# ATR-FTIR Spectral Analysis and Soluble Components of PM10 And PM2.5 Particulate Matter over the Urban Area of Palermo (Italy) during Normal Days and Saharan Events

Daniela Varrica, Elisa Tamburo, Marcello Vultaggio, Ida Di Carlo

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Daniela Varrica, Elisa Tamburo, Marcello Vultaggio, Ida Di Carlo. ATR-FTIR Spectral Analysis and Soluble Components of PM10 And PM2.5 Particulate Matter over the Urban Area of Palermo (Italy) during Normal Days and Saharan Events. International Journal of Environmental Research and Public Health, 2019, 16 (14), pp.2507. 10.3390/ijerph16142507 . insu-03469364

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Article

# ATR-FTIR Spectral Analysis and Soluble Components of PM₁₀ And PM₂.₅ Particulate Matter over the Urban Area of Palermo (Italy) during Normal Days and Saharan Events

Daniela Varrica <fnref n="1" />*, Elisa Tamburo <fnref n="1" />, Marcello Vultaggio <fnref n="2" /> and Ida Di Carlo <fnref n="3" />

Received: 7 May 2019; Accepted: 26 June 2019; Published: 13 July 2019

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**Abstract:** Several epidemiological studies have shown a close relationship between the mass of particulate matter (PM) and its effects on human health. This study reports the identification of inorganic and organic components by attenuated total reflectance-Fourier-transform infrared spectroscopy (ATR-FTIR) analysis in PM₁₀ and PM₂.₅ filters collected from three air quality monitoring stations in the city of Palermo (Sicily, Italy) during non-Saharan dust events and Saharan events. It also provides information on the abundance and types of water-soluble species. ATR-FTIR analysis identified sulfate, ammonium, nitrate, and carbonate matter characterized by vibrational frequencies at 603, 615, 670, and 1100 cm⁻<fnref n="1" /> (SO₄<fnref n="2" />⁻); at 1414 cm⁻<fnref n="1" /> (NH₄⁺); at 825 and 1356 cm⁻<fnref n="1" /> (NO₃⁻); and at 713, 730, and 877 cm⁻<fnref n="1" /> (CO₃<fnref n="2" />⁻) in PM₁₀ and PM₂.₅ filters. Moreover, aliphatic hydrocarbons were identified in the collected spectra. Stretching frequencies at 2950 cm⁻<fnref n="1" /> were assigned to CH₃ aliphatic carbon stretching absorptions, while frequencies at 2924 and 2850 cm⁻<fnref n="1" /> indicated CH₂ bonds. In filters collected during Saharan dust events, the analysis also showed the presence of absorbance peaks typical of clay minerals. The measurement of soluble components confirmed the presence of a geogenic component (marine spray and local rocks) and secondary particles ((NH₄)₂SO₄, NH₄NO₃) in the PM filters. ATR-FTIR characterization of solid surfaces is a powerful analytical technique for identifying inorganic and organic compounds in samples of particulate matter.

**Keywords:** particulate matter; PM₁₀ and PM₂.₅; ATR-FTIR; ionic soluble components; saharan dust events; sirocco winds

## 1. Introduction

The urban air people breathe contains several solid and gaseous chemicals that have significant negative effects on public health [1–3]. Several epidemiological studies have shown a close relationship between air pollution and various respiratory tract diseases (allergies, asthma, lung emphysema), lung cancer, and cardiopulmonary mortality, which commonly affect urban populations [4–9]. The World Health Organization (WHO) [10] and the Directive of the European Parliament [11] established that daily values in Europe for concentrations of particulate matter with sizes of ≤10 and ≤2.5 µm (i.e., PM₁₀ and PM₂.₅) should not exceed 50 µg/m<fnref n="3" /> and 25 µg/m<fnref n="3" />, respectively. Particulate matter with a size ≤10 µm is considered to be particularly detrimental to human health, but the nature of the PM is equally crucial as particle types have highly variable toxicity levels. Particulate matter comprises a range of particles such as mineral dust, metals, metalloids, sea salts, ammonium nitrate

<footnote n="1">¹ Dipartimento Scienze della Terra e del Mare (DiSTeM), Via Archirafi 22, 90123 Palermo, Italy</footnote>

<footnote n="2">² Risorse Ambiente Palermo (RAP), Piazzetta B. Cairoli, 90123 Palermo, Italy</footnote>

<footnote n="3">³ CNRS/INSU-Université d'Orléans—BRGM, UMR 7327, Institut des Sciences de la Terre d'Orléans, 1A rue de la Férollerie, 45071 Orléans, France</footnote>

<footnote>* Correspondence: daniela.varrica@unipa.it; Tel.: +39-91-23861644</footnote>
and sulfate, organic compounds, and elemental carbon. The abundance of the various organic and inorganic components is temporally and spatially variable [12]. Some are directly emitted into the atmosphere by either natural or anthropogenic sources (primary particles), while others are the result of homogeneous or heterogeneous nucleation and condensation of gaseous precursors (secondary particles). The Mediterranean area is often affected by Saharan dust events, which increase PM₁₀ and PM₂.₅ concentrations beyond European recommended values, mainly in southern Europe. Saharan dust is a mixture of mineral particles (quartz, calcite, dolomite, and clay minerals) and organic matter [13]. Some studies have suggested that Saharan dust has a significantly negative impact on air quality, visibility, and human health [14–16]. Several authors described increased asthma, rhinitis, cardiovascular disease, and mortality [17,18]. Other authors found no association between dust events and hospitalizations [19–23], increased mortality, or increased potential oxidative water-soluble fractions in PM₁₀ and PM₂.₅ [24] compared to anthropogenic dust.

Water-soluble components (WSCs) are among the main components of total particulate matter [25,26], typically contributing about 50%–70% of the weight. WSCs are associated with degraded atmospheric visibility and adverse effects on human health [27–29]—they also contribute to the formation of acid rain, which promotes the faster decay of buildings. The main analytical technique used to determine water-soluble components is ion chromatography (IC). In recent years, Fourier-transform-infrared spectroscopy (FTIR) has become important in identifying aerosol composition and quantifying the mass of organic and inorganic compounds in particulate matter [30–33]. FTIR coupled with accessories like attenuated total reflectance (ATR) allows the analysis of a wide range of solid and liquid components [34].

In this study, we present data on the chemical composition of water-soluble components in PM₁₀ and PM₂.₅ samples collected in an urban area of southern Italy. The city of Palermo, chosen for our case study, is affected by urban pollution and natural particulate matter from a range of sources. The principal sources in the study area are gasoline- and diesel-powered vehicles, an active commercial and tourist harbor, domestic heating, and a geogenic component that includes soil erosion, marine aerosol, and sporadic Saharan dust events. The aim of this paper is to identify the principal functional groups of inorganic and organic components in atmospheric aerosols by ATR-FTIR analysis. Moreover, we report the results of FTIR analysis carried out on samples of PM₁₀ and PM₂.₅ filters taken during Saharan dust events that affected the Mediterranean area.

## 2. Materials and Methods

### 2.1. Site Details

Palermo is the largest urban area of Sicily, with about 680,000 inhabitants and a metropolitan area populated by more than 1 million people. The city is situated on the north-western coast of the island, bordered on the northeast by the Tyrrhenian Sea and surrounded by mountains (Monti di Palermo) reaching 500–1000 m above sea level (Figure 1).

The study area is entirely covered by sedimentary rocks (limestone, clay, marly-clay, and white or yellow quaternary biocalcarenite). The climate of Palermo is typically Mediterranean, with hot summers and temperate winters. Among the stations studied, only Boccadifalco (BF) station records weather data representative of the entire agglomeration where the other stations of the present study (Giulio Cesare (GC) and Di Blasi (DB) are located. Figure 2 shows the wind rose of the sampling period (November 2008–February 2009). From the monthly wind roses during the winter months, the prevailing wind direction is from the WNW and WSW sectors. In the same period, close to 5% wind direction from the S and SSE sectors (Sirocco winds) has been registered. During autumn and spring in the city, there are frequent warm winds coming from south-east (Sirocco winds) carrying dust raised from the Sahara Desert region throughout the Mediterranean basin. Over the sampling period, the weather monitoring station located in the peripheral area of Palermo (BF station) registered six periods of 1–2 days of Saharan dust intrusions.
<figure><img src="image_4.png" /><figcaption>**Figure 1.** Location of study area with sampling sites. BF, Boccadifalco; DB, Di Blasi; GC, Giulio Cesare.</figcaption></figure>

<figure><img src="image_5.png" /><figcaption>**Figure 2.** Prevailing winds at Palermo during the sampling period.</figcaption></figure>

## 2.2. *Sampling Sites*

A total of 348 daily samples, 308 PM₁₀ and 40 PM₂.₅, were collected from November 2008 to February 2009. To meet the requirements of Directive 1999/30/EC (EU Commission, 1999), PM₁₀ sampling was performed according to European Standard EN12341 (CEN, 1998), with a low-volume system equipped with a sampling inlet head (Zambelli Explorer Plus Controller 16) operating at a constant sampling rate (2.3 m³h⁻¹). Particles were collected on standard 47 mm quartz filters (Advantec, grade QR100). The sampling time was 24 h, from midnight to midnight. PM₂.₅ sampling was performed according to European standard EN 14907 (CEN 2005). At Di Blasi (DB) station, simultaneous sampling
of PM₁₀ and PM₂.₅ was carried out. PM₁₀ mass determination was performed by β-ray attenuation method, model Environment MP101M.C (CNR-Italy certified). The beta attenuation instrument is compliant with EN 12341 for PM₁₀ and is approved as federal equivalent method by US the Environmental Protection Agency for PM₁₀. The detection is done every 2 hours (12 detections in 24 hours). Initial and final weighing of PM₁₀ and PM₂.₅ filters were carried out in a temperature- and humidity-controlled room (T = 20 ± 1 °C, RH = 50 ± 5%) after the filters had been conditioned for 48 h before and after sampling. Three air quality monitoring stations belonging to the municipal monitoring network (RAP-ex AMIA) were chosen for this study (Figure 1).

The Di Blasi (DB) station is located close to a crossroads with traffic lights at pedestrian crossings and is characterized by high traffic flow, consisting of cars, heavy-duty vehicles, and buses. Giulio Cesare (GC) station is situated in a large square in front of the railway station, exposed to heavy traffic composed of cars as well as urban and regional buses. The Boccadifalco (BF) station is a suburban background station, situated leeward of the sea breeze, without any direct influence of urban activities. It has lower traffic density than the other stations and was selected as a control site to monitor the hypothetical background level of pollution. Filters used for analysis were selected based on the simultaneity of daily sampling between the three monitoring stations. ATR-FTIR spectroscopy was used to analyze 13 PM₁₀ filters from the suburban background station (BF), 36 PM₁₀ filters from the urban station (GC), 40 PM₂.₅ filters from the urban station (DB), and one composite sample of Saharan dust deposited in Palermo town. A total of 1 g of Saharan dust was taken near GC station using a plastic brush and tray and stored in plastic bags. The sample was initially sieved through a 63 µm sieve to remove coarse components. Afterward, screening through a 20 µm mesh sieve was necessary to obtain a finer fraction for FTIR analysis. The following were analyzed for water-soluble ions: 13 PM₁₀ filters from BF station, 30 PM₁₀ filters from GC station and 30 PM₂.₅ filters from DB station.

## 2.3. Analytical Procedures

### 2.3.1. FTIR Spectra

A Bruker Optics (Tensor 27) IR (Bruker Corporation, Billerica, MA, USA) spectrometer equipped with a deuterated triglyceride sulfate detector was operated with Opus software from Bruker to obtain the spectra of ambient air samples. An ATR accessory with a germanium crystal flat plate was coupled with the spectrometer for data acquisition. Aerosol sample spectra were obtained over wavelengths between 4000 and 400 cm⁻¹ (mid-infrared region) with 2 cm⁻¹ resolution by averaging 32 scans. Each aerosol sample was scanned by placing the quartz fiber filter sample-side down on the ATR crystal and applying the pressure tower. Each IR spectrum was corrected for optical effects with the ATR correction algorithm in Opus. A blank quartz fiber spectrum was obtained with each set of daily samples to account for any changes in the absorbance bands due to instrument drift. Between each sample spectrum acquisition, the ATR crystal was cleaned with ethanol, and an air background spectrum was obtained. The FTIR operation method is explained in Doyle [35] and Simonescu [36].

### 2.3.2. Water-Soluble Ions

Water-soluble ions were extracted from filter samples with 20 mL ultra-pure Milli-Q (Merck Millipore, Burlington, MA, USA) water (18MΩ cm) and shaken for 24h. The extracts were filtered through a 0.45 µm pore size polytetrafluoroethylene filter (Sartorius) and then stored in sterile 50 mL polypropylene centrifuge tubes. Each extract was analyzed the day after the extraction procedure for Ca²⁺, Mg²⁺, Na⁺, K⁺, Cl⁻, SO₄²⁻, and NO₃⁻ ions by ion chromatography (Dionex 100), with precision better than ± 5%. Cations were measured using a Dionex IonPac CS12A (Thermo Fisher Scientific, Waltham, MA, USA) column with 20 mM methanesulfonic acid as the eluent. Anions were measured using a Dionex IonPac AS14 (Thermo Fisher Scientific, Waltham, MA, USA) with 3.5 M Na₂CO₃ and 1.0 mM NaHCO₃ as the eluent. The limit of detection was evaluated by solution extracts for three blank filters in 0.02–0.05 and 0.04–0.05 mg/L for cations and anions, respectively. NH₄⁺ ions were
determined spectrophotometrically at λ = 420 nm (Thermo Scientific Evolution 600) using Nessler's reagent (0.09 mol/L solution of potassium tetraiodomercurate (II) ($K_2[HgI_4]$)) in 2.5 mol/L potassium hydroxide). The ion chromatograph operation method is explained in Michalski [37].

# 3. Results and Discussion

## 3.1. Mass Levels of PM₁₀ and PM₂.₅

Table 1 shows the mass levels of PM₁₀ at the urban and peripheral stations (GC, DB, and BF) and of PM₂.₅ at the urban DB station.

<table><caption>**Table 1.** Characteristics of PM₁₀ and PM₂.₅ samples at the three monitoring stations during non-Saharan dust events and Saharan dust events. Mass values expressed in µg/m³. # indicates measurements carried out simultaneously.</caption><thead><tr><th colspan="5">November 2008–February 2009</th></tr><tr><th></th><th colspan="2">PM<sub>10</sub></th><th colspan="2">PM<sub>2.5</sub></th></tr><tr><th></th><th>BF station</th><th>GC station</th><th>DB station #</th><th>DB station #</th></tr></thead><tbody><tr><td>N</td><td>95</td><td>108</td><td>105</td><td>40</td></tr><tr><td>Mean</td><td>16</td><td>39</td><td>42</td><td>29</td></tr><tr><td>Std.Dev.</td><td>7</td><td>11</td><td>11</td><td>6</td></tr><tr><td>Median</td><td>15</td><td>39</td><td>43</td><td>30</td></tr><tr><td>Min</td><td>8</td><td>16</td><td>13</td><td>13</td></tr><tr><td>Max</td><td>44</td><td>69</td><td>74</td><td>40</td></tr><tr><td>Q<sub>10</sub></td><td>10</td><td>26</td><td>28</td><td>22</td></tr><tr><td>Q<sub>25</sub></td><td>12</td><td>32</td><td>35</td><td>25</td></tr><tr><td>Q<sub>75</sub></td><td>17</td><td>46</td><td>49</td><td>33</td></tr><tr><td>Q<sub>90</sub></td><td>27</td><td>53</td><td>55</td><td>37</td></tr><tr><th colspan="5">Saharan Dust Events</th></tr><tr><td>N</td><td>7</td><td>7</td><td>8</td><td>4</td></tr><tr><td>Mean</td><td>130</td><td>158</td><td>133</td><td>78</td></tr><tr><td>Dev.St</td><td>89</td><td>81</td><td>59</td><td>28</td></tr><tr><td>Min</td><td>67</td><td>97</td><td>89</td><td>59</td></tr><tr><td>Max</td><td>261</td><td>276</td><td>220</td><td>120</td></tr></tbody></table>

The mean PM₂.₅ and PM₁₀ concentrations fall within the range reported for European urban areas [38–40]. The highest mean PM₁₀ value was observed at the urban DB station (42 µg/m³), one of the most heavily traffic-exposed sites in Palermo, followed by GC station (39 µg/m³) and BF station (16 µg/m³). The average PM₂.₅ value observed at DB station is 29 µg/m³. For the 112 days analyzed (November 2008–February 2009), Saharan dust events influenced mass levels in the Palermo atmosphere on about 6% of the days. During these events, concentrations of 130–158 µg/m³ and 78 µg/m³ were measured for PM₁₀ and PM₂.₅, respectively. In Palermo in February 2009, PM₂.₅ reached a daily concentration of 120 µg/m³ and PM₁₀ reached values between 220 and 276 µg/m³ following a high-intensity Saharan dust event. The value of PM₂.₅ is comparable to that found by Remoundaki et al. [41] in Athens in February 2009 (100 µg/m³). During other, less-intense Saharan dust events, PM₂.₅ concentrations (average 62 µg/m³) increased by 50% and PM₁₀ (average 86–119 µg/m³) by 65–80%. The values reported are higher than those published in previous studies concerning southern Italy (Rome: PM₂.₅, 25.6 µg/m³; PM₁₀, 47.2 µg/m³ [16]; Salento: PM₂.₅, 36.6 µg/m³; PM₁₀, 137 µg/m³ [24]; Bari: PM₂.₅, 31–49 µg/m³; PM₁₀, 50–71 µg/m³ [42]), but the higher percentages during Saharan dust events are comparable [24,43–45]. In general, the contribution of particulate matter is evidenced in coarse rather than fine fractions [41]. The influence of Saharan dust on the Mediterranean basin has been estimated to be about 10–20% per year, thus many European countries have exceeded the PM limits recommended by the European Directive. The PM₂.₅/PM₁₀ ratio has been widely used in
environmental studies as an indicator of the contribution from stationary vs. mobile source emissions to the environment.

The average PM<sub>2.5</sub>/PM<sub>10</sub> ratio measured at DB station is 0.70. This value is typical of urban environments with high traffic density [26,40,46–49]. During Saharan events, the PM<sub>2.5</sub>/PM<sub>10</sub> ratio was only 0.58, indicating a greater natural contribution of coarse than fine particles.

## 3.2. Spectral Analysis

The ATR spectra of PM<sub>10</sub> and PM<sub>2.5</sub> are shown in Figure 3a–c. The spectra identify different inorganic and organic molecules (Table 2).

<figure><img src="image_6.png" /><figcaption>**Figure 3.** FTIR spectra of (a) suburban PM<sub>10</sub> filter (BF station); (b) urban PM<sub>10</sub> filter (GC station); and (c) urban PM<sub>2.5</sub> filter (DB station). For each spectrum, we also report the spectrum of a blank quartz filter (black line) for comparison.</figcaption></figure>
Some peaks have no well-defined forms, and the presence of a shoulder indicates that there are overlapping peaks due to several different types of molecules absorbing IR radiation within the same range. From comparing the spectra, it is observed that the samples are dominated by inorganic components common to all stations.

In PM₁₀ and PM₂.₅ filters, we observed vibrational frequencies typical for sulfate, ammonium, nitrate, and carbonate ions (603, 615, 670, and 1100 cm⁻¹ (SO₄²⁻); 1414 cm⁻¹ (NH₄⁺); 825 and, 1356 cm⁻¹ (NO₃⁻); and 713, 730, and 877 cm⁻¹ (CO₃²⁻). The presence of (NH₄)₂SO₄ and NH₄NO₃ compounds is supported by spectra shown in Figure 3b,c revealing absorption frequencies at 825 and 1356 cm⁻¹ (group NO₃⁻), at 615 and 1100 cm⁻¹ (group SO₄²⁻), and at 1414 cm⁻¹ (NH₄⁺ ion) [30,50]. The inferred 1100 cm⁻¹ peak is a shoulder of the peak observed at 1060 cm⁻¹. The 1100 cm⁻¹ peak is assigned to the v3 asymmetrical stretching vibration of sulfate ion [51,52].

In all spectra (for coarse and fine particles), absorption frequencies at 1620 cm⁻¹ and in the range of 3240–3400 cm⁻¹ have been detected that can be attributed to O–H stretching, indicating crystalline water in gypsum [34,53].

The presence of CaSO₄ × 2H₂O is more evident in coarse than fine particles. The common presence of CaSO₄ × 2H₂O signals supports the widely accepted hypothesis that the sulfation process is important in urban environments [54]. Varrica et al. [55] observed CaSO₄ × 2H₂O crust on CaCO₃ particles by scanning electron microscopy (SEM) of samples also collected in Palermo. In samples of “black crust” formed on historical buildings in Palermo, Montana et al. [56] determined δ³⁴S values ranging from –0.5 to +5.0‰ (vs. Vienna Cañon Diablo Troilite (VCDT) scale), which suggests that most of the sulfur was derived from fossil fuel combustion. Moreover, Cesari et al. [43] observed that during Saharan dust events, the dominant form of sulfate is calcium sulfate rather than (NH₄)₂SO₄. The absorption peaks at 713, 730, and 877 cm⁻¹ are typical for the CO₃ group [53,57,58], and the FTIR analysis of pure crystalline calcite and dolomite confirms that these peaks are related to CaCO₃. The peaks of halite between 1000 and 1200 cm⁻¹ are not clearly visible due to the absorption linked with the quartz filter. In the GC and BF samples, there is also a peak at 1620 cm⁻¹ that can be attributed to one of the peaks of halite; at 1414 cm⁻¹ the peak of halite is not visible as it is very small and overlaps with the ammonium ion peak.

<table><caption>**Table 2.** Typical peaks of inorganic and organic molecules identified in filter samples during non-Saharan events and Saharan dust events.</caption><thead><tr><th>Species</th><th>Frequency (cm<sup>-1</sup>) in This Study</th><th>Frequency (cm<sup>-1</sup>) from Literature</th><th>References</th></tr></thead><tbody><tr><td colspan="4"><strong>Non-Saharan Events</strong></td></tr><tr><td>SO<sub>4</sub><sup>2-</sup></td><td>603; 615; 670; 1100</td><td>608; 615; 670; 1100</td><td>[30,35,36,51–53]</td></tr><tr><td>CO<sub>3</sub><sup>2-</sup></td><td>713; 730; 877</td><td>713; 730; 873; 877</td><td>[53,57,58]</td></tr><tr><td>NO<sub>3</sub><sup>-</sup></td><td>825; 1356</td><td>825; 1318–1410; 1350</td><td>[30,58]</td></tr><tr><td>NH<sub>4</sub><sup>+</sup></td><td>1414</td><td>1414</td><td>[50]</td></tr><tr><td>C=C</td><td>1510–1596</td><td>1463–1511–1596</td><td>[59,61]</td></tr><tr><td>C-H</td><td>1460; 2850; 2920; 2950</td><td>2850–2920; 2800–3000</td><td>[30,31,34,58–60]</td></tr><tr><td>Water (OH)</td><td>1620; 3200–3400; 3620</td><td>1620; 3200–3400; 3620</td><td>[34,53,62]</td></tr><tr><td>Al-O-Si</td><td>540</td><td>540</td><td>[57,58]</td></tr><tr><td>Si-O</td><td>1030</td><td>1030</td><td>[30,62]</td></tr><tr><td>C = O</td><td>1720</td><td>1720; 1722</td><td>[34,58]</td></tr><tr><td colspan="4"><strong>Saharan Dust Events</strong></td></tr><tr><td>O-Si-O</td><td>423; 463; 520</td><td>426; 468; 525</td><td>[63]</td></tr><tr><td>SO<sub>4</sub><sup>2-</sup></td><td>603; 615; 670; 1110</td><td>608; 615; 670; 1100</td><td>[30,60]</td></tr><tr><td>CO<sub>3</sub><sup>2-</sup></td><td>713; 730; 780; 877;1433</td><td>713; 730; 873; 877</td><td>[58,62]</td></tr><tr><td>Al-O-Si</td><td>750</td><td>750</td><td>[63,64]</td></tr><tr><td>Al-Al-OH</td><td>912</td><td>910</td><td>[62,65]</td></tr><tr><td>NO<sub>3</sub><sup>-</sup></td><td>825; 1356</td><td>825; 1318–1410; 1350</td><td>[30,32,58]</td></tr><tr><td>NH<sub>4</sub><sup>+</sup></td><td>1414</td><td>1414</td><td>[50]</td></tr><tr><td>C = C</td><td>1510–1596</td><td>1463–1511–1596</td><td>[59,61]</td></tr><tr><td>C-H</td><td>1460; 2800–3000</td><td>1460; 2850–2920; 2800–3000</td><td>[30,31,34,58,59]</td></tr><tr><td>Water (OH)</td><td>688; 1620; 1685; 3260–3400; 3620; 3669; 3695</td><td>688; 1620; 3200–3400; 3620; 3669; 3695</td><td>[34,62,63,66]</td></tr><tr><td>Si-O</td><td>1010; 1032</td><td>1010; 1030; 1031</td><td>[30,62,67]</td></tr></tbody></table>
Organic compounds are identified in the coarse and fine particle fractions of the urban stations but are absent from the filters collected at the suburban station. The aliphatic hydrocarbons (2850, 2920, and 2950 cm⁻¹) were clearly identified in the collected spectra (Figure 3b,c) [30,31,34,59–61]. The stretching frequency at 2950 cm⁻¹ is assigned to CH₃ aliphatic carbon stretching absorption, while the frequencies at 2924 and 2850 cm⁻¹ are due to CH₂ bonds. An absorption peak at 1460 cm⁻¹ comprises contributions from bending of CH₃ and CH₂ aliphatic carbon bonds [30,59]. Vibration around 1460 cm⁻¹ is a shoulder of the peak at 1414 cm⁻¹. The spectra for PM₂.₅ filters also show an absorbance peak at 1596 cm⁻¹, identified as a C = C group [59,61]. The identification of other peaks for C = C aromatic group (1463–1511–1596 cm⁻¹) is complicated by overlapping peaks due to several different types of molecules that absorb IR radiation within the same range.

### 3.3. Spectral Analysis Of Samples Collected During Saharan Dust Episodes

The particulate matter collected during Saharan dust events show peaks belonging to a group of clay minerals, which were not detected during non-Saharan events. Figure 4 shows the ATR spectra of the urban area (GC) PM₁₀ filter, the urban area (DB) PM₂.₅ filter, and the Saharan dust.

<figure><img src="image_7.png" /><figcaption>**Figure 4.** FTIR spectra of urban PM₁₀ (GC, yellow line) and PM₂.₅ (DB, red line) filters. Blue line is FTIR spectrum of Saharan dust deposited in Palermo.</figcaption></figure>

Peaks at wavenumbers of 423, 463, and 520 cm⁻¹ are associated with the O–Si–O bending of palygorskite and illite (426, 468, and 525 cm⁻¹) [63]. The peak at 750 cm⁻¹ identifies the inner layer vibration of Al–O–Si groups in illite [63,64]. Previous studies assigned the peak at 912 cm⁻¹ to the deformation of Al–Al–OH groups in the dioctahedral layer of palygorskite [62,65]. The identification of kaolinite is characterized by the presence of peaks at 1010, 1032, and 1114 cm⁻¹, representing the Si–O stretching group [67]. Peaks at 1032 and 1114 cm⁻¹ are not distinct because they simultaneously characterize various molecules that vibrate in the same IR intervals, creating peak overlaps.

Peaks at 3260, 3400, 3620, 3669, and 3695 cm⁻¹ are all linked to the vibration of –OH groups belonging to different clay minerals. Peaks at 3260 and 3400 cm⁻¹ are reported to relate to water stretching in palygorskite [63,65]. The OH groups located between tetrahedral and octahedral sheets are characterized by absorption near 3620 cm⁻¹ in all clay minerals. They reside at the octahedral surface of the layers, forming weak hydrogen bonds with the oxygens of the Si–O–Si bonds on the lower surface of the next layer. A strong band at 3695 cm⁻¹ relates to the in-phase symmetric stretching vibration. Weak absorptions at 3669 cm⁻¹ are assigned to out-of-plane stretching vibrations [68,69]. In these samples, we found the same organic components as observed in the samples taken during non-Saharan events.
### 3.4. Water-Soluble Ions

Table 3 shows the mean concentrations of soluble components of PM₁₀ and PM₂.₅ filters. Inorganic ions represent about 50%–70% of the total mass of PM₁₀ and PM₂.₅.

<table><caption>**Table 3.** Soluble ion concentrations. Data expressed in µg/m³. nss, non-sea salt; ΣTP, total mass of ions; TPM, total particulate matter (µg/m³).</caption><thead><tr><th rowspan="2"></th><th colspan="2">PM<sub>10</sub></th><th>PM<sub>2.5</sub></th></tr><tr><th>BF station</th><th>GC station</th><th>DB station</th></tr></thead><tbody><tr><td>F<sup>-</sup></td><td>0.15</td><td>0.15</td><td>0.17</td></tr><tr><td>Cl<sup>-</sup></td><td>1.19</td><td>1.70</td><td>0.64</td></tr><tr><td>NO<sub>3</sub><sup>-</sup></td><td>2.30</td><td>4.13</td><td>2.91</td></tr><tr><td>SO<sub>4</sub><sup>2-</sup></td><td>2.69</td><td>2.26</td><td>2.49</td></tr><tr><td>Na<sup>+</sup></td><td>1.14</td><td>1.47</td><td>0.74</td></tr><tr><td>K<sup>+</sup></td><td>0.23</td><td>0.27</td><td>0.23</td></tr><tr><td>Mg<sup>2+</sup></td><td>0.20</td><td>0.24</td><td>0.09</td></tr><tr><td>Ca<sup>2+</sup></td><td>0.78</td><td>1.60</td><td>1.33</td></tr><tr><td>NH<sub>4</sub><sup>+</sup></td><td>0.96</td><td>1.32</td><td>1.52</td></tr><tr><td>nssSO<sub>4</sub><sup>2-</sup></td><td>2.44</td><td>2.05</td><td>2.10</td></tr><tr><td>ΣTM</td><td>9.64</td><td>13.1</td><td>10.1</td></tr><tr><td>TPM</td><td>19.5</td><td>37.0</td><td>29.3</td></tr></tbody></table>

About 60% and 70% of total ions analyzed in PM₁₀ and PM₂.₅ filters, respectively, are made up of NH₄⁺, NO₃⁻, and SO₄²⁻. For urban stations (PM₁₀ and PM₂.₅) the ammonium and calcium ions (expressed in neq/m³) are the most abundant cations. Magnesium and potassium are less abundant, contributing only about 1% to the total content of particulate matter. If the soluble calcium is derived from the alteration of carbonate rocks, a geogenic contribution of 10–14% of the total mass of the PM₁₀ fraction from urban and suburban stations is estimated. In the fine PM₂.₅ fraction, a geogenic contribution is estimated to account for 9% of the total mass at the urban station.

NO₃⁻ and SO₄²⁻ anions have the highest concentration at all stations. In this study, the contribution of marine sulfate was calculated to have been around 6–10% in PM₁₀ and 3% in PM₂.₅ fractions. The main source of SO₄²⁻ in the atmosphere is from gas-to-particle conversion of SO₂. NO₃⁻ ions derive from the reaction of hydroxyl radicals, formed by photolysis of ozone molecules, with NOₓ emitted by fossil fuel combustion. High concentrations of ammonium, sulfate, and nitrate ions demonstrate their involvement in secondary particulate formation. A significant correlation between NH₄⁺ and (nssSO₄²⁻ + NO₃⁻) has been found (r = 0.90, p < 0.05; Figure 5), confirming the formation of ammonium sulfate and nitrate following neutralization of aerosol through heterogeneous atmospheric chemical reactions [47,70–72].

<figure><img src="image_8.png" /><figcaption>**Figure 5.** Plot of NO₃⁻+nss-SO₄²⁻ vs NH₄⁺ ion concentrations. Data expressed in neq/m³.</figcaption></figure>
These sequences of reactions are strongly influenced by ambient temperature, relative humidity conditions, incidence of solar radiation, and above all the concentration of primary gases [73]. The equivalent ratio of NH<sub>4</sub><sup>+</sup>/nss-SO<sub>4</sub><sup>2-</sup> in urban PM<sub>10</sub> and PM<sub>2.5</sub> is more than 1.5, characterizing the ambient atmosphere as ammonium-rich [74]. Nevertheless, as Figure 5 shows, the concentration of ammonium ions is insufficient to completely neutralize H<sub>2</sub>SO<sub>4</sub> and HNO<sub>3</sub>. Total neutralization of the acid species is linked to the presence of carbonate rocks, abundant in the study area. The highest chlorine and sodium contents found in coarse samples (GC and BF) range between 1.70 and 1.19 µg/m<sup>3</sup> and 1.14 and 1.45 µg/m<sup>3</sup>, respectively. The main source of Cl<sup>-</sup> and Na<sup>+</sup> in the study area is marine spray, accounting for 11-15% of the total mass in the PM<sub>10</sub> fraction from urban and suburban stations. For fine PM<sub>2.5</sub> fraction, sea salt contribution is estimated to account for 9% of the total mass at DB station. The average Na/Cl equivalent ratio measured in the PM<sub>10</sub> and PM<sub>2.5</sub> filters ranges between 1.4 and 1.8. These values are higher than those of seawater (0.85) and halite (1.0), suggesting a loss of chlorine ions due to chemical reactions that involve NaCl and HNO<sub>3</sub> or H<sub>2</sub>SO<sub>4</sub>, bringing the formation of NaNO<sub>3</sub> or Na<sub>2</sub>SO<sub>4</sub> and gaseous HCl [66]. Similarly, a deficit of ammonium with respect to the collective concentration of SO<sub>4</sub><sup>2+</sup> and NO<sub>3</sub><sup>-</sup> (neq/m<sup>3</sup>) suggests that a proportion of these ions is lost via formation of NH<sub>4</sub>Cl or HCl and NH<sub>3</sub> [47,51].

**4. Conclusions**

The main objective of this study was to verify the potential of ATR-FTIR to identify organic and inorganic groups present in PM₁₀ and PM₂.₅. The use of ATR-FTIR led to the identification of absorption bands characteristic of sulfate, ammonium, nitrate, and carbonate by vibrational frequencies at 603, 615, 670, and 1100 cm⁻¹ for SO₄²⁻, at 1414 cm⁻¹ for NH₄⁺, at 825 and 1356 cm⁻¹ for NO₃⁻, and at 713, 730, and 877 cm⁻¹ for CO₃²⁻ common to all filter types (PM₁₀ and PM₂.₅). Vibration frequencies at 1620 cm⁻¹ and in the range of 3240-3400 cm⁻¹ indicate O-H stretching of crystalline water in gypsum. The presence of gypsum in the particulate matter of Palermo confirms the hypothesis that sulfation processes play an important role in urban areas. Moreover, in urban spectra, several organic compounds were identified, while aliphatic compounds were not detected at the suburban station. The ATR-FTIR analysis of filters taken during Saharan dust events shows the presence of absorbance peaks typical for clay minerals. The minerals found were palygorskite, illite, and kaolinite, which are typical for Saharan desert environments.

The water-soluble components represent about 50%-70% of the total mass of PM₁₀ and PM₂.₅. Nitrate and sulfate ions had the highest concentrations at all stations, confirming their involvement in secondary particulate formation. The results show that ammonium ions are not able to neutralize most of the nitric and sulfuric acids present in aerosols. The main geogenic sources in the study area are marine spray and local rocks.

The data of this study shows that ATR-FTIR, used here as a qualitative approach, is a powerful analytical technique for the identification of inorganic and organic compounds in PM₁₀ and PM₂.₅ filters. Moreover, the simplicity of the substrate preparation, the excellent reproducibility of the results, the non-destruction of the sample, and above all the fast identification of components of particulate matter confirm the opportunity to use this analytical technique for qualitative analysis, and to characterize variations in the chemical composition of aerosol particles during intense pollution episodes.

**Author Contributions:** Conceptualization, D.V. and I.D.C.; Data curation, D.V., E.T. and I.D.C.; Formal analysis, D.V., E.T. and I.D.C.; Funding acquisition, D.V.; Methodology, M.V.; Writing—original draft, D.V., E.T. and I.D.C.

**Acknowledgments:** This work was supported by Miur (funds FFR2018, D. Varrica). We would like to thank Risorse Ambiente Palermo (RAP, ex AMIA) of Palermo (Italy) (http://www.rapspa.it/site/) for providing the filter samples.

**Conflicts of Interest:** The authors declare no conflict of interest.
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