Abstract

It has been suggested that the inner eyewall structure may play an important role in the secondary eyewall formation (SEF) of tropical cyclones (TCs). This study is to further examine the role of the inner eyewall structure by comparing two numerical experiments, which were conducted with the same large-scale environment and initial and boundary conditions but different grid sizes. The SEF was simulated in the experiment with the finer grid spacing, but not in the other.Comparing the eyewall structure in the simulated TCs with and without the SEF indicates that the eyewall structure can play an important role in the SEF. For the simulated TC with the SEF, the eyewall is more upright with stronger updrafts, accompanied by a wide eyewall anvil at a higher altitude. Compared to the simulated TC without the SEF, diagnostic analysis reveals that the cooling outside the inner eyewall is induced by the sublimation, melting and evaporation of hydrometeors falling from the eyewall anvil. The cooling also induces upper-level dry, cool inflow below the anvil, prompting the subsidence and moat formation between the inner eyewall and the spiral rainband. In the simulated TC without the SEF, the cooling induced by the falling hydrometeors is significantly reduced and offset by the diabatic warming. There is no upper-level dry inflow below the anvil and no moat formation between the inner eyewall and the spiral rainband. This study suggests that a realistic simulation of the intense eyewall convection is important to the prediction of the SEF in the numerical forecasting model.

Highlights

  • Many intense tropical cyclones (TCs) usually undergo the secondary eyewall formation (SEF)(Fortner, 1958; Willoughby, 1982)

  • Given a negative radial gradient of vorticity outside the primary eyewall, vortex Rossby waves (VRWs) propagate outward and stop at a stagnation radius, where the mean flow strengthens through the interaction of eddies with the azimuthal-mean vortex (Montgomery and Kallenbach, 1997; Qiu et al, 2010; Chen and Yau, 2001; Hogsett and Zhang, 2009; Dai et al, 2021)

  • A secondary eyewall forms through the found that the secondary eyewall can be simulated in a barotropic model when the preexisting outer convection is stretched into a closed vorticity band by the rotation of the inner vortex

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Summary

Introduction

Many intense tropical cyclones (TCs) usually undergo the secondary eyewall formation (SEF). Zhu and Zhang (2006) proposed that varying cloud microphysics processes affect the timing of the spinup of the secondary eyewall since the differences in the inner eyewall convection and the rainband structure of the simulated TCs. Numerical simulations showed that changing the terminal velocity of snow led to changes in the magnitude and distribution of the diabatic heating of inner-core convection at outer radii, which is important for the SEF (Zhu and Zhu, 2015). The CFAD illustrates the frequency distribution of the vertical motion of the indicated values at each altitude in the region of the 10-km radially inside and outside of the radius of the maximum tangential wind (RMW) for two simulations.

Buoyancy effects
Diabatic heating
Subsidence in response to the diabatic cooing
Findings
Summary
Full Text
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