Convective Mass-Flux From Long Term Radar Reflectivities Over Darwin, Australia

Journal Article (2021)
Author(s)

A. C.M. Savazzi (TU Delft - Atmospheric Remote Sensing)

Christian Jakob (Monash University)

AP Siebesma (Royal Netherlands Meteorological Institute (KNMI), TU Delft - Atmospheric Remote Sensing)

Research Group
Atmospheric Remote Sensing
Copyright
© 2021 A.C.M. Savazzi, Christian Jakob, A.P. Siebesma
DOI related publication
https://doi.org/10.1029/2021JD034910
More Info
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Publication Year
2021
Language
English
Copyright
© 2021 A.C.M. Savazzi, Christian Jakob, A.P. Siebesma
Research Group
Atmospheric Remote Sensing
Issue number
19
Volume number
126
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Abstract

Most cumulus parametrizations today make use of a simple conceptual model of convection, called the mass-flux approach. This approach depicts convection as an ensemble of updrafts and downdrafts occurring within a model grid-box. The aim of this study is to determine convective mass-fluxes and their constituents on the scale of a 100 km GCM grid-box from a C-band polarimetric radar and thereafter investigate the relative role of area fraction and vertical velocity in determining the shape and magnitude of bulk mass-flux profiles. We make use of observational estimates of these quantities spanning 13 wet seasons in the tropical region of Darwin. Following a bulk approach, the results show that the distribution of mass-flux is positively skewed and its mean profile peaks at 4 km. This is the result of constant area fractions and increasing vertical velocities below that level. Above 4 km, in-cloud vertical velocity plays a marginal role compared to the convective area fraction in controlling mass-flux profiles.