2014
DOI: 10.1002/2013jd020276
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Relationships between layer-mean radar reflectivity and columnar effective radius of warm cloud: Numerical study using a cloud microphysical bin model

Abstract: The relationship between the layer-mean radar reflectivity, Ze, and the columnar effective particle radius, Re, in evolving shallow warm clouds was investigated by numerical experiments using a hybrid cloud microphysical model and a forward simulator of satellite measurements. Changes in the cloud/rain droplet size distributions were traced in a kinematically driven warm cloud for various values of number concentration of cloud condensation nuclei (CCN) and maximum updraft velocity. In contrast to previous int… Show more

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Cited by 3 publications
(10 citation statements)
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“…Grabowski (2016) recently proposed a "piggybacking" approach that separates dynamical and microphysical impacts on deep convection. Kuba et al (2014Kuba et al ( , 2015) used a two-dimensional kinematic driver model (Shipway and Hill 2012) to study shallow cloud properties simulated by a spectral bin cloud microphysics scheme and examined the differences between NDW6 and the bin scheme; the bin scheme examined here is a cloud microphysical model with a two-moment bin method based on Kuba and Fujiyoshi (2006) and modified by Kuba and Murakami (2010), and will be referred to as the KF-bin scheme. To investigate the relationships between cloud microphysical processes and satellite observational data, Suzuki and Stephens (2008) examined the relationships between mean radar reflectivity, Z e , and mean particle effective radius, R e , values for shallow clouds retrieved from satellite observations and used this information to identify warm cloud microphysical processes.…”
Section: Comparison With a Bin Microphysics Schemementioning
confidence: 99%
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“…Grabowski (2016) recently proposed a "piggybacking" approach that separates dynamical and microphysical impacts on deep convection. Kuba et al (2014Kuba et al ( , 2015) used a two-dimensional kinematic driver model (Shipway and Hill 2012) to study shallow cloud properties simulated by a spectral bin cloud microphysics scheme and examined the differences between NDW6 and the bin scheme; the bin scheme examined here is a cloud microphysical model with a two-moment bin method based on Kuba and Fujiyoshi (2006) and modified by Kuba and Murakami (2010), and will be referred to as the KF-bin scheme. To investigate the relationships between cloud microphysical processes and satellite observational data, Suzuki and Stephens (2008) examined the relationships between mean radar reflectivity, Z e , and mean particle effective radius, R e , values for shallow clouds retrieved from satellite observations and used this information to identify warm cloud microphysical processes.…”
Section: Comparison With a Bin Microphysics Schemementioning
confidence: 99%
“…Suzuki et al (2010b) further analyzed the contoured frequency by optical depth (CFODD) for vertical profiles of radar reflectivity as a function of cloud optical depth from cloud top to investigate cloud microphysical processes based on a methodology adapted from Nakajima et al (2010). Kuba et al (2014) reproduced a diagram proposed by Suzuki and Stephens (2008) using a kinematic driver model (Shipway and Hill 2012) with the KF-bin scheme and a forward simulator of satellite measurements. Changes in the size distribution of cloud droplets and raindrops were traced in the two-dimensional kinematic driver model (Shipway and Hill 2012) for a warm cloud.…”
Section: Comparison With a Bin Microphysics Schemementioning
confidence: 99%
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