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摘要
The uncertainty in particle size distribution retrievals is analyzed theoretically and numerically when using aerosol optical depth (AOD) data affected by three distinct error-inducing effects. Specifically, circumsolar radiation (CS), optical mass (OM), and solar disk's brightness distribution (BD) effects are taken into consideration here. Because of these effects, the theoretical AOD is affected by an error, partial derivative AOD, that consequently translates into errors in the determined (apparent) particle size distribution (PSD). Through comparison of the apparent and the true size distributions, the relative error, partial derivative PSD, is calculated here as a function of particle radius for various instrument's fields of view (aperture) and solar zenith angles. It is shown that, in general, the CS effect overestimates the number of submicron-sized particles, and that the significance of this effect increases with the aperture. In case of maritime aerosols, the CS effect may also lead to an underestimation of the number concentration of large micron-sized particles. The BD and OM effects become important, and possibly predominant, when AOD is low. Assuming large particles dominate in the atmosphere, the BD effect tends to underestimate the concentration of the smallest aerosol particles. In general, the PSD(apparent)/PSD(true) ratio is affected by the CS effect equally over all particle sizes. The relative errors in PSD are typically smaller than 40-60%, but can exceptionally exceed 100%, which means that the apparent PSD may then be twice as large as the true PSD. This extreme situation typically occurs with maritime aerosols under elevated humidity conditions. Recent instruments tend to be designed with smaller apertures than ever before, which lower the CS-induced errors to an acceptable level in most cases.
- 出版日期2012-5
