Mercury isotopes of atmospheric particle bound mercury for source apportionment study in urban Kolkata

The particle bound mercury (PBM) in urban-industrial areas is mainly of anthropogenic origin, and is derived from two principal sources: Hg bound to particulate matter directly emitted by industries and power generation plants, and adsorption of gaseous elemental mercury (GEM) and gaseous oxidized mercury (GOM) on air particulates from gas or aqueous phases. Here, we measured the Hg isotope composition of PBM in PM10 samples collected from three locations, a traffic junction, a waste incineration site and an industrial site in Kolkata, the largest metropolis in Eastern India. Sampling was carried out in winter and monsoon seasons between 2013–2015. The objective was to understand whether the isotope composition of the PBM represents source composition. The PBM collected from the waste burning site showed little mass independent fractionation (MIF) (D199Hg = + 0.12 to -0.11‰), similar to the signature in liquid Hg and Hg ores around the world with no seasonal variations. Samples from the industrial site showed mostly negative MDF and MIF (δ202Hg = -1.34 to -3.48 ‰ and D199Hg = + 0.01 to -0.31‰). The MDF is consistent with PBM generated by coal combustion however, the MIF is 0.15‰ more negative compared to the Hg isotope ratios in Indian coals. The traffic junction PBM is probably not produced in situ, but has travelled some distances from nearby industrial sources. The longer residence time of this PBM in the atmosphere has resulted in-aerosol aqueous photoreduction. Thus, the MIF displays a larger range (D199Hg = + 0.33 to -0.30‰) compared to the signature from the other sites and with more positive values in the humid monsoon season. Different Hg isotopic signature of PBM in the three different sampling locations within the same city indicates that both source and post emission atmospheric transformations play important roles in determining isotopic signature of PBM.


Introduction
Global anthropogenic mercury (Hg) emissions have been exceeding natural emissions since the industrial revolution (Fitzgerald, 1995;Schuster et al., 2002;Fitzgerald et al., 2005).In the past several decades, emerging economies such as China and India have become the major contributors of anthropogenic Hg emissions (UNEP, 2013), as a consequence of increased production of chlorine, metals, waste incineration, coal combustion, cement production and brick manufacturing (Chen et al., 2014).As atmospheric fallouts are Domain Editor-in-Chief Elementa: Science of the Anthropocene • 4: 000098 • doi: 10.12952/journal.elementa.000098the dominant source of Hg over most of the Earth's surface (Mason et al., 1994;Morel et al., 1998), there is a growing need to quantify atmospheric mercury emission inventories in the Indian subcontinent and China which are home to more than 40% of the global population.
In the atmosphere, Hg exists in two oxidation states, 0 and + 2, and three different operationally defined forms, (G)aseous (E)lemental (M)ercury [GEM; Hg 0 ], (G)aseous (O)xidized (M)ercury compounds [GOM; Hg II ] and (P)articulate/aerosol (B)ound (M)ercury [PBM; Hg (p) ].GEM is the dominant form of atmospheric Hg and generally accounts for >95% of total Hg in uncontaminated air (Schroeder and Munthe, 1998;Liu et al., 2010).GEM has a residence time of 0.5-2 years in the atmosphere and is therefore distributed nearly homogenously around the globe.Studies by Weiss-Penzias et al. (2003) indicated that atmospheric emissions of GEM from Asia can be transported across the Pacific within five days.However as GEM has limited solubility in water, it remains largely unavailable to fish and other living organisms.Atmospheric GEM is ultimately oxidized to GOM which is water soluble and contributes towards wet deposition (Lin and Pekhonen, 1999).GEM and GOM can bind to aerosols or particles and the particle bound mercury (PBM) can remain in the atmosphere for several weeks before being deposited locally and regionally.The wet and dry deposition of Hg near a point source is dominated by GOM and PBM, respectively (Lin et al., 2006).
In pristine rural environments, GOM and PBM are typically present in concentrations less than 10 pg/m 3 , but in polluted urban-industrial areas and during atmospheric Hg depletion events, their concentration levels can reach in excess of 300 pg/m 3 (Lindberg et al., 2002;Sprovieri et al., 2002;Liu et al., 2010).PBM is largely of anthropogenic origin and can account for up to 40% of total atmospheric Hg in industrialized regions (Xiao et al., 1991).Recent measurements of PBM in several urban/industrial areas have documented that Hg can be associated with large particles (>2.5 µm) and in concentrations similar to those of the vapour phase Hg (ng/m 3 ) (Hacon et al.,1995;Hladíková et al., 2001;Tsai et al., 2003).GOM and PBM therefore form a significant fraction of the total atmospheric Hg emissions, particularly during coal combustion and municipal waste incineration (Capri, 1996;Pirrone et al., 2001).
A major challenge in source apportionment studies of Hg remains in the fact that it is difficult to identify and quantify different sources once Hg is dispersed and intermixed in the environment (Lindberg et al., 2007).The discovery of mass dependent fractionation (MDF) and mass independent fractionation (MIF) of mercury isotopes (Bergquist and Blum, 2007) have opened up the door to a new method for tracing Hg pollution and investigating Hg behaviour in the environment.Hg has seven stable isotopes ( 196 Hg, 198 Hg, 199 Hg, 200 Hg, 201 Hg, 202 Hg and 204 Hg) out of which the two odd mass isotopes undergo MIF, usually yielding products that are anomalously enriched or depleted in 199 Hg and 201 Hg (Bergquist and Blum, 2007;Schauble, 2007;Biswas et al., 2008;Ghosh et al., 2008;Carignan et al., 2009;Das et al., 2009Das et al., , 2013;;Laffont et al., 2009;Sherman et al., 2009Sherman et al., , 2010Sherman et al., , 2012;;Sonke, 2011;Chen et al., 2012;Jackson andMuir, 2012, Perrot et al., 2012;Sonke and Blum, 2013).MIF of an isotope of even mass number ( 200 Hg) has also been detected in atmospheric Hg (Gratz et al., 2010;Chen et al., 2012;Sherman et al., 2012, Rolison et al., 2013, Wang et al., 2015) and has been suggested to be caused by photo-induced oxidation of GEM on the surfaces of aerosols and particles in the tropopause (Chen et al., 2012).
To the best of our knowledge, only one study (Rolison et al., 2013) has looked into the Hg isotopic composition of PBM which can form an important component of atmospheric Hg deposition in urban environments.In the present study, Hg isotopic measurements were performed for PM 10 (particulate matter with size ≤10 micron) samples collected from three locations (a traffic junction, a waste incineration site and an industrial estate) for two seasons, winter and monsoon.The objective of this study was to understand: 1) whether the isotopic composition of the PBM represents the isotopic composition of source, 2) post emission isotopic fractionation during the processes that transport and transform particulate Hg in the atmosphere, and 3) seasonal variation of the isotopic composition of the PBM.

Site description
PBM samples were collected in and around Kolkata (22°32′N, 88°22′E), India in two seasons, winter and monsoon.Kolkata (erstwhile Calcutta) is the capital of West Bengal and is the third most populous city in India according to the 2011 census.The city has a tropical wet and dry climate.The annual mean temperature is 26.8°C with three distinct seasons, summer, monsoon and winter.Winter lasts for about two months between December and January.Temperature starts to rise in the spring months of February to April.The hot and humid summer lasts from May to June with May being the hottest month.Rain lashes the city between June and September brought by the Bay of Bengal branch of the Southwest monsoon.Post monsoon, the temperature cools down during autumn (October-November).Previous studies conducted in different Indian metropolises reported the highest pollutant levels during the cooler months (as the inversion layer remains close to the ground) and the lowest pollutant levels during the monsoon (Chowdhury, 2004;Spiroska et al., 2011;WBPCB, 2012).To capture the seasonal variation of PBM concentrations and isotopic compositions, if any, we specifically collected samples in winter and monsoon seasons between December 2013 and August 2015.Elementa: Science of the Anthropocene • 4: 000098 • doi: 10.12952/journal.elementa.000098Samples were collected from three locations; a traffic junction, a landfill site and a small industrial town (Figure 1).The traffic junction site is a busy crossing in south Kolkata with no major industries located within a 5 km radius.The landfill site, popularly known as Dhapa dumping ground, is located in the eastern fringe of Kolkata.The disposal site has served the City of Kolkata as an uncontrolled dumping ground since 1981.Little or no soil cover has been applied historically.Although Dhapa does not have any incineration plant, it is a common practice to burn waste in the open air.Waste is also burnt at the Bantala Leather Complex behind Dhapa.These burning practices are in the "unorganised sector".The industrial town, Uttarpara is located in the suburbs of Kolkata, approximately 15 km north of the city on the banks of the River Ganges.There are mainly iron foundries and wagon manufacturing companies in Uttarpara Belt.From the sampling location, several flue gas stacks can be observed.The town is well connected to the city of Kolkata by rail and road.Local trains are the most popular mode of transportation and road traffic in Uttarpara is lesser compared to any traffic junctions in Kolkata.

Sample collection
A Deployable Particulate Sampler (DPS) pumps (Leland Legacy) with a pumping efficiency of 10 L/min was used to collect the PM 10 .For each sample the pump ran ∼24-50 hours and sampled ∼14.4-30 cubic meter air.The PM was collected on 47 mm quartz filters.Prior to the sampling, the quartz filters were dried overnight at 400 °C in an oven, weighed and packed in Millipore petri slides with a cover to prevent any contamination.After sampling, filters were immediately sealed in the petri slides and stored in a refrigerator until analysis.

Chemical analysis
The filters were weighed before acid digestion to gravimetrically calculate the PM 10 concentrations.Chemical extraction was carried out within one month of sampling.Depending on PM concentrations, the filters were digested in 8-10 ml, 20% v/v inverse aqua regia (3:1 HNO 3 :HCl) in closed Teflon microwave vessels in a Milestone microwave system (ETOS EZ, Italy).The microwave radiation power was 1200 W, the temperature was ramped to 120°C in 15 minutes and then held at 120°C for 30 minutes.The vessels were opened several hours after cooling down to room temperature.The samples were then filtered through 0.22 µm PES membrane filters.Aliquots of the prepared samples were diluted and analysed for Hg and 5 trace metal (Ni, Cu, Zn, As, and Pb) concentrations using an Agilent 7700 series Inductively Coupled Plasma-Mass Spectrometer (ICP-MS Japan) equipped with a 3 rd generation He reaction/collision cell (ORS 3 ) to minimize interferences, particularly formed from the digestion HCl matrix (Das et al., 2015).The operating conditions used for the analysis of samples are shown in Table S1.The ICP-MS operating parameters, such as torch position, sampling depth, extraction and ion focusing lenses voltages, omega lenses voltages, quadrupole settings, and carrier and blend gas flow rates were optimized daily by aspirating a 1.0 µg/L solution of Ce, Co, Li, Mg, Tl and Y in 2 wt % HNO 3 .Oxides and doubly charged ion ratios were kept below 2%.The 201 Hg isotope was measured, as it is free from polyatomic overlap of WO.Detection Limit (DL) and Background Equivalent Concentration (BEC) for 201 Hg were 7.5 ppt and 42 ppt respectively.HNO 3 and HCl (ultrapure grade) used in the experiment were purchased from J. T. Baker (Canada).Ultra-pure water with 18.2 MΩ -cm resistivity was used (Super-Q; Millipore, USA) for sample and standard preparations.
Hg isotope ratio analyses were performed on a Neptune Plus MC-ICP-MS (Thermo Scientific, Germany) using sample standard (NIST SRM 3133) bracketing technique at the Earth Observatory of Singapore, Nanyang Technological University.The sample solution was reduced to Hg vapour by freshly prepared 3% w/v% SnCl 2 in 1 N HCl in a cold vapor hydride generator (CETAC,200 HGX).Before introduction into the plasma, the Hg vapour was mixed with a dry Tl aerosol (NIST SRM 997, 205 Tl/ 203 Tl=2.38714) from a Cetac Aridus II fitted with an ESI nebulizer for instrumental mass bias correction using exponential fractionation law.Typical instrument sensitivity was 200 mV on 202 Hg in a 1 ppb NIST SRM 3133 Hg standard with an uptake rate of 350 µl min −1 at a 6 rpm pump speed.While measuring the isotope ratios of the samples, total Hg concentrations were also calculated by comparing the signal intensity of 202 Hg in 1 ppb bracketing standards with the sample.The total Hg concentrations of the sample extracts were compared to the values obtained by analysing the samples with the Agilent 7700 series ICP-MS.The maximum differences in concentration obtained by these two different methods were ≤12%.The NIST SRM 3133 bracketing standard was prepared in the same matrix (20% v/v, 3:1 HNO 3 :HCl) as the samples to avoid any matrix effects.
The isotopes 198 Hg, 199 Hg, 200 Hg, 201 Hg, 202 Hg, 203 Tl, and 205 Tl were measured on faraday cups L3, L2, L1, C, H1, H2 and H3, respectively, in static collection mode with a 4 s integration time, and 60 ratios per run.Background corrections were done by beam defocusing.Washout time varied between 5 to 10 minutes until the wash signal stabilized at ≤1% of the preceding measured solution.The MDF of Hg isotopes were expressed as the per mil deviation of the sample relative to the NIST 3133 standard using the delta notation (δ x Hg ‰) and defined by the following equation (Blum and Bergquist, 2007) / 198 Hg) sample / ( xxx Hg/ 198 Hg) SRM 3133] -1) * 1000 MIF of Hg isotopes were defined by the deviation from the theoretically predicted MDF and was expressed as (Bergquist and Blum, 2007),

Blanks, recovery, and uncertainty
A blank filter that was taken to the field was chemically treated in the same way as the samples to determine procedural blank.The total procedural blank, including instrumental background was ≤15 pg and was considered insignificant compared to the amount of Hg extracted from the samples (3.5-10.7 ng).To validate both digestion and ICP-MS methods, blank filters were spiked with Hg standards and treated in the same way as the samples.Recoveries from these spiked filters ranged from 83-96%.The UM-Almaden Hg inter laboratory standard was repeatedly analysed as a secondary standard during the course of analysis.The isotope ratios [δ 202 Hg = −0.55‰± 0.14‰, D 199 Hg = 0.01‰ ± 0.09‰, and D 201 Hg = −0.03‰± 0.11‰ (2SD, n = 12)] are identical within errors to the proposed values by Blum and Bergquist (2007) (Table S3).The values of long-term analytical uncertainties of the UM-Almaden were used as uncertainties on sample Hg isotope compositions.However in those samples where triplicate analyses were performed, we reported the uncertainties determined from our own analyses.

Results
Table S2 summarizes the trace metal concentrations and Hg isotope compositions of 52 PM 10 samples, together with background information including sampling period, average temperature, average humidity, PM 10 concentration, and PBM concentration.Statistical data, e.g.mean, median, 1SD and maximum-minimum values from three locations and in two seasons are reported in Table 1 and Figure   scavenge particulate Hg from the air as evidenced from the large fraction of Hg in rainwater being bound to particles (Munthe, 1993).Secondly, precipitation increases soil humidity, which in turn limits the proportion of wind-blown soil and decreases air particulate concentrations and particulate Hg bound to wind-blown soil material (Fang et. al., 2001).High PM concentrations will likely increase the substrates that Hg can potentially adhere to.Hence, it is not surprising that PM 10 concentrations correlate with PBM concentrations (R 2 = 0.62, Figure S1) as has been observed in other studies (Fang et al., 2001).PBM is a minor form (∼10% of total atmospheric Hg) of anthropogenic Hg, emitted directly to the atmosphere by industrial emissions.It is however often formed by adsorption or partition of gaseous Hg onto a particle surface (Sommar et al., 1997;Brandon et al., 2001).High concentrations of PBM have been reported from many places around the world like Alta Floresta in the Amazon Basin (∼100 ng/m 3 , Hacon et al.,1995), Beijing (0.360-0.440 ng/m 3 , Wang et al., 2002), Taiwan (0.34-5.8 ng/m 3 for PM 2.5 and 0.05-3.1 ng/m 3 for PM 2.5-10 , Tsai et al., 2003), Detroit (0.12-0.55 ng/m 3 , Pirrone et al., 1995), Slovak Republic (0.22-4.47 ng/m 3 , Hladíková et al., 2001).PBM concentrations measured in the present study are comparable with those obtained from the Southeast Asian megacities and industrial cities of the West.However, they are far higher than the reported numbers from US, such as Wisconsin (0.0021-0.028 ng/m 3 , Lamborg et al., 1995), Florida (0.0049-0.0093 ng/m 3 , Guentzel et al., 2001) and are much higher than the background values of 0.001 to 0.086 ng/m 3 (Keeler et al., 1995).

Isotopic composition of atmospheric mercury
The Hg isotope signature is a useful tool in understanding sources, tracking specific chemical pathways and monitoring the sinks (Sonke and Blum, 2013).MDF of Hg isotopes can occur in almost all kinetic and equilibrium reactions (Blum et al., 2014).MIF of odd Hg isotopes (D 199 Hg and D 201 Hg) can be triggered by photochemical reduction of Hg(II) and MeHg, aqueous Hg(II)-thiol complexation under equilibrium conditions, evaporation under equilibrium conditions and abiotic dark reduction (Bergquist and Blum, 2007;Zheng et al., 2007;Estrade et al., 2009;Wiederhold et al., 2010;Zheng and Hintelmann, 2010).In combination, MDF and MIF can be a strong tool to track Hg cycle.
Atmospheric Hg composition has been measured in GEM (Demers et al., 2013, Gratz et al., 2010;Rolison et al., 2013, Sherman et al., 2010;Yin et. al., 2013), GOM (Rolison et al., 2013), PBM (Rolison et al., 2013), precipitation (Chen et al., 2012;Demers et. al., 2013;Gratz et al., 2010;Sherman et al., 2012;Wang et al., 2015) and snow (Sherman et al., 2010).Direct measurements of atmospheric GEM showed negative MIF (D 199 Hg from −0.41 to 0.06‰), consistent with the prediction that atmospheric Hg contains complimentary MIF signatures of aquatic reservoirs (Bergquist and Blum, 2007).However GEM samples collected from diverse localities such as Arctic (Sherman et al., 2010), Great Lake Region (Gratz et al., 2010), a semi-rural coastal environment in Mississippi (Rolison et al., 2013), a forest in northeastern Wisconsin, USA (Demers The PBM was collected in two seasons, winter (W) and monsoon (M) from three locations, waste incineration site, industrial site and traffic junction (n = 52).Following the usual box plot notation, the horizontal line inside the box represents the median, the horizontal lines at the upper and lower end of the box represent the 3 rd and 1 st quartile, respectively.The ends of the whiskers are 1.5 times the inter quartile range (IQR).The outliers are marked beyond the whiskers.doi: 10.12952/journal.elementa.000098.f002Elementa: Science of the Anthropocene • 4: 000098 • doi: 10.12952/journal.elementa.000098et. al., 2013) and Wanshan mercury mine in Guizhou province, SW China showed a wide range of δ 202 Hg (−3.88 to + 0.93‰).Hg in precipitation has significant positive D 199 Hg ranging from -0.16‰ to + 1.16‰ (Demers et. al., 2013;Gratz et al., 2010;Sherman et al., 2010;Chen et al., 2012;Wang et al., 2015) and is thought to be caused by photoreduction in cloud droplets.Recent studies also reported MIF of even Hg isotopes (D 200 Hg) in atmospheric samples, mainly precipitation and snow, that are thought to be triggered by photo-oxidation in the tropopause (Gratz et al., 2010;Chen et al., 2012;Sherman et al., 2012;Wang et al., 2015).However atmospheric Hg isotope composition can be widely variable depending on mixing of different sources and in-source and post-emission fractionation.
The Hg isotope composition of Arctic snow invoked the speculation about the importance of heterogeneous chemistry involving Hg-halogen radical pair intermediates (Sherman et al., 2010).Rain Hg isotope composition stimulated investigations regarding in-cloud photo-reduction and complex reaction mechanisms causing even isotope MIF in upper atmosphere (Chen et al., 2012;Gratz et al., 2010;Sherman et al., 2012;Wang et al., 2015).Measurement of species specific isotope composition of Hg opened up the possibility of measuring Hg isotopes during important atmospheric events like wet and dry deposition (Rolison et al., 2013).As PBM is an important species in urban and polluted environments, isotope fingerprinting of PBM is necessary for an increased understanding of source(s), atmospheric transport and transformation processes.

Waste incineration
In this study, the sampling location was close to the largest municipal dumping site of the city where open burning of waste is a common practice.During incineration, almost 100% of Hg passes in the flue gas (van Velzen et al., 2002).In waste incineration plants, the flue gas containing particulate matter, heavy metals, sulfur dioxide etc. passes through the flue gas cleaning systems that generally causes isotope fractionation (Sun et al., 2013).However, in the present case, open burning of the wastes results in the emission of atmospheric GEM and particulate Hg with similar isotopic composition as that of the waste, with little to no MIF.The main Hg bearing components in municipal solid wastes are batteries, thermometers and thermostats, pigment and paint residues, fluorescent lamps and dental residues (Kearney & Franklin, 1992).All these components use The shaded field is the range for Indian coal after Sun et al. (2014).2SD determined by reproducibility of the UM-Almaden standard and repeat analysis of samples triplicates.The arrow shows -0.5 ‰ shift in δ 202 Hg of PBM relative to feed coal as modelled by Sun et al. (2014).Hg extracted from ores.There is evidence for natural fractionation of Hg isotopes in liquid mercury (δ 202 Hg = -1.06‰ to + 0.05‰ and D 199 Hg = -0.05‰ to + 0.03‰) (Estrade et al. 2009;Laffont et al., 2011), cinnabar (Hintelmann and Lu, 2003;Stetson et al., 2009) and hydrothermal ores and fluids (Smith et al., 2005(Smith et al., , 2008;;Sherman et al., 2009).δ 202 Hg in ore samples can display large variations caused by isotopic fractionation during ore formation (Sherman et al., 2009, Stetson et al., 2009).Statistically significant MIF has not been reported from ore samples.The Hg isotope ratios of PBM measured from the waste incineration site also show small MIF (D 199 Hg = -0.11‰ to + 0.12‰).The δ 202 Hg measured in this study (δ 202 Hg = -0.78‰ to -0.39‰) is similar to cinnabar ores measured by Stetson et al. (2009) from McDermitt, Nevada (δ 202 Hg = -0.70‰ to -0.42‰ and D 199 Hg = -0.04‰ to + 0.04‰) and liquid Hg isotope composition (Estrade et al., 2009;Laffont et al., 2011).However, more studies are required on Hg isotope compositions of Hg bearing municipal wastes to test this hypothesis.

Industrial site
The main industries near the sampling location are iron foundries.The foundries mainly cast gray iron.Hence besides coal combustion, the high temperature metal smelting process can be a potential source of Hg.Basic raw materials used by the foundry units are pig iron and different types of scrap excluding automobile parts.Sometimes alloying elements such as nickel, chromium, copper, vanadium, and titanium are added.To test the main source(s) of Hg in the air particulates, we measured several trace metal concentrations as anthropogenic end members have distinct trace metal signatures (Table S2).For example, coal combustion primarily releases arsenic and lead while metal smelting releases copper, zinc, chromium and nickel, among others (Pacyna, 1987).In our study, Hg shows strong correlation with As (0.74) and Pb (0.71) (Table S4), which indicates the major source to be coal combustion (Pacyna et al., 2010).
To mitigate the effect of long-range transport of PBM from the roads in the urban area to the suburban industrial areas, the sampling pump in the industrial site was placed within close proximity (several hundred meters) of the flue gas stacks.The industry management informed that 70% of the feed coal comes from the local coal fields whereas the rest 30% is Australian coal.Mercury isotopes can be a reliable tool to trace the Hg emissions from coal combustion, because coal from different geographical regions typically has distinctive Hg isotopic signatures (Sun et al., 2014), and there is a small and predictable isotopic fractionation between feed coal and bulk flue gas emissions (Sun et al., 2013).Sun et al. (2014) proposed a double Rayleigh isotope fractionation model to predict speciated coal Hg isotope emissions.Based on their model, δ 202 Hg can shift by −0.5‰ for emitted PBM relative to the feed coal.The most fractionated δ 202 Hg of Indian coal reported so far is -2.86‰ (Sun et al., 2014).This will generate PBM with δ 202 Hg of -3.36‰ which within analytical uncertainty, is consistent with the measured number of the most fractionated PBM sample from the industrial site (Figure 3).D 199 Hg of Indian coal shows a large range from + 0.28‰ to -0.15‰ (Sun et al., 2014) with most of the samples concentrating around 0. However, none of the Hg species in the stack emission produce MIF.Hence, GEM, GOM and PBM from coal combustion can retain a similar MIF signature as that of feed coal.D 199 Hg of PBM collected from the industrial sites in this study overlapped the range expected for Indian coal with several samples showing up to -0.31‰ MIF.Post emission in cloud photoreduction would cause a positive shift in the observed D 199 Hg.Therefore, the -0.15‰ shift of the few PBM samples from the feed coal isotope values cannot be explained by post emission reactions in the atmosphere.We speculate that the sampled PBM have two sources, Indian coal and a second source which has more negative D 199 Hg.The second source could be either Australian Coal or background GEM adhering to PM 10 , or combination of both.As we do not have any information on the Hg isotope ratios of Australian coal, we cannot predict a mixing model for PBM isotopes from the two different feed coals.However previous studies have reported negative D 199 Hg in GEM, up to -0.4‰ (Rolison et al., 2013).Assuming a simple binary mixing model, 60% of the most fractionated GEM (D 199 Hg = -0.4‰)adhering to PM 10 mixed with 40% of PBM emitted by the most fractionated Indian coal (D 199 Hg = -0.15‰)can produce PBM D 199 Hg of -0.3‰.In absence of exact feed coal data and isotopic composition of background GEM, we interpret that the overall observed PBM isotopic composition in the industrial site samples is broadly consistent with coal combustion emission models proposed by Sun et al. (2014).

Traffic junction
The Hg content in gasoline is much lower (Conaway et al., 2005;Won et al., 2007) compared to coal (Yudovich and Ketris, 2005).Studies show that both in idling and driving modes, the automobile exhaust gas mainly contains GEM with no detectable levels of PBM or GOM (Won et al., 2007).As road transport is considered the dominant source of PM 10 (Senaratne et al., 2005), we envisage the high concentrations of PBM in the traffic junction samples are due to availability of PM that forms the substrate for GEM + GOM to adhere.The waste incineration site is within 5 km radius of the traffic junction and there are numerous small and medium scale industries within 10 km radius.Hence the traffic junction PBM source is likely mixed between traffic emission, coal combustion, waste incineration and re-emission of previously deposited road dust.Elementa: Science of the Anthropocene • 4: 000098 • doi: 10.12952/journal.elementa.000098 The PBM isotope composition of traffic junction samples shows a wide range and cannot be attributed to one source.Hg only moderately correlates with As (0.55) (Table S4), indicating coal combustion to be at least one of the sources.However, as Hg does not correlate with any of the other trace metals measured in this study, the sources remain inconclusive.δ 202 Hg has a ∼3‰ range and D 199 Hg varies from + 0.33 to -0.30‰.The only published isotope study on PBM reported similar δ 202 Hg ratios from -1.61‰ to -0.12‰, however, the MIF was strongly positive with D 199 Hg ranging from + 0.36‰ to + 1.27‰ (Rolison et al., 2013).Rolison et al. explained the observed MDF by coal combustion supported by air mass back trajectory analysis and the positive MIF by in-aerosol photoreduction.PM 10 can be composed of non-hygroscopic material like dust, fly ash, carbon and hygroscopic sulphate, nitrate and sea salt (ten Brink et al., 1997).In the monsoon season, the Southwest Monsoon winds originating in the Bay of Bengal blow over the city.Hence, the presence of hygroscopic components in the PM 10 combined with a high relative humidity can trigger aqueous photo reduction reactions (Bergquist and Blum, 2007) in minute scale within the aerosol leaving the aerosols enriched in odd MIF.In addition, the PBM in the traffic junction is envisaged to have travelled a longer distance with a longer atmospheric residence time as compared to the PBM collected in the industrial and waste burning sites.Therefore, in situ atmospheric redox reactions are more likey to occur in PBM samples from the traffic junction site.We therefore consider the large spread in MIF in our data caused by a combination of retention of original source signature and in aerosol photo reduction.

Seasonal variation
Statistical tests were performed in order to understand whether the winter and monsoon isotope ratios (δ 202 Hg and D 199 Hg) differ significantly at the industrial site and traffic junction.As there are too few data points for the waste incineration site for both seasons, the tests could not be performed for those samples.The nonparametric Mann-Whitney-Wilcoxon test was first performed to check whether there is any seasonal variation of δ 202 Hg and D 199 Hg in the industrial site and traffic junction.This test gave statistically significant evidence (p-value = 0.04, at 0.05 significant level) only for the D 199 Hg in the traffic junction.To further investigate whether the difference in the winter and monsoon D 199 Hg in the traffic junction is real, their descriptive statistics were analysed (Table 1).We note that the mean values are -0.06‰ in winter versus 0.1‰ in monsoon.Since the skewness of D 199 Hg of the traffic junction for both the seasons was low (winter data = 0.09 and monsoon data =0.03), it is assumed that the distributions are reasonably close to normal, thus allowing the two sample t-Test to be conducted.The results of the t-Test (t = -2.28,df = 21.1, p-value = 0.03) lead to a conclusion that mean values of the winter and monsoon data are significantly different at the 0.05 significance level.The boxplots of the winter and monsoon data (Figure 2) also illustrate the median D 199 Hg of the monsoon season to be higher than the winter.On the basis of the above discussion, it is concluded that the mean as well as the median of D 199 Hg is higher in monsoon vis-à-vis winter in the traffic junction.
The average humidity during the monsoon season is high, increasing the scope of in aerosol photoreduction in the hydroscopic PM 10 particles.This can leave the PBM enriched in the odd isotopes (Gratz et al., 2010).We also see a moderate correlation between humidity and D 199 Hg (R 2 = 0.55) in the traffic junction site for monsoon season strengthening our hypothesis.Residence time of PBM in the atmosphere also possibly plays a significant role in post emission atmospheric transformations.Higher values of D 199 Hg were not seen in the industrial and waste burning site during the monsoon season as they were collected near the point source.Hence, the residence time of PBM in the atmosphere was significantly shorter than that in the traffic junction.

Conclusion
We have reported for the first time the Hg isotopic composition of PBM in PM 10 from near point sources of emission; a traffic junction, a waste burning site and an industrial site in and around heavily polluted Kolkata.All samples displayed negative MDF, while the MIF varied between -0.31‰ to + 0.33‰.Within the same city, the industrial, waste incineration and urban traffic site revealed different PM 10 Hg isotope signatures.The results demonstrated that the PBM isotopic composition in the industrial site overall fits the model predicting coal combustion emission (Sun et al., 2014).Though we do not know the Hg isotopic composition of bulk municipal waste, we assume it is similar to that of Hg ore and liquid Hg with practically zero MIF.The PBM emitted by open burning also showed very little MIF.The traffic junction PBM showed a larger variation within one season and also across seasons.Though vehicular emission is the single largest source of PM in urban air, it is not a major source of PBM.Hence the high PBM measured in the traffic junction is possibly due to scavenging of background GOM and GEM by the plentiful air particulates.The back ground GOM and GEM in the city air come from numerous industries around the city and waste burning.The residence time and distance travelled is higher than the PBM at the other two sampled sites.Hence the original isotopic signature of the source can be modified by atmospheric processes which are the likely cause for the larger spread in isotope ratios.Moreover, PM 10 composition is different in two seasons.While the winter PM 10 composition is dominated by dust blowing from the north, the monsoon PM 10 can be dominated by hydroscopic particles such as sea salt when the air mass blows from over the Bay of Bengal.Elementa: Science of the Anthropocene • 4: 000098 • doi: 10.12952/journal.elementa.000098 Hence in aerosol, aqueous photoreduction might be more dominant during the monsoon season resulting in statistically slightly higher mean positive MIF as compared to winter data.In summary, this study shows that isotopic composition of PBM can be a powerful tool to determine point sources.However, atmospheric reactions can modify the source signature if the PBM has a considerable long residence time in the atmosphere and/or it has travelled long distances prior to deposition.