Fig. 4. Near-molecular level organic aerosol (OA) source composition.
Only four out of the five identified sources are shown as the HR-EESI-ToF is not sensitive to the water-insoluble hydrocarbon-like OA (HOA). Carbon number distribution (a, b, d & g) of biomass burning OA (BBOA), cold-season primary OA (CPOA), cold-season OA (COOA), and urban oxygenated OA (UOOA) [left panels], and their corresponding family-specific (CxHyOz>0 and CxHyOz≥0Nm) mass defect (Δm/z, difference from integer mass) plots (c, e, f, h & i) are shown in the middle and right panels. The relative intensity of CxHyOz>0 and CxHyOz≥0Nm family species binned according to H:C ratios shows clear differences in the source composition. The colored circles represent the carbon number (Nc), and their size is proportional to the relative intensity of the corresponding species in each OA factor. Every straight dashed line represents a group with species having same # H and C and/or N but different number of oxygen atoms. Formulae for dominant ions in COOA, CPOA and UOOA are annotated in the graph. The relative contribution by species to different compound classes to the total signal intensity illustrates secondary COOA as most oxidized and dominated by both CHO and CHN1O; UOOA as more aromatic and less oxidized, and dominated by CHO. CPOA, on the other hand, is more of aliphatic origin with CHN2 dominance.