mass, and therefore the size distribution that governs how efficiently an SAI deployment scatters sunlight.
Tracking condensation and coagulation over longer timescales remains challenging in a chamber. Particle and gas losses to the chamber walls compete with the processes of interest, and they add uncertainty to both the measurements and the analysis that follows. Characterizing wall loss as a function of particle size and gas-phase species will reduce that uncertainty: correcting measured size distributions for the loss terms recovers coagulation and growth rates that can be compared against microphysics schemes.