Metal ions are key components in atmosphere that potentially
affect
the optical properties and photochemical reactivity of atmospheric
humic-like substances (HULIS), while this mechanism is still unclear.
In this study, we demonstrated that atmospheric HULIS coupled with
Fe3+, Cu2+, Zn2+, and Al3+ exhibited distinct optical properties and reactive intermediates
from that of HULIS utilizing three-dimensional fluorescence spectroscopy
and electron paramagnetic resonance spectroscopy. The HULIS components
showed light absorption that increased by 56% for the HULIS-Fe3+ system, fluorescence blue shift, and fluorescence quenching,
showing a certain dose–effect relationship. These are mainly
attributed to the fact that the highly oxidative HULIS chromophores
have a stronger complexing ability with Fe3+ ions than
the other metal ions. In addition, triplet organics (promoting ratio:
53%) and reactive oxygen species (promoting ratio: 82.6%) in the HULIS-Fe3+ system showed obvious generation promotion. Therefore, the
main assumption of the photochemical mechanisms of atmospheric HULIS
in the HULIS-Fe3+ system is that Fe3+ ions can
form 3HULIS*-Fe3+ complexation with photoexcited 3HULIS* and then transition to the ground state through energy
transfer, electron transfer, or nonradiative transition, accompanied
by the formation of singlet oxygen and hydroxyl radicals. Our results
provide references for evaluating the radiative forcing and aging
effect of metal ions on atmospheric aerosols.