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Altostratus cloud
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Altostratus is a middle-altitude cloud genus made up of water droplets, ice crystals, or a mixture of the two. Altostratus clouds are formed when large masses of warm, moist air rise, causing water vapor to condense. Altostratus clouds are usually gray or blueish featureless sheets, although some variants have wavy or banded bases. The sun can be seen through thinner altostratus clouds, but thicker layers can be quite opaque.
Altostratus clouds usually predict the arrival of warm fronts. Once altostratus clouds associated with a warm front arrive, continuous rain or snow will usually follow in the next 12 to 24 hours. Although altostratus clouds predict the arrival of warmer, wetter weather, they themselves do not produce significant precipitation. Thunderstorms can be embedded in altostratus clouds, however, bringing showers.
Because altostratus clouds can contain ice crystals, they can produce some optical phenomena like iridescence and coronas.
Description
[edit]
Altostratus clouds are generally gray or blue-tinged with a largely-uniform blanket-like appearance. They do not have distinct features, and usually do not produce precipitation. The name "altostratus" comes from the conjugation of the Latin words "altum", meaning "high", and "stratus", meaning "flat" or "spread out".[1][2] Altostratus clouds can produce virga, causing the cloud base to appear hazy.[3] While they do not produce significant precipitation, altostratus clouds can cause light sprinkles or even small rain showers.[4] Consistent rainfall and lowering of the cloud base causes altostratus to become nimbostratus.[5]
Unlike most other types of clouds, altostratus clouds are not subdivided into cloud species due to their largely-featureless appearance.[6] However, they still appear in five varieties: Altostratus duplicatus, opacus, radiatus, translucidus, and undulatus.[7] Altostratus duplicatus is a rare form of altostratus clouds composed of two or more layers of cloud.[8] Translucidus is a translucent form of altostratus clouds, meaning that the sun or moon can be seen through the cloud,[9] whereas the opacus variety is opaque.[10] Radiatus is another rare variety. It has parallel bands of cloud that stretch toward the horizon.[11] The undulatus variety has an wavy appearance—the underside of the cloud appears to rise and fall.[12]
Altostratus and altocumulus clouds, both of which are mid-level clouds,[4] are commonly measured together in cloud cover studies. Together, they cover around 25% of the Earth's surface on average[13] based on CALIPSO satellite data.[14] This constitutes roughly one third of the Earth's total cloud cover.[13] By itself, separated from altocumulus, altostratus covers ~16% of the Earth's surface.[13] Altostratus cloud cover varies seasonally in temperate regions, with significantly less coverage in the summer months as compared to the other seasons. Additionally, altostratus cloud cover varies by latitude, with tropical regions having vastly fewer altostratus clouds when compared to temperate or polar regions.[15] Altostratus and altocumulus cover roughly 22% of the ocean's surface based on surface measurements, with minimal variation based on season.[16]
Altostratus clouds are warmest at the bottom and coldest at the top,[17] with a fairly consistent[18] lapse rate of 5 to 7 °C per kilometer (14 to 20 °F per mile) inside the cloud. The lapse rate is the rate at which the temperature decreases with altitude.[19] Higher lapse rates (i.e. the faster temperature drops with increasing altitude) were associated with colder clouds.[18] The average temperature of altostratus clouds, based on data collected from roughly 45° to 80° latitude, varied from around −16 to −45 °C (3.2 to −49 °F). Warmer temperatures occurred during summer and colder temperatures during winter.[17]
Inside altostratus clouds, the relative humidity is generally greatest towards the top of the cloud decreasing slowly and roughly linearly towards the bottom. The lowest part of the cloud has the lowest relative humidity.[17] Below the bottom of the cloud, the relative humidity drops rapidly.[20]
Microphysical properties
[edit]Altostratus can be composed of water droplets, supercooled water droplets, and ice crystals,[4] but ice crystals make up the vast majority.[21] In some altostratus clouds made of ice crystals, very thin horizontal sheets of water droplets can appear seemingly at random, but they quickly disappear.[22] The sizes of the ice crystals in the cloud tended to increase as altitude decreased. However, close to the bottom of the cloud, the particles decreased in size again. During the sampling of one cloud, scientists noted a halo while flying near the top of the cloud, which indicated that the ice crystals were hexagonal near the top. However, farther down, the ice crystals became more conglomerated.[23][24] Mixed-phase (containing both ice and water) altostratus clouds contain a "melt layer", below which the ice crystals tend to melt into water droplets. These water droplets are spheres and thus fall much faster than ice crystals, collecting at the bottom of the cloud.[25]
Formation
[edit]
Altostratus clouds form when a large mass of warm air rises, causing water vapor in the atmosphere to condense onto nuclei (small dust particles), forming water droplets and ice crystals.[26] These conditions usually happen at the leading edge of a warm front, where cirrostratus clouds thicken and lower until they transition into altostratus clouds.[2] Alternatively, nimbostratus clouds can thin into altostratus.[27] Altostratus can even form from the spreading of the upper anvil cloud or the middle column of a thunderstorm.[27]
Altostratus clouds are mid-level clouds[4] that form from 2,000 to 4,000 metres (6,600 to 13,000 ft) above sea level in polar regions. In temperate regions, the ceiling increases drastically, allowing altostratus clouds to form between 2,000 to 7,000 metres (6,600 to 23,000 ft). In tropical regions, altostratus can reach even higher, forming from 2,000 to 8,000 metres (6,600 to 26,000 ft).[3] They can range from 1,000 to 5,000 metres (3,300 to 16,000 ft) in thickness[3] and can cover hundreds of kilometers of the Earth's surface.[28]
Use in forecasting
[edit]Altostratus clouds tend to form ahead of warm fronts or occluded fronts and herald their arrival.[2] These warm fronts bring warmer air into the region. Occluded fronts form when a faster-moving cold front catches up to a warm front, and the temperature after the frontal system passes may rise or fall.[29] As the frontal system approaches, cirrostratus clouds will thicken into altostratus clouds, which then gradually thicken further into nimbostratus clouds.[2][30] If the frontal system is occluded, cumulonimbus clouds may also be present.[29] Once the altostratus clouds have arrived, rain or snow will usually follow in the next 12 to 24 hours.[30]
Instability in the atmosphere can embed thunderstorms in an altostratus cloud,[3] although altostratus clouds themselves do not produce storms.[4]
Effects on climate
[edit]Globally, clouds reflect around 50 watts per square meter[a] of short-wave solar radiation back into space, cooling the Earth by around 12 °C (22 °F), an effect largely caused by stratocumulus clouds. However, at the same time, they reflect around 30 watts per square meter of long-wave (infrared) black body radiation emitted by the Earth back to Earth's surface, heating the Earth by around 7 °C (13 °F)—a process called the greenhouse effect. Cirrus and altostratus clouds are the top two sources of this heating effect. This combination of heating and cooling sums out to a net loss of 20 watts per square meter globally, cooling the Earth by roughly 5 °C (9.0 °F).[31][32][33][34]
Altostratus clouds are the only cloud genus besides cirrus clouds to exhibit a net global heating effect on Earth and its atmosphere; however, cirrus have a heating effect that is four times as potent as altostratus (2 watts per square meter versus only 0.5 watts per square meter).[35]
Optical phenomena
[edit]Altostratus clouds can produce bright halos when viewed from the air,[3] but not when viewed from the ground.[36] Halos can take the appearance of rings, arcs, or spots of white or multicolored light and are formed by the reflection and refraction of sunlight or moonlight shining through ice crystals in the cloud.[37] Light diffraction through altostratus clouds can also produce coronas, which are small, concentric pastel-colored rings of light around the sun or moon. They can also be iridescent, with often-parallel bands of bright color projected on a cloud. Unlike the halos, the coronas and iridescence can be seen from Earth's surface.[2][38]
Relation to other clouds
[edit]
Altostratus and altocumulus clouds are the two genera of mid-level clouds that usually form between 2,000 and 6,100 m (6,500 and 20,000 ft).[4][39] These are given the prefix "alto-". These clouds are formed from ice crystals, supercooled water droplets, or liquid water droplets.[4]
Above the mid-level clouds are three different genera of high-level clouds, cirrus, cirrocumulus, and cirrostratus, all of which are given the prefix "cirro-". High-level clouds usually form above 6,100 m (20,000 ft).[4][39][40] Cirrocumulus and cirrostratus are sometimes informally referred to as cirriform clouds because of their frequent association with cirrus.[41]
Below the mid-level clouds are the low-level clouds, which usually form below 2,000 m (6,500 ft) and do not have a prefix.[4][39] The two genera that are strictly low-level are stratus, and stratocumulus. These clouds are composed of water droplets, except during winter when they are formed of supercooled water droplets or ice crystals if the temperature at cloud level is below freezing. Three additional genera usually form in the low altitude range, but may be based at higher levels under conditions of very low humidity. They are the genera cumulus, and cumulonimbus, and nimbostratus. These are sometimes classified separately as clouds of vertical development, especially when their tops are high enough to be composed of supercooled water droplets or ice crystals.[42][4]
Cirrostratus
[edit]
Cirrostratus clouds can appear as a smooth veil in the sky[43] or as a striated sheet.[40] They are sometimes similar to altostratus and are distinguishable from the latter because the sun or moon is always clearly visible through transparent cirrostratus, in contrast to altostratus which tends to be opaque or translucent.[44] Cirrostratus come in two species, fibratus and nebulosus.[45] The ice crystals in these clouds vary depending upon the height in the cloud. Towards the bottom, at temperatures of around −35 to −45 °C (−31 to −49 °F), the crystals tend to be long, solid, hexagonal columns. Towards the top of the cloud, at temperatures of around −47 to −52 °C (−53 to −62 °F), the predominant crystal types are thick, hexagonal plates and short, solid, hexagonal columns.[46][47] These clouds commonly produce halos, and sometimes the halo is the only indication that such clouds are present.[30] They are formed by warm, moist air being lifted slowly to a very high altitude.[48] When a warm front approaches, cirrostratus clouds become thicker and descend forming altostratus clouds,[4] and rain usually begins 12 to 24 hours later.[30]
Altocumulus
[edit]
Altocumulus clouds are small patches or heaps of white or light gray cloud.[49][4] Like altostratus, altocumulus are composed of a mixture of water droplets, supercooled water droplets, and ice crystals. Although altocumulus clouds are mid-level clouds that form at roughly the same altitude as altostratus clouds, their formation methods are completely different. Altocumulus forms from convective (rising) processes,[4] whereas altostratus is usually formed by descending and thickening cirrostratus.[2]
Stratus
[edit]
Stratus are low-level clouds that are usually visually similar to altostratus.[4] Stratus comes in two species: nebulosus, a largely-featureless flat gray cloud sheet, and fractus, shattered fragments of cloud[50] often called "scud".[4] Opaque varieties of altostratus and stratus nebulosus clouds can be virtually indistinguishable from each other to the naked eye, to the point that the World Meteorological Organization suggests that one of the few ways to distinguish between these clouds is to check what types of clouds came before them.[51] Altostratus clouds, because they tend to form from warm fronts,[2] are usually preceded by high-level cirriform clouds.[51] Stratus clouds tend to form by cooling air masses, often at night,[52] and thus are not usually preceded by other types of clouds.[51]
Nimbostratus
[edit]Nimbostratus are low-level (sometimes classified as vertical) rain-bearing stratus clouds. Unlike the sprinkles or light drizzles that altostratus or stratus can produce, nimbostratus produces heavy, continuous rain or snow. These clouds are thick and dark enough to entirely blot out the sun.[4][53] Nimbostratus has no species[54] or varieties.[55] Like altostratus, nimbostratus clouds can be made of ice crystals, supercooled water droplets, or water droplets.[56]
See also
[edit]Notes
[edit]- ^ To break this number, down into practical terms, 50 watts is enough energy to raise the temperature of 1 liter (1 kilogram) of water by .012 °C every second or around 43 °C every hour. This amount of energy is being reflected by the averaged global cloud cover every single square meter.
Sources
[edit]- Footnotes
- ^ Cohn et al. 2017, Section 2.3.5.1
- ^ a b c d e f g "Altostratus clouds". Meteorological Office of the UK. Retrieved 25 March 2022.
- ^ a b c d e "Altostratus". International Cloud Atlas. World Meteorological Organization. Retrieved 25 March 2022.
- ^ a b c d e f g h i j k l m n o p Funk, Ted. "Cloud Classifications and Characteristics" (PDF). The Science Corner. NOAA. p. 1. Retrieved 25 March 2022.
- ^ Ahrens 2006, p. 194
- ^ Cohn et al. 2017, Section 2.3.5.2
- ^ Cohn et al. 2017, Section 2.3.5.3
- ^ Cohn et al. 2017, Section 2.3.5.3.3
- ^ Cohn et al. 2017, Section 2.3.5.3.1
- ^ Cohn et al. 2017, Section 2.3.5.3.2
- ^ Cohn et al. 2017, Section 2.3.5.3.5
- ^ Cohn et al. 2017, Section 2.3.5.3.4
- ^ a b c Sassen & Wang 2012, p. 688
- ^ Sassen & Wang 2012, p. 679
- ^ Sassen & Wang 2012, p. 686
- ^ Warren et al. 1988, Table 9b
- ^ a b c Yang & Zou 2013, p. 6010
- ^ a b Yang & Zou 2013, p. 6013
- ^ Yang & Zou 2013, p. 6011
- ^ Danne et al. 1999, p. 181
- ^ Sassen & Wang 2012, pp. 679–680
- ^ Platt 1977, p. 344
- ^ Field 1999, p. 1929
- ^ Field 1999, p. 1933
- ^ Danne et al. 1999, p. 182
- ^ "Clouds and How They Form". Center for Science Education. University Corporation for Atmospheric Research. Retrieved 28 March 2022.
- ^ a b Cohn et al. 2017, Section 2.3.5.5
- ^ Cohn et al. 2017, Section 2.3.5.7
- ^ a b "Weather Fronts". Center for Science Education. University Corporation for Atmospheric Research. Retrieved 28 March 2022.
- ^ a b c d Ahrens 2006, p. 120
- ^ "Cloud Climatology". International Satellite Cloud Climatology Program. National Aeronautics and Space Administration. Retrieved 12 July 2011.
- ^ "Cloud Radiative Effect". Geophysical Fluid Dynamics Laboratory. National Oceanic and Atmospheric Administration. Retrieved 29 March 2022.
- ^ L'Ecuyer et al. 2019, p. 6213
- ^ Riebeek, Holli (3 June 2010). "Global Warming: Feature Articles". Earth Observatory. National Aeronautics and Space Administration. Retrieved 29 March 2022.
- ^ L'Ecuyer et al. 2019, p. 6205
- ^ Cohn et al. 2017, Section 2.3.5.6.2
- ^ Cohn et al. 2017, Section 3.2.3.1
- ^ Cohn et al. 2017, Section 3.2.3.2 – 3.2.3.3
- ^ a b c "Classifying clouds". World Meteorological Organization. 18 January 2017. Archived from the original on December 18, 2023. Retrieved 14 March 2022.
- ^ a b Hubbard 2000, p. 340
- ^ "Cirriform – Glossary of Meteorology". American Meteorological Society. Retrieved 23 February 2022.
- ^ Koermer, Jim (2011). "Plymouth State Meteorology Program Cloud Boutique". Plymouth State University. Archived from the original on 10 May 2009. Retrieved 2 April 2012.
- ^ Cohn et al. 2017, Section 2.3.3.1
- ^ Day 2005, p. 56
- ^ Cohn et al. 2017, Section 2.3.3.2
- ^ Parungo 1995, p. 254
- ^ Parungo 1995, p. 256
- ^ Hamilton 2007, p. 24
- ^ Cohn et al. 2017, Section 2.3.4.1
- ^ Cohn et al. 2017, Section 2.3.8.2
- ^ a b c Cohn et al. 2017, Section 2.3.5.6.6
- ^ Cohn et al. 2017, Section 2.3.8.8
- ^ Cohn et al. 2017, Section 2.3.6.1
- ^ Cohn et al. 2017, Section 2.3.6.2
- ^ Cohn et al. 2017, Section 2.3.6.3
- ^ Cohn et al. 2017, Section 2.3.6.7
- Bibliography
- Ahrens, C. Donald (February 2006). Meteorology Today: An Introduction to Weather, Climate, and the Environment (8th ed.). Brooks Cole. ISBN 978-0-495-01162-0. OCLC 693475796.
- Cohn, Stephen; Bruhn, Michael; Anderson, George; Atkinson, Roger; Campos, Marinés; Galati, Federico; Lovell, Ernest; Rae, Colleen; Rüedi, Isabelle; Tam, Kwong Hung; Thürig-Jenzer, Eliane; Trice, Jim (2017). International Cloud Atlas. World Meteorological Organization. Retrieved 25 March 2022.
- Danne, O.; Quante, M.; Milferstädt, D.; Lemke, H.; Raschke, E. (February 1999). "Relationships between Doppler Spectral Moments within Large-Scale Cirro- and Altostratus Cloud Fields Observed by a Ground-Based 95-GHz Cloud Radar". Journal of Applied Meteorology and Climatology. 38 (2). American Meteorological Society: 175–189. Bibcode:1999JApMe..38..175D. doi:10.1175/1520-0450(1999)038<0175:RBDSMW>2.0.CO;2.
- Day, John A. (August 2005). The Book of Clouds. Sterling. ISBN 978-1-4027-2813-6. OCLC 61240837.
- Field, Paul R. (June 1999). "Aircraft Observations of Ice Crystal Evolution in an Altostratus Cloud". Journal of Applied Meteorology. 56 (12): 1925–1941. Bibcode:1999JAtS...56.1925F. CiteSeerX 10.1.1.595.2059. doi:10.1175/1520-0469(1999)056<1925:AOOICE>2.0.CO;2. ISSN 1520-0469.
- Hamilton, Gina (1 September 2007). Blue Planet – Air (eBook). Milliken Publishing. ISBN 978-1-4291-1613-8.
- Hang, Yun; L'Ecuyer, Tristan; Henderson, David; Matus, Alexander; Wang, Zhien (1 October 2019). "Reassessing the Effect of Cloud Type on Earth's Energy Balance in the Age of Active Spaceborne Observations. Part II: Atmospheric Heating". Journal of Climate. 32 (19). American Meteorological Society: 6219–6236. Bibcode:2019JCli...32.6219H. doi:10.1175/JCLI-D-18-0754.1.
- Hubbard, Richard Keith (5 May 2000). "Glossary". Boater's Bowditch: The Small Craft American Practical Navigator (2nd ed.). International Marine/Ragged Mountain Press. ISBN 978-0-07-136136-1.
- "Altostratus Cloud (in Atmospheric Chemistry)" (PDF). IUPAC Compendium of Chemical Terminology (2 ed.). International Union of Pure and Applied Chemistry (IUPAC). 1997. Archived from the original (PDF) on 4 March 2016. Retrieved 20 April 2011.
- L'Ecuyer, Tristan; Hang, Yun; Matus, Alexander; Wang, Zhien (1 October 2019). "Reassessing the Effect of Cloud Type on Earth's Energy Balance in the Age of Active Spaceborne Observations. Part I: Top of Atmosphere and Surface". Journal of Climate. 32 (19). American Meteorological Society: 6197–6217. Bibcode:2019JCli...32.6197L. doi:10.1175/JCLI-D-18-0753.1.
- Parungo, F. (May 1995). "Ice Crystals in High Clouds and Contrails". Atmospheric Research. 38 (1–4): 249–262. Bibcode:1995AtmRe..38..249P. doi:10.1016/0169-8095(94)00096-V. OCLC 90987092.
- Platt, C. M. R. (April 1977). "Lidar Observation of a Mixed-Phase Altostratus Cloud". Journal of Applied Meteorology. 16 (4): 339–345. Bibcode:1977JApMe..16..339P. doi:10.1175/1520-0450(1977)016<0339:LOOAMP>2.0.CO;2. ISSN 0021-8952.
- Sassen, Kenneth; Wang, Zhien (2012). "The Clouds of the Middle Troposphere: Composition, Radiative Impact, and Global Distribution". Surveys in Geophysics. 33 (3–4): 677–691. Bibcode:2012SGeo...33..677S. doi:10.1007/s10712-011-9163-x. S2CID 129776090.
- Warren, Stephen G.; Hahn, Carol J.; London, Julius; Chervin, Robert M.; Jenne, Roy L. (December 1988). "Global Distribution of Total Cloud Cover and Cloud Type Amounts over the Ocean". Office of Energy Research. United States Department of Energy. doi:10.2172/5415329. Retrieved 26 March 2022.
- Yang, S.; Zou, X. (15 August 2013). "Temperature Profiles and Lapse Rate Climatology in Altostratus and Nimbostratus Clouds Derived from GPS RO Data". Journal of Climate. 26 (16). American Meteorological Society: 6000–6014. Bibcode:2013JCli...26.6000Y. doi:10.1175/JCLI-D-12-00646.1.
Altostratus cloud
View on GrokipediaPhysical Characteristics
Appearance and Varieties
Altostratus clouds present as a grayish or blue-gray sheet or layer with a uniform, fibrous, or striated appearance, often covering the entire sky or large portions of it.[1] This featureless or subtly textured veil creates a diffused, watery light that partially reveals the position of the sun or moon in thinner sections, while thicker areas obscure celestial bodies entirely.[10] The overall effect is a somber, overcast sky without distinct edges or billows, distinguishing altostratus from more turbulent cloud forms.[1] These clouds form at mid-level altitudes, typically between 2 and 7 kilometers (6,500 to 23,000 feet) in temperate regions, though they occur lower at 2 to 4 kilometers (6,500 to 13,000 feet) in polar areas.[4] Their vertical thickness varies from about 1 kilometer to more than 5 kilometers (3,300 to over 16,500 feet), allowing for substantial optical depth that influences visibility.[4] According to the World Meteorological Organization (WMO) classification, altostratus exhibits several varieties based on transparency, layering, and arrangement. The translucidus variety features thinner sections that permit a translucent, watery view of the sun, while the opacus variety is denser and opaque, fully blocking solar or lunar discs.[11] The duplicatus variety appears as two or more superimposed layers with uneven bases, and radiatus shows parallel bands converging toward the horizon.[11] Additionally, undulatus displays wavy, undulating bases across the layer.[11] Supplementary features enhance identification of altostratus. Praecipitatio indicates ongoing precipitation reaching the ground, while virga consists of trailing precipitation streaks that evaporate before impact.[11] The translucency in varieties such as translucidus arises partly from embedded ice crystals scattering light.[1]Microphysical Composition
Altostratus clouds consist primarily of water droplets in their lower portions, with typical diameters of 10 to 20 μm, transitioning to predominantly ice crystals in the upper, colder regions where crystal diameters can extend up to 100 μm or more.[12][13] The combined liquid and ice water content in these clouds generally ranges from 0.1 to 0.5 g/m³, reflecting their stratiform nature with moderate condensation levels.[12] These clouds exhibit mixed-phase characteristics, where supercooled water droplets coexist with ice crystals—such as aggregates, dendrites, and hexagonal plates—at temperatures below 0°C, often spanning -1°C to -31°C.[12] This coexistence facilitates processes like the Bergeron-Findeisen mechanism, promoting gradual cloud thickening as ice crystals grow at the expense of surrounding vapor and droplets.[12] Particle distribution within altostratus forms uniform horizontal layers with minimal vertical turbulence, differing markedly from the disorganized structures in convective clouds; liquid water content often increases with height in single-layer formations.[12]Formation Processes
Atmospheric Conditions
Altostratus clouds form in stable, moist air masses at mid-tropospheric levels, typically requiring high relative humidity within the layer to support widespread condensation without significant vertical development. The temperature lapse rate in these environments approximates the moist adiabatic rate, ranging from 6 to 9°C per kilometer, which promotes gradual cooling and uniform cloud layer formation rather than convective instability.[14] In synoptic-scale settings, altostratus often develops ahead of warm or occluded fronts in mid-latitudes, where isentropic lift elevates moist air parcels along surfaces of constant potential temperature.[15] This uplift mechanism arises from large-scale convergence in baroclinic zones, fostering the slow ascent necessary for stratiform cloud decks spanning hundreds of kilometers. The characteristic air masses involve warm, moist tropical or maritime air overriding denser, cooler polar air at frontal boundaries, resulting in frontal convergence that supplies the moisture for cloud initiation.[16] Vertical wind shear remains minimal, allowing the cloud layer to maintain its horizontal uniformity without disruption from differential horizontal motions.[17] In polar regions, altostratus can also form within 2-4 km thick layers during polar low development, driven by cyclone-induced uplift in cold marine air outbreaks, a process highlighted in pre-2023 studies as understudied due to limited observations in high-latitude environments.[4][18][19]Developmental Stages
Altostratus clouds initiate their lifecycle as a thin layer of altostratus translucidus, forming through the gradual thickening of cirrostratus via sustained atmospheric uplift associated with approaching frontal systems.[20] This initial stage often emerges ahead of precipitation, as the veil-like cirrostratus descends and condenses further, transitioning into a uniform, grayish-blue sheet that partially veils the sun.[10] In the maturation phase, the cloud layer progressively thickens to altostratus opacus over several hours to a day, driven by continued uplift that promotes droplet coalescence and enhances the cloud's optical depth, ultimately obscuring solar visibility.[21] This evolution reflects increasing water content and droplet size, with the layer expanding vertically while maintaining a featureless, stratified appearance.[22] During the advanced stage, if uplift intensifies, altostratus opacus can transform into nimbostratus, marking the onset of widespread, steady precipitation as the cloud base lowers and rain or snow begins to fall.[21] Conversely, dissipation occurs through atmospheric drying or subsidence, which evaporates the cloud layer or disperses it, depending on synoptic persistence.[10] Altostratus may also form through other processes, including the thinning of nimbostratus layers or the spreading out of the upper parts of cumulonimbus or altocumulus sheets.[5]Meteorological Applications
Weather Forecasting
Altostratus clouds serve as key indicators in short-term weather forecasting, often signaling the impending arrival of precipitation. Their presence typically precedes steady light to moderate rain or snow within 6 to 24 hours, as the mid-level cloud layer advances ahead of warm fronts or low-pressure systems.[17][23] As altostratus thickens, a lowering of the cloud base—often from around 3 km to 1-2 km—heralds the transition to more persistent rainfall, eventually evolving into nimbostratus if conditions intensify.[24][10] Observers rely on ground-based visual cues for real-time assessment, particularly noting the translucidus variety where the sun appears diffused or "watery" through the semi-transparent sheet, indicating thinner sections less likely to produce immediate rain.[7] Radar reflectivity provides quantitative support, with values of 10-20 dBZ commonly associated with the onset of light precipitation from altostratus, allowing meteorologists to track the cloud's precipitation potential as it approaches.[25][26] In numerical weather prediction models like the European Centre for Medium-Range Weather Forecasts (ECMWF) Integrated Forecasting System and the Global Forecast System (GFS), altostratus is represented through cloud parameterization schemes that incorporate mid-level moisture and humidity profiles to simulate layer formation and evolution.[27][28] These schemes enhance the accuracy of frontal system timing by better resolving moisture advection, contributing to improved short-range precipitation forecasts. Recent advancements in AI-driven analysis using all-sky camera data have boosted identification of precipitating clouds, achieving up to 99% accuracy in determining rainfall potential.[29]Indicators of Frontal Systems
Altostratus clouds serve as a primary indicator of an approaching warm front, typically appearing 300 to 600 km ahead of the frontal boundary in mid-level layers formed by the gradual lifting of warm, moist air over cooler air masses.[30] As the front advances, these clouds thicken progressively, often leading to light precipitation and providing an early warning of steady rain or snow. In occluded fronts, where a cold front overtakes a warm front, altostratus exhibits faster thickening due to intensified uplift and convergence at the occlusion line.[31] The typical sequence of clouds in advancing frontal systems positions altostratus after the initial high-level cirrostratus and before the lower, rain-bearing nimbostratus, reflecting the descending cloud bases as the front nears.[32] A noticeable lowering of the altostratus base further signals the transition to occlusion, as the cloud layer merges with lower stratus formations and intensifies precipitation.[32] In mid-latitudes, altostratus presence commonly forecasts rain within 12 to 36 hours, allowing for preparation against prolonged overcast conditions and drizzle.[33] Regionally, variations occur; in tropical zones, altostratus links to monsoon onset, with bases elevated at 4 to 6 km owing to the warmer, more expansive troposphere that supports broader stratiform development.[34]Environmental and Climatic Roles
Radiation and Climate Effects
Altostratus clouds influence Earth's radiative balance by reflecting shortwave radiation and trapping longwave radiation. Mid-level clouds like altostratus have albedos typically ranging from 0.4 to 0.8, reflecting incoming solar radiation and contributing to a cooling effect at the top of the atmosphere.[35] Globally, cloud shortwave forcing is around -50 W/m², with mid-level clouds playing a role in this reflection. Conversely, they emit downward longwave radiation, providing a warming effect at the surface, estimated at 20-30 W/m² under overcast conditions in mid-latitudes.[36] The net radiative effect of mid-level clouds is generally cooling in mid-latitudes due to greater shortwave reflection compared to longwave trapping. They contribute to the overall global cloud radiative forcing of approximately -20 to -30 W/m². In polar regions, the longwave warming may dominate during winter. Altostratus enhances the planetary albedo relative to clear-sky conditions.[37] Cloud feedbacks involving mid-level clouds like altostratus are positive, amplifying warming through changes in cover and thickness with temperature increases. Aerosol-cloud interactions increase droplet numbers, enhancing scattering and contributing to the global effective radiative forcing from aerosol-cloud interactions of -1.0 ± 0.7 W/m². The IPCC AR6 notes the importance of mid-level clouds in extratropical feedbacks, with improved representation in recent models. Altostratus plays a role in extratropical weather systems, influencing cyclone development; CMIP6 models better capture their feedbacks.[38]Contribution to Precipitation
Altostratus clouds may produce light precipitation, such as drizzle or snow, often in the form of virga that evaporates before reaching the ground. Precipitation arises through collision-coalescence in lower portions and the Bergeron process in upper levels, but rates are typically low, less than 1 mm per hour.[39][1] Precipitation from altostratus is limited by dry air layers below, leading to frequent virga. In mid-latitudes, altostratus contributes minimally to total rainfall, mainly during stable frontal systems. Globally, their role in annual precipitation in temperate zones is small, with output increasing as they thicken into nimbostratus during fronts. Broader studies indicate potential increases in mid-level cloud-associated precipitation due to atmospheric moistening from climate warming.[10][38]Associated Phenomena
Optical Effects
Altostratus clouds, particularly the translucidus variety, allow the sun or moon to appear as a bright spot with a watery or fuzzy outline due to the diffuse transmission of light through their relatively thin layers of water droplets or ice crystals. This effect arises from the scattering and partial absorption of visible light, creating a ground-glass-like veil that vaguely reveals the celestial body without sharp contours.[40] In thinner portions of altostratus, coronas—colored rings surrounding the sun or moon with angular diameters typically 5–10 degrees—can form through diffraction by small, nearly uniform water droplets (often <25 μm in diameter). The mechanism follows Fraunhofer diffraction, where shorter wavelengths (blue) appear innermost and longer ones (red) outermost, with the ring size inversely proportional to droplet diameter via θ ≈ (λ / D), where θ is the angular radius, λ the wavelength, and D the particle size. These phenomena are most vivid in layers with narrow size distributions but are less common in uniform altostratus compared to thinner altocumulus.[41] Advanced optical effects like iridescence (swirling patches of spectral colors) or parhelia (sundogs) are possible but infrequent in altostratus, as the clouds' relatively uniform particle sizes and mixed-phase composition limit the spatial variability needed for pronounced interference or refraction patterns. Unlike cirrostratus, altostratus rarely produces strong halos, as confirmed by the absence of typical ice-crystal refraction signatures such as 22° rings.[40][41] The optical thickness of altostratus significantly reduces light transmission and contrast, leading to diminished visibility of underlying features. In the opacus variety, this results in color desaturation, where the sky takes on a uniform gray tone due to multiple scattering that randomizes photon directions and suppresses chromatic effects.[42][43]Other Meteorological Features
Altostratus clouds exhibit minimal low-level turbulence due to their stratiform structure and stable atmospheric layering, though some moderate turbulence may occur at mid-levels within the cloud layer.[44] These clouds often form in association with steady winds in frontal zones, where the gradual ascent of warm air over cooler masses promotes their development without intense shear.[45] In aviation contexts, this relative stability contributes to predictable flight conditions, but pilots must remain vigilant for occasional embedded turbulence during transitions to thicker cloud forms. Supplementary phenomena linked to altostratus include virga, where precipitation falls from the cloud but evaporates before reaching the ground, often appearing as hanging streaks beneath the cloud base.[6] Rare instances of thunder can occur during the thickening stages of altostratus, particularly when embedded convective elements develop prior to full transition to nimbostratus, as reported in pilot observations of lightning within these layers.[46] Additionally, the extensive cloud cover can lead to acoustic effects, such as muffled propagation of distant sounds, resulting from the dampening of sound waves by the dense overhead layer acting as a partial barrier.[47] Observational tools like lidar reveal the slow evolution of altostratus, capturing gradual changes in backscatter over hours as the cloud layer thickens uniformly.[48] For aviation, altostratus typically reduces surface visibility to 5-10 km due to the uniform gray veil diffusing sunlight, though this is generally better than under lower stratus decks and allows for visual flight rules operations with caution.[49]Relations to Other Cloud Types
Comparison with Cirrostratus
Altostratus clouds form at mid-level altitudes, typically between 2 and 7 kilometers (6,500 to 23,000 feet), whereas cirrostratus clouds occupy higher levels, ranging from 5 to 13 kilometers (20,000 to 40,000 feet). Altostratus primarily consist of a mixture of water droplets and ice crystals, with water droplets often dominant in their lower portions, while cirrostratus are composed exclusively of ice crystals. In appearance, altostratus present as thicker, gray or blue-gray sheets that cover much of the sky and obscure the sun or moon, preventing the casting of shadows on the ground, in contrast to the thinner, whiter, and more veil-like cirrostratus, which allow the sun or moon's disc to remain visible and cast shadows.[50][10] A common transition occurs when cirrostratus clouds thicken and descend through cooling and moisture addition, evolving into altostratus as they lower into warmer air layers.[51] Both cloud types can produce optical halos around the sun or moon due to ice crystal refraction, though these effects are more pronounced and frequent in cirrostratus and often fainter or absent in the denser altostratus.[50][10] Meteorologically, both altostratus and cirrostratus often appear ahead of warm or occluded fronts, sharing origins in large-scale lifting of moist air.[51] However, cirrostratus typically signals an approaching front 24 hours or more before precipitation, serving as an early indicator, while altostratus indicates the front is nearer, often within 6 to 12 hours, and may thicken into nimbostratus to produce rain or snow.[51] Unlike cirrostratus, which do not produce virga or precipitation, altostratus can exhibit virga—trails of falling precipitation that evaporate before reaching the ground—though this high-altitude persistence is less characteristic of altostratus compared to cirrostratus in transitional phases.[50][10][52]Comparison with Altocumulus
Altostratus and altocumulus clouds both occupy the mid-levels of the atmosphere, typically between 2 and 7 kilometers (6,500 and 23,000 feet) above the surface, but they differ markedly in structure and formation processes.[1][53] Altostratus manifests as a continuous, uniform gray or bluish sheet or layer, often striated or fibrous, that covers much of the sky with a stable, horizontally extensive appearance.[1] In contrast, altocumulus appears as white or gray patches, sheets, or layers composed of discrete, rounded masses, rolls, or laminae, exhibiting a more patchy and weakly convective texture.[53] This distinction arises from altostratus forming in stable air masses lifted by large-scale synoptic systems, while altocumulus develops through localized convection within conditionally unstable layers.[13]| Aspect | Altostratus | Altocumulus |
|---|---|---|
| Structure | Continuous, layered sheets; minimal vertical development | Discrete puffs or rolls; greater vertical development (typically 0.5–2 km thick for elements) |
| Precipitation | Possible light, continuous rain or snow; may thicken to produce steady precipitation | Mostly virga or no precipitation at the surface; rare light showers |
| Associated Weather | Indicates approach of steady warm fronts or cyclonic activity | Signals diurnal instability or elevated convection, often in fair weather or pre-thunderstorm conditions |