Quantifying functional group compositions of household fuel-burning emissions

Abstract

Globally, billions of people burn fuels indoors for cooking and heating, which contributes to millions of chronic illnesses and premature deaths annually. Additionally, residential burning contributes significantly to black carbon emissions, which have the highest global warming impacts after carbon dioxide and methane. In this study, we use Fourier transform infrared spectroscopy (FTIR) to analyze fine-particulate emissions collected on Teflon membrane filters from 15 cookstove types and 5 fuel types. Emissions from three fuel types (charcoal, kerosene, and red oak wood) were found to have enough FTIR spectral response for functional group (FG) analysis. We present distinct spectral profiles for particulate emissions of these three fuel types. We highlight the influential FGs constituting organic carbon (OC) using a multivariate statistical method and show that OC estimates by collocated FTIR and thermal–optical transmittance (TOT) are highly correlated, with a coefficient determination of 82.5 %. As FTIR analysis is fast and non-destructive and provides complementary FG information, the analysis method demonstrated herein can substantially reduce the need for thermal–optical measurements for source emissions.

1 Introduction

Residential burning is a major source of organic carbon (OC) and contributes approximately 30 % of global emissions of black carbon, which is estimated to have the third-highest global warming impact after carbon dioxide and methane . The World Health Organization (WHO) estimates that close to 4 million premature deaths per year are associated with exposure to household air pollution, mainly from solid-fuel burning . Recent studies have typically categorized fine particulate matter (PM${}_{\mathrm{2.5}}$) emissions from household fuel-burning emissions by mass, OC, and elemental carbon (EC) emission factors using gravimetric and thermal–optical methods (e.g., IMPROVE and NIOSH protocols) . However, thermal–optical OC–EC measurements can sometimes take more than 45 min per sample and are destructive, while providing limited information as OC and EC alone are only bulk properties of carbonaceous particles.

In contrast to thermal–optical methods, Fourier transform infrared spectroscopy (FTIR) measurements take a few minutes per sample, they are non-destructive and highly reproducible, and they provide more chemical information. FTIR measurements have been shown to be in good agreement with common methods for the chemical characterization of organic matter (OM) such as aerosol mass spectrometry (AMS) and thermal–optical analysis . However, FTIR has not been extensively used for the chemical analysis of primary particulate emissions from residential burning.

In the current study, we use FTIR to quantify the organic functional group (FG) composition of PM${}_{\mathrm{2.5}}$ emissions from cookstoves collected on polytetrafluoroethylene (PTFE) filters. We find that OC estimates from FTIR measurements and regression modeling are in good agreement with those from thermal–optical transmittance (TOT). Our analysis highlights spectral differences among fuels (charcoal, kerosene, red oak wood, alcohol, and liquefied petroleum gas) and their particulate emissions during combustion. Estimates of aromatics and polycyclic aromatic hydrocarbons (PAHs) from FTIR measurements of particulate emissions from charcoal, kerosene, and red oak wood are compared with those using gas chromatography–mass spectrometry (GS–MS) measurements. Estimates of aromatics and PAHs from FTIR measurements have been previously unavailable for primary source emissions. The implications of this study include the widened and improved analytical chemical portfolio for aerosol PM${}_{\mathrm{2.5}}$ emissions, leading to increased laboratory throughput and understanding of the compositional attributes of a known toxic PM${}_{\mathrm{2.5}}$ component.

2 Materials and methods

An overview of cookstove testing, emissions sampling, OC–EC measurements, GC–MS PAH measurements, FTIR measurements, and post-processing are illustrated via a flow chart in Fig. . The details of measurements and post-processing either described or cited from previous publications are in the subsections below. In short, a range of stoves and fuels were tested for burn emissions, from which parallel PTFE membrane and quartz fiber (QF) filter samples were collected. PTFE filters were used to measure gravimetric PM${}_{\mathrm{2.5}}$ mass and then scanned using transmission-mode FTIR. The quartz filters were used to measure TOT OC–EC and GC–MS PAHs. From these sets of measurements, partial least squares regression (PLSR) models were built for the identification of important FTIR group frequencies for OC and PAH, and the peak fitting and quantification of FGs, OC, and OM $/$ OC were performed.

Figure 1

Flow chart from sample collection to measurements, post-processing, and results.

[Figure omitted. See PDF]

2.1 Cookstove emissions testing and sampling

Cookstove emissions tests were conducted at the U.S. Environmental Protection Agency cookstove test facility in Research Triangle Park, North Carolina. Details of the facility and protocols are described in previous publications . We analyzed 152 samples from 15 different stoves and 5 fuel types, pictured in Fig. . Fuels tested covered charcoal (56 samples), kerosene (21 samples), red oak wood (69 samples), alcohol (3 samples), and liquefied petroleum gas (LPG) (3 samples).

Figure 2

Photo showing 15 stoves used in this work. Charcoal stoves: (a) EcoZoom Jet, (b) Prakti Leo, (c) Envirofit CH4400, (d) Jikokoa (inset), and (e) Éclair (inset). Kerosene stoves: (f) Butterfly Wick (model 2668), and (g) Butterfly Pressure (model  2412). Red oak wood stoves: (h) Jiko Poa, (i) Envirofit G3300, (j) Philips HD4012, (k) Home stove (Biolite), (l) Eco Chula XXL (inset), and (m) three-stone fire (inset). Alcohol stove: (n) Cleancook (inset). LPG stove: (o) Sol gas.

[Figure omitted. See PDF]

In this study, particulate emissions from stoves during the Water Boiling Test (WBT) were sampled. The WBT protocol (version 4, Global Alliance for Clean Cookstoves, 2014) includes three test phases: (1) a high-power cold-start (CS) phase in which the stove, pot, and water are at ambient temperature at the beginning of the test phase; (2) a high-power hot-start (HS) phase in which the stove is hot at the beginning of the test phase; and (3) a low-power simmering phase (SIM) in which the water temperature is kept 3 °C below the boiling point (Sect. S1 in the Supplement) . A modified protocol described by was used for the charcoal stove.

PM${}_{\mathrm{2.5}}$ was sampled isokinetically on QF (47 mm diameter Tissuquartz™ pure quartz no binder, Pall Corporation) filters and PTFE membrane filters (47 mm diameter Teflon^® membrane, Pall Corporation) positioned in parallel and downstream of PM${}_{\mathrm{2.5}}$ cyclones (URG; Chapel Hill, NC) at a flow rate of 16.7 L min${}^{-\mathrm{1}}$. PM${}_{\mathrm{2.5}}$ was also sampled downstream of the PTFE filter using a QF back filter for artifact correction. The ratio between OC on QF back and front filters ranged between 0.06–1.79. The filter-based PM${}_{\mathrm{2.5}}$ sampling was conducted in a primary dilution tunnel (15.2 cm) for low-emission fuel–cookstove combinations (e.g., forced-draft biomass stoves) and in a secondary dilution tunnel (25.4 cm) for those with high emissions (e.g., natural-draft biomass stoves) to avoid overloading filters. Volumetric flow rates were $\sim$ 4.0 and $\sim$ 26.8 m${}^{\mathrm{3}}$ min${}^{-\mathrm{1}}$ in the primary and secondary dilution tunnels respectively. With the steady-flow dilution tunnel system, dilution ratios vary as cookstove emissions fluctuate during testing. Temperatures at the filter sampling locations varied between 24–50 °C and 21–26 °C for the primary and secondary dilution tunnels respectively. After sampling, filters were stored in filter petri dishes at $-$20 °C to minimize volatilization and chemical reactions.

2.2 Measurements

From the PTFE and QF filter samples collected, three quantitative measurements were obtained on all samples for use in FTIR post-processing: gravimetric PM${}_{\mathrm{2.5}}$ mass, TOT OC–EC measurements, and GC–MS PAH measurements. PM${}_{\mathrm{2.5}}$ mass was determined by weighing the PTFE filters (Pall Gelman) gravimetrically with a microbalance (MC5 Micro Balance, Sartorius) before and after sampling. The FTIR spectra were gathered in transmission mode on the sampled PTFE filters. For FTIR analysis, the mid-infrared spectra in the 4000–400 cm${}^{-\mathrm{1}}$ range were obtained using a Bruker-Vertex 80 FTIR instrument equipped with an $\mathit{\alpha }$ deuterated lanthanum alanine doped triglycine sulfate (DLaTGS) detector, at a resolution of 4 cm${}^{-\mathrm{1}}$ and in transmission mode, averaging over 64 scans.

OC and EC on QF samples were measured using a thermal–optical transmittance instrument (TOT; Sunset Laboratory) and a revised NIOSH method 5040 . Blank PTFE and QF filters were also collected at the cookstove test facility, and the associated PM${}_{\mathrm{2.5}}$ mass, OC, and EC backgrounds were measured and subtracted from test samples. In order to make measurements on QF (EC, OC, GC–MS) and PTFE (FTIR, gravimetric) filters more comparable (i.e., to minimize the differences due to volatilization and adsorption artifacts for semivolatile aerosols), artifact correction was performed. For this purpose, the values measured on the QF back filters were subtracted from those on the QF samples in parallel to the PTFE filter.

Thermal-extraction GC–MS (TEx–GC–MS), as described by , was used to identify and quantify individual PAHs in sampled cookstove emissions for kerosene and red oak wood fuels. Briefly, a 0.4 cm${}^{\mathrm{2}}$ QF punch (or three punches for artifact filters and low-emission samples from LPG) was placed inside a glass tube that was pre-baked to 550 °C and spiked with 1 mL of an internal standard mixture containing deuterated PAH compounds. Following automated tube insertion into the oven unit, the sample was heated to 325 °C at a rate of 50 °C min${}^{-\mathrm{1}}$ and held for 11 min; 50 mL min${}^{-\mathrm{1}}$ of helium ($\mathrm{He}$) flowed over the sample. Desorbate was directed to a cryogenically cooled programmable temperature vaporization inlet at $-$85 °C, operating in splitless mode. The GC inlet was rapidly heated at 720 °C min${}^{-\mathrm{1}}$ to 325 °C. The sample was chromatographed on an ultra-low-bleed capillary column (DB-5, 30 m $\times$ 0.25 mm I.D. $\times$ 0.25 $\mathrm{\mu }$m film thickness) with $\mathrm{He}$ as the carrier gas (1 mL min${}^{-\mathrm{1}}$). The GC oven was temperature-programmed as follows: 65 °C for 10 min ramped to 325 °C at a rate of 10 °C min${}^{-\mathrm{1}}$ and held for 15 min.

Chromatographed compounds (listed in Sect. S2) were detected using an Agilent 5973 MS detector operating in selected ion monitoring mode. The internal standard method and a multi-level linear ($R^{\mathrm{2}}>\mathrm{0.9}$) calibration were used (0.1–1 ng) for PAH quantification. A mid-level calibration check was performed daily prior to sample analysis and was used as a continuing calibration in cases where measured and fixed concentrations were not within 20 %. Daily checks were within 20 % for most targets, even when replicated over months. Mid-level check recoveries for PAHs were within 105 % $\pm$ 33 % on average. PAHs below their detection limit were reported as “not detected”. Retention time shifts were negligible ($<$ 1 %) throughout the analysis. Target analyte validation was achieved using the retention times and isotopic fragment ratios exceeding a 3 : 1 signal-to-noise ratio. Carryover tests were performed by reheating the TEx sample/apparatus immediately following the initial extraction and then examining the GC–MS chromatogram for the presence of target compounds, which indicated an extraction efficiency of $>$ 98 %. Naphthalene was the only PAH detected (0.16 $\pm$ 0.11 ng) above its method detection limit (0.02 ng) in the blank filters. Similar to EC and OC, artifact correction was performed for PAHs by subtracting values of the quartz back filters from those of the parallel filters.

2.3 Post-processing

The following subsections describe or cite from previous publications that describe the post-processing methods applied to the FTIR spectra to identify and quantify FGs.

2.3.1 Baseline correction and blank subtraction

The FTIR spectra were baseline corrected using smoothing splines to remove the contribution of light scattering by the PTFE filter membrane and particles and absorption by carbonaceous material . For this work, the fitting procedure described by was extended to wavenumbers below 1500 cm${}^{-\mathrm{1}}$ to access additional regions of the spectra. To reduce the influence of the PTFE absorption peak in the region 1300–1000 cm${}^{-\mathrm{1}}$, a scaled version of a baseline-corrected blank filter spectrum was subtracted from each baseline-corrected sample spectrum . The blank spectrum used for subtraction was selected for each sample from a database of blank spectra (built from scans of similar batch of filters) using the closely matched intensity of the PTFE peak around 1150 cm${}^{-\mathrm{1}}$). The final spectrum is the difference between the baseline-corrected sample and the scaled baseline-corrected blank spectra (Sect. S3). This procedure allowed us to identify and quantify some organic FG absorptions such as the out-of-plane (OOP) aromatic $\mathrm{CH}$ bands that are otherwise partially masked by the PTFE absorption bands.

Graphitic carbon contributes to the mid-infrared spectra through weak absorption bands of carbon bonds in aromatic rings near 1600–1500 cm${}^{-\mathrm{1}}$ and electronic transition absorptions . Both have been implicated in conferring capabilities for quantification of EC content by FTIR spectrometry and statistical models in previous studies , and our current analysis further supports the value of the electronic transition in quantification. The values of the smoothing spline baselines fitted to each sample spectra at 4000 cm${}^{-\mathrm{1}}$ were regressed against the magnitude of corresponding EC and OC loadings (major components of PM${}_{\mathrm{2.5}}$ in this study). A relatively large and statistically significant coefficient for EC (2.2 times the coefficient of OC, $R^{\mathrm{2}}=\mathrm{0.72}$; Sect. S4) suggests that EC contributes significantly to the FTIR baseline of combustion aerosols and may be used for quantitative prediction of EC .

2.3.2 Quantification of functional groups

After determining the important FGs (by the variable importance in projection (VIP) scores method detailed in Sects. S5 and S6), their abundances were quantified using a multiple peak-fitting algorithm . Aliphatic $\mathrm{CH}$ (a$\mathrm{CH}$), aromatic $\mathrm{CH}$ (r$\mathrm{CH}$), alcohol $\mathrm{COH}$ (a$\mathrm{COH}$), carboxylic acid ($\mathrm{COOH}$), and non-acid carbonyl (na$\mathrm{CO}$) groups were quantified in this work. OC concentrations and OM : OC ratios were then calculated using FG abundances with minimal assumptions about the number of carbon atoms attached to each FG .

For the calibration of aromatic CH groups using the OOP bending mode, we used the 12 samples of anthracene (${\mathrm{C}}_{\mathrm{14}}{\mathrm{H}}_{\mathrm{10}}$) analyzed by for the aromatic $\mathrm{CH}$ stretching mode. Anthracene powder (Sigma-Aldrich) was dissolved in high-purity methanol (Fisher Scientific, Inc.), atomized with a constant output atomizer (TSI, Inc. model 3076) in nitrogen flow, and deposited on 37 mm PTFE filters (Pall Gelman) restricted to a 1 cm diameter collection spot with a custom-made PTFE mask . Areal mass loadings for these samples spanned a range between 26.8 and 1040 $\mathrm{\mu }$g cm${}^{-\mathrm{2}}$. The spectra acquired by FTIR were pre-treated according to Sect. , and the bending mode peak near 750 cm${}^{-\mathrm{1}}$ was used to build a calibration, as described by and . In this case, the peak height is used rather than the peak area, and the calibration coefficient (interpreted as molar absorptivity) was estimated to be 0.017 cm${}^{\mathrm{2}}$ mol${}^{-\mathrm{1}}$ of CH bond with a fit of $R^{\mathrm{2}}=\mathrm{0.93}$. The mass loading of PAHs was estimated from the quantified bonds assuming an effective C $/$ H molar ratio of 1.4 (similar to anthracene) to account for additional carbon atoms of PAHs associated with the measured aromatic CH bonds.

3 Results and discussion

In the following subsections, we first present overall OC, EC, and PM${}_{\mathrm{2.5}}$ measurements among different fuel types, test phases, and stoves. Thereafter, we present the FTIR spectra of particulate emissions qualitatively as well as those of unburned fuels. TOT OC measurements are then combined statistically with the FTIR spectra to identify influential FGs for OC. Finally, influential FGs are quantified to estimate OC, OM, and OM $/$ OC, as well as to compare with TOT OC and GC–MS PAH measurements.

3.1

OC, EC, and PM${}_{\mathrm{2.5}}$ emission factors

OC, EC, and PM${}_{\mathrm{2.5}}$ emission factors, expressed in grams of emission per megajoule of energy delivered to the pot, are shown in Fig. . We observe a significant variation across red oak fueled stoves in terms of emission factors (Fig. ). In particular, the three-stone fire and the Envirofit G3300 stove (natural draft) have relatively high emission factors of OC and EC accompanied by lower modified combustion efficiencies (MCEs; Sect. S7). On the other hand, gasifier stoves such as Eco Chula XXL have higher MCEs and around 10 times lower EC and OC emissions. Lower absorbances are also noticeable in the FTIR spectra of the Eco Chula XXL stove, especially in the CS and HS phases. OC and EC emission factors are slightly lower in the SIM phase compared to CS and HS phases. Nevertheless, the variations observed in the PM composition from red oak combustion across phases (characterized by elemental-carbon-to-total-carbon ratio, EC $/$ TC, where TC $=$ OC $+$ EC) are not substantial when compared to the variability in each phase (Figs.  and S6). The average EC $/$ TC for red oak combustion aerosols is 0.58 $\pm$ 0.19. This value is on the higher end of the values reported in previous studies on the emission factors of particles emitted from wood-burning cookstoves (0.07–0.64) .

Figure 3

Emission factors (mg MJ${}^{-\mathrm{1}}$) of gravimetric PM${}_{\mathrm{2.5}}$ and artifact-corrected TOT OC and EC, separated by fuel type and test phase (CS – cold start, HS – hot start, and SIM – simmering). Blue crosses show the median for each category.

[Figure omitted. See PDF]

Variation in emission factors across phases is more significant for charcoal combustion emissions compared to other fuels. The HS phase has the highest OC emission factor (Fig. ). The EC emission factor and the EC $/$ TC ratio increase significantly in the CS phase. The average EC $/$ TC ratios of charcoal combustion aerosols for the CS phase and all phases combined are 0.78 $\pm$ 0.23 and 0.30 $\pm$ 0.40 respectively. The variability in results was observed in charcoal combustion tests due to non-uniform fuel and differences in combustion conditions. Lump charcoal (not briquettes) was used for testing because it was representative of fuel usually used in low- to middle-income countries. Charcoal had non-uniform size and shape, and it was screened between 2.5 and 5.0 cm. Variation in the fuel bed packing due to the non-uniform pieces and variation in the carbonization of the charcoal can affect combustion and emissions. Kerosene was used as an accelerant to ignite the charcoal for all cold-start test phases, with a small amount of wood kindling used for the EcoZoom stove only, where red oak was $\sim$ 9 % of total fuel mass consumed. No accelerant was used during the hot-start or simmer test phases. Different combustion characteristics between stoves strongly influence emissions. For example, turbulence/mixing within the combustion chamber of a traditional charcoal stove is a key factor in the devolatilization of fuel and formation of organic PM . Field testing of traditional charcoal stoves finds relatively steady emissions of CO (and hence modified combustion efficiency) during the entire test period, while contributions of PM${}_{\mathrm{2.5}}$, black carbon (BC), and light scattering ($B_{\mathrm{sp}}$, $\mathit{\lambda }$ $=$ 635 nm, an optical-based proxy for EC) largely occur during the ignition period (e.g., 62 % and 67 % of BC and $B_{\mathrm{sp}}$ respectively occurred during the first 20 % of testing) . Therefore, both particle composition and emission rate change drastically during charcoal ignition, indicative of the highly variable process.

3.2 FTIR spectra and interpretation

Figure  exhibits distinct spectral profiles for PM${}_{\mathrm{2.5}}$ emitted from the combustion of different fuel types. The FTIR spectra of alcohol and LPG particulate emissions were omitted as they were noisy and had organic absorptions comparable to those of blank filters. This observation is corroborated by the negative or close-to-zero TOT OC measurements for alcohol and LPG emissions.

Figure 4

Average mid-infrared spectra of unburned fuels and their particulate emissions separated by source and test phase. The emission spectra are shown in terms of emission factors (absorbance divided by MJ energy delivered to the pot). Shaded bands show the mean spectrum $\pm$0.5 standard deviation. CS – cold start, HS – hot start, and SIM – simmering. Features in the region between 1000–1300 cm${}^{-\mathrm{1}}$, which have interferences from PTFE filters, have been omitted. The spectra from unburned fuels (blue lines), presented with arbitrary scaling, are taken from the literature: for charcoal, for kerosene, and for red oak.

[Figure omitted. See PDF]

The spectra of red oak combustion aerosols display a strong and broad band at 3500 cm${}^{-\mathrm{1}}$ related to a$\mathrm{COH}$ across all phases. This group is abundant in wood constituents (lignin, cellulose, and hemicellulose). In addition, medium a$\mathrm{CH}$ absorbances at 3000–2800 cm${}^{-\mathrm{1}}$, medium carbonyl $\mathrm{CO}$ absorbances at around 1700 cm${}^{-\mathrm{1}}$, and strong aromatic $\mathrm{C}=\mathrm{C}$ absorbances at 1600 cm${}^{-\mathrm{1}}$ are observed in the spectra of red oak combustion aerosols. The absorption band attributed to the lignin aromatic ring stretching vibration at 1515 cm${}^{-\mathrm{1}}$ is also prominent in several spectra , consistent with the existence of aromatic compounds with similar structure to monolignols, which are found in plants. Aromatic $\mathrm{CH}$ OOP bands at around 750 cm${}^{-\mathrm{1}}$ and occasionally aromatic stretching a$\mathrm{CH}$ bands at around 3050 cm${}^{-\mathrm{1}}$ are also visible in the FTIR spectra. The mean spectrum of the SIM phase has the weakest aromatic OOP band among all phases. Levoglucosan signatures described by are observed in several spectra for all three phases. Inorganic nitrate absorbances at 1400 and 830 cm${}^{-\mathrm{1}}$ are visible in some red oak samples, especially in CS and HS phases.

The mid-infrared spectrum of unburned kerosene fuel (from ) displays strong a$\mathrm{CH}$ peaks and weak r$\mathrm{CH}$ stretching (3050 cm${}^{-\mathrm{1}}$) absorbances. This is consistent with kerosene fuel being predominantly composed of hydrocarbons, the majority of which are straight-chain and cyclic with the rest being aromatic . An elemental analysis of unburned kerosene fuel (Sect. S8) also shows the insignificant contribution of elements other than $\mathrm{H}$ and $\mathrm{C}$ and a molar H $/$ C ratio of about 2 : 1, suggesting long-chain or cyclic alkanes.

In contrast, a$\mathrm{CH}$ absorbances are much weaker in the particulate emissions of kerosene combustion in all three phases, with high $\mathrm{CH}\mathrm{3}$/$\mathrm{CH}\mathrm{2}$ peak ratios that indicate branched or small hydrocarbons. Furthermore, r$\mathrm{CH}$ absorptions are more prominent in the particulate emissions, suggesting a significant formation of aromatic hydrocarbons and PAHs during the combustion. In the majority of spectra, moderate a$\mathrm{COH}$ absorbances are observed. In several samples taken from the emissions of the kerosene wick-type cookstove, a sharp $\mathrm{CO}$ carbonyl peak at 1695 cm${}^{-\mathrm{1}}$ is observed (Sect. S9). This peak is accompanied by a broad peak at 3400–2400 cm${}^{-\mathrm{1}}$ (with doublets at 2600 and 2400 cm${}^{-\mathrm{1}}$ attributed to the dimerized carboxylic acid $\mathrm{OH}$), suggesting high abundances of carboxylic acids . The carbonyl peak with a relatively low frequency and the high abundance of r$\mathrm{CH}$ indicate the existence of aromatic acids. Aromatic signatures appear to be more prominent in the CS and HS phases.

The charcoal spectrum (from ) has weak a$\mathrm{CH}$ and carbonyl $\mathrm{CO}$ absorbances, and strong aromatic $\mathrm{C}=\mathrm{C}$ and a$\mathrm{COH}$ absorbances. The weak a$\mathrm{CH}$ peaks are consistent with the low hydrogen content of the fuel (Sect. S8) However, the mid-infrared spectra of particulate emissions from charcoal combustion show strong a$\mathrm{CH}$ peaks (Fig. ). The a$\mathrm{CH}$ peaks are especially prominent in the HS phase in which charcoal is added to the hot fuel bed (Fig. S1). In addition, the carbonyl $\mathrm{CO}$ peak at 1700 cm${}^{-\mathrm{1}}$ emerges in the charcoal combustion spectra in the HS phase, while being absent in the charcoal spectrum itself. This observation suggests the formation of carbonyls during charcoal pyrolysis and burning. Charcoal combustion in the cold-start (CS) phase has the highest EC emission factor (Fig. ), concurrent with prominent $\mathrm{C}=\mathrm{C}$ absorbances at around 1600 cm${}^{-\mathrm{1}}$ in the FTIR spectra. The ratio of the aromatic $\mathrm{C}=\mathrm{C}$ peak (1600 cm${}^{-\mathrm{1}}$) to aromatic $\mathrm{CH}$ (750 cm${}^{-\mathrm{1}}$) is higher for charcoal-burning aerosols compared to other fuels, suggesting that aromatic compounds are poor in hydrogen ($=\mathrm{C}-\mathrm{H}$ groups).

3.3 Quantified functional groups from FTIR spectra

Organic functional groups aliphatic $\mathrm{CH}$ (a$\mathrm{CH}$), aromatic $\mathrm{CH}$ (r$\mathrm{CH}$), alcohol $\mathrm{COH}$ (a$\mathrm{COH}$), carboxylic acid ($\mathrm{COOH}$), and non-acid carbonyl (na$\mathrm{CO}$) were quantified by peak fitting to mid-infrared. The results of peak fitting are shown in Fig.  in terms of OM emission factors and OM $/$ OC ratios (FG emission factor values and corresponding absorption bands from , , and are tabularized in Sect. S10). OC estimated by FTIR from the abundances of FGs (“FG OC”) is highly correlated with TOT OC measurements ($R^{\mathrm{2}}=\mathrm{0.83}$; Fig. S14). However, FG OC underpredicts TOT OC by around 40 %, although artifact correction has been performed for TOT OC using QF back filters. This underprediction can be attributed to the imperfect correction of quartz adsorption artifacts, volatilization of compounds from particles on PTFE filters, uncharacterized FGs, uncertainty in FG absorption coefficients, underprediction of the fractional carbon associated with each FG, and the operationally defined EC and OC separation threshold for TOT. Volatilization losses off filters (following a denuder) for urban ambient samples have been reported to be on the order of 10 % , though the amount may be different for fresh emissions that can contain substances that can revolatilize . Underprediction in OC due to uncharacterized FGs is reported to be on the order of 8 %–20 % considering the range of structures in compounds expected in OM . OC estimates by TOT have been reported to be higher than that by reflectance correction by 0 %–35 % due to the charring profile through the filter . The magnitude of each contribution across samples can vary substantially. A combination of these factors can lead to the overall discrepancy observed in this study, which is on the higher end relative to comparisons of FTIR OC or OM to different techniques in previous studies e.g.,. Nonetheless, the consistent mass recovery permits us to make systematic comparisons regarding the OM composition using FG analysis.

Figure 5

(a–c) OM emission factors calculated from mid-infrared spectroscopy, separated by functional group contribution, and averaged over each phase. (d–f) OM $/$ OC ratios calculated from mid-infrared spectroscopy and separated by functional group contribution. CS – cold start, HS – hot start, and SIM – simmering.

[Figure omitted. See PDF]

The concentration of r$\mathrm{CH}$ was estimated in this work using the OOP band (750 cm${}^{-\mathrm{1}}$), which is more distinguishable than the stretching-mode vibration (3050 cm${}^{-\mathrm{1}}$) previously used. The OOP peak has a comparatively higher absorption coefficient and does not overlap significantly with other group frequencies as does the stretching mode peak (e.g., with the ammonium $\mathrm{NH}$ stretch). Peaks of the two vibrational modes exhibit a strong relationship (Fig. S11), but the OOP peak is expected to have higher sensitivity due to the aforementioned reasons. Contrary to the peak at 3050 cm${}^{-\mathrm{1}}$, the peak at 1600 cm${}^{-\mathrm{1}}$ attributed to aromatic $\mathrm{C}=\mathrm{C}$ is not highly correlated with the OOP peak (Fig. S12), especially for red oak burning aerosols – likely due to high abundance of lignin pyrolysis products substituted rings. However, a qualitative relationship between r$\mathrm{CH}$ and TOT EC concentrations, dependent on fuel type, can be observed (Fig. S13).

Figure 6

Scatter plot of aromatic $\mathrm{CH}$ concentration estimated using the peak at 750 cm${}^{-\mathrm{1}}$ and GC–MS total PAH concentration.

[Figure omitted. See PDF]

The estimates of r$\mathrm{CH}$ using this OOP bend are highly correlated ($R^{\mathrm{2}}=\mathrm{0.84}$; slope $=$ 19.6) with the total PAH concentration by GC–MS measured for kerosene and red oak wood fuels (Fig. ). The VIP scores of the GC–MS total PAH concentration regressed against mid-infrared absorbances also indicate the importance of the 750 cm${}^{-\mathrm{1}}$ band for PAHs (Fig. ). The $\mathrm{C}=\mathrm{C}$ band near 1500–1600 cm${}^{-\mathrm{1}}$ is also indicated as a predictive feature but exhibits less selectivity toward PAHs since contributions from other aromatic structures present – such as graphitic carbon and lignin – are also present. The magnitude of PAHs and aromatic estimated using the OOP band at 750 cm${}^{-\mathrm{1}}$ is almost an order of magnitude higher than that measured by GC–MS, probably due to this band accounting for other unmeasured aromatic and PAH compounds. While our calibration for the total PAH is based on a single compound, variations in absorption coefficients on the order of 30 % for the same FGs across different compounds have been reported . Furthermore, the C $/$ H ratio assumed (1.4) for calculation of PAH concentrations by FTIR (Sect. ) is a conservative one, considering that the range of C $/$ H values for compounds measured by GC–MS in this study was 1.0–2.0 (Sect. S2), and the highest abundance was found for compounds with C $/$ H greater than 1.44 (e.g., pyrene, fluoranthene, benzo-a-pyrene). The adoption of higher values for this ratio leads to higher estimates of PAH, OM mass, and proportion of PAH in estimated OM; the value of this and the absorption coefficient can be further constrained in future studies with additional experiments and inverse modeling approaches e.g.,. In summary, the apparent difference in magnitude of FTIR and GC–MS estimates of PAH abundance is beyond the levels of our anticipated uncertainty and likely stems from the difference in approach between FG and molecular level analysis toward quantification of mass concentrations .

Figure 7

VIP scores of GC–MS sum of PAHs regressed against the FTIR spectra.

[Figure omitted. See PDF]

Summarizing the FTIR composition analysis, red oak combustion aerosols have the highest mean OM emissions factors for all phases (Fig. ), consistent with TOT OC measurements (Fig. ). For all three phases, a$\mathrm{COH}$, a$\mathrm{CH}$, and r$\mathrm{CH}$ groups constitute the majority of OM. Among different phases, the simmering (SIM) phase has a slightly lower OM emission. The r$\mathrm{CH}$ group abundance is significantly lower in the SIM phase. The lower concentration of this group in the SIM phase is also observed for other fuel types. This is also reflected in the higher OM $/$ OC ratio of this phase compared to other phases. The average OM $/$ OC ratio of red oak combustion aerosols is estimated to be around 1.7.

Kerosene combustion has the lowest average OM emissions factors compared to other fuels in all phases (Fig. ; around 4 times lower than red oak). Interestingly, while kerosene OC and EC is not necessarily higher than others (Fig. ), its proportion of aromatic $\mathrm{CH}$ (r$\mathrm{CH}$) is higher (Fig. ). No clear difference is observed between the mean OM emission factor among different phases. The r$\mathrm{CH}$ is estimated to be the most prominent FG for the kerosene burning aerosols followed in order by a$\mathrm{COH}$, a$\mathrm{CH}$, and $\mathrm{COOH}$. The average OM $/$ OC ratio is 1.8 for the kerosene aerosols. Like red oak, the SIM phase has the highest OM $/$ OC ratio due to a higher abundance of $\mathrm{COOH}$ (more oxygenated) and a lower abundance of r$\mathrm{CH}$ (likely due to more complete combustion).

Charcoal-burning aerosols have average OM emission factors slightly lower than those of red oak combustion (Fig. ). The a$\mathrm{CH}$ group is the most important FG for charcoal-burning aerosols, constituting up to 50 % of OM. The a$\mathrm{COH}$ and r$\mathrm{CH}$ are the most abundant groups after a$\mathrm{CH}$. Other FGs exist in negligible amounts in charcoal-burning aerosols. The average OM $/$ OC ratio for charcoal-burning aerosols is 1.6, slightly lower than that of other fuels. Like other fuel types, the SIM phase has the highest OM $/$ OC ratio and the lowest abundance of aromatics.

There is a dearth of estimates of OM $/$ OC ratios from cookstove emissions for direct comparison. The similarity in the range of OM $/$ OC ratios (1.6–1.8) between fossil fuel and red oak combustion in this work stands in slight contrast to differences observed in a previous study comparing primary OM from coal combustion and wood burning in furnaces, where average OM $/$ OC ratios were 1.4 and 1.6 respectively, which were similar to AMS . The current values are higher than reported by AMS for submicron HOA (1.3–1.5) though closer to the range of laboratory-generated and inverse-modeled BBOA ($>$ 1.5) . OM $/$ OC estimates from FTIR can be biased high if some unfunctionalized carbon is not considered in the calculation ; in that case, the OM $/$ OC would reflect the ratio for polyfunctional carbon atoms that are extracted by our current FTIR calibrations. In the study by , the FTIR OM was estimated to be 30 % higher than AMS measurements without collection efficiency correction, while FTIR OC is underestimated by about 40 % compared to TOT OC in this work. proposed an approach to find parameters for estimation of FTIR OC (including calibration coefficients and undetected carbon fraction) that were most consistent with the observed TOR OC concentrations in collocated ambient measurements. These model parameters were then used to obtain revised estimates of OM $/$ OC, which resulted in lower OM $/$ OC estimates as the original FTIR OC estimates underpredicted the TOR OC concentrations by approximately 40 %. Such an approach can also be considered for further investigation of cookstove primary emissions. Nonetheless, the bias of TOT OC is systematically similar across fuel types in this work, so the relative differences among them reported here are likely to be consistent with respect to this source of bias. Differences in absorptivities for the same functional group found in different compounds across sources may exist, but they are not accounted for in this study. More studies in this area are warranted given the difficulty in quantifying OM $/$ OC using various techniques and a lack of definitive reference methods. Molecular methods sample a small subset of molecules present , AMS relies on calibrations to a set of selected representative compounds to adjust for ionization losses , reconstructed fine mass regression is subject to compounding analytical errors , and the estimation of OM through thermo-gravimetric analysis is prohibitively labor-intensive (and is also subject to compounding analytical errors).

Previous studies correlate aromatics and PAHs with mutagenicity and carcinogenicity . Our analysis shows that these compounds are abundant even in relatively clean fuels (i.e., with low emission factors) like kerosene, which has a magnitude of emitted aerosol PAH as high as charcoal, suggesting its harmfulness. This observation, along with the highly oxygenated FGs present in kerosene OM, is consistent with previous studies providing some evidence that kerosene emissions may impair lung function and increase infectious illness, asthma, and cancer risks .

4 Conclusions

This paper introduces FTIR as a measurement technique that can provide new insights into the organic composition of aerosol emissions from cookstoves, in which variations in composition and overall emissions due to the fuel type and operational phase of the cookstove are evaluated. The FTIR analysis is applied directly to filters collected for gravimetric mass analysis and does not require an additional sampling line. The OM composition in terms of oxygenated functional groups – carboxylic acids, carbonyls, and alcohols – and PAHs varies substantially across fuel types and, in some cases, the operational phase of the stove. Additionally, a qualitative comparison of emitted OM to the composition of the fuel is demonstrated through comparison of the aerosol spectra to the spectra of the unburned fuel. The overall organic carbon estimated by FTIR is approximately 60 % of that estimated by thermal–optical transmittance, with an $R^{\mathrm{2}}$ of 0.82. This mass recovery is on the low end of previously reported OC and OM comparisons against thermal–optical methods or aerosol mass spectrometry and may indicate the additional sampling artifacts in emissions studies, the greater presence of carbon associated with uncharacterized functional groups, or skeletal carbon atoms that are missed by FTIR. A new development introduced in this paper is the quantification of PAH concentrations – particularly important in fresh emissions – based on the OOP bending absorption peak of aromatics by FTIR, which is more prominent than the stretching vibrations observed in the functional group region of the spectrum. The estimate of PAH hydrocarbon mass loadings by FTIR is found to be 5-fold greater than that summed up from 16 PAHs analyzed by GC–MS, likely because FTIR estimates account for unmeasured PAH compounds in the samples. Thus FTIR can potentially provide an additional dimension of information for toxicity studies of emitted aerosols.

Data availability

Data for this work can be found at 10.5281/zenodo.10970006 and 10.5281/zenodo.4882967 .

The supplement related to this article is available online at: https://doi.org/10.5194/amt-17-2401-2024-supplement.

Author contributions

EYL, AMD, MDH, and ST conceived of the project and manuscript. GS performed the filter sample collection and gravimetric analysis, WTP directed the OC-EC and PAH measurements and analysis, and EYL performed the FTIR measurements. EYL, GS, WMC, JJJ, WTP, and ST contributed further data curation. AMD, JJJ, MDH, LMR, and ST provided resources and/or acquired financial support for the project. EYL, AY, and ST provided and implemented code and supporting algorithms and code components and prepared data visualization. EYL, AMD, MDH, and ST provided oversight and leadership responsibility for research planning and execution, including mentorship. EYL, AY, WMC, MDH, and ST contributed to the initial draft, and all authors contributed to the review and editing of the written manuscript.

Competing interests

The contact author has declared that none of the authors has any competing interests.

Disclaimer

The views expressed in this article/chapter are those of the authors and do not necessarily represent the views or policies of the U.S. Environmental Protection Agency. Mention of trade names or commercial products does not constitute endorsement or recommendation for use. Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.

Acknowledgements

The authors thank the U.S. Environmental Protection Agency Office of Air Quality Planning and Standards for their administrative support and the Office of Research and Development for Quality Assurance support.

Financial support

This research has been supported by the Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung (grant no. 200021_172923).

Review statement

This paper was edited by Rebecca Washenfelder and reviewed by two anonymous referees.