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- W2904755549 abstract "Abstract Dual‐polarization radar observations of Hurricane Irma (2017) provide new insight into the microphysical structure of a mature tropical cyclone that can be tied to the cyclone dynamics. The primary eyewall exhibited a radar signature of hydrometeor size sorting, which implied that large drops fell out near persistent upward motion in the front‐right quadrant of the storm, while smaller drops were advected downstream. In the outer rainbands, convective initiation was also preferred in the front‐right quadrant, whereas stratiform precipitation was predominant downwind. For both the primary eyewall and outer rainbands, the preferred quadrant for convective initiation was consistent with the expected kinematic asymmetry of a tropical cyclone in weak environmental wind shear but with moderate translation speed. The developing secondary eyewall exhibited a different asymmetry that indicated a stratiform‐to‐convective transition associated with heavy precipitation in the rear quadrants. This transition is consistent with hypothesized dynamical theories for secondary eyewall formation." @default.
- W2904755549 created "2018-12-22" @default.
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- W2904755549 date "2018-12-19" @default.
- W2904755549 modified "2023-10-01" @default.
- W2904755549 title "Examining Storm Asymmetries in Hurricane Irma (2017) Using Polarimetric Radar Observations" @default.
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- W2904755549 doi "https://doi.org/10.1029/2018gl080739" @default.
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