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Data from NASA satellites and from aircraft were used to show that the model did a good job of reproducing the formation and evolution of Gert. This paper examines computer simulations of Tropical Storm Gert , which formed in the Gulf of Mexico during the National Aeronautics and Space Administration s NASA Tropical Cloud Systems and Processes TCSP Experiment, to investigate the development of low-level circulation and, in particular, whether stratiform or hot tower processes were responsible for the storm s formation. The simulation shows that a mix of both stratiform and convective rainfall occurred within Gert.

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One hypothesis suggests that the surface circulation forms from a "top-down" approach in which a storm s rotating circulation begins at middle levels of the atmosphere and builds down to the surface through processes related to light "stratiform" horizontally extensive precipitation.

Another hypothesis suggests a bottom-up approach in which deep thunderstorm towers convection play the major role in spinning up the flow at the surface.

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These "hot towers" form in the area of the mid-level circulation and strongly concentrate this rotation at low levels within their updrafts. Merger of several of these hot towers then intensifies the surface circulation to the point in which a storm forms. This paper examines computer simulations of Tropical Storm Gertwhich formed in the Gulf of Mexico during the National Aeronautics and Space Administration s NASA Tropical Cloud Systems and Processes TCSP Experiment, to investigate the development of low-level circulation and, in particular, whether stratiform or hot tower processes were responsible for the storm s formation.

Braun, Scott A. One hypothesis suggests that the surface circulation forms from a "top-down" approach in which a storm s rotating circulation begins at middle levels of the atmosphere and builds down to the surface through processes related to light "stratiform" horizontally extensive precipitation.

Another hypothesis suggests a bottom-up approach in which deep thunderstorm towers convection play the major role in spinning up the flow at the surface. These "hot towers" form in the area of the mid-level circulation and strongly concentrate this rotation at low levels within their updrafts.

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Merger of several of these hot towers then intensifies the surface circulation to the point in which a storm forms.