Dry lines, squall lines, and sea breezes are examples of phenomena observed by mesonets. Due to the space and time scales associated with mesoscale phenomena and microclimates, weather stations comprising a mesonet are spaced closer together and report more frequently than synoptic scale observing networks, such as the WMO Global Observing System (GOS) and US ASOS. The term mesonet refers to the collective group of these weather stations, which are usually owned and operated by a common entity. Mesonets generally record in situsurface weather observations but some involve other observation platforms, particularly vertical profiles of the planetary boundary layer (PBL).[5] Other environmental parameters may include insolation and various variables of interest to particular users, such as soil temperature or road conditions (the latter notable in Road Weather Information System (RWIS) networks).
The distinguishing features that classify a network of weather stations as a mesonet are station density and temporal resolution with sufficiently robust station quality. Depending upon the phenomena meant to be observed, mesonet stations use a spatial spacing of 1 to 40 kilometres (0.6 to 20 mi)[6] and report conditions every 1 to 15 minutes. Micronets (see microscale and storm scale), such as in metropolitan areas such as Oklahoma City,[7]St. Louis, and Birmingham UK, are yet denser in spatial and sometimes temporal resolution.[8]
^Marshall, Curtis H. (11 Jan 2016). "The National Mesonet Program". 22nd Conference on Applied Climatology. New Orleans, LA: American Meteorological Society.
^Fujita, Tetsuya Theodore (1962). A Review of Researches on Analytical MesoMeteorology. SMRP Research Paper. Vol. #8. Chicago: University of Chicago. OCLC7669634.