Therefore, in this study, we implement a radiative closure study from VIS-NIR to TIR for a dust case over Santa Cruz Tenerife (28.473N, 16.247W) on June 19, 2022, based on observations from AERONET, Micro-Pulse Lidar Network (MPLNET) and the spaceborne Atmospheric Infrared Sounder (AIRS). Including most of the uncertainty sources from necessary assumptions, our result shows that ~95% of the TIR brightness temperatures simulated based on AERONET-retrieved DC-PSD among the range of error is warmer than that from AIRS, meaning that using the AERONET-retrieved properties can hardly make a radiative closure with TIR observations. Afterward, we adjusted the AERONET-retrieved DC-PSD to be larger by referring to the in-situ measured Fennec-SAL PSD while keeping the total surface area unchanged. We found that the sensitivity of AERONET observations to this change in DC-PSD is mainly within 5%, while using the adjusted DC-PSD can very much improve the TIR radiative closure.
The result indicates that although the AERONET-retrieved DC-PSD is well-established in VIS-NIR channels, it is highly possible to miss a portion of coarse particles due to the limited sensitivity in VIS-NIR and lead to underestimated extinction in TIR. Combining VIS-NIR and TIR observations can improve the retrieval of DC-PSD, which is important in evaluating dust total mass concentration.
Supplementary URL: https://doi.org/10.22541/essoar.170355039.95598312/v1

