TY - JOUR
T1 - Structural changes preceding rapid intensification in tropical cyclones as shown in a large ensemble of idealized simulations
AU - Miyamoto, Yoshiaki
AU - Nolan, David S.
N1 - Funding Information:
Acknowledgments. Y. Miyamoto was partly supported by JSPS Scientific Research 26-358 for the JSPS Fellowship program for overseas researchers. D. Nolan was supported by NASA through Grant NNX16AP19G. The numerical simulations were performed at the Center for Computational Sciences at the University of Miami. The authors are grateful for fruitful discussions with Drs. Rob Rogers, John Kaplan, Hua Chen, and Leon Nguyen and also thank two anonymous reviewers for providing comments and suggestions.
Funding Information:
Y. Miyamoto was partly supported by JSPS Scientific Research 26-358 for the JSPS Fellowship program for overseas researchers. D. Nolan was supported byNASAthrough Grant NNX16AP19G. The numerical simulations were performed at the Center for Computational Sciences at the University of Miami. The authors are grateful for fruitful discussions with Drs. Rob Rogers, John Kaplan, Hua Chen, and Leon Nguyen and also thank two anonymous reviewers for providing comments and suggestions
Publisher Copyright:
© 2018 American Meteorological Society.
PY - 2018/2/1
Y1 - 2018/2/1
N2 - Structural changes that precede rapid intensification (RI) of tropical cyclones (TCs) are examined in a full-physics model by conducting a large ensemble (270) of idealized TC simulations. The processes leading to RI in a representative case with moderate shear are consistent with previous studies for weakly sheared cases. The most distinct changes are that the vortex tilt and the vortex size begin to decrease more rapidly 6 h before the onset of RI. A vorticity budget analysis for the upper layer around the low-level center reveals that the vertical vorticity is increased by vertical advection, stretching, and tilting terms before RI, whereas the horizontal advection is small. Thus, the upright vortex structure is not achieved through a vortex alignment process but rather is built upward by deep convection. The ensemble simulations are generated by changing the intensity and size of the initial vortex, the magnitude of vertical wind shear, and the translation speed. The ensemble members that show RI are consistent with the control case and many previous studies: before the onset of RI, the intensity gradually increases, the radius of maximum tangential wind (RMW) decreases, the flow structure becomes more symmetric, the vortex tilt decreases, and the radius of maximum convergence approaches the radius of maximum winds. A dimensionless parameter representing a tendency for the formation of the vertically upright structure is considered. The product of this parameter and the local Rossby number is significantly larger for TCs that exhibit RI in the next 24 h.
AB - Structural changes that precede rapid intensification (RI) of tropical cyclones (TCs) are examined in a full-physics model by conducting a large ensemble (270) of idealized TC simulations. The processes leading to RI in a representative case with moderate shear are consistent with previous studies for weakly sheared cases. The most distinct changes are that the vortex tilt and the vortex size begin to decrease more rapidly 6 h before the onset of RI. A vorticity budget analysis for the upper layer around the low-level center reveals that the vertical vorticity is increased by vertical advection, stretching, and tilting terms before RI, whereas the horizontal advection is small. Thus, the upright vortex structure is not achieved through a vortex alignment process but rather is built upward by deep convection. The ensemble simulations are generated by changing the intensity and size of the initial vortex, the magnitude of vertical wind shear, and the translation speed. The ensemble members that show RI are consistent with the control case and many previous studies: before the onset of RI, the intensity gradually increases, the radius of maximum tangential wind (RMW) decreases, the flow structure becomes more symmetric, the vortex tilt decreases, and the radius of maximum convergence approaches the radius of maximum winds. A dimensionless parameter representing a tendency for the formation of the vertically upright structure is considered. The product of this parameter and the local Rossby number is significantly larger for TCs that exhibit RI in the next 24 h.
KW - Hurricanes
KW - Hurricanes/typhoons
KW - Tropical cyclones
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U2 - 10.1175/JAS-D-17-0177.1
DO - 10.1175/JAS-D-17-0177.1
M3 - Article
AN - SCOPUS:85042231147
SN - 0022-4928
VL - 75
SP - 555
EP - 569
JO - Journal of the Atmospheric Sciences
JF - Journal of the Atmospheric Sciences
IS - 2
ER -