A054-07
Observation-Enabled Assessment of Simulated Southern Ocean Aerosol and INP Populations in the Community Atmosphere Model Version 6
Abstract:
Observations from the DOE-ARM MARCUS ship-based campaign, the ground-based MICRE study, and the NSF SOCRATES flights confirm marine sources dominate the SO aerosol, with some influence of dust aerosol detected above clouds. Low INP concentrations measured both in the SO marine boundary layer and aloft suggest that this pristine aerosol sustains low-level supercooled liquid clouds over the SO.
Instrument simulators, designed based on instrumentation specifications, were “deployed” in CAM6 simulations over the SO study periods with dynamics specified from reanalysis data. Simulated marine and dust aerosol vertical profiles roughly matched observations, with maximum sea salt number concentrations (Nss) in the marine boundary layer and maximum dust number concentrations (Ndst) above 4 km. Below 3 km, Nss were a factor of 100 higher than Ndst, though simulated Ndst range over 3 orders of magnitude likely due to variability in simulated dust scavenging. Because the ice nucleation ability of dust aerosol is three orders of magnitude greater than that of marine aerosol for a given aerosol surface area, we find that errors even for low Ndst impacted predicted INP populations. In fact, INPs estimated from CAM6 simulated aerosol quantities resulted in dust-dominated INP populations at all altitudes, inconsistent with SO observations.
Following the SO aerosol and INP assessment, observationally-guided modifications to specific processes, including dust aerosol scavenging, estimated impacts of marine organic aerosol, and INP parameterizations, will be investigated to reduce INP prediction biases. The improvements achieved from this study will ultimately facilitate observation-enabled evaluation and development for cloud processes subsequent to primary ice nucleation.