A prominent
source of hydroxyl radicals (•OH),
nitrous acid (HONO) plays a key role in tropospheric chemistry. Apart
from direct emission, HONO (or its conjugate base nitrite, NO2
–) can be formed secondarily in the atmosphere.
Yet, how secondary HONO forms requires elucidation, especially for
heterogeneous processes involving numerous organic compounds in atmospheric
aerosols. We investigated nitrite production from aqueous photolysis
of nitrate for a range of conditions (pH, organic compound, nitrate
concentration, and cation). Upon adding small oxygenates such as ethanol, n-butanol, or formate as •OH scavengers,
the average intrinsic quantum yield of nitrite [Φ(NO2
–)] was 0.75 ± 0.15%. With near-UV-light-absorbing
vanillic acid (VA), however, the effective Φ(NO2
–) was strongly pH-dependent, reaching 8.0 ± 2.1%
at a pH of 8 and 1.5 ± 0.39% at a more atmospherically relevant
pH of 5. Our results suggest that brown carbon (BrC) may greatly enhance
the nitrite production from the aqueous nitrate photolysis through
photosensitizing reactions, where the triplet excited state of BrC
may generate solvated electrons, which reduce nitrate to NO2 for further conversion to nitrite. This photosensitization process
by BrC chromophores during nitrate photolysis under mildly acidic
conditions may partly explain the missing HONO in urban environments.
Brown
carbon (BrC) absorbs radiation in the near-UV and visible
ranges, affecting atmospheric photochemistry and radiative forcing.
Our understanding on the photochemical transformation of BrC is still
limited, especially when mixed with the abundant and photochemically
labile inorganic salt, nitrate. Herein, we investigate the photochemical
reactions of four BrC chromophores, including two methoxyphenols and
two nitrophenols. Experiments were conducted in the absence and presence
of different concentrations of H2O2 and nitrate
with lights of 254 and 313 nm. The results show that the pseudo-first-order
decay rate constants (k) of these four BrC compounds
at 313 nm illumination were approximately 10 times lower than those
at 254 nm, demonstrating longer lifetimes of these BrC chromophores
under tropospherically relevant irradiation. Photo-enhancement in
the visible range was observed in most experiments, with those under
313 nm illumination lasting longer, indicating the prolonged effects
of nascent and transformed BrC chromophores on radiative forcing.
Methoxyphenols had higher averaged k values than
nitrophenols during direct photolysis with 254 or 313 nm lights, but
the k values for nitrophenols under high-nitrate
(or high-H2O2) conditions approached those of
methoxyphenols. The photo-enhancement in the visible range for methoxyphenols
in the presence of nitrate was substantially contributed by nitro
products, while that for nitrophenols was mainly contributed by hydroxylated
and/or dimerized products. Our results reveal the similarity and difference
between the photolysis of methoxyphenols and nitrophenols, which may
help better understand the aging of different types of BrC for better
model representation of their effects on radiative forcing.
Review on the annual PM10 concentrations over a 10-year period shows that Macau is subjected to severe fine particulate pollution. Investigations of its variation in monthly and daily time scales with the local meteorological records reveal further details. It is found that a distinct feature of the Asian monsoon climates, the changes of wind direction, mainly controls the general trend of PM10 concentration in a year. The monsoon driven winter north-easterly winds bring upon Macau dry and particle enriched air masses leading to a higher concentration in that period while the summer south-westerly winds transport humid and cleaner air to the region leading to a lower PM10 value. This distinct seasonal feature is further enhanced by the lower rainfall volume and frequency as well as mixing height in winter and their higher counterparts in summer. It is also found that the development of tropical cyclones near Macau could also impose episode like PM10 concentration spikes due to the pre-typhoon induced stagnant air motion followed by the swing of wind direction to the northerly.
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