Abstract. Brown carbon (BrC) plays an essential impact on radiative forcing
due to its ability to absorb sunlight. In this study, the optical properties
and molecular characteristics of water-soluble and methanol-soluble organic
carbon (OC; MSOC) emitted from the simulated combustion of biomass and coal
fuels and vehicle emissions were investigated using ultraviolet–visible (UV–vis)
spectroscopy, excitation–emission matrix (EEM) spectroscopy, and
Fourier transform ion cyclotron resonance mass spectrometry (FT-ICR MS)
coupled with electrospray ionization (ESI). The results showed that these
smoke aerosol samples from biomass burning (BB) and coal combustion (CC) had
a higher mass absorption efficiency at 365 nm (MAE365) than vehicle
emission samples. A stronger MAE365 value was also found in MSOC than
water-soluble organic carbon (WSOC), indicating low polar compounds would
possess a higher light absorption capacity. Parallel factor (PARAFAC) analysis
identified six types of fluorophores (P1–6) in WSOC including two
humic-like substances (HULIS-1) (P1 and P6), three protein-like substances
(PLOM) (P2, P3, and P5), and one undefined substance (P4). HULIS-1 was mainly from
aging vehicle exhaust particles; P2 was only abundant in BB aerosols; P3 was
ubiquitous in all tested aerosols; P4 was abundant in fossil burning
aerosols; and P5 was more intense in fresh vehicle exhaust particles. The
MSOC chromophores (six components; C1–6) exhibited consistent
characteristics with WSOC, suggesting the method could be used to indicate
the origins of chromophores. FT-ICR mass spectra showed that CHO and CHON
were the most abundant components of WSOC, but S-containing compounds
appeared in a higher abundance in CC aerosols and vehicle emissions than BB
aerosols, while considerably fewer S-containing compounds largely with CHO
and CHON were detected in MSOC. The unique formulas of different sources in the van Krevelen (VK) diagram presented different molecular distributions.
To be specific, BB aerosols with largely CHO and CHON had a medium H ∕ C and
low O ∕ C ratio, while CC aerosols and vehicle emissions largely with
S-containing compounds had an opposite H ∕ C and O ∕ C ratio. Moreover, the
light absorption capacity of WSOC and MSOC was positively associated with
the unsaturation degree and molecular weight in the source aerosols. The
above results are potentially applicable to further studies on the EEM-based or
molecular-characteristic-based source apportionment of chromophores in
atmospheric aerosols.
Water-soluble humic like substances (HULIS) in smoke particles emitted from combustion of biomass materials and coal were characterized by ultrahigh-resolution Fourier transform ion cyclotron resonance mass spectrometry. The formulas identified were classified into four main groups: CHO, CHON, CHOS, and CHONS. The average H/C and O/C ratios are 1.13-1.33, 1.01-1.13, 1.26-1.48, 1.09-1.24 and 0.21-0.41, 0.27-0.45, 0.41-0.46, 0.44-0.61 for the CHO, CHON, CHOS, and CHONS groups, respectively. The CHO compound was the predominant component (43%-72%) of the smoke HULIS from biomass burning (BB) and coal combustion, followed by the CHON group for BB-smoke HULIS and the S-containing groups (i.e., CHOS and CHONS) for coal-smoke HULIS. These results indicate that the primary HULIS emitted from biomass burning contain a high abundance of CHON species, which appear to be made up mainly of oxidized nitrogen functional groups such as nitro compounds and/or organonitrates. The coal-smoke HULIS contained more compounds with relatively low molecular weight and high aromaticity index (AI). They were significantly enriched in S-containing compounds with high double bond equivalent (≥4), and O/S ratios suggest that they are most likely made up of aromatic organosulfates and nitrooxy organosulfates that are usually found in polluted atmospheres. These findings imply that the primary emissions from combustion of biomass and coal fuels are potential sources of water-soluble HULIS in an atmospheric matrix and that coal combustion is an especially important source of sulfate compounds.
Protein mobility in living cells is vital for cell function. Both cytosolic viscosity and weak protein-protein interactions affect mobility, but examining viscosity and weak interaction effects is challenging. Herein, we demonstrate the use of (19) F NMR spectroscopy to measure cytoplasmic viscosity and to characterize nonspecific protein-protein interactions in living Escherichia coli cells. The origins of resonance broadening in Escherichia coli cells were also investigated. We found that sample inhomogeneity has a negligible effect on resonance broadening, the cytoplasmic viscosity is only about 2-3 times that of water, and ubiquitous transient weak protein-protein interactions in the cytosol play a significant role in governing the detection of proteins by using in-cell NMR spectroscopy.
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