# Characteristics of Atmospheric Metalliferous Particles during Large-Scale Fireworks in Korea

Authors: Zang-Ho Shon; Ju-Hee Jeong; Yoo-Keun Kim
Journal: Advances in Meteorology
 (2015)

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## Abstract

The effect of large-scale firework events on urban background trace metal concentrations was investigated using 24 hr data collected over 3 days at three sites in Busan Metropolitan City, Republic of Korea, during the falls (Oct.) of 2011–2013. The firework events increased local background concentrations of trace metals as follows: K (1.72 times), Sr (2.64 times), As (2.86 times), Pb (2.91 times), and Al (5.44 times). The levels of some metals did not always drop to background level one day after the firework event. The contribution of fireworks to trace metal concentration levels (and emissions) for 2011 event was negligible compared to 2012 and 2013 events due to different meteorological conditions (precipitation). In addition, the impact of firework events on the ambient concentration levels of trace metals was likely to be different depending on their chemical speciation. The impact of firework events in Busan on urban air quality (trace metal) was less intense compared to other similar festivals worldwide. The largest emission of trace metals and elements from firework burning was represented by K (128–164 kg), followed by Pb, Cd, Cu, Mg, Ba, As, Al, Ga, Co, and Na.


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## Body

## 1. Introduction

Enhancement of trace metal loading in the air is of great concern to air quality, as it adversely affects human health. Exposure to elevated concentrations of metals such as As, Cd, Co, Cr, Ni, Pb, and Se can cause cancer through inhalation of fine particles, although they constitute only a small fraction of the total particulate matter (PM) by mass [1, 2]. Unlike continuous traffic emission, sporadic firework (crackers and sparkles) burning is one of the unique sources of airborne particles that include massive amounts of trace metals such as Zn, Ba, Pb, K, and Sr during a short period of time [3]. Fireworks also generate gaseous air pollutants such as SO2, NOx (NO + NO2), octachlorinated dioxins, furans, and hexachlorobenzene, including the primary emission of O3 without NOx participation [3–6]. Fireworks events have been concentrated within special periods during specific times of year, such as New Year’s Eve (worldwide), the Diwali festival (November, India), Las Fallas (March, Spain), and Lantern Festival (February, China).The predominance of metal species in airborne particles during the burning of fireworks depends on their chemical fractions. In other words, fireworks contain various chemicals, such as potassium nitrate, potassium chlorate, potassium perchlorate, charcoal, sulfur, manganese, sodium oxalate, aluminum and iron dust powder, strontium nitrate, and barium nitrate, for their own purposes [7]. Potassium salts such as nitrate, chlorate, and perchlorate are widely used as oxidizers in fireworks. Al and Mg are widely used as metallic fuels in pyrotechnics, and Al is also used to give silvery or “flitter” type effects. For coloring effects, Sr, Na, Cu, Ba, and Ca are used to exhibit red, yellow, blue, green, and orange, respectively [8]. Pb can be used for achieving a steady and reproducible burning rate [9]. Despite their toxicity, a limited number of studies on metal emissions from fireworks have been reported in the literature [10, 11]. The annual emissions of Al, Mg, Na, Ba, Sr, Ti, and Cu released from fireworks and other explosives in the UK during 2002 were estimated to be 86, 73 (7.6% of total UK emissions), 5.5 (0.5%), 65, 10, 5, and 3 (6%) tons, respectively [10]. In Passant [10], the contribution of metal emissions from fireworks and other explosives to their total emissions in the UK was available only for Mg, Na, and Cu.One of the interesting episodic (and periodic) sources of trace metals in the atmosphere of Korea is the “Busan Fireworks Festival (BFF),” which takes place every October. The BFF is one of the most significant fireworks festivals in Asia. During the BFF, tens of thousands of fireworks and state-of-the-art lasers light up the sky in harmony with the theme song of the festival against a backdrop of the sea and a 2-level suspension bridge, Gwangan Bridge, drawing crowds of over 1 million visitors each year. The objective of this study was to investigate the impact of fireworks on the short-term spatiotemporal variation of trace metals in PM during three BFF events. The characteristics of trace metals and elements making up the PM after firework burning were investigated using the atmospheric measurements and a high-resolution meteorological model simulation. This study also provides the first attempt to assess the emission rates of various trace metals from the burning of fireworks.


## 2. Materials and Methods

### 2.1. Site and Measurements

Field measurements at three coastal sites (A1–A3) in Busan, Republic of Korea, were performed during Oct. 2011–2013 to assess the impact of fireworks released from Gwangan Bridge (or Diamond Bridge, DB) on the spatiotemporal distribution of trace metals in PM (total suspended particle, TSP) (Figure1). Sampling site A1, an air quality monitoring site operated by Busan Metropolitan City Institute of Health & Environment (BMCIHE), is located 2.0 km west of the bridge (DB); site A2 is located in a regional office of Busan Environmental Corporation, 1.1 km south of the DB; and site A3 is located at Busan Yachting Center, 0.6 km east of the DB. The fireworks during the BFF events were set off over the bridge and from barges simultaneously, starting exactly at 20:00 LST (local standard time), for one hour.Figure 1
Location map of sampling sites (A1–A3) of trace metals and elements during the firework event days of 2011–2013 and meteorological monitoring sites (M1 and M2). Solid black circles represent environmental monitoring sites, where the concentrations of criteria air pollutants (O3, PM10, NO2, CO, etc.) are routinely measured.PM samples were collected on a Whatman QM-A quartz microfiber filter (8 × 10 inches) using a high volume air sampler (SIBATA HV-1000F, Japan) operating at a flow rate of 1000 L min−1. Twenty-four-hour (11:00 am to 11:00 am) integrated samples were obtained during three consecutive days, Oct. 28–30, 2011, Oct. 27–29, 2012, and Oct. 25–27, 2013, for the three BFF events, respectively. The dates of the firework events during 2011–2013 were Oct. 29, 28, and 26, respectively. One-fourth of each filter was extracted in 30 mL of 1.03 M HNO3 + 2.23 M HCl mixture by keeping it in an ultrasonic bath for 2 hr at 100°C. Metallic compounds and elements in the filtrates were measured by inductively coupled plasma Optical Emission Spectroscopy (Varian ICP-OES 720-ES). Five analytes (Pb, Cd, Cr, Cu, and As) were measured during the 2011 BFF event, and ten analytes (Pb, Cd, Cr, Cu, As, Al, Ca, Na, K, and Sr) were examined during the 2012 and 2013 events.To examine the impact of fireworks on air quality (especially, PM10 (particles with diameter of 10 micrometers or less) concentration) in Busan, distributions of PM10 were investigated during the daytime (07:00–18:00 LST) and nighttime (19:00–06:00 LST) for the 2012 and 2013 BFF events due to wide spatial and temporal coverage of PM10 observations instead of trace metals. These analyses were carried out based on hourly concentrations of PM10 observed at eighteen (for 2012) and nineteen (for 2013) environmental monitoring sites in Busan, operated by the Korean Ministry of Environment (Figure 1). In order to deduce the dispersion of trace metals released from the BFF events, the observations of meteorological variables (e.g., temp., RH, wind speed, wind direction, and rainfall) obtained at two meteorological monitoring sites (M1 and M2) close to the environmental monitoring sites (Figure 1) and numerical simulation of wind fields were used in this study.


### 2.2. Estimation of Trace Metal Emissions in PM

The emissions of trace metals and elements in PM were estimated using their emission factors and the amounts of firework consumed. The data of firework consumption was obtained from the Organizing Committee for Busan Culture and Tourism Festival (http://festival.busan.kr/KOR/index.asp). Detailed information on the fireworks used during the BFF events of 2012-2013 is presented in Supplementary Table 1 in the Supplementary Material available online at http://dx.doi.org/10.1155/2015/423275 and discussed in Section 3.4. The emission factors of trace metals and elements in PM were adopted from the study of Croteau et al. 2010. Croteau et al. 2010 reported the emission factors of trace metals and elements for various types of fireworks, including Dragon Eggs, Ribbon Fuses, Roman Candles, and Fountains (4 types). In this study, the emission factors of aerial shell types of fireworks were set to the average value of the above four types due to lack of data. The emission factor of fountain fireworks was set to the average value of those of four fountain types. The emission factor of cakes was set to the average value of Roman Candles and Dragon Eggs due to the similarity of the fireworks type. The emission factors of other fireworks such as mine, comet, frame, strobe, row, igniter, and delay chain were also set to the average value of the above four types. The emission factors of Co, As, and Cd were adopted from Passant [10].


### 2.3. Meteorological Model Description

In order to analyze the air mass pathway of metal-rich particles after the burning of fireworks during the BFF events, the meteorological model Weather Research and Forecasting (WRF) version 3.6, which includes fully compressible nonhydrostatic equations, was employed [12]. The model domain was divided into five domains using the two-way nesting method (Supplementary Table 2). The finest domain for the Busan region consisted of 42 sigma vertical levels and 121 × 121 grid cells, with a horizontal mesh width of 0.5 km covering about 34.91°–35.42°N and 128.74°–129.45°E. Detailed descriptions of the grid information and physical options used for the simulation are given in Supplementary Table 2. The initial/lateral boundary conditions were generated by interpolating the National Center for Environmental Prediction (NCEP) Final Analysis (FNL) fields and the sea surface temperature (SST) data. Moreover, the Objective Analysis technique (OBSGRID) was used to improve the first-guess gridded analysis through incorporation of high-resolution (in time and space) surface- and upper-level observations. The surface boundary conditions were extracted using the Environmental Geographic Information System (EGIS: a 90 m resolution) land cover and the Shuttle Radar Topography Mission (SRTM: 90 m) topography data sets. To simulate the flow structure and wind fields for the 2012 and 2013 BFF events, the WRF simulations were conducted for a period of 144 hr per event (from 00 UTC on the 24th to 00 UTC on the 30th of October 2012 and from 00 UTC on the 22nd to 00 UTC on the 28th of October 2013, resp.), including a spin-up time. Meanwhile, since the spatial coverage of trace metal observations is restricted to three sites only, PM10 as a proxy for trace metals was used to identify indirectly the air mass pathway in atmospheric dispersion of trace metals after the burning of fireworks, combined with the WRF model results (wind field simulation).


## 2.1. Site and Measurements

Field measurements at three coastal sites (A1–A3) in Busan, Republic of Korea, were performed during Oct. 2011–2013 to assess the impact of fireworks released from Gwangan Bridge (or Diamond Bridge, DB) on the spatiotemporal distribution of trace metals in PM (total suspended particle, TSP) (Figure1). Sampling site A1, an air quality monitoring site operated by Busan Metropolitan City Institute of Health & Environment (BMCIHE), is located 2.0 km west of the bridge (DB); site A2 is located in a regional office of Busan Environmental Corporation, 1.1 km south of the DB; and site A3 is located at Busan Yachting Center, 0.6 km east of the DB. The fireworks during the BFF events were set off over the bridge and from barges simultaneously, starting exactly at 20:00 LST (local standard time), for one hour.Figure 1
Location map of sampling sites (A1–A3) of trace metals and elements during the firework event days of 2011–2013 and meteorological monitoring sites (M1 and M2). Solid black circles represent environmental monitoring sites, where the concentrations of criteria air pollutants (O3, PM10, NO2, CO, etc.) are routinely measured.PM samples were collected on a Whatman QM-A quartz microfiber filter (8 × 10 inches) using a high volume air sampler (SIBATA HV-1000F, Japan) operating at a flow rate of 1000 L min−1. Twenty-four-hour (11:00 am to 11:00 am) integrated samples were obtained during three consecutive days, Oct. 28–30, 2011, Oct. 27–29, 2012, and Oct. 25–27, 2013, for the three BFF events, respectively. The dates of the firework events during 2011–2013 were Oct. 29, 28, and 26, respectively. One-fourth of each filter was extracted in 30 mL of 1.03 M HNO3 + 2.23 M HCl mixture by keeping it in an ultrasonic bath for 2 hr at 100°C. Metallic compounds and elements in the filtrates were measured by inductively coupled plasma Optical Emission Spectroscopy (Varian ICP-OES 720-ES). Five analytes (Pb, Cd, Cr, Cu, and As) were measured during the 2011 BFF event, and ten analytes (Pb, Cd, Cr, Cu, As, Al, Ca, Na, K, and Sr) were examined during the 2012 and 2013 events.To examine the impact of fireworks on air quality (especially, PM10 (particles with diameter of 10 micrometers or less) concentration) in Busan, distributions of PM10 were investigated during the daytime (07:00–18:00 LST) and nighttime (19:00–06:00 LST) for the 2012 and 2013 BFF events due to wide spatial and temporal coverage of PM10 observations instead of trace metals. These analyses were carried out based on hourly concentrations of PM10 observed at eighteen (for 2012) and nineteen (for 2013) environmental monitoring sites in Busan, operated by the Korean Ministry of Environment (Figure 1). In order to deduce the dispersion of trace metals released from the BFF events, the observations of meteorological variables (e.g., temp., RH, wind speed, wind direction, and rainfall) obtained at two meteorological monitoring sites (M1 and M2) close to the environmental monitoring sites (Figure 1) and numerical simulation of wind fields were used in this study.


## 2.2. Estimation of Trace Metal Emissions in PM

The emissions of trace metals and elements in PM were estimated using their emission factors and the amounts of firework consumed. The data of firework consumption was obtained from the Organizing Committee for Busan Culture and Tourism Festival (http://festival.busan.kr/KOR/index.asp). Detailed information on the fireworks used during the BFF events of 2012-2013 is presented in Supplementary Table 1 in the Supplementary Material available online at http://dx.doi.org/10.1155/2015/423275 and discussed in Section 3.4. The emission factors of trace metals and elements in PM were adopted from the study of Croteau et al. 2010. Croteau et al. 2010 reported the emission factors of trace metals and elements for various types of fireworks, including Dragon Eggs, Ribbon Fuses, Roman Candles, and Fountains (4 types). In this study, the emission factors of aerial shell types of fireworks were set to the average value of the above four types due to lack of data. The emission factor of fountain fireworks was set to the average value of those of four fountain types. The emission factor of cakes was set to the average value of Roman Candles and Dragon Eggs due to the similarity of the fireworks type. The emission factors of other fireworks such as mine, comet, frame, strobe, row, igniter, and delay chain were also set to the average value of the above four types. The emission factors of Co, As, and Cd were adopted from Passant [10].


## 2.3. Meteorological Model Description

In order to analyze the air mass pathway of metal-rich particles after the burning of fireworks during the BFF events, the meteorological model Weather Research and Forecasting (WRF) version 3.6, which includes fully compressible nonhydrostatic equations, was employed [12]. The model domain was divided into five domains using the two-way nesting method (Supplementary Table 2). The finest domain for the Busan region consisted of 42 sigma vertical levels and 121 × 121 grid cells, with a horizontal mesh width of 0.5 km covering about 34.91°–35.42°N and 128.74°–129.45°E. Detailed descriptions of the grid information and physical options used for the simulation are given in Supplementary Table 2. The initial/lateral boundary conditions were generated by interpolating the National Center for Environmental Prediction (NCEP) Final Analysis (FNL) fields and the sea surface temperature (SST) data. Moreover, the Objective Analysis technique (OBSGRID) was used to improve the first-guess gridded analysis through incorporation of high-resolution (in time and space) surface- and upper-level observations. The surface boundary conditions were extracted using the Environmental Geographic Information System (EGIS: a 90 m resolution) land cover and the Shuttle Radar Topography Mission (SRTM: 90 m) topography data sets. To simulate the flow structure and wind fields for the 2012 and 2013 BFF events, the WRF simulations were conducted for a period of 144 hr per event (from 00 UTC on the 24th to 00 UTC on the 30th of October 2012 and from 00 UTC on the 22nd to 00 UTC on the 28th of October 2013, resp.), including a spin-up time. Meanwhile, since the spatial coverage of trace metal observations is restricted to three sites only, PM10 as a proxy for trace metals was used to identify indirectly the air mass pathway in atmospheric dispersion of trace metals after the burning of fireworks, combined with the WRF model results (wind field simulation).


## 3. Results and Discussion

### 3.1. 2011 BFF Event (Oct. 29, 2011)

In 2011, the average concentrations of five trace metals, Pb, Cd, Cr, Cu, and As, on the day of the BFF event (Oct. 29) were found to be20.8±5.5, 0.5±0.1, 3.2±1.4, 15.3±6.9, and 6.8±0.7 ng m−3, respectively (Table 1 and Figure 2). The trace metal masses were in the order Pb > Cu > As > Cr > Cd. None of the concentrations were higher than those during the previous day, excluding As, which was a factor of 1.3–1.8 higher except at the A1 site. The As concentration (6.5 ng m−3) at the A1 site on the BFF day was similar to that (6.1 ng m−3) during the previous day. On the next day (Oct. 30), the characteristics of the five trace metals remained the same as the event day. However, the As concentrations (9.8–10.6 ng m−3) at all three sites were a factor of 1.5 (A1)–2.9 (A2) higher than those during the day before the event day (Oct. 28). The trace metal concentrations on Oct. 29-30 were very similar, except for As. The insignificant differences in the trace metal concentrations during these two days were likely to be related to washout effects of the trace metals on the BFF day due to rainfall (9.3 mm).Table 1
Statistical summary (mean ± standard deviation) of meteorological parameters at two sites M1-M2 during the daytime (a) and nighttime (b) and daily mean concentrations of trace metal and elements at three sites A1–A3  (c) during the study periods.
(a)
Daytime
Parameters
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Temp. (°C)
19.1 ± 2.4
19.3 ± 1.1
17.3 ± 0.7
17.4 ± 1.1
19.9 ± 2.2
17.6 ± 3.0
17.6 ± 2.0
16.4 ± 2.3
16.3 ± 2.9
RH (%)
56.1
66.4
73.8
91.5
46.3
57.8
48.7
51.3
46.3
Wind speed (m s−1)
2.0 ± 0.7
2.4 ± 0.9
2.2 ± 0.8
1.7 ± 1.3
3.1 ± 1.1
1.3 ± 0.7
2.5 ± 0.8
1.7 ± 0.6
2.4 ± 1.2
Wind direction
NE/NW
NE/NW
NE
NE
NW/SW
SW/SE
NE
NW/NE
SW
Rainfall (mm)
0
0
0
97
0
0
0
0
0
PM10 (μg m−3)∗
19.9 ± 6.3
22.9 ± 6.7
13.1 ± 4.8
24.4 ± 7.6
27.2 ± 8.8
34.9 ± 4.6
49.2 ± 6.4
34.6 ± 5.4
40.3 ± 7.2
O3 (ppb)∗
—
33 ± 5
35 ± 2
27 ± 8
48 ± 3
34 ± 18
41 ± 12
36 ± 7
45 ± 12
∗Concentrations at the A1 site.
(b)
Nighttime
Parameters
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Temp. (°C)
17.6 ± 0.8
16.1 ± 0.5
15.1 ± 0.7
18.6 ± 0.8
14.4 ± 2.2
15.1 ± 1.2
12.7 ± 1.6
12.1 ± 2.2
11.3 ± 2.0
RH (%)
68.2
84.6
71.4
83.5
55.1
65.9
61.3
66.8
63.2
Wind speed (m s−1)
1.6 ± 0.7
2.4 ± 0.9
2.4 ± 0.6
2.3 ± 0.9
1.0 ± 0.6
1.3 ± 0.9
1.6 ± 0.5
0.9 ± 0.5
0.3 ± 0.3
Wind direction
NE/NW
NE
NE/NW
SW
NW/SW
NW
NW
NW/SW
NE
Rainfall (mm)
0
9.3
0
38
0
0
0
0
0
PM10 (μg m−3)∗
18.6 ± 2.5
19.6 ± 7.6
22.9 ± 3.9
19.1 ± 7.7
32.5 ± 5.0
31.0 ± 5.2
42.8 ± 3.4
35.2 ± 5.5
34.5 ± 2.9
O3 (ppb)∗
37 ± 3
34 ± 5
31 ± 2
34 ± 4
30 ± 6
35 ± 5
25 ± 8
32 ± 8
34 ± 10
∗Concentrations at the A1 site.
(c)
All day
Metal and elements
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Pb (ng m−3)
31.9 ± 2.0
20.8 ± 5.5
20.7 ± 0.7
15.0 ± 2.6
43.7 ± 7.6
34.3 ± 14.5
30.3 ± 11.0
37.3 ± 11.7
30.7 ± 5.7
Cd (ng m−3)
0.8 ± 0.2
0.5 ± 0.1
0.4 ± 0.1
<0.1
1.0 ± 0.0
0.67 ± 0.58
<0.1
<0.1
<0.1
Cr (ng m−3)
4.4 ± 2.0
3.2 ± 1.4
2.6 ± 0.6
9.7 ± 0.6
12.7 ± 0.6
12.7 ± 2.5
1.7 ± 1.5
2.7 ± 1.5
1.3 ± 2.3
Cu (ng m−3)
27.5 ± 9.5
15.3 ± 6.9
15.6 ± 8.7
10.3 ± 3.1
27.7 ± 10.3
21.7 ± 13.3
15.3 ± 4.0
25.7 ± 11.0
29.3 ± 19.7
As (ng m−3)
5.4 ± 1.5
6.8 ± 0.7
10.1 ± 0.4
<0.1
1.0 ± 1.0
6.3 ± 7.6
6.0 ± 3.0
3.0 ± 5.2
1.0 ± 1.7
Sr (ng m−3)
3.0 ± 1.7
5.7 ± 1.5
3.7 ± 1.2
5.3 ± 0.6
14.3 ± 19.6
3.0 ± 1.0
Al (μg m−3)
0.06 ± 0.01
0.32 ± 0.09
0.21 ± 0.07
0.54 ± 0.03
0.47 ± 0.06
0.34 ± 0.04
K (μg m−3)
0.32 ± 0.03
0.42 ± 0.02
0.31 ± 0.08
0.29 ± 0.03
0.52 ± 0.39
0.22 ± 0.17
Na (μg m−3)
4.3 ± 2.6
2.3 ± 0.2
2.7 ± 0.5
0.80 ± 0.32
0.70 ± 0.36
0.35 ± 0.29
Ca (μg m−3)
0.28 ± 0.07
1.0 ± 0.3
0.68 ± 0.20
1.10 ± 0.08
0.85 ± 0.12
0.73 ± 0.08Figure 2
Concentrations of metals during the Busan Fireworks Festival event (Oct. 29) in 2011, measured at three monitoring sites (A1–A3).
(a)
A1
(b)
A2
(c)
A3Predominance of Pb and Cu in trace metal distribution during the pre-BFF day was the same as that after the burning of fireworks (Oct. 29-30), implying no significant contribution of fireworks burning to their total emissions in this event. In contrast, the ratios of As to Cr (2.1–3.9) after the burning of fireworks were significantly higher than that (1.2) during the pre-BFF day, implying significant contribution of fireworks burning to As levels. Note that an annual median (mean) ratio of As to Cr for TSP in Busan in 2011 was 0.8 (0.5) [13]. Annual mean concentration of As in 2011 was 6.2±1.7 ng m−3. Significant enhancement of As concentration during postfireworks was also observed in Taiwan [14]. Note that the concentrations of trace metals during the event day might be significantly reduced due to rainfall. Meanwhile, firework metals during the study period of 2011 exhibited significant positive correlation (r = 0.67~0.91), except for As (negative correlation, r = −0.46~−0.67), pointing their common source (fireworks) (not shown).The meteorological conditions during the three days, observed at two Automatic Weather Stations (AWS) operated by Korea Meteorological Administration (KMA) near the sampling sites, are presented in Table1. Mean daytime temperature and relative humidity were 17.3–19.3°C and 56.1–73.8%, respectively. The main wind direction and mean wind speed during the daytime of the event day were NE (and NW) and 2.4 m s−1, respectively. The mean temperature during the nighttime was 1.5–3.2°C lower than the daytime, while relative humidity was 9.3% higher. Wind speeds during the nighttime were 1.6–2.4 m s−1, showing no distinct difference between day and night. The higher mean concentration at the A3 site can be ascribed in part to the air mass pathway (NE and NW), which may have carried the firework air mass to the sampling site.Out of the three aerosol sampling sites, the PM10 concentration data during the day of the BFF event were available only at site A1. The PM10 concentrations at the A1 site (19.6 μg m−3) during the nighttime of the event day were lower than those (22.9 μg m−3) during the daytime. The PM10 concentrations during the daytime on the next day (13.1 μg m−3) dropped by 30%. This was likely due mainly to the influence of moderate rainfall during the nighttime of the event day. In contrast, the O3 concentrations (34 ppb) during the nighttime of the event day were similar to those (33 ppb) during the daytime, indicating different sources/destruction mechanisms between these two air pollutants. In general, nighttime O3 concentration is lower than daytime O3 concentration due to nighttime titration by NO.


### 3.2. 2012 BFF Event (Oct. 28, 2012)

In 2012, the average concentrations of six trace metals Pb, Cd, Cr, Cu, As, and Sr on the BFF event day (Oct. 28) were found to be44±8, 1.0, 13±1, 28±10, 1.0±1.0, and 5.7±1.5 ng m−3, respectively (Table 1 and Figure 3). In 2012, the distributions of trace metal concentrations were somewhat different from those in 2011. For instance, the trace metal masses were in the order Pb > Cu > Cr > Sr > As, Cd. The As concentration (1.0 ng m−3) was significantly lower compared to that during the 2011 event (6.8 ng m−3). In contrast to the 2011 event, all concentrations during the event day were higher than those during the previous day. The most significant enhancement of trace metal concentration was observed for Pb (44 ng m−3), which was a factor of 2.91 higher than the concentration (15 ng m−3) during the previous day (Oct. 27). Strong enhancement of Pb (oxidizer) level (7 times) after firework burning was also reported in Spain [15]. Significant enhancement (2.7 times) of Cu (as a colorant: blue) concentration during the event day was also observed compared to the pre-BFF day. Unlike 2011 event, the ratio of As to Cr (0.1) during the BFF event day was significantly lower than the annual mean ratio (1.6±1.0) in TSP in 2012 [16], implying insignificant contribution of fireworks burning to As levels. Compared to an annual mean concentration of As (11±16 ng m−3) in 2012, As concentration during the event day was significantly lower, suggesting an insignificant role of fireworks in its ambient level. The ratio dropped to the annual mean ratio next day. In addition, Sr (as a colorant: red) concentration during the event day was somewhat (1.9 times) enhanced, which is one of key tracers (Ba (264 times), K (18 times), and Sr (15 times) of firework burning in Diwali festival [17]). In general, the enhancement of trace metal concentrations during the event day was somewhat weakened (20–43%) compared to those during the next day (Oct. 29). Compared to the 2011 event, the spatial variation of trace metal concentrations with the sampling sites was generally slightly less, except for As.Figure 3
Concentrations of metals and elements during the Busan Fireworks Festival event (Oct. 28) in 2012, measured at three monitoring sites (A1–A3). The concentrations of K, Ca, Al, and Na were scaled down by a factor of 100.
(a)
A1
(b)
A2
(c)
A3The concentrations of the four elements examined were significantly higher than those of the six trace metals, up to three orders of magnitude. For instance, the average concentrations of the elements Al, K, Na, and Ca on the BFF event day were found to be0.32±0.09, 0.42±0.02, 2.34±0.22, and 1.01±0.33 μg m−3, respectively (Table 1). The masses of the four elements were in the order Na > Ca > K > Al. The Na concentrations were a factor of 2.3–7.3 higher than the concentrations of other elements possibly due to sea-salt origin. All concentrations were higher during the event day than during the previous day, except for Na. Concentrations of K (as the oxidizer and tracer in firework burning) and Ca (as a colorant: orange) during the event day were a factor of 1.3 and 3.6 higher than those during pre-BFF day, respectively. Of the four elements, Al (as metallic fuel) concentration (0.32 μg m−3) during the BFF day increased significantly by a factor of 5.4 compared to the previous day (0.06 μg m−3). During the day after the event day, all concentrations decreased to some extent (26–34%), except for Na (16% increase possibly due to the influence of marine air masses), compared to the event day. In general, trace metals and elements such as Cr, Cu, Al, Ca, and Sr during the study period of 2012 exhibited significant correlation between themselves, suggesting their common source (Table 3). The fraction of mineral dust of earth’s crust origin in the aerosol samples can be calculated using the Al concentration (8%, [18]). The fractions of mineral dust during the three days (Oct. 27–29) were 2.1, 8.4, and 8.4% of the total PM10 mass, respectively, indicating an insignificant fraction of mineral dust during the pre-BFF day. The increase of the mineral dust fraction (contamination) after firework burning might be related to the Al emission from fireworks, as Al is also used to give the silvery or “flitter” type effect.The mean daytime temperature and relative humidity were 17.4–19.9°C and 46.3–91.5%, respectively. On Oct. 27, there was significant rainfall (67.5 mm). The main wind direction and mean wind speed during the night of the event day were NW (and SW) and 1.0 m s−1, respectively. The meteorological conditions during the 2012 event were somewhat different from those during the 2011 event. The mean nighttime temperature was 2.4–5.5°C lower than that during the daytime, while the relative humidity was 8-9% higher, except for Oct. 27. Since wind speeds during the nighttime were relatively weak (1.0–2.3 m s−1), the trace metals after the burning of fireworks might not be widely dispersed, causing their accumulation.Unlike the 2011 event, the PM10 concentrations at the A1 site were higher during the nighttime of the event day (32.5 μg m−3) than during the daytime (27.2 μg m−3). The PM10 concentrations during the daytime of the next day (34.9 μg m−3) were similar to those during the nighttime of the event day. The fireworks might have caused up to a 10 μg m−3 increase of PM10 (i.e., the difference between during nighttime and during daytime of the event day) at the coastlines and around the inland regions adjacent to Gwangan Bridge (Figure 4). This suggested that fireworks might increase PM10 levels by up to 37%. Similar enhancement of PM10 levels was also observed during the Diwali festival [4, 17, 19]. Overall, large or moderate increases of PM10 were shown in most of areas (18 sites) during the nighttime of the event day. The main cause of this increase can likely be ascribed to the fireworks, according to the monthly mean PM10 concentrations during the nighttime (40.2 μg m−3) and daytime (43.9 μg m−3) for Oct. 2012 in Busan. In general, the PM10 concentration during the nighttime was somewhat lower than that of the daytime, except for during the fireworks event. Geographical patterns in the increase of PM10 concentration were distinguished in part due to the effects of meteorological conditions (the northwesterly (NW) and southwesterly (SW) winds) during the nighttime of the event day (Figure 5). Unlike the 2011 event, O3 concentrations during the nighttime of the event day (30 ppb) were lower than those during the daytime (48 ppb). This pattern was also observed during the 2013 event.Figure 4
Distribution of daytime ((a) and (d)) and nighttime ((b) and (e)) PM10 concentrations and concentration differences between nighttime and daytime ((c) and (f)) during the BFF event days.Figure 5
Surface wind field at 10 m AGL distribution simulated by the WRF model in the evening (21:00 LST) of the BFF event day, early morning (03:00 LST), and morning (09:00 LST) of the next day in 2012-2013.


### 3.3. 2013 BFF Event (Oct. 26, 2013)

In 2013, the average concentrations of six trace metals Pb, Cd, Cr, Cu, As, and Sr on the BFF event day were found to be37±12, <0.1, 2.7±1.5, 26±11, 3.0±5.2, and 14±20 ng m−3, respectively (Table 1 and Figure 6). In 2013, the distribution of trace metal concentration was somewhat different from those during the event days of 2011-2012. In this case, the trace metal masses were in the order Pb > Cu > Sr > As > Cr > Cd. In addition, the Sr concentration (14 ng m−3) was significantly higher (by a factor of 2.7) compared to the pre-BFF day (5.3 ng m−3), even of the 2012 event (5.7 ng m−3). The ratios of As to Cr (0.8–1.1) after the burning of fireworks (Oct. 26-27) were significantly lower than that (3.5) during the pre-BFF day (Oct. 25). An annual mean ratio (0.3) of As (2.4 ng m−3) to Cr (9.1 ng m−3) for PM10 in 2013 was significantly lower than that (1.1) during the BFF day [20]. Concentrations of As during the event day were similar to the annual mean level of As, whereas Cr was a factor of 3.4 lower than the annual mean, indicating an insignificant contributor of fireworks to ambient Cr level. Like the 2012 event, all concentrations were somewhat higher during the event day than on the previous day (Oct. 25), except for As. Concentrations of Pb, Cr, and Cu during the event day were a factor of 1.2, 1.6, and 1.7 higher than those during the pre-BFF day. This suggested that fireworks might contribute to the enhancement in trace metal concentration. The As concentration decreased both during the event day (50%) and on the next day (84%), compared to the previous day (Oct. 25).Figure 6
Concentrations of metals and elements during the Busan Fireworks Festival event (Oct. 26) in 2013, measured at three monitoring sites (A1–A3). The concentrations of K, Ca, Al, and Na were scaled down by a factor of 100.
(a)
A1
(b)
A2
(c)
A3Interestingly, the concentrations of the trace metals measured during the day after the event day dropped significantly to the levels observed during the pre-BFF day (Oct. 25), with even lower concentrations of As and Sr. This suggested that the dilution time of the air mass at the sampling site may be less than 24 hr. Compared to the 2012 event, the spatial variation of trace metal concentrations over the sampling sites was somewhat higher. The concentrations of Pb (37 ng m−3) and Cu (26 ng m−3) in TSP during the BFF in 2013 were somewhat higher than their annual mean concentrations in PM10 (27 and 22 ng m−3, resp.), whereas Cd concentration (<0.1 ng m−3) during the BFF in 2013 was lower than annual mean values (0.4 ng m−3). This suggested that the impact of firework events on the ambient concentration levels of trace metals was likely to be different depending on their chemical speciation. In this comparison, we assume that these trace metal concentrations between TSP and PM10 are not significant. According to Wang et al. [8], there was no significant difference in Pb and Cu between PM10 and PM2.5 during Lantern Festival in Beijing.The average concentrations of the four elements Al, K, Na, and Ca on the BFF event day were found to be0.47±0.06, 0.52±0.39, 0.70±0.36, and 0.85±0.12 μg m−3, respectively (Table 1). Unlike the 2012 event, the masses of the four elements were in the order Ca > Na > K > Al. The Ca concentration was a factor of 1.2–1.8 higher than the concentrations of other elements. The fractions of mineral dust during the three days (Oct. 25–27) were 13.9, 16.6, and 11.5% of the total PM10 mass, respectively, indicating insignificant fractions of mineral dust during the pre-BFF day. In contrast to trace metal, all concentrations were generally lower during the event day than during the previous day, except for K (as a tracer of firework burning). The concentrations of the element K (0.52 μg m−3) during the BFF day were somewhat enhanced by a factor of 1.72 compared to the previous day (0.30 μg m−3), due to the role in black powder (as the main oxidizer during burning). During the day after the event day, all concentrations decreased to below the pre-BFF concentration levels. The correlation during the study period of 2013 was generally weaker than that during the study period of 2012. In addition, very weak negative correlation between Na and other elements was observed in 2012, whereas significant positive correlation between Na, Al, and K was observed in 2013. This suggested that the sources of Na might be different from those of trace metals during the BFF day.The mean daytime temperature and relative humidity were 16.3–17.6°C and 46.3–51.3%, respectively. The main wind direction and mean wind speed during the night of the event day were NW (and SW) and 0.9 m s−1, respectively. The mean temperature during the nighttime was 4.3–5.0°C lower than that during the daytime, while the relative humidity was 12.6–16.9% higher. Since wind speeds during the nighttime were relatively calm (0.3–1.6 m s−1), the trace metals after firework burning might not be widely dispersed.Unlike the previous events, the PM10 concentrations at the A1 site during the nighttime of the event day (35.2 μg m−3) appeared to be similar to those during the daytime (34.6 μg m−3). In addition, the PM10 concentrations during the daytime of the next day (40.3 μg m−3) were higher than those during the nighttime of the event day. In contrast to the 2012 event, the effect of fireworks on PM10 concentration was shown in some areas (downwind) of Busan, though the magnitude was somewhat low (up to 6 μg m−3 increase) (Figure 4). For instance, during the nighttime of the event, moderate increases of the PM10 occurred mainly in the areas to the northwest of DB, whereas large (or moderate) decreases (2–20 μg m−3) of the PM10 occurred in most other areas of Busan. On average, the monthly PM10 concentrations during the nighttime and daytime for Oct. 2013 were 36.4 μg m−3 and 40.4 μg m−3, respectively. Therefore, the increase of PM10 concentration at the northwest areas was likely due mainly to the fireworks. The concentration differences were likely related in part to the meteorological conditions for each event (Figure 5). For instance, the main wind direction for the 2011 event did not change the next day, whereas that for the 2012 event changed from NW to SW on the next day (with some influence of SE wind). However, the main wind direction for the 2013 event changed from NW to SW on the next day, without influence of other wind directions. As shown in Figure 1, SW wind may have the potential to increase the PM10 concentration due to the anthropogenic sources near the sampling site, whereas SE wind can carry coarse particles of marine origin to some extent, causing lower fractions of fine particles. Meanwhile, annual mean concentrations of PM10 in Busan during 2000 to 2013 ranged from 43 (2012) to 62 (2000) μg m−3 with a downward trend (a slope of −1.48 μg m−3 yr−1, r2=0.76) [21]. Thus, the burning of fireworks might become a significant contributor to ambient PM10 levels in the future due to a long-term downward trend of PM10.Like the 2011 and 2012 events, the O3 concentrations during the nighttime of the event day (32 ppb) were also similar to those during the daytime (36 ppb). This unique similarity in the O3 concentrations between daytime and nighttime of the event day might be related in part to the primary emission of O3 without NOx participation [6].


### 3.4. Comparison of BFF with Other Major Festivals of the World

The magnitudes of trace metal enhancement during the BFF events were much smaller compared to the Diwali festival in India, wherein a tendency of trace metal enhancement was observed (Table2). For instance, the concentrations of Ba, K, Al, and Sr during the Diwali festival (Hyderabad and Delhi) were several tens of times up to 3 orders of magnitude higher than the background values [17, 22]. Significant enhancement of elemental carbon (40.5 μg m−3, 4.3 times) and PM10 (753 μg m−3, 2.49 times) was also observed during the Diwali festival, and firework aerosol contributed 23–33% to the ambient PM10 [4, 17, 19]. However, the PM10 concentrations at the A1 sites observed herein during the BFF events were not higher than the urban (Busan) background levels, due in part to interference from local anthropogenic sources and the long distance (2 km) from the fireworks burst. This suggested that the burning of fireworks might be an insignificant source of PM10 at the A1 site.Table 2
Comparison of chemical components and elemental concentrations of particles during fireworks events.
Diwali India
Lantern Festival
Las Fallas Valencia
World Cup Milan
New Year Mainz
July 4, USA
This study
PM10
507
466
42
46–71
8 (PM2.5)
20–35
S
O
4
2
-
8.3
2.7–5.1
36
N
O
3
-
<0.4–4.5
6.5
N
H
4
+
1.2
0.9–2.5
2.4
OC
10 (OM + EC)
7.9–13
EC
1.3–5.4
1
Fe
6
5
0.4
0.5–1.7
30
Na
14
4
0.3
0.05
0.7–2.3
Mg
21
6
0.5
<0.1–0.6
42
Al
38
10
1.8 (Al2O3)
0.4–0.7
92
0.3–0.5
Si
0.8–1.8
0.07
S
53
40
0.8–1.8
0.5
Cl
6
20
<0.07–0.2
5.1
K
47
50
5
0.2–1.0
33
0.9
0.4–0.5
P
1.4
0.3
0.07
Ca
17
7
1.1
0.3–1.5
0.03
0.8–1.0
Ti ng
1700
50
28–53
15
V
330
12
<6
8
Cr
290
1.9
<4–11
2.7–12.7
Mn
930
400
7–35
3
Sn
12
Ni
70
2.8
2–7
Cu
550
600
64
20–105
4
15–28
Zn
820
3000
38
82–276
8
Br
7
4–12
2
Pb
360
1100
244
9–57
8
21–44
Sr
140
800
82
<3–139
9
6–14
Ba
16800
4500
303
<20–156
28
Sb
49
Diwali, 2009, Delhi, Lantern Festival, 2006, Beijing, China; India; Las Fallas, 2005, Valencia, Spain; FIFA World Cup victory, 2006, Milan, Italy; New Year, 2005, Mainz, Germany; Independence Day, 1990, Washington State, USA.Table 3
Correlation between elements over the study period in 2012 (Oct. 27–Oct. 29)–2013 (Oct. 25–Oct. 27).
(a)
2012
Pb
Cd
Cr
Cu
As
Al
K
Na
Ca
Sr
Pb
—
0.722
0.908
—
0.847
0.469
−0.366
0.795
0.669
Cd
—
—
—
—
—
—
—
—
Cr
0.462
—
0.615
0.513
−0.428
0.564
0.295
Cu
—
0.832
0.299
−0.300
0.801
0.737
As
—
—
—
—
—
Al
0.535
−0.516
0.987
0.808
K
−0.088
0.513
0.521
Na
−0.419
0.051
Ca
0.869
Sr
—: correlation coefficients between Cd, As, and other elements were not available due to being below detection limit levels for Cd and As.
(b)
2013
Pb
Cd
Cr
Cu
As
Al
K
Na
Ca
Sr
Pb
—
−0.034
0.547
—
0.174
0.395
0.106
0.135
0.366
Cd
—
—
—
—
—
—
—
—
Cr
0.522
—
0.362
0.574
0.504
0.145
0.496
Cu
—
−0.096
0.468
0.179
−0.131
0.379
As
—
—
—
—
—
Al
0.500
0.827
0.934
0.445
K
0.722
0.333
0.946
Na
0.756
0.613
Ca
0.286
Sr
—: correlation coefficients between Cd, As, and other elements were not available due to being below detection limit levels for Cd and As.During the Lantern Festival in Beijing, the concentrations of primary inorganic components such as Ba, K, Sr, Cl−, Pb, and Mg as well as secondary organic components such as oxalate, malonate, succinate, and glutarate were reported to be over five times higher than those in the preevent days [8]. The primary inorganic components and secondary organic components during fireworks were mainly in the fine and coarse modes, respectively [8]. The impact of fireworks on the physical characteristics of aerosol particles such as the number concentration of small accumulation modes (100–500 nm) causing a clear shift of the particles from nucleation and Aitken mode to small accumulation mode at the peak of the fireworks event was also reported [23]. Notably, elevated levels of K, Al, Ti, Mg, Pb, Ba, Sr, Cu, and Sb (up to 3 times) were also observed during Las Fallas in Spain [3]. In addition, during the firework event in Milan (Italy) for the celebration of wining the football World Cup (2006), enhancement of the Sr (120 times), Mg (22 times), Ba (12 times), K (11 times), and Cu (6 times) metal concentrations was reported [24]. Although the sampling time (24 hr: 11 am to 11 am) in the present study was relatively long, the enhancement of some trace metals and elements was within the same orders of magnitude compared to the literature.


### 3.5. Emission of Trace Metals and Elements during the BFF Events

In 2012, 26,447 fireworks were used, while the amount used in 2013 increased by 37% (36,176) compared to 2012 (Supplementary Table1). Aerial shell type fireworks made up 29% (8,245)–31% (10,316) of the total fireworks, with diameters of 3–25 inches and the dominant size of 5-6 inches. The charge quantities of aerial shells are linearly dependent on their diameters (0.03–3 kg shot−1). Fireworks such as igniter, mine, comet, row, and Niagara Fall (2,060–10,000) were also used significantly during the events. In order to assess the uncertainties of emission estimates of trace metals after firework burning, the best emission estimates were calculated using average values of the emission factors obtained from Croteau et al. 2010, while the maximum and minimum emission estimates were obtained using the lowest and highest emission factors among the four types of fireworks, respectively.The largest metal emission during the events was K (128–164 kg), followed by Pb, Cd, Cu, Mg, Ba, As, Al, Ga, Co, and Na (Table4). Emissions of other trace metals and elements were less than 1 kg. The total emissions of trace metals and elements during the 2013 event were a factor of 1.28 higher than those during the 2012 event. Interestingly, enhancement of the Pb concentration by a factor of 2.91 during the 2012 event was supported by the current emission strength of Pb. Meanwhile, the annual anthropogenic emissions of Zn, Pb, Ni, Co, Sb, Na, Cd, and K in Korea during the year 2011 were reported to be 89, 19, 13, 8, 6, 1.9, 0.2, and 0.01 tons, respectively (http://ncis.nier.go.kr/prtr/index.do). In general, firework burning might be an insignificant contributor to the national atmospheric emissions. However, firework burning might be a predominant emission source of airborne K.Table 4
Estimated emissions of trace metals from the BFF during the study periods (in kg).
Elements
2012
2013
Max.
Min.
Best
Max.
Min.
Best
TSP
502.762
240.608
393.578
644.490
308.435
504.946
K
161.602
82.597
127.829
207.158
105.881
164.064
Mg
24.420
4.669
12.052
31.304
5.985
15.424
Ba
22.624
0.108
8.284
29.002
0.138
10.707
Na
4.309
0.205
1.098
5.524
0.262
1.403
Ca
2.478
0.079
0.323
3.176
0.101
0.413
Cu
28.370
0.162
15.754
36.368
0.207
20.157
Al
6.823
2.729
4.471
8.747
3.499
5.727
Pb
96.961
0.007
36.903
124.295
0.009
47.664
Ga
5.028
0.017
1.853
6.445
0.022
2.394
Sr
2.550
0.031
0.249
3.268
0.039
0.318
Zn
2.262
0.086
0.723
2.900
0.110
0.936
Fe
2.011
0.151
0.807
2.578
0.193
1.031
Bi
1.939
0.000
0.618
2.486
0.000
0.787
P
0.190
0.040
0.095
0.244
0.051
0.121
Mn
0.140
0.036
0.083
0.180
0.046
0.106
Ti
0.255
0.010
0.060
0.327
0.013
0.077
Cr
0.431
0.006
0.139
0.552
0.008
0.178
Sn
0.072
0.001
0.029
0.092
0.001
0.037
Si
1.257
0.014
0.402
1.611
0.018
0.514
Cr6+
0.043
0.001
0.024
0.055
0.001
0.031
Rb
0.032
0.012
0.021
0.041
0.015
0.027
Sb
0.019
0.000
0.007
0.024
0.000
0.010
V
0.169
0.001
0.021
0.216
0.002
0.026
Te
0.025
0.000
0.010
0.032
0.000
0.013
Co
1.594
2.076
As
4.787
6.232
Cd
23.967
31.204
Total
866.77
331.57
635.78
1111.12
425.04
816.62


## 3.1. 2011 BFF Event (Oct. 29, 2011)

In 2011, the average concentrations of five trace metals, Pb, Cd, Cr, Cu, and As, on the day of the BFF event (Oct. 29) were found to be20.8±5.5, 0.5±0.1, 3.2±1.4, 15.3±6.9, and 6.8±0.7 ng m−3, respectively (Table 1 and Figure 2). The trace metal masses were in the order Pb > Cu > As > Cr > Cd. None of the concentrations were higher than those during the previous day, excluding As, which was a factor of 1.3–1.8 higher except at the A1 site. The As concentration (6.5 ng m−3) at the A1 site on the BFF day was similar to that (6.1 ng m−3) during the previous day. On the next day (Oct. 30), the characteristics of the five trace metals remained the same as the event day. However, the As concentrations (9.8–10.6 ng m−3) at all three sites were a factor of 1.5 (A1)–2.9 (A2) higher than those during the day before the event day (Oct. 28). The trace metal concentrations on Oct. 29-30 were very similar, except for As. The insignificant differences in the trace metal concentrations during these two days were likely to be related to washout effects of the trace metals on the BFF day due to rainfall (9.3 mm).Table 1
Statistical summary (mean ± standard deviation) of meteorological parameters at two sites M1-M2 during the daytime (a) and nighttime (b) and daily mean concentrations of trace metal and elements at three sites A1–A3  (c) during the study periods.
(a)
Daytime
Parameters
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Temp. (°C)
19.1 ± 2.4
19.3 ± 1.1
17.3 ± 0.7
17.4 ± 1.1
19.9 ± 2.2
17.6 ± 3.0
17.6 ± 2.0
16.4 ± 2.3
16.3 ± 2.9
RH (%)
56.1
66.4
73.8
91.5
46.3
57.8
48.7
51.3
46.3
Wind speed (m s−1)
2.0 ± 0.7
2.4 ± 0.9
2.2 ± 0.8
1.7 ± 1.3
3.1 ± 1.1
1.3 ± 0.7
2.5 ± 0.8
1.7 ± 0.6
2.4 ± 1.2
Wind direction
NE/NW
NE/NW
NE
NE
NW/SW
SW/SE
NE
NW/NE
SW
Rainfall (mm)
0
0
0
97
0
0
0
0
0
PM10 (μg m−3)∗
19.9 ± 6.3
22.9 ± 6.7
13.1 ± 4.8
24.4 ± 7.6
27.2 ± 8.8
34.9 ± 4.6
49.2 ± 6.4
34.6 ± 5.4
40.3 ± 7.2
O3 (ppb)∗
—
33 ± 5
35 ± 2
27 ± 8
48 ± 3
34 ± 18
41 ± 12
36 ± 7
45 ± 12
∗Concentrations at the A1 site.
(b)
Nighttime
Parameters
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Temp. (°C)
17.6 ± 0.8
16.1 ± 0.5
15.1 ± 0.7
18.6 ± 0.8
14.4 ± 2.2
15.1 ± 1.2
12.7 ± 1.6
12.1 ± 2.2
11.3 ± 2.0
RH (%)
68.2
84.6
71.4
83.5
55.1
65.9
61.3
66.8
63.2
Wind speed (m s−1)
1.6 ± 0.7
2.4 ± 0.9
2.4 ± 0.6
2.3 ± 0.9
1.0 ± 0.6
1.3 ± 0.9
1.6 ± 0.5
0.9 ± 0.5
0.3 ± 0.3
Wind direction
NE/NW
NE
NE/NW
SW
NW/SW
NW
NW
NW/SW
NE
Rainfall (mm)
0
9.3
0
38
0
0
0
0
0
PM10 (μg m−3)∗
18.6 ± 2.5
19.6 ± 7.6
22.9 ± 3.9
19.1 ± 7.7
32.5 ± 5.0
31.0 ± 5.2
42.8 ± 3.4
35.2 ± 5.5
34.5 ± 2.9
O3 (ppb)∗
37 ± 3
34 ± 5
31 ± 2
34 ± 4
30 ± 6
35 ± 5
25 ± 8
32 ± 8
34 ± 10
∗Concentrations at the A1 site.
(c)
All day
Metal and elements
2011
2012
2013
Oct. 28
Oct. 29
Oct. 30
Oct. 27
Oct. 28
Oct. 29
Oct. 25
Oct. 26
Oct. 27
Pb (ng m−3)
31.9 ± 2.0
20.8 ± 5.5
20.7 ± 0.7
15.0 ± 2.6
43.7 ± 7.6
34.3 ± 14.5
30.3 ± 11.0
37.3 ± 11.7
30.7 ± 5.7
Cd (ng m−3)
0.8 ± 0.2
0.5 ± 0.1
0.4 ± 0.1
<0.1
1.0 ± 0.0
0.67 ± 0.58
<0.1
<0.1
<0.1
Cr (ng m−3)
4.4 ± 2.0
3.2 ± 1.4
2.6 ± 0.6
9.7 ± 0.6
12.7 ± 0.6
12.7 ± 2.5
1.7 ± 1.5
2.7 ± 1.5
1.3 ± 2.3
Cu (ng m−3)
27.5 ± 9.5
15.3 ± 6.9
15.6 ± 8.7
10.3 ± 3.1
27.7 ± 10.3
21.7 ± 13.3
15.3 ± 4.0
25.7 ± 11.0
29.3 ± 19.7
As (ng m−3)
5.4 ± 1.5
6.8 ± 0.7
10.1 ± 0.4
<0.1
1.0 ± 1.0
6.3 ± 7.6
6.0 ± 3.0
3.0 ± 5.2
1.0 ± 1.7
Sr (ng m−3)
3.0 ± 1.7
5.7 ± 1.5
3.7 ± 1.2
5.3 ± 0.6
14.3 ± 19.6
3.0 ± 1.0
Al (μg m−3)
0.06 ± 0.01
0.32 ± 0.09
0.21 ± 0.07
0.54 ± 0.03
0.47 ± 0.06
0.34 ± 0.04
K (μg m−3)
0.32 ± 0.03
0.42 ± 0.02
0.31 ± 0.08
0.29 ± 0.03
0.52 ± 0.39
0.22 ± 0.17
Na (μg m−3)
4.3 ± 2.6
2.3 ± 0.2
2.7 ± 0.5
0.80 ± 0.32
0.70 ± 0.36
0.35 ± 0.29
Ca (μg m−3)
0.28 ± 0.07
1.0 ± 0.3
0.68 ± 0.20
1.10 ± 0.08
0.85 ± 0.12
0.73 ± 0.08Figure 2
Concentrations of metals during the Busan Fireworks Festival event (Oct. 29) in 2011, measured at three monitoring sites (A1–A3).
(a)
A1
(b)
A2
(c)
A3Predominance of Pb and Cu in trace metal distribution during the pre-BFF day was the same as that after the burning of fireworks (Oct. 29-30), implying no significant contribution of fireworks burning to their total emissions in this event. In contrast, the ratios of As to Cr (2.1–3.9) after the burning of fireworks were significantly higher than that (1.2) during the pre-BFF day, implying significant contribution of fireworks burning to As levels. Note that an annual median (mean) ratio of As to Cr for TSP in Busan in 2011 was 0.8 (0.5) [13]. Annual mean concentration of As in 2011 was 6.2±1.7 ng m−3. Significant enhancement of As concentration during postfireworks was also observed in Taiwan [14]. Note that the concentrations of trace metals during the event day might be significantly reduced due to rainfall. Meanwhile, firework metals during the study period of 2011 exhibited significant positive correlation (r = 0.67~0.91), except for As (negative correlation, r = −0.46~−0.67), pointing their common source (fireworks) (not shown).The meteorological conditions during the three days, observed at two Automatic Weather Stations (AWS) operated by Korea Meteorological Administration (KMA) near the sampling sites, are presented in Table1. Mean daytime temperature and relative humidity were 17.3–19.3°C and 56.1–73.8%, respectively. The main wind direction and mean wind speed during the daytime of the event day were NE (and NW) and 2.4 m s−1, respectively. The mean temperature during the nighttime was 1.5–3.2°C lower than the daytime, while relative humidity was 9.3% higher. Wind speeds during the nighttime were 1.6–2.4 m s−1, showing no distinct difference between day and night. The higher mean concentration at the A3 site can be ascribed in part to the air mass pathway (NE and NW), which may have carried the firework air mass to the sampling site.Out of the three aerosol sampling sites, the PM10 concentration data during the day of the BFF event were available only at site A1. The PM10 concentrations at the A1 site (19.6 μg m−3) during the nighttime of the event day were lower than those (22.9 μg m−3) during the daytime. The PM10 concentrations during the daytime on the next day (13.1 μg m−3) dropped by 30%. This was likely due mainly to the influence of moderate rainfall during the nighttime of the event day. In contrast, the O3 concentrations (34 ppb) during the nighttime of the event day were similar to those (33 ppb) during the daytime, indicating different sources/destruction mechanisms between these two air pollutants. In general, nighttime O3 concentration is lower than daytime O3 concentration due to nighttime titration by NO.


## 3.2. 2012 BFF Event (Oct. 28, 2012)

In 2012, the average concentrations of six trace metals Pb, Cd, Cr, Cu, As, and Sr on the BFF event day (Oct. 28) were found to be44±8, 1.0, 13±1, 28±10, 1.0±1.0, and 5.7±1.5 ng m−3, respectively (Table 1 and Figure 3). In 2012, the distributions of trace metal concentrations were somewhat different from those in 2011. For instance, the trace metal masses were in the order Pb > Cu > Cr > Sr > As, Cd. The As concentration (1.0 ng m−3) was significantly lower compared to that during the 2011 event (6.8 ng m−3). In contrast to the 2011 event, all concentrations during the event day were higher than those during the previous day. The most significant enhancement of trace metal concentration was observed for Pb (44 ng m−3), which was a factor of 2.91 higher than the concentration (15 ng m−3) during the previous day (Oct. 27). Strong enhancement of Pb (oxidizer) level (7 times) after firework burning was also reported in Spain [15]. Significant enhancement (2.7 times) of Cu (as a colorant: blue) concentration during the event day was also observed compared to the pre-BFF day. Unlike 2011 event, the ratio of As to Cr (0.1) during the BFF event day was significantly lower than the annual mean ratio (1.6±1.0) in TSP in 2012 [16], implying insignificant contribution of fireworks burning to As levels. Compared to an annual mean concentration of As (11±16 ng m−3) in 2012, As concentration during the event day was significantly lower, suggesting an insignificant role of fireworks in its ambient level. The ratio dropped to the annual mean ratio next day. In addition, Sr (as a colorant: red) concentration during the event day was somewhat (1.9 times) enhanced, which is one of key tracers (Ba (264 times), K (18 times), and Sr (15 times) of firework burning in Diwali festival [17]). In general, the enhancement of trace metal concentrations during the event day was somewhat weakened (20–43%) compared to those during the next day (Oct. 29). Compared to the 2011 event, the spatial variation of trace metal concentrations with the sampling sites was generally slightly less, except for As.Figure 3
Concentrations of metals and elements during the Busan Fireworks Festival event (Oct. 28) in 2012, measured at three monitoring sites (A1–A3). The concentrations of K, Ca, Al, and Na were scaled down by a factor of 100.
(a)
A1
(b)
A2
(c)
A3The concentrations of the four elements examined were significantly higher than those of the six trace metals, up to three orders of magnitude. For instance, the average concentrations of the elements Al, K, Na, and Ca on the BFF event day were found to be0.32±0.09, 0.42±0.02, 2.34±0.22, and 1.01±0.33 μg m−3, respectively (Table 1). The masses of the four elements were in the order Na > Ca > K > Al. The Na concentrations were a factor of 2.3–7.3 higher than the concentrations of other elements possibly due to sea-salt origin. All concentrations were higher during the event day than during the previous day, except for Na. Concentrations of K (as the oxidizer and tracer in firework burning) and Ca (as a colorant: orange) during the event day were a factor of 1.3 and 3.6 higher than those during pre-BFF day, respectively. Of the four elements, Al (as metallic fuel) concentration (0.32 μg m−3) during the BFF day increased significantly by a factor of 5.4 compared to the previous day (0.06 μg m−3). During the day after the event day, all concentrations decreased to some extent (26–34%), except for Na (16% increase possibly due to the influence of marine air masses), compared to the event day. In general, trace metals and elements such as Cr, Cu, Al, Ca, and Sr during the study period of 2012 exhibited significant correlation between themselves, suggesting their common source (Table 3). The fraction of mineral dust of earth’s crust origin in the aerosol samples can be calculated using the Al concentration (8%, [18]). The fractions of mineral dust during the three days (Oct. 27–29) were 2.1, 8.4, and 8.4% of the total PM10 mass, respectively, indicating an insignificant fraction of mineral dust during the pre-BFF day. The increase of the mineral dust fraction (contamination) after firework burning might be related to the Al emission from fireworks, as Al is also used to give the silvery or “flitter” type effect.The mean daytime temperature and relative humidity were 17.4–19.9°C and 46.3–91.5%, respectively. On Oct. 27, there was significant rainfall (67.5 mm). The main wind direction and mean wind speed during the night of the event day were NW (and SW) and 1.0 m s−1, respectively. The meteorological conditions during the 2012 event were somewhat different from those during the 2011 event. The mean nighttime temperature was 2.4–5.5°C lower than that during the daytime, while the relative humidity was 8-9% higher, except for Oct. 27. Since wind speeds during the nighttime were relatively weak (1.0–2.3 m s−1), the trace metals after the burning of fireworks might not be widely dispersed, causing their accumulation.Unlike the 2011 event, the PM10 concentrations at the A1 site were higher during the nighttime of the event day (32.5 μg m−3) than during the daytime (27.2 μg m−3). The PM10 concentrations during the daytime of the next day (34.9 μg m−3) were similar to those during the nighttime of the event day. The fireworks might have caused up to a 10 μg m−3 increase of PM10 (i.e., the difference between during nighttime and during daytime of the event day) at the coastlines and around the inland regions adjacent to Gwangan Bridge (Figure 4). This suggested that fireworks might increase PM10 levels by up to 37%. Similar enhancement of PM10 levels was also observed during the Diwali festival [4, 17, 19]. Overall, large or moderate increases of PM10 were shown in most of areas (18 sites) during the nighttime of the event day. The main cause of this increase can likely be ascribed to the fireworks, according to the monthly mean PM10 concentrations during the nighttime (40.2 μg m−3) and daytime (43.9 μg m−3) for Oct. 2012 in Busan. In general, the PM10 concentration during the nighttime was somewhat lower than that of the daytime, except for during the fireworks event. Geographical patterns in the increase of PM10 concentration were distinguished in part due to the effects of meteorological conditions (the northwesterly (NW) and southwesterly (SW) winds) during the nighttime of the event day (Figure 5). Unlike the 2011 event, O3 concentrations during the nighttime of the event day (30 ppb) were lower than those during the daytime (48 ppb). This pattern was also observed during the 2013 event.Figure 4
Distribution of daytime ((a) and (d)) and nighttime ((b) and (e)) PM10 concentrations and concentration differences between nighttime and daytime ((c) and (f)) during the BFF event days.Figure 5
Surface wind field at 10 m AGL distribution simulated by the WRF model in the evening (21:00 LST) of the BFF event day, early morning (03:00 LST), and morning (09:00 LST) of the next day in 2012-2013.


## 3.3. 2013 BFF Event (Oct. 26, 2013)

In 2013, the average concentrations of six trace metals Pb, Cd, Cr, Cu, As, and Sr on the BFF event day were found to be37±12, <0.1, 2.7±1.5, 26±11, 3.0±5.2, and 14±20 ng m−3, respectively (Table 1 and Figure 6). In 2013, the distribution of trace metal concentration was somewhat different from those during the event days of 2011-2012. In this case, the trace metal masses were in the order Pb > Cu > Sr > As > Cr > Cd. In addition, the Sr concentration (14 ng m−3) was significantly higher (by a factor of 2.7) compared to the pre-BFF day (5.3 ng m−3), even of the 2012 event (5.7 ng m−3). The ratios of As to Cr (0.8–1.1) after the burning of fireworks (Oct. 26-27) were significantly lower than that (3.5) during the pre-BFF day (Oct. 25). An annual mean ratio (0.3) of As (2.4 ng m−3) to Cr (9.1 ng m−3) for PM10 in 2013 was significantly lower than that (1.1) during the BFF day [20]. Concentrations of As during the event day were similar to the annual mean level of As, whereas Cr was a factor of 3.4 lower than the annual mean, indicating an insignificant contributor of fireworks to ambient Cr level. Like the 2012 event, all concentrations were somewhat higher during the event day than on the previous day (Oct. 25), except for As. Concentrations of Pb, Cr, and Cu during the event day were a factor of 1.2, 1.6, and 1.7 higher than those during the pre-BFF day. This suggested that fireworks might contribute to the enhancement in trace metal concentration. The As concentration decreased both during the event day (50%) and on the next day (84%), compared to the previous day (Oct. 25).Figure 6
Concentrations of metals and elements during the Busan Fireworks Festival event (Oct. 26) in 2013, measured at three monitoring sites (A1–A3). The concentrations of K, Ca, Al, and Na were scaled down by a factor of 100.
(a)
A1
(b)
A2
(c)
A3Interestingly, the concentrations of the trace metals measured during the day after the event day dropped significantly to the levels observed during the pre-BFF day (Oct. 25), with even lower concentrations of As and Sr. This suggested that the dilution time of the air mass at the sampling site may be less than 24 hr. Compared to the 2012 event, the spatial variation of trace metal concentrations over the sampling sites was somewhat higher. The concentrations of Pb (37 ng m−3) and Cu (26 ng m−3) in TSP during the BFF in 2013 were somewhat higher than their annual mean concentrations in PM10 (27 and 22 ng m−3, resp.), whereas Cd concentration (<0.1 ng m−3) during the BFF in 2013 was lower than annual mean values (0.4 ng m−3). This suggested that the impact of firework events on the ambient concentration levels of trace metals was likely to be different depending on their chemical speciation. In this comparison, we assume that these trace metal concentrations between TSP and PM10 are not significant. According to Wang et al. [8], there was no significant difference in Pb and Cu between PM10 and PM2.5 during Lantern Festival in Beijing.The average concentrations of the four elements Al, K, Na, and Ca on the BFF event day were found to be0.47±0.06, 0.52±0.39, 0.70±0.36, and 0.85±0.12 μg m−3, respectively (Table 1). Unlike the 2012 event, the masses of the four elements were in the order Ca > Na > K > Al. The Ca concentration was a factor of 1.2–1.8 higher than the concentrations of other elements. The fractions of mineral dust during the three days (Oct. 25–27) were 13.9, 16.6, and 11.5% of the total PM10 mass, respectively, indicating insignificant fractions of mineral dust during the pre-BFF day. In contrast to trace metal, all concentrations were generally lower during the event day than during the previous day, except for K (as a tracer of firework burning). The concentrations of the element K (0.52 μg m−3) during the BFF day were somewhat enhanced by a factor of 1.72 compared to the previous day (0.30 μg m−3), due to the role in black powder (as the main oxidizer during burning). During the day after the event day, all concentrations decreased to below the pre-BFF concentration levels. The correlation during the study period of 2013 was generally weaker than that during the study period of 2012. In addition, very weak negative correlation between Na and other elements was observed in 2012, whereas significant positive correlation between Na, Al, and K was observed in 2013. This suggested that the sources of Na might be different from those of trace metals during the BFF day.The mean daytime temperature and relative humidity were 16.3–17.6°C and 46.3–51.3%, respectively. The main wind direction and mean wind speed during the night of the event day were NW (and SW) and 0.9 m s−1, respectively. The mean temperature during the nighttime was 4.3–5.0°C lower than that during the daytime, while the relative humidity was 12.6–16.9% higher. Since wind speeds during the nighttime were relatively calm (0.3–1.6 m s−1), the trace metals after firework burning might not be widely dispersed.Unlike the previous events, the PM10 concentrations at the A1 site during the nighttime of the event day (35.2 μg m−3) appeared to be similar to those during the daytime (34.6 μg m−3). In addition, the PM10 concentrations during the daytime of the next day (40.3 μg m−3) were higher than those during the nighttime of the event day. In contrast to the 2012 event, the effect of fireworks on PM10 concentration was shown in some areas (downwind) of Busan, though the magnitude was somewhat low (up to 6 μg m−3 increase) (Figure 4). For instance, during the nighttime of the event, moderate increases of the PM10 occurred mainly in the areas to the northwest of DB, whereas large (or moderate) decreases (2–20 μg m−3) of the PM10 occurred in most other areas of Busan. On average, the monthly PM10 concentrations during the nighttime and daytime for Oct. 2013 were 36.4 μg m−3 and 40.4 μg m−3, respectively. Therefore, the increase of PM10 concentration at the northwest areas was likely due mainly to the fireworks. The concentration differences were likely related in part to the meteorological conditions for each event (Figure 5). For instance, the main wind direction for the 2011 event did not change the next day, whereas that for the 2012 event changed from NW to SW on the next day (with some influence of SE wind). However, the main wind direction for the 2013 event changed from NW to SW on the next day, without influence of other wind directions. As shown in Figure 1, SW wind may have the potential to increase the PM10 concentration due to the anthropogenic sources near the sampling site, whereas SE wind can carry coarse particles of marine origin to some extent, causing lower fractions of fine particles. Meanwhile, annual mean concentrations of PM10 in Busan during 2000 to 2013 ranged from 43 (2012) to 62 (2000) μg m−3 with a downward trend (a slope of −1.48 μg m−3 yr−1, r2=0.76) [21]. Thus, the burning of fireworks might become a significant contributor to ambient PM10 levels in the future due to a long-term downward trend of PM10.Like the 2011 and 2012 events, the O3 concentrations during the nighttime of the event day (32 ppb) were also similar to those during the daytime (36 ppb). This unique similarity in the O3 concentrations between daytime and nighttime of the event day might be related in part to the primary emission of O3 without NOx participation [6].


## 3.4. Comparison of BFF with Other Major Festivals of the World

The magnitudes of trace metal enhancement during the BFF events were much smaller compared to the Diwali festival in India, wherein a tendency of trace metal enhancement was observed (Table2). For instance, the concentrations of Ba, K, Al, and Sr during the Diwali festival (Hyderabad and Delhi) were several tens of times up to 3 orders of magnitude higher than the background values [17, 22]. Significant enhancement of elemental carbon (40.5 μg m−3, 4.3 times) and PM10 (753 μg m−3, 2.49 times) was also observed during the Diwali festival, and firework aerosol contributed 23–33% to the ambient PM10 [4, 17, 19]. However, the PM10 concentrations at the A1 sites observed herein during the BFF events were not higher than the urban (Busan) background levels, due in part to interference from local anthropogenic sources and the long distance (2 km) from the fireworks burst. This suggested that the burning of fireworks might be an insignificant source of PM10 at the A1 site.Table 2
Comparison of chemical components and elemental concentrations of particles during fireworks events.
Diwali India
Lantern Festival
Las Fallas Valencia
World Cup Milan
New Year Mainz
July 4, USA
This study
PM10
507
466
42
46–71
8 (PM2.5)
20–35
S
O
4
2
-
8.3
2.7–5.1
36
N
O
3
-
<0.4–4.5
6.5
N
H
4
+
1.2
0.9–2.5
2.4
OC
10 (OM + EC)
7.9–13
EC
1.3–5.4
1
Fe
6
5
0.4
0.5–1.7
30
Na
14
4
0.3
0.05
0.7–2.3
Mg
21
6
0.5
<0.1–0.6
42
Al
38
10
1.8 (Al2O3)
0.4–0.7
92
0.3–0.5
Si
0.8–1.8
0.07
S
53
40
0.8–1.8
0.5
Cl
6
20
<0.07–0.2
5.1
K
47
50
5
0.2–1.0
33
0.9
0.4–0.5
P
1.4
0.3
0.07
Ca
17
7
1.1
0.3–1.5
0.03
0.8–1.0
Ti ng
1700
50
28–53
15
V
330
12
<6
8
Cr
290
1.9
<4–11
2.7–12.7
Mn
930
400
7–35
3
Sn
12
Ni
70
2.8
2–7
Cu
550
600
64
20–105
4
15–28
Zn
820
3000
38
82–276
8
Br
7
4–12
2
Pb
360
1100
244
9–57
8
21–44
Sr
140
800
82
<3–139
9
6–14
Ba
16800
4500
303
<20–156
28
Sb
49
Diwali, 2009, Delhi, Lantern Festival, 2006, Beijing, China; India; Las Fallas, 2005, Valencia, Spain; FIFA World Cup victory, 2006, Milan, Italy; New Year, 2005, Mainz, Germany; Independence Day, 1990, Washington State, USA.Table 3
Correlation between elements over the study period in 2012 (Oct. 27–Oct. 29)–2013 (Oct. 25–Oct. 27).
(a)
2012
Pb
Cd
Cr
Cu
As
Al
K
Na
Ca
Sr
Pb
—
0.722
0.908
—
0.847
0.469
−0.366
0.795
0.669
Cd
—
—
—
—
—
—
—
—
Cr
0.462
—
0.615
0.513
−0.428
0.564
0.295
Cu
—
0.832
0.299
−0.300
0.801
0.737
As
—
—
—
—
—
Al
0.535
−0.516
0.987
0.808
K
−0.088
0.513
0.521
Na
−0.419
0.051
Ca
0.869
Sr
—: correlation coefficients between Cd, As, and other elements were not available due to being below detection limit levels for Cd and As.
(b)
2013
Pb
Cd
Cr
Cu
As
Al
K
Na
Ca
Sr
Pb
—
−0.034
0.547
—
0.174
0.395
0.106
0.135
0.366
Cd
—
—
—
—
—
—
—
—
Cr
0.522
—
0.362
0.574
0.504
0.145
0.496
Cu
—
−0.096
0.468
0.179
−0.131
0.379
As
—
—
—
—
—
Al
0.500
0.827
0.934
0.445
K
0.722
0.333
0.946
Na
0.756
0.613
Ca
0.286
Sr
—: correlation coefficients between Cd, As, and other elements were not available due to being below detection limit levels for Cd and As.During the Lantern Festival in Beijing, the concentrations of primary inorganic components such as Ba, K, Sr, Cl−, Pb, and Mg as well as secondary organic components such as oxalate, malonate, succinate, and glutarate were reported to be over five times higher than those in the preevent days [8]. The primary inorganic components and secondary organic components during fireworks were mainly in the fine and coarse modes, respectively [8]. The impact of fireworks on the physical characteristics of aerosol particles such as the number concentration of small accumulation modes (100–500 nm) causing a clear shift of the particles from nucleation and Aitken mode to small accumulation mode at the peak of the fireworks event was also reported [23]. Notably, elevated levels of K, Al, Ti, Mg, Pb, Ba, Sr, Cu, and Sb (up to 3 times) were also observed during Las Fallas in Spain [3]. In addition, during the firework event in Milan (Italy) for the celebration of wining the football World Cup (2006), enhancement of the Sr (120 times), Mg (22 times), Ba (12 times), K (11 times), and Cu (6 times) metal concentrations was reported [24]. Although the sampling time (24 hr: 11 am to 11 am) in the present study was relatively long, the enhancement of some trace metals and elements was within the same orders of magnitude compared to the literature.


## 3.5. Emission of Trace Metals and Elements during the BFF Events

In 2012, 26,447 fireworks were used, while the amount used in 2013 increased by 37% (36,176) compared to 2012 (Supplementary Table1). Aerial shell type fireworks made up 29% (8,245)–31% (10,316) of the total fireworks, with diameters of 3–25 inches and the dominant size of 5-6 inches. The charge quantities of aerial shells are linearly dependent on their diameters (0.03–3 kg shot−1). Fireworks such as igniter, mine, comet, row, and Niagara Fall (2,060–10,000) were also used significantly during the events. In order to assess the uncertainties of emission estimates of trace metals after firework burning, the best emission estimates were calculated using average values of the emission factors obtained from Croteau et al. 2010, while the maximum and minimum emission estimates were obtained using the lowest and highest emission factors among the four types of fireworks, respectively.The largest metal emission during the events was K (128–164 kg), followed by Pb, Cd, Cu, Mg, Ba, As, Al, Ga, Co, and Na (Table4). Emissions of other trace metals and elements were less than 1 kg. The total emissions of trace metals and elements during the 2013 event were a factor of 1.28 higher than those during the 2012 event. Interestingly, enhancement of the Pb concentration by a factor of 2.91 during the 2012 event was supported by the current emission strength of Pb. Meanwhile, the annual anthropogenic emissions of Zn, Pb, Ni, Co, Sb, Na, Cd, and K in Korea during the year 2011 were reported to be 89, 19, 13, 8, 6, 1.9, 0.2, and 0.01 tons, respectively (http://ncis.nier.go.kr/prtr/index.do). In general, firework burning might be an insignificant contributor to the national atmospheric emissions. However, firework burning might be a predominant emission source of airborne K.Table 4
Estimated emissions of trace metals from the BFF during the study periods (in kg).
Elements
2012
2013
Max.
Min.
Best
Max.
Min.
Best
TSP
502.762
240.608
393.578
644.490
308.435
504.946
K
161.602
82.597
127.829
207.158
105.881
164.064
Mg
24.420
4.669
12.052
31.304
5.985
15.424
Ba
22.624
0.108
8.284
29.002
0.138
10.707
Na
4.309
0.205
1.098
5.524
0.262
1.403
Ca
2.478
0.079
0.323
3.176
0.101
0.413
Cu
28.370
0.162
15.754
36.368
0.207
20.157
Al
6.823
2.729
4.471
8.747
3.499
5.727
Pb
96.961
0.007
36.903
124.295
0.009
47.664
Ga
5.028
0.017
1.853
6.445
0.022
2.394
Sr
2.550
0.031
0.249
3.268
0.039
0.318
Zn
2.262
0.086
0.723
2.900
0.110
0.936
Fe
2.011
0.151
0.807
2.578
0.193
1.031
Bi
1.939
0.000
0.618
2.486
0.000
0.787
P
0.190
0.040
0.095
0.244
0.051
0.121
Mn
0.140
0.036
0.083
0.180
0.046
0.106
Ti
0.255
0.010
0.060
0.327
0.013
0.077
Cr
0.431
0.006
0.139
0.552
0.008
0.178
Sn
0.072
0.001
0.029
0.092
0.001
0.037
Si
1.257
0.014
0.402
1.611
0.018
0.514
Cr6+
0.043
0.001
0.024
0.055
0.001
0.031
Rb
0.032
0.012
0.021
0.041
0.015
0.027
Sb
0.019
0.000
0.007
0.024
0.000
0.010
V
0.169
0.001
0.021
0.216
0.002
0.026
Te
0.025
0.000
0.010
0.032
0.000
0.013
Co
1.594
2.076
As
4.787
6.232
Cd
23.967
31.204
Total
866.77
331.57
635.78
1111.12
425.04
816.62


## 4. Summary and Conclusions

We analyzed the impact of large-scale firework burning on urban background trace metal and elemental concentrations and estimated their emission rates during the October month of 2011–2013. During the 2011 BFF event, trace metal concentrations were not higher than those of the previous day. In contrast, the concentrations of trace metals and elements during the BFF event days of 2012-2013 were higher than those during the pre-BFF days. The enhancement of local background concentrations of trace metals was as follows: K (1.72 times), Sr (2.64 times), As (2.86 times), Pb (2.91 times), and Al (5.44 times). Dispersion patterns of the trace metals and elements after firework burning might be significantly different due to the meteorological conditions, indicating different impact on their concentration levels according to geographic location. In addition, the impact of firework events on the ambient concentration levels for trace metals was likely to be different depending on their chemical speciation. In general, firework metals during the study period exhibited significant positive correlation, pointing their common source. During the 2012 BFF event, the effect of the fireworks caused moderate increases (at least up to 10μg m−3) of PM10 (as a proxy for trace metal dispersion) concentrations in all areas of Busan. In contrast, the increase of PM10 concentrations (up to 6 μg m−3 increase) during the nighttime of the 2013 BFF event occurred only at the northwest areas influenced directly by the fireworks. In general, the concentrations of the trace metals and elements examined during the day after the event dropped significantly to the levels observed during the pre-BFF day, suggesting lifetimes of one day or so. The impact of firework burning on the PM10 concentration varied depending on the event day and locations. This suggested that the PM10 concentrations at the measurement sites were likely affected by metrological conditions and local anthropogenic sources, such as on-road mobile sources. The burning of fireworks might become a significant contributor to ambient PM10 levels in the future due to a long-term downward trend of PM10.Various types of fireworks such as aerial shell, mine, comet, row, and Niagara Fall (26,447 for 2012 BFF and 36,176 for 2013 BFF) were used during the BFF event days, which have diverse burst heights (up to 500 m) and sizes (up to 400 m). Of the trace metals, the emissions of K (128–164 kg), Pb (37–48), Cd (24–31), Cu (16–20), and Mg (12–15) were significant. In general, firework burning might be an insignificant contributor to the national atmospheric emissions of trace metals, except for K. In future study, the emission factors of trace metals for the burning of a various types of firework, which is the major contributor to the uncertainty in emission estimates, should be examined to reduce the uncertainties. In the future study, the atmospheric dispersion of trace metals during the burning of fireworks will be simulated by a high-resolution dispersion model such as Computational Fluid Dynamics (CFD) model using the emission rates of trace metals estimated in this study.



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*Source: 423275-2015-07-08.xml*