Simulating organic aerosol in Delhi with WRF-Chem using the volatility-basis-set approach: exploring model uncertainty with a Gaussian process emulator
The nature and origin of organic aerosol in the atmosphere remain unclear. The gas–particle partitioning of semi-volatile organic compounds (SVOCs) that constitute primary organic aerosols (POAs) and the multigenerational chemical aging of SVOCs are particularly poorly understood. The volatility bas...
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Veröffentlicht in: | Atmospheric chemistry and physics 2023-05, Vol.23 (10), p.5763-5782 |
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Zusammenfassung: | The nature and origin of organic aerosol in the
atmosphere remain unclear. The gas–particle partitioning of semi-volatile
organic compounds (SVOCs) that constitute primary organic aerosols (POAs) and
the multigenerational chemical aging of SVOCs are particularly poorly
understood. The volatility basis set (VBS) approach, implemented in air
quality models such as WRF-Chem (Weather Research and Forecasting model with Chemistry), can be a useful tool to describe emissions
of POA and its chemical evolution. However, the evaluation of model
uncertainty and the optimal model parameterization may be expensive to probe
using only WRF-Chem simulations. Gaussian process emulators, trained on
simulations from relatively few WRF-Chem simulations, are capable of
reproducing model results and estimating the sources of model uncertainty
within a defined range of model parameters. In this study, a WRF-Chem VBS
parameterization is proposed; we then generate a perturbed parameter
ensemble of 111 model runs, perturbing 10 parameters of the WRF-Chem model
relating to organic aerosol emissions and the VBS oxidation reactions. This
allowed us to cover the model's uncertainty space and to compare outputs from
each run to aerosol mass spectrometer observations of organic aerosol
concentrations and O:C ratios measured in New Delhi, India. The simulations
spanned the organic aerosol concentrations measured with the aerosol mass spectrometer (AMS). However,
they also highlighted potential structural errors in the model that may be
related to unsuitable diurnal cycles in the emissions and/or failure to
adequately represent the dynamics of the planetary boundary layer. While the
structural errors prevented us from clearly identifying an optimized VBS
approach in WRF-Chem, we were able to apply the emulator in the following two periods: the
full period (1–29 May) and a subperiod period of 14:00–16:00 h LT (local
time) on 1–29 May. The combination of emulator analysis and model
evaluation metrics allowed us to identify plausible parameter combinations
for the analyzed periods. We demonstrate that the methodology presented in
this study can be used to determine the model uncertainty and to identify the
appropriate parameter combination for the VBS approach and hence to provide
valuable information to improve our understanding of OA production. |
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ISSN: | 1680-7324 1680-7316 1680-7324 |
DOI: | 10.5194/acp-23-5763-2023 |