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			<titleStmt><title level='a'>An intercomparison study of four different techniques for measuring the chemical composition of nanoparticles</title></titleStmt>
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				<publisher></publisher>
				<date>01/01/2023</date>
			</publicationStmt>
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				<bibl> 
					<idno type="par_id">10437056</idno>
					<idno type="doi">10.5194/acp-23-6613-2023</idno>
					<title level='j'>Atmospheric Chemistry and Physics</title>
<idno>1680-7324</idno>
<biblScope unit="volume">23</biblScope>
<biblScope unit="issue">11</biblScope>					

					<author>Lucía Caudillo</author><author>Mihnea Surdu</author><author>Brandon Lopez</author><author>Mingyi Wang</author><author>Markus Thoma</author><author>Steffen Bräkling</author><author>Angela Buchholz</author><author>Mario Simon</author><author>Andrea C. Wagner</author><author>Tatjana Müller</author><author>Manuel Granzin</author><author>Martin Heinritzi</author><author>Antonio Amorim</author><author>David M. Bell</author><author>Zoé Brasseur</author><author>Lubna Dada</author><author>Jonathan Duplissy</author><author>Henning Finkenzeller</author><author>Xu-Cheng He</author><author>Houssni Lamkaddam</author><author>Naser G. Mahfouz</author><author>Vladimir Makhmutov</author><author>Hanna E. Manninen</author><author>Guillaume Marie</author><author>Ruby Marten</author><author>Roy L. Mauldin</author><author>Bernhard Mentler</author><author>Antti Onnela</author><author>Tuukka Petäjä</author><author>Joschka Pfeifer</author><author>Maxim Philippov</author><author>Ana A. Piedehierro</author><author>Birte Rörup</author><author>Wiebke Scholz</author><author>Jiali Shen</author><author>Dominik Stolzenburg</author><author>Christian Tauber</author><author>Ping Tian</author><author>António Tomé</author><author>Nsikanabasi Silas Umo</author><author>Dongyu S. Wang</author><author>Yonghong Wang</author><author>Stefan K. Weber</author><author>André Welti</author><author>Marcel Zauner-Wieczorek</author><author>Urs Baltensperger</author><author>Richard C. Flagan</author><author>Armin Hansel</author><author>Jasper Kirkby</author><author>Markku Kulmala</author><author>Katrianne Lehtipalo</author><author>Douglas R. Worsnop</author><author>Imad El Haddad</author><author>Neil M. Donahue</author><author>Alexander L. Vogel</author><author>Andreas Kürten</author><author>Joachim Curtius</author>
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			<abstract><ab><![CDATA[Abstract. Currently, the complete chemical characterization of nanoparticles(<100nm) represents an analytical challenge, since these particlesare abundant in number but have negligible mass. Several methods forparticle-phase characterization have been recently developed to betterdetect and infer more accurately the sources and fates of sub-100nmparticles, but a detailed comparison of different approaches is missing.Here we report on the chemical composition of secondary organic aerosol(SOA) nanoparticles from experimental studies of α-pinene ozonolysisat −50, −30, and −10∘C and intercompare the results measured by differenttechniques. The experiments were performed at the Cosmics Leaving OUtdoorDroplets (CLOUD) chamber at the European Organization for Nuclear Research(CERN). The chemical composition was measured simultaneously by fourdifferent techniques: (1) thermal desorption–differential mobility analyzer(TD–DMA) coupled to a NO3- chemical ionization–atmospheric-pressure-interface–time-of-flight (CI–APi–TOF) massspectrometer, (2) filter inlet for gases and aerosols (FIGAERO) coupled to anI− high-resolution time-of-flight chemical ionization mass spectrometer(HRToF-CIMS), (3) extractive electrospray Na+ ionizationtime-of-flight mass spectrometer (EESI-TOF), and (4) offline analysis offilters (FILTER) using ultra-high-performance liquid chromatography (UHPLC)and heated electrospray ionization (HESI) coupled to an Orbitraphigh-resolution mass spectrometer (HRMS). Intercomparison was performed bycontrasting the observed chemical composition as a function of oxidationstate and carbon number, by estimating the volatility and comparing thefraction of volatility classes, and by comparing the thermal desorptionbehavior (for the thermal desorption techniques: TD–DMA and FIGAERO) andperforming positive matrix factorization (PMF) analysis for the thermograms.We found that the methods generally agree on the most important compoundsthat are found in the nanoparticles. However, they do see different parts ofthe organic spectrum. We suggest potential explanations for thesedifferences: thermal decomposition, aging, sampling artifacts, etc. Weapplied PMF analysis and found insights of thermal decomposition in theTD–DMA and the FIGAERO.]]></ab></abstract>
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<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1">Introduction</head><p>So far there is no well-established instrument and technique to measure the complete chemical composition of ultrafine (&lt; 100 nm) secondary organic aerosol (SOA) particles. However, several analytical techniques have recently been developed in order to better advance our understanding on their chemistry. Techniques that are capable of measuring sub-30 nm particles include the Volatile Aerosol Component Analyzer (VACA) <ref type="bibr">(Curtius et al., 1998)</ref>, thermal desorption-chemical ionization mass spectrometry (TD-CIMS) <ref type="bibr">(Voisin et al., 2003)</ref>, the Nano Aerosol Mass Spectrometer (NAMS) <ref type="bibr">(Wang et al., 2006)</ref>, the aerosol timeof-flight mass spectrometer <ref type="bibr">(Laitinen et al., 2009)</ref>, the inlet for the size-resolved collection of aerosols <ref type="bibr">(Phares and Collier, 2010)</ref>, the Chemical Analyzer for Charged Ultrafine Particles (CAChUP) <ref type="bibr">(Gonser and Held, 2013)</ref>, electrostatic precipitation-electrospray ionization mass spectrometry (EP-ESI-MS) <ref type="bibr">(He et al., 2015)</ref>, droplet-assisted inlet ionization (DAII) <ref type="bibr">(Horan et al., 2017)</ref>, and online aerosol chemical characterization by the extractive electrospray ionization-ultra-high-resolution mass spectrometer (EESI-Orbitrap) <ref type="bibr">(Lee et al., 2020)</ref>. Single-particle analysis by mass spectrometry methods based on aerodynamics, light scattering, and laser desorption ionization are suitable for particles with larger sizes. These methods include, for example, the aerosol mass spectrometer (AMS) described in <ref type="bibr">Jayne et al. (2000)</ref> and the suite of single-particle methods described in the review by <ref type="bibr">Bzdek et al. (2012)</ref>. The detection of particles with d &lt; 100 nm using these techniques becomes difficult because the scattering efficiency decreases when the particle diameter becomes smaller.</p><p>Using the Cosmics Leaving OUtdoor Droplets (CLOUD) chamber at the European Organization for Nuclear Research (CERN), we simultaneously used four different techniques for measuring the chemical composition of ultrafine particles and intercompare the results:</p><p>1. thermal desorption-differential mobility analyzer (TD-DMA) coupled to a NO - 3 chemical ionizationatmospheric-pressure-interface-time-of-flight (CI-APi-TOF) mass spectrometer <ref type="bibr">(Wagner et al., 2018)</ref>, 2. filter inlet for gases and aerosols (FIGAERO) coupled to an I -high-resolution time-of-flight chemical ionization mass spectrometer (HRToF-CIMS) <ref type="bibr">(Lopez-Hilfiker et al., 2014)</ref>, 3. extractive electrospray Na + ionization time-of-flight mass spectrometer (EESI-TOF) <ref type="bibr">(Lopez-Hilfiker et al., 2019)</ref>, and 4. offline analysis of filters (FILTER) using ultra-highperformance liquid chromatography (UHPLC) and heated electrospray ionization (HESI) coupled to an Orbitrap high-resolution mass spectrometer (HRMS) <ref type="bibr">(Ungeheuer et al., 2021)</ref>.</p><p>None of the techniques presented in this work represent the perfect instrument. In fact, a perfect instrument would be the one that is able to quantitatively measure all the hundreds of organic compounds that are present not only in the newly formed particles in the lab, but also in aerosol particles present in the ambient, i.e., with larger particles being present as well and at low mass concentration of the ultrafine particles. A perfect instrument should also be able to identify the molecular structures (including their isomeric and spatial configuration) at high time resolution and in real time. Such an ideal instrument does not exist, and at present, a combination of techniques is required for a more complete characterization of SOA <ref type="bibr">(Hallquist et al., 2009)</ref>.</p><p>In order to compare the techniques mentioned above and to gain insights into their limitations (due to decomposition during evaporation, different ionization techniques, etc.), we performed &#945;-pinene ozonolysis experiments at -50, -30, and -10 &#8226; C. For the experiments at -50 and -30 &#8226; C TD-DMA, FIGAERO, and EESI-TOF were intercompared, while for the experiment at -10 &#8226; C FILTER, FIGAERO, and EESI-TOF were intercompared. We carried out the indepth intercomparison by (a) comparing the observed composition as a function of oxidation state and carbon number; <ref type="bibr">(b)</ref> estimating the volatility and comparing the fraction of ultralow-volatility (ULVOCs), extremely low-volatility (ELVOCs), low-volatility (LVOCs), semi-volatile (SVOCs), and intermediate-volatility (IVOCs) organic compounds; and (c) comparing the thermograms (for the thermal desorption techniques: TD-DMA and FIGAERO) and performing positive matrix factorization (PMF) analysis on the thermograms.</p><p>Because the four techniques provide chemical composition, and more specifically the carbon, hydrogen, and oxygen content (CHO), we determined the carbon oxidation state (OSc), which is a metric for the degree of the oxidation of organic species in the atmosphere <ref type="bibr">(Kroll et al., 2011)</ref>. It is calculated based on the ratios O : C and H : C and is useful to describe organic mixtures upon oxidation processes. In addition, we estimated the volatility (as introduced by <ref type="bibr">Donahue et al., 2011, and</ref><ref type="bibr">modified by Stolzenburg et al., 2018)</ref> and determined the volatility classes to which the detected compounds belong. Regarding the thermal desorption methods (TD-DMA and FIGAERO) we investigated the thermal behavior of the detected species. Both instruments first collect particles, and subsequently the particles are evaporated in order to transfer their constituents to the gas phase. When a temperature ramp is applied, the species that are adsorbed on the surface gradually desorb (as represented on a thermogram). In order to evaluate whether the thermal desorption methods lead to significant decomposition during evaporation, we applied a method called positive matrix factorization <ref type="bibr">(Paatero and Tapper, 1994;</ref><ref type="bibr">Buchholz et al., 2020)</ref>, in which a data set matrix is expressed in terms of the sum of factor matrices and a residual matrix. Thermal decomposition of FIGAERO particle-phase data has been reported previously. D' <ref type="bibr">Ambro et al. (2019)</ref> observed that some of the major components of IEPOX (isoprene-derived epoxydiol) in SOA such as C 5 H 10 O 3 and C 5 H 12 O 4 are likely artifacts of thermal decomposition. <ref type="bibr">Lopez-Hilfiker et al. (2015)</ref>, <ref type="bibr">Stark et al. (2017)</ref>, and <ref type="bibr">Wang and Hildebrandt Ruiz (2018)</ref> have addressed the importance of considering thermal decomposition for assessing the chemical composition and volatility properties of SOA in techniques in which the aerosol is heated before or during the analysis. In this study, we evaluate thermal decomposition of TD-DMA samples for the first time and intercompare the results with FIGAERO.</p><p>Lastly, we present an overview of the advantages and disadvantages for the different methods. All methods presented here agreed on the most dominant compounds that are found in the nanoparticles. Nevertheless, they do see different parts of the organic spectrum. Therefore, the techniques are complementary. The four techniques described in this work are feasible for measuring sub-100 nm SOA particles and represent an important analytical development.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2">Methods</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.1">Experimental approach</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.1.1">The CLOUD chamber experiment</head><p>We conducted experiments in the CLOUD chamber at CERN to study pure biogenic new particle formation (NPF) without the presence of nitrogen oxides (NO x ). The CLOUD chamber is a stainless-steel cylinder with a volume of 26.1 m 3 and has been extensively described by <ref type="bibr">Kirkby et al. (2011)</ref> and <ref type="bibr">Duplissy et al. (2016)</ref>. To create the particles, NPF was induced by continuously adding &#945;-pinene and ozone into the chamber. The monoterpene concentration was regulated by an evaporation source, in which dry nitrogen (N 2 ) passes through an evaporator containing liquid &#945;-pinene at a precisely controlled temperature. Ozone was produced by exposing cryogenic O 2 to UV light and was introduced directly into the chamber via a separate line. The relative humidity was adjusted with a temperature-controlled Nafion humidifier using ultrapure Millipore water. All the precursor gases were homogenously mixed in the chamber by two magnetically driven Teflon fans placed at the top and at the bottom of the chamber. The temperature was kept constant by an insulated thermal housing, which surrounds the chamber. The &#945;-pinene mixing ratio was measured by a proton transfer reaction time-of-flight (PTR-TOF) mass spectrometer <ref type="bibr">(Graus et al., 2010;</ref><ref type="bibr">Breitenlechner et al., 2017)</ref>, whereas ozone was measured by a TEI 49C ozone analyzer (Thermo Environmental Instruments). The experiments relevant for this work were performed at -50, -30, and -10 &#8226; C. The &#945;-pinene mixing ratio ranged between 1 and 8 ppbv, and ozone was approximately 100 ppbv.</p><p>Table <ref type="table">1</ref> presents the most important features for the instruments used in this work. We categorize the techniques according to certain criteria: continuous-or discontinuousoperation mode, evaporation method, phase measured, ionization technique, reagent ion, target substances, occurrence of significant thermal decomposition, and whether the technique allows size-resolved analysis of aerosol particles to be performed.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.1.2">Thermal desorption-differential mobility analyzer</head><p>(TD-DMA) coupled to a NO - 3 chemical ionizationatmospheric-pressure-interface-time-of-flight (CI-APi-TOF) mass spectrometer</p><p>The TD-DMA coupled to a NO - 3 CI-APi-TOF analyzes the chemical composition of nanoparticles in a semicontinuous mode of operation. The design and characterization have been reported by <ref type="bibr">Wagner et al. (2018)</ref>. This method allows gas-and particle-phase measurements using the same ionization technique. Individual results of gas-and particlephase comparison of the same chemical system as in this study were reported in <ref type="bibr">Caudillo et al. (2021)</ref>. While the gasphase measurement is taking place with the CI-APi-TOF mass spectrometer, the TD-DMA samples particles from the chamber. The TD-DMA can perform size-resolved and nonsize-resolved measurements. In any case, the particles are first charged by an X-Ray source and then transferred to the differential mobility analyzer (DMA) unit. When a sizeresolved measurement is desired, a specific voltage is applied to the central electrode inside the DMA unit. Subsequently, a sheath flow will carry only particles with specific electrical mobility and will conduct them through the DMA. In contrast, during a non-size-resolved measurement, no voltage to the central electrode and no sheath flow are applied, and a fraction of the particles charged by the X-ray source will pass through the DMA unit. For the experiments reported in the present study, we performed non-size-resolved measurements in order to maximize the mass collected and to be comparable to the other methods that do not perform size selection.</p><p>The particle collection takes place by electrostatic precipitation on a platinum-rhodium (90 : 10) filament placed inside the central electrode. After a certain collection time (&#8764; 3 h for the experiment at -30 &#8226; C and &#8764; 5 h for the experiment at -50 &#8226; C), an electric current is applied to the filament, which causes its direct heating. We estimate based on the filament resistance that the temperature gradually increased up to approximately 600 &#8226; C in a period of &#8764; 1 min (details of the heating curve are discussed in Sect. 3.2).</p><p>The vapors that evaporate from the heated particles are carried by an N 2 flow to the nitrate CI-APi-TOF for chemical composition analysis. For chemical ionization of the vapors, nitrate reagent ions (HNO 3 ) n NO - 3 with n = 0-2 are created by a corona discharge <ref type="bibr">(K&#252;rten et al., 2011;</ref><ref type="bibr">K&#252;rten et al., 2014)</ref>. Some of the vapor molecules are ionized and subsequently detected by the APi-TOF mass spectrometer. A second heating cycle of the particle-collecting filament is performed afterwards (without particle collection) in order to estimate the instrumental background due to the heating of the inlet line; this enables a more accurate determination of particle constituents. The particle constituents are estimated by subtracting the second heating from the first heating. Besides the particle and background estimations, a second heating up to &#8764; 600 &#8226; C ensures that the filament is clean and avoids memory effects for the next measurement. With the nitrate ionization technique, sulfuric acid <ref type="bibr">(Jokinen et al., 2012)</ref>, iodic acid <ref type="bibr">(He et al., 2021)</ref>, methane sulfonic acid <ref type="bibr">(Shen et al., 2022)</ref>, and highly oxygenated molecules <ref type="bibr">(Kirkby et al., 2016;</ref><ref type="bibr">Simon et al., 2020</ref>) can be detected.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.1.3">Filter inlet for gases and aerosols (FIGAERO)</head><p>coupled to an I -high-resolution time-of-flight chemical ionization mass spectrometer (HRToF-CIMS)</p><p>FIGAERO coupled to an I -HRToF-CIMS was first described by <ref type="bibr">Lopez-Hilfiker et al. (2014)</ref> and optimized for CLOUD operation conditions by <ref type="bibr">Wang et al. (2020)</ref>. FI-GAERO uses a multi-port to measure in alternation both the gas and particle phases following the same general procedure as the TD-DMA-CI-APi-TOF. While the gas phase is analyzed, particle collection takes place on a polytetrafluoroethylene (PTFE) filter, and after a certain collection time (in this study 15 min), the filter is automatically moved into the ion-molecule reactor and exposed to a pure N 2 gas flow.</p><p>The N 2 flow is gradually heated to evaporate the particles by thermal desorption using a temperature-programmed heating curve. For the measurements reported in this study, the temperature was slowly ramped from room temperature up to 150 &#8226; C in approximately 15 min (an example of the heating curve is discussed in Sect. 3.2). When the heating cycle ends a new collection starts, and the process repeats. Thus, the 15 min collection period is followed by a 15 min desorption period, which implies two collections per hour (resulting in a resolution of 30 min). The detection technique is based on iodide-molecule adduct ionization. Iodine ions I -, I - 3 , and (H 2 O)I -are generated from a solution of methyl iodide (CH 3 I) and a Po-210 ion source <ref type="bibr">(Lee et al., 2014)</ref>. With this soft-ionization technique, the FIGAERO-HRToF-CIMS can detect intermediately oxygenated organic molecules <ref type="bibr">(Wang et al., 2020;</ref><ref type="bibr">Stolzenburg et al., 2018;</ref><ref type="bibr">Lopez-Hilfiker et al., 2016)</ref>, organosulfates, and inorganic acids such as sulfuric acid and nitric acid. a TD-DMA can take both size-resolved and non-size-resolved measurements. For this work, non-size-resolved measurements were chosen in order to maximize the mass collected and to intercompare with the particle-phase instruments. b In this work, only the particle-phase measurements are reported. c Gas and particle phases can be measured by using the dual EESI-TOF configuration.</p><p>2.1.4 Extractive electrospray Na + ionization time-of-flight mass spectrometer (EESI-TOF)</p><p>The extractive electrospray ionization time-of-flight mass spectrometer <ref type="bibr">(Lopez-Hilfiker et al., 2019</ref>) is a technique used for online particle-phase measurements without batch collection. This technique aims to provide the chemical composition of organic particles in real time (1 s). It is also possible to measure the gas phase by using the dual configuration <ref type="bibr">(Lee et al., 2022)</ref>. In the beginning of the sampling process, the aerosol sample passes through the inlet line, where a carbon denuder is located to remove the gas-phase molecules.</p><p>The particles then collide with electrospray droplets, and the soluble components are extracted and ionized. Then, solvent evaporation occurs in a heated stainless-steel capillary, leading to Coulomb fissioning and/or direct ion desorption. Finally, ions enter a time-of-flight mass spectrometer. The EESI-TOF here uses an electrospray solution of pure water doped with 100 ppm NaI and is running in the positiveion mode. This enables the measurements of SOA species as adducts with Na + . With this ionization method, most organic compounds that are relevant for atmospheric SOA particles can be analyzed, such as intermediately oxygenated organic molecules with the exception of species that are not oxygenated and organosulfates <ref type="bibr">(Lopez-Hilfiker et al., 2019)</ref>.</p><p>2.1.5 Offline analysis of filters (FILTER) using ultra-high-performance liquid chromatography (UHPLC) and heated electrospray ionization (HESI) coupled to an Orbitrap high-resolution mass spectrometer (HRMS)</p><p>This procedure was optimized and described in detail by <ref type="bibr">Ungeheuer et al. (2021)</ref>. The method enhances the separation of organic compounds with high resolution and enables the determination of the accurate mass. The analysis consists mainly of four steps: sampling, extraction, separation, and detection.</p><p>First, the particles were collected from a flow of 5 L min -1 on a 47 mm diameter Emfab&#8482; filter (Pall Life Science, USA) during approximately 17 h for the experiment at -10 &#8226; C (see Table <ref type="table">2</ref> and Fig. <ref type="figure">S1</ref>). After sampling, the filter was stored at -18 &#8226; C to avoid possible losses by evaporation. The filter was cut into small pieces (approximately 3 &#215; 3 mm) and extracted two times in 0.2 mL solution (mixture of 90 % water and 10 % methanol) for 20 min. After each extraction step, the extract was filtered through a syringe filter (PTFE with a pore size of 0.2 &#181;m). For chromatographic separation a gradient of ultrapure water (eluent A, Milli-Q Reference A+, Merck Millipore) and methanol (eluent B, Optima LC/MS grade, Fisher Scientific) was applied. Both eluents were mixed with 0.1 % formic acid (v/v) for improved chromato-graphic performance. The injection volume was 5 &#181;L, the flow rate was 400 &#181;L min -1 , and the temperature was 40 &#8226; C. The gradient started with 1 % eluent B (0-0.5 min), increased linearly to 99 % eluent B (0.5-14 min), stayed at 99 % eluent B (14-16 min), was backflushed in 1 min, and equilibrated in 3 min, resulting in a total run time of 20 min. Negative ionization mode was used for the detection, in which the molecular ions [M-H] -are produced by deprotonation. The ion source settings used for this purpose were -3.5 kV spray voltage, 40 psi sheath gas, 8 arbitrary units auxiliary gas, and 262.5 &#8226; C capillary temperature. The scan range in full MS was 50-750 m/z, with a mass-resolving power of about 70 k at m/z 200. For data-dependent MS 2 (ddMS 2 ) the resolution was 17.5 k. Fragments were produced in a higher-energy collisional dissociation (HCD) cell with stepped collision energies of 15, 30, and 45 eV.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2">Data analysis</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.1">Data processing</head><p>TD-DMA, FIGAERO, and EESI-TOF data were processed using IGOR Pro 7 (WaveMetrics, Inc., USA) and Tofware (Version 3.1.2, Aerodyne Inc., USA). The data from the offline method were processed with Compound Discoverer 3.2 (Thermo Fisher Scientific). The postprocessing was done using MATLAB R2022a (MathWorks, Inc., USA).</p><p>TD-DMA data were corrected by the mass-dependent transmission efficiency in the mass classifier <ref type="bibr">(Heinritzi et al., 2016)</ref> and normalized by the nitrate reagent ions. FIGAERO data were averaged to 1 min and normalized by the reagent ions. EESI-TOF signals were averaged to 10 s and normalized by the most abundant electrospray ion (NaINa + ). In order to align the sampling times for the different techniques and perform a more direct particle-phase comparison, we selected as a reference the TD-DMA and FILTER collection times. Thus, for the comparison at -30 and -50 &#8226; C, EESI-TOF particle signals were averaged, and FIGAERO particle signals were integrated during the period in which the TD-DMA collected particles (&#8764; 3 and 5 h, respectively), while for the comparison at -10 &#8226; C, the EESI-average and FIGAERO-integration period corresponded to the time when the particles were collected with the FILTER for the offline analysis (&#8764; 17 h). Figure <ref type="figure">1</ref> provides an overview of a representative experiment at -30 &#8226; C. The overview of the experiments at -10 and -50 &#8226; C are shown in Fig. <ref type="figure">S1</ref> in the Supplement. Table <ref type="table">2</ref> summarizes the sampling conditions during the experiments reported in this study (for the purpose of the intercomparison), including the particle number concentration, mass concentration, and median mass diameter (MMD) calculated from the scanning mobility particle sizer (SMPS). The MMD indicates the particle size measured by the SMPS for which 50 % of the aerosol mass is contained in smaller particles, and 50 % is contained in larger particles. From Table <ref type="table">2</ref> it can be seen that, for the experiments at -30 (e) Particle phase measured by FIGAERO; the gray shaded areas refer to the particle collection period and the yellow shaded areas to the desorption period. FIGAERO measured in a semicontinuous mode, namely 15 min particle collections followed by 15 min desorption periods. In order to intercompare with EESI-TOF and TD-DMA, FIGAERO signals were integrated during the period where the TD-DMA collected particles (&#8764; 3 h); seven FIGAERO particle samples were integrated during the 3 h comparison period. (f) Particle phase measured by the TD-DMA; the TD-DMA collection period was approximately 3 h, while the desorption period lasted around 1 min, followed by a second heating for estimating the background.</p><p>and -50 &#8226; C, MMD av &lt; 100 nm, while for the experiment at -10 &#8226; C, MMD av &#8764; 106 nm.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.2.2">PMF analysis</head><p>One of the main questions we want to answer in this work is whether the thermal desorption methods (TD-DMA and FIGAERO) experience significant decomposition during the desorption process. To answer this question, we utilized PMF analysis. This method was originally described by <ref type="bibr">Paatero and Tapper (1994)</ref> for analyzing time series of mass spectra from ambient observations, and it was implemented by Buchholz et al. ( <ref type="formula">2020</ref>) with thermal desorption data for identifying different processes during particle evaporation. We therefore applied the same procedure as <ref type="bibr">Buchholz et al. (2020)</ref> to the TD-DMA and FIGAERO thermal desorption profiles (for the &#945;-pinene oxidation experiment at -30 &#8226; C and 20 % RH only). For the analysis, we separately processed 1 s TD-DMA and 1 s FIGAERO thermograms. Since the FIGAERO measures in a semicontinuous mode, we chose a representative thermogram. Both TD-DMA and FIGAERO data sets were background subtracted. For the TD-DMA background, we used the second heating cycle that is performed immediately after the first heating (described in Sect. 2.1.2). For the FIGAERO background, we used a period in which no significant particle load was present in the chamber (at the beginning of the experiment). We considered only the organic compounds and excluded the reagent ions for this analysis. We ran the PMF software using the CNerror scheme (based on the noise of each ion) and up to 10 different solutions. Four-factor TD-DMA and six-factor FIGAERO solutions (discussed later in Sect. 3.2.1) were chosen as the most interpretable results by (a) comparing the residuals and by looking at which solution captured the total signal and certain species the best (e.g., C 8 H 12 O 4 ) and <ref type="bibr">(b)</ref> by finding an equilibrium between good reconstructed signal and physically interpretable results. This means that for the solutions presented here, a higher number of factors likely improves the residuals; nevertheless, we chose the solution with the smallest number of factors that can still provide realistic information.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3">Results and discussion</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.1">Chemical composition comparison</head><p>Figure <ref type="figure">2</ref> shows the OS C , calculated as OS C = 2 &#215; O : C -H : C (an approximation stated by <ref type="bibr">Kroll et al., 2011)</ref>, against the number of carbon atoms for &#945;-pinene oxidation products in the particle phase at -30 &#8226; C and 20 % RH, as measured by three different techniques: TD-DMA, FIGAERO, and EESI-TOF. For all techniques, the highest intensities correspond to compounds with 10 carbon atoms (C 10 ), for which the oxidation state varies between 0.5 and -1.5, depending on the measurement technique.</p><p>Compounds with more than 10 carbon atoms were also detectable by the TD-DMA, FIGAERO, and EESI-TOF.</p><p>The TD-DMA and FIGAERO detected compounds with fewer than five carbon atoms and OS C &gt;0, which, in contrast, are not detected by the EESI-TOF (this feature is discussed in Sect. 3.2.1). In order to simplify the comparison, we calculated the fraction of species containing fewer than 10 carbon atoms (C &lt;10 ), 10 carbon atoms (C 10 ), and more than 10 carbon atoms (C &gt;10 ), since this can provide insight into the detected fraction of monomers and dimers for each technique (Fig. <ref type="figure">2d</ref>). Approximately 42 %, 32 %, and 23 % of the signals correspond to C &lt;10 ; 47 %, 65 %, and 53 % to C 10 ; and around 11 %, 3 %, and 24 % to C &gt;10 . These percentages were measured by the TD-DMA, FIGAERO, and EESI-TOF, respectively. Figure <ref type="figure">S2</ref> in the Supplement displays the results for the experiments at -50 &#8226; C. In every case, C 10 represents the highest fraction detected by all the techniques in this experiment. Nevertheless, we do see significant differences between the techniques for C &lt;10 , C 10 , and C &gt;10 .</p><p>The chemical ionization utilized by the TD-DMA (nitrate, NO -</p><p>3 ) is more sensitive towards highly oxygenated species, while the FIGAERO (iodide, I -) detects intermediately oxygenated species with higher sensitivity. In Figs. S3 and S4 in the Supplement, we present the results (number of oxygen atoms vs. number of carbon atoms) at -30 and -50 &#8226; C, respectively. From the figures (Figs. <ref type="figure">S3</ref> and<ref type="figure">S4</ref>) we observe that more oxygenated species contribute more to the total signal in TD-DMA than in FIGAERO. This observation is consistent with the sensitivity that one would expect according to the chemical ionization. The electrospray ionization (Na + ) for the EESI-TOF is usually more sensitive towards intermediately oxygenated species, even though in the results presented here, it seems to capture the whole spectrum very well.</p><p>Besides the reagent ion selectivity, several factors can explain the quantitative differences. For example, both the TD-DMA and FIGAERO detect a lower fraction of C &gt;10 (11 % and 3 % compared to 24 % for the EESI-TOF). The TD-DMA and FIGAERO techniques are based on thermal desorption, which may cause decomposition of thermally unstable compounds during evaporation (as discussed in more detail in Sect. 3.2.1). On the other hand, the resulting fractions of C &gt;10 can be influenced by the ionization method employed: chemical ionization and electrospray are softionization techniques, for which one can expect little fragmentation. Thus, we presume that thermal decomposition during evaporation could be the most significant factor that explains these differences.</p><p>Figure <ref type="figure">3</ref> presents the results for the experiment conducted at -10 &#8226; C (&#945;-pinene oxidation products at 80 % RH) for particles collected on a filter and analyzed by the UHPLC-HESI-HRMS (offline method; Fig. <ref type="figure">3a</ref>). FIGAERO and EESI-TOF results are shown in Fig. <ref type="figure">3b</ref> and<ref type="figure">c</ref>, respectively. Overall, fewer compounds are detected by UHPLC-HESI-HRMS than by FIGAERO and EESI-TOF. The highest intensities in Fig. <ref type="figure">3a</ref>  . Ions with the same formulas are also detected by the FIGAERO and EESI-TOF, but the contribution to the total signal differs. The results at -10 &#8226; C (number of oxygen atoms vs. number of carbon atoms) are shown in Fig. <ref type="figure">S5</ref> in the Supplement. By applying the UHPLC-HESI-HRMS method, it is possible to distinguish between compounds with identical chemical formulas (isomers). For the experiment reported here, two isomers for C 8 H 12 O 4 , C 10 H 16 O 3 , and C 10 H 16 O 5 , as well as three isomers for C 10 H 16 O 4 and C 10 H 16 O 6 were detected. The detection of these isomers is enabled by the chromatographic separation (their interaction with a reversed-phase column results in different retention times and therefore makes the separation feasible). However, complementary experiments are needed to investigate the molecular structure. Furthermore, Fig. <ref type="figure">3d</ref> shows the contributions of the C &lt;10 , C 10 , and C &gt;10 fractions to the total signal for the FILTER, FIGAERO, and EESI-TOF. At -10 &#8226; C, the fraction of compounds with more than 10 carbon atoms (C &gt;10 ) has the smallest contribution to the total signal (14 %, 5 %, and 24 % for the FILTER, FI-GAERO, and EESI-TOF, respectively). The fractions C &lt;10 and C 10 do not seem to have a clear tendency; they both contribute substantially to the total signal in each technique.</p><p>For the methods utilizing electrospray ionization (EESI-TOF and UHPLC-HESI-HRMS), the polarity plays an im- portant role. The EESI-TOF ran in the positive mode, allowing the SOA species to be detected as adducts with Na + , while HESI utilized in the offline method ran in the negative mode, in which molecular ions are produced by deprotonation. <ref type="bibr">Surdu et al. (2021)</ref> used an aerosol growth model based on the condensation of organic vapors and demonstrated that the chemical composition measured by the EESI-TOF (in the positive mode as in this study) is consistent with the expected condensed oxidation products with small differences. On the other hand, <ref type="bibr">Ungeheuer et al. (2021)</ref>, who utilized the UHPLC-HESI-HRMS method, reported that the detection of ester molecules was accomplished only in the positive-ionization mode (1000 compounds were detected in the positive mode, while only 16 were detected in the negative mode). Besides the polarity, several other factors can influence the electrospray ionization response, such as analyte chargeability and surface activity <ref type="bibr">(Cech and Enke, 2001)</ref>, and therefore impact the completeness of the chemical composition of aerosol particles.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Volatility classes</head><p>We estimated the volatilities of the detected particle-phase compounds and associated them with defined volatility classes. We used the parametrization introduced in Donahue et al. ( <ref type="formula">2011</ref>) and modified by <ref type="bibr">Stolzenburg et al. (2018)</ref>. This approach has been also discussed in <ref type="bibr">Simon et al. (2020)</ref> and <ref type="bibr">Wang et al. (2020)</ref>. The volatility was approximated from the number of carbon and oxygen atoms in the specific molecules, and it was first defined at 300 K. By using the Clausius-Clapeyron equation, the volatility was then shifted according to the corresponding experimental temperature. The evaporation enthalpy was approximated according to <ref type="bibr">Donahue et al. (2011)</ref> and <ref type="bibr">Epstein et al. (2009)</ref>. Thereafter the volatility was associated with any of the following classes: ULVOCs, ELVOCs, LVOCs, SVOCs, and IVOCs.</p><p>Figures <ref type="figure">4</ref> and<ref type="figure">5</ref> show the contribution of each volatility class to the total particle signal for the corresponding experiment and for each technique. The results at -50 &#8226; C are reported in Fig. <ref type="figure">S6</ref> in the Supplement. For the experiment at -30 &#8226; C (Fig. <ref type="figure">4</ref>), LVOCs constitute the higher fraction for the TD-DMA, FIGAERO, and EESI-TOF. EESI-TOF detects the highest fraction of ULVOCs (&#8764; 12 % compared to 6 % and 2 % measured by TD-DMA and FIGAERO, respectively). An IVOC fraction (&#8764; 8 %) is only detected by the EESI-TOF. At -10 &#8226; C (Fig. <ref type="figure">5</ref>), semi-volatile organic compounds (SVOCs) contribute the most to the total particle signal for the FILTER, FIGAERO, and EESI-TOF. Very small fractions of ULVOCs are also detected by all the techniques. The EESI-TOF detects a higher fraction of IVOCs (20 %) than FILTER and FIGAERO (2 % and 4 %), respectively. Taking into account the particle load (&#8764; 1-3 &#181;g m -3 ) and size of the particles (diameter &lt; 100 nm), it is possible that a significant fraction of IVOCs measured by the EESI-TOF results from measurement artifacts, as seen in previous studies using EESI <ref type="bibr">(Surdu et al., 2021)</ref>. Several reasons (or a com- bination of them) can explain this feature: (a) the Na + ionization technique may be more sensitive to less oxygenated organic compounds than the I -or NO - 3 techniques, (b) some amount of the gas phase likely broke through the charcoal denuder (although its efficiency is &gt;99 %) and reached the detector <ref type="bibr">(Lee et al., 2021</ref>, reported that the EESI-TOF is more sensitive toward gas-phase analytes as compared to their particle-phase counterparts), and (c) some ion-induced fragmentation can possibly occur.</p><p>Overall, we observed that the contribution of the lowestvolatility classes (ULVOC, ELVOC, and LVOC) increases as the temperature decrease. This observation reflects two opposing temperature effects, as discussed in <ref type="bibr">Ye et al. (2019)</ref> based on FIGAERO results: autoxidation and thus the extent of oxidation are reduced at low temperatures, but any given compound is much less volatile at low temperatures because of the strong dependency between saturation concentration and temperature.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.2">Thermal desorption methods: TD-DMA and FIGAERO</head><p>Figure <ref type="figure">6</ref> shows the thermograms obtained by FIGAERO and TD-DMA for three different species detected in the &#945;-pinene ozonolysis experiment at -30  TD-DMA temperature is increased up to 600 Additionally, we display in Fig. <ref type="figure">6</ref> the second TD-DMA heating. A second heating is performed immediately after the first heating, without particle collection. This performance allows us to estimate the signal coming from the particles and the signal coming from the background due to the inlet line. From the background measurement, it can be seen that the particle constituents measured by the TD-DMA have been efficiently evaporated.  </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>PMF results</head><p>The results of the PMF analysis of the TD-DMA data are shown in Fig. <ref type="figure">7</ref>, which contains the factor mass spectra (Fig. <ref type="figure">7a-d</ref>), the factor thermograms (Fig. <ref type="figure">7e</ref>), and the contribution of each factor to the total signal (Fig. <ref type="figure">7f</ref>). We found that four factors are the best choice to reconstruct the TD-DMA data and to provide the most interpretable results (the residuals are shown in Fig. <ref type="figure">S7</ref> in the Supplement). We numbered the factors according to their peak desorption temperatures (Fig. <ref type="figure">7e</ref>). F1 TD-DMA , which desorbs at the very first stages of the heating cycle, includes organic compounds with molecular masses between 150 and 250 Da (M av = 211.6 Da), with a carbon, hydrogen, and oxygen average content (CHO ac ) of 9.2, 14.6, and 5.4, respectively. F1 TD-DMA contains mainly compounds in the monomer region (see Fig. <ref type="figure">S8</ref> in the Supplement). F2 TD-DMA desorbs right after F1 TD-DMA . The mass average (M av ) is 230.7 Da, and the CHO ac is 10.0, 16.1, and 5.9. Compounds in the monomer region also contribute to this factor (see Fig. <ref type="figure">S8</ref> in the Supplement). F3 TD-DMA shows a clear contribution of both monomers and dimers for the time when the time series shows a broadened peak. CHO ac is 10.8, 16.7, and 5.5, and M av = 234.5 Da. Lastly, F4 TD-DMA is dominated (&#8764; 60 % of the signal intensity) by a high signal with molecular mass of 172.18 Da, which corresponds to C 8 H 12 O 4 . This is reflected by lower values of CHO ac and M av compared to the other factors (CHO ac = 8.6, 12.8, and 4.5; M av = 188.2 Da). By looking closer into F4 TD-DMA (Fig. <ref type="figure">7d</ref>), we observe that some compounds with mass &lt; 200 Da also contribute to this factor. By integrating each factor thermogram (Fig. <ref type="figure">7e</ref>), we calculated that F1 TD-DMA and F2 TD-DMA contribute to &#8764; 70 % of the total signal, while F3 TD-DMA and F4 TD-DMA make up &#8764; 30 % of the total signal, as shown in Fig. <ref type="figure">7f</ref>.</p><p>For the purpose of comparison, we present in Fig. <ref type="figure">8</ref> the results from applying PMF to the FIGAERO thermal desorption data for a solution with six factors. Figure <ref type="figure">8a</ref>-f contain the factor mass spectra, Fig. <ref type="figure">8g</ref> contains the factor thermograms, and Fig. <ref type="figure">8h</ref> shows the contribution of each factor to the total particle signal (the residuals and the factors expressed in terms of their oxygen content and mass are shown in Figs. S9 and S10 in the Supplement, respectively). F1 FIGAERO , F2 FIGAERO , and F3 FIGAERO (Fig. <ref type="figure">8ac</ref>) show a distinct contribution from monomers and similar mass spectra but display different thermal profiles (in Fig. <ref type="figure">8g</ref>). Specifically, F2 FIGAERO and F3 FIGAERO exhibit well-defined thermal profiles (&#8764; 15 &#8226; C difference in T max ). However, F1 FIGAERO shows a broader profile with no distinct maximum. We suspect that F1 FIGAERO can be related to some of the following causes to some extent: (a) limited resolution of the chosen PMF solution at T &lt; 50 &#8226; C, likely related to the presence of two neighboring factors that were not resolved completely; <ref type="bibr">(b)</ref> interference from volatile material already evaporating at the beginning of the thermogram; and (c) adsorption of gaseous compounds. Reason (b) could be related to the procedure initiating the desorption, where the filter is flushed with N 2 at ambient temperature before starting the heating ramp, which would likely affect the most volatile material. F4 FIGAERO and F5 FIGAERO (Fig. <ref type="figure">8d</ref> and<ref type="figure">e</ref>) show a contribution from both monomers and dimers, with a very similar CHO ac and M av . However, they show different thermogram behavior (&#8764; 20 &#8226; C difference for T max ; Fig. <ref type="figure">8g</ref>). F6 FIGAERO shows mainly contributions from compounds with low mass (&lt; 200 Da) and desorbs mainly at the very end of the heating curve. The contribution of each factor to the total signal is shown in Fig. <ref type="figure">8h</ref>.</p><p>As mentioned previously, we observed some factors with similar CHO ac and M av but different thermal behavior, possibly due to the presence of isomers. Molecules with the same composition but different structure and functional groups may exhibit different volatilities. In fact, functionality is one of the driving factors that determines volatility <ref type="bibr">(Pankow and Asher, 2008;</ref><ref type="bibr">Wang et al., 2020)</ref>. The mass spectrometry techniques reported here are not able to determine the molec- ular structure. We further note that the factors F4 TD-DMA and F6 FIGAERO desorb mainly at the very last stage of the heating curves, although they both have a clear contribution of compounds with mass &lt; 200 Da and one of the lowest oxygen contents of all factors (i.e., the lowest degree of oxidation). We suspect that F4 TD-DMA (Fig. <ref type="figure">7d</ref>) and F6 FIGAERO (Fig. <ref type="figure">8g</ref>) are comprised primarily of products of thermal decomposition; the heat applied to desorb the particles instead cleaves certain chemical bonds in (larger) molecules before these could desorb. Small compounds are generally expected to desorb before the transmitted thermal energy (i.e., the desorption temperature) is high enough to cause such decomposition. However, F4 TD-DMA and F6 FIGAERO thermal profiles also exhibit a small peak at lower temperatures (observed more clearly in Fig. <ref type="figure">8g</ref> at &#8764; 40-50 &#8226; C), which is likely direct desorption. This may suggest that the low-temperature peak stems from monomers desorbing directly, while the broad high-temperature peak represents decomposing dimers/oligomers, which are then detected at the composition of the corresponding monomers. Previous studies applying PMF analysis to FIGAERO thermal desorption data also observed the presence of one or more factors dominated by thermal decomposition products for &#945;-pineneand sesquiterpene-derived SOA <ref type="bibr">(Buchholz et al., 2020;</ref><ref type="bibr">Li et al., 2021)</ref>. Those studies concluded that thermal decomposition was the main volatilization process at desorption tempera-tures above 100 &#8226; C, with differences between the observed SOA types.</p><p>By applying PMF analysis to thermal desorption data we observed that often, several factors are needed to explain the behavior of a single ion. One example is shown in the thermal profile of C 8 H 12 O 4 for both FIGAERO and TD-DMA (in the Supplement Fig. <ref type="figure">S11</ref>). Particularly, F4 TD-DMA and F6 FIGAERO explain the C 8 H 12 O 4 signal at higher temperatures. This is consistent with previous observations. Lopez-Hilfiker et al. ( <ref type="formula">2015</ref>) reported a significant contribution of thermal decomposition to the detection of C 8 H 12 O 4 in the &#945;pinene ozonolysis system and stated that small acids present in higher-than-expected concentrations in SOA are likely entirely due to thermal decomposition. In our previous work <ref type="bibr">(Caudillo et al., 2021)</ref>, we presented individual results of the gas and particle phases of the same chemical system as in this study using the same ionization and detention scheme. We found that C 8 H 12 O 4 contributed &#8764; 10 times more to the particle than to the gas phase.</p><p>Furthermore, in the present study, the presence of the other PMF factors suggests that either there are at least three isomers with distinguishable volatility, or there are different thermal decomposition processes occurring at different desorption temperatures which all form C 8 H 12 O 4 as a stable product. There are some studies that suggest possible decomposition pathways. For example, <ref type="bibr">Hyttinen et al. (2022)</ref>  Table <ref type="table">3</ref> summarizes some advantages and disadvantages that should be considered when applying the methods presented here to the measurement of laboratory-generated sub-100 nm diameter SOA. When measuring particle chemical composition, the time needed for collecting enough particles (mass) should be carefully considered. This fact becomes a challenge when analyzing nanoparticles, since the small particles do not contribute significantly to the overall SOA mass. In that regard, EESI-TOF and FIGAERO provide a faster response (every 1 s and 30 min, respectively) than the other two methods and allow near-real-time monitoring. This is especially convenient when the chemical composition changes continuously (i.e., in complex environments or during oxidative-flow reactor or chamber experi-ments). In fact, the EESI-TOF's total particle signal exhibited a good correlation with the mass concentration calculated from the scanning mobility particle sizer (SMPS) measurements (r 2 &gt;0.94; Fig. <ref type="figure">S12</ref> in the Supplement). Despite the fact that there is a size dependence on EESI-TOF sensitivity, EESI-TOF sensitivity decreases as the size of the particles increases <ref type="bibr">(Lee et al., 2021)</ref>. The particle collection periods for TD-DMA and FILTER (offline analysis) were much longer and depended on the particle load and limit of detection. Besides the low time resolution, a main disadvantage of longer collection times is that aerosol aging may occur. This can potentially change the chemical composition and therefore lead to inaccurate aerosol speciation. Several studies have reported positive and negative artifacts caused by adsorption of gases on the collection surfaces, longer sampling periods, and volatilization of organic species either during collection or during storage <ref type="bibr">(Turpin et al., 1994;</ref><ref type="bibr">Subramanian et al., 2004;</ref><ref type="bibr">Kristensen et al., 2016)</ref>.</p><p>The mass spectrometers coupled to TD-DMA and FI-GAERO (nitrate CI-APi-TOF and iodide HRToF-CIMS, respectively) can perform gas-phase measurements while the particle collection takes places. EESI-TOF in the dual configuration can measure both the particle and gas phases quasisimultaneously. This allows for a direct comparison between the gas and particle phases. Nevertheless, these mass spectrometry techniques can only identify chemical formulas, but </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Instrument</head><p>Advantages Drawbacks TD-DMA + NO - 3 CI-APi-TOF -Size-resolved particle collection -Gas phase can be measured during particle collection and gas and particle intercomparison -Detection immediately after collection -Resolution might depend on the particle load (collection time &#8764; 3 and 5 h) a -Thermal fragmentation is possible FIGAERO + I -HRToF-CIMS -Gas phase can be measure during particle collection and gas and particle intercomparison -Detection immediately after collection -Time resolution of 30 min: semicontinuous -Non-size-resolved particle collection -Resolution of 30 min: semicontinuous -Thermal fragmentation is possible Na + EESI-TOF -Continuous measurement, 1 s time resolution -Gas phase can be measure using the dual configuration -Non-size-resolved particle collection -Size-dependent sensitivity FILTER UHPLC-HESI-HRMS method -Differentiates between clusters and molecules (pre-separation makes sure that the compounds are not fragments) -Identifies isomers b using chromatography for separation -Non-size-resolved particle collection -Resolution might depend on the particle load (collection time &#8764; 17 h) a -Detection not immediately after collection, first stored -Possible aging, sampling artifacts a Collection period for the experiments reported here for TD-DMA and FILTER. b An assumption about the structure can be expressed by doing complementary experiments.</p><p>with some limitations. Thus, it is not possible, for example, to provide structural information or identification of isomers. In contrast, the UHPLC-HESI-HRMS offline method has the advantage of being able to distinguish between clusters, molecules, and isomers based on the chromatographic separation. Furthermore, the fragmentation pattern (via MS 2 experiments) can provide hints to interpret the functional groups and can be used for unambiguous compound identification. Hence, UHPLC-HRMS can provide robust analytical insight of the stable compounds.</p><p>The thermal desorption methods (TD-DMA and FI-GAERO) exhibit significant thermal decomposition of compounds with desorption temperatures above 100 &#8226; C. For the EESI this seems to be less of an issue in general, but in some specific studies thermal decomposition was found to be relevant <ref type="bibr">(Bell et al., 2022)</ref>. PMF analysis of the thermal desorption data from the TD-DMA and FIGAERO could separate the contribution of products from thermal decomposition from those directly desorbing. However, even with this method, it is not possible to obtain information about the original compounds decomposing and their true volatility. The observed decomposition temperature can be used as an upper limit for volatility (i.e., their true volatility is lower than that associated with the apparent desorption temperature).</p><p>For the FILTER method, the compounds collected on the filter have to be extracted into a liquid phase for the UHPLC separation. The choice of solvents for this extraction will determine which fraction of organic compounds will be ana-lyzed. The water-methanol mixture used in this study will extract polar, hydrophilic compounds similar to the watersoluble organic carbon category. Note that the exposure to water (or other solvents) may lead to chemical reactions, e.g., hydrolysis of (hydro)peroxides. The selective extraction and potential aqueous-phase chemistry may explain the smaller number of compounds detected with the FILTER method. However, for the compounds that do get analyzed, a much deeper understanding can be achieved (e.g., separation of isomers).</p><p>The ionization technique also plays a role in the final detection. If the ionization technique is not soft enough, this can result in fragmentation and affects the final response in the detection. In principle, the ionization techniques utilized by the instruments reported here are soft, meaning that no significant fragmentation occurs during the detection. Nevertheless, the ionization efficiency is different between the techniques. For example, with the nitrate reagent ion, highly oxygenated species can be better detected, while the ionization techniques used for FIGAERO and EESI-TOF (I -and Na + , respectively) are more sensitive to intermediately oxygenated organic compounds. The UHPLC-HESI-HRMS can be operated in both polarity modes, however, and can therefore detect species that are able to either donate protons (in the negative mode) or form clusters with protons or sodium (in the positive mode).</p><p>The complete characterization of species in the particle phase in terms of chemical formula and structure represents an analytical challenge. In this sense, the full identification of organic compounds is only possible by combining different techniques.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4">Conclusions</head><p>In this study, we present an overview of four different methods for measuring the chemical composition of ultrafine particles, and we describe their capabilities to detect organic compounds. Specifically, we reported the particlephase composition from &#945;-pinene ozonolysis at -50, -30, and -10 &#8226; C. In all the cases, the highest portion of detected compounds correspond to species with 10 and fewer than 10 carbon atoms (C 10 , C &lt;10 ). The EESI-TOF generally detected a higher fraction (compared to the other techniques: TD-DMA, FIGAERO, and FILTERS) of compounds with more than 10 carbon atoms (C &gt;10 ). In terms of volatility classes, EESI-TOF detected a higher fraction of ULVOCs in all the experiments reported here, especially for those at lower temperatures (-50 and -30 &#8226; C). We presume that several factors can explain these differences, i.e., thermal decomposition of large compounds (for the thermal desorption methods), for which we applied positive matrix factorization on the thermal profiles and suggested a four-factor solution for TD-DMA and a six-factor solution for the FIGAERO. Specifically, we suspect that F4 TD-DMA and F6 FIGAERO might be related to thermal decomposition to some extent. The PMF factors dominated by direct desorption can be interpreted as volatility classes, characterized by their T max values (the peak in the respective temperature desorption profiles). Nevertheless, further calibration experiments are needed to determine the relation between T max and saturation concentration. With the offline method, UHPLC-HESI-HRMS, we were able to verify the presence of isomers (two isomers for C 8 H 12 O 4 , C 10 H 16 O 3 , and C 10 H 16 O 5 and three isomers for C 10 H 16 O 4 and C 10 H 16 O 6 ), which represents an important advantage over the online methods reported here.</p><p>While the methods generally agree on the most important compounds that are found in the nanoparticles, they all have their strengths and shortcomings. A major limit of these methods is that the measurements of the chemical compounds are not quantitative, and only rough estimates of the exact contributions of a compound to the overall chemical composition can be made. However, knowing the limitations of each method and using combinations of the available methods can provide deeper insights into the chemical composition and volatility of nanoparticles.  <ref type="bibr">325656, 316114, 314798, 325647, 341349, and 337549)</ref>; the European Research Council, HORIZON EUROPE (ATM-GTP, grant no. 742206); and the Prince Albert II of Monaco Foundation (grant no. 2859).</p><p>Review statement. This paper was edited by John Liggio and reviewed by three anonymous referees.    </p></div><note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_0"><p>Atmos. Chem. Phys., 23, 6613-6631, 2023 https://doi.org/10.5194/acp-23-6613-2023 L. Caudillo et al.: An intercomparison study of four different techniques</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_1"><p>https://doi.org/10.5194/acp-23-6613-2023 Atmos. Chem. Phys., 23, 6613-6631, 2023</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_2"><p>Atmos. Chem. Phys., 23, 6613-6631, 2023 https://doi.org/10.5194/acp-23-6613-2023</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_3"><p>m -3 (obtained by integrating the normalized mass concentration from the SMPS), the gray shaded areas refer to the particle collection period used for the comparison with EESI-TOF and FIGAERO. The sample collection period for the intercomparison was determined by the FILTER at -10 &#186;C and by the TD-DMA at -50 &#186;C.</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_4"><p>each system. (d) Fraction of species in the particle-phase containing less than 10 carbon atoms (C&lt;10), 10 carbon atoms (C10), and more than 10 carbon atoms (C&gt;10). The fraction was calculated by normalizing the intensities by the total signal in each system.</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_5"><p>chemical-ionization mass spectrometer, and (c) EESI-TOF: Extractive Electrospray Na + Ionization time-of-flight mass spectrometer. The level of &#945;-pinene was between 1 and 3 ppbv while the ozone level was ~100 ppbv. The symbol sizes in (a), (b), and (c) represent the intensities normalized by the total signal in each system. (d) Fraction of species in the particle-phase containing less than 10 carbon atoms (C&lt;10), 10 carbon atoms (C10), and more than 10 carbon atoms (C&gt;10). The fraction was calculated by normalizing the intensities by the total signal in each system.</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" n="20" xml:id="foot_6"><p>% RH, (a) F1 FIGAERO, (b) F2 FIGAERO, (c) F3 FIGAERO, (d) F4 FIGAERO, (e) F5 FIGAERO and, (f) F6 FIGAERO are the factors mass spectra expressed in terms of number of oxygens against the neutral ion mass. The colorscale represents the intensity normalized by the total particle signal. The particle-phase signal has been background corrected.</p></note>
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