Hurricane Wilma's Hot Towers seen by TRMM 10/17/2005 at 1754Z
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On October 17, 2005 at 1754 Zulu, Wilma was classified as a Tropical Storm with sustained wind speeds of only 45 knots. Forty hours later the storm had increased its intensity to category five status with sustained winds of 150 knots. Spikes in the rain structure known as 'Hot Towers' indicate storm intensity. 'Hot Towers' refers to tall cumulonimbus clouds and has been seen as one of the mechanisms by which the intensity of a tropical cyclone is maintained. Because of the size (1-20 km) and short duration (30 minute to 2 hours) of these hot towers, studies of these events have been limited to descriptive studies from aircraft observations, although a few have attempted to use the presence of hot towers in a predictive capacity. Before TRMM, no data set existed that could show globally and definitively the presence of these hot towers in cyclone systems. Aircraft radar studies of individual storms lack global coverage. Global microwave or infrared sensor observations do not provide the needed spatial resolution. With a ground resolution of 5 km, the TRMM Precipitation Radar provided the needed data set for examining the predictive value of hot towers in cyclone intensification.
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Deep convective 15 km clouds (in red) can be seen in the eyewall of Tropical Storm Wilma on October 17, 2005.
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The TRMM spacecraft's Precipation Radar (PR) instrument observed 15 km towers in the eyewall of Hurricane Wilma.
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Hurricane Wilma's vertical rain structure in kilometers. The high towers are shown in red.
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