This study examines the tropical cyclone(TC)eyes over the North Indian Ocean(NIO)from 2013 to 2023.TCs feature a warm and cloud-free region called the eye.In recent years,meteorologists have taken a keen interest in g...This study examines the tropical cyclone(TC)eyes over the North Indian Ocean(NIO)from 2013 to 2023.TCs feature a warm and cloud-free region called the eye.In recent years,meteorologists have taken a keen interest in geometric and thermodynamic characteristics of TC’s eye as these attributes are useful for operational forecasting of TCs.In this study,we analyzed data from the INSAT-3D/R satellite,passive microwave imagery,and thermodynamic parameters over an 11-year period(2013–2023).Analysis showed that 37.73%of the TCs developed an eye over the NIO,with 60%of these occurring in the Arabian Sea(AS)and 40%in the Bay of Bengal(BoB).The eye was observed most frequently approximately 36 h(1.5 days)after the storm's onset(>34 knots).The mean maximum sustained wind speed at which an eye formed was 66 knots,with a standard deviation of 14.26 over the NIO.The average estimated central pressure of the eye was 982.15 hPa.TCs'eyes formed at an average latitude of 13.60°N and longitude of 83.67°E in the BoB,with standard deviations of 2.33°and 5.93°,respectively.The average radius of a TC's eye was 22.3 km(with a diameter of 44.6 km)over the NIO.The calculated Eye Roundness Value(ERV)was 0.59,with a range from 0.5 to 0.8.The average intensity of TC's eyes over the NIO was classified as Dvorak’s T4.0(64–89 knots).The dominant pattern observed before the formation of the TC's eye was the Curved Band Pattern.Our results indicated that as one moves poleward,both the size and number of eyes increase.The findings of this study are valuable for operational forecasters and disaster managers in mitigating socioeconomic impacts and preserving human lives.展开更多
文摘This study examines the tropical cyclone(TC)eyes over the North Indian Ocean(NIO)from 2013 to 2023.TCs feature a warm and cloud-free region called the eye.In recent years,meteorologists have taken a keen interest in geometric and thermodynamic characteristics of TC’s eye as these attributes are useful for operational forecasting of TCs.In this study,we analyzed data from the INSAT-3D/R satellite,passive microwave imagery,and thermodynamic parameters over an 11-year period(2013–2023).Analysis showed that 37.73%of the TCs developed an eye over the NIO,with 60%of these occurring in the Arabian Sea(AS)and 40%in the Bay of Bengal(BoB).The eye was observed most frequently approximately 36 h(1.5 days)after the storm's onset(>34 knots).The mean maximum sustained wind speed at which an eye formed was 66 knots,with a standard deviation of 14.26 over the NIO.The average estimated central pressure of the eye was 982.15 hPa.TCs'eyes formed at an average latitude of 13.60°N and longitude of 83.67°E in the BoB,with standard deviations of 2.33°and 5.93°,respectively.The average radius of a TC's eye was 22.3 km(with a diameter of 44.6 km)over the NIO.The calculated Eye Roundness Value(ERV)was 0.59,with a range from 0.5 to 0.8.The average intensity of TC's eyes over the NIO was classified as Dvorak’s T4.0(64–89 knots).The dominant pattern observed before the formation of the TC's eye was the Curved Band Pattern.Our results indicated that as one moves poleward,both the size and number of eyes increase.The findings of this study are valuable for operational forecasters and disaster managers in mitigating socioeconomic impacts and preserving human lives.
