4.7 Article

Exploring dimethyl sulfide (DMS) oxidation and implications for global aerosol radiative forcing

期刊

ATMOSPHERIC CHEMISTRY AND PHYSICS
卷 22, 期 2, 页码 1549-1573

出版社

COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/acp-22-1549-2022

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资金

  1. U.S. Department of Energy (DOE) [DE-SC0018934]
  2. U.S. DOE Office of Science, Office of Biological and Environmental Research (BER)
  3. Earth and Environmental System Modeling (EESM) program as part of its Earth System Model Development (ESMD) activity
  4. NASA [80NSSC18K0630, 80NSSC19K0124, 80NSSC21K1451]
  5. Atmospheric Radiation Measurement (ARM)
  6. DOE's Atmospheric System Research, an Office of Science Biological and Environmental Research program
  7. U.S. Department of Energy (DOE) [DE-SC0018934] Funding Source: U.S. Department of Energy (DOE)

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This study reexamines the atmospheric oxidation chemistry of DMS, particularly under pristine conditions, and its impact on aerosol indirect radiative forcing (IRF). By expanding the oxidation pathway of DMS, we found that the additional pathways can delay the formation of sulfate aerosols and alter their spatial distribution and radiative impacts. The improved model results in better agreement with observed concentrations of DMS, MSA, HPMTF, and sulfate in most marine regions.
Aerosol indirect radiative forcing (IRF), which characterizes how aerosols alter cloud formation and properties, is very sensitive to the preindustrial (PI) aerosol burden. Dimethyl sulfide (DMS), emitted from the ocean, is a dominant natural precursor of non-sea-salt sulfate in the PI and pristine present-day (PD) atmospheres. Here we revisit the atmospheric oxidation chemistry of DMS, particularly under pristine conditions, and its impact on aerosol IRE. Based on previous laboratory studies, we expand the simplified DMS oxidation scheme used in the Community Atmospheric Model version 6 with chemistry (CAM6-chem) to capture the OH-addition pathway and the H-abstraction pathway and the associated isomerization branch. These additional oxidation channels of DMS produce several stable intermediate compounds, e.g., methanesulfonic acid (MSA) and hydroperoxymethyl thioformate (HPMTF), delay the formation of sulfate, and, hence, alter the spatial distribution of sulfate aerosol and radiative impacts. The expanded scheme improves the agreement between modeled and observed concentrations of DMS, MSA, HPMTF, and sulfate over most marine regions, based on the NASA Atmospheric Tomography (ATom), the Aerosol and Cloud Experiments in the Eastern North Atlantic (ACE-ENA), and the Variability of the American Monsoon Systems (VAMOS) Ocean-Cloud-Atmosphere-Land Study Regional Experiment (VOCALS-REx) measurements. We find that the global HPMTF burden and the burden of sulfate produced from DMS oxidation are relatively insensitive to the assumed isomerization rate, but the burden of HPMTF is very sensitive to a potential additional cloud loss. We find that global sulfate burden under PI and PD emissions increase to 412 Gg S (+29 %) and 582 Gg S (+8.8 %), respectively, compared to the standard simplified DMS oxidation scheme. The resulting annual mean global PD direct radiative effect of DMS-derived sulfate alone is -0.11 W m(-2). The enhanced PI sulfate produced via the gas-phase chemistry updates alone dampens the aerosol IRF as anticipated (-2.2 WM-2 in standard versus -1.7 W m(-2), with updated gas-phase chemistry). However, high clouds in the tropics and low clouds in the Southern Ocean appear particularly sensitive to the additional aqueous-phase pathways, counteracting this change (-2.3 W m(-2)). This study confirms the sensitivity of aerosol IRF to the PI aerosol loading and the need to better understand the processes controlling aerosol formation in the PI atmosphere and the cloud response to these changes.

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