Abstract

Satellite rainrate estimation is a great challenge, especially in mesoscale convective systems (MCSs), which is mainly due to the absence of a direct physical connection between observable cloud parameters and surface rainrate. The machine learning technique was employed in this study to estimate rainrate in the MCS domain via using cloud top temperature (CTT) derived from a geostationary satellite. Five kinds of machine learning models were investigated, i.e., polynomial regression, support vector machine, decision tree, random forest, and multilayer perceptron, and the precipitation of Climate Prediction Center morphing technique (CMORPH) was used as the reference. A total of 31 CTT related features were designed to be the potential inputs for training an algorithm, and they were all proved to have a positive contribution in modulating the algorithm. Random forest (RF) shows the best performance among the five kinds of models. By combining the classification and regression schemes of the RF model, an RF-based hybrid algorithm was proposed first to discriminate the rainy pixel and then estimate its rainrate. For the MCS samples considered in this study, such an algorithm generates the best estimation, and its accuracy is definitely higher than the operational precipitation product of FY-4A. These results demonstrate the promising feasibility of applying a machine learning technique to solve the satellite precipitation retrieval problem.

Highlights

  • Most vigorous rainstorms are generated by so-called mesoscale convective systems (MCSs) [1,2], which are commonly defined as a cluster of vigorous precipitating clouds with a horizontal scale exceeding 100 km [3]

  • Depending on the form of organization, MCS could be classified as a squall line, mesoscale convective complex (MCC), mesoscale convective vortex (MCV), etc. [2,4]

  • The satellite-generated MCS samples were practically composed of cloud top temperature (CTT) snapshots with about 15 min intervals, and the rainrate estimation was fulfilled on each pixel for a certain MCS image

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Summary

Introduction

Most vigorous rainstorms are generated by so-called mesoscale convective systems (MCSs) [1,2], which are commonly defined as a cluster of vigorous precipitating clouds with a horizontal scale exceeding 100 km [3]. The combination of high intensity, large area, and long lifetime of such violent precipitation systems tends to produce extremely massive rainfall and possibly leads to various hydrological or geological disasters, such as floods, landslides, etc. In the MCS, there usually are many convective cells that are dependent on each other, appearing as an ensemble of cumulonimbus clouds with particular organizations. Depending on the form of organization, MCS could be classified as a squall line, mesoscale convective complex (MCC), mesoscale convective vortex (MCV), etc. In terms of the precipitation-generating regime, it is notable that convective precipitation and stratiform

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