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Hail is a form of solid precipitation.[1] It is distinct from ice pellets (American English "sleet"), though the two are often confused.[2] It consists of balls or irregular lumps of ice, each of which is called a hailstone.[3] Ice pellets generally fall in cold weather, while hail growth is greatly inhibited during low surface temperatures.
Unlike other forms of water ice precipitation, such as graupel (which is made of rime ice), ice pellets (which are smaller and translucent), and snow (which consists of tiny, delicately crystalline flakes or needles), hailstones usually measure between 5 mm (0.2 in) and 15 cm (6 in) in diameter.[1] The METAR reporting code for hail 5 mm (0.20 in) or greater is GR, while smaller hailstones and graupel are coded GS.
Hail is possible during most thunderstorms (as it is produced by cumulonimbus),[4] as well as within 2 nmi (3.7 km) of the parent storm. Hail formation requires environments of strong, upward motion of air within the parent thunderstorm (similar to tornadoes) and lowered heights of the freezing level. In the mid-latitudes, hail forms near the interiors of continents, while, in the tropics, it tends to be confined to high elevations.
There are methods available to detect hail-producing thunderstorms using weather satellites and weather radar imagery. Hailstones generally fall at higher speeds as they grow in size, though complicating factors such as melting, friction with air, wind, and interaction with rain and other hailstones can slow their descent through Earth's atmosphere. Severe weather warnings are issued for hail when the stones reach a damaging size, as it can cause serious damage to human-made structures, and, most commonly, farmers' crops.
Definition
[edit]Any thunderstorm which produces hail that reaches the ground is known as a hailstorm.[5] An ice crystal with a diameter of >5 mm (0.20 in) is considered a hailstone.[4] Hailstones can grow to 15 cm (6 in) and weigh more than 0.5 kg (1.1 lb).[6]
Unlike ice pellets, hailstones are often layered[7] and can be irregular and clumped together.[citation needed] Hail is composed of transparent ice or alternating layers of transparent and translucent ice at least 1 mm (0.039 in) thick, which are deposited upon the hailstone as it travels through the cloud, suspended aloft by air with strong upward motion until its weight overcomes the updraft and falls to the ground. Although the diameter of hail is varied, in the United States, the average observation of damaging hail is between 2.5 cm (1 in) and golf-ball-sized 4.4 cm (1.75 in).[8]
Stones larger than 2 cm (0.79 in) are usually considered large enough to cause damage. The Meteorological Service of Canada issues severe thunderstorm warnings when hail that size or above is expected.[9] The US National Weather Service has a 1 in (2.5 cm) diameter threshold, effective January 2010, an increase over the previous threshold of 0.75 in (1.9 cm) hail.[10] Other countries have different thresholds according to local sensitivity to hail; for instance, grape-growing areas could be adversely impacted by smaller hailstones. Hailstones can be very large or very small, depending on how strong the updraft is: weaker hailstorms produce smaller hailstones than stronger hailstorms (such as supercells), as the more powerful updrafts in a stronger storm can keep larger hailstones aloft.
Formation
[edit]Hail forms in strong thunderstorm clouds, particularly those with intense updrafts, high liquid-water content, great vertical extent, large water droplets, and where a good portion of the cloud layer is below freezing (0 °C; 32 °F).[4] These types of strong updrafts can also indicate the presence of a tornado.[11] The growth rate of hailstones is impacted by factors such as higher elevation, lower freezing zones, and wind shear.[12]
Layer nature of the hailstones
[edit]
Like other precipitation in cumulonimbus clouds, hail begins as water droplets. As the droplets rise and the temperature goes below freezing, they become supercooled water and will freeze on contact with condensation nuclei. A cross-section through a large hailstone shows an onion-like structure. This means that the hailstone is made of thick and translucent layers, alternating with layers that are thin, white and opaque. Former theory suggested that hailstones were subjected to multiple descents and ascents, falling into a zone of humidity and refreezing as they were uplifted.[citation needed] This up and down motion was thought to be responsible for the successive layers of the hailstone. New research, based on theory as well as field study, has shown this is not necessarily true.[citation needed]
The storm's updraft, with upwardly directed wind speeds as high as 110 mph (180 km/h),[13] blows the forming hailstones up the cloud. As the hailstone ascends, it passes into areas of the cloud where the concentration of humidity and supercooled water droplets varies. The hailstone's growth rate changes depending on the variation in humidity and supercooled water droplets that it encounters. The accretion rate of these water droplets is another factor in the hailstone's growth. When the hailstone moves into an area with a high concentration of water droplets, it captures the latter and acquires a translucent layer. Should the hailstone move into an area where mostly water vapor is available, it acquires a layer of opaque white ice.[14]

Furthermore, the hailstone's speed depends on its position in the cloud's updraft and its mass. This determines the varying thicknesses of the layers of the hailstone. The accretion rate of supercooled water droplets onto the hailstone depends on the relative velocities between these water droplets and the hailstone itself. This means that generally the larger hailstones will form some distance from the stronger updraft, where they can pass more time growing.[14] As the hailstone grows, it releases latent heat, which keeps its exterior in a liquid phase. Because it undergoes "wet growth", the outer layer is sticky (i.e. more adhesive), so a single hailstone may grow by collision with other smaller hailstones, forming a larger entity with an irregular shape.[16]
Hail can also undergo "dry growth", in which the latent heat release through freezing is not enough to keep the outer layer in a liquid state. Hail forming in this manner appears opaque due to small air bubbles that become trapped in the stone during rapid freezing. These bubbles coalesce and escape during the "wet growth" mode, and the hailstone is more clear. The mode of growth for a hailstone can change throughout its development, and this can result in distinct layers in a hailstone's cross-section.[17]
The hailstone will keep rising in the thunderstorm until its mass can no longer be supported by the updraft. This may take at least 30 minutes, based on the force of the updrafts in the hail-producing thunderstorm, whose top is usually greater than 10 km high. It then falls toward the ground while continuing to grow, based on the same processes, until it leaves the cloud. It will later begin to melt as it passes into air above freezing temperature.[18]
Thus, a unique trajectory in the thunderstorm is sufficient to explain the layer-like structure of the hailstone. The only case in which multiple trajectories can be discussed is in a multicellular thunderstorm, where the hailstone may be ejected from the top of the "mother" cell and captured in the updraft of a more intense "daughter" cell. This, however, is an exceptional case.[14]
Factors favoring hail
[edit]Hail is most common within continental interiors of the mid-latitudes, as hail formation is considerably more likely when the freezing level is below the altitude of 11,000 ft (3,400 m).[19] Movement of dry air into strong thunderstorms over continents can increase the frequency of hail by promoting evaporational cooling, which lowers the freezing level of thunderstorm clouds, giving hail a larger volume to grow in. Accordingly, hail is less common in the tropics despite a much higher frequency of thunderstorms than in the mid-latitudes because the atmosphere over the tropics tends to be warmer over a much greater altitude. Hail in the tropics occurs mainly at higher elevations.[20]
Hail growth becomes vanishingly small when air temperatures fall below −30 °C (−22 °F), as supercooled water droplets become rare at these temperatures.[19] Around thunderstorms, hail is most likely within the cloud at elevations above 20,000 ft (6,100 m). Between 10,000 ft (3,000 m) and 20,000 ft (6,100 m), 60% of hail is still within the thunderstorm, though 40% now lies within the clear air under the anvil. Below 10,000 ft (3,000 m), hail is equally distributed in and around a thunderstorm to a distance of 2 nmi (3.7 km).[21]
Scientific study
[edit]Beginning in Spring 2025, scientists in the United States engaged in a field study known as the "In-situ Collaborative Experiment for Collection of Hail In the Plains" (ICECHIP).[22] The project, which is studying hail processes in thunderstorms in two areas known as "hail alleys"–the Great Plains and along Colorado and Wyoming's Front Range of the Rocky Mountains–is the world's largest field campaign ever devoted to studying hail, involving 100 scientists from four countries and 11 states.[23] It is expected to shed light on many unanswered questions about hail formation and growth.[24]
Climatology
[edit]Hail occurs most frequently within continental interiors at mid-latitudes and is less common in the tropics, despite a much higher frequency of thunderstorms than in the mid-latitudes.[25] Hail is also much more common along mountain ranges because mountains force horizontal winds upwards (known as orographic lifting), thereby intensifying the updrafts within thunderstorms and making hail more likely.[26] The higher elevations also result in there being less time available for hail to melt before reaching the ground. One of the more common regions for large hail is across mountainous northern India, which reported one of the highest hail-related death tolls on record in 1888.[27] China also experiences significant hailstorms.[28] Central Europe and southern Australia also experience a lot of hailstorms. Regions where hailstorms frequently occur are southern and western Germany, northern and eastern France, southern and eastern Benelux, and northern Italy.[29] In southeastern Europe, Croatia and Serbia experience frequent occurrences of hail.[30] Some mediterranean countries register the maximum frequency of hail during the Fall season.[29]
In North America, hail is most common in the area where Colorado, Nebraska, and Wyoming meet, known as "Hail Alley".[31] Hail in this region occurs between the months of March and October during the afternoon and evening hours, with the bulk of the occurrences from May through September. Cheyenne, Wyoming is North America's most hail-prone city with an average of nine to ten hailstorms per season.[32] To the north of this area and also just downwind of the Rocky Mountains is the Hailstorm Alley region of Alberta, which also experiences an increased incidence of significant hail events.
Hailstorms are also common in several regions of South America, particularly in the temperate latitudes. The central region of Argentina, extending from the Mendoza region eastward towards Córdoba, experiences some of the most frequent hailstorms in the world, with 10–30 storms per year on average.[33] The Patagonia region of southern Argentina also sees frequent hailstorms, though this may be partially due to graupel (small hail) being counted as hail in this colder region.[33] The triple border region between the Brazilian states of Paraná, Santa Catarina, and Argentina, in southern Brazil is another area known for damaging hailstorms.[34] Hailstorms are also common in parts of Paraguay, Uruguay, and Bolivia that border the high-frequency hail regions of northern Argentina.[35] The high frequency of hailstorms in these areas of South America is attributed to the region's orographic forcing of convection, combined with moisture transport from the Amazon and instability created by temperature contrasts between the surface and upper atmosphere.[33] In Colombia, the cities of Bogotá and Medellín also see frequent hailstorms due to their high elevation. Southern Chile also sees persistent hail from mid April through October.

Short-term detection
[edit]Weather radar is a very useful tool to detect the presence of hail-producing thunderstorms. However, radar data has to be complemented by a knowledge of current atmospheric conditions which can allow one to determine if the current atmosphere is conducive to hail development.
Modern radar scans many angles around the site. Reflectivity values at multiple angles above ground level in a storm are proportional to the precipitation rate at those levels. Summing reflectivities in the Vertically Integrated Liquid or VIL, gives the liquid water content in the cloud. Research shows that hail development in the upper levels of the storm is related to the evolution of VIL. VIL divided by the vertical extent of the storm, called VIL density, has a relationship with hail size, although this varies with atmospheric conditions and therefore is not highly accurate.[36] Traditionally, hail size and probability can be estimated from radar data by computer using algorithms based on this research. Some algorithms include the height of the freezing level to estimate the melting of the hailstone and what would be left on the ground.
Certain patterns of reflectivity are important clues for the meteorologist as well. The three body scatter spike is an example. This is the result of energy from the radar hitting hail and being deflected to the ground, where they deflect back to the hail and then to the radar. The energy took more time to go from the hail to the ground and back, as opposed to the energy that went directly from the hail to the radar, and the echo is further away from the radar than the actual location of the hail on the same radial path, forming a cone of weaker reflectivities.
More recently, the polarization properties of weather radar returns have been analyzed to differentiate between hail and heavy rain.[37][38] The use of differential reflectivity (), in combination with horizontal reflectivity () has led to a variety of hail classification algorithms.[39] Visible satellite imagery is beginning to be used to detect hail, but false alarm rates remain high using this method.[40]
Size and terminal velocity
[edit]
The size of hailstones is best determined by measuring their diameter with a ruler. In the absence of a ruler, hailstone size is often visually estimated by comparing its size to that of known objects, such as coins.[41] Using objects such as hen's eggs, peas, and marbles for comparing hailstone sizes is imprecise, due to their varied dimensions. The UK organisation, TORRO, also scales for both hailstones and hailstorms.[42]
When observed at an airport, METAR code is used within a surface weather observation which relates to the size of the hailstone. Within METAR code, GR is used to indicate larger hail, of a diameter of at least 0.25 in (6.4 mm). GR is derived from the French word grêle. Smaller-sized hail, as well as snow pellets, use the coding of GS, which is short for the French word grésil.[43]

Terminal velocity of hail, or the speed at which hail is falling when it strikes the ground, varies. It is estimated that a hailstone of 1 cm (0.39 in) in diameter falls at a rate of 9 m/s (20 mph), while stones the size of 8 cm (3.1 in) in diameter fall at a rate of 48 m/s (110 mph). Hailstone velocity is dependent on the size of the stone, its drag coefficient, the motion of wind it is falling through, collisions with raindrops or other hailstones, and melting as the stones fall through a warmer atmosphere. As hailstones are not perfect spheres, it is difficult to accurately calculate their drag coefficient - and, thus, their speed.[44]
Size comparisons to objects
[edit]In the United States, the National Weather Service reports hail size as a comparison to everyday objects. Hailstones larger than 1 inch in diameter are denoted as "severe."[45]
| Diameter (inches) | Everyday Object |
|---|---|
| 0.25 - 0.375 | Pea |
| 0.50 | Small Marble |
| 0.75 | Penny |
| 0.88 | Nickel |
| 1.00 (15/16") | Quarter |
| 1.25 | Half Dollar |
| 1.50 | Walnut/Ping Pong Ball |
| 1.75 | Golf Ball |
| 2.00 | Lime |
| 2.50 | Tennis Ball |
| 2.75 | Baseball |
| 3.00 | Large Apple |
| 4.00 | Softball |
| 4.50 | Grapefruit |
| 4.75 - 5.00 | Computer CD/DVD |

Hail records
[edit]Megacryometeors, large rocks of ice that are not associated with thunderstorms, are not officially recognized by the World Meteorological Organization as "hail", which are aggregations of ice associated with thunderstorms, and therefore records of extreme characteristics of megacryometeors are not given as hail records.
- Heaviest: 1.02 kg (2.2 lb); Gopalganj District, Bangladesh, 14 April 1986.[46][47]
- Largest diameter officially measured: 7.9 in (20 cm) diameter, 18.622 in (47.3 cm) circumference; Vivian, South Dakota, 23 July 2010.[48]
- Largest circumference officially measured: 18.74 in (47.6 cm) circumference, 7.0 in (17.8 cm) diameter; Aurora, Nebraska, 22 June 2003.[47][49]
- Greatest average hail precipitation: Kericho, Kenya experiences hailstorms, on average, 50 days annually. Kericho is close to the equator and the elevation of 2,200 metres (7,200 ft) contributes to it being a hot spot for hail.[50] Kericho reached the world record for 132 days of hail in one year.[51]
Hazards
[edit]
Hail can cause serious damage, notably to automobiles, aircraft, skylights, glass-roofed structures, livestock, and most commonly, crops.[32] Hail damage to roofs often goes unnoticed until further structural damage is seen, such as leaks or cracks. It is hardest to recognize hail damage on shingled roofs and flat roofs, but all roofs have their own hail damage detection problems.[53] Metal roofs are fairly resistant to hail damage, but may accumulate cosmetic damage in the form of dents and damaged coatings. In 2023, hailstorms cost the United States $46 billion in damage to cars, roofs, and crops, according to the Insurance Institute for Business & Home Safety (IBHS).[54]
Hail is one of the most significant thunderstorm hazards to aircraft.[55] When hailstones exceed 0.5 in (13 mm) in diameter, planes can be seriously damaged within seconds.[56] The hailstones accumulating on the ground can also be hazardous to landing aircraft. Hail is a common nuisance to drivers of automobiles, severely denting the vehicle and cracking or even shattering windshields and windows unless parked in a garage or covered with a shielding material. Wheat, corn, soybeans, and tobacco are the most sensitive crops to hail damage.[27] Hail is one of Canada's most expensive hazards.[57]
Massive hailstones have been known to cause concussions or fatal head trauma to people caught outside without shelter. Hailstorms have been the cause of costly and deadly events throughout history. Some researchers have suggested that a hail storm was the cause of the deaths of several hundred nomads around the 9th century in Roopkund, Uttarakhand, India, though this has been disputed.[58][59] On April 30, 1888 a severe hailstorm killed more than 200 people in the Moradabad district of India. Fatal injuries are more rare in the modern era; in the US for example, despite hail causing billions of dollars in damage every year and large hail (>2 inches (5.1 cm) diameter) being fairly common, only three people have been known to be struck and killed by hail since modern records have been kept.[60]
Accumulations
[edit]
Narrow zones where hail accumulates on the ground in association with thunderstorm activity are known as hail streaks or hail swaths,[61] which can be detectable by satellite after the storms pass by.[62] Hailstorms normally last from a few minutes up to 15 minutes in duration.[32] Accumulating hail storms can blanket the ground with over 2 in (5.1 cm) of hail, cause thousands to lose power, and bring down many trees. Flash flooding and mudslides within areas of steep terrain can be a concern with accumulating hail.[63]
Depths of up to 18 in (0.46 m) have been reported. A landscape covered in accumulated hail generally resembles one covered in accumulated snow and any significant accumulation of hail has the same restrictive effects as snow accumulation, albeit over a smaller area, on transport and infrastructure.[64] Accumulated hail can also cause flooding by blocking drains, and hail can be carried in the floodwater, turning into a snow-like slush which is deposited at lower elevations.
On somewhat rare occasions, a thunderstorm can become stationary or nearly so while prolifically producing hail and significant depths of accumulation do occur; this tends to happen in mountainous areas, such as the July 29, 2010 case[65] of a foot of hail accumulation in Boulder County, Colorado. On June 5, 2015, hail up to four feet deep fell on one city block in Denver, Colorado. The hailstones, described as between the size of bumble bees and ping pong balls, were accompanied by rain and high winds. The hail fell in only the one area, leaving the surrounding area untouched. It fell for one and a half hours between 10:00 pm and 11:30 pm. A meteorologist for the National Weather Service in Boulder said, "It's a very interesting phenomenon. We saw the storm stall. It produced copious amounts of hail in one small area. It's a meteorological thing." Tractors used to clear the area filled more than 30 dump truck loads of hail.[66]

Research focused on four individual days that accumulated more than 5.9 inches (15 cm) of hail in 30 minutes on the Colorado front range has shown that these events share similar patterns in observed synoptic weather, radar, and lightning characteristics,[67] suggesting the possibility of predicting these events prior to their occurrence. A fundamental problem in continuing research in this area is that, unlike hail diameter, hail depth is not commonly reported. The lack of data leaves researchers and forecasters in the dark when trying to verify operational methods. A cooperative effort between the University of Colorado and the National Weather Service is in progress. The joint project's goal is to enlist the help of the general public to develop a database of hail accumulation depths.[68]
Suppression and prevention
[edit]During the Middle Ages, people in Europe used to ring church bells and fire cannons to try to prevent hail, and the subsequent damage to crops. Updated versions of this approach are available as modern hail cannons. Cloud seeding after World War II was done to attempt to eliminate the hail threat,[13] particularly across the Soviet Union, where it was claimed a 70–98% reduction in crop damage from hail storms was achieved by deploying silver iodide in clouds using rockets and artillery shells.[69][70] But these effects have not been replicated in randomized trials conducted in the West.[71] Hail suppression programs have been undertaken by 15 countries between 1965 and 2005.[13][27]
See also
[edit]References
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- ^ "Hailstorm". Glossary of Meteorology. American Meteorological Society. 2009. Archived from the original on 2011-06-06. Retrieved 2009-08-29.
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- ^ "Hail Basics". NOAA National Severe Storms Laboratory. Archived from the original on 2023-10-11. Retrieved 2024-04-14.
Hailstones can have layers of clear and cloudy ice if the hailstone encounters different temperature and liquid water content conditions in the thunderstorm. The conditions experienced by the hailstone can change as it passes horizontally across or near an updraft.
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- ^ "SA-METAR". Alaska Air Flight Service Station, Federal Aviation Administration. 2007-04-10. Archived from the original on May 1, 2008. Retrieved 2009-08-29.
- ^ "Hail Basics". National Severe Storms Laboratory, National Oceanic and Atmospheric Administration. 2006-11-15. Archived from the original on 2009-05-06. Retrieved 2009-08-28.
- ^ National Weather Service (July 26, 2021). "National Weather Service Instruction 10 - 1605" (PDF). Archived (PDF) from the original on June 27, 2023. Retrieved June 26, 2023.
- ^ "World: Heaviest Hailstone". wmo.asu.edu. ASU World Meteorological Organization. Archived from the original on 2015-06-29. Retrieved 2016-07-23.
- ^ a b "Appendix I – Weather Extremes" (PDF). San Diego, California: National Weather Service. Archived from the original (PDF) on 28 May 2008. Retrieved 2010-06-01.
- ^ "Record Setting Hail Event in Vivian, South Dakota on July 23, 2010". Aberdeen, South Dakota: National Weather Service. 30 July 2010. Archived from the original on 1 August 2010. Retrieved 2010-08-03.
- ^ "Largest Hailstone in U.S. History Found". nationalgeographic.com. National Geographic. Archived from the original on 2010-04-20. Retrieved 2010-08-20.
- ^ "What Places in the World Usually Have the Most Hail in One Year?". 2013-04-12. Archived from the original on 2017-10-17. Retrieved 2017-10-16.
- ^ Glenday, Craig (2013). Guinness World Records 2014. Guinness World Records Limited. p. 22. ISBN 978-1-908843-15-9.
- ^ Cline, Joseph L. (May 1926). "HAILSTORM AT DALLAS, TEX., MAY 8, 1926". Monthly Weather Review. 54 (5): 216. Bibcode:1926MWRv...54..216C. doi:10.1175/1520-0493(1926)54<216a:HADTM>2.0.CO;2. Retrieved 2025-08-23.
- ^ "Hail Damage to Roofs". adjustersinternational.com. Adjusting Today. Archived from the original on 2015-10-16. Retrieved 2009-12-11.
- ^ "More damaging than tornadoes, hail may finally get the scientific attention it deserves". www.science.org. Retrieved 2025-02-26.
- ^ Field, P.R.; Hand, W.H.; Cappelluti, G.; et al. (November 2010). "Hail Threat Standardisation" (PDF). European Aviation Safety Agency. RP EASA.2008/5. Archived from the original (PDF) on 2013-12-07.
- ^ "Hazards". aviationweather.ws. Federal Aviation Administration. 2009. Archived from the original on 2010-03-25. Retrieved 2009-08-29.
- ^ Coppola, Damon P. (2007). Introduction to international disaster management. Butterworth-Heinemann. p. 62. ISBN 978-0-7506-7982-4.
- ^ Orr, David (2004-11-07). "Giant hail killed more than 200 in Himalayas". Telegraph Group Unlimited via the Internet Wayback Machine. Archived from the original on 2005-12-03. Retrieved 2009-08-28.
- ^ Ferreira, Becky (2019-08-20). "Nobody Knows Why Hundreds of People Died at This Creepy Himalayan Lake". Retrieved 2025-05-09.
- ^ Christopher C. Burt (2020-05-23). "U.S. Hailstone and Hailstorm Records". Weather Underground.
- ^ "Hail Climatology". National Severe Storms Laboratory, National Oceanic and Atmospheric Administration. 2006-10-09. Archived from the original on 2009-06-13. Retrieved 2009-08-29.
- ^ Peters, Albert J. (2003-03-03). "Crop Hail Damage Assessment" (PDF). inria.fr. Institut National De Recherche En Informatique Et En Automatique. Archived from the original (PDF) on 2011-07-21. Retrieved 2009-08-28.
- ^ Carmichael, Harold (2009-06-15). "Sudbury lashed by freak storm; hail pummels downtown core". Sudbury Star. Sun Media. Archived from the original on 2009-06-16. Retrieved 2009-08-28.
- ^ Schlatter, Thomas W.; Doesken, Nolan (September 2010). "Deep Hail: Tracking an Elusive Phenomenon". Weatherwise. 63 (5). Taylor & Francis: 35–41. Bibcode:2010Weawi..63e..35S. doi:10.1080/00431672.2010.503841. ISSN 0043-1672. S2CID 191481064. Retrieved 2015-08-09. [permanent dead link]
- ^ Rubino, Joe (2010-07-29). "Boulder County cleans up Nederland-area roadways after foot-deep hailstorm". Colorado Daily. Archived from the original on 2015-06-10. Retrieved 2014-12-20.
- ^ Mitchell, Kirk (5 June 2015). "One Denver block buried under up to 4 feet of hail". The Denver Post. Archived from the original on 6 June 2015. Retrieved 7 June 2015.
- ^ Kalina, E.; et al. (26 October 2015). "Colorado Plowable Hailstorms: Synoptic Weather, Radar and Lightning Characteristics". Weather and Forecasting. 31 (2): 663. Bibcode:2016WtFor..31..663K. doi:10.1175/WAF-D-15-0037.1. Archived from the original on 18 February 2021. Retrieved 28 June 2019.
- ^ "Deep Hail Project – Report your hail depth!!". University of Colorado Boulder. Archived from the original on 2016-07-08. Retrieved 2016-06-14.
- ^ Abshaev, M. T.; Abshaev, A. M.; Malkarova, A. M. (22–24 October 2007). Radar Estimation of Physical Efficiency of Hail Suppression Projects. 9th WMO Scientific Conference on Weather Modification. Antalya, Turkey. pp. 228–231.
- ^ Abshaev, M. T.; Abshaev, A. M.; Malkarova, A. M. (2012). "Estimation of antihail projects efficiency considering the tendency of hail climatology change". WWRP. 2012–2. Bali, Indonesia: 10th WMO Scientific Conference on Weather Modification: 1–4.
- ^ Federer, B.; Waldvogel, A.; Schmid, W.; et al. (1986-07-07). "Main Results of Grossversuch IV". Journal of Climate and Applied Meteorology. 25 (7): 917–957. Bibcode:1986JApMe..25..917F. doi:10.1175/1520-0450(1986)025<0917:MROGI>2.0.CO;2. JSTOR 26182470.
Further reading
[edit]- Rogers and Yau (1989). A Short Course in Cloud Physics. Massachusetts: Butterworth-Heinemann. ISBN 0-7506-3215-1.
- Jim Mezzanotte (2007). Hailstorms. Gareth Stevens Publishing. ISBN 978-0-8368-7912-4.
- Snowden Dwight Flora (2003). Hailstorms of the United States. Textbook Publishers. ISBN 978-0-7581-1698-7.
- Narayan R. Gokhale (1974). Hailstorms and Hailstone Growth. State University of New York Press. ISBN 978-0-87395-313-9.
- Duncan Scheff (2001). Ice and Hailstorms. Raintree Publishers. ISBN 978-0-7398-4703-9.
External links
[edit]- Hail Storm Research Tools Archived 2022-02-02 at the Wayback Machine at hailtrends.com
- Hail Factsheet (archived) from ucar.edu
- U.S. Billion-dollar Weather and Climate Disasters Archived 2018-07-26 at the Wayback Machine at NOAA.gov
Definition and Characteristics
Definition
Hail is a form of solid precipitation consisting of balls or irregular lumps of ice that form within the updrafts of thunderstorm clouds. These ice particles, known as hailstones, typically range from 5 mm to 50 mm in diameter, though they can grow larger under favorable conditions. Unlike liquid rain or snow, hail develops through the freezing of supercooled water droplets around a nucleus, resulting in dense, layered structures that fall to the ground when they become too heavy to be supported by the cloud's updrafts.[8][2] The term "hail" originates from Old English hagol or hægl, meaning "hailstone" or "frozen precipitation," derived from Proto-Germanic *haglaz, which traces back to the Proto-Indo-European root *kaghlo- signifying "small stone" or "hail." This etymology reflects the ancient recognition of hail as sharp, stone-like ice that can "harass" crops, property, and people due to its potential for significant damage during storms. Hail's hazardous reputation stems from its ability to dent vehicles, shatter windows, and injure individuals, often occurring suddenly within severe thunderstorms.[9] Hail is distinguished from softer forms of frozen precipitation like graupel, also known as soft hail or snow pellets, which consist of fragile, rimed snow particles typically smaller than 5 mm and lacking the hard, concentric layers formed by repeated freezing. True hail, in contrast, comprises hard ice that results from multiple cycles of accretion and freezing, producing opaque rime layers alternating with clearer ice shells. For severe weather reporting in the United States, the National Weather Service classifies hail as severe when it reaches or exceeds 1 inch (25.4 mm) in diameter, triggering warnings for potential widespread damage.[10][11]Distinction from Other Precipitation
Hail is distinguished from other forms of frozen precipitation primarily by its formation within intense convective processes, resulting in larger, denser ice particles that exhibit unique structural characteristics, unlike the smaller, more uniform pellets or crystals produced in layered atmospheric temperature profiles typical of winter weather.[10] In contrast to sleet, which consists of small, round ice pellets typically 2 to 6 millimeters in diameter formed when partially melted snowflakes refreeze during descent through a subfreezing layer near the surface, hail develops into larger, irregularly shaped stones without such uniform simplicity.[12] Sleet lacks the concentric layering seen in hail due to its origin as frozen raindrops rather than accreted supercooled droplets in turbulent updrafts.[13] Graupel, often mistaken for small hail, forms as soft, opaque, and fragile pellets through the rime coating of snowflakes by supercooled water droplets, resulting in a spongy texture that crushes easily under pressure and lacks the translucent, onion-like layering of hail.[10] While graupel particles are generally smaller than 5 millimeters and disintegrate readily upon handling, hail maintains a hard, dense composition capable of reaching diameters exceeding 25 millimeters.[13] Snow differs fundamentally from hail in its crystalline structure and low density, arising from the direct deposition of water vapor onto ice nuclei in cold clouds to form delicate, branched flakes that aggregate into fluffy accumulations, whereas hail comprises compact, solid ice masses from the freezing of liquid water.[14] The airy, low-density nature of snow, often with densities below 0.1 g/cm³, contrasts sharply with hail's higher density, typically around 0.9 g/cm³, reflecting their disparate growth mechanisms.[13] Observationally, hail is associated with towering cumulonimbus clouds during warm-season thunderstorms, frequently accompanied by thunder, lightning, and heavy rain, setting it apart from the steady, stratiform precipitation of sleet, graupel, or snow that occurs under stable, cold frontal conditions without convective intensity.[15]Formation
Process of Hail Formation
Hail formation begins in the strong updrafts of cumulonimbus clouds associated with thunderstorms, where regions of supercooled water droplets exist at temperatures below 0°C. These droplets, which remain liquid due to the lack of sufficient ice nuclei, freeze upon encountering suitable nuclei such as dust particles, bacterial cells, or other atmospheric aerosols. Freezing typically occurs between 0°C and -40°C through heterogeneous nucleation, creating small ice particles known as embryos that serve as the starting point for hailstone development.[2][16] The initial growth of these embryos integrates the Bergeron-Findeisen process, in which ice crystals preferentially attract water vapor from the air because the saturation vapor pressure over ice is lower than over supercooled liquid water at the same temperature. This diffusion of vapor onto the ice surfaces causes the crystals to enlarge while nearby supercooled droplets evaporate to supply the vapor. As the growing ice particles are carried upward, they transition to riming, a process where they collide with supercooled droplets that freeze instantly upon impact, adding opaque layers of rime ice and significantly increasing the particle's mass.[17] Embryonic hailstones undergo a cyclical growth process driven by the thunderstorm's updrafts, which must exceed approximately 20 m/s to repeatedly lift the particles through the freezing levels of the cloud. Each cycle allows further accretion of supercooled water via riming, building concentric layers until the hailstone's mass causes its terminal velocity to surpass the updraft speed. At this point, the hailstone is no longer supported and descends, potentially passing through warmer regions before falling as precipitation, though in intense storms, multiple traversals can produce larger stones.[18][3] The updraft velocity threshold critical for sustaining this process can be approximated using air parcel theory, which models the buoyant ascent of air in thunderstorms. The minimum updraft speed required to reach the necessary heights for hail growth is where is the acceleration due to gravity (), is the parcel's temperature excess over the environment, is the vertical distance traversed, and is the absolute environmental temperature. This arises from the buoyancy equation , integrated assuming constant buoyancy to yield , providing the speed at which a parcel accelerates to height . In practice, updrafts must exceed hailstone terminal velocities, often 20 m/s or more, to enable the repeated cycles essential for significant hail development.[19]Internal Structure of Hailstones
Hailstones typically exhibit a concentric, onion-like layered structure visible in cross-sections, consisting of alternating bands of clear and opaque ice that reflect successive episodes of growth in varying atmospheric conditions. Clear layers form during wet growth regimes, where accreted supercooled water spreads across the surface and freezes slowly, allowing air bubbles to escape and resulting in denser, translucent ice. Opaque layers, in contrast, arise from dry growth, characterized by rapid freezing of supercooled droplets that traps air bubbles, producing milky or rime ice with lower density. These layers can number from 2 to 6 or more in individual hailstones, indicating multiple fluctuations between growth modes rather than strictly cyclic updraft traversals.[20][21][22] The density of hailstones varies significantly between layers, averaging 800–900 kg/m³ overall, but opaque rime layers are less dense (often 100–800 kg/m³) due to the incorporation of air pockets during rapid freezing. Clear ice layers approach the density of pure ice at approximately 917 kg/m³, as the slower freezing process minimizes void formation. These variations influence the hailstone's overall mass and fall behavior, with spongy structures in wet-growth regions further reducing local density through retained liquid or partial freezing.[23][24] Analysis of hailstone internal structure relies on techniques such as thin-section microscopy, where samples are sliced to 150 µm thickness and examined under transmitted light or crossed polaroids to reveal bubble distributions, crystal sizes, and layer boundaries. Computed tomography (CT) scans provide non-destructive 3D imaging, quantifying layer densities via Hounsfield units and identifying off-center nuclei or irregular growth patterns in giant hailstones up to 12 cm in diameter. Isotopic studies of δ²H and δ¹⁸O in successive layers trace growth history by correlating compositions with ambient temperatures, distinguishing embryo formation (often -8.7°C to -33.4°C) from outer shells and revealing vertical trajectories with minimal or alternating movement. These methods indicate wet growth in regimes where surface temperatures reach 0°C (typically associated with environmental temperatures above -10°C and high liquid water content) versus dry growth below -10°C, where immediate freezing dominates.[25][21][22][20] At the core, hailstones usually feature an embryo of frozen raindrops or graupel particles less than 1 cm in diameter, providing the initial nucleus for radial growth and often exhibiting symmetry in well-developed specimens. Graupel embryos form through aggregation of ice crystals and riming in colder regions, while frozen raindrops initiate in warmer, mixed-phase zones; isotopic signatures in embryos frequently point to formation below -20°C via mineral dust nucleation. This central structure anchors the layered accretion, with subsequent shells building outward in response to updraft encounters.[20][22]Environmental Factors Favoring Hail
Hail formation is favored in environments characterized by high thermodynamic instability, particularly convective available potential energy (CAPE) values exceeding 1500 J/kg, which provide the energy for strong updrafts necessary to suspend hailstones during growth.[26] Steep lapse rates, often greater than 7°C/km in the lower troposphere, further enhance this instability by allowing air parcels to accelerate rapidly upon ascent, contributing to the development of supercell thunderstorms capable of producing significant hail.[27] These conditions are most conducive when surface heating intensifies buoyancy, enabling parcels to reach the hail growth zone between -10°C and -30°C. Moderate low-level moisture, typically indicated by precipitable water (PWAT) values of 20-35 mm, supplies the supercooled liquid water essential for hailstone accretion while allowing strong updrafts; excessively high PWAT can water-load updrafts and favor rain over large hail.[28] Vertical wind shear exceeding 15-20 m/s in the 0-6 km layer promotes storm organization into rotating supercells.[29] This shear separates updraft and downdraft regions, prolonging storm duration and allowing hail to grow larger before falling; without sufficient shear, storms may dissipate quickly or produce only small hail.[30] The combination of moisture and shear is critical, as excessive dryness can limit liquid water availability, whereas overly saturated environments may favor rain over hail. Geographically, hail is most prevalent in mid-latitude continental regions like the U.S. Great Plains, known as "Hail Alley," where frequent clashes between warm, moist Gulf air and dry, cool continental air masses generate the necessary instability and shear.[2] This area experiences 7-9 hail days per year on average due to these synoptic patterns. In contrast, tropical regions produce hail less frequently because of weaker updrafts and higher freezing levels, which reduce the time available for hail growth despite high moisture.[31] Seasonally, hail peaks in spring and summer, when diurnal heating maximizes CAPE and low-level moisture convergence, with activity shifting northward across the Plains from April to July.[32]Physical Properties
Size and Shape Variations
Hailstones exhibit a wide spectrum of sizes, typically ranging from small graupel particles of 5–10 mm in diameter, often likened to peas, to larger stones reaching 40 mm (golf ball-sized) or even 100 mm (softball-sized) in exceptional cases.[33][34] Most hailstones fall within the smaller end of this range, with diameters under 25 mm comprising the majority in typical storms.[2] The shapes of hailstones vary significantly, often appearing as oblate spheroids, triaxial ellipsoids, or irregular forms with protuberances such as spikes, lobes, or conical protrusions.[35][34] Aerodynamic tumbling during descent contributes to oblate or irregular morphologies, while the stone's density influences shape stability, with lower-density hail tending toward more irregular configurations.[34] Conical shapes and spiky lobes are particularly associated with dry growth regimes, where rapid freezing without surface melting leads to opaque, low-density rime ice structures.[35] To quantify size and shape variations, researchers employ hail pads—typically styrofoam panels covered in thin aluminum foil—deployed on the ground to capture impact imprints from falling stones.[36] These imprints allow for analysis of dent diameters and distributions, enabling reconstruction of hailstone size spectra and kinetic energy estimates through calibrated measurements.[37] Complementary methods include manual caliper measurements and 3D laser scanning of collected samples for precise axis ratios and volumes.[34] Factors such as prolonged exposure to strong updrafts in thunderstorms drive larger hail sizes by extending the time available for accretion of supercooled water droplets.[38] High-wind conditions during growth can further promote irregular shapes like cones or spikes, reflecting turbulent trajectories and variable collection efficiencies.[35] Internal layering from alternating wet and dry growth phases may contribute to overall size buildup but primarily affects density rather than external morphology.[38]Terminal Velocity
The terminal velocity of a hailstone represents the constant speed it reaches during free fall when the downward gravitational force balances the upward drag force from the air. This equilibrium occurs when the weight of the hailstone, , equals the drag force, , where is the mass, is gravitational acceleration (), is air density, is terminal velocity, is the drag coefficient, and is the cross-sectional area. Solving for yields the formula For spherical hailstones, this simplifies to where is hailstone density (typically around 900 kg/m³) and is diameter, assuming and .[39] The drag coefficient for hailstones ranges from 0.5 to 1.0, varying with size, shape irregularity, and surface roughness; smoother, spherical hailstones approach 0.5, while lobed or rough ones exceed 0.8. Terminal velocities increase with hailstone size due to greater mass relative to drag area, following roughly . Representative values at sea level include approximately 10–14 m/s for 10 mm diameter hail and 40–50 m/s for 50 mm diameter hail.[39][40][41] Environmental conditions modify terminal velocity beyond size effects. Lower air density at higher altitudes reduces drag, increasing by up to 20–30% compared to sea level for the same hailstone, as . Partial melting during descent decreases mass and effective diameter, thereby reducing and altering trajectory.[39][41][2] The kinetic energy of a falling hailstone, , scales quadratically with terminal velocity, amplifying the potential for structural stress upon impact as size and fall speed increase. This relationship underscores how larger hailstones, despite rarer, pose disproportionate threats due to elevated energy delivery.[41][39] Wind tunnel experiments using 3D-printed replicas of natural hailstones have validated these models, confirming that irregular shapes elevate and reduce by 10–20% relative to spheres of equivalent volume, with measurements aligning closely to the drag balance equation across Reynolds numbers from to .[24]Records and Comparisons
The largest verified hailstone on record in the United States measured 8 inches (20.3 cm) in diameter, with a circumference of 18.6 inches (47.2 cm), and fell near Vivian, South Dakota, on July 23, 2010.[4] This specimen, weighing approximately 1.94 pounds (0.88 kg), remains the benchmark for diameter in North America, surpassing previous records and highlighting the extreme conditions in supercell thunderstorms. Globally, while heavier hailstones have been documented—such as those weighing up to 1.02 kg (2.25 lb) in Bangladesh in 1986—the Vivian stone holds the record for diameter.[42] More recent notable events include a hailstorm in Texas on May 25, 2025, producing stones up to 6 inches (15 cm) in diameter near Afton, though no verified measurements have exceeded the 2010 record as of 2025.[43] Another significant occurrence was in Vigo Park, Texas, on June 2, 2024, where a hailstone measured 7.25 inches (18.4 cm) in diameter, approaching but not surpassing the U.S. record.[44] To visualize hail sizes, common diameters are often compared to everyday objects, aiding in understanding their scale and relative rarity:| Diameter | Approximate Size Analogy | Typical Context |
|---|---|---|
| 1 cm (0.4 in) | Marble | Common in weak thunderstorms; minimal hazard. |
| 4 cm (1.6 in) | Ping-pong ball | Severe hail threshold; frequent in moderate storms. |
| 7 cm (2.8 in) | Baseball or golf ball | Indicates strong updrafts; less common. |
| 20 cm+ (7.9 in+) | Softball or bowling ball | Extreme events; requires prolonged supercell conditions. |
