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Two-dimensional offline chromatographic fractionation for the characterization of humic-like substances in atmospheric aerosol particles Tobias Spranger, Dominik van Pinxteren, and Hartmut Herrmann Environ. Sci. Technol., Just Accepted Manuscript • Publication Date (Web): 23 Mar 2017 Downloaded from http://pubs.acs.org on March 24, 2017
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Two-dimensional offline chromatographic
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fractionation for the characterization of humic-like
3
substances in atmospheric aerosol particles
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Tobias Spranger, Dominik van Pinxteren and Hartmut Herrmann*
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Leibniz-Institut für Troposphärenforschung (TROPOS), Permoserstr. 15, 04318 Leipzig,
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Germany
7
8
Organic carbon in atmospheric particles comprises a large fraction of chromatographically
9
unresolved compounds, often referred to as humic-like substances (HULIS), which influence
10
particle properties and impacts on climate, human health and ecosystems. To better understand
11
its composition, a two-dimensional (2D) offline method combining size-exclusion (SEC) and
12
reversed-phase liquid chromatography (RP-HPLC) using a new spiked gradient profile is
13
presented. It separates HULIS into 55 fractions of different size and polarity, with estimated
14
ranges of molecular weight and octanol/water partitioning coefficient (log P) from 160–900
15
g/mol and 0.2–3.3, respectively. The distribution of HULIS within the 2D size vs. polarity space
16
is illustrated with heat maps of UV absorption at 254 nm. It is found to strongly differ in a small
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example set of samples from a background site near Leipzig, Germany. In winter, most intense
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signals were obtained for largest molecules (>520 g/mol) with low polarity (log P ~ 1.9), while
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in summer smaller (225 – 330 g/mol) and more polar (log P ~ 0.55) molecules dominate The
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method reveals such differences in HULIS composition in a more detailed manner than
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previously possible and can therefore help to better elucidate the sources of HULIS in different
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seasons or at different sites. Analyzing Suwannee river fulvic acid as a common HULIS
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surrogate shows a similar polarity range, but clearly larger sizes than atmospheric HULIS.
24 25
Introduction
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The atmospheric organic aerosol has been a topic of intense research over the past 15 years,
27
because aerosol particles contain a large fraction of organic carbon (OC) besides from inorganic
28
ions, elemental carbon (EC) and silicates. The organic fraction can contribute up to 70 % of the
29
total particle mass1 and therefore alters microphysical particle properties like hygroscopicity2-4,
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surface tension5 and the ability of particles to serve as cloud condensation nuclei (CCN
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activity).4, 6, 7 Thus OC plays an important role for the formation of clouds and the earth radiative
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budget.8 Moreover, organic particle constituents are expected to be involved in a wide variety of
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human health issues9, 10 and are critical because of their input into ecosystems.8
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Despite its importance for humans and environment only a small fraction (5 - 30 %) of OC has
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been identified on a molecular level11, mainly due to its high complexity with thousands of
36
different substances.12, 13 Typically, OC is dominated by a group of substances often referred to
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as humic-like substances (HULIS) with a contribution of 20 - 80 % to the water soluble organic
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carbon (WSOC) in atmospheric aerosol particles.14 HULIS are operationally defined by their
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extraction method from aerosol particles. Currently, different solid phase extraction (SPE)
40
methods are applied, leading to differences in the chemical composition of extracted HULIS.15-20
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The term HULIS originally derived from a proposed similarity to humic and fulvic substances
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from terrestrial systems21, but several studies have shown significant differences to those with
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regard to (i) molecular size22-25, (ii) aromaticity25-27, (iii) elemental composition28 and (iv) CCN
44
activity.2, 6 HULIS can be found in the most different atmospheric environments, such as rural25,
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29, 30
46
be most important source of HULIS, as the highest concentration can be measured there14, 30, 35,
47
36
48
sources are discussed in the literature.40 While newer analytical techniques like ultra-high-
49
resolution mass spectrometry (UHRMS) help to understand the chemical composition better, the
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high complexity of HULIS still remains a major problem.13, 41
, urban30-32, marine32, high alpine28, 33 and tropical rainforest.3, 34 Biomass burning seems to
, but also the secondary formation from volatile organic carbon37-39 as well as potential marine
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Thus, there is a strong need for chromatographic techniques to at least fractionate the complex
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mixture to get a better understanding of its composition. One-dimensional reversed-phase liquid
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chromatography (RP-HPLC) with a linear gradient, however, leads to unresolved broad bands
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with only some individual peaks on top both for HULIS and Suwannee river fulvic acid (SRFA),
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a fulvic acid mixture commonly used as a HULIS surrogate material.42,
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distinct features in the chromatographic signals of humic substances, Hutta et al. proposed a
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stepwise gradient profile demonstrating a separation of terrestrial humic substances into ten
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fractions,42, 43 This method was also applied to a NaOH-extract of aerosol particles, leading to a
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lower number of fractions with only low signal intensities, however. A different
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chromatographic technique commonly applied to complex mixtures of environmental samples is
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size-exclusion chromatography (SEC). Even though in SEC humic substances often resolve into
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one or two broad peaks only, fractions with different average molecular weight could still be
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extracted from these separations.44-47 Three SEC fractions were reported for SRFA, when using
43
To induce more
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an appropriate mobile phase.23, 31, 48 In studies of atmospheric fog or particle extracts, SEC also
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lead to at least three fractions.31, 48 However, inferring size information of the typically rather
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small atmospheric organic compounds ( 25 min) was weakened. Very high
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amounts of MeOH (more than 30 %) deteriorated the separation. 20% MeOH was thus chosen as
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the optimal mixing ratio, consistent with recommendations by the column manufacturer. The
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final mobile phase conditions lead to five partially resolved fractions for all tested filters with
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only small differences in their retention times (RSD 0.7-1.2 %) regardless of the intensity of UV
168
absorption. Even under optimized conditions a baseline separation of individual fraction cannot
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be expected, because HULIS are known to be a very complex mixture of mainly small molecules
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(< 1000 g/mol) and thus only a part of the columns dynamic range is effectively used for the
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separation (roughly 30%).
172 173
Characterization of the SEC fractions.
174
To characterize the five SEC-fractions, UV-Vis and ESI-Time-of-flight (ToF)-MS
175
measurements were performed. The UV-Vis spectra were measured during the 1st-dimension
176
separation with the use of the DAD in a range of 190 nm-500 nm. The absorption maxima
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(Figure 2) are between 204-210 nm with a steady decay of the signal into the visible light range,
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similar to previous literature results.15, 17, 20, 26 Atmospheric organic particulate material with an
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absorption in the near-UV (300-400 nm) and visible light range (>400 nm) is also associated
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with the term “brown carbon” (BrC) and can have an impact on the radiative forcing of the
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atmosphere61. The obtained HULIS spectra thus highlight a linkage between HULIS and BrC.
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The coefficient E2 / E3 (absorption at 250 nm/ absorption at 365 nm) is a parameter indicating
183
relative molecular sizes for aromatic moieties containing molecules in humic/ fulvic acids, and
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dissolved organic matter in river and lakewater.62-65 As larger aromatic molecules have on
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average a stronger absorption at 365 nm than smaller ones due to larger π-systems and stronger
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π-π*-excitation, the E2/E3-value is smaller for larger molecules. HULIS are expected to contain
187
aromatic structures as well, which is why we applied this to study trends in average molecular
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size between the SEC fractions. The averaged E2/E3-values from all filter measurements are
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presented in Table 1 and show a clear (nearly) linear increase for the fractions 1 to 5,
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corroborating a decreasing average molecular size with increasing retention time as expected. In
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the ESI-ToF-MS spectra (Figure S2), a huge variety of signals was observed in all five fractions.
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Their average mass can be calculated with different methods66, here we use the number averaged
193
molar mass MWn and the mass averaged molar mass MWw as defined in eqs. (1) and (2).
194
(1)
=
∑( )
∑( )
195
(2)
=
∑( )
∑( )
196
Mn is an individual m/z value and I the intensity of the corresponding signal. These parameters
197
(MWn and MWw) likely do not accurately reflect the true average molar masses due to different
198
ionization and transmission efficiencies of individual substances in ESI-MS, . The observed mass
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ranges and distributions are also heavily influenced by the instrument settings for ionization and
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transmission. Therefore, the average masses and also the mass spectra shown in Figure S2 only
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serve as relative comparisons between the SEC fractions and should not be used as a comparison
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with other measurements in the literature. Both values show a clear decrease in the average
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molar mass for later eluting fractions in both ionization modes (Table 1). Even though SEC
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retention is determined by hydrodynamic radii and these are not necessarily strictly correlated
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with molecular masses for chemically complex mixtures like HULIS, this result still indicates
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broadly decreasing molecular sizes in the 5 SEC fractions. To characterize the SEC fractions
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further and to investigate the correlation between molar mass and retention time for a complex
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mixture we performed a calibration with a variety of standard substances, which are listed in
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Table S3 and are expected to have at least some similarity to HULIS constituents in terms of
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molecular size and chemical functionalities. This approach is considered superior to the usually
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performed SEC calibration using polymeric standard substances (like PSS, PEG, PMA) since it
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better represents the complexity of atmospheric organic aerosol constituents and also allows for
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more data points in the relevant mass range between 100-1000 g/mol. The calibration curve
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(Figure S3) shows a linear correlation between the logarithmic molar mass and the retention time
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(with R2 = 0.926). Overall, the different characterization approaches clearly show, that molecular
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size is the main separation mechanism for the proposed SEC method, despite the large chemical
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inhomogeneity of HULIS.
218 219
RP-HPLC development.
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Due to its complex nature, resolving all individual constituents of the HULIS mixture with RP-
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HPLC is not possible. Using a typical linear gradient leads to a broad unresolved band with only
222
some superimposed individual peaks, as shown in Figure 3 A. For humic substances and a NaOH
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extract of aerosol particles it was shown that using a stepwise gradient (with increasing content
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of DMF in the organic phase) leads to a somewhat improved fractionation.42 Using a similar
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gradient with ACN or MeOH as organic solvent (due to the higher polarity of atmospheric
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samples compared to soil samples) a comparable fractionation for atmospheric HULIS and
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SRFA was observed as shown in Figure 3 B. Both solvents gave similar results, but ACN was
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preferred due to the weaker background signal and the reduced backpressure in the gradient
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steps. While the stepwise gradient is an improvement over the standard linear gradient with
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respect to inducing distinct features in the UV signal, the purity of the fractions was just around
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70-80 % for a 5-step gradient and even worse for a 10-step gradient. The purity was determined
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by extracting the selected fraction, reinjecting it into the HPLC and measuring its distribution
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over all fractions. A purity of 100 % would result if UV absorption was measured only in the
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selected fraction in the second run with no overlap to neighboring fractions. To improve the
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purity of the fractions, several variants of a new and unique gradient profile were tested. The
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profile consists of repetitively increasing, decreasing, and constant organic eluent fractions,
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which were varied in terms of their slopes and lengths. The final gradient profile is shown in
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Figure 3 C and lead to a highly reproducible separation into 11 fractions with RSDs of start/stop
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retention times of individual fractions < 0.1 % and RSDs of the peak areas < 0.9 % and a fraction
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purity between 95 – 99 %, tested for a selection of samples and fractions. This new gradient
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profile on its own, as a 1D-experiment, yields chromatographic features indicating even small
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differences in the distribution of hydrophobicity within a HULIS sample, which could be easily
243
overlooked with the stepwise or linear gradient profiles. In addition, it is very well suited for
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fraction collection in multidimensional approaches due to the well-defined fraction peaks. To get
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a better understanding of the range of substances expected in the different fractions, a variety of
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substances with different polarities (Table S3) were tested for the fraction they would end up in.
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Compound polarities were characterized by the octanol-water partitioning coefficient P or log P.
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The log P values were calculated using ALGOPS 2.167 and taken as the average from the
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different models in ALGOPS with its corresponding standard deviation. For carboxylic acids, log
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P values were calculated from the non-dissociated form as it should be the dominating form in
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the acidified eluent. The measurements show a linear correlation of log P with the fraction
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number (R2 = 0.784; Figure S4), very similar to the linear correlation of log P with retention time
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obtained from one tested linear gradient (R2 = 0.794, not shown). The retention times from linear
254
gradient run also correlate strongly with the retention times from a spiked gradient run
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(R2 = 0.957). Both results indicate that the spiked gradient has the same separation mechanism as
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a traditional linear gradient. The calibration was therefore used to determine the log P ranges of
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the individual fractions, as shown below.
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2D-Approach.
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To increase the number of fractions HULIS and other samples can be separated into, the
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optimized SEC fractionation was combined with the spiked gradient RP-HPLC in a 2D-offline
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method. Therefore, the five SEC fractions of multiple sample injections were collected,
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concentrated as described in the experimental section, and injected into the RP-HPLC, leading to
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a total of 55 final fractions.
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As a first application, SRFA was analyzed with the new 2D-method. Even though SRFA did not
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show clear peaks in the SEC we separated into 5 fractions within the 1st dimension, splitting the
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main peak at different retention times as shown in Figure 4 A. The results of the fractionation are
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visualized in a heat map constructed from the SEC and RP-HPLC separations on x- and y-axis,
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respectively, and the fraction of total UV absorption at 254 nm on a color scale, indicating the
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signal distribution across the 55 individual fractions. To estimate physical properties from the
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retention times in the two dimensions, we used the above-described calibrations with standard
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compounds. This way the height of each rectangle in the heat map represents a constant log P
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range of 0.31, while the width represents different ranges of molecular weight (MW). It has to be
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noted that the scale direction of the SEC axis has been reversed to give increasing MW along the
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axis. In Figure 4 A, the first fraction thus includes molecules between approx. 320 – 450 g/mol,
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while the molecular ranges for the following fractions are approx. 450 – 550, 550 – 650, 650 –
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750, and 750 – 1000 g/mol. The 2D heat map shows the global maximum of the UV-absorption
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(6.2 % of the total absorption) for molecules between 550 – 650 g/mol with a log P of ~ 1.44.
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Molecules within the same size range but with slightly lower polarity have a similar fractional
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absorption of 6.0 %. The 3rd most intense peak derives from larger molecules (650 – 750 g/mol)
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with lower polarity (log P ~ 2.06) with a fractional absorption of 5.8 %. In general, there is a
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clear trend of increasing polarity with decreasing molecular size for SRFA.
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The obtained results for the size range of SRFA constituents are comparable to data from the
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literature. Stenson et al.68 measured most signals between 350 – 1200 m/z with an ESI-Fourier
285
transform ion cyclotron resonance MS (FTICR-MS) and the highest intensity around 500 m/z.
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This maximum is lower than the one in our measurement, which might be related to a stronger
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UV-absorption of larger molecules. In addition, ESI-MS intensities of individual signals are
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prone to severe interferences from the multitude of analytes and the obtained mass spectra likely
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do not fully represent the true composition.69 For a better comparison with atmospheric HULIS
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samples, the 2D analysis of SRFA was repeated with SEC fraction limits identical to those
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typically applied to atmospheric samples, while the HPLC fractions remained unchanged (Figure
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4 B). For these fraction limits, the majority of the absorption derives from only the first SEC
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fraction for the largest molecules, which is in contrast to the HULIS samples discussed in the
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following, where absorption is distributed across all five fractions.
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Application to atmospheric samples.
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To demonstrate the potential of the developed 2D approach for ambient HULIS samples, we
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analyzed four filter samples from the Melpitz field site near Leipzig, Germany and compared the
300
results among each other and with SRFA. Melpitz is a mid-European rural background station
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with strong influences from continental polluted air masses for eastern wind directions
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(especially in winter) and mixed maritime-continental air masses for western wind directions.70
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To study the variability of HULIS composition under different conditions, filters from summer
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and winter with eastern and western air mass inflow were analyzed (Table S1). For the
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atmospheric implication of these analyses it would helpful to have information about the
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concentrations in each of the 55 fractions, additionally to the fractional absorption. For an
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estimation of concentration from absorption, the UV-absorption of the aqueous filter extracts,
308
defined as total peak area from the SEC measurements, was correlated with the WSOC
309
concentrations measured separately by TOC analysis as described above. The data show a strong
310
linear correlation (R2 = 0.901, Figure S5) for the four filter samples, indicating a good agreement
311
between UV-absorption at 254 nm and the WSOC concentration. With the assumption that the
312
correlation is identical for every fraction, the fractional UV-absorption could be regarded as a
313
measure for the distribution of WSOC within a sample. For a larger number of samples,
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however, it is likely that the observed correlation will be different due to different chemical
315
compositions, depending on the sources of the sampled particles. Additionally, it is also likely
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that the UV-detector response differs within one sample for the different fractions, especially for
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the SEC. Larger, more aromatic substances should have a stronger absorption than smaller ones
318
and therefore, the observed correlation of total absorption with WSOC should be taken with
319
caution and the fractional absorption can just be a rough estimate of the distribution of organic
320
mass in the two-dimensional size versus polarity space.
321
The 2D heat maps of four analyzed ambient samples are shown in Figure 5. A comparison of
322
HULIS (Figure 5) and SRFA (Figure 4) 2D heat maps shows a very similar distribution of the
323
polarity for both sample types, but large differences in the size distribution. For SRFA 80 % of
324
the fractional absorption derives from molecules larger than 520 g/mol. Even for the most similar
325
ambient case WW, this value is only 37 %. Molecules smaller than 450 g/mol are responsible for
326
9 % of the UV-absorption only for SRFA, but 44 – 78 % for the studied HULIS samples, making
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SRFA only very roughly suited as surrogate standard for ambient HULIS.
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The analyzed ambient samples also reveal clear differences between the HULIS extracts. For
329
the winter samples at least two maxima can be identified, the global one for the largest molecules
330
(>520 g/mol) with medium polarity (log P of 1.6-2.2; two fractions with 5.1% of total UV-
331
absorption each) and one local maximum (4 % fractional absorption) at medium sizes (320-
332
450 g/mol) and slightly higher polarity (log P ~ 1.75). In the winter west sample (WW), the first
333
and second maximum are slightly shifted to higher polarity compared to the winter east samples
334
(WE), with a fractional absorption for the global maximum of 6.1 % and 3.5 % for the 2nd
335
maximum. Additionally, there is a third weak maximum at medium size and high polarity (log
336
P ~ 0.5) with a fractional absorption of 3.5 %. For the summer samples, more absorption arises
337
in the smaller and more polar fractions. This trend is most distinct for the summer west sample
338
(SW), where the absorption of the fraction with the largest molecules is very small. Only 6 % of
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the total absorption arises from this SEC fraction, while the absorption from the largest
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molecules of the summer east sample (SE) is 24 % and the average of both winter samples is
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32 %. SW has a very sharp and intense global maximum (6.1 %) for molecules between 229 –
342
337 g/mol and a log P ~ 0.5. This fraction is also present in SE, but not as a maximum and only
343
with a fractional UV-absorption of 2.7 %. SE has its global maximum (4.6 %) for medium sized
344
molecules and a log P around 1.1 and the 2nd maximum (4.1 %) in the same fraction as the global
345
maximum of WW. These four samples already show clear differences in the composition of
346
HULIS depending on the season and the air mass inflow. The winter HULIS seems to consist of
347
larger and less polar molecules than the summer HULIS, which might be related to emissions
348
from biomass burning or other combustion processes. The smaller and more polar molecules are
349
most likely linked to secondary formation from volatile organic precursor compounds.
350
Comparing SW to WE, around 70 % of the total UV-absorption is relocated within the 2D size
351
vs. polarity space, highlighting the large differences in the composition of HULIS that can occur
352
even at one same sampling site in different air mass regimes. Moreover, the developed 2D
353
method is also able to identify and illustrate more subtle differences within the four regimes
354
themselves (compare Figure 5 with Figure S6). The most distinct differences can be seen for SW
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and SW-2, where the SEC fraction with largest molecules (>520 g/mol) is responsible for 6%
356
and 25% of total signal intensity, respectively. This demonstrates the potential of the method to
357
resolve chemical differences between different HULIS compositions. More detailed studies on a
358
larger set of ambient samples will be done and can be expected to yield further interesting
359
insights into the chemical composition of HULIS from different atmospheric regimes. It is also
360
highly likely that the different compositions lead to different aerosol particle properties like
361
hygroscopicity, CCN activation, interaction with radiation, particle toxicity, and ecosystem
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impacts. The developed 2D-LC fractionation will also enable detailed downstream analytical
363
studies of the individual fractions and with regard to the different absorption properties, new
364
possibilities for future studies of light absorbing BrC in atmospheric particles.
365 366 367
FIGURES
368 Figure 1. SEC chromatograms of the winter east HULIS sample with different concentrations of
370
ammonium hydrogen carbonate.
normalized absorbance
369
371 372
Figure 2. UV-spectra of all five fractions of the winter east HULIS sample, normalized to
373
maximum of each fraction.
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A
B
C
374 375
Figure 3. RP-HPLC chromatograms of the winter east HULIS sample with a linear (A), stepwise
376
(B) and the new spiked gradient (C).
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SRFA
A OH O
3
OH
O H
2.49 H
H
Fractional UV−absorption
log P
O
2
O
0.06
OH
0.04 O
1.24
CH3
0.02
OH
1
O
OH
O
0.69 OH OH O
0 200
300
400
500 600 700800 1000
MW / g/mol
25.5 29.5
26.6
22.9 24.5
21.9 20.9 19.9
22.9 22.0
18.5
Time SEC / min
B
log P
3
Fractional UV−absorption
2
0.10 0.05 1
0 200
377
300
400
500 600 700800 1000
MW / g/mol
378
Figure 4. 2D heat maps of molecular size, polarity and fractional UV absorption for SRFA with
379
two different fraction limits (in minutes) for the SEC and the corresponding SEC chromatogram
380
in the middle: A optimized fraction limits for SRFA; B fraction limits set as for an average
381
atmospheric sample.
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WE [WSOC] = 4.25 µg/m3
[WSOC] = 6.87 µg/m3 3
Fractional UV−absorption 0.06
2
0.04
log P
log P
3
Fractional UV−absorption 0.05 0.04 0.03 0.02 0.01
2
0.02 1
1
0
0 200
300
400
500 600 700 800
200
300
MW / g/mol
400
500 600 700 800
MW / g/mol
SW
SE [WSOC] = 3.11 µg/m3
[WSOC] = 3.00 µg/m3 3
Fractional UV−absorption 0.06
2
0.04
log P
log P
3
Fractional UV−absorption
2
0.04 0.03 0.02
0.02 1
0
0 200
382
0.01 1
300
400
500 600 700 800
200
MW / g/mol
300
400
500 600 700 800
MW / g/mol
383
Figure 5. 2D heat maps of WW, WE, SW and SE. The color scale is set to the corresponding
384
maximum value of each 2D chromatogram.
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TABLES
387
Table 1. Characterization of the SEC fractions of the winter east HULIS sample: Average time
388
window, absorption coefficient (E2/E3: 254 nm/365 nm) and the average molecular weights,
389
calculated with different approaches from number (MWn) and mass averaged (MWw) negative
390
ESI mass spectra as well as from a calibration with standard compounds. See text for details. Fraction
Average time E2/E3 window
MWn (negative mode)
MWw (negative mode)
MWcalibration at taverage
1
19.6 – 22.5
3.80 ± 0.34
775.0
806.7
681.6
2
22.5 – 23.4
4.58 ± 0.48
713.2
749.2
491.2
3
23.4 – 25.3
5.93 ± 0.47
675.0
726.0
388.3
4
25.3 – 27.4
6.70 ± 0.73
655.7
703.0
276.4
5
27.4 – 29.5
7.28 ± 0.80
620.1
671.2
192.4
391 392 393
ASSOCIATED CONTENT
394
Supporting Information
395
The Supporting Information is available free of charge on the ACS Publications website.
396
Studied filter samples with sampling date, wind direction, OC and WSOC measurements (Table
397
S1); SEC chromatograms with different mixing ratios of the mobile phase (Figure S1); Table of
398
spiked gradient profile (Table S2); List of all substances used for the calibration of both
399
separation dimensions with the corresponding measured data (Table S3); LC-ESI-ToF-MS
400
spectra of the five SEC fractions from the winter east HULIS sample (Figure S2); Calibration
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curve for the SEC (Figure S3); Calibration curve for the RP-HPLC (Figure S4); Correlation plot
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of the measured UV-absorption and TOC measurements (Figure S5) (PDF).
403 404
AUTHOR INFORMATION
405
Corresponding Author
406
* Phone: 49 341 2717 7024. Fax: 49 341 2717 99 7024. E-mail:
[email protected].
407
Author Contributions
408
The manuscript was written through contributions of all authors and all authors have given
409
approval to the final version of the manuscript
410
Notes
411
The authors declare no competing financial interest.
412
ACKNOWLEDGMENT
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This work was funded by the German Research Foundation (DFG) in the project HuCar as PI
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1102/4-1 and HE 3086/28-1. The authors would also like to thank Gerald Spindler, Anett Dietze,
415
and Anke Rödger for providing the filter samples and additional data.
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