What is the difference between a tornado and a hurricane?

Both tornadoes and hurricanes are characterized by extremely strong horizontal winds that swirl around their center and by a ring of strong upward motion surrounding downward motion in their center. In both tornadoes and hurricanes, the tangential wind speed far exceeds the speed of radial inflow or of vertical motion.

Hurricanes always and tornadoes usually rotate counterclockwise in the northern hemisphere and clockwise in the southern hemisphere. The Earth's rotation determines this direction for the storms' rotation in each hemisphere. Local winds are sometimes able to cause a tornado to form that spins in the opposite direction from the typical direction for that hemisphere.

The most obvious difference between a tornado and hurricane is that a hurricane's horizontal scale is about a thousand times larger than a tornado. In addition, hurricanes and tornadoes form under different circumstances and have different impacts on the atmosphere.

Tornadoes are small-scale circulations, that are rarely more than a few hundred feet across when they touch the ground. Most tornadoes grow out of severe thunderstorms that develop in the high wind-shear environment of the United States Central Plains during spring and early summer.  Many tornadoes form when the large-scale wind flow leads to a violent clash between moist, warm air traveling north from the Gulf of Mexico and cold, dry, continental air coming from the United States Northwest. Tornadoes can also form in many other locations and from other forcing factors. For example, a hurricane making landfall may trigger many tornadoes to form.

Tornado wind speeds may reach 100 to 300 mph and cause havoc on the ground, but tornadoes typically last only a few minutes and rarely travel more than 10 or 20 miles along the ground. Tornadoes have little impact on storms that spawn them or collectively on the global circulation of the atmosphere.

Hurricanes, on the other hand, are large-scale circulations that are 60 to over 1,000 miles across. Hurricanes form near the Equator, generally between 5 and 20 degrees latitude, but never right on the Equator. Hurricanes always form over the warm waters of the tropical oceans and generally where the sea-surface temperature exceeds 26.5°C (76°F).

A hurricane may travel thousands of miles and persist over several days or weeks. During its lifetime, a hurricane will transport a significant amount of heat up from the ocean surface and into the upper troposphere or even lower stratosphere. Even though hurricanes form only sporadically, they do affect the global atmosphere's circulation in measurable ways, although this is still an active area of research.

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2002

Tropical Cyclone Winston Hits Fiji

The GPM core observatory satellite flew directly above tropical cyclone Winston on February 20, 2016 at 0941 UTC. Tropical cyclone Winston had sustained winds estimated at 155 kts (178 mph) at that time. A rainfall analysis derived from data collected by GPM's Microwave Imager (GMI) and Dual-frequency Precipitation Radar (DPR) instruments found that in addition to powerful winds Winston was dropping rain at a rate of over 169 mm (6.7 inches) per hour in the western side of the eye. Tropical cyclone WINSTON is the most powerful storm to hit Fiji. At least one fatality has already occurred. The

GPM Again Examines Powerful Tropical Cyclone Uriah

Both yesterday and today the GPM core observatory satellite had excellent views of tropical cyclone Uriah in the South Indian Ocean. Uriah was intensifying with winds of about 115 kts (132 mph) on February 17, 2016 at 1651 UTC when the GPM satellite passed above. A rainfall analysis derived from GPM's Microwave Imager (GMI) and Dual-frequency Precipitation Radar (DPR) data collected with that pass revealed that Uriah had a well defined circular eye. Rain was measured by DPR falling at a rate of over 179 mm (7 inches) per hour on the southern side of Uriah's eye wall. GPM passed over again on

GPM Examines Tropical Cyclone Uriah

Over the past view days the GPM core observatory satellite has had good looks at tropical cyclone URIAH in the South Indian Ocean west of Australia. On February 15, 2016 at 1706 UTC GPM flew directly over the center of the tropical cyclone and measured rainfall in a well defined circulation. GPM's Dual-frequency Precipitation Radar (DPR) instrument discovered that rain was falling at a rate of over 127 mm (5 inches) per hour in a band of intense storms south of the cyclone's center. When GPM's Radar sliced through tropical storm URIAH on February 15, 2016 it also found that the intense

Intensifying South Pacific Tropical Cyclone Winston Viewed By GPM

Tropical cyclone activity has recently increased in the South Pacific Ocean. Four tropical cyclones have formed in this area in 2016. The GPM core observatory satellite had an excellent view of tropical cyclone Winston on February 11, 2016 at 1253 UTC. Winston was located east of Vanuatu with tropical storm force winds of about 55 kts when GPM passed over head. Winston's rainfall was measured by GPM's Microwave Imager (GMI) and Dual-frequency Precipitation Radar (DPR) instruments. GPM's radar data revealed that Winston was dropping rain at a rate of over 60 mm (2.4 inches) per hour on the

GPM Views Tropical Cyclone Forming Near Madagascar

The GPM core observatory satellite flew over a forming tropical cyclone in the South Indian Ocean between Madagascar and Reunion on February 8, 2016 at 2137 UTC. Low vertical wind shear will assist in the evolution of the tropical low as it moves slowly toward the southwest. Rainfall derived from GPM's Microwave Imager (GMI) and Dual-frequency Precipitation Radar (DPR) data revealed that powerful convective storms near Madagascar's eastern coast were found to be dropping rain at a rate of over 94 mm (3.7 inches) per hour. 3-D measurements were made of convective storm tops with GPM's radar