The outer-core size of tropical cyclones (TCs) is vital for evaluating their destructive potential.
The outer-core size of tropical cyclones (TCs) is vital for evaluating their destructive potential. It is usually defined as the radius of gale-force wind (R17), but accurately forecasting R17 is challenging owing to our incomplete understanding of the physical mechanism that determines it. Nonetheless, there is a general consensus that the TC outer-core size is mainly regulated by the TC’s outer spiral rainbands. The factors conducive to the development and organization of convection in the outer-core region of TCs are also favorable for the maintenance and expansion of their outer-core size.
Researchers from Nanjing University, China, and University of Reading, UK, investigated the statistical relationships between environmental thermodynamic and dynamic factors and TC outer-core size in the South China Sea. They provide strong evidence that among all possible environmental factors, the low-level environmental helicity has the most profound impact on TC outer-core size, regardless of whether the TCs are local or migrating from the western Pacific Ocean.
Helicity is a kinematic predictor for intense convections. Positive helicity means that the rotation-axis of the flow is in the same direction as the flow—that is, the wind rotates and moves in the direction of rotation. Usually, a clockwise veering hodograph will produce positive helicity, and interestingly, scientists observe that positive helicity can be beneficial for the organization and persistence of intense convections.
The composite analyses carried out in this study indicate that the environmental helicity could have a large impact on convective activities within the TC outer-core region. Large positive environmental helicity favors the occurrence of intense and long-lasting convection, strong radial inflow, large angular momentum import, and thus large R17. These results have recently been published in Atmospheric and Oceanic Science Letters.
Read more at Institute of Atmospheric Physics, Chinese Academy of Sciences
Image: Severe Typhoon In-Fa (2021) (Credit: Xiaoyong Zhuge)
