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Polycyclic aromatic hydrocarbons (PAHs) and their alkylated-, nitro- and oxy-derivatives in the atmosphere over the Mediterranean and Middle East seas

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  • knoell Germany GmbH

Abstract and Figures

Polycyclic aromatic hydrocarbons (PAHs), their alkylated (RPAHs), nitrated (NPAHs) and oxygenated (OPAHs) derivatives are air pollutants. Many of these substances are long-lived, can undergo long-range atmospheric transport and adversely affect human health upon exposure. However, the occurrence and fate of these air pollutants has hardly been studied in the marine atmosphere. In this study, we report the atmospheric concentrations over the Mediterranean Sea, the Red Sea, the Arabian Sea, the Gulf of Oman and the Arabian Gulf, determined during the AQABA (Air Quality and Climate Change in the Arabian Basin) project, a comprehensive ship-borne campaign in summer 2017. The average concentrations of ∑27PAHs, ∑19RPAHs, ∑11OPAHs and ∑17NPAHs, in the gas and particulate phase, were 2.85 ± 3.35 ng m−3, 0.83 ± 0.87 ng m−3, 0.24 ± 0.25 ng m−3 and 4.34 ± 7.37 pg m−3, respectively. The Arabian Sea region was the cleanest for all substance classes, with concentrations among the lowest ever reported. Over the Mediterranean Sea, we found the highest average burden of ∑26PAHs and ∑11OPAHs, while the ∑17NPAHs were most abundant over the Arabian Gulf (known also as Persian Gulf). 1,4 Naphthoquinone (1,4-O2NAP) followed by 9-fluorenone and 9,10-anthraquinone were the most abundant studied OPAHs in most samples. The NPAH composition pattern varied significantly across the regions, with 2 nitronaphthalene (2-NNAP) being the most abundant NPAH. According to source apportionment investigations, the main sources of PAH derivatives in the region were ship exhaust emissions, residual oil combustion and continental pollution. All OPAHs and NPAHs except 2-NFLT, which were frequently detected during the campaign, showed elevated concentrations in fresh shipping emissions. In contrast, 2-nitrofluoranthene (2-NFLT) and 2-nitropyrene (2-NPYR) were highly abundant in aged shipping emissions due to secondary formation. Apart from 2-NFLT and 2-NPYR, also benz(a)anthracene-7,12-dione and 1,4-O2NAP had significant photochemical sources. Another finding was that the highest concentrations of PAHs, OPAHs and NPAHs were found in the sub-micrometre fraction of particulate matter (PM1).
Total concentration (logarithmic scale) of ∑ 27 PAHs, in (a) and (b), ∑ 11 OPAHs in (c) and (d) and ∑ 17 NPAHs in (e) and (f) during the first leg in (a), (c), (e) and the second leg in (b), (d), (f). Spatial resolution of data limited to sampling stretches (see Fig. S1). The concentrations of the PAH derivatives in a few samples in the remote sea regions were among the lowest ever reported, while other samples reached concentration levels previously found at suburban sites. The samples from near Sicily and 295 Sardinia in the Mediterranean Sea, near the Suez Canal and over the Gulfs showed a total concentration of 0.1-1.4 ng m -3 and 1.2-47 pg m -3 for the ∑ 11 OPAHs and ∑ 17 NPAHs, respectively. The concentrations of the individual substances are similar to air samples from a rural and an urban site in Chile (Scipioni et al., 2012), a rural site in France (Albinet et al., 2007), a suburban site in the USA (Bamford and Baker, 2003) and a background site in the Czech Republic (Nežiková et al., 2021). NPAHs and OPAHs have rarely been examined in the marine environment. A study by Lammel et al. (2017) investigated the 300 3-4-ring NPAHs in the eastern Mediterranean under the influence of long-range transport from central and eastern Europe in summer 2012. The concentration of the ∑ 11 3-4-ring NPAHs (23.7 pg m -3 ) was one order of magnitude higher than the concentration of the sum of the same NPAHs in the Mediterranean Sea in our study (2.75 pg m -3 ). The concentration of the
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1
Polycyclic aromatic hydrocarbons (PAHs) and their alkylated-,
nitro- and oxy-derivatives in the atmosphere over the Mediterranean
and Middle East seas
Marco Wietzoreck1, Marios Kyprianou², Benjamin A. Musa Bandowe1, Siddika Celik3, John N.
Crowley4, Frank Drewnick3, Philipp Eger4, Nils Friedrich4, Minas Iakovides2, Petr Kukučka5, Jan Kuta5,
5
Barbora Nežiková5, Petra Pokorná6, Petra Přibylová5, Roman Prokeš5,7, Roland Rohloff4, Ivan Tadic4,
Sebastian Tauer4, Jake Wilson1, Hartwig Harder4, Jos Lelieveld2,4, Ulrich Pöschl1, Euripides G.
Stephanou2,8, Gerhard Lammel1,5
1Multiphase Chemistry Department, Max Planck Institute for Chemistry, Mainz, 55128, Germany
2Climate and Atmosphere Research Centre, Cyprus Institute, Nicosia, 2121, Cyprus
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3Particle Chemistry Department, Max Planck Institute for Chemistry, Mainz, 55128, Germany
4Atmospheric Chemistry Department, Max Planck Institute for Chemistry, Mainz, 55128, Germany
5RECETOX, Faculty of Science, Masaryk University, Brno, 625 00, Czech Republic
6Department of Aerosol Chemistry and Physics, Institute of Chemical Process Fundamentals of the CAS, Prague, 165 02,
Czech Republic
15
7The Czech Academy of Sciences, Global Change Research Institute, Brno, 603 00, Czech Republic
8Department of Chemistry, University of Crete, Heraklion, 70013, Greece
Correspondence to: Gerhard Lammel (g.lammel@mpic.de)
Abstract. Polycyclic aromatic hydrocarbons (PAHs), their alkylated (RPAHs), nitrated (NPAHs) and oxygenated (OPAHs)
derivatives are air pollutants. Many of these substances are long-lived, can undergo long-range atmospheric transport and
20
adversely affect human health upon exposure. However, the occurrence and fate of these air pollutants has hardly been
studied in the marine atmosphere. In this study, we report the atmospheric concentrations over the Mediterranean Sea, the
Red Sea, the Arabian Sea, the Gulf of Oman and the Arabian Gulf, determined during the AQABA (Air Quality and Climate
Change in the Arabian Basin) project, a comprehensive ship-borne campaign in summer 2017. The average concentrations of
27PAHs, ∑19RPAHs, 11OPAHs and ∑17NPAHs, in the gas and particulate phase, were 2.85 ± 3.35 ng m-3, 0.83 ± 0.87 ng
25
m-3, 0.24 ± 0.25 ng m-3 and 4.34 ± 7.37 pg m-3, respectively. The Arabian Sea region was the cleanest for all substance
classes, with concentrations among the lowest ever reported. Over the Mediterranean Sea, we found the highest average
burden of ∑26PAHs and ∑11OPAHs, while the ∑17NPAHs were most abundant over the Arabian Gulf (known also as Persian
Gulf). 1,4-Naphthoquinone (1,4-O2NAP) followed by 9-fluorenone and 9,10-anthraquinone were the most abundant studied
OPAHs in most samples. The NPAH composition pattern varied significantly across the regions, with 2-nitronaphthalene (2-
30
NNAP) being the most abundant NPAH. According to source apportionment investigations, the main sources of PAH
derivatives in the region were ship exhaust emissions, residual oil combustion and continental pollution. All OPAHs and
NPAHs except 2-NFLT, which were frequently detected during the campaign, showed elevated concentrations in fresh
shipping emissions. In contrast, 2-nitrofluoranthene (2-NFLT) and 2-nitropyrene (2-NPYR) were highly abundant in aged
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shipping emissions due to secondary formation. Apart from 2-NFLT and 2-NPYR, also benz(a)anthracene-7,12-dione and
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1,4-O2NAP had significant photochemical sources. Another finding was that the highest concentrations of PAHs, OPAHs
and NPAHs were found in the sub-micrometre fraction of particulate matter (PM1).
1 Introduction
Air pollution contributes to the global burden of respiratory and cardiovascular diseases (Shiraiwa et al., 2017; Lelieveld et
al., 2019). The Red Sea and especially the Arabian Gulf region are prone to major risks by air particulate matter (PM) and
40
gas phase pollutants due to the hot and arid climate leading to high dust concentrations and photochemical activity (Lelieveld
et al., 2009). In combination with high anthropogenic emissions from highly populated cities, intense marine traffic due to
major trade routes (Johansson et al., 2017) and a strong petrochemical industry, air pollution can be significant in these
regions (Lelieveld et al., 2015).
One major class of air pollutants are polycyclic aromatic hydrocarbons (PAHs) and their alkylated (RPAHs), nitrated
45
(NPAHs) and oxygenated (OPAHs) derivatives. Several of these substances are classified as carcinogenic or possibly
carcinogenic (IARC, 1983, 1989, 2018; OEHHA, 2021). Moreover, many polycyclic aromatic compounds (PACs) show
strong mutagenic (Durant et al., 1996; Clergé et al., 2019) and ecotoxic effects (el Alawi et al., 2002; Sverdrup et al., 2002a,
b). Quinones, a major subgroup of OPAHs, have received more attention in recent years due to their potential to contribute
to oxidative stress on cell level (Bolton et al., 2000; Walgraeve et al., 2010; Xiong et al., 2017; Lyu et al., 2018). Although
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some PAH derivatives show even higher toxicity than their parent PAHs (Durant et al., 1996; Collins et al., 1998; Turcotte et
al., 2011; IARC, 2018; Lee et al., 2017; Clergé et al., 2019), their atmospheric concentrations, their cycling and fate are not
well studied. Alkylated 3-ring-PAHs are more persistent, bioaccumulative, and toxic than the parent 3-ring-PAHs, which
have been identified within Europe (ECHA, 2021) as substances with persistent, bioaccumulative, and/or toxic properties
(PBT). According to Wassenaar and Verbruggen (2021) alkylated 3-ring-PAHs could also be considered as PBT.
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PAHs, OPAHs, NPAHs and RPAHs are formed by incomplete combustion of fossil fuels, biomass and waste (Baek et al.,
1991; Lee et al., 2003; Walgraeve et al., 2010; Bandowe and Meusel, 2017). Apart from these pyrogenic sources, PAHs,
especially low-molecular-weight PAHs and RPAHs, and some PAH derivatives can originate from petrogenic sources and
spills of petroleum hydrocarbons (Andersson and Achten, 2015; Zhao et al., 2015; Abbas et al., 2018). In addition to these
so-called primary emissions, NPAHs and OPAHs can also be formed by secondary formation by reactions of PAHs with
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atmospheric oxidants (Finlayson-Pitts and Pitts, 1999; Keyte et al., 2013). For most PAH derivatives, the contribution from
secondary formation is not known. It was shown that 2-nitrofluoranthene (2-NFLT) is formed in gas phase reactions and was
not found in direct emissions, while the opposite was reported for 1-nitropyrene (1-NPYR) (Arey et al., 1986; Bamford and
Baker, 2003). Therefore, the ratio 2-NFLT/1-NPYR can be used as an indicator for the relative contributions of secondary
formation reactions in the gas phase compared to primary emitted compounds (Bamford and Baker, 2003).
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The concentration of PAHs in ambient air as well as other environmental compartments has been studied quite extensively in
the last decades (Baek et al., 1991; Srogi, 2007; Ravindra et al., 2008), especially for the 16 USEPA-prioritized PAHs
(Keith, 2015). However, our knowledge about the distribution of PAH derivatives is still limited (Andersson and Achten,
2015; Lammel, 2015; Bandowe and Meusel, 2017; Iakovides et al., 2021). There are several studies reporting atmospheric
concentrations of OPAHs and NPAHs in the particulate and the gas phase at urban and semi-urban sites (Bamford and
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Baker, 2003; Garcia et al., 2014; Li et al., 2015; Tomaz et al., 2016; Alves et al., 2017; Kitanovski et al., 2020).
Rural/continental background and remote continental sites were investigated in a small number of studies, indicating that
several NPAHs and OPAHs are ubiquitous (Ciccioli et al., 1996; Tsapakis and Stephanou, 2007; Brorström-Lundén et al.,
2010; Scipioni et al., 2012; Tang et al., 2014; Nežiková et al., 2021). Their detection in the Antarctic (Vincenti et al., 2001;
Minero et al., 2010) confirms the long-range transport potential (Keyte et al., 2013). This is supported by global modelling
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studies of NPAHs (Wilson et al., 2020; Kelly et al., 2021). However, fewer studies have determined the pollutant
concentrations in the marine environment, in polluted sea regions or in marine background air. Tsapakis and Stephanou
(2007) and Lammel et al. (2017) measured NPAHs and OPAHs at an eastern Mediterranean marine background location,
while Zhang et al. (2018) sampled air on Tuoji Island in the Yellow Sea. To the best of our knowledge, there is no study
measuring NPAHs and OPAHs over the open ocean. The knowledge about the sources of pollution and the atmospheric fate
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processes such as gas-particle partitioning, photochemical degradation and deposition in the marine environment is crucial
for understanding the distribution and fate of these pollutants, although very little is known (Keyte et al., 2013). In addition,
these processes in marine air are crucial for modelling the distribution of these substances and the concentrations are needed
for the validation of modelling results (Wilson et al., 2020).
The objective of this study was to determine the concentrations in the gas and particulate phase of the PAHs, RPAHs,
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NPAHs and OPAHs in the Mediterranean Sea and around the Arabian Peninsula including the Red Sea, Arabian Sea and the
Arabian Gulf region. We aimed to study the gas-particle partitioning and the mass size distributions of PACs in the
atmosphere of a hot marine environment. Furthermore, we provide information about the sources of air pollution in these
regions.
2 Methods
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2.1 The AQABA ship campaign
The Air Quality and Climate in the Arabian Basin (AQABA) campaign took place in summer 2017 from the 25 June until
the 01 September 2017, sailing on a research vessel (Kommandor Iona) from Toulon, France, to Kuwait City, Kuwait, and
back, with a 2-day stop in Jeddah, Saudi Arabia (first leg) and a 5-day stop in Kuwait. The sampling was performed only
during cruise and outside the 12 nautical miles zones of the countries in the Mediterranean Sea (MS), Suez Canal, Red Sea
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(RS), Arabian Sea (AS, in the northern Indian Ocean), Gulf of Oman (OG) and the Arabian Gulf (AG, also known as the
Persian Gulf). For the evaluation, the Red Sea is split into northern Red Sea (NRS) and southern Red Sea (SRS). The Suez
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Canal is included into the northern Red Sea region; the Gulf of Aden is part of the Arabian Sea. The sampling regions and
sampling cruises are shown in Fig. S1 in the Supplement.
2.2 Sampling
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2.2.1 Air sampling for analysis of PAHs, OPAHs and NPAHs
The air pollutants were sampled separately in gas and particulate phases in polyurethane foams (PUFs, Molintan a.s.,
Břeclav, Czech Republic) and on quartz microfibre filters (QFFs, QMA type, Whatman, Sheffield, United Kingdom),
respectively, by active air sampling on the observation deck (in the front part of the vessel, around 7.7 m a.s.l. and 55 m
away from the stack). The aerosol was sampled as PM10 (all particles with an aerodynamic equivalent diameter of <10 µm)
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by a Digitel sampler (DH77, Hegnau, Switzerland). Additionally, PM was collected size-segregated with 6 size fractions (5
stages + backup filter) within PM10 (PM<0.49µm (backup filter), PM0.49-0.95µm, PM0.95-1.5µm, PM1.5-3µm, PM3-7µm and PM7-10µm)
using a high-volume sampler (Baghirra HV 100-P, Prague, Czech Republic) equipped with a cascade impactor inlet (TE-
235, Tisch Environmental, Inc., Cleves, USA). All filters were pre-baked at 300 °C for 12 h and the PUFs were pre-cleaned
(8 h Soxhlet extraction in acetone and 8 h in dichloromethane (DCM)) before wrapping them into two layers of aluminium
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foil, placing into zip-lock polyethylene bags and keeping them frozen at -20 °C prior to deployment. After exposure, the
samples were wrapped in aluminium foil and kept in polyethylene zip-lock bags at -20 °C during storage. During the whole
cruise, 62 air samples (gas and particulate phase) and 30 size-resolved PM samples were collected together with 6 field
blanks. Detailed sampling information is provided in Supplement Fig. S1 and in Table S1.
2.2.1 Air sampling for analysis of PAHs and RPAHs
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45 air (gas and particulate phase) samples for the determination of PAHs and alkylated PAHs were collected on the monkey
deck of the research vessel (around 4 m higher and 5 m less far away from the stack compared to the samplers for PAHs,
OPAHs and NPAHs) during the campaign, using a high-volume air sampler (GMWL-2000H; General Metal Works, Cleves,
USA). In contrast to the Digitel high volume sampler, total suspended particles (TSP) instead of PM10 were collected. The
sampling duration varied from 6 to 24 h and the total volume of each air sample ranged from 318 to 1428 m3 (Table S1 in the
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Supplement). Pre-combusted QFFs (3 h at 420 °C) and pre-extracted PUF plugs (8.0 x 7.5 cm, Ziemer, Langerwehe,
Germany) were used for the collection of particulate and gaseous phases, respectively. TSP mass was gravimetrically
determined. Filters were pre- and post-sampling weighed on a microbalance (KERN GmbH, Balingen, Germany; 1.0-5 g
readability) at constant temperature (21±2 °C) and relative humidity (45±10%) conditions.
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2.3 Sample preparation and analysis
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2.3.1 PAHs, OPAHs and NPAHs
PUFs and QFFs were extracted using automated Soxhlet extraction (40 minutes Soxhlet extraction followed by 20 minutes
of solvent rinsing) with DCM in a B-811 extraction unit (Büchi, Flawil, Switzerland). Prior to extraction, the samples were
spiked with deuterated nitro-PAHs (1-nitronaphthalene-d7, 2-nitrofluorene-d9, 9-nitroanthracene-d9, 3-nitrofluoranthene-d9,
1-nitropyrene-d9, 6-nitrochrysene-d11, 6-nitrobenzo[a]pyrene-d11) and deuterated PAHs (d8-naphthalene, d10-
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phenanthrene, d12-perylene) as surrogate standards.
The extract was cleaned up using a silica column (5 g of silica, 0.0630.200 mm, activated at 150 °C for 12 hours, 10%
deactivated with water) and 1 g Na2SO4. The sample was loaded onto the column and the target substances were eluted by 5
mL n-hexane, followed by 50 mL DCM. The volume of the eluate was then reduced by a stream of nitrogen in a TurboVap
II (Caliper LifeSciences, Mountain View, USA) concentrator unit and transferred into a GC vial, spiked with p-terphenyl and
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PCB 121 (syringe standards), and the final volume in the vial was adjusted to 200 μL.
Polycyclic aromatic compounds (PACs) in the sample extracts were analysed at the Trace Analytical Laboratory of the
research centre RECETOX at the Masaryk University in Brno, Czech Republic, similar to the method described by Nežiková
et al. (2021). The target compounds in this analysis were 26 PAHs, 1S-heterocycle, 1 RPAH, 17 NPAHs and 11 OPAHs. All
target PAHs, OPAHs and NPAHs including their acronyms are shown in Table 1. The physico-chemical properties of all
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targeted compounds are shown in Table S2.
The analysis of PAHs was performed by gas chromatography (GC, 7890A, Agilent, Santa Clara, USA) equipped with a 60
m x 0.25 mm x 0.25 µm Rxi-5Sil MS column (Restek, Bellefonte, USA) coupled to a mass spectrometer (MS, 7000B triple
quadrupole, Agilent, Santa Clara, USA). 1 μL of sample was injected splitless at 280 °C with He as carrier gas at a constant
flow rate of 1.5 mL min-1. The GC program was as follows: 80 °C (1 min hold), then heated at a rate of 15 °C min-1 to 180
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°C, followed by 5 °C min-1 to 310 °C (20 min hold). The MS was operated in positive electron ionization (EI+) mode with
selected ion monitoring (SIM). The SIM m/z ratios and the retention times of the targeted PAHs are shown in Table S3a.
NPAHs and OPAHs were analysed by GC atmospheric pressure chemical ionization tandem mass spectrometry (GC-APCI-
MS/MS) on a Waters Xevo TQ-S MS (Waters, Mildford, USA) coupled to a GC (GC 7890, Agilent, Santa Clara, USA). The
MS was operated under dry source conditions in multiple reactions monitoring (MRM) mode. The GC was fitted with a 30
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m x 0.25 mm × 0.25 µm Rxi-5Sil MS column (Restek, Bellefonte, USA). The injection of 1 µL of the sample was splitless at
270 °C. He was used as carrier gas at a constant flow rate of 1.5 mL min-1. The oven temperature program was as follows: 90
°C (1 min hold), then heated at a rate of 40 °C min-1 to 180 °C, followed by 5 °C min-1 to 320 °C (6 min hold). The MRM
m/z ratios and the retention times of the targeted OPAHs and NPAHs are given in Table S3b.
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2.3.2 RPAHs
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For alkylated PAHs, particulate and gas-phase samples were extracted and cleaned-up separately following a procedure
described in detail elsewhere (Iakovides et al., 2021). Each fraction was reduced to approximately 0.3 mL by rotary
evaporation, transferred to 1.1 mL GC vials and further evaporated almost to dryness under a gentle stream of nitrogen at -10
°C to minimize evaporation losses. Prior to GC/MS analysis, a known amount of internal standard mixture (4-20 ng of
anthracene-d10 in iso-octane) was added in each GC vial to assess the analyte recovery in the collected samples. The sample
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extracts were analysed at the Cyprus Institute (Cyprus). The target compounds in this analysis were phenanthrene (PHE) and
18 RPAHs, which are shown in Table 1.
The analysis was carried out on a GC (7890N GC, Agilent, Santa Clara, USA) equipped with a deactivated fused silica guard
column (5 m, Agilent, Santa Clara, USA) followed by a 30 m × 0.25 mm × 0.25 μm fused silica column (DB-5MS, J&W,
Santa Clara, USA). The GC was coupled to a mass selective detector (5977B Inert MSD, Agilent, Santa Clara, USA)
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operating in EI mode. Either 1 or 2 μL of the final extract were injected into the column using a cool-on-column inlet (80 °C
constant temperature) with a column flow rate of 1.0 mL/min. The GC oven program was modified to 80 °C initial
temperature, hold for 1 min, heated at a rate of 21 °C min-1 to 150 °C, 5 °C min-1 to 300 °C and finally hold for 20 min (54
min total run time). The transfer line was kept at 300 °C, while the MS quadrupole and ion source temperature were held at
150 and 230 °C, respectively. Molecular ions used for the identification are shown in Table S3c.
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Table 1: Target compounds and their acronyms.
Compound
Acronym
Compound
Acronym
Polycyclic aromatic
hydrocarbons:
PAHs
1,3-/2,10-/3,9-/3,10- Dimethylphenanthrene
1,3-/2,10-/3,9-
/1,10-M2PHE
Naphthalene
NAP
1,6-/2,9- Dimethylphenanthrene
1,6-/2,9-M2PHE
Acenaphthylene
ACY
1,7-Dimethylphenanthrene
1,7-M2PHE
Acenaphthene
ACE
2,3-Dimethylphenanthrene
2,3-M2PHE
Fluorene
FLN
1,9-/4,9- Dimethylphenanthrene
1,9-/4,9-M2PHE
Phenanthrene
PHE
1,8-Dimethylphenanthrene
1,8-M2PHE
Anthracene
ANT
Retene (1-methyl-7-isopropylphenanthrene)
RET
Fluoranthene
FLT
Oxygenated PAHs:
OPAHs
Pyrene
PYR
1,4-Naphthoquinone
1,4-O2NAP
Benzo(b)fluorene
BBN
Naphthalene-1-aldehyde
1-(CHO)NAP
Benzo(ghi)fluoranthene
BGF
9-Fluorenone
9-OFLN
Cyclopenta(cd)pyrene
CCP
9,10-Anthraquinone
9,10-O2ANT
Benzo(a)anthracene
BAA
1,4-Anthraquinone
1,4-O2ANT
Triphenylene
TPH
9,10-Phenanthrenequinone
9,10-O2PHE
Chrysene
CHR
11H-Benzo(a)fluoren-11-one
11-OBaFLN
Benzo(b)fluoranthene
BBF
11H-Benzo(b)fluoren-11-one
11-OBbFLN
Benzo(j)fluoranthene
BJF
Benzanthrone (7H-benz(de)anthracene-7-one)
BAN
Benzo(k)fluoranthene
BKF
Benz(a)anthracene-7,12-dione
7,12-O2BAA
Benzo(e)pyrene
BEP
5,12-Naphthacenequinone
5,12-O2NAC
Benzo(a)pyrene (benzo(def)chrysene)
BAP
Nitrated PAHs:
NPAHs
Perylene
PER
1-Nitronaphthalene
1-NNAP
Indeno(123-cd)pyrene
INP
2-Nitronaphthalene
2-NNAP
Dibenz(ah)anthracene
DBA
3-Nitroacenaphthene
3-NACE
Dibenz(ac)anthracene
DCA
5-Nitroacenaphthene
5-NACE
Benzo(ghi)perylene
BPE
2-Nitrofluorene
2-NFLN
Anthanthrene
ATT
9-Nitroanthracene
9-NANT
Coronene
COR
9-Nitrophenanthrene
9-NPHE
Benzonaphthothiophene
BNT
3-Nitrophenanthrene
3-NPHE
Alkylated PAHs:
RPAHs
2-Nitrofluoranthene
2-NFLT
1-Methylphenanthrene
1-MPHE
1-Nitropyrene
1-NPYR
2-Methylphenanthrene
2-MPHE
2-Nitropyrene
2-NPYR
3-Methylphenanthrene
3-MPHE
7-Nitrobenzo(a)anthracene
7-NBAA
4-Methylphenanthrene
4-MPHE
6-Nitrochrysene
6-NCHR
3,6-Dimethylphenanthrene
3,6-M2PHE
1,3-Dinitropyrene
1,3-N2PYR
2,6-Dimethylphenanthrene
2,6-M2PHE
1,6-Dinitropyrene
1,6-N2PYR
2,7-Dimethylphenanthrene
2,7-M2PHE
1,8-Dinitropyrene
1,8-N2PYR
6-Nitrobenzo(a)pyrene
6-NBAP
2.4 Supporting parameters
Further description of analytical methods and other supporting parameters such as meteorological data, PM10 mass and
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concentrations of transition metals, elemental carbon (EC) and organic carbon (OC) can be found in the Supplement. The
methods and the resulting data of other additional supporting parameters during the AQABA campaign used in this paper are
reported in the following studies: a) The ship exhaust filter, black carbon (BC) and surface PAH concentrations as well as
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bypassing ships, potentially influencing the sampled air, in Celik et al. (2020), b) O3, nitrogen oxides (NOx, i.e. NO+NO2)
and OH radicals in Tadic et al. (2020), c) O3, NO2 and SO2 in Eger et al. (2019) and d) NOx and NOy (i.e. NOx+organic and
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inorganic oxides of nitrogen) in Friedrich et al. (2021). Measurements of OH radicals were done using the HydrOxyl Radical
measurement Unit based in fluorescence Spectroscopy (HORUS) instrument (Martinez et al., 2010; Hens et al., 2014), with
the Inlet Pre-Injector (IPI) modification (Novelli, et al., 2014). The measurement of the actinic flux was done by a spectral
radiometer as described in Meusel et al. (2016). The measurement of polychlorinated biphenyls (PCBs),
hexachlorocyclohexanes (HCHs), dichlorodiphenyl-trichloroethane and isomers (DDX), other organochlorine pesticides
185
(drins) was done similar to Lammel et al. (2016).
2.5 Aerosol source apportionment
Positive Matrix Factorization (EPA PMF 5.0) was applied to the PM10 chemical composition using the concentrations of OC,
EC, BC and metals in both PMF groups and the sum of PCBs, HCHs, DDX, drins, PAHs, NPAHs and OPAHs only in group
1 and selected individual PAHs, OPAHs and NPAHs in group 2 to obtain source profiles and their contributions. All Digitel
190
high-volume samples were considered in the PMF runs including those with contamination from the ship’s stack. The data
matrix was prepared in compliance with the procedure described by Polissar et al. (1998). The final matrices had 62 samples
with 26 and 30 species in group 1 and 2, respectively.
To estimate the optimal number of sources, the PMF model was run several times with different model settings and 3 to 7
factors tested. The Q values (Qtrue, Qrobust and Qexpected/theoretical), the resulting source profiles, and the scaled residuals were
195
examined. The optimum number of factors was chosen based on an adequate fit of the model to the data, as shown by the
scaled residual histograms and physically interpretable results. The most stable solutions were found for 5 factors by extra
modelling uncertainties of 26 % and 19 % for group 1 and group 2, respectively. All runs converged, the scale residuals were
normally distributed and no swaps were observed with the displacement error analysis, indicating that there was limited
rotational ambiguity (Table S9).
200
2.6 Air mass origin
Residence time distributions of air mass histories, 10 days backward in time, were studied using the FLEXPART Lagrangian
particle dispersion model, with ECMWF meteorological data (0.5°×0.5°, 3-hourly; Seibert and Frank, 2004; Stohl et al.,
2005). The output is a measure of the time the computational particles (fictive air parcels) resided in grid cells. Per 24 h
sampling time, 100000 particles were released at a height of 100 m a.s.l..
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2.7 Quality control
More information about the analytical quality assurance such as the filtering of the samples against contamination by the
own ship exhaust, the quality control of the analysis of the PAH derivatives (recoveries, blank correction, detection
frequencies, limits of quantifications (LOQs)) and a summary of PMF diagnostics is given in the Supplement (Chapter S1.5).
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3 Results and discussion
210
3.1 Occurrence of PAHs and PAH derivatives
The average total (sum of gaseous and particulate phase) concentrations of the pollutants in the different sea regions are
shown in Fig. 1. The average total concentrations (range in brackets) of the sum of one pollutant class from all high-volume
air samples of the ∑16PAHs, ∑27PAHs (including the S-heterocycle BNT), ∑19RPAHs (range without RET), 11OPAHs and
17NPAHs were 2.92 ± 3.34 (0.14-17.28) ng m-3, 2.99 ± 3.35 (0.15-17.34) ng m-3, 0.85 ± 0.87 (0.19-3.41) ng m-3, 0.24 ±
215
0.25 (0.04-1.42) ng m-3 and 4.34 ± 7.37 (0.69-46.50) pg m-3, respectively. All the data is filtered for contamination with the
stack of our research vessel (details given in S1.5.1 in the Supplement). The detection frequencies of the compounds in the
high-volume samples are shown in Fig. S1. All targeted PAHs, RPAHs and OPAHs were detected at least in one sample.
From the 17 targeted NPAHs, 7 were detected in at least one high-volume sample. All total concentrations of the individual
compounds and individual samples can be found in the Supplement, Tables S10-S14. Individual phases’ concentrations are
220
presented and discussed in a separate communication.
The spatial distribution of the concentrations of the different substance classes in both legs is shown in Fig. 2. The plot only
shows the average concentration of each sampling stretch, which could also be impacted by individual local plumes at
distinct times and locations. As visible in Figs. 1 and 2, the cleanest region, with the lowest concentration of all substance
classes, was the Arabian Sea in the Indian Ocean. The average air concentrations (in brackets upper and lower estimate when
225
using LOQ instead of LOQ/2 and 0 instead of LOQ/2, respectively) over the Arabian Sea were 0.59 (0.57-0.61) ng m-3, 0.59
(no significant difference) ng m-3, 47.8 (24.1-71.4) pg m-3 and 0.89 (0.29-1.49) pg m-3 for the 27PAHs, ∑19RPAHs,
11OPAHs and 17NPAHs, respectively. These concentrations are among the lowest ever reported levels of the PAHs and
PAH derivatives. The air masses originated from the Indian Ocean and from parts of Somalia with no significant sources of
PAHs or PAH derivatives (Fig. S3d). Similarly, findings from the same campaign for other air pollutants showed the lowest
230
concentration over the Arabian Sea (Bourtsoukidis et al., 2019; Eger et al., 2019; Pfannerstill et al., 2019; Tadic et al., 2020;
Wang et al., 2020). As shown in Fig. 2 a), c) and e), several samples in the Arabian Sea are missing in the first leg due to
rejection as possibly contaminated by the stack of our research vessel Kommandor Iona (detailed overview of rejected
samples and method description in Table S4 and Chapter S1.5.1, respectively). The Mediterranean Sea showed the highest
average concentration of the 27PAHs and ∑11OPAHs, i.e. 4.40 ng m-3 and 0.37 ng m-3, respectively. As illustrated in Fig. 2,
235
the pollutant concentration over the Mediterranean Sea during the first leg differed from that of the second leg. The
concentration of the 27PAHs during the first leg (2.20 ng m-3) was significantly lower (p<0.05, Student’s t-test) than during
the second leg (5.18 ng m-3). The difference was also significant (p<0.05, Student’s t-test) for the 11OPAHs. The air mass
histories (Fig. S2 and S3a) reveal that the difference is related to the different origin of the air masses. During the first leg,
the sampled air predominantly originated from northern Africa and the western Mediterranean Sea, while during the second
240
leg, the prevailing air masses came from north, transporting polluted air from large parts of Europe, including coastal areas
and islands as also reported by Tadic et al. (2020). The northerly wind is a typical large-scale circulation pattern in summer
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over the Mediterranean Sea (Lelieveld et al., 2002). The highest concentrations of the PAH derivatives throughout the entire
cruise were found in sample D58 in the Mediterranean Sea close to Sicily. The concentrations of ∑11OPAHs and ∑17NPAHs
were 1.42 ng m-3 and 46.5 pg m-3, respectively. Sample D54, sampled 400 km south-east of Sicily, showed the highest
245
concentration of the ∑27PAHs, especially of the low-molecular-weight PAHs (2-3-ring PAHs). These samples will be
evaluated in more detail in Sect. 3.3.4.
The concentration of the ∑17NPAHs was similar during both legs in the Mediterranean Sea. On the one hand, 2-NFLT and 2-
NPYR were more abundant during the first leg, possibly due to higher secondary formation in aged air (Atkinson and Arey,
1994; Arey et al., 1986) On the other hand, the primarily emitted 1-NPYR (Atkinson and Arey, 1994) as well as 2-NNAP
250
(having primary and secondary sources, Zhuo et al., 2017; Atkinson and Arey, 1994) had a higher concentration during the
second leg. In contrast to the PAHs and OPAHs, the concentration of the ∑19RPAHs in the air over the Mediterranean Sea
was higher (not significant, p=0.14, Student’s t-test) and not lower during the first leg compared to the second leg. The
different result for the RPAHs can firstly be explained by the different sampling intervals of the air sampler for the RPAHs
(see Table S1). The RPAHs were not collected at the end of the campaign close to Sicily and Sardinia, where a high burden
255
of PACs was measured. Second, north of Egypt in the Mediterranean Sea, close to the Suez Canal during the first leg, high
concentrations of the MPHEs and M2PHEs were found, possibly due to intense marine traffic concentrating or even
queueing before entering into the Suez Canal.
The average concentration of the 17NPAHs over the Mediterranean Sea was 5.23 pg m-3, which was slightly higher than the
average concentration over the northern Red Sea (4.52 pg m-3) and the Gulf of Oman (4.37 pg m-3) but slightly lower than
260
the average concentration over the Arabian Gulf (6.65 pg m-3). The concentration of the ∑19RPAHs over the Mediterranean
Sea (0.81 ng m-3) was similar to the Gulf of Oman (0.83 ng m-3) and lower than over the Arabian Gulf (1.12 ng m-3), too.
Similar to the NPAHs and RPAHs, most other air pollutants (e.g. non-methane hydrocarbons, carbonyl compounds, NOx,
NOz, O3, SO2) measured during the AQABA campaign showed the highest concentration in the Arabian Gulf (Bourtsoukidis
et al., 2019; Eger et al., 2019; Pfannerstill et al., 2019; Tadic et al., 2020; Wang et al., 2020; Friedrich et al., 2021).
265
The concentration of the 17NPAHs over the southern Red Sea was 1.68 pg m-3. Similar as for the ∑17NPAHs, the southern
Red Sea was the region with the second lowest concentrations of the ∑27PAHs and the 11OPAHs (0.94 ng m-3 and 88.3 pg
m-3, respectively). The pollutant burden was low since the air was predominantly coming from eastern Africa, mainly from
Sudan, Eritrea and western and southern parts of Egypt (Fig. S3c), areas with low population and industrial emitter densities.
Air over the northern Red Sea, including the Suez Canal, is more polluted owing to the dense shipping traffic in the canal
270
(Bourtsoukidis et al., 2019), the vicinity of the megacity Cairo and the densely populated and urbanised Nile Delta. The total
concentration of the 19RPAHs over the northern Red Sea was 0.93 ng m-3. The highest concentration was measured in air
close to Jeddah, which was almost one order of magnitude higher polluted than the other samples.
As shown in Fig. 1, the Gulf of Oman and the Arabian Gulf were similarly polluted as the northern Red Sea. The
concentrations of the 27PAHs and the 11OPAHs were higher (but not significantly according to Student’s t-test) in the
275
Arabian Gulf (2.8 ng m-3 and 181 pg m-3, respectively) compared to the Gulf of Oman (2.0 ng m-3 and 161 pg m-3,
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respectively). The air masses sampled in the Gulf of Oman were mainly transported from Oman, United Arab Emirates, Iran
and the Arabian Sea (Fig S3e). The predominant wind direction in the Arabian Gulf during the first leg was northwest
transporting air from Qatar, Bahrain, Kuwait and Iraq (Fig S3f, 28-30 July 2017), while during the second leg, the wind
changed to northeast, increasing the contribution of air advected from Iran (Fig. S3f, 4-6 August 2017). A significantly
280
higher (p<0.05, Student’s t-test) concentration of the 27PAHs prevailed during advection from northeast (second leg, 3.53
ng m-3) than from northwest (first leg, 1.69 ng m-3).
Figure 1: Total concentration (gas + particulate phase) of PAC groups across sea regions (MS: Mediterranean Sea; NRS: northern
Red Sea; SRS: southern Red Sea; AS: Arabian Sea; OG: Gulf of Oman; AG: Arabian Gulf; Empty square: mean value; Grey
285
triangles: Measurement points (difficult to see within the boxed); Box with additional borders: interquartile range (IQR) bound by
the 75th and 25th percentile and range of 1.5 IQR; Horizontal line: Median).
(a)
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Figure 2: Total concentration (logarithmic scale) of ∑27PAHs, in (a) and (b), 11OPAHs in (c) and (d) and ∑17NPAHs in (e) and (f)
during the first leg in (a), (c), (e) and the second leg in (b), (d), (f). Spatial resolution of data limited to sampling stretches (see Fig.
S1).
The concentrations of the PAH derivatives in a few samples in the remote sea regions were among the lowest ever reported,
while other samples reached concentration levels previously found at suburban sites. The samples from near Sicily and
295
Sardinia in the Mediterranean Sea, near the Suez Canal and over the Gulfs showed a total concentration of 0.1-1.4 ng m-3 and
1.2-47 pg m-3 for the ∑11OPAHs and 17NPAHs, respectively. The concentrations of the individual substances are similar to
air samples from a rural and an urban site in Chile (Scipioni et al., 2012), a rural site in France (Albinet et al., 2007), a
suburban site in the USA (Bamford and Baker, 2003) and a background site in the Czech Republic (Nežiková et al., 2021).
NPAHs and OPAHs have rarely been examined in the marine environment. A study by Lammel et al. (2017) investigated the
300
34-ring NPAHs in the eastern Mediterranean under the influence of long-range transport from central and eastern Europe in
summer 2012. The concentration of the 1134-ring NPAHs (23.7 pg m-3) was one order of magnitude higher than the
concentration of the sum of the same NPAHs in the Mediterranean Sea in our study (2.75 pg m-3). The concentration of the
(d)
(c)
(e)
(f)
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samples with the lowest urban influence, found by Lammel and colleagues, were closer to our observed concentrations. In
contrast to the NPAHs, the concentration of the 64-ring PAHs was in the same order of magnitude. Lammel and colleagues
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found 426 pg m-3 as average of all samples and 284 pg m-3 as average of the samples with the lowest urban influence, while
we determined a concentration of 366 pg m-3 for the sum of the same PAHs. From the same study, Lammel et al. measured
1-NPYR, 2-NFLT and 2-NPYR in marine background air being 0.21, 1.68 and 0.92 pg m-3, whereas respective
concentrations were 0.42, 0.93 and 0.069 pg m-3 in air over the whole transect of the Mediterranean Sea of our campaign.
The lower levels of secondarily formed 2-NFLT and 2-NPYR can be explained by significant long-range transport from NOx
310
poor areas, notably northern Africa during the first leg. One decade earlier, in the eastern Mediterranean Sea in summer
2001, Tsapakis and Stephanou (2007) report approximately one order of magnitude higher values, i.e. 29 and 21 pg m-3 for
2-NFLT and 2-NPYR, respectively. Furthermore, they determined 9,10-O2ANT and 9-OFLN (34.2 and 46.3 pg m-3,
respectively), which was in the same range as our measurements in the Mediterranean Sea with 95.4 and 36.2 pg m-3,
respectively.
315
The concentrations of NPAHs (40, 90 and 60 pg m-3 for 1-NPYR, 2-NFLT and 2-NPYR, respectively) in source regions of
the Mediterranean such as Athens (Marino et al., 2000) were approximately three orders of magnitude higher than those in
our study over the Mediterranean Sea. This urban to marine background gradient is a lot smaller for the OPAHs compared to
the NPAHs. In summer 2013, Alves et al. (2017) found at a suburban site in Athens an air concentration of 9, 28 and 242 pg
m-3 for 9,10-O2ANT, 9-OFLN and BAN, respectively. This is one order of magnitude lower for 9,10-O2ANT, the same
320
magnitude for 9-OFLN and one order of magnitude higher for BAN compared to our results in the Mediterranean Sea. This
suggests longer lifetimes or higher formation rates of OPAHs than NPAHs.
Harrison et al. (2016) measured PAHs and its derivatives at three sites along the east coast of the Red Sea, in a plume of a
major point source (petrochemical complex). 9,10-O2ANT had a concentration between 3.15 and 4.02 ng m-3, which is two
orders of magnitude higher than in the particulate phase of samples over the northern Red Sea in our study. The
325
concentration of 5,12-O2NAC was between one and two orders of magnitude higher, while the difference was smaller for
7,12-O2BAA. The difference of the individual NPAHs concentrations between the measurements at the coast from Harrison
et al. and our measurements offshore is even more pronounced. The concentrations of 2-NNAP, 2-NFLT, 1-NPYR, 2-NPYR
and 7-NBAA were over three orders of magnitude higher in the plume measured by Harrison and colleagues. In contrast, the
PAH concentration was almost similar (for low-molecular-weight PAHs) or only one order of magnitude higher (for high-
330
molecular-weight PAHs, i.e. 5-7-ring PAHs) onshore. This, again, points to short atmospheric lifetimes of NPAHs. The OH
reaction rate coefficients of PAHs and NPAHs are similar (Table S2, US EPA, 2019), but NPAHs are more prone to
photolysis (Fan et al., 1996; Keyte et al., 2013; Wilson et al., 2020). This is furthermore supported by findings that the
NPAH/PAH ratios in mid-latitudes are higher in winter than in summer, obviously since the photochemical sink of NPAHs
in summer overcompensates the higher formation potential as a source of NPAHs (Nežiková et al., 2021). Nassar et al.
335
(2011) measured PAHs and two NPAHs in the area of Greater Cairo. The concentration of 1-NPYR in the study was around
one order of magnitude higher than that in the air measured on the ship over the Suez Canal. In contrast, the concentration of
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the low-molecular-weight PAHs was in the same range, while the concentrations of high-molecular-weight PAHs offshore
were one or more orders of magnitude lower.
Few studies report MPHE and M2PHE in the coastal marine atmosphere, the open sea, background and urban sites. Tsapakis
340
and Stephanou (2005) analysed atmospheric samples collected offshore over the eastern Mediterranean Sea and at a
background station in north-eastern Crete (Greece) and reported total (gas and particulate phase) concentrations for ∑MPHE
of 13.6 ng m-3 and for ∑M2PHE of 6.5 ng m-3, respectively. Mandalakis et al. (2002) reported gas and particulate phase
concentrations of 6.07 ng m-3 and 3.17 ng m-3 for ∑MPHE and ∑M2PHE, respectively, in the Saronikos Gulf, which is
impacted by busy marine traffic and the shipyard industry along the coast (Valavanidis et al., 2008). In the same study,
345
corresponding concentrations of 6.95 ng m-3 for ∑MPHE and of 4.17 ng m-3 for ∑M2PHE were reported for the urban
atmosphere of Athens, and respectively 0.52 ng m-3 and 0.34 ng m-3 for the background urban agglomeration. The
concentrations in our study were comparably to the background concentrations, i.e. 0.51 ng m-3 and 0.33 ng m-3 for ∑MPHE
and ∑M2PHE, respectively.
The results of the ∑MPHE in the gas phase (0.47 ng m-3) in our study are also comparable to concentrations over the south-
350
eastern Mediterranean Sea and the Aegean Sea measured by Castro-Jiménez et al. (2012), i.e. 0.58 ng m-3 and 0.61 ng m-3,
respectively, but lower than over the western Mediterranean Sea, the Ionian Sea and the Black Sea. On an Atlantic Ocean
transect from the Netherlands to South Africa, concentrations of 1-MPHE as low as 0.022 ng m-3 were reported, compared to
0.45 ng m-3 for samples taken closer to Europe and western Africa (Jaward et al., 2004). In our study 1-MPHE ranged
between 0.026 and 0.49 ng m-3.
355
3.2 Composition patterns
(a)
(b)
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Figure 3: Relative amount of (a) 16 EPA-PAHs, (b) RPAHs, (c) OPAHs, (d) NPAHs across sea regions (MS: Mediterranean Sea;
360
NRS: northern Red Sea; SRS: southern Red Sea; AS: Arabian Sea; OG: Gulf of Oman; AG: Arabian Gulf). Full names of the
substances are given in Sects. 2.3.1, 2.3.2 and Tables 1 and S2.
3.2.1 PAHs
The substance patterns of PAHs in the six different sea regions are shown in Fig. 3a. PHE was by far the most abundant
PAH in all regions (average contribution of 49 %), followed by FLN, ACE, FLT and PYR with average contributions of 24
365
%, 10 %, 6 % and 5 %, respectively. It can be noted that the PAH composition patterns were similar in all regions. However,
the patterns of the Mediterranean Sea and the southern Red Sea differed from the other regions. The contribution of PHE in
the southern Red Sea was higher than the average, while it was lower than the average in the Mediterranean Sea. The
opposite could be observed for FLN. The different pattern in the Mediterranean Sea was mainly caused by the samples from
the second leg with high influence of aerosols from Europe.
370
3.2.2 RPAHs
The distribution pattern of RPAHs among the campaign regions is presented in Fig. 3b. The RPAHs did not show significant
regional differences in the composition pattern. 2-MPHE, 1-MPHE and 3-MPHE were the most abundant alkylated PAH
species throughout the campaign, making up 22 %, 16 % and 12 % of the total RPAHs measured. Among the M2PHEs, 1,6-
and 2,9-M2PHE were the most abundant compounds.
375
3.2.3 OPAHs
As shown in Fig. 3c, the regional differences between the OPAH composition patterns are more pronounced than the
regional average PAH and RPAH patterns. 1,4-O2NAP, 9,10-O2ANT and 9-OFLN were the most abundant OPAHs, with an
average contribution of 35 %, 22 % and 11 %, respectively. The high share of 9,10-O2ANT and 9-OFLN was also found at
(c)
(d)
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several continental sites (Albinet et al., 2007; 2008; Li et al., 2015; Wei et al., 2015; Drotikova et al., 2020; Lammel et al.,
380
2020; Jariyasopit et al., 2021; Nežiková et al., 2021). In several of these papers, 1,4-O2NAP was not measured. Nežiková et
al. (2021) and Jariyasopit et al. (2021) only found small relative amounts of 1,4-O2NAP at the continental background site
Košetice and in the Athabasca oil sands region in Canada, respectively. In contrast, Wei et al. (2015) and Lammel et al.
(2020) found relatively high contributions to the total amount of OPAHs at urban sites in China and in the Czech Republic,
respectively. Bandowe et al. (2014) observed higher concentrations of 1,4-O2NAP in summer in PM2.5 compared to the cold
385
season, although the partitioning of the compound will be shifted to the gas phase in summer. This would lead to lower
concentrations in summer since the degradation rates of most PACs are expected to be higher in the gas phase (Feilberg et
al., 1999; Keyte et al., 2013). They hypothesized that 1,4-O2NAP is significantly formed by secondary formation, as also
shown by Kautzman et al. (2010) and Keyte et al. (2013). This can be supported by the low winter to summer ratio of 1,4-
O2NAP despite higher emissions in winter at Košetice (Nežiková et al., 2021). High secondary formation in plumes
390
especially in the Mediterranean Sea and the Arabian Gulf (as explained in Sect. 3.3.4), as well as low reaction rates for the
degradation of 1,4-O2NAP compared to all other OPAHs (Table S2, Atkinson et al., 1989) might explain the high relative
contribution of this quinone in our study. Except for the samples from the Gulf of Oman, 1,4-O2NAP always had the highest
contribution of 25-40 %. This quinone is frequently reported having a high ability to produce reactive oxygen species
(Charrier and Anastasio, 2012; Verma et al., 2015).
395
In the Gulf of Oman, the contribution from high-molecular-weight OPAHs (4-ring OPAHs) was higher compared to the
other regions. The composition pattern of the samples from the Arabian Sea differed from the other samples because of a
lower share of 9,10-O2ANT and a higher share of 1-(CHO)NAP. The same was true for the samples of the first leg in the
Mediterranean Sea (see Table S16). 1-(CHO)NAP has been reported prominent among OPAHs from urban and other
polluted sites, but not generally (Albinet et al., 2007; 2008 (partly); Wei et al., 2015; Tomaz et al., 2016; Lammel et al., 2020
400
(in Kladno)).
3.2.4 NPAHs
Similar to the OPAHs, the regional differences in the NPAH composition pattern are more pronounced than the PAH and
RPAH patterns. As illustrated in Fig. 3d, the most abundant NPAHs were 2-NNAP, 3-NPHE, 2-NFLT and 1-NPYR, with an
average contribution of 45 %, 18 %, 15 % and 12 %, respectively. The contribution of 2-NNAP ranged between one third
405
and half in all regions. However, it was not detected above LOQ in the gas phase of samples from the Arabian Sea. Due to
the total detection frequency of >30 %, the values were replaced by LOQ/2 what could lead to an overestimation in this case.
A large fractional contribution of NNAPs, 3-NPHE and 2-NFLT was also found by Lammel et al. (2017) in the eastern
Mediterranean Sea. At the continental site in the study from Lammel et al., as well as in other previous studies at continental
sites, 2-NFLT, 9-NANT and 1-NNAP were the most abundant NPAHs (Bamford and Baker et al., 2003; Albinet et al., 2007;
410
2008; Tomaz et al., 2016; Drotikova et al., 2020; Lammel et al., 2020; Nežiková et al., 2021). In our study, 9-NANT had a
significant contribution only in the northern Red Sea. We found only a few samples with 9-NANT >LOQ (LOQs in Table
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S6c). The reason for the low contribution during the entire campaign might be the relatively high LOQ compared to other
NPAHs (Table S6c) or that 9-NANT is prone to photolysis, which could have been high in this campaign because of high
solar irradiation. The significance of photodegradation of 9-NANT is also supported by lower contributions in summer
415
compared to the cold season, as found by Tomaz et al. (2016) and Nežiková et al. (2021). However, it can also be caused by
seasonal variation in the emission sources or a higher degradation rate in the gas phase based on the significantly lower
particulate fraction in summer (Tomaz et al., 2016; Nežiková et al., 2021). The same might be true for 1-NNAP. In contrast
to our campaign, several other studies found significant amounts of 1-NNAP in air samples at mid-latitude but continental
sites (Bamford and Baker et al., 2003; Albinet et al., 2007; 2008; Tomaz et al., 2016; Drotikova et al., 2020, Lammel et al.,
420
2020; Nežiková et al., 2021). The low contribution of 1-NNAP in air over the Mediterranean and around the Arabian
Peninsula could also be due to the relatively high LOQ in PUFs (Table S6c) or the photodegradation of 1-NNAP, which is
faster than of 2-NNAP, as described by Feilberg et al. (1999). We hypothesize that the comparably low rate constants for the
photodegradation as well as for the reaction with OH (Table S2, US EPA, 2019) are one reason for the high relative
contribution of 2-NNAP. 2-NNAP is frequently detected in continental sites but mostly with lower relative contributions
425
than 1-NNAP, 9-NANT and 2-NFLT (Bamford and Baker et al., 2003; Albinet et al., 2007; 2008; Tomaz et al., 2016;
Drotikova et al., 2020, Lammel et al., 2020; Nežiková et al., 2021). Only at a remote site in Chile, 2-NNAP was also found
to have a very high relative contribution, which was explained by direct emissions or transport assuming a long atmospheric
lifetime (Scipioni et al., 2012). The resistance to photochemical degradation can also be supported by the finding from
Nežiková et al. (2021) that the relative contribution of 2-NNAP is higher in summer than in winter. However, this can also
430
be due to different emission sources or stronger secondary formation in summer (Zhuo et al., 2017).
The fractional contribution of 1-NPYR is high in the Gulf of Oman and the Arabian Gulf. This can be explained by a
significant amount of 1-NPYR in the exhaust of fossil fuel combustion (IARC, 2018; Zhao et al., 2015) and its high
abundance near petrochemical industries (Caumo et al., 2018). It is used as a marker for primary emissions since it does not
have significant secondary sources (Arey et al., 1986). The relatively short estimated lifetime of 1-NPYR in air due to
435
photodegradation (Feilberg and Nielsen, 2000) and the small reaction rate with OH (Table S2, US EPA, 2019) could explain
its low contribution in the Mediterranean Sea, since we sampled relatively aged air samples in that region. The relatively
high contribution of 1-NPYR in the Arabian Sea might be due to bypassing ships (Table S18) as we found 1-NPYR highly
abundant in the ship exhaust (Sect. 3.3.1). The high contribution of 1-NPYR in samples D40-42, in or close to the Gulf of
Aden, is possibly due to pollution from coastal cities in the northeastern province of Somalia. The continental influence of
440
these samples is also shown in the results of the PMF analysis (Fig. 4b). The large contribution of long-range transported
aerosols in the Mediterranean Sea is also illustrated by the high contribution of 2-NFLT, which is formed in secondary
processes (Arey et al., 1986). The contribution of 2-NFLT is also high in the southern Red Sea and the Arabian Sea, two
regions with minor influence of primary emissions but higher fraction of long-range transported aerosols. 3-NPHE, which
has primary and secondary sources (Atkinson and Arey, 1994; Heeb et al., 2008; Ringuet et al., 2012a), has an almost similar
445
contribution in all regions. This could be explained by various different sources or a long mean atmospheric lifetime.
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3.3 Source apportionment
3.3.1 Sources of PAH derivatives by PMF
As shown in Figs. 4 and S4 as well as described in the Supplement (Chapter S2.4.1), the PMF analysis, revealed five
different source factors, namely fresh and aged shipping emissions, continental emissions, residual oil combustion and desert
450
dust.
The PAHs, NPAHs and OPAHs in the air over the Mediterranean Sea and in the seas around the Arabian Peninsula are
believed to originate primarily from fresh and aged shipping emissions. Fresh shipping emissions, mainly from the ship stack
of our research vessel Kommandor Iona, were predominantly apparent during the first leg due to the prevailing wind
direction. Aged shipping emissions contributed to air pollution mainly in regions with congested marine routes such as the
455
Suez Canal (4 July 2017 and 20-23 August 2017), the Bab al-Mandab Strait near Djibouti (16-17 July 2017) and the Strait of
Hormuz, especially near Fujairah (26-28 July 2017 and 5-6 August 2017). The amount of bypassing ships, potentially
influencing the sampled air, based on the data from Celik et al. (2020), is given in Table S18.
Another important source of PAH derivatives were continental emissions. Based on the distribution of residence times of air
masses during these sampling times, we could conclude that these emissions mainly came from Europe (especially received
460
in the Mediterranean Sea, but also in the Arabian Gulf), countries around the Arabian Gulf (mainly received there) and
Egypt (mainly received in the northern Red Sea). Furthermore, the PACs originated from residual oil combustion. High
factor contributions (Figs. 4b and S4b) in the period between 24 July and 6 August 2017 were linked to the samples collected
in the Gulf of Oman and the Arabian Gulf and influenced by the emissions in the coastal areas and offshore (Fig. S3e and f)
as also reported by Bourtsoukidis et al. (2019), Eger et al. (2019), Pfannerstill et al. (2019) and Wang et al. (2020). The
465
source factor identified with minimum contributions of NPAH and OPAHs was desert dust. The finding of PAH derivatives
in the factor desert dust could be explained by mixing of dust with other emissions sources such as continental pollution or
shipping emissions. The concentration of the factor desert dust peaked primarily during a period of Sahara dust outbreaks
(from 13-18 July 2017), while samples were collected over the Red Sea and over the western part of the Gulf of Aden (Fig.
S3c and d, see also Eger et al. (2019)). Dust emitted on the Arabian Peninsula is evident during the sail in the Gulf of Oman
470
and the Arabian Gulf (24 July and 6 August 2017, Fig. S3d and e) but mixed with several other sources.
The contribution of the individual OPAHs and NPAHs can be seen in PMF group 2 in Figs. 4 and 5, showing the relative
contributions of each factor to the concentration of each substance. All PACs targeted in the PMF run (group 2) had a
significant contribution from fresh shipping emissions as their source. Moreover, by comparing several samples with a
significant influence of the exhaust from the own stack (samples D16; 17; 20; 22; 23; 28; 37; 38; see Table S4 and Fig. S4)
475
to the stack filtered regional average concentrations, we could show that almost all detected PAHs, NPAHs and OPAHs were
elevated in the samples with fresh shipping emissions (Table S17). 1-NPYR showed the highest ratio of contaminated to
filtered samples among the NPAHs, while 11-OBaFLN and 1-(CHO)NAP had the highest ratio among the OPAHs. All
targeted OPAHs showed a ratio higher than 1. For the NPAHs, only 2-NFLT was not elevated except for a ratio of 5 in the
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Arabian Sea. 2-NFLT had been reported to be present in diesel particulate matter (Bamford et al., 2003; Zimmermann et al.,
480
2012). However, this was explained by the gas phase formation of 2-NFLT after emission during sample collection.
Surprisingly, the concentration of 2-NPYR was significantly elevated in the fresh shipping emissions. This is unexpected, as
2-NPYR was reported absent in diesel exhaust (Bamford et al., 2003) and believed to be formed through secondary
formation only (Finlayson-Pitts and Pitts, 1999; Wilson et al., 2020). Zhao et al. (2019; 2020) found significant amounts of
2-NPYR in ship exhaust gas depending on the fuel type and the engine loading. They report high emissions of this
485
compound, especially with heavy fuel oil use and mainly under low engine speeds. The abundance of 2-NPYR was
explained by secondary formation due to higher NOx emissions and higher residence times during these conditions. The
results from Zhao et al. (2019; 2020) and from our study suggest a very high formation rate of 2-NPYR. According to Keyte
et al. (2013) and Wilson et al. (2020), the reaction rate constant of PYR with OH is five times higher for 2-NPYR compared
to 2-NFLT but the yield of 2-NPYR is lower.
490
The large contribution of aged shipping emissions to the concentration of 2-NFLT and 2-NPYR (Fig. 5) illustrates the
importance of secondary formation of these two NPAHs. In contrast, 1-NPYR is not abundant in the aged shipping
emissions showing that there is no significant secondary formation. It has been reported that 1-NPYR arises solely from
primary emissions (Bezabeh et al., 2003; Reisen and Arey, 2005). The contribution of aged shipping emissions to the
occurrence of 3-NPHE could either be explained by the higher atmospheric half-life of 79 h compared to 2-NFLT, 1-NPYR
495
and 2-NPYR (Table S2, US EPA, 2019) or by secondary formation as previously suggested (Tomaz et al., 2017). All
detected OPAHs were abundant in the aged shipping emissions. Their abundance points to a long lifetime or formation in the
atmosphere. The relative contributions of 11-OBaFLN, BAN and 7,12-O2BAA were relatively small (Fig. 5). For 5,12-
O2NAC and 1,4-O2NAP, the contribution of aged shipping emissions was higher. It was previously reported that from the
measured OPAHs, 1,4-O2NAP, 1-(CHO)NAP, 9-OFLN, 9,10-O2ANT, 1,4-O2ANT, 9,10-O2PHE, 11-OBaFLN and 7,12-
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O2BAA can be formed from the reaction of parent-PAHs with oxidants (Helmig and Harger, 1994; Perraudin et al., 2007;
Wang et al., 2007; Gao et al., 2009; Ringuet et al., 2012a; Keyte et al., 2013; Dang et al., 2015). Based on the previous
findings from literature and the results of the PM factor aged shipping emissions”, a contribution from secondary formation
to the burden of 1,4-O2NAP and 7,12-O2BAA is likely, in addition to the known secondarily formed substances 2-NPYR and
2-NFLT. Since BAN and 11-OBaFLN have not been found as secondary formation products but highly abundant in primary
505
emissions (Albinet et al., 2007; Ringuet et al., 2012a; Clergé et al., 2019), we hypothesize that their contribution to aged
shipping emissions is only due to their atmospheric lifetime. Since the primary emitted 1-NPYR is not abundant in aged
shipping emissions, it shows that BAN and 11-OBaFLN have a higher atmospheric lifetime than 1-NPYR. Since the
estimated lifetime due to oxidation by OH is higher for 1-NPYR than for the two OPAHs (Table S2, US EPA, 2019),
degradation of 1-NPYR is expected to be governed by photodegradation (Feilberg and Nielsen) as already mentioned in
510
Sect. 3.2.4. Since there is not much data in the literature about 5,12-O2NAC, it’s abundance in aged shipping emissions can
either be due to high atmospheric lifetime or secondary formation.
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1-NPYR and 3-NPHE seem to be good tracers for oil combustion, hence the correlation with emissions from the
petrochemical industry in the Gulf of Oman and the Arabian Gulf. 1-NPYR and 3-NPHE are known to be emitted during
combustion of oil (Streibel et al., 2017). In addition, all OPAHs included into the PMF, except for 1,4-O2NAP, originated
515
directly or secondarily from residual oil combustion.
Except for 11-OBaFLN, all considered PAHs, OPAHs and NPAHs are partly from continental pollution (Fig. 4a). The
abundance of these air pollutants in continental pollution, including 11-OBaFLN, has been shown in many studies (Bamford
and Baker, 2003; Albinet et al., 2007; 2008; Wei et al., 2015; Tomaz et al., 2016; Drotikova et al., 2020; Lammel et al.,
2020; Nežiková et al., 2021). The missing contribution of continental pollution to the concentration of 11-OBaFLN might be
520
because of its comparably low atmospheric half-life due to degradation by OH (Table S2, US EPA, 2019). Continental
pollution was highly abundant in the Mediterranean Sea (Fig. 4b), where we found the highest concentrations of the OH
radical of the entire AQABA campaign. 1,4-O2NAP has a comparably high contribution of approx. 50 % by this factor. As
explained in Sect. 3.2.3, this might be explained by high relative concentrations at the source, high atmospheric lifetime and
secondary formation during the transport of the air to the sampler. In contrast, 1,4-O2NAP seems to be significantly less
525
abundant in pollution from the combustion of residual oil (Fig. 4a) and marine diesel (Table S17). However, more research is
needed to evaluate this aspect in more detail. All PACs are abundant in desert dust, except for BAP and 2-NPYR. The
presence of PAHs and PAH derivatives, especially 1-NPYR and 1,4-O2NAP in the factor desert dust (Fig. 4a) may indicate
co-emissions of dust and PACs in the region (e.g. close to onshore industries).
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Figure 4: PMF group 2: (a) Factor profiles (Bars: Concentration of the species, black squares: Percentage of the species explained,
box: Displacement (DISP) average, whiskers: DISP max and DISP min) and (b) time series of factor contributions to sample
composition.
Figure 5: Relative contribution of the five factors resolved by PMF to the concentration of each substance in PMF group 2.
535
(a)
(b)
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3.3.2 Source attribution by PAHs and alkylated PAHs
The ratio of the particulate concentration of BAP to BAP+BEP is often used as a marker for the ageing of atmospheric
particles since photodegradation of BAP is faster than of BEP (Tobiszewski and Namieśnik, 2012). A concentration ratio
BAP/(BAP+BEP) of less than 0.5 indicates photochemically aged aerosols. The ratio was <0.5 in all regions and 0.5 in the
Arabian Sea (see Fig. S5). The somewhat elevated ratio in the Arabian Sea might be caused by local ship plumes (for
540
number of encounters see Table S18; identification based on Celik et al. (2020)) and other offshore emissions, which
contributed to the mostly long-range transported and aged air pollution in the region. This is also supported by Bourtsoukidis
et al. (2019) studying non-methane hydrocarbons during the AQABA campaign.
The relatively low ratios in all other regions might be explained by the low amount of primary sources of air pollutants on
sea except for ship traffic and some emissions from the offshore oil and gas industry. Thus, the pollution from urban and
545
industrial areas, which are located mostly on the coast, is already slightly aged when reaching the sampler on the ship
depending on the proximity to the emission sources. This could also be the explanation why the second-highest regional
average values were found in the southern and the northern Red Sea receiving the emissions from the nearby coast as well as
from the intense ship traffic in the region. The lowest regional average BAP/(BAP+BEP) values were detected in the Gulf of
Oman and the Arabian Gulf. Air mass histories of sample D33 showed that a significant amount of aerosols came from less
550
populated areas of Iran with a low amount of primary emissions (Fig. S3f, Wang et al., 2020). The results in the
Mediterranean Sea can be divided into the first leg with a lower BAP/(BAP+BEP) ratio due to the prevalent westerly winds
bringing aged air from Africa and from the sea and the second leg with higher ratios due to pollution from close European
coastal areas and islands. The samples D58 and D49-52, close to Sicily and the Greek islands, respectively, showed the
highest BAP/(BAP+BEP) ratios.
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The ratio of ΣMPHE/PHE <1 indicates pyrogenic origin of PAHs for most days in the Red Sea, while a ratio of
ΣMPHE/PHE >1 indicates petrogenic origin, i.e. from unburned fuel (Gogou et al., 1996), which occurred during the period
from the 8-9 July 2017 in the northern Red Sea. Findings by Bourtsoukidis et al. (2020) could tentatively provide an
explanation for the high ratio of ΣMPHE/PHE observed, namely degassing from the Red Sea Deep water.
The ratio of the sum of the four MPHE homologues to PHE (ΣMPHE/PHE) and the ratio 1,7-M2PHE /(1,7-M2PHE + 2,6-
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M2PHE) are given in Table S14. The distribution patterns and the concentration ratio 1,7-M2PHE/(1,7-M2PHE + 2,6-
M2PHE) may be interpreted by considering the emission sources of these compounds. Bläsing et al. (2016) characterised and
compared patterns of alkylated PAHs in gaseous and particulate emissions from road traffic (diesel), domestic heating,
inland navigation vessels (INVs) and ocean-going vessels (OGVs). The ratio of 1,7-M2PHE/(1,7-M2PHE + 2,6-M2PHE) was
used to distinguish the above-mentioned emissions. Thus, the ratio of 1,7-M2PHE/(1,7-M2PHE + 2,6-M2PHE) for INVs
565
(0.370.62) is comparable with that from road traffic and domestic heating. In comparison, 1,7-M2PHE/(1,7-M2PHE + 2,6-
M2PHE) for marine oil combustion (as used for OGVs) was 0.68 (Budzinski et al., 1995). In the present study, the calculated
average ratios were 0.63 (first leg) and 0.66 (second leg) for the Mediterranean, 0.64 and 0.62 for the Red Sea, 0.66 and 0.71
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for the Oman Gulf, 0.73 and 0.67 for the Arabian Gulf, respectively, and 0.61 (second leg) for the Arabian Sea. The
calculated values for 1,7-M2PHE/(1,7-M2PHE + 2,6-M2PHE) in the present study are within the range, 0.60-0.70, proposed
570
by Bläsing et al. (2016) as an indicator for the emissions of OGVs.
3.3.3 Source attribution by NPAHs and OPAHs
Similar to the ratio of BAP/(BAP+BEP), the ratio of 2-NFLT/1-NPYR can indicate the photochemical age of aerosols. A
ratio <5 shows the predominance of combustion sources, while a higher ratio indicates photochemically aged aerosols
(Ciccioli et al., 1996). As illustrated in Fig. 6a, the highest regional average ratio of 2-NFLT/1-NPYR but also with the
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highest absolute and relative standard deviation was found over the Mediterranean Sea, followed by the southern and the
northern Red Sea. However, the ratio was in only two samples (D1 and D58, collected over the Mediterranean Sea) higher
than 5. In contrast, the ratio of BAP to BEP suggests aged aerosols in several samples as explained in Sect. 3.2.2.
The reason for the low incidence of high ratios could be that the concentrations of atmospheric oxidants OH and NO3
radicals as well as NO2 in some sea regions during the campaign were low (Bourtsoukidis et al., 2019; Tadic et al., 2020;
580
Friedrich et al., 2021). The difference might be caused by different oxidants being responsible for degradation of BAP and
formation of 2-NFLT. BAP, which is predominantly in the particulate phase, is mainly degraded by heterogeneous reaction
with ozone (Shiraiwa et al., 2009), while 2-NFLT is mainly formed by homogeneous reaction of FLT with OH or NO3
(Atkinson and Arey, 1994; Reisen and Arey, 2005) and subsequent reaction with NO2. Ozone concentrations varied between
20 ppbv (in the Arabian Sea) and 150 ppbv (in the Arabian Gulf), while the variation of NOx was higher (from 50 pptv in
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Arabian Sea to more than 10 ppbv in the northern Red Sea and the Arabian Gulf) (Tadic et al., 2020; Friedrich et al., 2021).
The highest NOx mixing ratios were found in the Northern Red Sea and the Gulf region, especially close to the Suez Canal,
Kuwait and Fujairah (Tadic et al., 2020; Friedrich et al., 2021). NO2 concentrations are generally significantly smaller in the
marine environment than on land, as shown by satellite data (Roşu et al., 2019) due to the short lifetime (Schaub et al., 2007;
Shah et al., 2020) and missing sources for NOx on sea except for ship traffic and the offshore oil and gas industry. Friedrich
590
et al. (2021) calculated NO2 lifetimes of less than 6h during the AQABA campaign, which means that land-based NOx
emissions will be degraded before reaching the sampler for several samples, especially in parts of the Mediterranean Sea.
Missing primary sources and high degradation due to high OH radical concentrations explain the low NOx mixing ratios over
the Mediterranean Sea (Friedrich et al., 2021). However, NO2 is crucial for the formation of 2-NFLT competing with O2 to
either form NPAHs or OPAHs, respectively (Kamens et al., 1994; Finlayson-Pitts and Pitts, 1999; Atkinson and Arey,
595
2007).
The average 2-NFLT/1-NPYR ratio in air sampled over the Mediterranean Sea was significantly higher (p<0.05, Student’s t-
test) than in the air from Arabian Sea and the Gulf of Oman, respectively. Similarly, the ratio over the northern Red Sea was
significantly higher (p<0.05, Student’s t-test) than over both Gulf regions. In polluted air near the coast (e.g. as found in the
Red Sea and at the beginning and the end of the campaign in the Mediterranean Sea) and in plumes (in samples D1, D30,
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D48 and D58), the 2-NFLT/1-NPYR ratio was high. These samples explain the high average 2-NFLT/1-NPYR ratio in the
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Mediterranean Sea and the northern Red Sea. The ratio can rise during transport of the pollutants. However, the formation of
2-NFLT slows down or stops probably due to low concentrations of the parent-PAH (FLT), the atmospheric oxidants OH
and NO3 or NO2 since formation of 2-NFLT depends on these reactants (Wilson et al., 2020). This was also shown by
Lammel et al. (2017), who found much larger yields of 2-NFLT and 2-NPYR in the marine background with urban influence
605
compared to the marine background without significant pollution sources.
In contrast to the regions with polluted air, a low ratio was observed in air over the Arabian Sea and in the parts of the
Mediterranean Sea far from the coast. Due to these samples with low 2-NFLT/1-NPYR ratios in the Mediterranean Sea, the
standard deviation of the regional average ratio is the highest among all sea regions. The average ratio in the Arabian Sea
was only 0.36 (taking LOQ/2 values of 1-NPYR into account). This points to primary sources (as indicated in Sect. 3.3.2)
610
and/or very low NO2 concentrations in the sampled air masses, as shown by Friedrich et al. (2021). When secondary
formation far away from sources is not significant anymore, the differences in characteristic time for chemical (which is
primarily photolysis) and physical sinks (which is primarily particle deposition) determine the ratio 2-NFLT/1-NPYR. One
influencing factor might be the difference in deposition velocity of the two compounds due to the different particulate
fractions, which is lower for 2-NFLT (not shown, gas-particle partitioning is studied in a separate paper). A lower particulate
615
mass fraction of 2-NFLT might lead to a slower deposition of this compound compared to 1-NPYR, which would lead to
higher ratios. In contrast, a lower ratio would be the result of the faster degradation of 2-NFLT by OH and ozone compared
to the degradation of 1-NPYR (Table S2, USEPA, 2019). In contrast, 1-NPYR is probably more prone to photodegradation,
although the photodegradation rates strongly depend on the aerosol composition (Feilberg and Nielsen, 2000). The removal
and degradation rates are reported to be approximately similar (Kamens et al., 1994; Fan et al., 1996; Feilberg and Nielsen,
620
2000; Albinet et al., 2008). However, this may not be the case in this study due to exceptionally low particulate mass
fractions of the PACs due to the high temperature and the low EC and OC concentrations in the aerosols (Table S15). If
degradation of 2-NFLT plays a larger role in the investigated regions, the ratio of 2-NFLT/1-NPYR would decrease with
time, when there is no formation of 2-NFLT. This might be another explanation for the low 2-NFLT/1-NPYR ratios in some
sea regions. However, more research is needed on the exact kinetics influencing the ratio, especially the photolysis rate
625
coefficients. At continental sites, the ratio of 2-NFLT/1-NPYR mostly increases with distance to the emission source due to
the significant formation of 2-NFLT (Ciccioli et al., 1996; Nežiková et al., 2021).
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Figure 6: Box-Whisker plot of the ratios (a) 2-NFLT/1-NPYR and (b)2-NFLT/2-NPYR across sea regions (MS: Mediterranean
Sea; NRS: northern Red Sea; SRS: southern Red Sea; AS: Arabian Sea; OG: Gulf of Oman; AG: Arabian Gulf; Empty square:
630
mean value; Filled, grey triangles: Measurement points; Box with additional borders: interquartile range (IQR) bound by the 75th
and 25th percentile and range of 1.5 IQR; Horizontal line: Median).
Since 2-NPYR is almost entirely formed by the reaction of PYR with OH radicals during daytime, while 2-NFLT can be
formed by daytime reaction with OH as well as by nighttime reaction with NO3, the ratio of 2-NFLT/2-NPYR can reveal the
predominant formation pathway of NPAHs (Feilberg et al., 2001; Bamford and Baker, 2003). The main formation pathway
635
during the campaign was the OH radical initiated formation, since the average concentration ratio of 2-NFLT/2-NPYR was
15.1 ± 11.6. This is close to a ratio of 5-10, suggesting the predominant formation of NPAHs by OH radicals and far from a
ratio of >100, which would indicate reactions mainly involving the NO3 radical. This result is similar to the findings by Tang
et al. (2014) at a remote site on a Japanese peninsula. Lammel et al. (2017) determined even lower 2-NFLT/2-NPYR ratios
in the eastern Mediterranean Sea, also pointing to a predominant NPAH formation by hydroxyl radicals.
640
As illustrated in Fig. 6b, the lowest average ratio (9.5) was found in the northern Red Sea, while the ratio of 15.8 (first leg:
22.3; second leg: 13.4) in the Mediterranean Sea was the highest regional average value. The high value in the
Mediterranean Sea during the first leg was due to two exceptionally high values in samples D1 and D5. The formation of
these NPAHs will be largely determined by the accumulated nighttime NO2 and the actinic flux during the day, the air mass
had been exposed to prior sampling. For example, samples D52 and D56 had relatively high ratios since the aerosols have
645
picked up NOx emissions from the urban areas of Athens and Istanbul (D52) or Rome and Naples (D56) in a previous night,
which can be converted to the NO3 radical by the reaction with ozone. Whereas the samples D50 and D54, which had not
picked up NOx emissions from particular source areas within 48h, did not show a high 2-NFLT/2-NPYR ratio.
3.3.4 PAHs and derivatives in photochemically aged pollution
A high ratio of the secondarily formed PAH derivatives 2-NPYR and 2-NFLT (Arey et al., 1986; Bamford and Baker, 2003;
650
Reisen and Arey, 2005) to their parent PAHs indicates long-range transported aerosols with a significant concentration of the
(a)
(b)
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atmospheric oxidants OH and NO3 as well as NO2. Similar to the ratio of 2-NFLT/1-NPYR, the highest ratios were observed
in air over the Mediterranean Sea (especially during the first leg in aged aerosols). We determined the highest ratios in
sample D1 at the beginning of the campaign close to Sardinia and Sicily. Another high ratio was found in sample D30 in the
Arabian Gulf. As already revealed by Wang et al. (2020), photochemically aged air reached the ship from the first night of
655
the first leg in the Arabian Gulf (28 July 2017 16:00 UTC) until the 30 July 2017 at 00:00 UTC (see air mass histories in Fig.
7a), as evidenced by high mixing ratios of some carbonyl compounds such as acetone. After that, the air was dominated by
fresh emissions, while approaching Kuwait. According to the distribution of residence times of air masses, the air arrived
from northwest with influence of several oil fields and refineries in that region (Fig. 7b and S3f; Bourtsoukidis et al., 2019;
Pfannerstill et al., 2019; Wang et al., 2020). Thus, the samples from the first leg in the Arabian Gulf were affected by fresh
660
emissions as well as photochemically aged air. Apart from 2-NFLT/FLT and 2-NPYR/PYR, several other PAH derivatives
to parent-PAH concentration ratios (e.g. 1,4-O2NAP/NAP, 9-OFLN/FLN and 9,10-O2ANT/ANT) were also elevated in
sample D30, showing the high contribution of photochemically aged air. In addition, the results indicate that these PAH
derivatives are secondarily formed or significantly slower degraded and deposited than their parent PAH.
Another sample with a high ratio of secondarily formed NPAHs is sample D48 in the northern Red Sea nearby the Suez
665
Canal. Similar to the first night in the Arabian Gulf, Wang et al. (2020) determined a high OH exposure during the first night
in the Gulf of Suez (from the 22-23 August 2017) accompanied by a high mixing ratio of acetone. The finding that aerosols
sampled between the 22 and 23 August 2017 (D48) were atmospherically aged, is supported the high PAH derivative/parent
PAH ratios (e.g. of 2-NFLT/FLT, 2-NPYR/PYR, 7-NBAA/BAA, 1,4-O2NAP/NAP and 9,10-O2ANT/ANT). The enhanced
formation of NPAHs and OPAHs from atmospheric reactions in this area commensurate with high concentrations of NO2,
670
and comparably high production rates of the NO3 radical in this sea region, as reported by Eger et al. (2019). In addition,
sample D48 is also affected by primary emissions, e.g., from oil refineries and shipping emissions (Bourtsoukidis et al.,
2019). This is supported by the PMF, suggesting aged shipping emissions as well as continental pollution as the major
sources.
Generally, low and high NPAH/PAH and OPAH/PAH ratios coincided with NOx and radical availabilities. The highest
675
concentrations of PAHs (D54) as well as of NPAHs and OPAHs (D58) were found in air masses carrying continental
pollution, sampled in the Mediterranean Sea (from south-east Europe, covering major urban areas including Thessaloniki
and Istanbul as well as from Sicily, Corsica, Sardinia and parts of continental Italy, respectively; Figs. 7c and d). While
night-time sample D54 corresponded to low NOx and low OH and NO3 radical concentrations, 24 h sample D58
corresponded to high OH and NOx concentrations (Tadic et al., 2020; Friedrich et al., 2021).
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Figure 7: Distribution of residence times of air masses received in the Arabian Gulf: (a) D30 (29-30 July 2017), (b) D31 (3-4 August
2017) and the Mediterranean Sea: (c) D54-55 (27-28 August 2017), (d) D58 (29-30 August 2017) using FLEXPART Lagrangian
particle dispersion model samples.
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3.3.5 Significance of OPAHs and NPAHs photochemical sources
We found a significant positive correlation of 7,12-O2BAA with the ratio of 2-NFLT/1-NPYR (r=0.83, p<0.05), which is
typically used as an indicator for the contribution of PAH derivatives formed from oxidative reactions. Several laboratory
studies have shown that 7,12-O2BAA is formed from the heterogeneous reaction of BAA with O3 alone and also with the
combination of O3 and NO2 (Gao et al., 2009; Ringuet et al., 2012a, b). The formation of 7,12-O2BAA from the
690
photochemical reaction of BAA has also been reported (Jang and McDow, 1997; Shen et al., 2007). In our current study, the
quinone weakly, not significantly correlated with ozone (r=0.25, p=0.11), the OH concentration (r=0.29, p=0.11) and the
actinic flux (r=0.23, p=0.14). The weak correlation of the ratio of 7,12-O2BAA and the parent-PAH BAA with the actinic
flux (r=0.28, p=0.07) was the strongest correlation among all PAH derivative/PAH ratios. However, the secondary formation
of 7,12-O2BAA is expected to be only a part of the total burden of this quinone. We also found correlations with primary
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(a)
(b)
(c)
(d)
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pollutants, suggesting primary emissions. Similarly, Lin et al. (2015) reported that around 30 % of 7,12-O2BAA in
atmospheric PM sampled in Beijing was secondarily formed.
Lin and colleagues (2015) also found significant secondary formation of 3-NPHE and 7-NBAA. Tomaz et al. (2017) even
suggested 3-NPHE to be used as a marker for secondary formation from PHE. However, 3-NPHE is not or only to trace
amounts formed by homogeneous reactions with OH or NO3 (Atkinson and Arey, 1994; Helmig and Harger, 1994; Lee and
700
Lane, 2010). Though, Ringuet et al. (2012a) reported the formation of 3-NPHE and 7-NBAA by heterogeneous formation
with atmospheric oxidants. Liu et al. (2019) found a correlation between 2-NFLT and 7-NBAA. We observed a significant
correlation of the ratio 2-NFLT/1-NPYR with 3-NPHE (r=0.44, p<0.05) but not with 7-NBAA (r=0.01, p=0.91). 7-NBAA
was positively correlated with the concentration of the NO3 radical and NO2 (r=0.60, p<0.05 and r=0.67, p<0.05,
respectively), but not with the OH radical. 3-NPHE showed a weak correlation with NO2 (r=0.28, p=0.1) and the actinic flux
705
(0.25, p=0.11). Based on the high emission factors of 3-NPHE and 7-NBAA in diesel combustion (Heeb et al., 2008; Zhao et
al., 2019), we expect primary pollution as the major source of these compounds and only a minor contribution from
secondary formation. This is supported by Zhuo et al. (2017), who report a contribution from secondary formation of only 3-
10 % to the total concentration of 3-NPHE in the city Nanjing in eastern China.
The secondary formation of 2-NNAP and 1,4-O2NAP has already been determined earlier (Atkinson and Arey, 1994;
710
Kautzman et al., 2010; Keyte et al., 2013) and was suggested by source attribution (Zhuo et al., 2017). 2-NNAP correlated
with the ratio 2-NFLT/1-NPYR (r=0.46, p<0.01), while 1,4-O2NAP only showed a weak correlation with the ratio (r=0.29,
p=0.06). 2-NNAP correlated with NO2 (r=0.38, p<0.05). 1,4-O2NAP showed a weak positive correlation with O3 (r=0.22,
p=0.14). Both compounds are highly abundant in primary emissions, as already mentioned. Thus, 2-NNAP and 1,4-O2NAP
might have contributions from primary and secondary formation depending on the region.
715
From the literature, it is known that 9-OFLN and 9,10-O2ANT can be formed in the atmosphere, mainly through the reaction
of their parent PAH with O3 and OH (Helmig and Harger, 1994; Perraudin et al., 2007; Wang et al., 2007; Keyte et al.,
2013). In addition, source analysis of polluted air in the Chinese megacity Nanjing showed a significant contribution of
secondarily formed 9-OFLN and 9,10-O2ANT to the total concentration (Zhuo et al., 2017). In our dataset, we could find a
positive correlation of these two OPAHs (significant only for 9-OFLN) with the concentration of O3 (r=0.42, p<0.01 and
720
r=0.27, p=0.08, respectively). Furthermore, 9-OFLN showed a significant positive correlation with the ratio 2-NFLT/1-
NPYR (r=0.33, p<0.05), while 9,10-O2ANT only showed a weak correlation (r=0.22, p=0.15). Based on the results from the
PMF and other literature, we expect primary emissions as the major source of both OPAHs with a small contribution of
secondary formation to the concentration of 9-OFLN and 9,10-O2ANT.
1-(CHO)NAP was already reported to be secondarily formed by ozonolysis from ACY, 1-methylnaphthalene and possibly
725
other precursors within hours (Dang et al., 2015). It is significantly correlating with the ratio of 2-NFLT/1-NPYR (r=0.42,
p<0.05) and shows a very weak, not significant correlation with ozone (r=0.11, p=0.47). 5,12-O2NAC showed a very weak
correlation with ozone (r=0.18, p=0.25). However, we are not aware of any study showing secondary formation of this
quinone. In contrast, 11-OBbFLN can be formed by the reaction of the parent PAH with ozone (Ringuet et al., 2012a).
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However, we did not find any correlation. Thus, there is no clear indication for significant secondary formation of 11-
730
OBaFLN, 11-BbOFLN and BAN, based on the correlation analysis.
In conclusion, our observations indicate photochemical sources to significantly have influenced 2-NFLT, 2-NPYR, 1,4-
O2NAP and 7,12-O2BAA levels, while this was not the case for 1-NPYR, 11-OBaFLN, 11-BbOFLN and BAN. Indications
for secondary formation but possibly only minor were found for 2-NNAP, 3-NPHE, 7-NBAA, 9-OFLN, 1-(CHO)NAP and
9,10-O2ANT.
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3.4 Mass size distributions
The highest concentrations of PAHs, OPAHs and NPAHs are found in the sub-micrometre fraction of particulate matter,
PM1. Fig. 8 shows the campaign average mass size distributions of the PAHs and PAH derivatives. The mass size
distributions of PAHs, NPAHs and OPAHs are mainly unimodal given the coarse size resolution of the impactor with 6 size
ranges within PM10. The maximum was found in particles with an aerodynamic diameter <0.49 μm. For the sum of PAHs,
740
four samples showed an apparently unimodal distribution with a maximum at a particle diameter of 0.490.95 µm in the
accumulation mode instead of the lowest particle size. In addition, three samples (two in the Arabian Gulf and one in the
Arabian Sea) showed a bimodal distribution with maxima in particles with an aerodynamic diameter <0.49 µm and of 0.95
1.5 µm. For the sum of NPAHs, only one sample (in the Mediterranean Sea) showed an apparently unimodal distribution
with a maximum in another aerodynamic particle diameter range than <0.49 μm (0.490.95 µm). Since we did not resolve
745
the <0.49 μm size fraction, more modes in the sub-micrometre fraction, as found by di Filippo et al. (2010) cannot be
excluded.
The ratio between the concentrations in particles <0.49 μm compared to the concentrations in coarse mode PM particles is
greater for high-molecular-weight PACs compared to low-molecular-weight PACs and higher for PAH derivatives compared
to the parent-PAHs. This can be explained by the lower vapour pressure of PAH derivatives and high-molecular-weight
750
PAHs compared to the parent-PAHs and low-molecular-weight PAHs. Compounds with lower vapour pressure are less
subject to redistribution across particles sizes during transport (Degrendele et al., 2014). The process of redistribution is
more effective that the pollutants reach higher particle size fractions than the process of coagulation of particles to form
larger particles, which would transfer low vapour pressure PACs to bigger particle size fractions. The dependency of the
vapour pressure on the mass median diameter was only found for PAHs and was not significant. This can partly be explained
755
by limited explanatory power of the mass median diameter in this study due to low concentrations of e.g. the 3-ring PAHs
and some NPAHs, leading to no detectable amount in coarse mode particles. The NPAHs generally had a low concentration
in our study and the low-molecular-weight PAHs were not abundant in PM since these substances are preferable in the gas
phase. The campaign average mass median diameters of the target compounds are shown in the Supplement Table S19.
Since the process of redistribution depends on time, a shift of the mass median diameter to larger particles sizes is found for
760
aged aerosols (see exemplary Fig. S6). For instance, Lammel et al. (2017) found two maxima for the 4-ring PAHs at a
marine background site (same cascade impactor as the one used in this study). The second maximum was explained by aged
(a)
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aerosols at the marine site. The samples showing a maximum of the sum of PAHs at higher particle diameters in our study
can also be attributed to aged aerosols (aged samples C6 and C7 in Arabian Gulf; C27, C28 in Mediterranean Sea without
close primary emission sources; C22 in very clean air over the Arabian Sea, C24 in southern Red Sea possibly because of
765
Saharan dust).
(b)
(c)
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Figure 8: Campaign average mass size distributions of (a) 27PAHs, (b) 11OPAHs and (c) ∑17NPAHs during the campaign;
770
including standard deviation as error bars.
4 Conclusions
For the first time, PAHs and their derivatives were measured in the marine environment around the entire Arabian Peninsula
in a comprehensive ship campaign. The atmospheric average concentrations of ∑27PAHs, ∑19RPAHs, ∑11OPAHs and
17NPAHs in the gas and particulate phase were 2.85 ± 3.35 ng m-3, 0.83 ± 0.87 ng m-3, 0.24 ± 0.25 ng m-3 and 4.34 ± 7.37
775
pg m-3, respectively. The lowest burden of all targeted pollutant classes was observed in the Arabian Sea with concentrations
among the lowest ever reported, followed by the southern Red Sea. The highest average concentrations of the PAHs and the
OPAHs were detected in the Mediterranean Sea, while the NPAHs were most abundant in the Arabian Gulf. It was observed
that the regional differences in the composition patterns of the NPAHs and OPAHs were more pronounced than those of the
PAHs and RPAHs. 1,4-O2NAP, 9-OFLN and 9,10-O2ANT were the most abundant OPAHs. The NPAH composition pattern
780
was dominated by a high contribution of 2-NNAP, followed by 1-NPYR, which was highly abundant in the Gulf region.
Photochemical formation of 2-NFLT, 2-NPYR, 2-NNAP, 3-NPHE, 7-NBAA, 1,4-O2NAP, 1-(CHO)NAP, 9-OFLN, 9,10-
O2ANT and 7,12-O2BAA was indicated, while for 1-NPYR, 11-OBaFLN, 11-OBbFLN and BAN secondary sources were
not significant.
Source apportionment showed that the PAHs and their nitrated and oxygenated derivatives mainly originated from fresh and
785
aged shipping emissions. All OPAHs and NPAHs except 2-NFLT, which were frequently detected during the campaign,
showed elevated concentrations in fresh shipping emissions. 1-NPYR among the NPAHs and 11-OBaFLN and 1-
(CHO)NAP among the OPAHs showed the highest relative increase in their concentration. In contrast, 2-NFLT and 2-NPYR
were highly abundant in aged shipping emissions due to secondary formation. 1-NPYR, 3-NPHE and several OPAHs had a
significant contribution from residual oil combustion. PAH derivatives were clearly enriched in long-range transported
790
plumes from polluted regions in Egypt, the Arabian Gulf, and southern and eastern Europe. Throughout the campaign, the
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highest concentrations of PAHs, OPAHs and NPAHs were found in the sub-micrometre fraction of particulate matter (PM1).
Due to redistribution, the mass median diameter was shifted to higher values in long-range transported aerosols.
Data availability. The data used in this study are archived and distributed through the KEEPER service of the Max Planck
795
Digital Library (https://keeper.mpdl.mpg.de, last access: 12 December 2021) and have been available from August 2019 to
all scientists agreeing to the AQABA protocol.
Supplement. The supplement related to this article is available online at:
800
Author contributions. MW evaluated the data and wrote the manuscript. GL supervised this study. MI and RP did the
sampling. MK, MI and ES provided the data about alkylated PAHs and wrote this part. PPo performed the PMF and wrote
the part. BN created the FLEXPART Lagrangian particle dispersion model results. JK provided the data about metals. PK
and PPr performed the PAH, NPAH and OPAH sample preparation and analysis. IT created GPS plots and provided NOx
and O3 data. NF, PE and JNC contributed measurements of NO2, NOX, NOy O3 and SO2. RR and ST provided OH radical
805
data. JW was involved in the discussion about the sources. The stack filter and information about bypassing ships as well as
BC and surface PAH concentrations were provided by FD and SC. HH took responsibility for the scientific coordination of
the field campaign on board the research vessel. JL designed the AQABA campaign. GL designed this study, supported by
ES and UP. All authors contributed to data interpretation and manuscript revision and approved the submitted version.
810
Competing interests. The authors declare that they have no conflict of interest.
Acknowledgements. We thank Hays Ships Ltd, Captain Pavel Kirzner and the Kommandor Iona’s ship crew for the great
support. We would like to thank Marcel Dorf and Claus Koeppel for the organization of the campaign, Hartwig Harder for
the management on board, and all other participants and supporters of the campaign. We thank Benedikt Steil for processing
815
meteorological data and Jan Schuladen for the data about the actinic flux. We also thank Abdulaziz al Senafi (Kuwait Inst. of
Scientific Research). In addition, we thank Ondrej Sanka for the assistance in the plotting of sampling stretches. This
research was supported by the Max Planck Society and by the Czech Ministry of Education, Youth and Sports - Research
Infrastructure RECETOX RI (No LM2018121 and CZ.02.1.01/0.0/0.0/16_013/0001761), the project CETOCOEN
EXCELLENCE (No CZ.02.1.01/0.0/0.0/17_043/0009632) and the Czech Science Foundation (GACR #20-07117S). This
820
project was supported from the European Union’s Horizon 2020 research and innovation programme under grant agreement
No 857560. This publication reflects only the author's view and the European Commission is not responsible for any use that
may be made of the information it contains.
Financial support. The article processing charges for this open-access publication were covered by the Max Planck Society.
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Review statement.
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... In terms of PAHs in the atmosphere, their seasonal variability and temporal distribution were widely investigated in Asia (Park et al., 2002;Guo et al., 2003;Chiang et al., 2003;Hong et al., 2007;He et al., 2010;Shi et al., 2010;Lai et al., 2011;Herlekar et al., 2012;Wang et al., 2015Wang et al., , 2016Ambade, 2018;Meshram et al., 2018;Nguyen et al., 2018;Simayi et al., 2018;Liu et al., 2019;Kumar et al., 2020Kumar et al., , 2020aAmbade and Sethi, 2021;Kongpran et al., 2021;Sonwani et al., 2022;Xue et al., 2022;Zhan et al., 2022), North America (Galarneau et al., 2014;Tevlin et al., 2021), South America (Teixeira et al., 2013), and Europe (Yunker et al., 2002;Albinet et al., 2007;Pindado and Perez, 2011;Ringuet et al., 2012;Alves et al., 2015Alves et al., , 2017Kozielska et al., 2015;Tomaz et al., 2016;Lewandowska et al., 2018;Siudek and Frankowski, 2018;Lhotka et al., 2019;Lim et al., 2021;Matos et al., 2021;Sánchez-Piñero et al., 2021;Lara et al., 2022;Naydenova et al., 2022;Wietzoreck et al., 2022). The particulate matter of aerodynamic diameter less than 10 μm (PM 10 ) plays an important role in the atmospheric cycle of PAHs. ...
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In this study, the results of PM10-bound PAH measurements were subjected to positive matrix factorization (PMF) approach and diagnostic ratios to investigate their levels, seasonal variability, impact of primary anthropogenic sources, and human health risk via the inhalation route. Daily ground-based observations were carried out at a representative coastal site in Gdynia (northern Poland), from April to December 2019. The concentrations of Σ13PAHs in PM10 varied between 0.45 ng m⁻³ and 54.02 ng m⁻³, with a mean of 5.22 ± 8.67 ng m⁻³. A clear seasonality and distribution profiles of PM10-bound PAHs were observed as a result of local/remote sources and meteorological conditions. The highest Σ13PAH concentration was found in December (18.56 ± 16.45 ng m⁻³) and the lowest values were observed between June and September (3.89 ± 0.52 ng m⁻³). The PMF-based analysis revealed five factors, suggesting the importance of primary anthropogenic sources of PAHs, i.e. coal combustion, biomass burning, gasoline/diesel vehicles, industrial and shipping activities as well as natural gas combustion. In summer, PAH levels were mostly controlled by local shipping emissions as well as traffic-related and non-combustion sources such as photochemical decomposition. The winter PAH maxima were attributed to a strong increase in residential coal combustion. A Spearman's rank correlation and multilinear regression analysis showed that ambient temperature and NO× had a significant impact on intra-annual variability in PM10-bound PAH transformation in this region. PAH congeners in coarse-size fraction were positively correlated with SO2, indicating their shared anthropogenic sources. The annual mean of epidemiologically based ILCR value was 6.6 × 10⁻⁵. This work indicates a potential carcinogenic risk for the local population and a significant difference in BaPeq levels between the individual seasons in this region.
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Thirty-four air samples were collected from 2013 to 2015, at a semi-rural site in Eastern Mediterranean (Island of Crete), to study the atmospheric occurrence of polycyclic aromatic hydrocarbons (PAHs), polychlorinated biphenyls (PCBs) and organochlorine pesticides (OCPs) in the gas and particulate phase. Average levels (gaseous and particulate phase) of PAHs (36 compounds, 11–18 ng/m³), PCBs (49 congeners, 77–93 pg/m³) and OCPs (23 substances, 77–140 pg/m³) were comparable to those reported for similar locations worldwide. Multiple-linear regression analysis, performed to relate atmospheric concentrations with meteorological conditions, revealed as main controlling factors local sources for PAHs and long-range transport (LRT) for PCBs and OCPs. The consideration of parent-metabolite ratios for most OCPs excluded fresh inputs. The application of the potential source contribution function (PSCF) identified Black Sea and eastern Balkans as likely sources for PCBs and OCPs. Significant linear correlations (R² = 0.79–0.98) were determined between the partitioning coefficients (logKp) and partial vapor pressures (logPL0) for most air samples for PAHs and PCBs excepting OCPs. Slope mr values were close to −1 for PAHs and OCPs indicating gas/particle partitioning close to equilibrium. The corresponding mr values for PCBs were shallower (<-0.60) denoting non-equilibrium conditions and potential sampling artefacts. The octanol-air partition coefficient absorption model, logKp-logKoa, did not offer robust evidence for the evaluation of the atmospheric partitioning of the studied compounds. Experimentally determined particle fractions (ϕ) fitted better with the typical remote and rural curves as predicted by the Junge-Pankow model for most PAHs and PCBs but not for OCPs. The Koa-fom absorptive model could not adequately simulate the measured ϕ values for the majority of the compounds.
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Nitrated and oxygenated polycyclic aromatic hydrocarbons (NPAHs, OPAHs) are abundant in the atmosphere and contribute significantly to the health risk associated with inhalation of polluted air. Despite the health hazard they pose, NPAHs and OPAHs were rarely included in monitoring. The aim of this study is to provide the first multi-year temporal trends of the concentrations, composition pattern and fate of NPAHs and OPAHs in air from a site representative of background air quality conditions in central Europe. Samples were collected every second week at a rural background site in the Czech Republic during 2015–2017. Concentrations ranged from 1.3 to 160 pg m⁻³ for Σ17NPAHs, from 32 to 2600 pg m⁻³ for Σ10OPAHs and from 5.1 to 4300 pg m⁻³ for Σ2O-heterocycles. The average particulate mass fraction (θ) ranged from 0.01 ± 0.02 (2-nitronaphthalene) to 0.83 ± 0.22 (1-nitropyrene) for individual NPAHs and from <0.01 ± 0.01 (dibenzofuran) to 0.96 ± 0.08 (6H-benzo (c,d)pyren-6-one) for individual OPAHs and O-heterocycles. The multiyear variations showed downward trends for a number of targeted compounds. This suggests that on-going emission reductions of PAHs are effective also for co-emitted NPAHs and OPAHs.