| dc.description.abstract |
Tropical cyclones (TCs) represent one of the most prevalent and devastating forms of natural
disasters. Despite their significant impact, accurately predicting tropical cyclones (TCs) remains a
challenging endeavour due to the complexities involved. Over the past fifty years, numerous
theories have been proposed to elucidate the genesis and intensification of TCs. However, no single
theory has been able to explain the genesis and intensification of TC fully. Consequently, there
remains a division among scientists regarding a comprehensive understanding of TC formation.
The current study conducted in the North Indian Ocean (NIO) aims to provide new insights into the
various stages involved in the genesis and intensification of TCs from low-pressure systems (LPS).
This study employed data from the NCEP FNL reanalysis of 1x1 degree resolution as input for the
Weather Research and Forecasting (ARW) model of version 4. We utilized the domain
configuration of child and parent domain through one-way nesting. A combination of Kain-Fritsch
(new Eta) scheme for cumulus parameterization and the WRF Single-Moment 6 class (WSM6)
graupel scheme for microphysics was incorporated in model run. The findings indicate that upper
wind circulations and the geographical positioning of LPS are critical to the genesis and
intensification of TCs. An upper cyclonic circulation located to the left or northwest of the centre,
along with an anticyclonic circulation or poleward winds to the right or northeast, significantly
increases the likelihood of TC formation. Furthermore, the dominance of upper-level westerlies
over LPS creates favourable conditions for the genesis of TCs. Easterly winds tend to hinder both
genesis and intensification in the NIO. Additionally, proximity to coastal regions can adversely
affect TC genesis. Vertical wind shear (VWS) values between 3 and 10 m/s are crucial for the
transformation of LPS into TCs. Sustained declines in central pressure and mid-level Geopotential
Height (GPH) foster an environment conducive to both the TC genesis and intensification. Sea
Surface Temperatures (SST) exceeding 26°C and a radial gradient in SST enhance the likelihood of
TC genesis. The warming of the inner core of LPS is favourable for both the genesis and
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heightened intensity of TCs. Minimum potential vorticity (PV) of 1 at the upper level is critical for
TC genesis, with a sustained increase in upper PV over time supporting further intensification. The
Convective Available Potential Energy (CAPE) was lowest at the centre of the LPS, with CAPE
values ranging from 2000 to 4000 J/kg within the LPS, which are conducive to tropical cyclone
genesis.. A maximum CAPE value of 5000 J/kg during the genesis stage indicates potential for
high-intensity TCs. Elevated relative humidity at mid-level altitudes and a symmetric cloud band
pattern around the centre of the LPS significantly promote the genesis of TCs and enhance the
potential for high-intensity TCs. The boundary layer air is substantially influenced by heat flux
from the underlying warm sea surface. Continuous enhancement of upward vertical heat flux
accelerates the genesis and intensification of TCs. Despite differences in data resolution, scale, and
domain configuration, the model results and analyses derived from the European Centre for
Medium-Range Weather Forecasts (ECMWF) concerning TC genesis and intensification
substantially corroborate each other. Thus, the outcomes of this study are deemed reliable. The
insights acquired from this research are invaluable in enhancing accurate predictions of TC genesis
and intensification in the NIO. This study will serve as a guiding tool for governmental departments
in Bangladesh and India, assisting in the protection of human life and the mitigation of damage to
property, infrastructure, environment, and biodiversity resulting from TCs. Various government
agencies will have sufficient time to be well-equipped to execute timely responses and implement
appropriate disaster management measures. |
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