TY - JOUR
T1 - Lidar Ratio–Depolarization Ratio Relations of Atmospheric Dust Aerosols
T2 - The Super-Spheroid Model and High Spectral Resolution Lidar Observations
AU - Kong, Senyi
AU - Sato, Kaori
AU - Bi, Lei
N1 - Funding Information:
The authors acknowledge the NOAA Air Resources Laboratory (ARL) for the provision of the HYSPLIT transport and dispersion model and READY website (https://www.ready.noaa.gov), and the scattering properties obtained from TAMUdust2020. The authors also acknowledge the DISCOVER-AQ NASA LaRC HSRL2 data used in this study publicly available at https://www-air.larc.nasa.gov/cgi-bin/ArcView/discover-aq.co-2014?B200=1, and ORACLES Science Team (2020), Moffett Field, CA, NASA Ames Earth Science Project Office (ESPO) for the ORACLES P-3 Orion HSRL2 data used in this study publicly available at doi:10.5067/Suborbital/ORACLES/P3/2018_V2. K. Sato was supported by The Japan Aerospace Exploration Agency (EarthCARE satellite mission); JSPS (KAKENHI grant JP17H06139); Shiseido Female Researcher Science Grant; Ministry of Education, Culture, Sports, Science and Technology (MEXT; Initiative for Realizing Diversity in the Research Environment); Collaborative Research Program of the Research Institute for Applied Mechanics, Kyushu University (Fukuoka, Japan). L. Bei was supported by National Natural Science Foundation of China (42022038). A portion of the computations was performed on the National Supercomputer Center in Guangzhou (NSCC-GZ) and the cluster at State Key Lab of CAD&CG at Zhejiang University.
Publisher Copyright:
© 2022 The Authors.
PY - 2022/2/27
Y1 - 2022/2/27
N2 - The backscattering optical properties of an ensemble of randomly oriented dust particles at a wavelength of 355 nm were comprehensively studied by examining the invariant imbedding T-matrix results of the super-spheroid dust model. In particular, we focused on the lidar ratio ((Formula presented.)) and depolarization ratio ((Formula presented.)) relations of dust aerosols to aid interpretation of data from the Atmospheric Lidar (ATLID) instrument that will be onboard the Earth Cloud, Aerosol and Radiation Explorer (EarthCARE) satellite. Super-spheroid models with various aspect ratios ((Formula presented.)), roundness parameters (Formula presented.), and refractive indices were investigated over a wide range of particle sizes and compared to the observation data of the National Aeronautics and Space Administration (NASA) Langley 355-nm airborne high spectral resolution lidar. We found that super-spheroid dust particles with different sets of (Formula presented.) and (Formula presented.) could be used to model almost the entire range of the observed joint distributions of (Formula presented.) and (Formula presented.). The (Formula presented.) relation could effectively discriminate among dust particle types. The observed (Formula presented.) and (Formula presented.) values with the largest population density were best covered by models with n > 2, especially by those with (Formula presented.) varying from 2.4 to 3.0.
AB - The backscattering optical properties of an ensemble of randomly oriented dust particles at a wavelength of 355 nm were comprehensively studied by examining the invariant imbedding T-matrix results of the super-spheroid dust model. In particular, we focused on the lidar ratio ((Formula presented.)) and depolarization ratio ((Formula presented.)) relations of dust aerosols to aid interpretation of data from the Atmospheric Lidar (ATLID) instrument that will be onboard the Earth Cloud, Aerosol and Radiation Explorer (EarthCARE) satellite. Super-spheroid models with various aspect ratios ((Formula presented.)), roundness parameters (Formula presented.), and refractive indices were investigated over a wide range of particle sizes and compared to the observation data of the National Aeronautics and Space Administration (NASA) Langley 355-nm airborne high spectral resolution lidar. We found that super-spheroid dust particles with different sets of (Formula presented.) and (Formula presented.) could be used to model almost the entire range of the observed joint distributions of (Formula presented.) and (Formula presented.). The (Formula presented.) relation could effectively discriminate among dust particle types. The observed (Formula presented.) and (Formula presented.) values with the largest population density were best covered by models with n > 2, especially by those with (Formula presented.) varying from 2.4 to 3.0.
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U2 - 10.1029/2021JD035629
DO - 10.1029/2021JD035629
M3 - Article
AN - SCOPUS:85125139483
VL - 127
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
SN - 2169-897X
IS - 4
M1 - e2021JD035629
ER -