Dispersion of droplet size distributions in supercooled nonā€precipitating stratocumulus from aircraft observations obtained during the Southern Ocean Cloud Radiation Aerosol Transport Experimental Study

The characteristics of cloud droplet size distributions and statistical relations of the relative dispersion (epsilon) with the vertical velocity (w) and with the interstitial aerosol concentration (N-ia) are investigated for ubiquitous supercooled shallow stratocumulus observed over the Southern Oc...

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Bibliographic Details
Published in:Journal of Geophysical Research: Atmospheres
Other Authors: Wang, Yang (author), Zhao, Chuanfeng (author), McFarquhar, Greg M. (author), Wu, Wei (author), Reeves, Mike (author), Li, Jiming (author)
Format: Article in Journal/Newspaper
Language:English
Published: 2021
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Online Access:https://doi.org/10.1029/2020JD033720
Description
Summary:The characteristics of cloud droplet size distributions and statistical relations of the relative dispersion (epsilon) with the vertical velocity (w) and with the interstitial aerosol concentration (N-ia) are investigated for ubiquitous supercooled shallow stratocumulus observed over the Southern Ocean (SO) using aircraft measurements obtained during the Southern Ocean Cloud Radiation Aerosol Transport Experimental Study. Distinct vertical variations have been found using 36 non-precipitating cloud profiles. The cloud droplet effective radius (r(e)) increases nearly monotonically from 5.3 +/- 1.9 mu m at cloud base to 9.4 +/- 2.2 mu m at cloud top. The epsilon decreases rapidly from cloud base (0.42 +/- 0.13) and then remains relatively constant in the upper cloud layer (0.27 +/- 0.09). This study also shows robust dependence of epsilon on both N-ia and w. The epsilon increases (decreases) with increasing N-ia (w) at a 95% confidence level when values of w (low N-ia) are restricted to a small range. The important roles of aerosols and dynamics on epsilon are demonstrated and are crucial to estimating aerosol indirect radiative forcing, especially for pristine SO regions where models almost universally underestimate reflected radiation. 1852977