Thursday, 10 January 2019: 10:30 AM
North 124A (Phoenix Convention Center - West and North Buildings)
The NOx chemical lifetime in the atmosphere is nonlinearly related to its concentration and is strongly coupled to the available OH. Direct observation of changes in the NOx emissions and lifetime over the past decades therefore provides information about the oxidative capacity of the atmosphere. Doing so required the development of a new satellite NO2 retrieval (BEHR v3.0B) with sufficiently detailed a priori data including daily variations. Using the new BEHR retrieval, we observe shifts from NOx-suppressed to NOx-limited chemistry in several US cities, implying that OH concentrations will decrease in step with future NOx emissions reductions. We examine how this change can explain the observed slowdown in US NOx reductions after circa 2010 and show the impact that not explicitly accounting for changes in lifetime has on emissions constraints. We compare the observed changes in NOx lifetime with those computed in a state-of-science model and discuss the implications for our current understanding of the kinetics governing the NOx and HOx cycles.
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