TY - JOUR
T1 - Broadening of modeled cloud droplet spectra using bin microphysics in an eulerian spatial domain
AU - Morrison, Hugh
AU - Witte, Mikael
AU - Bryan, George H.
AU - Harrington, Jerry Y.
AU - Lebo, Zachary J.
N1 - Funding Information:
Acknowledgments. This work was partially supported by U.S. DOE Atmospheric System Research (ASR) Grant DE-SC0016579. JYH acknowledges support from the U.S. DOE ASR Grant DE-SC0012827. ZJL acknowledges support from the U.S. DOE ASR Grant DE-SC0016354. MKW acknowledges support from NCAR’s Advanced Study Program. High performance computing was provided by NCAR’s Computational Information Systems Laboratory. The National Center for Atmospheric Research is sponsored by the National Science Foundation. We thank J. Jensen for discussion and W. Grabowski for discussion and comments on an earlier draft of the paper. Comments and suggestions from A. Igel and two anonymous reviewers improved the paper. We also thank the UCLA-LES team for developing and maintaining the LES code, including B. Stevens, T. Heus, A. Seifert, and C. Hohenegger.
Publisher Copyright:
© 2018 American Meteorological Society.
PY - 2018/11/1
Y1 - 2018/11/1
N2 - This study investigates droplet size distribution (DSD) characteristics from condensational growth and transport in Eulerian dynamical models with bin microphysics. A hierarchy of modeling frameworks is utilized, including parcel, one-dimensional (1D), and three-dimensional large-eddy simulation (LES). The bin DSDs from the 1D model, which includes only vertical advection and condensational growth, are nearly as broad as those from the LES and in line with observed DSD widths for stratocumulus clouds. These DSDs are much broader than those from Lagrangian microphysical calculations within a parcel framework that serve as a numerical benchmark for the 1D tests. In contrast, the bin-modeled DSDs are similar to the Lagrangian microphysical benchmark for a rising parcel in which Eulerian transport is not considered. These results indicate that numerical diffusion associated with vertical advection is a key contributor to broadening DSDs in the 1D model and LES. This DSD broadening from vertical numerical diffusion is unphysical, in contrast to the physical mixing processes that previous studies have indicated broaden DSDs in real clouds. It is proposed that artificial DSD broadening from vertical numerical diffusion compensates for underrepresented horizontal variability and mixing of different droplet populations in typical LES configurations with bin microphysics, or the neglect of other mechanisms that broaden DSDs such as growth of giant cloud condensation nuclei. These results call into question the ability of Eulerian dynamical models with bin microphysics to investigate the physical mechanisms for DSD broadening, even though they may reasonably simulate overall DSD characteristics.
AB - This study investigates droplet size distribution (DSD) characteristics from condensational growth and transport in Eulerian dynamical models with bin microphysics. A hierarchy of modeling frameworks is utilized, including parcel, one-dimensional (1D), and three-dimensional large-eddy simulation (LES). The bin DSDs from the 1D model, which includes only vertical advection and condensational growth, are nearly as broad as those from the LES and in line with observed DSD widths for stratocumulus clouds. These DSDs are much broader than those from Lagrangian microphysical calculations within a parcel framework that serve as a numerical benchmark for the 1D tests. In contrast, the bin-modeled DSDs are similar to the Lagrangian microphysical benchmark for a rising parcel in which Eulerian transport is not considered. These results indicate that numerical diffusion associated with vertical advection is a key contributor to broadening DSDs in the 1D model and LES. This DSD broadening from vertical numerical diffusion is unphysical, in contrast to the physical mixing processes that previous studies have indicated broaden DSDs in real clouds. It is proposed that artificial DSD broadening from vertical numerical diffusion compensates for underrepresented horizontal variability and mixing of different droplet populations in typical LES configurations with bin microphysics, or the neglect of other mechanisms that broaden DSDs such as growth of giant cloud condensation nuclei. These results call into question the ability of Eulerian dynamical models with bin microphysics to investigate the physical mechanisms for DSD broadening, even though they may reasonably simulate overall DSD characteristics.
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U2 - 10.1175/JAS-D-18-0055.1
DO - 10.1175/JAS-D-18-0055.1
M3 - Article
AN - SCOPUS:85056112404
SN - 0022-4928
VL - 75
SP - 4005
EP - 4030
JO - Journal of the Atmospheric Sciences
JF - Journal of the Atmospheric Sciences
IS - 11
ER -