NASA scientists use the computer modeling field including the NCAR Mesoscale Model Version 5 (MM5) model to study the winds and updrafts near the hurricane's eye. An updraft is the vertical upward movement of air inside of a storm. This research focuses on the processes that impact the formation, intensification, movement, structure, and precipitation organization of hurricanes. An MM5 simulation of Hurricane Bonnie (1998) suggests that the timing and location of individual updrafts that produce the rainfall (often concentrated on very small-scales) are controlled by intense, small-scale regions of rapidly swirling flow in the eyewall. The winds in hurricanes are often described in terms of radial (in toward the center or out away from it) and tangential (the swirling flow around a hurricane) winds. By looking at the urad field, one can see where the main inflow and outflow regions of the storm are, which can be important for a variety of reasons. Eyewall mesovortices are small scale rotational features found in the eyewalls of intense tropical cyclones. In these vortices, wind speed can be up to 10% higher than in the rest of the eyewall. Eyewall mesovortices are a significant factor in the formation of tornadoes after tropical cyclone landfall. Mesovortices can spawn rotation in individual thunderstorms (a mesocyclone), which leads to tornadic activity. At landfall, friction is generated between the circulation of the tropical cyclone and land. This can allow the mesovortices to descend to the surface, causing large outbreaks of tornadoes. Note: NASA scientists are using high resolution models to try to understand the rainfall structure observed by the TRMM satellite. Animator: Lori Perkins (NASA/GSFC), Greg Shirah (NASA/GSFC), Alex Kekesi (GST), James W. Williams (GST). Scientist: Scott Braun (NASA/GSFC), Owen Kelley (George Mason University). Platforms/Sensors/Data Sets: Mesoscale Model Version 5 (MM5)/MM5.