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Environ Eng Res > Volume 24(1); 2019 > Article
Lee, Yang, Kim, and Han: Effects of organic carbon and UV wavelength on the formation of dissolved gaseous mercury in water under a controlled environment


The effects of UV wavelength and dissolved organic carbon (DOC) on the formation of dissolved gaseous mercury (DGM) were investigated in a controlled environment. To remove any other influences than UV wavelength and DOC, purified water was used as the working solution. DGM was instantly produced with irradiation of all UV lights even without DOC; whereas, there was no noticeable increase of DGM during irradiation of visible light. The amount of formed DGM increased as the DOC concentration increased even in dark conditions; however, UV-B irradiation significantly promoted DGM production with DOC present. The rate constants of reduction ranged from 1.4 × 10−6 s−1 to 3.5 × 10−5 s−1, with the lower values occurring under the dark condition without DOC and the higher values resulting under UV-B irradiation and high DOC concentration. However, DGM production was not linearly correlated with the DOC concentration at higher range of DOC in this study. Future studies should investigate the effects of DOC concentration on mercury (Hg) reduction over the broad range of DOC concentrations with different DOC structures and with other influencing parameters.

1. Introduction

Mercury (Hg) differs from other heavy metals because it can exist as gas and consequently can cycle between various environmental media. Atmospheric Hg mostly exists as inorganic forms; however, once it is deposited into water and soil surfaces, it can be converted to methyl Hg, which is the most toxic form, mainly by anaerobic bacteria in aquatic and/or terrestrial ecosystems [14]. Methyl Hg is then bio-magnified through the food chain and hence effectively accumulating in carnivorous fish and humans. Atmospheric Hg sources are typically classified as anthropogenic sources, natural sources, or re-emissions of Hg which was previously deposited on surfaces. According to the United Nations Environment Programme [5], two-thirds of the total global Hg emissions is produced from natural surfaces including aquatic and soil surfaces. In an aquatic system, Hg mainly exists as divalent forms and either in dissolved or particulate forms as inorganic and organic complexes [68]. Divalent Hg can be reduced through biotic and abiotic processes to elemental Hg (Hg0), the dominant form of dissolved gaseous mercury (DGM). Since Hg0 has a high vapor pressure and low Henry’s Law constant [9], DGM is assumed to be readily volatilized to the atmosphere once it is formed on a water surface. Therefore, the reduction process is highly important for the removal pathway of Hg pools in an aquatic ecosystem while it is connected to the significant input to the atmospheric Hg pool.
Divalent Hg can be reduced either via biotic processes by small-size phytoplankton or bacteria and via abiotic processes [1017]. Abiotic reduction is regarded to be more important than biotic processes especially in surface water. Many previous studies have suggested that solar radiation was the most important factor for abiotic reduction mechanisms; therefore, DGM formation typically follows a same diel pattern of solar radiation, which results in a high formation rate at midday and low formation rate at night [1821]. UV lights are considered more effective on DGM formation than visible light [22]. However, other studies observed irregular diel fluctuations of DGM concentration [10, 23], which indicates that other factors in addition to solar radiation must be influencing the oxidation-reduction of Hg. Dissolved organic carbon (DOC) concentrations are also acknowledged to be an important factor for Hg reduction. Most studies found that DGM concentrations clearly increased with the presence of DOC [14, 2022, 2425]. At the same time, other studies have demonstrated that an increasing DOC concentration caused a decrease in the ratio of DGM to total mercury [26], possibly because high DOC concentrations result in the enhanced stability of Hg(II) complexes with DOC [27] or DOC caused attenuation of solar radiation [2830]. On the other hand, some studies showed the interacting effects of DOC and solar radiation. Allard and Arsenie [31] suggested that Hg(II) must be complexed with DOC for photoreduction to occur.
Most previous studies tracked the relationship between DGM concentration and various environmental parameters in the natural environment to identify the influencing factors on Hg reduction. However, reduction and oxidation always occurs concurrently in natural environments, making it difficult to identify the sole effect of the parameters on Hg reduction or Hg oxidation. In addition, it is difficult to interpret the DGM formation that results from a single parameter because parameters unpredictably interact with each other in the natural environment.
In this study, DGM production was continuously tracked in a controlled environment to identify the individual and combined effects of the two most important parameters influencing DGM formation: the wavelength of light and DOC concentration. Purified water was used in this study because multitudinous parameters that are not identified or considered in experiments can unpredictably interact with each other in lake or ocean sample.

2. Methods

2.1. Experimental Design

2.1.1. Working solutions

Since the total Hg concentrations are typically found in the range of 0.5 to 10 ng L−1 in most of lakes [14, 23, 32], the working solutions containing 1 ng L−1 and 10 ng L−1 of Hg were prepared from a 100 ppm stock Hg(NO3)2 (SPEX CertiPrep, preserved with 5% HNO3) in this study. A 0.5 mL of 100 ppm standard solution was added to a 50 mL glass tube filled with 10 mL of ultra-purified water. Purified water was added up to the total volume of 50 mL in order to make 1 ppm solution. A 0.5 mL of 1 ppm solution was then diluted with 49.5 mL of purified water to make 0.01 ppm. 1 mL and 0.1 mL of 0.01 ppm solution were diluted with ultra-purified water for a total volume of 1 L to obtain final concentrations of 10 ng L−1 and the 1 ng L−1, respectively. The solutions were placed in a 1 L glass bottle capped with a glass stopper and equilibrated for a minimum of 24 h before the experiment. This working solution was used to identify the effects of light wavelength and DOC concentration on DGM formation, which is explained in detail below.

2.1.2. Wavelength experiment

A glass bottle filled with 1 L of working solution (Hg concentration = 10 ng L−1) was placed in a water bath (JSWV-06T) to maintain a constant temperature of 24°C inside of the chamber, which was made of a black acrylic panel in order to prevent the light from entering. Inside the chamber, UV-A (320–380 nm), UV-B (280–320 nm), and UV-C (200–280 nm) lamps were fixed on the wall and electric lines were connected to the on/off switches outside of the chamber through the hole (Fig. 1). The intensities of UV-A, UV-B, and UV-C were 0.148 mW cm−2, 0.136 mW cm−2, and 0.054 mW cm−2, respectively. Before starting the irradiation, the working solution was purged with zero-Hg air in the dark until the Hg concentration became close to or less than the background concentration (1–1.5 pg L−1). Once Hg readings under dark conditions dropped to less than the background concentration, the lamps were turned on. Each lamp was on for 2 h, off for 1 hour, and on again for 2 h, which was maintained to be consistent for all experiments. Two hours of irradiation and one hour of darkness were chosen as independent variables in our experimental setup because the irradiation time was not a controlling factor to be tested in this study. Since large variations in DGM concentrations can occur over short timeframes, DGM concentrations were continuously measured every 5 min using a Tekran 2537B throughout the experiments.

2.1.3. DOC experiment

In order to identify the effect of DOC concentration on DGM formation, different amounts of humic acid sodium salt (Aldrich Cas-No.: 68131-04-4) were dissolved in the purified water to obtain four different DOC concentrations ranging from 0 to 4 mg L−1. DOC concentrations in the working solutions were quantified using a TOC analyzer (Sievers 5310 C, GE, USA). Each sample was analyzed three or four times and the average DOC concentrations were 0, 1, 2.38, and 3.92 mg L−1. Relative standard deviations (RSD) were 1.0, 3.8, and 0.5% for DOC concentrations of 1, 2.38, and 3.92 mg L−1, respectively. Hg concentration in the working solution was set to be 1 ng L−1 for this experiment.
DGM concentrations in the working solutions with different DOC concentrations were continuously measured under both dark conditions and UV-B irradiation. Samples were purged by ultra-high-purity air under the dark condition until DGM concentration became less than the background concentration, at which time the UV-B lamp was turned on again for 90 min.

2.2. DGM Analysis

To measure DGM, 1 L of working solution was placed into a 1 L glass bottle capped with a glass stopper with inlet and outlet tubes. A zero-air tank was connected to the glass inlet tube with a Teflon stopcock to purge the solutions at a flow rate of 1.5 L min−1. Stripped DGM was withdrawn into the outlet tube connected to a Tekran 2537B to continuously measure DGM concentration; values were logged every five minutes (Fig. 1). A soda-lime trap was placed between the glass bottle and Tekran 2537B to remove water vapor and possible impurities that could possibly inhibit the detection of the Tekran instrument. A glass bottle with working solution was placed in a thermostatic water bath (JSWB-06T) to maintain a constant temperature of 24°C inside a black acrylic chamber throughout the experiment.
Tekran 2537B is a cold vapor atomic fluorescence spectrometry (CVAFS). Inside a Tekran 2537B, there are two gold cartridges where Hg vapor is collected. The gathered Hg was thermally desorbed at 525°C and carried by an ultra-high-purity argon stream into a detector and excited by light at a wavelength of 253.7 nm. The excited atoms fluoresce at the same wavelength which was detected by a photomultiplier tube. The signal was converted to a voltage which was relayed to a computer.
In order to check whether there was any leakage in the sampling line, a stopcock was situated as the dotted line in Fig. 1 so that ultra-high-purity air was introduced into the Tekran 2537B (Fig. 1). It was determined that there was no leakage if the flow rate shown in Tekran 2537B was less than 0.05 L min−1 when a ultra-high-purity air regulator was closed off.

2.3. QA/QC

The Tekran 2537B was calibrated using an internal permeation source before each experiment. Manual injections were also used to evaluate the automated calibration using a saturated mercury vapor standard. A certain volume of Hg saturated air (0, 10, 20, 30, and 50 μL) was withdrawn by a gas tight syringe (Hamilton) from a closed flask containing about 2–3 mL of metallic mercury and injected into the manual injection port of the Tekran 2537B. The flask was maintained at 16.6°C by being immersed in a temperature-regulated water bath. Injected mercury mass was calculated from the temperature dependent density and the volume of Hg-saturated air withdrawn, and a calibration curve was obtained for both cartridges (R2 > 0.9995). The relative percent difference between the manual injection and automated calibration was less than 2%. A recovery rate (94 ± 3%) was obtained by directly injecting Hg vapor into the Teflon tubing line between the ultra-high-purity air cylinder and the Tekran 2537B.
Cleaning procedures were in alignment with the United States Environment Protection Agency’s method 1631E [33]. All Teflon and glass parts were first heated in 4 M HCl at 65–75°C for at least 48 h and then filled with 1% HCl solution at 60–70°C in an oven overnight.

3. Results and Discussion

3.1. Effect of UV Wavelength on DGM Formation

To identify the effect of UV wavelength, a working solution of 10 ng-Hg L−1 was used. The working solution was purged with ultra-high-purity air in the dark until the DGM concentration became less than 1.5 pg L−1 before starting the irradiation. As soon as the UV lights were applied, DGM concentrations abruptly increased for all 3 conditions (i.e., UV-A, UV-B, and UV-C), but the increments were different (Fig. 2). In the experiment with UV-A, DGM concentrations rapidly increased, reached a plateau at approximately 5.6 pg L−1 within 20 min, and then maintained for 2 h until the termination of UV-A irradiation. When the UV-A lamp was off, DGM concentrations immediately dropped to 1 pg L−1 within 15 min, and as soon as UV-A lamp was turned on again, it increased instantaneously. As soon as UV-B irradiated, DGM concentration also immediately increased to around 30 pg L−1, which is approximately 5 times higher than the increment with UV-A irradiation, and started exponentially decreasing to 12 ng L−1 (Fig. 2). This occurrence was likely due to the decreasing amount of reducible Hg.
When the UV-C lamp was switched to on, DGM concentrations also reached a peak of around 5 pg L−1 within 10 min and then gradually decreased during the 1st 2-h irradiation; however, during the second 2-h irradiation experiment, DGM slowly increased, which was not observed in the experiments with UV-A and UV-B (Fig. 2). In addition, under the dark condition in between two UV-C irradiation sessions, DGM did not drop as much as it did in the UV-A and UV-B experiments. The somewhat different results from UV-C irradiation may indicate that UV-C promotes the production of reducible Hg as well as Hg reduction. Not all the divalent Hg is in a reducible form, and the size of the reducible fraction is dependent on the incident wavelengths [34]. Previous research suggested that more reducible Hg was observed under radiation of shorter wavelengths of UV (UV-B rather than UV-A) [9]; however, there are not, as yet, any studies that have investigated the effect of UV-C on a fraction of reducible Hg in water. There are a few studies investigating the effect of wavelength of light on Hg emissions from soil surface. Park et al. [35] found that Hg emission from soil surface increased under UV-A and UV-B radiation because UV radiation wavelengths directly reduced Hg2+ to Hg0 in the soil surface. However, they also found that Hg was rather deposited onto the soil surface with UV-C exposure, indicating that atmospheric Hg0 was oxidized to Hg2+ in the air, followed by being deposited to the soil. Choi and Holsen [36] also observed that atmospheric Hg was oxidized with UV-C exposure. Although these previous results cannot be directly compared with our experiments aimed at Hg reduction in water, UV-C seems to have oxidative capacity, which can possibly generate the reducible Hg(II) in water. In this experiment using a three-wave lamp (visible light), DGM formation was not observed, which indicates that only UV is involved in Hg reduction mechanisms (Fig. S1).
In this experiment, DGM formed in the sample was continuously removed by purging with ultra-high-purity air to prevent the back-reduction; therefore, it followed the kinetics of gross reduction, that is, the reaction
where Hgr(II) indicates the reducible Hg in the sample. Assuming pseudo-first order kinetics, the following equations apply:
DGM formation rates (d[DGM]/dt) were compared for different wavelength lamps. The DGM formation rate was the highest for UV-B, followed by UV-A and UV-C (Table 1). Since the light intensity was different for the UV-A, UV-B, and UV-C lamps used in this study (0.147 mW cm−2, 0.136 mW cm−2, and 0.054 mW cm−2 for UV-A, UV-B, and UV-C, respectively), the DGM formation rates considering the light intensity (pg-cm2 L−1-J−1) were also compared. The results indicated that the highest DGM formation rate was for UV-B, followed by UV-C and UV-A (Fig. 3). During the first 2-h and the second 2-h irradiations, the total DGM production amounts were 201.2, 840.5, and 161.9 pg for UV-A, for UV-B, and UV-C, respectively (Table 1). Because the irradiation time was limited to 4 h for each UV light, the total possible production amount of DGM via a photo-reduction mechanism was not identified in this study. It will be worthwhile to conduct a similar experiment in the future until no further Hgr(II) is available for reduction (which means no further DGM is produced) with a lower Hg(II) injection amount and longer irradiation time.
Because Hgr(II) can better absorb UV-B light rather than UV-A and UV-C lights, DGM formation was the highest with UV-B radiation. According to Nriagu [37], Hg compounds combined with ions and organocomplex can absorb the light of 270–400 nm wavelengths which corresponds to UV-A and UV-B. Other studies also suggested that DGM formation under UV-B light was the highest when compared with those for UV-A [3839]. According to Garcia et al. [22], about 61–73% of total photo-induced DGM was reduced by UV radiation and only approximately 27% was produced by visible light. Amyot et al. [40] also found that maximum DGM levels produced under visible and UV radiation (UV-A + UV-B) were twice the amount of formed DGM by visible light alone in a controlled laboratory experiment. Increased DGM formation under all UV radiation was clearly observed in our study; however, DGM did not show an identifiable increment under visible light.

3.2. Effect of DOC Concentration on DGM Formation

3.2.1. DGM formations under dark condition

Hg reduction was studied under various DOC concentrations including 0.0, 1.0, 2.4, and 3.9 mg L−1. DGM concentrations were continuously measured in the dark condition during the 90 min prior to UV-B irradiation. DGM concentration decreased and reached a plateau within 40 min for 0.0, 1.0, 2.4, and 3.9 mg L−1 of DOC concentration. After DGM reached a plateau, average DGM formation rates were calculated, and they were 0.12 ± 0.02, 0.22 ± 0.05, 0.40 ± 0.10, and 0.53 ± 0.03 pg L−1 min−1 for 0.0, 1.0, 2.4, and 3.9 mg L−1 of DOC concentrations in the working solution, respectively (Table 2). Increasing DGM formation rates with increasing DOC concentration suggests that DOC facilitates Hg reduction even without light and without microbial activity. Previous researches proposed that Hg2+ could be directly reduced by humic substances via ligand metal charge transfer [31, 35, 41]. Alberts et al. [42] also reported that Hg2+ could be directly reduced by humic substances under the assumption that quinone or semiquinone moieties in organic matter were involved in the transfer of electrons that led to Hg reduction.

3.2.2. DGM formations under UV-B radiation

DOC is often acknowledged to be important in the photo-reduction of Hg [14, 25, 4344]. In order to identify the effect of DOC concentrations on DGM photo-production, UV-B was irradiated on the samples with various DOC concentrations (0.0, 1.0, 2.4, and, 3.9 mg L−1) and DGM concentrations were continuously tracked. The initial Hg(II) concentration was 1 ng L−1. All samples were purged with ultra-high-purity air for 90 min under the dark condition before UV-B irradiation. UV-B was selected instead of UV-A or UV-C since it exhibited the highest DGM production among three different wavelengths of UV (Fig. 2). As soon as the UV-B lamp was on, DGM concentrations instantly increased for all samples; although, the increments were different. DGM formation rates clearly increased as DOC concentrations increased from 0 to 3.9 mg L−1 (Table 2), which suggested a positive effect of DOC concentrations on DGM formation with UV-B irradiation. According to previous studies [14, 4546], DOC absorbed solar radiation and emitted electrons which reduced Hg, as in Eq. (4) and (5). In addition, photolysis of DOC can form reactive reductants, such as HO2, that reduces Hg(II) [4748].
If all DOC in the sample was photolyzed, the production of electron and DGM would increase logarithmically as DOC concentration increased. The relationship between DGM formation rate and DOC concentration was found to be more likely to follow the logarithmic equation than the linear equation, as shown in Table 2; however, it is not conclusive due to the insufficient sample number and future work is worthwhile to be conducted with a wide range of DOC concentration.
Many previous studies [24, 4950] found a similar result that DGM formation by lights increased in the presence of fulvic and humic acid. However, there are also several other studies demonstrating a negative effect of DOC on Hg reduction. Amyot et al. [29] observed lower DGM production in high DOC lakes and Watras et al. [26] found that an increasing DOC concentration was related to an exponential decrease in the DGM/TM ratio. In the laboratory work by Garcia et al. [22], there was a strong positive correlation between DGM production and DOC concentration under UV-A radiation whereas DGM production was negatively correlated with UV-B radiation. The contradictory results were likely caused by differing conditions. In this study, DGM production was traced under the gross reduction condition that was maintained by continuously stripping formed DGM from the samples. However, Hg reduction and oxidation concurrently occurred in the most reference studies [22, 26, 29, 49], which suggests that DOC and UV-B might affect oxidation as well as reduction mechanisms.

3.3. Rate Constants for Hg Reduction

Using Eq. (6) and (7), the rate constant for gross reduction, kr could be calculated from the experimental data. It was assumed that the initial concentration of Hgr(II) was equal to the total injected Hg in the working solutions. Differential equations were solved numerically, as follows.
When UV light was on, the DGM amount produced during unit time (d[DGM]/dt) started to increase, reached a plateau within 25 min, and then maintained relatively consistent production during the first irradiation period (Fig. 2). In this study, kr was averaged based on the DGM production rate shown during the plateau section. The reduction constants, kr were 1.9 × 10−6 s−1, 8.6 × 10−6 s−1, and 1.4 × 10−6 s−1 for UV-A, UV-B, and UV-C, respectively (Fig. 4).
The reduction constants were also identified under various DOC concentrations. Without UV radiation, kr ranged from 2.2 × 10−6 s−1 to 9.7 × 10−6 s−1 (upper panel of Fig. 4), showing that kr increased as DOC increased even under the dark condition. Please note that the total Hg injected in the working solutions was 10 ng L−1 in the experiments with UV wavelengths (lower panel of Fig. 4); whereas, it was 1 ng L−1 in the experiment with DOC (upper panel of Fig. 4). Under the irradiation of UV-B, kr also noticeably increased as DOC increased. The reduction constants were 1.0 × 10−5 s−1, 2.4 × 10−5 s−1, 2.7 × 10−5 s−1, and 3.5 × 10−5 s−1 for 0.0, 1.0, 2.4, and 3.9 mg L−1 of DOC concentrations, respectively. The rate of increase on kr was the most evident when DOC increased from 0 to 1 mg L−1, and then subsided afterwards, although kr continued to increase. The highest DOC concentration was set to 3.9 mg L−1 in this study because DOC typically ranges from 1 to 4 mg L−1 in most of the reservoirs in Korea [5154]. A slowdown in the rate of increase in kr indicates that there may be a different relationship between DGM production and DOC concentration at higher ranges of DOC concentration. In fact, a good number of studies [22, 26, 29] that utilized DOC concentrations that were in a much higher range than in this study, demonstrated a negative relationship between DGM concentration (or production) and DOC concentration.
The reduction rate constant reported by other studies varied from 1.7 × 10−6 s−1 [55] to 1.2 × 10−3 s−1 [56] in seawater and from 7.76 × 10−5 [39] to 2.9 × 10−4 s−1 [56] in freshwater. These values were obtained from seawater or freshwater in which microorganisms were present; whereas, ultra-purified water was used in this study. Therefore, the somewhat lower kr obtained in this study was anticipated because microbial reduction did not occur. In addition, kr is dependent on the UV light intensity [39, 57], so it cannot be simply compared without the consideration of light intensity. In the studies conducted by Qureshi et al. [58] and Soerensen et al. [59], kr was expressed as αI, where α is a constant (m2 s−1 W−1) and I is the UV light intensity (W m−2). In this study, the slopes, α were calculated to be 1.3 × 10−6, 6.3 × 10−6, and 2.5 × 10−6 m2 s−1 W−1 for UV-A, UV-B, and UV-C without DOC, respectively, which were similar to the value (1.7 × 10−6 m2 s−1 W−1) proposed by Soerensen et al. [59]. With the existence of DOC, α ranged from 7.4 × 10−6 to 3.5 × 10−5 m2 s−1 W−1 under UV-B radiation, which was a slightly higher range than the values reported by Soerensen et al. [59]. It should be noted that the work by Soerensen et al. [59] used seawater and that the Hg photoreduction tends to be inhibited by the presence of chlorides, which may compete with organic matter for binding with Hg [31, 58].

4. Conclusions

Many previous studies have investigated the influencing factors on Hg reduction mechanisms in aquatic environments; however, most studies were conducted in natural environments such as lakes and oceans where reduction and oxidation simultaneously occur. In this study, DGM formation was studied under different UV wavelengths and DOC concentrations in a controlled environment. DGM formation significantly increased with irradiation of all UV lights even without DOC; whereas, there was no noticeable increase of DGM production with visible light. The DGM formation rate was the highest for UV-B, which indicated that Hg can better absorb UV-B light rather than UV-A and UV-C lights. With DOC concentrations of 0.0, 1.0, 2.4 and 3.9 mg L−1, DGM formation increased as DOC concentration increased even under the dark condition, which demonstrated that divalent Hg can be directly reduced by DOC without light. When the UV-B irradiation started, DGM production was instantly enhanced and it increased as DOC concentration increased. The increment of DGM production was the highest when DOC increased from 0 to 1 mg L−1 and slowed down afterwards, which suggests that DGM production may not be linearly correlated with DOC concentration at higher ranges of DOC. This possibility could be a reason why many previous studies found conflicting results for the relationship between DGM and DOC concentrations. In addition, the DOC structure and composition can also affect the DGM production rate [12, 21]. DGM production should be tracked over a broad range of DOC concentrations with different DOC structures in future studies to identify the effect of DOC.
The calculated rate constants for reduction (kr) in this study ranged from 1.4 × 10−6 s−1 to 3.5 × 10−5 s−1 with the lower values occurring under the dark condition without DOC and the higher values resulting under the UV-B radiation with high DOC concentration condition. Even without DOC present, DGM was undoubtedly produced under UV radiation, which is contradictory to the findings by Allard and Arsenie [27] that Hg must be complexed with DOC for photoreduction to occur. The kr calculated in this study was placed in a somewhat lower range than those obtained from seawater and freshwater in previous studies because microbial reduction did not occur.

Supplementary Materials


This work was funded by a National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIP) (Grant No. 2015R1A2A203008301) and by the Korea Ministry of Environment (MOE) as part of the “Environmental Health Action Program” (2015001370001).


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Fig. 1
Schematic design of the experimental setup for identifying the effects of light wavelength and dissolve organic carbon (DOC) concentration on dissolved gaseous mercury (DGM) production.
Fig. 2
Changes in dissolved gaseous mercury (DGM) concentrations every 5 min during irradiation of different wavelengths of UV light.
Fig. 3
Formation rate of dissolved gaseous mercury (DGM) normalized by light intensity during the first and second irradiation of UV-A, UV-B, and UV-C.
Fig. 4
Rate constants for Hg reduction with four different concentrations of dissolved organic carbon (DOC) under the dark condition and UV-B irradiation (upper panel) and with irradiation of UV-A, UV-B, and UV-C without DOC (lower panel).
Table 1
DGM Formation Rate and Cumulative Amounts of DGM Produced during Irradiation with UV-A, UV-B, and UV-C Lamps. Note That the Initial Hg(II) Concentration Was 10 ng L−1 in a Working Solution
Radiation intensity (mW cm−2) DGM formation rate (pg L−1 min−1) Cumulative DGM production (pg)

Irradiation-1st Irradiation-2nd Irradiation-1st Irradiation-2nd
UV-A 0.148 0.99 ± 0.20 0.69 ± 0.18 118.5 82.7
UV-B 0.136 4.54 ± 1.13 2.52 ± 0.32 551.0 289.5
UV-C 0.054 0.75 ± 0.16 0.60 ± 0.13 91.9 70.0
Table 2
Different DGM Concentrations and Formation Rates under Various DOC Concentrations in a Working Solution. Note That the Initial Hg(II) Concentration Was 1 ng L−1 in a Working Solution
Condition DOC concentrations (mg L−1)

0.0 1.0 2.4 3.9
DGM concentration within first 10 min (pg L−1) Dark 82.70 41.22 32.41 38.70
DGM formation rate (pg L−1 min−1) Dark 0.12 ± 0.02 0.22 ± 0.05 0.40 ± 0.10 0.54 ± 0.03
UV-B irradiation 0.51 ± 0.10 1.16 ± 0.18 1.37 ± 0.46 1.58 ± 0.29
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