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			<titleStmt><title level='a'>Characterizing the Atmospheric Mn Cycle and Its Impact on Terrestrial Biogeochemistry</title></titleStmt>
			<publicationStmt>
				<publisher>Global Biogeochemical Cycles</publisher>
				<date>04/01/2024</date>
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				<bibl> 
					<idno type="par_id">10534522</idno>
					<idno type="doi">10.1029/2023GB007967</idno>
					<title level='j'>Global Biogeochemical Cycles</title>
<idno>0886-6236</idno>
<biblScope unit="volume">38</biblScope>
<biblScope unit="issue">4</biblScope>					

					<author>Louis Lu</author><author>Longlei Li</author><author>Sagar Rathod</author><author>Peter Hess</author><author>Carmen Martínez</author><author>Nicole Fernandez</author><author>Christine Goodale</author><author>Janice Thies</author><author>Michelle Y Wong</author><author>Maria Grazia Alaimo</author><author>Paulo Artaxo</author><author>Francisco Barraza</author><author>Africa Barreto</author><author>David Beddows</author><author>Shankarararman Chellam</author><author>Ying Chen</author><author>Patrick Chuang</author><author>David D Cohen</author><author>Gaetano Dongarrà</author><author>Cassandra Gaston</author><author>Darío Gómez</author><author>Yasser Morera‐Gómez</author><author>Hannele Hakola</author><author>Jenny Hand</author><author>Roy Harrison</author><author>Philip Hopke</author><author>Christoph Hueglin</author><author>Yuan‐Wen Kuang</author><author>Katriina Kyllönen</author><author>Fabrice Lambert</author><author>Willy Maenhaut</author><author>Randall Martin</author><author>Adina Paytan</author><author>Joseph Prospero</author><author>Yenny González</author><author>Sergio Rodriguez</author><author>Patricia Smichowski</author><author>Daniela Varrica</author><author>Brenna Walsh</author><author>Crystal Weagle</author><author>Yi‐Hua Xiao</author><author>Natalie Mahowald</author>
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			<abstract><ab><![CDATA[<title>Abstract</title> <p>The role of manganese (Mn) in ecosystem carbon (C) biogeochemical cycling is gaining increasing attention. While soil Mn is mainly derived from bedrock, atmospheric deposition could be a major source of Mn to surface soils, with implications for soil C cycling. However, quantification of the atmospheric Mn cycle, which comprises emissions from natural (desert dust, sea salts, volcanoes, primary biogenic particles, and wildfires) and anthropogenic sources (e.g., industrialization and land‐use change due to agriculture), transport, and deposition, remains uncertain. Here, we use compiled emission data sets for each identified source to model and quantify the atmospheric Mn cycle by combining an atmospheric model and in situ atmospheric concentration measurements. We estimated global emissions of atmospheric Mn in aerosols (<10μm in aerodynamic diameter) to be 1,400Gg Mn year<sup>−1</sup>. Approximately 31% of the emissions come from anthropogenic sources. Deposition of the anthropogenic Mn shortened Mn “pseudo” turnover times in 1‐m‐thick surface soils (ranging from 1,000 to over 10,000,000years) by 1–2 orders of magnitude in industrialized regions. Such anthropogenic Mn inputs boosted the Mn‐to‐N ratio of the atmospheric deposition in non‐desert dominated regions (between 5×10<sup>−5</sup>and 0.02) across industrialized areas, but that was still lower than soil Mn‐to‐N ratio by 1–3 orders of magnitude. Correlation analysis revealed a negative relationship between Mn deposition and topsoil C density across temperate and (sub)tropical forests, consisting with atmospheric Mn deposition enhancing carbon respiration as seen in in situ biogeochemical studies.</p>]]></ab></abstract>
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<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1.">Introduction</head><p>The contribution of manganese (Mn) as an essential micronutrient to biogeochemical carbon (C) cycling has been increasingly recognized in both terrestrial and marine environments. Though often in trace amount, Mn has the potential to act as the driving factor for biogeochemical cycling when it becomes limiting in various ecosystems <ref type="bibr">(Ahlgren et al., 2014;</ref><ref type="bibr">Browning et al., 2021;</ref><ref type="bibr">J. A. M. Moore et al., 2021</ref>; O. W. <ref type="bibr">Moore et al., 2023;</ref><ref type="bibr">Whalen et al., 2018)</ref>. Despite its importance to advancing the understanding of ecosystem functioning, little effort has been made to constrain and quantify different components of the global Mn biogeochemical cycle, let alone the atmospheric Mn cycle. Atmospheric deposition has been identified to serve as a major source of trace metal(loid)s to soils on land <ref type="bibr">(He &amp; Walling, 1997;</ref><ref type="bibr">Herndon et al., 2011;</ref><ref type="bibr">Kaste et al., 2003;</ref><ref type="bibr">Puchelt et al., 1993;</ref><ref type="bibr">Wang et al., 2022)</ref> as well as surface water in ocean <ref type="bibr">(Mahowald et al., 2018)</ref>. We thus focused on delineating the atmospheric component of the global Mn biogeochemical cycle using observation-model combined approaches and thereafter presented a case study of its application to terrestrial ecosystems.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1.1.">Atmospheric Mn Cycle</head><p>Metals are present in the atmosphere mainly in the form of aerosols <ref type="bibr">(Mahowald et al., 2018)</ref>. There are a variety of natural sources of Mn, such as desert dust (the single dominant source), sea salts, volcanoes, wildfires, and primary biogenic particles (PBPs) <ref type="bibr">(Nriagu, 1989;</ref><ref type="bibr">Pacyna &amp; Pacyna, 2001)</ref>. In addition to natural sources of atmospheric Mn deposition, humans can perturb the global atmospheric Mn cycle by significantly altering desert dust cycling and adding anthropogenic emission sources such as combustion <ref type="bibr">(Mahowald et al., 2018)</ref>. Anthropogenic aerosols have the potential to induce a more rapid impact on ecosystems compared to natural aerosols because of their higher solubility owing to their smaller particle size, higher carbon content, chemical and surface associations, and reactions that occur during the process of combustion <ref type="bibr">(Desboeufs et al., 2005;</ref><ref type="bibr">Jang et al., 2007;</ref><ref type="bibr">Sedwick et al., 2007;</ref><ref type="bibr">Voutsa &amp; Samara, 2002)</ref>.</p><p>While global budgets for many metals have been estimated previously, their spatial distribution is more unknown. <ref type="bibr">Nriagu (1989)</ref> made the first attempt to estimate Mn emissions to the atmosphere. <ref type="bibr">Nriagu (1989)</ref> and <ref type="bibr">Pacyna and Pacyna (2001)</ref> identified desert dust as the single dominant source and estimated the contribution of anthropogenic sources to be approximately 11%. <ref type="bibr">Mahowald et al. (2018)</ref> estimated that anthropogenic emissions represent &#8764;1% of the total aerosol Mn sources. Uncertainties are high due to the lack of observational data, and so far, there have been no detailed spatially explicit studies of the atmospheric Mn cycle. Therefore, a better estimation of the Mn source budget (both natural and anthropogenic) along with its spatial distribution is necessary for understanding the global Mn cycle and its influence on terrestrial ecosystems.</p><p>In this study, we conducted the first 3-d modeling of the emission, atmospheric transport, and deposition of atmospheric Mn from multiple sources including natural and anthropogenic dust, sea salts, volcanoes, wildfires, and PBPs. We compiled emission data sets for each source and soil Mn concentration measurements for the emission modeling and model calibration, respectively. We synthesized observational and modeling evidence to characterize the spatial distribution of atmospheric Mn and to assess the anthropogenic perturbation to it in both PM 2.5 and PM 10 size fractions (atmospheric particulate matter, PM, &lt;2.5 and 10 &#956;m in aerodynamic diameter, respectively), which were used as common measures for aerosols in the atmosphere and included in the model <ref type="bibr">(Mahowald et al., 2014;</ref><ref type="bibr">Ryder et al., 2019)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1.2.">Relevance to Terrestrial Ecosystems</head><p>Mn has been identified to be closely related to forest soil C turnover because of its role in regulating soil organic matter (SOM) decomposition by enhancing the activity of lignin-decay enzymes (mainly Mn peroxidase, MnP) and hence the oxidative decomposition of lignin <ref type="bibr">(Berg et al., 2007;</ref><ref type="bibr">Hofrichter, 2002)</ref>. Mn limitation and the associated fungal community change from nitrogen (N) deposition have been proposed as an explanation for the suppressing effect of long-term atmospheric N deposition on SOM decomposition (J. A. M. <ref type="bibr">Moore et al., 2021;</ref><ref type="bibr">Whalen et al., 2018)</ref>. Thus, higher Mn availability from anthropogenic activity could minimize the soil carbon accumulation observed under N deposition.</p><p>Studies have assessed the relationship between Mn availability and soil C turnover rates using various indicators including Mn concentration in litter, rate or extent of decomposition of litter <ref type="bibr">(Berg, 2000;</ref><ref type="bibr">Berg et al., 2007</ref><ref type="bibr">Berg et al., , 2010;;</ref><ref type="bibr">Davey et al., 2007;</ref><ref type="bibr">Trum et al., 2015)</ref>, soil Mn and total C concentrations <ref type="bibr">(Stendahl et al., 2017)</ref>, MnP enzymatic activity, and fungal community structures <ref type="bibr">(Kranabetter et al., 2021;</ref><ref type="bibr">J. A. M. Moore et al., 2021;</ref><ref type="bibr">Whalen et al., 2018)</ref>. However, no previous study has examined the impact of atmospheric Mn deposition (despite its potential to be the major source of Mn addition in surficial layers) on soil C turnover, nor has such a relationship been quantified on a global scale.</p><p>Therefore, we made a first attempt to tease out the potential relationship between Mn deposition and SOM in global forest ecosystems based on modeled Mn deposition, testing relationships between Mn availability and broad scale patterns. To understand the importance of atmospheric deposition as a flux in the Mn cycle and as a source of Mn addition to soils in terrestrial ecosystems, we interpreted soil Mn "pseudo" turnover times and Mnto-N ratios in deposition as well as the relationship between Mn deposition and C density in topsoil.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.">Materials and Methods</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.1.">Soil Mn Observations and Interpolation</head><p>Two of the outlined major emission sources, desert and agricultural dust, are directly related to Mn concentration in surficial soil layers. On average, the upper continental crust, in part based on loess analyses, contains 0.1% manganese oxide by weight <ref type="bibr">(Rudnick &amp; Gao, 2003)</ref>, which is equivalent to 775 mg kg -1 of Mn. However, soil Mn composition can deviate from this value depending on the in-situ weathering status of the regolith and external inputs of Mn <ref type="bibr">(Brantley &amp; White, 2009)</ref>. Considering this spatial heterogeneity, an inverse distance weighted (IDW) interpolation approach was taken based on 2,068 field observations compiled from 94 studies found using the Thomson Web of Science Core Collection on 20 March 2022 and the soil characterization database provided in National Cooperative Soil Survey, NCSS (Figure <ref type="figure">1a</ref>; Text S1 in Supporting Information S1). The observations suggested a mean topsoil Mn concentration of 681 mg kg -1 , which is slightly smaller than, but close enough to the value derived from the averaged upper crust; therefore, a base case was set up assuming a constant soil Mn concentration of 775 mg kg -1 and used for comparison with the interpolated soil map in model analysis.</p><p>The constructed soil map from linear IDW interpolation was a fairly good representation of observations (r = 0.66; Figure <ref type="figure">1b</ref>) given the model grid resolution and the fact that many observational sites clustered in a single grid. There were many more observations in developed countries (especially North America and Europe) in the Northern Hemisphere mid-latitudes than the higher latitudes and the tropics, where the distance to the nearest observation could be large (Figure <ref type="figure">S1a</ref> in Supporting Information S1). To partly cover the uncertainties arising from the sparseness of observational sites, an uncertainty value that equals one standard deviation (after removing outliers &gt;Q3 + 1.5 * IQR or &lt;Q1 -1.5 * IQR), 393 mg kg -1 , was assigned to each grid in the interpolated soil map and used along with the constant Mn base case in later sensitivity tests for "pseudo" turnover times computation. A cross validation was conducted for the interpolation to further evaluate its robustness (Figure <ref type="figure">S1b</ref> in Supporting Information S1).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.">Atmospheric Modeling</head><p>We simulated global atmospheric Mn emissions, transport, and deposition using the Community Atmosphere Model, version 6 (CAM6), the atmospheric component of the Community Earth System Model (version 2; CESM2) developed at the National Center for Atmospheric Research <ref type="bibr">(Hurrell et al., 2013;</ref><ref type="bibr">Liu et al., 2011)</ref>, with the four-mode (Aitken, accumulation, coarse, and primary) modal aerosol model <ref type="bibr">(Liu et al., 2016)</ref>. Three out of the four modes contain dust aerosols which are modeled as eight different types of dust mineral components <ref type="bibr">(Hamilton et al., 2019;</ref><ref type="bibr">Li et al., 2021</ref><ref type="bibr">Li et al., , 2022;;</ref><ref type="bibr">Liu et al., 2011;</ref><ref type="bibr">Scanza et al., 2015)</ref>. Model simulations were conducted for 4 years, with the last 3 years (2013-2015) used for analysis <ref type="bibr">(Computational and Information Systems Laboratory, 2019)</ref>. We nudged the model toward MERRA2 meteorology fields <ref type="bibr">(Gelaro et al., 2017)</ref>.</p><p>The model simulates three-dimensional transport and wet and dry deposition for gases and particles which are internally/externally mixed within/between the modes. The dry deposition parameterization follows <ref type="bibr">Petroff and Zhang (2010)</ref> as previously implemented in CAM6 <ref type="bibr">(Li et al., 2022</ref>; see descriptions therein for the wet deposition Global Biogeochemical Cycles 10.1029/2023GB007967 scheme as well). We modified the model to allow for the advection of Mn from different sources. Both natural and anthropogenic sources were determined to possess large uncertainties in strength. We used a first estimate assuming that the full uncertainty range is one order of magnitude. Therefore, we included a range of values (typically a factor of 10) for the Mn contribution from each source (Table <ref type="table">1</ref>). To better fit the observational data, Note. Desert and agricultural dust Mn budget values were obtained from the dust model simulations which used as input the Mn composition of soils constructed using IDW interpolation (Section 2.1). Alternatively, assuming a constant soil Mn fraction (base case) yielded 1,300 Gg year -1 and 510 Gg year -1 (both within the uncertainty range) for desert dust and agricultural dust, respectively. a Nriagu (1989). b <ref type="bibr">Mahowald et al. (2018)</ref>. Mn in surface soils), which are spatially averaged and plotted as circles filled with colors corresponding to their Mn concentration <ref type="bibr">(Abanda et al., 2011;</ref><ref type="bibr">Alfaro et al., 2015;</ref><ref type="bibr">Alongi et al., 2004;</ref><ref type="bibr">Andruszczak, 1975;</ref><ref type="bibr">Asawalam &amp; Johnson, 2007;</ref><ref type="bibr">Becquer et al., 2010;</ref><ref type="bibr">Beygi &amp; Jalali, 2018;</ref><ref type="bibr">Bibak et al., 1994;</ref><ref type="bibr">Boente et al., 2017;</ref><ref type="bibr"/> we tuned the model making a particular effort to adjust anthropogenic emissions both because of their larger uncertainties compared to natural emissions and because the largest discrepancies occurred over industrialized regions (see below). The "tuning" method was based on the optimization of two parameters most related to the model performance, coefficient of determination (R 2 ) and root mean squared error (RMSE) and considered both natural and anthropogenic sources in both size fractions (Text S1 in Supporting Information S1). In addition, we report our best estimates and assume a large uncertainty: in most cases at least one order of magnitude because of the limited data as previous studies suggested (e.g., <ref type="bibr">Mahowald et al., 2018;</ref><ref type="bibr">Nriagu, 1989)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.1.">Desert Dust</head><p>The desert dust sources of Mn refer to mineral particles entrained into the atmosphere by strong winds at the soil surface in arid unvegetated or loosely vegetated regions, where soils are prone to wind erosion, and play a major role in the global aerosol budget <ref type="bibr">(Boucher et al., 2013;</ref><ref type="bibr">Vandenbussche et al., 2020;</ref><ref type="bibr">Zender et al., 2003)</ref>. The emissions, transport, and deposition of dust aerosols, including seasonal and interannual variability, are all prognostic in the model. We applied the same dust emission scheme <ref type="bibr">(Kok, Mahowald, et al., 2014;</ref><ref type="bibr">Kok, Albani, et al., 2014)</ref> as in <ref type="bibr">Wong et al. (2021)</ref>, and tuned the model to obtain a global mean aerosol optical depth of 0.03 <ref type="bibr">(Li et al., 2022)</ref> based on observational estimates <ref type="bibr">(Ridley et al., 2016)</ref>. Transport and deposition of Mn were simulated separately according to the size mode <ref type="bibr">(Liu et al., 2016)</ref>, following treatment on dust aerosols as described in <ref type="bibr">Albani et al. (2014)</ref>. In addition, to improve the simulation of aerosols in the coarse and accumulation modes, we modified the model by using the geometric median diameter (GMD) as that initialized in CAM5 and geometric standard deviation as well as the edges of the predicted coarse-mode GMD following <ref type="bibr">Li et al. (2022)</ref>.</p><p>Because desert dust is generated from soil, we assumed that the soil Mn concentration is the same as the Mn in the dust, regardless of particle size, as we had no information on the size segregation of the soil Mn. The model simulation using the interpolated Mn soil map had Mn emissions in desert dust of 950 Gg year -1 , which was lower compared to 1,300 Gg year -1 in the base case which assumed a constant soil Mn fraction (Table <ref type="table">1</ref>). Both are larger than the range (42-400 Gg year -1 ) stated in <ref type="bibr">Nriagu (1989)</ref>, and more similar to the value (900 Gg year -1 ) given by <ref type="bibr">Mahowald et al. (2018)</ref>. Note that the amount of dust is very sensitive to the size range included in the estimates (e.g., <ref type="bibr">Mahowald et al., 2014)</ref>. Using the range of values from the literature, the uncertainty range of 480-4,800 Gg Mn year -1 was assigned.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.2.">Agricultural Dust</head><p>Agricultural land use and land cover change induced by human activities can boost mineral dust emissions through various mechanisms that increase soil erodibility, such as increasingly exposing soil surface and altering hydrologic cycles <ref type="bibr">(Ginoux et al., 2012;</ref><ref type="bibr">Webb &amp; Pierre, 2018)</ref>. Satellite-based analysis suggests that it represents 25% of global dust emissions <ref type="bibr">(Ginoux et al., 2012)</ref>. To account for agricultural dust, we applied data sets of crop fraction of present agricultural land from the Coupled Model Intercomparison Project Phase 5 (CMIP5) data sets <ref type="bibr">(Hurtt et al., 2011)</ref>. We separately computed the crop sources of dust (identified using the above data set) and tuned these sources for each region to match those estimated from satellites, with the exception of Australia, where we assumed only 15% of the dust is anthropogenic, consistent with other studies (e.g., <ref type="bibr">Bullard et al., 2008;</ref><ref type="bibr">Mahowald et al., 2009;</ref><ref type="bibr">Webb &amp; Pierre, 2018)</ref>. The discrepancy in Australia between the results of <ref type="bibr">Ginoux et al. (2012)</ref> and other studies (Table <ref type="table">S1</ref> in Supporting Information S1) may be caused by the large drought during the time period studied by <ref type="bibr">Ginoux et al. (2012)</ref>. Whether agriculture has significantly altered the Mn concentration at the soil surface remains uncertain, therefore, we adopted the same interpolated soil map for calculation of Mn fraction as in the case of desert dust. This approach provides a global emissions of 370 Gg Mn year -1 with a range of 190-1,900 Gg Mn year -1 (Table <ref type="table">1</ref>).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.3.">Sea Spray</head><p>Sea-spray aerosols are produced by the bubble-bursting process typically resulting from whitecap generation under high wind conditions in the boundary layer <ref type="bibr">(O'Dowd &amp; de Leeuw, 2007)</ref>. We used prognostic sea spray included in CAM6 <ref type="bibr">(Liu et al., 2011)</ref> and assumed a constant concentration of 95 &#956;g Mn kg -1 in sea-spray aerosols <ref type="bibr">(Nriagu, 1989)</ref>. Sea-spray aerosols were estimated to emit 0.26 Gg Mn year -1 with an uncertainty range of 0.13-1.3 Gg Mn year -1 (Table <ref type="table">1</ref>), falling within the range given by <ref type="bibr">Nriagu (1989)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Global Biogeochemical Cycles</head><p>10.1029/2023GB007967</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.4.">Volcanoes</head><p>Studies have shown that volcanoes can be an important contributor to trace elements in aerosols, such as Mn, through eruptive activities and degassing <ref type="bibr">(Mahowald et al., 2018;</ref><ref type="bibr">Sansone et al., 2002)</ref>. We assumed only noneruptive sources for this study <ref type="bibr">(Spiro et al., 1992)</ref>, with a constant source across the time periods. For volcanic sources, the concentration of trace elements is commonly expressed using their ratio to sulfur (S). We adopted a mass-based ratio of 12 &#215; 10 -4 Mn/S from <ref type="bibr">Nriagu (1989)</ref> and multiplied it with the concentration of sulfur given in the data set <ref type="bibr">(Spiro et al., 1992)</ref> to derive Mn. We estimated non-eruptive volcanic emissions to be 3.9 Gg Mn year -1 with a range of 2.0-20 Gg Mn year -1 , lying at the lower end of the range provided by <ref type="bibr">Nriagu (1989)</ref> (Table <ref type="table">1</ref>).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.5.">Primary Biogenic Particles</head><p>PBPs are a diverse group of airborne particles such as bacteria, fungal spores, pollen, viruses and algae that are directly released from the biosphere into the atmosphere <ref type="bibr">(China et al., 2020;</ref><ref type="bibr">Despr&#233;s et al., 2012)</ref>. Like volcanoes, they are not explicitly simulated in the default CAM6 model but act as a non-negligible aerosol metal source <ref type="bibr">(Mahowald et al., 2018)</ref>. Following <ref type="bibr">Brahney et al. (2015)</ref>, we adopted parameterized PBP data that are temporally constant and based on the assumption of a leaf area index dependent source for vegetative and insect debris. We also included a pollen source based on <ref type="bibr">Heald and Spracklen (2009)</ref> and a bacteria parameterization <ref type="bibr">(Burrows et al., 2009)</ref>. The emission, transport, and deposition of PBPs were simulated using a separate tracer. We assumed the Mn fraction to be 60 mg kg -1 in PBPs <ref type="bibr">(Nriagu, 1989)</ref> and estimated its emission to be 2.0 Gg Mn year -1 with a range of 1.0-10 Gg Mn year -1 (Table <ref type="table">1</ref>).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.6.">Wildfires</head><p>Aerosols emitted from wildfires can significantly contribute to atmospheric Mn <ref type="bibr">(Nriagu, 1989)</ref>, especially in densely forested regions that are fire-prone <ref type="bibr">(Krawchuk et al., 2009)</ref>. Various emission data sets that use satellitebased remote sensing or other black carbon (BC) proxies are available for wildfires <ref type="bibr">(van der Werf et al., 2004;</ref><ref type="bibr">Van Marle et al., 2017)</ref>. Here, we employed the Coupled Model Intercomparison Project (CMIP6) wildfire data set as the source of BC emissions <ref type="bibr">(Van Marle et al., 2017)</ref>, taking advantage of its coverage of both natural fires and human influence on wildfires, including deforestation fires and control of current wildfires. To convert BC to Mn concentrations, we calculated the Mn to BC ratios in coarse (PM 10 ) and fine (PM 2.5 ) fractions (similar to <ref type="bibr">Hamilton et al., 2022;</ref><ref type="bibr">Mahowald et al., 2005)</ref> using observational data at specific sites located in the Amazon rainforest and upper southern Africa dominated by wildfires <ref type="bibr">(Maenhaut et al., 1999;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, Rajta, et al., 2000;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, et al., 2002)</ref>. We derived a ratio of 10.58 mg g -1 for the coarse fraction and 0.23 mg g -1 for the fine fraction and estimated global wildfire contributions to be 43 Gg Mn year -1 with a range of 21-210 Gg Mn year -1 (Table <ref type="table">1</ref>). These values are higher than those reported in <ref type="bibr">Nriagu (1989)</ref> based on more observations.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.7.">Industrial Emissions</head><p>Industrial emissions of Mn include anthropogenic fossil-fuel combustion, biomass burning, and related activities.</p><p>Because Mn has many biogeochemical properties similar to those of Fe <ref type="bibr">(Canfield et al., 2005)</ref>, we assumed the co-occurrence of Mn with Fe and used an updated detailed Fe emission inventory for 2010 developed using a Speciated Pollutant Emissions Wizard <ref type="bibr">(Bond et al., 2004;</ref><ref type="bibr">Rathod et al., 2020)</ref>. This inventory covers Fe emission from fossil fuel burning, wood combustion, and smelting in the industrial, transport, and residential sectors globally <ref type="bibr">(Alves et al., 2011;</ref><ref type="bibr">Arditsoglou et al., 2004;</ref><ref type="bibr">Block &amp; Dams, 1976;</ref><ref type="bibr">C&#243;rdoba et al., 2012;</ref><ref type="bibr">Davison et al., 1974;</ref><ref type="bibr">de Souza et al., 2010;</ref><ref type="bibr">Dreher et al., 1997;</ref><ref type="bibr">H. K. Hansen et al., 2001;</ref><ref type="bibr">Huffman et al., 2000;</ref><ref type="bibr">Koukouzas et al., 2007;</ref><ref type="bibr">Linak et al., 2000a</ref><ref type="bibr">Linak et al., , 2000b;;</ref><ref type="bibr">Machado et al., 2006;</ref><ref type="bibr">Mamane et al., 1986;</ref><ref type="bibr">Martinez-Tarazona et al., 1990;</ref><ref type="bibr">Meij, 1994;</ref><ref type="bibr">Querol et al., 1995;</ref><ref type="bibr">Schmidl et al., 2008;</ref><ref type="bibr">R. D. Smith et al., 1979;</ref><ref type="bibr">Steenari et al., 1999;</ref><ref type="bibr">Stegemann et al., 2000;</ref><ref type="bibr">Tsai &amp; Tsai, 1998;</ref><ref type="bibr">Watson et al., 2001;</ref><ref type="bibr">H. Zhang et al., 2012)</ref>. We then used estimates of the ratio of Mn to Fe in each type of source to obtain a new emission inventory for Mn (Table <ref type="table">S2</ref> in Supporting Information S1). Detailed data and citations are provided in Data Set S3. We estimated the global industrial emission to be 69 Gg Mn year -1 and assign an uncertainty of 35-350 Gg Mn year -1 (Table <ref type="table">1</ref>), assuming that the overall range will have one order of magnitude uncertainty. There is still a large uncertainty in these first estimates of Mn, and we consider elevated sources as well in later sections to better match the observational data.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Global Biogeochemical Cycles</head><p>10.1029/2023GB007967</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.3.">Atmospheric Observations</head><p>Atmospheric observations of Mn concentrations in particulate matter (PM) were compiled and compared with the model output to assess the performance and tune the model. We compiled atmospheric Mn observational data from a variety of global data set networks and sites <ref type="bibr">(Wiedinmyer et al., 2018)</ref>. The available data were collected using a variety of time periods and using different chemical speciation analyses as described in detail in each study (Data Set S2). Most of the data were collected with size segregation between PM 2.5 and PM 10 size categories (e.g., <ref type="bibr">Hand et al., 2019)</ref>. Some observational studies used coarse (PM 10-2.5 with aerodynamic diameter between 2.5 and 10 &#956;m) and fine (PM 2.5 ) size categories instead (e.g., <ref type="bibr">Maenhaut et al., 1999;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, Rajta, et al., 2000;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, et al., 2002)</ref>. In this case, the two sizes were summed to compute PM 10 for model comparison. X-ray fluorescence is the most frequently used detection method to measure Mn concentrations. The Mn quantification was unavailable at some stations if concentrations were lower than their method detection limit (MDL). In other sites Mn was measured using inductively coupled plasma mass spectrometry (ICP-MS). In total, we obtained more data points for PM 2.5 (N = 699) than PM 10 (N = 204) because many sites focused only on PM 2.5 , such as from the Interagency Monitoring of Protected Visual Environments (IMPROVE) remote/rural network in the US <ref type="bibr">(Hand et al., 2017</ref><ref type="bibr">(Hand et al., , 2019))</ref>. Detailed descriptions of site and method, as well as other elemental/total Mn PM data can be found within each referenced study (Data Set S2). While there exists limited deposition elemental data, there was not enough data to warrant detailed comparisons here, and the absolute values of dry deposition were often difficult to measure <ref type="bibr">(Prospero et al., 1996;</ref><ref type="bibr">Schutgens et al., 2016)</ref>. We ignored particles larger than 10 &#956;m in aerodynamic diameter here, because of the limited data, although the missed fraction of aerosols could be important for biogeochemistry in some regions <ref type="bibr">(Adebiyi et al., 2023)</ref>. <ref type="bibr">Hand et al. (2019)</ref> reported that collocated sites from the US Environmental Protection Agency (EPA) and IMPROVE recorded different coarse aerosol mass (PM 10-2.5 ), with the value at EPA sites being 10% higher than at IMPROVE sites and a 28% difference between these estimates, suggesting that different samplers could have different acuteness of size fractionation for PM 10 and PM 2.5 <ref type="bibr">(Hand et al., 2019)</ref>. Overall, with a correlation coefficient of 0.9 and a slope of 0.9, the two sets of sites agreed with each other, but the difference brought by sampler biases should still be noted during later analysis and evaluation <ref type="bibr">(Hand et al., 2019)</ref>.</p><p>For comparison with the model, we computed annual means of atmospheric Mn concentration for each site. Particulate Mn has very low concentrations (&lt;1 &#956;g-m -3 ), and therefore in many cases the data can be below the detection limit. We applied the same procedure used by <ref type="bibr">Wong et al. (2021)</ref> to correct for this potential bias. If a site had more than half of its data values above the detection limit, we set the value of any samples below MDL at this site to be one-third of the MDL (shown in Data Set S2). If more than 50% of the data was below the MDL at a site, we did not include it in comparison to the model. These data were instead used to compute an upper bound based on their respective detection limits. Since many sites were close together in regions such as Europe and US, to better display the data and show the model comparison, observational data from different sites were averaged spatially within a grid cell that was two times the model resolution, or &#8764;2&#176;&#215; 2&#176; <ref type="bibr">(Schutgens et al., 2016)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.4.">Estimation of Pseudo-Turnover Time</head><p>The importance of atmospheric Mn deposition to the upper soil Mn reservoir was evaluated by calculating the soil Mn turnover time, which is defined as the total mass of Mn in upper soil (estimated to 1 m depth) in each grid cell divided by the estimated atmospheric deposition flux from simulation. The Mn mass was calculated using the average bulk density of soil, 1.4 g cm -3 (C. <ref type="bibr">Yu et al., 1993)</ref>, and the Mn concentration, which was derived by both assuming a constant Mn concentration as in upper continental crust (base case) and applying the Mn concentration from the interpolated soil map with assigned uncertainty as upper and lower bounds for sensitivity studies. The turnover time estimated here is "pseudo-turnover time" <ref type="bibr">(Wong et al., 2021)</ref> because we could not assume soil Mn to be in a steady state. The characterization of the pseudo-turnover time and comparison on a global scale allowed us to assess the ecological significance of atmospheric Mn deposition in the soil Mn reservoir in units of kiloyears <ref type="bibr">(Okin et al., 2004)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.5.">Correlation Analysis and Interpretation of Ecological Relevance</head><p>Whalen <ref type="bibr">et al. (2018)</ref> suggested Mn limitation as a mechanism for reduced decomposition under enhanced atmospheric N deposition; therefore, it might be helpful to consider Mn deposition together with N deposition. We</p><p>Global Biogeochemical Cycles 10.1029/2023GB007967 adopted a modeled annual N deposition data set (2&#176;&#215; 2&#176;) <ref type="bibr">(Brahney et al., 2015)</ref> and re-gridded our model output of the Mn deposition onto its resolution (2&#176;&#215; 2&#176;), followed by raster calculation of the ratio of atmospheric Mn deposition to N deposition, which might provide useful insights for the relative susceptibility of soil to Mn limitation following N deposition. We compared the Mn over N ratio in deposition to the concentration ratio in soils using total N concentration data at available National Cooperative Soil Survey (NCSS) sites. The ratio was computed using both natural Mn deposition and total Mn deposition (natural + anthropogenic) to understand how and where human activities altered this ratio.</p><p>To examine how atmospheric Mn deposition potentially influences the Mn limitation that could be related to decomposition and soil C storage in forest ecosystems <ref type="bibr">(Kranabetter et al., 2021;</ref><ref type="bibr">J. A. M. Moore et al., 2021;</ref><ref type="bibr">Stendahl et al., 2017;</ref><ref type="bibr">van Diepen et al., 2015;</ref><ref type="bibr">Whalen et al., 2018)</ref>, we performed a spatial correlation analysis between Mn deposition and topsoil (0-5 cm) C density derived from SoilGrids 2.0, a digital soil database that includes 230,000 soil profile observations from the World Soil Information Service and applies machine learning methods <ref type="bibr">(Poggio et al., 2021)</ref> to map the global distribution of soil properties at 250 m, resampled to our model resolution (1&#176;&#215; 1&#176;). Mn deposition outputs derived from both the constant base case and the IDW interpolation case were compared to see how sensitive the correlation is to different approaches to calculating the Mn amounts in dust. We identified the ecosystem type at each grid cell using the plant functional types in the Community Land Model, version 5 <ref type="bibr">(Lawrence et al., 2019)</ref>, taking the rubric of having more than 80% of the area covered by forest biomes. Because different forest ecosystems may have distinct soil Mn status and limitation conditions <ref type="bibr">(Berg et al., 2010)</ref>, they were divided into three subsystems: temperate forests, subtropical and tropical forests, and boreal forests, with the correlation analysis conducted both combinedly and separately.</p><p>Because SOM decomposition has long been understood to be controlled by a combination of several different factors, Mn deposition cannot be interpreted separately from other commonly outlined predictors such as precipitation (moisture), temperature, and N deposition <ref type="bibr">(Berg &amp; Matzner, 1997;</ref><ref type="bibr">Frey et al., 2014;</ref><ref type="bibr">Hartley et al., 2021;</ref><ref type="bibr">Sierra et al., 2015;</ref><ref type="bibr">Woo &amp; Seo, 2022;</ref><ref type="bibr">Zak et al., 2017;</ref><ref type="bibr">L. Zhang et al., 2019;</ref><ref type="bibr">F. Zhao et al., 2021</ref>). To include these potential constraints, simple and multilinear regression analyses were carried out with the addition of the three other factors: precipitation, temperature (long-term mean data from Terrestrial Air Temperature and Precipitation: 1900-2014 Gridded Monthly Time Series data provided by the NOAA PSL, Boulder, Colorado, USA, from their website at <ref type="url">https://psl.noaa.gov</ref>), and N deposition to test the significance of Mn deposition on topsoil C density. The multilinear regression was calculated following the ordinary least squares (OLS) method.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.">Results</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.1.">Mn Concentration in Atmospheric Particulate Matter (PM)</head><p>Mn in the model output was compared with the Mn concentration in atmospheric PM observation on a global scale. Here, we present three cases (Figures <ref type="figure">2</ref> and <ref type="figure">3</ref>) for the simulation with dust emission schemes created by linear interpolation (Section 2.1) to better examine the model sensitivity to anthropogenic emissions. We used the bounded observational data (Section 2.3) for all comparisons and scatter plots.</p><p>The natural case (Figure <ref type="figure">2a</ref>) was simulated without any emission from anthropogenic sources (industrial emission + agricultural dust). With only natural contributions, the model underestimated Mn concentration significantly in the PM 10 size fraction (Figure <ref type="figure">2b</ref>), especially over industrialized regions in Asia, Europe, and southern Africa, where the world's largest Mn mining industry is located (U.S. Geological Survey, 2022). The model also poorly simulated the relatively high Mn concentrations reported by several sites across North America. Only close to dust desert dominated regions in North Africa does the model simulate the concentrations well (Figure <ref type="figure">2a</ref>). The spatial distribution of Mn in western North Africa agrees with the observations on the location of Mn rich dust sources <ref type="bibr">(Rodr&#237;guez et al., 2020)</ref>.</p><p>When anthropogenic sources were added, using the default values described in Section 2.2, the model improved the simulation in industrialized regions (Figure <ref type="figure">3b</ref> and Figure <ref type="figure">S9</ref> in Supporting Information S1). The value of the correlation coefficient (r) increased 3-fold with RMSE on the same level (r = 0.089, RMSE = 0.025 in Figure <ref type="figure">2b</ref>; r = 0.27, RMSE = 0.023 in Figure <ref type="figure">3b</ref>), suggesting that the model performance improved with the addition of anthropogenic contributions. However, Mn concentrations at the major proportion of sites were still underestimated compared with the observations. Through iterative tuning, we found that the atmospheric concentrations were best matched when we increased the anthropogenic emissions by a factor of 1.9 (Text S1 in Supporting</p><p>Global Biogeochemical Cycles 10.1029/2023GB007967 Information S1). We defined our "best estimate" as the case with elevated anthropogenic emissions (Figures <ref type="figure">3a</ref> and <ref type="figure">3b</ref>) and denoted the unmodified scenario the "low anthro" case (Figure <ref type="figure">3c</ref>). While some stations were overestimated in the best estimate case, much fewer stations were, and the data spots were distributed more uniformly along the 1:1 line of the scatter plots, with r increased to 0.36. In many of the sites, there was a mismatch between the date of the measurement and the model simulation because of limited observations.  <ref type="bibr">Arimoto et al., 2003</ref><ref type="bibr">Arimoto et al., , 2006;;</ref><ref type="bibr">Artaxo et al., 2002;</ref><ref type="bibr">Atanacio &amp; Cohen, 2020;</ref><ref type="bibr">Barraza et al., 2017;</ref><ref type="bibr">Bergametti et al., 1989;</ref><ref type="bibr">Bozlaker et al., 2013</ref><ref type="bibr">Bozlaker et al., , 2019;;</ref><ref type="bibr">Y. Chen et al., 2006;</ref><ref type="bibr">Chuang et al., 2005;</ref><ref type="bibr">Cohen et al., 2004;</ref><ref type="bibr">DFM &amp; WSP, 2020;</ref><ref type="bibr">Dongarr&#224; et al., 2007</ref><ref type="bibr">Dongarr&#224; et al., , 2010;;</ref><ref type="bibr">European Monitoring and Evaluation Programme, 2020;</ref><ref type="bibr">Fuzzi et al., 2007;</ref><ref type="bibr">Gianini, Fischer, et al., 2012;</ref><ref type="bibr">Gianini, Gehrig, et al., 2012;</ref><ref type="bibr">Hand et al., 2017;</ref><ref type="bibr">Hsu et al., 2016;</ref><ref type="bibr">Hueglin et al., 2005;</ref><ref type="bibr">Kyll&#246;nen et al., 2020;</ref><ref type="bibr">Laing et al., 2014a</ref><ref type="bibr">Laing et al., , 2014b;;</ref><ref type="bibr">Mackey et al., 2013;</ref><ref type="bibr">Maenhaut &amp; Cafmeyer, 1998;</ref><ref type="bibr">Maenhaut, Cafmeyer, et al., 1997;</ref><ref type="bibr">Maenhaut, De Ridder, et al., 2002</ref><ref type="bibr">, Maenhaut, Fern&#225;ndez-Jim&#233;nez, et al., 2002;</ref><ref type="bibr">Maenhaut et al., 1999</ref><ref type="bibr">Maenhaut et al., , 2005</ref><ref type="bibr">Maenhaut et al., , 2008</ref><ref type="bibr">Maenhaut et al., , 2011;;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, Rajta, et al., 2000;</ref><ref type="bibr">Maenhaut, Fern&#225;ndez-Jim&#233;nez, Vanderzalm, et al., 2000;</ref><ref type="bibr">Maenhaut, Francois, et al., 1997;</ref><ref type="bibr">Maenhaut, Koppen, &amp; Artaxo, 1996;</ref><ref type="bibr">Maenhaut, Salma, et al., 1996;</ref><ref type="bibr">Maenhaut, Salomonovic, et al., 1996;</ref><ref type="bibr">Malm et al., 2007;</ref><ref type="bibr">McNeill et al., 2020;</ref><ref type="bibr">Mkoma, 2008;</ref><ref type="bibr">Mkoma et al., 2009a</ref><ref type="bibr">Mkoma et al., , 2009b;;</ref><ref type="bibr">Morera-G&#243;mez et al., 2018;</ref><ref type="bibr">Nyanganyura et al., 2007;</ref><ref type="bibr">Perez et al., 2008;</ref><ref type="bibr">Putaud et al., 2004</ref><ref type="bibr">Putaud et al., , 2010;;</ref><ref type="bibr">Rodr&#237;guez et al., 2011</ref><ref type="bibr">Rodr&#237;guez et al., , 2015;;</ref><ref type="bibr">Salma et al., 1997;</ref><ref type="bibr">Savoie et al., 1993;</ref><ref type="bibr">Smichowski et al., 2004;</ref><ref type="bibr">Swap et al., 2002</ref>; UK Department for Environment, Food, and Rural Affairs, n.d.; <ref type="bibr">Vanderzalm et al., 2003;</ref><ref type="bibr">Virkkula et al., 1999;</ref><ref type="bibr">Xiao et al., 2014)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Global Biogeochemical Cycles</head><p>10.1029/2023GB007967</p><p>We noticed that a few sites with high Mn concentrations across North America, including several peaks in the central United States, were still missed by the model in the best estimate case, suggesting that our estimation of anthropogenic source contributions could be lower than the actual in this region. Overall, our model agreed on the same order of magnitude of Mn concentration in atmospheric PM 10 as the observations and had the ability to, at least, partially represent the variability in their spatial distribution.</p><p>Despite the dominance of the PM 10 size fraction of the atmospheric Mn budget due to the coarse nature of dust (Table <ref type="table">1</ref>), Mn in atmospheric PM 2.5 is also important because of the high percentage of fine fraction in wildfires and industrial dust (Table <ref type="table">1</ref>) and the potential health risks that could be induced by inhalation of Mn in PM 2.5 in ambient air <ref type="bibr">(Cavallari et al., 2008;</ref><ref type="bibr">Exp&#243;sito et al., 2021)</ref>. Generally, we obtained similar global distribution patterns and results of the model-observation comparison as in PM 10 . With a more than tripled number of atmospheric Mn observations in the PM 2.5 size fraction, especially in the U.S., the model simulation better matched the observations across North America (Figure <ref type="figure">4a</ref>). The highest observation values were reported over industrialized regions in Europe and Asia and regions affected by desert dust generated in North Africa. Our model showed elevated atmospheric Mn levels in Europe and Asia compared to the Americas. Similarly, atmospheric Global Biogeochemical Cycles 10.1029/2023GB007967</p><p>Mn over industrialized regions was underrepresented by the model simulations in the natural case (Figure <ref type="figure">S2</ref> in Supporting Information S1), and we derived our best estimate by tuning the level of anthropogenic emissions toward the higher end by a factor of 1.9. With the best estimate case, our model showed a moderately good representation of the observations (Figures <ref type="figure">4b</ref> and <ref type="figure">4c</ref>). Having more observational sites might explain the slightly better performance of the comparison in the PM 2.5 size fraction than in the PM 10 size fraction.</p><p>We performed the same analysis using model simulations with constant soil Mn fraction (base case) and found the results changed quantitatively but not qualitatively (Figure <ref type="figure">S3</ref> in Supporting Information S1). Surface Mn concentration was elevated in regions affected by desert and agricultural dust (e.g., larger impact of Saharan dust on the Americas and central Asia) in the base case with higher aerosol budgets in these two sources (Table <ref type="table">1</ref>), Both methods produced simulation results that were of similar order of magnitude as the observations, but the model built with interpolation was determined to be a better match because of its stronger correlation and smaller RMSE (Figure <ref type="figure">3</ref> and Figure <ref type="figure">S3</ref> in Supporting Information S1). </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Global Biogeochemical Cycles</head><p>10.1029/2023GB007967</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.2.">Atmospheric Mn Budget and Source Apportionment</head><p>Our model predicted the global total Mn emission to be 1,400 Gg Mn year -1 with a range of 730-9,700 Gg Mn year -1 due to the uncertainty in each source (Table <ref type="table">1</ref>). The estimate was similar in magnitude to the reference value of 1,000 Gg Mn year -1 given by <ref type="bibr">Mahowald et al. (2018)</ref>. The model-simulated budget for each source was within or close to the estimated range from previous studies <ref type="bibr">(Mahowald et al., 2018;</ref><ref type="bibr">Nriagu, 1989)</ref>. The model estimated that 1,000 Gg Mn year -1 was emitted from natural sources with a range of 500-5,000 Gg Mn year -1 , while 440 Gg Mn year -1 was emitted from anthropogenic sources with a range of 225-2,300 Gg Mn year -1 (Table <ref type="table">1</ref>), suggesting that 31% (best estimate, with uncertainty ranging from 4% to 82%) of the atmospheric Mn arose from anthropogenic contribution.</p><p>While anthropogenic sources contributed to a significant portion of the total atmospheric Mn budget, our model suggested that their main influence was in the Northern Hemisphere, where the ratio of total to natural deposition was significantly greater than 1 (Figure <ref type="figure">5</ref>), and there was a high percentage of anthropogenic or industrial dust (Figures <ref type="figure">6c</ref> and <ref type="figure">6d</ref>), especially over industrialized regions in Asia, Europe, and the northeastern U.S. Hot spots in the Southern Hemisphere included eastern and southeastern Brazil, Peru, Chile, and southern Africa. High ratios of total to natural deposition in these regions indicated strong human perturbations (up to 10 times higher) on the Mn deposition rates (Figure <ref type="figure">5c</ref>). Industrial emissions were responsible for major regions dominated by anthropogenic deposition, while the distribution of agricultural deposition was more dispersed, with a wider coverage of cultivated areas worldwide (Figures <ref type="figure">6c</ref> and <ref type="figure">6d</ref>).</p><p>Desert dust represented over 90% of all natural sources of the atmospheric Mn deposition (Table <ref type="table">1</ref>). It dominated deposition within major deserts in North Africa, inland Australia, and Asia as well as regions that were affected by the transportation of desert dust produced in these systems <ref type="bibr">(Kellogg &amp; Griffin, 2006)</ref>. For example, the Global Biogeochemical Cycles 10.1029/2023GB007967</p><p>intercontinental transport of African dust to South America has been identified as an important source of new atmospheric deposition of P in the Amazon and could have a fertilization effect <ref type="bibr">(Okin et al., 2004;</ref><ref type="bibr">Ridley et al., 2012;</ref><ref type="bibr">H. Yu et al., 2015)</ref>. The dominance of desert dust and other natural sources (sea salts and volcanoes, which represented a very small fraction) was complementary with anthropogenic sources: desert dust dominated most of the Southern Hemisphere but became less influential at higher latitudes in the Northern Hemisphere as anthropogenic emissions concentrated there (Figure <ref type="figure">6a</ref>).</p><p>Although wildfires have a much lower budget than desert dust, they are the second-largest natural source of atmospheric Mn (Table <ref type="table">1</ref>). Together with PBPs, they were major players in regions that are less affected by desert dust and anthropogenic aerosols, such as the Amazon rainforest, upper southern Africa (and Madagascar), Indonesia, northern Canada and Alaska (Figure <ref type="figure">6b</ref>). Wildfires can displace large amounts of nutrients, including Mn, from terrestrial ecosystems <ref type="bibr">(Kauffman et al., 1995;</ref><ref type="bibr">Mahowald et al., 2005)</ref> which are then replenished by transported dust and sea salts, as well as anthropogenic depositions, similar to what was reported by <ref type="bibr">Wong et al. (2021)</ref> in the case of molybdenum (Mo).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.3.">Soil Mn Pseudo-Turnover Times</head><p>The pseudo-turnover time provides a metric of the ecological importance of atmospheric Mn deposition to the upper soil Mn reservoir <ref type="bibr">(Okin et al., 2004)</ref>. Using linear interpolation, we divided the estimated soil Mn concentration by the model simulated Mn deposition rates to compute pseudo-turnover times in upper soils <ref type="bibr">(Okin et al., 2004)</ref>. The estimated soil Mn pseudo-turnover time varied spatially, ranging from 1,000-10,000 years in regions dominated by desert dust to over 10,000,000 years at higher latitudes (Figure <ref type="figure">7a</ref>). To test the sensitivity of turnover times to different dust schemes, Mn deposition simulated in the base case and the constant Mn soil map were used to compute pseudo-turnover times for comparison (Figure <ref type="figure">7b</ref>). Again, results were qualitatively Global Biogeochemical Cycles 10.1029/2023GB007967 consistent despite small quantitative differences (e.g., turnover was slightly retarded in parts of the central and eastern U.S., where relatively high precipitation likely had produced a more advanced stage of weathering, deviating the soil Mn concentration from the upper crust average). We found that anthropogenic sources significantly shortened the soil Mn pseudo-turnover times in industrialized regions regardless of the interpolation method. For example, the atmospheric deposition sourced from anthropogenic emissions shortened the soil Mn pseudo-turnover time by 1-2 orders of magnitude from millions of years to as low as tens of thousands of years in eastern China and across Europe (Figures <ref type="figure">7a</ref>, <ref type="figure">7c</ref> and <ref type="figure">7b</ref>, <ref type="figure">7d</ref>). These trends indicate that human perturbation has the potential to accelerate Mn turnover in different terrestrial systems if the amount of anthropogenic activity remains at the same level or even rises in the future. The upper and lower bounds of the pseudo-turnover times were generated using those of the soil map (Figure <ref type="figure">S6</ref> in Supporting Information S1) and could be viewed as a reference for the uncertainty, which, in general, was within 0-1 order of magnitude as the estimated value.</p><p>Compared to the Mo pseudo-turnover time of 1,000-2,000,000 years <ref type="bibr">(Wong et al., 2021)</ref>, the estimated range of soil Mn pseudo-turnover times is wider, and the mean turnover time is longer, which is closer to the estimated range of P pseudo-turnover time (&#8764;104 to &#8764;107 years) in <ref type="bibr">Okin et al. (2004)</ref>. In the Amazon region, the soil Mn pseudo-turnover time ranged from hundreds of kiloyears in the northeast corner, which was subject to deposition from transported African dust, to thousands of kiloyears moving toward the central and southwestern regions.</p><p>Compared to the turnover times from other studies of macronutrients, the estimated Mn pseudo-turnover time here is orders of magnitude longer than the N turnover time of 177 years globally <ref type="bibr">(Rosswall, 1976)</ref> and the P turnover time of 50 years averaged across several stations in the Amazon rain forest <ref type="bibr">(Mahowald et al., 2005)</ref>, which was accelerated by human-induced land use change such as deforestation and biomass burning <ref type="bibr">(Andela et al., 2017;</ref><ref type="bibr">M. C. Hansen et al., 2013)</ref>. Overall, these comparisons illustrate the spatial variability of the soil Mn Global Biogeochemical Cycles 10.1029/2023GB007967 pseudo-turnover times and suggest that atmospheric deposition of Mn may play a non-negligible role in the terrestrial surface Mn cycle in many regions globally.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.4.">Linkage to N Deposition and C Storage</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.4.1.">Mn to N Ratio in Deposition</head><p>In addition to characterizing the atmospheric Mn cycle itself, we tested linkages of Mn availability to surface soil C observations and projected N deposition. Mn limitation has been proposed to explain the reduced organic matter decomposition in soils under chronic atmospheric N deposition (J. A. M. <ref type="bibr">Moore et al., 2021;</ref><ref type="bibr">Whalen et al., 2018)</ref>, which has the potential to regulate carbon sequestration in forest soils. Here, we calculated an Mn-to-N atmospheric deposition ratio, as low Mn-to-N deposition ratios could indicate where N deposition could slow lignin decay and thus facilitate soil carbon accumulation, while high Mn-to-N ratios could indicate where surface soils may not increase in soil carbon accumulation even with high N deposition rates alone.</p><p>We found that the ratio of Mn to N in the atmospheric deposition varies globally by several orders of magnitude (Figure <ref type="figure">8a</ref>). It could be as low as 5 &#215; 10 -5 in the northern latitudes and over 0.02 in desert dust dominated regions, where the dust composition is almost entirely of mineral nature with low N content (Davies-Barnard &amp; Friedlingstein, 2020; <ref type="bibr">Kanakidou et al., 2016)</ref>. Though the variability of the ratio is less when narrowed down to forest ecosystems, it still spans orders of magnitudes. Anthropogenic emissions increased the depositional ratio of Mnto-N in most parts of the world (even in Antarctica), with the impact in industrialized regions being the most substantial (Figure <ref type="figure">8a</ref>). When only considering the natural sources, we estimated that the Mn-to-N ratio is moderately low in major industrialized regions including northern Europe, eastern China, and the northeastern U. S., with the U.S. having lower ratios than Asia and Europe in general (Figure <ref type="figure">8b</ref>). Anthropogenic sources enhanced the Mn-to-N ratio in all these regions, with a stronger effect in China and Europe than in the U.S. Other Global Biogeochemical Cycles 10.1029/2023GB007967</p><p>areas with low Mn-to-N ratio under current deposition were either around the equator, where much nitrogen fixation occurred in soils as the source of dust emission (Davies-Barnard &amp; Friedlingstein, 2020), or at higher latitudes. In general, regions less affected by desert dust and anthropogenic aerosols had relatively low Mn-to-N ratios. This could be best illustrated in the Amazon Forest, where the northernmost portion influenced by African dust transportation <ref type="bibr">(Ridley et al., 2012)</ref> had a much higher Mn-to-N ratio than the central part (Figures <ref type="figure">8a</ref> and <ref type="figure">8b</ref>).</p><p>We compared the Mn-to-N ratio in atmospheric deposition to the in-situ ratio of Mn to N concentration in surficial soils at 1,319 available sites (mainly across the U.S.). For example, <ref type="bibr">Kranabetter et al. (2021)</ref> reported 541 mg kg -1 Mn and 0.77% total N in surficial soils in a temperate forest located on southern Vancouver Island. With the measurements in the abovementioned study, we calculated the in-situ Mn-to-N ratio in soil to be 0.067, which is over two orders of magnitude larger than the depositional Mn-to-N ratio of 0.00052 calculated using our gridded model output and the N deposition data set (extracting the value of the grid in which Vancouver Island was located). Considering all available soil observational sites that contained valid measurements of Mn and N concentrations (mainly from the NCSS data set), we obtained a median depositional Mn-to-N ratio of 0.00040 versus a median soil Mn-to-N ratio of 0.21, or typically one to three orders of magnitude lower than the soil concentration ratio (Figure <ref type="figure">8c</ref>). Regions with disproportionally low Mn-to-N ratios in atmospheric deposition are interpreted to be the most susceptible to potential Mn limitation, such as temperate and boreal forests in northeastern U.S., Canada, and northern Europe, in agreement with current field experimental results <ref type="bibr">(Kranabetter et al., 2021;</ref><ref type="bibr">Stendahl et al., 2017;</ref><ref type="bibr">Whalen et al., 2018)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.4.2.">Correlation With Topsoil C Density</head><p>To test the significance of atmospheric Mn deposition in decreasing soil Mn limitation and thus facilitating decomposition in forest ecosystems on a global scale, we correlated our simulated atmospheric Mn deposition with the topsoil (0-5 cm) C density derived from SoilGrids 2.0 <ref type="bibr">(Poggio et al., 2021)</ref> in (sub)tropical, temperate, or boreal forests. In each case, a simple linear regression between topsoil C density and each of the four factors was carried out, including Mn deposition. Our results revealed fairly good negative correlations (r &lt; -0.5) between topsoil organic C density and Mn deposition in temperate (r = -0.67) and (sub)tropical forests (r = -0.52; Figure <ref type="figure">9a</ref>). A similar negative relationship was determined between C density and N deposition in temperate forests (r = -0.69; Figure <ref type="figure">9b</ref>), where a significant positive relationship was obtained in the case of precipitation (r = 0.71; Figure <ref type="figure">9d</ref>). In addition, a negative correlation between C density and temperature was found only in (sub)tropical forest, though relatively weaker (r = -0.46; Figure <ref type="figure">9c</ref>). When we combined the three forest ecosystems for simple regression analysis, all factors showed statistically significant correlation, with Mn deposition (r = -0.37, p &lt; 0.0001) having the third strongest coefficient of determination (Table <ref type="table">2</ref>).</p><p>Using multilinear regression, we found a negative relationship between C density and Mn deposition across all forests (Table <ref type="table">2</ref>). Overall, the R-squared value of the OLS model reached 0.438, with the skew (-0.121), kurtosis (3.077), and Jarque-Bera test (1.790, p = 0.409) likely indicating normally distributed residuals. To check for multicollinearity, we computed a correlation matrix (Table <ref type="table">S3</ref> in Supporting Information S1) and found a positive correlation between Mn deposition and N deposition (r = 0.63, p &lt; 0.0001), providing the possibility that the negative correlation between topsoil C density and Mn deposition was a "byproduct" of the positive correlation between Mn and N deposition. A calculation of variance inflation factors obtained values &lt;2 for all individual variables (Table <ref type="table">S3</ref> in Supporting Information S1), suggesting that variables were only moderately correlated with each other, and multicollinearity was likely not problematic. Furthermore, we tested the correlation using normalized Mn (Mn-to-N ratio) and found it still negative and statistically significant for temperate and (sub)tropical forests (Figure <ref type="figure">S7a</ref> in Supporting Information S1). Of course, correlations can never show causality, so it is still possible that our results are spurious, but the statistical tests presented here are consistent with our hypothesis. We also conducted a correlation analysis using base case outputs under constant soil Mn assumption and found negative relationship significant regardless of the method we used to calculate Mn in dust (Figure <ref type="figure">S7b</ref> in Supporting Information S1). Therefore, it is reasonable to conclude that the Mn deposition could be a predictor of topsoil C density along with N deposition and other climatic factors in forest ecosystems (predominantly temperate and tropical). In fact, Mn addition to soils has been shown to increase C losses (e.g., CO 2 and dissolved organic carbon) during litter decomposition, suggesting increased Mn supply could result in decreased soil C storage <ref type="bibr">(Jones et al., 2020;</ref><ref type="bibr">Trum et al., 2015)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Global Biogeochemical Cycles</head><p>10.1029/2023GB007967</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.">Discussion</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.1.">Model-Observation Discrepancy</head><p>Although our model simulation results had a moderately good representation of the atmospheric observations under the best estimate scenario, many stations were still under-or over-predicted (Figures <ref type="figure">3</ref> and <ref type="figure">4</ref>). The discrepancy between the model and observations could arise from a variety of processes, with errors in the sources, deposition or transport pathways all contributing <ref type="bibr">(Loosmore, 2003;</ref><ref type="bibr">Mahowald et al., 2011)</ref>. For example, we were not able to include the emissions from direct volcanic eruptions due to the lack of data and thus constrained to apply non-eruptive degassing data only. Errors in estimates of dust deposition were thought to be of order of a factor of 10 <ref type="bibr">(Mahowald et al., 2011)</ref>. Because we derived Mn from industrial sources from a correlation with Fe (since these are the only spatially explicit mining emissions available: <ref type="bibr">Rathod et al., 2020)</ref>, emissions from nonferrous industries such as silico-manganese alloy, synthetic pyrolusite, and Mn chemical manufacturing plants were neglected <ref type="bibr">(Parekh, 1990)</ref>. Estimates of Table 2 Result Statistics of Simple and Multilinear Regression Between Topsoil C Content and Mn Deposition, N Deposition, Temperature, and Precipitation Variable name Simple linear regression Multilinear regression r p-value coef t P &gt; |t| Intercept 500.2603 39.248 0.000 Mn deposition -0.391 &lt;0.0001 -0.0114 -4.738 0.000 N deposition -0.493 &lt;0.0001 -0.0661 -7.505 0.000 Temperature 0.270 &lt;0.0001 4.1114 9.371 0.000 Precipitation 0.472 &lt;0.0001 8.9193 10.031 0.000 Global Biogeochemical Cycles 10.1029/2023GB007967 fugitive emissions from mining were not available, and thus not included in this study.</p><p>Another limitation is that, except for desert and agricultural dust, we used a constant emission factor for each source because we did not have sufficient data to assess the spatial variability of the Mn emission factors from different sources such as PBP, sea sprays, and volcanoes, which could vary within the ranges given in <ref type="bibr">Nriagu (1989)</ref>. For example, trace element composition could vary in materials formed by biological production in different water masses <ref type="bibr">(Kuss &amp; Kremling, 1999)</ref>. With the constant emission factor assumption, our model could over-or underestimate the observations, depending on the location of the site and its source apportionment.</p><p>While we found a negative correlation between topsoil C density and our simulated atmospheric Mn deposition in (sub)tropical and temperate forests, we did not find a relationship in boreal forests. These results are surprising given the observational findings from northern Swedish boreal forests, where Mn was found to act as a critical factor regulating C accumulation <ref type="bibr">(Stendahl et al., 2017)</ref>. This apparent discrepancy might be attributed to the limited number of soil observations within the boreal regime, introducing large uncertainty at the higher latitudes in our linear-interpolated soil map. With most soil observations located around the middle latitudes, it would not be surprising that we found stronger relationships than in the higher latitudes.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.2.">Limitations of the Observational Data</head><p>We collected atmospheric observations of Mn over six out of seven continents, but high spatial coverage was mostly restricted to industrialized countries. To improve our understanding of atmospheric contribution to the Mn cycle, more observations of the surface Mn concentration, especially in the coarse size fraction (as PM 10 observations are much fewer than those of PM 2.5 ), in currently less-observed areas such as the higher latitudes are needed to further constrain the model. While the total concentration of PM is commonly monitored, it is the element-specific PM measurements that are more valuable to advancing our understanding of the trace-metal biogeochemical cycles.</p><p>Mn concentration in surface PM was chosen over direct Mn depositional observations for model calibration because of its higher data availability and timeliness. In addition, Mn deposition could be due to particles much larger than PM 10 included here in the model. <ref type="bibr">Herndon et al. (2011)</ref> made an effort to compile observations of Mn deposition, in which many of the reported values were collected in the past century, suitable for historical analysis and comparison but outdated for the tuning of a contemporary model, given that industrial emissions had decreased following environmental regulations in many countries. For example, our estimated Mn deposition was much smaller than the estimates given by <ref type="bibr">Herndon et al. (2011)</ref> in the industrialized areas, while the natural components were more comparable. Another explanation for the difference is that direct depositional observations were usually close to the point emission source, whereas our model estimation was spatially averaged in each grid. As noted above, deposition data includes all size fractions, while here we consider only the size smaller than PM 10 . Moreover, depositional observations are patchier and less systematically compiled; thus the number of them is insufficient for model tuning. However, direct depositional observations are important, and if having enough of them, atmospheric models like this could be tuned with depositional data as well. Therefore, there are still needs for more up-to-date field measurements of metal deposition by size fraction.</p><p>There are more locations with soil Mn measurements than atmospheric observations, but they are concentrated mostly in Europe and the U.S. Because of the uneven distribution of the soil observations and the limited number of them across many countries, we are not able to capture the variability of the soil Mn concentration at finer scales. For example, we did not include in our interpolation approach measurements of Mn concentration at metal-contaminated sites associated with mining or other industries <ref type="bibr">(Lv et al., 2022)</ref>, which could be patchy but important across industrialized regions <ref type="bibr">(Herndon et al., 2011)</ref>, having potential feedbacks on the reemission of the aerosols as dust. We suggest the value of more measurements on not only Mn, but also other trace elements in soils, especially in more developing countries, the higher latitudes, and the tropics. NCSS's soil characterization and USGS's geochemical and mineralogical survey of soils of the conterminous United States (D. B. <ref type="bibr">Smith et al., 2013)</ref> can be proposed as model sampling campaigns which provide extensive and massive aerial coverage as well as highly compiled and sorted data sets.</p><p>Many studies <ref type="bibr">(Baize, 2010;</ref><ref type="bibr">Okin et al., 2004;</ref><ref type="bibr">Wong et al., 2021)</ref> have suggested that soil orders, which are the highest level of taxonomic classification, are typically inadequate when dealing with trace element concentrations Global Biogeochemical Cycles 10.1029/2023GB007967</p><p>in soils, because the intra-order variation is similar to the inter-order variation (Figure <ref type="figure">S8</ref> in Supporting Information S1). Better estimation might be achieved with more refined classification at lower taxonomic levels such as suborders and great groups, or even quantitatively with particle size distribution. However, fewer sites specify the abovementioned information, and at such levels, the conversion between different classification systems is more complex.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.3.">Anthropogenic Perturbation and Implications for C Cycling</head><p>Our model and observations suggest that anthropogenic perturbations played an important role in global atmospheric Mn cycling, contributing about 31% of the total emissions. Anthropogenic sources were the dominant contributor of emissions in most industrialized regions, especially in the northern hemisphere (Figure <ref type="figure">7</ref>) where they significantly accelerated Mn pseudo-turnover times in upper soils by enriching the atmospheric deposition in which the Mn-to-N ratio was boosted. Human activities, including industrialization and agricultural practices, likely alter Mn cycles by a factor of two or more in many associated areas (Figure <ref type="figure">6</ref>), on the same order of magnitude as the perturbation to the cycling of other metals such as Mo, aluminum (Al), lead (Pb), mercury (Hg), and vanadium (V) <ref type="bibr">(Rauch &amp; Pacyna, 2009;</ref><ref type="bibr">Schlesinger et al., 2017;</ref><ref type="bibr">Selin, 2009;</ref><ref type="bibr">Sen &amp; Peucker-Ehrenbrink, 2012;</ref><ref type="bibr">Wong et al., 2021)</ref>.</p><p>The terrestrial ecological relevance of Mn deposition is how it modulates relationships between N deposition and soil C dynamics. Our results reinforce the negative correlation between Mn and topsoil C density in temperate forests globally <ref type="bibr">(Kranabetter et al., 2021;</ref><ref type="bibr">Stendahl et al., 2017)</ref>, suggesting Mn availability is likely a limiting factor in SOM decomposition. This implies that if atmospheric deposition is the major source of Mn in surficial soil layers, it has the potential to facilitate oxidative C decomposition by reducing Mn limitation, and in regions that are sensitive to anthropogenic activities, humans might indirectly alter the C cycle by releasing Mncontaining aerosols into the atmosphere through industrial and agricultural activities. While a significant proportion of global C is stored in the soils and vegetation of temperate forests <ref type="bibr">(IPCC, 2000)</ref>, increased C emissions from decomposition promoted by Mn addition could be important to global C dynamics and climate feedbacks, exacerbating the ongoing escalating C emissions subjected to wildfires <ref type="bibr">(Phillips et al., 2022;</ref><ref type="bibr">B. Zhao et al., 2021)</ref>. Furthermore, our correlation analysis indicates a negative Mn-C relationship in (sub)tropical forests in addition to temperate forests, where empirical relationships between Mn and soil C have been found. This calls for additional research into Mn deposition and its dynamics associated with soil C turnover in (sub)tropical forest ecosystems.</p><p>Most of the current studies of Mn-C dynamics measured total Mn concentration or extractable/available Mn from soils or litter layers, and very few considered the contribution of atmospheric deposition to surface soils. Direct field studies that correlate Mn deposition and C turnover would help determine the mechanisms behind the broad scale patterns predicted by our model. More field measurements and experimental studies are required to further quantify the influence of Mn deposition on C cycling. For example, our current understanding would be improved if SOM at different stages of decomposition could be distinguished. <ref type="bibr">Berg et al. (2007)</ref> points out that Mn addition has a stronger effect on late-stage decomposition by enhancing lignin-degrading enzymes because microbes tend to decompose lignin after the more labile organic substrates <ref type="bibr">(Berg, 2014;</ref><ref type="bibr">Berg &amp; Matzner, 1997)</ref>. In addition, we focused on modeling the total extractable and/or acid digested Mn in soils and atmospheric deposition and did not consider Mn bioavailability explicitly, which is crucial to the microorganisms that are responsible for decomposition and can be regulated by the cycling of Mn in different oxidation states <ref type="bibr">(Keiluweit et al., 2015)</ref>. Incorporation of mechanisms constraining the bioavailability, mobility, and reactivity of Mn <ref type="bibr">(Keiluweit et al., 2015)</ref> in future model calibrations is essential for a more accurate interpretation. Finally, our estimated pseudo-turnover time and the Mn-to-N ratio could only partially represent the Mn status in soils because we did not include fluxes from other reservoirs in the Mn cycle. For instance, release of Mn(II) from clay mineral weathering and Mn(III, IV)-oxide reduction <ref type="bibr">(Canfield et al., 2005)</ref> could increase the available Mn concentration in soils, creating the gap between the Mn-to-N ratio in deposition and in soils.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.">Conclusions</head><p>In this study, we present, for the first time, a spatially explicit estimation of global atmospheric Mn sources, distribution, and deposition using a combined model-observation approach. We estimate that anthropogenic sources (440 Gg Mn year -1 ) represent approximately 31% of the total atmospheric Mn budget (1,400 Gg Mn Global Biogeochemical Cycles 10.1029/2023GB007967 year -1 ). Including this portion of Mn emissions in the model enhanced Mn deposition in many industrialized regions, which could accelerate soil Mn turnover as high as 100-fold and boost the Mn-to-N ratio in atmospheric deposition. Deposition of anthropogenic Mn from human activities has a high potential to facilitate SOM decomposition in temperate and (sub)tropical forest ecosystems, thus influencing C storage and the global C cycle. Given the scarcity of observations and limited understanding of atmospheric Mn sources, uncertainties are high in these estimations. Additional atmospheric and soil observations across different landscapes will help refine our model and the quantification of global biogeochemical cycles of trace metals like Mn. <ref type="bibr">Zhao, F., Wu, Y., Hui, J., Sivakumar, B., Meng, X., &amp; Liu, S. (2021)</ref>. Projected soil organic carbon loss in response to climate warming and soil water content in a loess watershed. Carbon Balance and Management, 16(1), 24. <ref type="url">https://doi.org/10.1186/s13021-021-00187-2</ref> Zorer, &#214;., <ref type="bibr">Ceylan, H., &amp; Do&#287;ru, M. (2009)</ref>. Determination of heavy metals and comparison to gross radioactivity concentration in soil and sediment samples of the Bendimahi River Basin (Van, Turkey). Water, <ref type="bibr">Air,</ref><ref type="bibr">&amp; Soil Pollution,</ref>, 75-87. <ref type="url">https://doi.org/10.1007/s11270- 008-9758-0</ref> </p></div><note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_0"><p>19449224, 2024, 4, Downloaded from https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023GB007967 by University Of Miami Libraries, Wiley Online Library on [20/08/2024]. See the Terms and Conditions (https://onlinelibrary.wiley.com/terms-and-conditions) on Wiley Online Library for rules of use; OA articles are governed by the applicable Creative Commons License</p></note>
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			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_2"><p>10.1029/2023GB007967</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_3"><p>2015-66299-P &amp; POLLINDUST CGL2011-26259 funded by ERDF and the Research State Agency of Spain.</p></note>
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