# Analysis Of Atmospheric Particle Growth Based On Vapor Concentrations Measured At The High-Altitude Gaw Station Chacaltaya In The Bolivian Andes

Arto Heitto, Cheng Wu, Diego Aliaga, Luis Blacutt, Xuemeng Chen, Yvette Gramlich, Liine Heikkinen, Wei Huang, Radovan Krejci, Paolo Laj, et al.

► To cite this version:

Arto Heitto, Cheng Wu, Diego Aliaga, Luis Blacutt, Xuemeng Chen, et al. .. Analysis Of Atmo-  
spheric Particle Growth Based On Vapor Concentrations Measured At The High-Altitude Gaw Sta-  
tion Chacaltaya In The Bolivian Andes. Atmospheric Chemistry and Physics, 2024, 24, pp.1315-1328.  
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Analysis of atmospheric particle growth based on vapor concentrations measured at the high-altitude GAW station Chacaltaya in the Bolivian Andes

Arto Heitto¹, Cheng Wu²,ª, Diego Aliaga³, Luis Blacutt⁴, Xuemeng Chen³, Yvette Gramlich²,
Liine Heikkinen², Wei Huang³, Radovan Krejci², Paolo Laj³,⁵, Isabel Moreno⁴, Karine Sellegrui⁶,
Fernando Velarde⁴, Kay Weinhold⁷, Alfred Wiedensohler⁷, Qiaozhi Zha³, Federico Bianchi³,
Marcos Andrade⁴, Kari E. J. Lehtinen¹, Claudia Mohr²,ᵇ, and Taina Yli-Juuti¹

¹Department of Technical Physics, University of Eastern Finland, 70211 Kuopio, Finland

²Department of Environmental Science and Bolin Centre for Climate Research,
Stockholm University, Stockholm, Sweden

³Institute for Atmospheric and Earth System Research/Physics, University of Helsinki, 00014 Helsinki, Finland

⁴Laboratorio de Física de la Atmósfera, Instituto de Investigaciones Físicas,
Universidad Mayor de San Andrés, La Paz, Bolivia

⁵Institute for Geosciences and Environmental Research (IGE), University of
Grenoble Alpes, Grenoble 38000, France

⁶CNRS, Laboratoire de Météorologie Physique (LaMP), Université Clermont Auvergne,
63000 Clermont-Ferrand, France

⁷Leibniz Institute for Tropospheric Research, 04318 Leipzig, Germany

ªnow at: Department of Chemistry and Molecular Biology, University of Gothenburg, Gothenburg, Sweden

ᵇnow at: Laboratory of Atmospheric Chemistry, Paul Scherrer Institute, Villigen, Switzerland

**Correspondence:** Arto Heitto (arto.heitto@uef.fi) and Cheng Wu (cheng.wu@gu.se)

Received: 21 March 2023 – Discussion started: 25 April 2023

Revised: 16 November 2023 – Accepted: 1 December 2023 – Published: 30 January 2024

**Abstract.** Early growth of atmospheric particles is essential for their survival and ability to participate in cloud formation. Many different atmospheric vapors contribute to the growth, but even the main contributors still remain poorly identified in many environments, such as high-altitude sites. Based on measured organic vapor and sulfuric acid concentrations under ambient conditions, particle growth during new particle formation events was simulated and compared with the measured particle size distribution at the Chacaltaya Global Atmosphere Watch station in Bolivia (5240 m a.s.l.) during April and May 2018, as a part of the SALTENA (Southern Hemisphere high-ALTitude Experiment on particle Nucleation and growth) campaign. Despite the challenging topography and ambient conditions around the station, the simple particle growth model used in the study was able to show that the detected vapors were sufficient to explain the observed particle growth, although some discrepancies were found between modeled and measured particle growth rates. This study, one of the first of such studies conducted on high altitude, gives insight on the key factors affecting the particle growth on the site and helps to improve the understanding of important factors on high-altitude sites and the atmosphere in general. Low-volatility organic compounds originating from multiple surrounding sources such as the Amazonia and La Paz metropolitan area were found to be the main contributor to the particle growth, covering on average 65 % of the simulated particle mass in particles with a diameter of 30 nm. In addition, sulfuric acid made a major contribution to the particle growth, covering at maximum 37 % of the simulated particle mass in 30 nm particles during periods when volcanic activity was detected on the area, compared to around 1 % contribution on days without volcanic activity. This suggests that volcanic emissions can greatly enhance the particle growth.
# 1 Introduction

In favorable conditions, atmospheric particles can act as cloud condensation nuclei (CCN) and activate to form cloud droplets. It is estimated that up to half of the particles acting as CCN are secondary aerosol particles formed in the atmosphere by nucleation of oxidized gases (Merikanto et al., 2009). These secondary aerosol particles form when low-volatility vapors cluster and grow into particles of 1–2 nm in diameter (Kulmala et al., 2013). The formed particles are required to experience further growth to reach CCN sizes, which are typically at least some tens of nanometers in dry diameter (Pierce and Adams, 2007; Reddington et al., 2017). Assuming the gas-phase concentrations are high enough to allow condensational growth of the particles, the fraction of newly formed particles that ends up growing to CCN sizes depends on the relative rates of particle growth and scavenging. The growth of particles serves as a source of CCN-sized particles, while their collisions with pre-existing larger particles reduces the production of potential CCN from the secondary aerosol.

For the initial step of atmospheric new particle formation (NPF), i.e., nucleation, the concentration of sulfuric acid is of essence (e.g., Kulmala and Kerminen, 2008; Sipilä et al., 2010). However, also ammonia, amines, and organic vapors are likely to partake in nucleation (Kulmala and Kerminen, 2008; Zhang et al., 2012; Kirkby et al., 2016). The nucleation mode particles grow when surrounding vapors condense on the particles. At least in areas dominated by biogenic emissions, the early growth is expected to be mostly governed by low and extremely low-volatility organic compounds (LVOCs and ELVOCs), although also semi-volatile organic compounds (SVOCs), sulfuric acid, and ammonia may contribute to the growth if their vapor concentrations are high (Yli-Juuti et al., 2013; Ehn et al., 2014; Tröstl et al., 2016; Mohr et al., 2017; Kerminen et al., 2018; Mohr et al., 2019).

Three key features define regional atmospheric NPF: (1) increase in particle concentration in nucleation mode (particles up to 25 nm in diameter); (2) formation of a new, distinct nucleation mode persisting for several hours; and (3) growth of the nucleation mode over several hours (Kulmala et al., 2012). If all these criteria are fulfilled continuously, it is characterized as an NPF event. NPF is a phenomenon frequently occurring in the atmosphere (Kulmala et al., 2004; Zhang et al., 2012; Kerminen et al., 2018). In previous studies, the growth rates (GRs) in the nucleation mode have been shown to be in general around $1–20 \text{ nm h}^{-1}$ (Yli-Juuti et al., 2011; Kerminen et al., 2018; Nieminen et al., 2018). The GRs at high-altitude sites fall usually in a similar order of magnitude, although there is a large variability between different sites (Sellegri et al., 2019): greater GRs have been found at the Southern Hemi-

spheric high-altitude sites as opposed to high-altitude sites in the Northern Hemisphere. However, the observation locations discussed in Sellegri et al. (2019) are scarce: two data sets (about 1 year in span) are investigated from the Southern Hemisphere (Chacaltaya (5240 m a.s.l.) and Maido (2160 m a.s.l.) stations) and four stations from the Northern Hemisphere (stations of Monte Cimone (2165 m a.s.l.), Jungfraujoch, (3580 m a.s.l.), Puy de Dôme (1465 m a.s.l.), and Nepal Climate Observatory–Pyramid (5079 m a.s.l.) – length of time series was between 1 and 4 years). The pattern of higher GRs at the Southern Hemisphere, as observed by Sellegri et al. (2019) for high-altitude sites, does not hold overall for all sites in the Northern and the Southern Hemisphere (Yli-Juuti et al., 2011; Nieminen et al., 2018). However, robust conclusions are hard to be drawn due to the limited data especially from the Southern Hemisphere (Kerminen et al., 2018; Laj et al., 2020). In addition to the scarcity of observational data, characterizing NPF events at high-altitude sites can be very challenging for various reasons. One is the complicated topography of the sites, where different air masses and updrafts and mountain winds from the lower altitudes mix up the air, which can make the continuous observation of one NPF event very difficult (Garcia et al., 2014; De Wekker and Kossman, 2015; Collaud Coen et al., 2018; Foucart et al., 2018; Sellegri et al., 2019; Casquero-Vera et al., 2020; Aliaga et al., 2021).

Here we analyze data from measurements that were conducted as part of the Southern Hemisphere high-ALTitude Experiment on particle Nucleation and growth (SALTENA) on the Chacaltaya (CHC) Global Atmosphere Watch (GAW) station (5240 m a.s.l.; 16.35° S, 68.13° W) in Bolivia (Bianchi et al., 2022). CHC can be simultaneously affected by long- and short-range aerosol and precursor vapors transport (Aliaga et al., 2021). On average at any given time, about 24% of the air arriving at Chacaltaya originates from the planetary boundary layer, and the other 76% comes from the free troposphere (Aliaga et al., 2021). At Chacaltaya, multiple NPF events have been observed to take place on the same day consequently (Rose et al., 2015). In this case, defining from which NPF event the nucleation mode particles originate may be difficult. In previous studies, the mean growth rates observed at the site were $10.31 \pm 14.65$ and $13.65 \pm 15.91 \text{ nm h}^{-1}$ in the particle diameter range of 3–7 and 7–20 nm, respectively (Sellegri et al., 2019). The GRs at the site were generally higher during the wet season (November to April) than the dry season (May to October) (Rose et al., 2015). The measurement period analyzed in this work was within the transition of the seasons, during April and May. In addition, one specific feature of the observations at the measurement site is the influence of volcanic emissions impacting at the site during the analyzed period in May, likely advected especially from the Sabancaya volcano (Bianchi et al., 2021; Aliaga et al., 2021).
This work focuses on the growth of newly formed parti-
cles at CHC during the SALTENA campaign. The growth of
secondary aerosol particles is simulated based on measured
ambient gas-phase concentrations of sulfuric acid and or-
ganic compounds, and these simulations are compared with
the observed particle growth during NPF events in April and
May 2018. Our aim is to investigate whether condensation
of the detected vapors can explain the observed growth of
nucleation mode particles in this complex environment, the
role that different vapors play in the growth, and how other
factors (i.e., ambient conditions) may contribute to the ob-
served particle growth. As measuring the composition of
the freshly formed nanoparticles currently remains a chal-
lenge, investigations based on gas-phase composition com-
bined with modeling may provide a much-needed increase in
understanding the particle growth process.

## 2 Methods

The data utilized in this study were collected at the Chacaltaya GAW station during April and May 2018. The Chacaltaya Station is a high-altitude measurement station (lat. -16.350500°, long. -68.131389°; 5240 m a.s.l.) on a slope of the Chacaltaya mountain, which is part of a mountain ridge of the Bolivian Andes. The air masses arriving at the station have varying origins, including the metropolitan area of La Paz, the Altiplano plane, the Pacific Ocean, and Amazonia (Chauvigné et al., 2019; Wiedensohler et al., 2018; Scholz et al., 2023). Altogether, 36 NPF events were detected during the entire measurement period over April and May 2018. We restrict the analysis to 14 events (11, 15 to 17, 21, and 22 April and 10, 13, 22, and 26 to 30 May; see Table S1 in the Supplement). The rest of the detected NPF events were left out of the analysis due to the lack of measurement data of one or several of the most important input parameters for the model or due to problems with instrument calibration. To analyze particle growth, we performed simulations with the particle condensation model constrained by measured vapor concentrations and compared the simulated particle growth with the observed growth based on particle size distribution measurements. By using measured vapor concentrations, we are simulating how these vapors can grow the freshly formed particles.

## 2.1 Instrumentation

Oxygenated organic vapors were measured with a Filter In-
let for Gases and AEROsols (FIGAERO) coupled with a
time-of-flight chemical ionization mass spectrometer (ToF-
CIMS) with iodide as reagent ion (Lopez-Hilfiker et al.,
2014). The FIGAERO-CIMS has two operational modes
and monitors gas and particle-phase organic composition
semi-continuously. The duration of the gas-phase mode was
120 min, and it samples ambient air directly into the ion-
molecule reactor (IMR). During the gas-phase mode, parti-

cles are simultaneously collected on a 25 mm polytetrafluoroethylene (PTPE) filter through another sampling port with a flow of 3.8 slpm (standard liter per minute). When the gas-phase measurement (particle collection) is done, the FIGAERO inlet is switched to the particle desorption mode and a heated nitrogen gas flow (2 slpm) is blown through the filter to evaporate the particle-phase compounds via temperature-programmed desorption. The duration of the particle deposition period was 50 min. More details about the instrument can be found in Lopez-Hilfiker et al. (2014) and Thornton et al. (2020). For each gas-phase measurement (120 min), we calculated four 30 min averaged data points.

For the conversion of the measured ion signal to mass con-
centrations, we took a maximum sensitivity of 20 cps pptv⁻¹
(counts per second per parts per trillion by volume) (per mil-
lion cps of reagent ion) from Lopez-Hilfiker et al. (2016) and
adjusted that for the different IMR pressure and flows go-
ing to the IMR in our measurements compared to the condi-
tions in Lopez-Hilfiker et al. (2016). In our study, the flow
containing iodide ions was 1.3 slpm. Due to using a corona
source (in April) and an X-ray ionizer (in May) as ioniza-
tion sources, the IMR pressure was set to 100 mbar in April
and 480 mbar in May. The gas-phase sample flow was con-
trolled by a critical orifice. With an ambient pressure of
about 530–540 mbar, the sample flow was about 1.1 slpm and
0.7 slpm in April and May, respectively. The ionizer and sam-
ple flows mix and interact in the IMR. The sensitivity due to
the changes in IMR pressure and the sampling flows (thus
the residence time of reagent ion and analytes, as well as the
time for their reaction) was 30 and 140 cps pptv⁻¹ in April
and May, respectively (for details see Supplement).

Gas-phase sulfuric acid concentration as well as organic
compounds were measured with a nitrate-CIMS (Tofwerk
AG, Thun, Switzerland). The especially designed inlet for
chemical ionization at ambient pressure is described by
Kürten et al. (2011) and Jokinen et al. (2012). The nitrate-
CIMS uses nitrate anions [(HNO₃)n (NO₃⁻), n = 0–2] as
reagent ions to ionize gas molecules. The sampling flow
was 10 slpm, mixed with 20 slpm sheath flow before detec-
tion. The signal of the detected compound in counts per
second is normalized to the sum of count rates of reagent
ions and then multiplied with the calibration coefficient
C = 1.5 × 10¹⁰ cm⁻³, which was determined after the cam-
paign using H₂SO₄ as calibrant, following the procedure by
Kürten et al. (2012). As the nitrate-CIMS was mainly sen-
sitive to highly oxygenated organic molecules (HOMs), we
compared the organic compounds measured by the nitrate-
CIMS and the FIGAERO iodide CIMS, and the absolute
amount of organics detected by the nitrate-CIMS was much
lower than that detected by FIGAERO–CIMS; thus, we
only used the organic vapor concentrations from FIGAERO–
CIMS for further modeling (Fig. S1).

The particle number size distribution was measured us-
ing a neutral cluster and air ion spectrometer (NAIS, Mirme
and Mirme, 2013) and a mobility particle size spectrom-
eter (MPSS, design TROPOS; Wiedensohler et al., 2018). The NAIS measured neutral and charged particles in the size range of 1–70 nm in diameter divided into 29 size bins. The time resolution of the NAIS data was 3.5 min. The MPSS detected particles in the size range 10–500 nm divided into 71 size bins with a time resolution of 2.5 min. The particle diameter in MPSS refers to dry size. As the particle sample transfers from outside ambient air to NAIS instrument, the temperature increase and RH decrease lead to evaporation of water. Due to a lack of information on the extent of water evaporation inside the instrument, the measured size in NAIS was also assumed to correspond to dry size in this study. In the analysis for acquiring the growth rates from measurements (see Sect. 2.3), only NAIS data were utilized. For the rest of the analysis involving particle number size distributions, NAIS data for particles from 3 to 30 nm and MPSS data for particles larger than 30 nm were combined to obtain a size distribution for the size range of 3–500 nm.

An automatic weather station (AWS) deployed in the main observatory recorded air temperature, relative humidity (RH), radiation, wind direction, and wind speed at a 1 min resolution.

## 2.2 Model

The particle growth model used in our analysis is the Model for Oligomerization and Decomposition in NAnoparticle Growth (MODNAG) introduced by Heitto et al. (2022). In this study, however, we only use the condensation part of MODNAG and exclude the oligomerization and decomposition, since the particle-phase reactions are omitted from this study for simplicity and due to the lack of data on relevant properties to constrain them. The model is a single aerosol particle condensation model, where condensation of organic vapors, sulfuric acid, ammonia, and water are considered. In this study measured vapor concentration of organic vapors and sulfuric acid were used as an input. It is worth noting that by doing this the reduction of ambient vapors by condensation sink is also indirectly taken into account in the model. The mass flux of each organic vapor and sulfuric acid between the gas and particle phase is calculated based on the difference between their ambient gas-phase concentrations and equilibrium vapor mass concentrations according to (Lehtinen and Kulmala, 2003)

$$ \frac{dm_j}{dt} = 2\pi (d_p + d_j)(D_p + D_j)\beta_{m,j}(C_j - C_{eq,j}), \quad (1) $$

where $d_j$ is the molecular diameter (m) and $D_j$ the gas-phase diffusion coefficient of the condensing compound j (m$^2$ s$^{-1}$); $C_j$ is the gas-phase mass concentration and $C_{eq,j}$ the equilibrium vapor mass concentration of compound j, respectively (note that both are here converted to units of kg m$^{-3}$); and $d_p$ is the diameter (m) and $D_p$ the diffusion coefficient of the particle (m$^2$ s$^{-1}$). $\beta_i$ is the transition regime correction factor. $C_{eq,j}$ is calculated based on the solution

effect and Kelvin effect as (e.g., Seinfeld and Pandis, 2016)

$$ C_{eq,j} = \gamma_j \chi_j C_{sat,j} \exp \left( \frac{4\sigma v_j}{RT d_p} \right), \quad (2) $$

where $\gamma_j$ is the activity coefficient, $\chi_j$ the mole fraction, $C_{sat,j}$ the pure compound saturation vapor concentration, $v_j$ the molar volume of compound j, $\sigma$ the surface tension of the particle, R the gas constant, and T the temperature. In this study we assume an ideal solution, and therefore the activity coefficient $\gamma_j$ is equal to 1.

$\beta_i$ in Eq. (1) is defined as (Fuchs and Sutugin, 1970)

$$ \beta_j = \frac{1 + Kn_j}{1 + \left( \frac{4}{3\alpha_{m,j}} + 0.377 \right) Kn_j + \frac{4}{3\alpha_{m,j}} Kn_j^2}, \quad (3) $$

where $\alpha_{m,j}$ is the mass accommodation coefficient and $Kn_j$ is the Knudsen number. In this study, $\alpha_{m,j}$ is assumed to be unity for all components. $Kn_j$ is defined as (Kulmala and Lehtinen, 2003)

$$ Kn_j = \frac{2\lambda_j}{d_p + d_j}, \quad (4) $$

where $\lambda_j$ is the mean free path of the condensing molecule, which is calculated as

$$ \lambda_j = \frac{3(D_p + D_j)}{\sqrt{c_p + c_j}}, \quad (5) $$

where $c_p$ and $c_j$ are the mean thermal speed of the particle and the condensing compound j, respectively.

In this study, we simulated a system that contains nine model compounds: six organic compounds (volatility bins), sulfuric acid, water, and ammonia. The mass fluxes of organics and sulfuric acid between the gas and particle phases are calculated in the model using Eq. (1). The particle water content is updated constantly by assuming that water is in equilibrium between the gas and particle phases. The amount of ammonia in the particle phase is calculated by requiring it to match a 1 : 1 molar ratio with sulfuric acid. This simplified assumption was necessary as gas-phase ammonia concentration data were not available. Due to the small mass of the ammonia molecule, this assumption does not cause significant uncertainty in the simulation results.

The six organic compounds are proxies for the measured organic vapors. For each measured organic compound, we assigned a saturation vapor mass concentration ($C_{sat}$) value at 298 K based on their molecular formula using the volatility parametrization by Li et al. (2016) and the temperature dependence of $C_{sat}$ by Epstein et al. (2010). Based on their volatilities, the observed organic compounds were then divided into six groups and represented with the volatility basis set (VBS, Donahue et al., 2006). The VBS bins ranged from $10^{-4}$ to $10^1$ µg m$^{-3}$ at 298 K. All compounds with a $C_{sat}$ lower than $10^{-4}$ µg m$^{-3}$ (all ELVOCs) were included
in the lowest volatility bin, and compounds belonging to the bins with $C_{sat}$ higher than $10^1 \mu g m^{-3}$ (most SVOCs and everything more volatile) were neglected. This was done as our sensitivity tests showed that all compounds with $C_{sat}$ of $10^{-4} \mu g m^{-3}$ or lower are effectively non-volatile from the point of view of the particle growth simulation in this study and that the contribution of compounds with $C_{sat}$ higher than $10^1 \mu g m^{-3}$ to the particle growth is negligible. The sum of the concentrations of the vapors in each VBS bin was assigned for the concentration of the corresponding organic model compound (i.e., VBS bin). The molar mass and gas-phase diffusion coefficients of the model compound were calculated as gas-phase-concentration-weighted averages of the compounds belonging to the respective VBS bin.

The time resolution of the model input data was 30 min; i.e., in the beginning all measurement data were averaged over 30 min. For each simulation time step, the properties and concentrations of organics as well as ambient temperature, pressure, and RH were linearly interpolated from the input data. For most of the time, a similar approach was also used for sulfuric acid. However, there were some gaps in the sulfuric acid data measured in April lasting over several hours. For these gaps in the data, the interpolation between measurements was not sufficient because of the strong diurnal variation of sulfuric acid concentrations. Instead, for these cases with missing sulfuric acid data (16 and 17 April) we approximated the concentration with a Gaussian distribution. For this, first the mean and standard deviation of the distribution were determined by fitting a Gaussian distribution to normalized sulfuric acid concentrations of all NPF days in May with constant air mass (see Sect. 2.3). Then the amplitude of the distribution for the day with gaps in the data was defined by fitting it to the available sulfuric acid data on that specific day. Illustration is shown in Fig. S2a–b.

The initial particle size in the model was approximately 2 nm, containing 40 molecules of sulfuric acid and ammonia and particle-phase water corresponding to gas–particle equilibrium. This small size was selected to minimize the influence of assumed initial particle composition on the simulated growth. The first geometric mean diameters of growing nucleation mode were detected typically starting at around 7–10 nm, depending on the day; and in these sizes, with the selected small initial size, the initial composition covers less than 5% of the simulated particle mass. The choice of starting time (onwards presented as local time, UTC–4) of the model simulation was not straightforward. To define a suitable starting time for the simulation, a number of simulations were performed with a range of starting times (with a 30 min resolution). We then calculated the root-mean-square difference between the simulated particle diameter and the geometric mean diameter of the observed nucleation mode to find the best-fit simulation. For this, only the geometric mean diameters up to 10 nm were considered to find the best fit for the beginning of the particle growth and to allow for a comparison of simulated and observed growth. On 6 d (16 April

and 13, 26, 27, 28, and 30 May 2018), however, the simulated growth reached the 7–10 nm size range later than the observed geometric mean diameter of the nucleation mode regardless of the starting time of the simulation; i.e., it was not possible to find a match between simulation and observations in this size range by adjusting the simulation starting time. In these cases, the gas-phase concentrations of organics and sulfuric acid were so low during the morning that the particle in the simulation grew to 7 nm very slowly. For these days we selected a simulation where the starting time was set at the time of sunrise, based on the assumption that the nucleation and the initial growth are mostly governed by sulfuric acid, the concentration of which is highly dependent on solar radiation (Mikkonen et al., 2011).

## 2.3 Calculating growth rates from observations and model

For calculating the particle diameter growth rates from observations, we used the method introduced by Dal Maso et al. (2005). The GR values were derived from the size distribution data measured with the NAIS. In this method, first, the geometric mean diameter of the nucleation mode at each time point is found by fitting a multi-modal log-normal size distribution to the measured particle number size distribution. Then, a straight line is fitted to the data points of time and geometric mean diameter over the growth period of the freshly nucleated particles to obtain the GR value. However, not all these data points were always included when fitting the line for the GRs as the geometric mean diameters did not always reflect a smoothly growing mode. Therefore, linear fitting was performed on different subsets of these data points, selected by inspecting the size distribution evolution. The fit that was estimated to best reflect the growing mode was selected as the base value, and different versions of the fit provided the uncertainty range. The GR values correspond mostly to the size range of 6–50 nm; however, the size range differs between days depending on the part of the growing mode from which the GR value was obtained most reliably. Such an approach was chosen as the aim was to compare observed and simulated particle growth.

From the modeled data, the GR was calculated from the change in the dry size of the particle (i.e., water excluded) during the period corresponding to the experimentally defined growth rate. This means that for each fitted GR from the measurements, a matching GR was defined from the models. When presenting the GR values, the base value of the GR from the model is the GR calculated from the same period as the base value from the measurements, and, analogous to measurements, the GRs from other periods provide the uncertainty range. On 6 d (10, 13, 22, and 28 to 30 May) two consecutive events were detected on the same day. For these days, only the first event is included in the analysis due to the challenges of separating particles nucleated from separate events.
The analysis of the growth during NPF events based on
observations requires – or includes an assumption – that the
air mass around the measurement site stays relatively homo-
geneous (regional NPF event) under stable atmospheric con-
ditions. A similar assumption is made when comparing the
simulations, constrained by observed vapor concentrations,
to the measured growth of the particles. This, however, may
not be the case for all of the events at the Chacaltaya sta-
tion. The complex topography of the surrounding area and
the varying source areas of aerosols make it possible for air
masses to change rapidly in the area, and the site is often
affected simultaneously by air masses originating from mul-
tiple source regions (Aliaga et al., 2021).

On 4 d (21 and 22 April and 26 and 27 May), around noon there was a sharp increase in the particle and organic vapor concentrations, especially in SVOC and LVOC concentrations, as well as in black carbon (BC) concentrations. This phenomenon was also reported by Aliaga et al. (2021), who concluded that this is an indication that a larger fraction of air mass had been in contact with the surface in the previous few days. The increased BC concentrations during these high-concentration periods (see Fig. S3) further indicate that the air mass has been influenced by the La Paz–El Alto metropolitan area. In the following, these days are addressed as days with inconstant or inhomogeneous air mass, and the rest of the days are addressed as days with constant or homogeneous air mass, respectively. We acknowledge that the air mass is probably not perfectly homogeneous all around the site in any of the studied events. However, the only subtle changes in measured particle number distributions and vapor concentrations imply that no drastic changes in air mass were occurring on events referred to in this study as days with homogeneous air mass. In April and May, the influence of air mass with high particle and vapor concentrations might last until the afternoon. In these cases, the changes in the particle size distribution observed at the station cannot be interpreted as continuous condensational growth of one particle population, and our model is not, in theory, expected to simulate the changes in particle size correctly. We applied our standard model simulations also for these days; however, we performed also additional simulations for these cases to address the issue of air mass changes. By assuming that the particles observed before and after the period with elevated particle and vapor concentrations are from the same air mass, we performed simulations for the growth during the NPF event by neglecting the measurements during the high-concentration period (i.e., surface-influenced air mass from the La Paz) and instead predicting what the conditions would have been in the original air mass, before the stark increase in particle and vapor concentrations. See Supplement for the details.

3 Results and discussion

Figure 1 shows the measured and modeled growth rates for each of the 14 NPF days included in the analysis. The figure shows with different markers the NPF events for which air masses were estimated to be fairly homogeneous throughout the growth (filled markers) and the events for which changes in air mass were assumed to affect the particle size distribution evolution and measured gas-phase concentrations (empty markers). The median and mean of measured GRs for the entire size range (~5–60 nm, depending on the event; see Table S1) were 2.0 and 2.6 nm h⁻¹ for all 14 d and 1.5 and 1.7 nm h⁻¹ for days with homogeneous air mass, respectively. This is notably slower than the median GR for April and May (9.92 and 5.82 nm h⁻¹ for the size range of 3–7 nm and 5.12 and 9.03 nm h⁻¹ for the size range of 7–20 nm, respectively) and the annual mean GR (10.31 and 13.65 nm h⁻¹ for size ranges of 3–7 and 7–20 nm, respectively) reported from the same site in previous studies (Rose et al., 2015; Sellegri et al., 2019). However, due to the limited data set in our study, this is not necessarily an indication of discrepancy.

It is also worth noting that the GRs in the previous stud-
ies were defined using the maximum concentration method
(Hirsikko et al., 2005), i.e., a different method compared to
this study. In the maximum concentration method, the GR
is determined by a linear fit to the data points of moment
of maximum concentration of each size bin, while in the so-
called mode-fitting GR method used in this study, the GR
is obtained by a linear fit to mode geometric mean diam-
eters determined at each moment. At the boreal forest site
Hyytiälä, the GR values calculated with these two methods
had an average relative difference of 16%, with the maxi-
mum concentration method typically producing higher GR
values (Yli-Juuti et al., 2011). Therefore, the difference in
obtained GR values between this study and the previous stud-
ies for the Chacaltaya site is larger than would be expected
from solely the differences in GR calculation methods. How-
ever, the growth rates calculated for high-altitude sites are ap-
parent growth rates, as the upslope winds and particle trans-
port may affect the values (Sellegri et al., 2019). It is there-
fore possible that the two methods are affected differently,
and we cannot exclude the possibility that the differences in
GRs between the studies are affected by the choice of GR
calculation method. In the previous study, Rose et al. (2015)
found that the GRs at the site are generally higher during the
wet season (November to April) than during the dry season
(May to October). The GRs determined in this study, how-
ever, showed the opposite, with the median GR in May being
higher than in April (2.2 and 1.1 nm h⁻¹, respectively), albeit
the highest GR value, exceeding 9 nm h⁻¹, was measured in
April. The deviation in our study from the seasonal differ-
ence in GR reported by Rose et al. (2015) can be related to
our study taking place at the transition period between the
seasons and including a limited number of NPF events.
For the analyzed events in April (squares in Fig. 1), the model overpredicted the growth, while during May (circles) for some events the modeled growth was overpredicted and for some events underpredicted. In April, sulfuric acid had very little contribution to the simulated particle growth (at a maximum 1.2% of particle mass of a 30 nm particle), whereas in May it had a large contribution during most events, as shown in Fig. 2b. This is in line with the sulfuric acid gas-phase concentrations being higher during May than during April (average concentrations during the analyzed events were $6.8 \times 10^6$ and $8.3 \times 10^5$ molec.cm$^{-3}$, respectively) due to occurrence of volcanic emissions in the area (Bianchi et al., 2022; Aliaga et al., 2021). This increase is illustrated in Fig 2a. The LVOC and ELVOC concentrations, on the other hand, were lower during May compared to April (average vapor concentrations during analyzed events for LVOCs were $2.3 \times 10^7$ and $6.0 \times 10^7$ molec.cm$^{-3}$ and for ELVOCs were $7.5 \times 10^5$ and $2.1 \times 10^6$ molec.cm$^{-3}$, respectively). Due to these differences in vapor concentrations, the simulated particle growth was dominated by LVOCs in April, while in May both LVOCs and sulfuric acid made a major contribution to particle mass. This is evident from mass fractions presented in Fig. 2b, which show the relative contributions of detected vapors on the simulated particle mass at 30 nm. It is worth noting that the variability of the growth rate in the simulation and the uncertainty of the measured GR are large for some events. This is due to the large variability in fitted GR values between the selected subsets of data points used to define the growth rates, as described in Sect. 2.3, and originates as the consecutive geometric mean diameters of nucleation mode exhibit deviation from a straight line. For the simulated GR, additional uncertainties are caused by uncertainties in measured organic vapor concentrations, which can be of ±50% (Mohr et al., 2019), and saturation concentrations of organic compounds, which can span over orders of magnitude (O'Meara et al., 2014). The effect of these possible uncertainties on the simulated GR is shown in Fig. S4. The modeled growth rate was sensitive for assumed ±50% uncertainty in the organic concentrations. This is the case, especially for growth events in April, for which model simulations shown in Fig. 1 overestimated the GR, while reducing the organic concentrations by 50% decreased the modeled GR to values lower than the measured GR. For April events the simulations with the assumed upper and lower limit of uncertainty for organic concentrations led to a large spread in the simulated GR. In May, on the other hand, the ±50% uncertainty in organic concentration affected the simulated GR less. The difference in the effect of uncertainty of organic concentrations between April and May is related to the higher organic concentrations in April compared to most events in May. The assumption of ±50% uncertainty in sulfuric acid concentration had a smaller effect on the simulated growth (Fig. S3).

Figure 3 presents the simulated particle growth compared to the measured evolution of particle size distribution and

<figure><img src="image_4.png" /></figure>

**Figure 1.** Modeled vs. measured growth rates of particles. Data from April and May are shown with squares and circles, respectively. The cases where air masses were estimated to be fairly homogeneous throughout the growth event (const) are shown with filled markers, and the cases where changes in air mass were assumed to affect the particle size distribution evolution (inconst) are shown with empty markers. The marker color describes the ratio of sulfuric acid and LVOC mass in the simulated particle at the last time point used to define the measured growth rate. The error bars in the measured GR represent the different GRs obtained using different subsets of nucleation mode peaks during the event. The error bars in the modeled GR represent the GRs calculated from the simulation for the same time frame as the corresponding GRs from measurements.

gas-phase concentrations of organics and sulfuric acid for four example days, 15 and 22 April and 10 and 27 May. Similar figures for all 14 d considered are presented in Fig. S4. The horizontal line visible at 30 nm in Fig. 3 results from combining the data from two instruments, NAIS and MPSS, which were not intercalibrated and compared to each other.

Each panel in Fig. 3 represents one category of days indicated by different markers in Fig. 1 (for rest of the days, see Fig. S5). Figure 3a shows an NPF event during April with relatively homogeneous air mass during the event (filled squares in Fig. 1, 4 d). On these days the gas-phase concentrations of organics stayed relatively constant and sulfuric acid concentrations were low. The measured GRs were between 0.9 and $1.4 \text{ nm h}^{-1}$ and modeled between 2.1 and $3.2 \text{ nm h}^{-1}$. The growth was overpredicted by the model for all these days. The simulated particle growth was dominated by LVOCs, although also ELVOCs had a clear role (8 to 10% of the mass in the 40 nm particle), as shown in Fig. 2.

Figure 3b shows an NPF event during April with changing air mass during the day (squares in Fig. 1, 2 d). The change in air mass can clearly be seen in the particle-phase measurements. Around 10:00 to 11:00 local time (UTC-4), within 1 h after the NPF event appeared, particle concentrations increased rapidly over a wide size range. Then, in
<figure><img src="image_5.png" /><figcaption>**Figure 2.** (a) Mean vapor concentrations of sulfuric acid and organics and (b) mass fractions of different compounds in the 30 nm particle in the model simulation for each analyzed day of NPF. The units “#/cm³” refer to molecules per cubic centimeter.</figcaption></figure>

<figure><img src="image_6.png" /><figcaption>**Figure 3.** Modeled particle growth (blue line), fitted geometric mean diameters of nucleation mode (cyan diamonds), measured particle size distribution, and measured gas-phase concentrations of organics and sulfuric acid (black lines with solid markers) as a function of time (local time, UTC-4) in (a) April with a homogeneous air mass, (b) April with an inhomogeneous air mass, (c) May with a homogeneous air mass, and (d) May with an inhomogeneous air mass. The particle diameter for the measured size distribution, modeled particle growth, and geometric mean diameters of nucleation mode is on the left y axis. Gas concentrations are on the y axis on the right.</figcaption></figure>
the afternoon, the particle concentrations decreased rapidly. The changes in organic vapor concentrations were, however, more subtle, and almost no change is seen in the ELVOC and LVOC concentrations. The measured growth rates were 2.2 and 9.5 nm h⁻¹, and the modeled GRs were 3.6 and 10.6 nm h⁻¹, respectively, for the 2 d in this category. For these days, too, the growth was dominated by LVOCs.

Figure 3c shows an NPF event during May with a relatively homogeneous air mass (filled circles in Fig. 1, 6 d). In May, sulfuric acid concentrations were high, and the organic vapor concentrations had some variability during the day. The measured growth rates were between 1.1 and 4.0 nm h⁻¹, and the modeled GRs were between 0.9 and 2.6 nm h⁻¹. For four of these 6 d, the growth was underpredicted (13 and 28 to 30 May), and for 2 d it was overpredicted (10 and 22 May). The main contributors to the growth were LVOCs and sulfuric acid.

Figure 3d shows an NPF event during May with a change in air mass (circles in Fig. 1, 2 d). On these days, the change in particle size distribution can most clearly be seen in the increase in > 100 nm particles. For the organic vapor concentrations, the change is clearly seen as a rapid increase in SVOC and LVOC compounds. The measured GRs for these 2 d were 2.3 and 4.9 nm h⁻¹, and the modeled GRs were 2.7 and 4.8 nm h⁻¹, respectively. The most important contributors to the growth were LVOC compounds, and unlike the other events in May with constant air mass, sulfuric acid had a negligible effect (see also Fig. 2b).

Considering the relative differences between measured and simulated GRs, no differences can be found between the different types of days described above. Interestingly, the model runs captured the GR values and changes between days rather well for the days with air mass changes, even though in theory the model is not sufficient to capture the effects of air mass changes on particle composition. For 6 out of 10 of the constant air mass days, the model captured the GR values within a factor of 2. Generally, the results suggest that the detected vapors and their measured concentrations are able to cover a large fraction of the observed particle growth. However, the model did not fully capture the variation between days, and no systematic difference between measured and modeled growth was found. This suggests that some significantly contributing vapors or factors were missing in the model input, i.e., not detected by the instruments. At the same time, due to occasional overestimation of the GR, this could also imply that the model is too efficient in condensing gases that it has. Alternatively, it may also be that the detected size distribution was significantly affected by processes not accounted for in the model. For instance, while sudden changes in air mass can be identified from the data, more gradient changes may not be noticed. Such factors may contribute to the differences between the observed and simulated particle GRs.

The difference between simulated and observed growth was further analyzed by calculating correlation coefficients

<table><caption>**Table 1.** Correlation coefficients (r) and (P) values of absolute and relative differences between measured and modeled growth rate against different parameters.</caption><thead><tr><th rowspan="2"></th><th colspan="2">GR<sub>meas</sub> - GR<sub>model</sub></th><th colspan="2">GR<sub>meas</sub>/GR<sub>model</sub></th></tr><tr><th>r value</th><th>P value</th><th>r value</th><th>P value</th></tr></thead><tbody><tr><td>H<sub>2</sub>SO<sub>4</sub> concentration</td><td>0.21</td><td>0.47</td><td>0.10</td><td>0.73</td></tr><tr><td>LVOC concentration</td><td>-0.51</td><td>0.060</td><td>-0.44</td><td>0.12</td></tr><tr><td>ELVOC concentration</td><td>-0.75</td><td>0.0021</td><td>-0.69</td><td>0.0065</td></tr><tr><td>Wind speed</td><td>-0.58</td><td>0.064</td><td>-0.42</td><td>0.20</td></tr><tr><td>Wind direction</td><td>0.66</td><td>0.028</td><td>0.76</td><td>0.0070</td></tr><tr><td>Temperature</td><td>-0.43</td><td>0.19</td><td>-0.41</td><td>0.21</td></tr><tr><td>RH</td><td>-0.077</td><td>0.82</td><td>-0.055</td><td>0.87</td></tr></tbody></table>

between the relative and absolute difference between measured and modeled GRs and various parameters included in the analysis (i.e., concentration of organics, sulfuric acid, RH, T, wind speed, wind direction; see Table 1 and Fig. S6). There was a strong negative correlation for the difference in GR (measured GR - modeled GR) with ELVOC concentration. With low (relative to analyzed days) ELVOC concentrations (~0.5 × 10⁶ molec. cm⁻³) the growth was mostly underestimated in the model, and with high ELVOC concentrations (~2 × 10⁶ molec. cm⁻³) the growth was overestimated in the model. With intermediate ELVOC concentrations the growth was slightly overestimated (Fig. S5). Statistically significant negative correlation was also found for the difference in GR values and LVOC concentration, temperature and wind speed, and positive correlation between the difference in GR and wind direction. The correlations between the difference in GR values and concentrations of organic vapors may be related to the calibration of the measurement instrument, the uncertainties of saturation concentrations of organic compounds, or the fact the instrument did not measure the entire distribution of compounds. However, the model is not sensitive to air temperature, wind speed, and wind direction, which are not included in the model at all. This suggests that the underlying reason for the differences is not necessarily directly dependent on these variables on themselves but may lie in, e.g., changes in air mass (and hence changes in chemical composition) that our model fails to capture.

As seen in Fig. 1, cases with an inhomogeneous air mass did not differ significantly from cases with a homogeneous air mass in terms of agreement between measured and simulated particle growth, although overall the GRs were larger on days with an inhomogeneous air mass. In May, the days with inhomogeneous air mass even showed slightly better relative agreement between measured and modeled GRs than most days with constant air mass. However, as discussed above, if the air mass changed during the event, the particles measured in the beginning represent a different particle population compared to the particles measured after the air mass change, and, consequently, the GR value calculated from the changes in nucleation mode geometric mean diameter may
not represent the real condensation growth rate. The sudden
changes in particle size distribution also led to different GR
values depending on which nucleation mode mean diameter
data points were included in the calculation of the GR, which
results in large uncertainties as indicated in Fig. 1. Also, the
model simulates the growth of one particle from the start of
the NPF to the end of the simulation, so even if the model
seems to capture a similar behavior to that observed in the
particle size distribution measurements, they may not repre-
sent the same processes if the air mass is not homogeneous.

The results show that the size of particles evolving in the
air mass detected in the morning and again possibly in the af-
ternoon may have had a notably slower GR compared to the
overall measured particle population. However, since only
the ensemble particle population can be measured, it is hard
to make any profound conclusions about how well our model
captures the growth in the air mass measured in the morning
for the cases with inhomogeneous air mass (see Fig. S7 for
more information).

## 4 Conclusions

We simulated the particle growth during NPF events at the
Chacaltaya GAW station based on detected organic vapor
and sulfuric acid concentrations for 14 NPF events dur-
ing April and May 2018. For most events (9 out of 14),
the model-simulated GR was within a factor of 2 of the
measurement-based value. According to the model simula-
tions constrained by detected vapor concentrations, the main
contributors to the growth were organic vapors, especially the
LVOC compounds. However, during several NPF events, sul-
furic acid had a major role, and it contributed in some cases
almost half of the simulated particle dry mass at 40 nm. This
implies that sulfuric acid from volcanic emissions (Bianchi
et al., 2022; Aliaga et al., 2021) also had a notable contribu-
tion to the particle growth in the area in May. The effect of
sulfuric acid on particle growth at the site is thus expected
to be highly dependent on volcanic activity as this effect was
not seen in previous studies when volcanoes were less active
(Rose et al., 2015).

Our results suggest that the detected vapors and their mea-
sured gas-phase concentrations were able to explain a large
part of the observed growth. However, based on the differ-
ences between measured and simulated growth rates, and
particularly due to the low performance of the model in cap-
turing the variation in GRs between days, it seems possible
that some significantly contributing vapors were not detected
and included in the model, properties of the condensing com-
pounds were not correctly estimated, and/or some other fac-
tors not included in the model were significantly affecting
the growth. The differences between measured and modeled
growth rates might have been affected by the difficulty in de-
termining the growth rate from the particle number size dis-
tribution during the campaign. Uncertainty in measured va-

por concentrations and estimated saturation vapor concentra-
tions of organic vapors may also contribute to the differences
between measured and simulated growth rates. Especially for
NPF events in April, the observed nucleation mode growth
was within simulations with assumed ±50% uncertainty in
the organic concentrations. As the growth rate was overes-
timated in simulations for all of the cases in April, uncer-
tainties in measured vapor concentrations are one potential
contributor to differences between model outputs and obser-
vations at least for April. In May, the growth rate was both
overestimated and underestimated, and therefore uncertainty
in vapor concentrations is less likely an explanation. Due to
the differences in the FIGAERO-CIMS instrument setup be-
tween April and May, uncertainties in the organic vapor con-
centrations may have affected results differently between the
2 months.

These results provide insights into the key factors affecting
the particle growth in this high-altitude location, particularly
the main vapors condensing onto the nanoparticles, high-
lighting the importance of low-volatility organic compounds
and, in addition, sulfuric acid during volcanic-activity peri-
ods. The results also demonstrate that the contribution of dif-
ferent vapors to the particle growth may vary between days
for this location. However, due to the uncertainties associ-
ated with the simulations, the results should not be inter-
preted as an exact but indicative representation of the par-
ticle growth. Also, the complexity of the surrounding topog-
raphy, meteorology, and source areas of air masses make it
challenging to define whether the measured particle popula-
tion stays the same during the observed event. Nevertheless,
as data on condensing vapors and studies that quantitatively
connect these data to nanoparticle growth are still scarce for
many atmospheric environments, especially on the Southern
Hemisphere, these results contribute to building an overall
understanding of NPF and particle growth to CCN sizes. Due
to the indicated dominant effect of organic vapors on the par-
ticle growth, the results highlight the importance of improved
knowledge of organic vapor properties and further develop-
ment and application of measurement techniques to identify
the wide selection of organic vapors in atmospheric environ-
ments.

**Code availability.** The code for MODNAG is available at
https://doi.org/10.5281/zenodo.8336713 (Heitto, 2023).

**Data availability.** The data sets are available upon request from
the corresponding authors.

**Supplement.** The supplement related to this article is available
online at: https://doi.org/10.5194/acp-24-1315-2024-supplement.
**Author contributions.** AH, CW, CM, and TYJ designed the study. AH conducted the simulations. CW, DA, LB, XC, RC, YG, LH, WH, PL, KS, KW, AW, QZ, FB, and CM provided observational data. FV, IM, and MA provided logistic support for the campaign and meteorological data from Chacaltaya. AH, CW, KEJL, CM, and TYJ analyzed the results. AH and TYJ prepared the manuscript with contribution from all co-authors.

**Competing interests.** At least one of the (co-)authors is a member of the editorial board of *Atmospheric Chemistry and Physics*. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.

**Disclaimer.** 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.** We acknowledge the IRD (Institut de Recherche pour le Développement) delegation in Bolivia for assisting with logistics and customs clearance for the instruments and the personnel of IIF-UMSA for assisting with the station functioning, maintenance, and electric troubleshooting. The instrumental deployment at the GAW station used in this study is supported by an international consortium funded by IRD, Centre National de la Recherche Scientifique (CNRS) and Ministère de la Recherche (under ACTRIS-FR activities), ICOS Network, Observatoire des Sciences de l'Univers de Grenoble (under Labex OSUG@2020), Leibniz Institute for Tropospheric Research, Consejo Superior de Investigaciones Científicas, and University of Stockholm.

**Financial support.** This research has been supported by the Academy of Finland (grant nos. 307331, 337550, and 337549) and the H2020 European Research Council (grant no. 850614).

**Review statement.** This paper was edited by Fangqun Yu and reviewed by two anonymous referees.

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