Articles | Volume 16, issue 21
https://doi.org/10.5194/gmd-16-6087-2023
© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License.
Description and performance of a sectional aerosol microphysical model in the Community Earth System Model (CESM2)
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- Final revised paper (published on 01 Nov 2023)
- Preprint (discussion started on 25 Apr 2023)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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- RC1: 'Comment on gmd-2023-79', Anonymous Referee #1, 28 Jul 2023
- RC2: 'Comment on gmd-2023-79', Anonymous Referee #2, 07 Aug 2023
- AC1: 'Comment on gmd-2023-79', Simone Tilmes, 26 Aug 2023
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AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Simone Tilmes on behalf of the Authors (28 Aug 2023)
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ED: Publish as is (06 Sep 2023) by Samuel Remy
AR by Simone Tilmes on behalf of the Authors (08 Sep 2023)
Review of “Description and performance of the CARMA sectional aerosol microphysical model in CESM2” by Tilmes et al. for publication in Geoscientific Model Development.
The paper provides a comparative evaluation of the performance of two aerosol microphysical schemes in simulations performed with two different configurations of the Community Earth System Model (CESM2). In one the sectional CARMA module is compared to the modal MAM4 module in the high-top version of CESM2 called WACCM-MA and applied to study of the 1991 Mount Pinatubo volcanic eruption and subsequent period. In the other the two aerosol modules are run in the low-top CAMchem configuration and applied to simulations of tropospheric and lower stratospheric aerosol in the context of the 2016-2018 ATom airborne observations. It is shown that for Pinatubo the performance of both CARMA and MAM4 are improved by distributing emissions over a region instead of prescribing over the volcano column alone. CARMA results in overall larger particles following Pinatubo, with a correspondingly shorter atmospheric lifetime. Two different nucleation schemes are tested in CARMA, its default Zhao scheme and the Vehkamäki scheme used in MAM4. Overall CARMA’s performance is better with its default scheme. Tropospheric aerosols are compared to MODIS AOD and ATom profile observations. Modeled profiles are generally similar between CARMA and MAM, each with its strengths and weaknesses in terms of species and regions. CARMA somewhat overestimates the mid-tropospheric sulfate relative to ATom, and MAM has consequently better agreement in the extinction profile. CARMA is shown to have overall better agreement with observed particle size distributions for both Pinatubo and ATom cases.
The paper is well organized and relatively comprehensive. It is suitable for publication with minor revisions. I suggest a couple of points below that could be expanded on to improve the discussion, and suggest numerous minor points.
Major points
Line 183 refers to sub-stepping for stability in process rates. Some additional information would be useful here, particularly as to how it impacts performance and accuracy. Do MAM4 and CARMA take similar approaches? Do they have similar accuracy tolerances? What are those?
Section 2.4.5 could be more explicit with respect to the size distributions of emissions, specifically how they compare to each other between CARMA and MAM. Lifetime numbers reported in Table 4 are more typical of AeroCom models in MAM than they are for CARMA, which is remarkably short for both dust and sea salt. This could be a consequence of emissions being strongly weighted toward largest size bins in CARMA. Some further detail here would be helpful instead of just referring to previous work. The discussion in 5.2.1 expands a bit more on this as well. The discussion seems a bit simplistic. It would be better to present in terms of efficiencies of processes instead of references to burdens. I know there is non-linearity in the microphysics, but in terms of the sink processes they are quasi linear in terms of the burden, so it’s not very illuminating to frame it that way. Instead, what seems clear, is that CARMA prefers dry deposition, which necessarily leaves less aerosol for wet removal. MAM is more the opposite.
Minor points
Line 102: For completeness, what is the mode width for the primary carbon mode?
Line 156: “Therefore the wet radius below 190 K” is a sentence fragment of unclear intent.
Line 169: s/b McFarlane
Line 171: “two moment cloud microphysics (?)” Unclear what the (?) means, maybe a missing reference?
Line 209: s/b McFarlane
Line 255: Here and elsewhere this note about photolysis of SOA. What does this mean? Is this a destruction pathway, or something to with photolysis chemistry? A reference would help.
Line 284: Suggest “correspondingly” instead of “somewhat” smaller throughput.
Line 3232: Do you really mean QFED here? Citation is Darmenov and da Silva (2015, https://ntrs.nasa.gov/citations/20180005253)
Figure 5, second panel: Since the behavior essentially asymptotes at 30 days, suggest you compress x-axis range to allow better inspection of the first 10 days in this figure, where the models are quite different.
Line 485 and rest of paragraph: Figure 9 is stated but actually Figure 8 is meant.
Line 502: Figure 9 is meant instead of Figure 8.
Table 4: Caption states lifetime given in years. This is incorrect, it should be days.
Line 537: What MODIS products are used here?
Figure 11: Positional labeling in caption caption (top, middle, bottom…) would make sense if there are six panels, but there are eight. Suggest label a, b, c, …
Line 576: “settling” instead of “settlement”
Line 582: Here and rest of paragraph Figure 11 actually s/b Figure 13 and Figure 12 actually s/b Figure 14