362 Simulating Sulfate Aerosol Size in the 2022 Hunga Tonga-Hunga Ha'apai Eruption Plume: Comparisons with Observations

Tuesday, 30 January 2024
Hall E (The Baltimore Convention Center)
Parker A Case, NASA Goddard Space Flight Center, Greenbelt, MD; and P. R. Colarco, G. Taha, E. Asher, S. Steenrod, Q. Liang, and L. Oman

Using the NASA GEOS Chemistry Climate Model (CCM) coupled to a detailed sectional aerosol microphysics model, we have simulated the January 2022 Hunga Tonga-Hunga Ha’apai (HTHH) volcanic plume. We have developed a version of the Global Modeling Initiative (GMI) chemistry mechanism to include the requisite sulfur chemistry and coupled it to the Community Aerosol and Radiation Model for Atmospheres (CARMA) sectional aerosol microphysics within the GEOS CCM. Our simulations focus on the lifecycle of stratospheric sulfur injected by the eruption–from the oxidation of the injected sulfur dioxide to the nucleation, growth, coagulation, hydration, and eventual settling of the volcanic sulfate aerosol particles. In order to constrain the simulated microphysics, we focus on comparing our model to observations with aerosol size information, namely in-situ particle counter observations and multi-wavelength satellite observations from OMPS-LP and SAGE-III. This eruption provides an interesting test case for our model; both the modeled gas-phase chemistry as well as the modeled aerosol microphysics are perturbed by the massive injection of water that accompanied the primary sulfur emissions from the eruption.
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