Convective storm detection is the meteorological observation, and short-term prediction, of deep moist convection (DMC). DMC describes atmospheric conditions producing single or clusters of large vertical extension clouds ranging from cumulus congestus to cumulonimbus, the latter producing thunderstorms associated with lightning and thunder. Those two types of clouds can produce severe weather at the surface and aloft.[1]
The ability to discern the presence of deep moist convection in a storm significantly improves meteorologists' capacity to predict and monitor associated phenomena such as tornadoes, large hail, strong winds, and heavy rain leading to flash flooding. It relies on direct eyewitness observations, for example from storm spotters; and on remote sensing, especially weather radar. Some in situ measurements are used for direct detection as well, notably, wind speed reports from surface observation stations. It is part of the integrated warning system, consisting of prediction, detection, and dissemination of information on severe weather to users such as emergency management, storm spotters and chasers, the media, and the general public.[2]
^Doswell, Charles A. III (2001). "Severe Convective Storms – An Overview". In Doswell, Charles A. III (ed.). Severe Convective Storms. Meteorological Monographs. Vol. 28, No. 50. Boston, MA: American Meteorological Society. ISBN 1-878220-41-1.
^Cite error: The named reference spotter history was invoked but never defined (see the help page).
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