Skip to main content
Log in

Kinetic Energy Budgets during the Rapid Intensification of Typhoon Rammasun (2014)

  • Original Paper
  • Published:
Advances in Atmospheric Sciences Aims and scope Submit manuscript

Abstract

In this study, Typhoon Rammasun (2014) was simulated using the Weather Research and Forecasting model to examine the kinetic energy during rapid intensification (RI). Budget analyses revealed that in the inner area of the typhoon, the conversion from symmetric divergent kinetic energy associated with the collocation of strong cyclonic circulation and inward flow led to an increase in the symmetric rotational kinetic energy in the lower troposphere. The increase in the symmetric rotational kinetic energy in the mid and upper troposphere resulted from the upward transport of symmetric rotational kinetic energy from the lower troposphere. In the outer area, both typhoon and Earth’s rotation played equally important roles in the conversion from symmetric divergent kinetic energy to symmetric rotational kinetic energy in the lower troposphere. The decrease in the symmetric rotational kinetic energy in the upper troposphere was caused by the conversion to asymmetric rotational kinetic energy through the collocation of symmetric tangential rotational winds and the radial advection of asymmetric tangential rotational winds by radial environmental winds.

摘 要

以往对于热带气旋快速增强机制的研究通常集中在最大风速所在的内核区域进行. 本研究对 2014 年的台风个例威马逊进行了分析, 除内核区域外, 还分析了台风外部区域快速增强期间的动能收支. 对低层旋转动能收支的分析显示, 在台风内区, 气旋式切向风和向内的辐散流相互作用造成的对称辐散动能向对称旋转动能的转换导致了对流层低层对称旋转动能的增加. 对流层中高层对称旋转动能的增加是由于对称旋转动能从对流层低层向中高层输送引起的. 在台风外区, 台风和地球自转在对流层低层的对称辐散动能向对称旋转动能的转换中发挥了同样重要的作用. 对流层高层对称旋转动能的减弱是通过对称切向旋转风和径向环境风对非对称切向旋转风的径向平流的相互作用引起的低层旋转动能向非对称旋转动能的转换所致. 本研究的结果表明, 低层入流在快速增强期间发挥了以下重要作用: 低层入流与向外位势梯度方向相反, 向外位势梯度将可将位能转换为对称辐散动能; 低层入流与气旋切向流相互作用, 将对称辐散动能转换为对称旋转动能; 低空入流导致台风内区向上运动, 将动能从对流层低层输送到对流层中高层.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Acknowledgements

The authors thank the Training Center of Atmospheric Sciences of Zhejiang University and two anonymous reviewers for their constructive comments and suggestions. We also thank Huiyan XU for deriving kinetic energy equations, Liguang WU and Huarui ZHAO for providing the MWT filter codes, Xinyong SHEN for improving the simulation of Typhoon Rammasun (2014), and Liangliang LI, and Chi ZHANG for valuable discussions. This study was supported by the National Natural Science Foundation of China (Grant No. 41930967).

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Xiaofan Li.

Additional information

Article Highlights

• The symmetric rotational kinetic energy in the troposphere increases during the rapid intensification of Typhoon Rammasun.

• The increase in the lower troposphere results from the conversion of symmetric divergent kinetic energy via the rotational- and divergent-flow interaction.

• The increase in the upper troposphere is due to transport of symmetric rotational kinetic energy from the lower troposphere by strong upward motions.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Quan, X., Li, X. Kinetic Energy Budgets during the Rapid Intensification of Typhoon Rammasun (2014). Adv. Atmos. Sci. 40, 78–94 (2023). https://doi.org/10.1007/s00376-022-2060-z

Download citation

  • Received:

  • Revised:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00376-022-2060-z

Key words

关键词

Navigation