2023
DOI: 10.1029/2022jd036955
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Simulating Southern Ocean Aerosol and Ice Nucleating Particles in the Community Earth System Model Version 2

Abstract: Southern Ocean (SO) low‐level mixed phase clouds have been a long‐standing challenge for Earth system models to accurately represent. While improvements to the Community Earth System Model version 2 (CESM2) resulted in increased supercooled liquid in SO clouds and improved model radiative biases, simulated SO clouds in CESM2 now contain too little ice. Previous observational studies have indicated that marine particles are major contributor to SO low‐level cloud heterogeneous ice nucleation, a process that ini… Show more

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Cited by 5 publications
(21 citation statements)
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References 74 publications
(125 reference statements)
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“…The lack of blank correction may also explain the higher INP concentrations reported from ACE measurements relative to those from CAPRICORN-1, CAP-2, and SOC, although differences in sampling time and location likely also play a role. Parameterizations for dust INPs based on global INP data and number concentrations of aerosols larger than 500 nm (DeMott et al, 2015) or aerosol surface area concentrations (Ullrich et al, 2017) overpredicted the observations from SOC and CAP-2, corroborating the growing consensus that the majority of boundary layer-INPs in this region are local, and of marine origin (Burrows et al, 2013;McCluskey et al, 2018aMcCluskey et al, , 2019McCluskey et al, , 2023Vergara-Temprado et al, 2017;Welti et al, 2020). The Although there is overall agreement between the campaigns, the SOC filter and CFDC measurements in the MBL are offset toward warmer concentrations relative to those from CAP-2.…”
Section: Capricorn-2 and Socrates Marine Boundary Layer Inp Observationssupporting
confidence: 61%
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“…The lack of blank correction may also explain the higher INP concentrations reported from ACE measurements relative to those from CAPRICORN-1, CAP-2, and SOC, although differences in sampling time and location likely also play a role. Parameterizations for dust INPs based on global INP data and number concentrations of aerosols larger than 500 nm (DeMott et al, 2015) or aerosol surface area concentrations (Ullrich et al, 2017) overpredicted the observations from SOC and CAP-2, corroborating the growing consensus that the majority of boundary layer-INPs in this region are local, and of marine origin (Burrows et al, 2013;McCluskey et al, 2018aMcCluskey et al, , 2019McCluskey et al, , 2023Vergara-Temprado et al, 2017;Welti et al, 2020). The Although there is overall agreement between the campaigns, the SOC filter and CFDC measurements in the MBL are offset toward warmer concentrations relative to those from CAP-2.…”
Section: Capricorn-2 and Socrates Marine Boundary Layer Inp Observationssupporting
confidence: 61%
“…Above cloud and upper tropospheric N n500 were consistent with the DeMott et al ( 2015) parameterization for dust (Figure S6b in Supporting Information S1), but N s values were still 1-2 orders of magnitude lower than the Ullrich et al (2017) dust parameterization (Figure S6c in Supporting Information S1). This discrepancy between the effectiveness of dust aerosol number-and surface area-based parameterizations has been reported previously for this region (McCluskey et al, 2019(McCluskey et al, , 2023. About half of the SOC research flights collected paired filter samples, with one in the MBL and one above cloud.…”
Section: Altitude Dependencementioning
confidence: 63%
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“…This riming frequency is similar to results over mid‐latitude Europe and the Arctic (Kneifel & Moisseev, 2020), although the riming frequency over Davis is slightly higher than the four Northern Hemisphere sites (3 − 5% at the Northern mid‐latitudes at −3°C, and 2% over the Arctic). Cleaner sites, with fewer aerosols and in particular fewer INPs (C. S. McCluskey et al., 2023; McCluskey et al., 2018; Raman et al., 2023; Vignon, Alexander, et al., 2021), have fewer but larger supercooled liquid water droplets, which enhance the possibility of riming. A high riming frequency was found during one summer event of triple‐wavelength radar observations at McMurdo Station, Antarctica (Tridon et al., 2022) which is qualitatively consistent with the Davis summer results presented here.…”
Section: Resultsmentioning
confidence: 99%