Wednesday, 10 January 2018
Exhibit Hall 3 (ACC) (Austin, Texas)
The diurnal cycle of the cirrus canopy of tropical cyclones (TCs) is a continuing area of research. It has been shown through observations that this diurnal cycle may be fundamental for changing storm intensity and structure as deep convection propagates outwards overnight (Dunion et al., 2014). Recent work on this subject has used a high resolution 3D model to explore this outward propagating, wave-like diurnal signal at cloud top height (O’Neill et al., 2017). Navarro et al. (2017) used a method analogous with the periodic Sawyer-Eliassen equations to simulate the dynamics by which the diurnal response is achieved. In the work presented here, we use more realistic (non-harmonic) diurnal forcings in a non-hydrostatic, linear model with arbitrary time dependence, known as 3DVPAS. We explore the transition between balanced and radiating responses, and compare the results to the harmonic cases from Navarro et al. (2017). This study will test the forcing on axisymmetric TCs of different sizes and strengths and with different stratifications.
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