In meteorology, a cloud is a visible mass of liquid droplets or frozen crystals made of water or various chemicals suspended in the atmosphere above the surface of a planetary body. These suspended particles are also known as aerosols and are studied in the cloud physics branch of meteorology.
Terrestrial cloud formation is the result of air in any of the lower three principal layers of Earth's atmosphere (collectively known as the homosphere) becoming saturated due to either or both of two processes: cooling of the air and adding water vapor. With sufficient saturation in the troposphere, precipitation will fall to the surface; an exception is virga, which evaporates before reaching the surface. Clouds that form at very high altitudes in the stratosphere and mesosphere do not contain sufficient moisture to generate any outfall of droplets or crystals.
Clouds in the troposphere, the atmospheric layer closest to Earth's surface, have Latin names due to the universal adaptation of Luke Howard's nomenclature. It was introduced in December 1802 and became the basis of a modern international system that classifies these tropospheric aerosols into several physical forms, then cross-classifies them as low, middle and high-étage according to cloud-base altitude range above Earth's surface. Clouds with significant vertical extent occupying more than one étage are often considered a distinct group or sub-group.
One physical form shows free-convective upward growth into low or vertical cumuliform heaps. Other more layered types appear as non-convective stratiform sheets, and as limited-convective stratocumuliform rolls or ripples. Both these layered forms have low, middle, and high-étage variants with the latter two identified respectively by the prefixes alto- and cirro-. Thin cirriform wisps are found only at high altitudes of the troposphere. In the case of clouds with vertical extent, prefixes are used whenever necessary to express variations or complexities in their physical structures. These include cumulo- for complex highly convective cumulonimbiform storm clouds, and nimbo- for thick stratiform layers with sufficient vertical depth to produce moderate to heavy precipitation.
This process of cross-classification produces ten basic genus-types or genera (see genus classification chart, far right), most of which can be divided into subtypes consisting of species that are often subdivided into varieties where applicable. Synoptic surface weather observations use code numbers to record and report any type of tropospheric cloud visible at scheduled observation times based on its height and physical appearance.
Clouds that form above the troposphere have common names for their main types, but are sub-classified alpha-numerically rather than with the elaborate system of Latin names given to cloud types in the troposphere. Clouds have been observed on other planets and moons within the Solar System, but, due to their different temperature characteristics, they are often composed of other substances such as methane, ammonia, and sulfuric acid as well as water.
- 1 Etymology
- 2 History of cloud science and nomenclature
- 3 Tropospheric clouds
- 3.1 Physical forms, étages, and cross-classification into genera
- 3.1.1 Physical forms
- 3.1.2 Étages
- 3.2 Species
- 3.3 Varieties
- 3.4 Accessory clouds and supplementary features
- 3.5 Mother clouds
- 3.6 Stratocumulus fields
- 3.7 Reporting and mapping cloud types
- 3.8 Formation: how the air becomes saturated
- 3.9 Distribution: variable global prevalence and association with organized weather systems
- 3.10 Determination of properties
- 3.1 Physical forms, étages, and cross-classification into genera
- 4 Polar stratospheric clouds
- 5 Polar mesospheric clouds
- 6 Clouds throughout the homosphere
- 7 Extraterrestrial
- 8 See also
- 9 References
- 10 Bibliography
- 11 External links
The origin of the term cloud can be found in the old English clud or clod, meaning a hill or a mass of rock. Around the beginning of the 13th. century, it was extended metaphorically to include rainclouds as masses of evaporated water in the sky because of the similarity in appearance between a mass of rock and a cumulus heap cloud. Over time, the metaphoric term replaced the original old English weolcan to refer to clouds in general.
The science of clouds is nephology.
History of cloud science and nomenclature
Aristotle and Theophrastus
Ancient cloud studies were not made in isolation, but were observed in combination with other weather elements and even other natural sciences. In about 340 BC the Greek philosopher Aristotle wrote Meteorologica, a work which represented the sum of knowledge of the time about natural science, including weather and climate. For the first time, precipitation and the clouds from which precipitation fell were called meteors, which originate from the Greek word meteoros, meaning 'high in the sky'. From that word came the modern term meteorology, the study of clouds and weather. Meteorologica was a work of intuitive rather than scientific study. Nevertheless, it was the first known work that attempted to treat a broad range of meteorological topics.
Several years after Aristotle's, book, his pupil Theophrastus put together a book on weather forecasting called The Book of Signs. Various indicators such as solar and lunar halos formed by high clouds were presented as ways to forecast the weather. The combined works of Aristotle and Theophrastus had such authority they became the main influence in the study of clouds, weather and weather forecasting for nearly 2000 years.
Luke Howard and Jean-Baptiste Lamarck
After centuries of speculative theories about the formation and behavior of clouds, the first truly scientific studies were undertaken by Luke Howard in England and Jean-Baptiste Lamark in France. Howard was a methodical observer with a strong grounding in the Latin language and used his background to classify the various tropospheric cloud types during 1803. He believed that the changing cloud forms in the sky could unlock the key to weather forecasting. Jean-Baptiste Lamarck had worked independently on cloud classification the previous year and had come up with a different naming scheme that failed to make an impression even in his home country of France because it used unusual French names for cloud types. His system of nomenclature included twelve categories of clouds, with such names as (translated from French) hazy clouds, dappled clouds and broom-like clouds. By contrast, Howard used universally accepted Latin, which caught on quickly. As a sign of the popularity of the naming scheme, the German dramatist and poet Johann Wolfgang von Goethe composed four poems about clouds, dedicating them to Howard. Classification systems would be proposed by Heinrich Dove of Germany in 1828 and Elias Loomis of the United States in 1841, but neither met with international success. An elaboration of Howard's system was formally adopted by the International Meteorological Conference in 1891.
First comprehensive classification
Howard's original system established three general cloud forms based on physical appearance and process of formation: cirriform (mainly detached and wispy), cumuliform or convective (mostly detached and heaped, rolled, or rippled), and non-convective stratiform (mainly continuous layers in sheets). These were cross-classified into lower and upper étages. Cumuliform clouds forming in the lower level were given the genus name cumulus from the Latin word for heap, and low stratiform clouds the genus name stratus from the Latin word for sheet or layer. Physically similar clouds forming in the upper étage were given the genus names cirrocumulus (generally showing more limited convective activity than low level cumulus) and cirrostratus, respectively. Cirriform clouds were identified as always upper level and given the genus name cirrus from the Latin for 'fibre' ot 'hair. To these, Howard added the genus nimbus for clouds of complex structure producing significant precipitation that came to be identified as a distinct nimbiform physical category.
In 1840, German meteorologist Ludwig Kaemtz added stratocumulus as a mostly detached low-étage genus of limited convection with both cumuliform- and stratiform characteristics. This had the effect of creating a stratocumuliform type that included rolled and rippled clouds classified separately from the more freely convective heaped cumulus genus clouds.
About fifteen years later, Emilien Renou, director of the Parc Saint-Maur and Montsouris observatories, began work on an elaboration of Howard's classifications that would lead to the introduction during the 1870s of altocumulus (physically more closely related to stratocumulus than to cumulus) and altostratus. These were respectively stratocumuliform and stratiform cloud genera of a newly defined middle étage above stratocumulus and stratus but below cirrocumulus and cirrostratus.
In 1880, Philip Weilbach, secretary and librarian at the Art Academy in Copenhagen, and like Luke Howard, an amateur meteorologist, proposed and had accepted by the permanent committee of the International Meteorological Organization (IMO), a forerunner of the present-day World Meteorological Organization (WMO), the designation of a new free-convective vertical or multi-étage genus type, cumulonimbus, which would be distinct from cumulus and nimbus and identifiable by its often very complex structure (frequently including a cirriform top and what are now recognized as multiple accessory clouds), and its ability to produce thunder. With this addition, a canon of ten tropospheric cloud genera was established that came to be officially and universally accepted. At about the same time, several cloud specialists proposed variations that came to be accepted as species subdivisions and varieties determined by more specific variable aspects of the structure of each genus.
In 1890, Otto Jesse revealed the discovery and idenification of the first clouds known to form above the troposphere. He proposed the name noctilucent which is Latin for night shining. Because of the extremely high altitudes of these clouds in what is now known to be the mesosphere, they could become illuminated by the a sun's rays when the sky was nearly dark after sunset and before sunrise. Three years later, Henrik Mohn revealed a similar discovery of nacreous clouds in what is now considered the stratosphere.
In 1896, the first cloud atlas sanctioned by the IMO was produced by Teisserenc de Borte based on collaborations with Hugo H. Hildebrandsson. The latter had become the first researcher to use photography for the study and classification of clouds in 1879.
20th century developments
A further modification of the genus classification system came when an IMC commission for the study of clouds put forward a refined and more restricted definition of the genus nimbus which was effectively reclassified as a stratiform cloud type. It was then renamed nimbostratus and published with the new name in the 1932 edition of the International Atlas of Clouds and of States of the Sky. This left cumulonimbus as the only nimbiform type as indicated by its root-name.
On April 1, 1960, the first successful weather satellite, TIROS I (Television Infrared Observation Satellite), was launched from Cape Canaveral, Florida by the National Aeronautics and Space Administration (NASA) with the participation of The US Army Signal Research and Development Lab, RCA, the US Weather Bureau, and the US Naval Photographic Center. During its 78 day mission, it relayed thousands of pictures showing the structure of large-scale cloud regimes, and proved that satellites could provide useful surveillance of global weather conditions from space.
In 1976, the United Kingdom Department of Industry published a modification of the international cloud classification system adapted for satellite cloud observations. It was co-sponsored by NASA and showed a change in name of the nimbiform type to cumulonimbiform, although the earlier name and original meaning pertaining to all rain clouds can still be found in some classifications.
Physical forms, étages, and cross-classification into genera
Clouds can be divided into five physical forms based on physical structure and process of formation. These forms are commonly used for the purpose of satellite analysis.
The individual genus types result from the physical forms being cross-classified by étage within the troposphere. The base-height range for each étage varies depending on the latitudinal geographical zone. A consensus exists as to the designation of high, middle, and low étages, the makeup of the basic canon of ten cloud genera that results from this cross-classification, and the étage designations of non-vertical genus types. Clouds with significant vertical extent occupy more than one étage and are commonly (but not always) treated as a separate group or sub-group, or given separate descriptions within the context of the standard étages.
Genus cirrus (high-étage)
Cirriform clouds generally have the appearance of detached or semi-merged filaments and form at high tropospheric altitudes.
Genus cumulus (low or multi-étage)
Cumuliform clouds typically appear in isolated heaps. They are the product of localized but generally free-convective lift and can vary in vertical extent depending on the stability characteristics of the air mass where they are forming.
Genus cumulonimbus (vertical/multi-étage)
The largest free-convective clouds occur in very unstable air and often have complex structures that include cirriform tops and multiple accessory clouds.
In general, stratiform clouds have a flat sheet-like structure and form at any altitude in the troposphere. Very low stratiform cloud can form when advection fog is lifted above surface level during breezy conditions.
Clouds of this physical structure have both cumuliform and stratiform characteristics in the form of rolls or ripples and generally form as a result of limited convection in slightly unstable air topped by an inversion layer. They can form at any altitude in the troposphere whenever there is sufficient moisture and lift.
High cirriform, stratocumuliform, and stratiform
Clouds of the high-étage form at altitudes of 3,000 to 7,600 m (10,000 to 25,000 ft) in the polar regions, 5,000 to 12,200 m (16,500 to 40,000 ft) in the temperate regions and 6,100 to 18,300 m (20,000 to 60,000 ft) in the tropical region. All cirriform clouds are classified as high and thus constitute a single genus cirrus (Ci). Stratocumuliform and stratiform clouds in the high-étage carry the prefix cirro-, yielding the respective genus names cirrocumulus (Cc) and cirrostratus (Cs). Strato- is excluded from cirrocumulus to avoid double prefixing.
- Genus cirrus (Ci):
- These are mostly fibrous wisps of delicate white cirriform ice crystal cloud that show up clearly against the blue sky. Cirrus are generally non-convective except castellanus and floccus genus subtypes which show limited convection. They often form along a high altitude jetstream and at the very leading edge of a frontal or low-pressure disturbance where they may merge into cirrostratus. These high clouds do not produce precipitation.
- Genus cirrocumulus (Cc):
- This is a pure white high-étage stratocumuliform layer of limited convection. It is composed of ice crystals or supercooled water droplets appearing as small unshaded round masses or flakes in groups or lines with ripples like sand on a beach. Cc occasionally form alongside cirrus and may be accompanied or replaced by cirrostratus clouds at the very leading edge of an active weather system.
- Genus cirrostratus (Cs):
- Cirrostratus is a thin non-convective stratiform ice crystal veil that typically gives rise to halos caused by refraction of the sun's rays. The sun and moon are visible in clear outline. Cirrostratus often thickens into altostratus ahead of a warm front or low-pressure area.
Middle stratocumuliform and stratiform
Clouds in the middle-étage are prefixed by alto-, yielding the genus names altocumulus (Ac) and altostratus (As). Strato- is also excluded from altocumulus. These clouds can form as low as 2,000 m (6,500 ft) above surface at any latitude, but may be based as high as 4,000 m (13,000 ft) near the poles, 7,000 m (23,000 ft) at mid latitudes, and 7,600 m (25,000 ft) in the tropics.
- Genus altocumulus (Ac):
- This is a middle-étage stratocumuliform cloud layer of limited convection that is usually appears in the form of irregular patches or more extensive sheets arranges in groups, lines, or waves. High altocumulus may resemble cirrocumulus but is usually thicker and composed of water droplets so that the bases show at least some light-grey shading. Opaque altocumulus associated with a weak frontal or low-pressure disturbance can produce virga, very light intermittent precipitation that evaporates before reaching the ground. If the altocumulus is mixed with moisture-laden altostratus, the precipitation may reach the ground.
- Genus altostratus (As):
- Altostratus is a mid-level opaque or translucent stratiform or non-convective veil of grey/blue-grey cloud that often forms along warm fronts and around low-pressure areas. Altostratus is usually composed of water droplets but may be mixed with ice crystals at higher altitudes. Widespread opaque altostratus can produce light continuous or intermittent precipitation. Precipitation commonly becomes heavier and more widespread if it thickens into nimbostratus.
Low stratocumuliform, stratiform, and cumuliform
Low-étage clouds are found from near surface up to 2,000 m (6,500 ft). Genus types in this étage either have no prefix or carry one that refers to a characteristic other than altitude.
- Genus stratocumulus (Sc):
- This genus type is a stratocumuliform cloud layer of limited convection, usually in the form of irregular patches or more extensive sheets similar to altocumulus but having larger elements with deeper-gray shading. Opaque stratocumulus can produce very light intermittent precipitation. This cloud often forms under a precipitating deck of altostratus or high-based nimbostratus associated with a well-developed warm front, slow-moving cold front, or low-pressure area. This can create the illusion of continuous precipitation of more than very light intensity falling from stratocumulus.
- Genus stratus (St):
- This is a flat or sometimes ragged non-convective stratiform type that sometimes resembles elevated fog. Only very weak precipitation can fall from this cloud (usually drizzle or snow grains), although heavier rain or snow may fall through a stratus layer from a higher precipitating cloud deck. When a low stratiform cloud contacts the ground, it is called fog if the prevailing surface visibility is less than 1 kilometer, although radiation and advection types of fog tend to form in clear air rather from from stratus layers. If the visibility increases to 1 kilometer or higher in any kind of fog, the visible condensation is termed mist.
- Genus cumulus (Cu) – little vertical extent:
- These are small detached fair-weather cumuliform clouds that have nearly horizontal bases and flattened tops, and do not produce rain showers.
Vertical or multi-étage stratiform, cumuliform, and cumulonimbiform (low to middle cloud base)
These clouds have low to middle-étage bases that form anywhere from near surface to about 2,400 m (8,000 ft). Some classifications limit the term vertical to upward-growing free-convective cumuliform and cumulonimbiform genera. Downward-growing nimbostratus can be as thick as most upward-growing vertical cumulus, but its horizontal extent tends to be even greater. This sometimes leads to the exclusion of this genus type from the group of vertical clouds. Classifications that follow this approach usually show nimbostratus either as low-étage to denote its normal base height range, or as middle, based on the altitude range at which it normally forms. Sometimes the terms multi-level or multi-étage are used for all very thick or tall cloud types including nimbostratus to avoid the association of 'vertical' with free-convective cumuliform only. Alternatively, some classifications do not recognize a vertical or multi-étage designation and include all vertical free-convective cumuliform and cumulonimbiform types with the low-étage clouds.
Nimbostratus and some cumulus in this group usually achieve moderate or deep vertical extent, but without towering structure. However, with sufficient airmass instability, upward-growing cumuliform clouds can grow to high towering proportions. Although genus types with vertical extent are often considered a single group, the International Civil Aviation Organization (ICAO) further distinguishes towering vertical clouds as a separate group or sub-group by specifying that these very large cumuliform and cumulonimbiform types must be identified by their standard names or abbreviations in all aviation observations (METARS) and forecasts (TAFS) to warn pilots of possible severe weather and turbulence. When towering vertical types are considered separately, they comprise the aforementioned cumulonimbus genus and one cumulus genus subtype, cumulus congestus (Cu con). This subtype is designated towering cumulus (Tcu) by ICAO. There is no stratiform type in this group because by definition, even very thick stratiform clouds cannot have towering vertical structure, although they may be accompanied by embedded towering cumuliform or cumulonimbiform types.
Moderate or deep vertical
- Genus nimbostratus (Ns):
- This is a diffuse dark-grey non-convective stratiform layer with great horizontal extent and moderate to great vertical development. It lacks towering structure and looks feebly illuminated from the inside. Ns normally forms from middle-étage altostratus and develops at least moderate vertical extent when the base subsides into the low étage during precipitation that can reach moderate to heavy intensity. It commonly achieves deep vertical development when it simultaneously grows upward into the high étage due to large scale frontal or cyclonic lift. The nimbo- prefix refers to its ability to produce continuous rain or snow over a wide area, aspecially ahead of a warm front.
- Genus cumulus (Cu) – moderate vertical extent:
- These cumuliform clouds of free convection have clear-cut medium-grey flat bases and white domed tops in the form of small sproutings and generally do not produce precipitation. They usually form in the low étage except during conditions of very low relative humidity when the clouds bases can rise into the middle altitude range.
These clouds are sometimes classified separately from the other vertical or multi-étage types because of their ability to produce severe turbulance.
- Genus cumulus (Cu) – great vertical extent:
- Increasing airmass instability can cause free-convective cumulus to grow very tall to the extent that the vertical height from base to top is greater than the base-width of the cloud. The cloud base takes on a darker grey coloration and the top commonly resembles a cauliflower. This cloud type can produce moderate to heavy showers.
- Genus cumulonimbus (Cb):
- This genus type is a heavy towering cumulonimbiform mass of free convective cloud with a dark-grey to nearly black base and a vary high top in the form of a mountain or huge tower. Cumulonimbus can produce thunderstorms, local very heavy downpours of rain that may cause flash floods, and a variety of types of lightning including cloud-to-ground that can cause wildfires. Other convective severe weather may or may not be associated with thunderstorms and include heavy snow showers, hail, strong wind shear, downbursts, and tornadoes. Of all these possible cumulonimbus-related events, lightning is the only one of these that requires a thunderstorm to be taking place since it is the lightening that creates the thunder. Cumulonimbus clouds can form in unstable airmass conditions, but tend to be more concentrated and intense when they are associated with unstable cold fronts.
Genus types are comminly divided into subtypes called species that indicate specific structural details. However, because these latter types are not always restricted by étage, some species can be common to several genera that are differentiated mainly by altitude.
Mostly stable stratocumuliform
Good examples of species common to more than one genus are the stratiformis and lenticularis types, each of which is common to mostly stable stratocumuliform genera in the high, middle, and low étages. (cirrocumulus, altocumulus, and stratocumulus, respectively). Stratiformis species normally occur in extensive sheets or in smaller patches where there is only minimal convective activity. Lenticularis species tend to have lens-like shapes tapered at the ends. They are most commonly seen as orographic mountain-wave clouds, but can occur anywhere in the troposphere where there is strong wind shear combined with sufficient airmass stability to maintain a generally flat cloud structure.
Stable cirriform and stratiform
Cirrus clouds have a couple of species that are unique to the wispy structures of this genus and an additional species which is also seen with high-étage stratiform clouds. Uncinus filaments with upturned hooks and spissatus filaments that merge into dense patches are both considered cirriform species. However, the species fibratus can be seen with cirrus and with cirrostratus that is transitional to or from cirrus. Cirrostratus at its most characteristic tends to be mostly of the stratiform species nebulosus, which creates a rather diffuse appearance lacking in structural detail. Altostratus and nimbostratus clouds always have this physical appearance without significant variation or deviation and, therefore, do not need to be subdivided into species. Low-étage stratus is also of the species nebulosus except when broken up into ragged sheets of stratus fractus.
Partly or mostly unstable cirriform and stratocumuliform
With increasing airmass instability, castellanus structures, which resemble the turrets of a castle when viewed from the side, can be found with any stratocumuliform genus. This species is also sometimes seen with convective patches of cirrus, as are the more detached tufted floccus species, which are common to cirrus, cirrocumulus, and altocumulus, but not stratocumulus.
Mostly unstable cumuliform and cumulonimbiform
Except for stratocumulus castellanus, local airmass instability in the low étage tends to produce clouds of the more freely convective cumulus and cumulonimbus genera, whose species are mainly indicators of degrees of vertical development. A cumulus cloud initially forms as a cloudlet of the species fractus or humilis that shows only slight vertical development. If the air becomes more unstable, the cloud tends to grow vertically into the species mediocris, then congestus, the tallest cumulus species. With further instability, the cloud may continue to grow into cumulonimbus calvus (essentially a very tall congestus cloud that produces thunder), then ultimately capillatus when supercooled water droplets at the top turn into ice crystals giving it a cirriform appearance.
Genus and species types are further subdivided into varieties whose names can appear after the species name to provide a fuller description of a cloud. Some cloud varieties are not restricted to a specific étage or physical structure, and can therefore be common to more than one genus or species.
All cloud varieties fall into one of two main groups. One group identifies the opacities of particular low and middle étage cloud structures and comprises the varieties translucidus (thin translucent), perlucidus (thick opaque with translucent breaks), and opacus (thick opaque). These varieties are always identifiable for cloud genera and species with variable opacity. All three are associated with the stratiformis species of altocumulus and stratocumulus. However, only two are seen with altostratus and stratus nebulosus whose uniform structures prevent the formation of a perlucidus variety. Opacity-based varieties are not applied to high-étage clouds because they are always translucent, or in the case of cirrus spissatus, always opaque. Similarly, these varieties are also not associated with moderate and towering vertical clouds because they are always opaque.
A second group describes the occasional arrangements of cloud structures into particular patterns that are discernable by a surface-based observer (cloud fields usually being visible only from a significant altitude above the formations). These varieties are not always present with the genera and species with which they are otherwise associated, but only appear when atmospheric conditions favor their formation. Intortus and vertebratus varieties occur on occasion with cirrus fibratus. They are respectively filaments twisted into irregular shapes, and those that are arranged in fishbone patterns, usually by uneven wind currents that favor the formation of these varieties. The variety radiatus is associated with cloud rows of a particular type that appear to converge at the horizon. It is sometimes seen with the fibratus and uncinus species of cirrus, the stratiformis species of altocumulus and stratocumulus, the mediocris and sometimes humilis species of cumulus, and with the genus altostratus.
Another variety, duplicatus (closely spaced layers of the same type, one above the other), is sometimes found with cirrus of both the fibratus and uncinus species, and with altocumulus and stratocumulus of the species stratiformis and lenticularis. The variety undulatus (having a wavy undulating base) can occur with any clouds of the species stratiformis or lenticularis, and with altostratus. It is only rarely observed with stratus nebulosus. The variety lacunosus is caused by localized downdrafts that create circular holes in the form of a honeycomb or net. It is occasionally seen with cirrocumulus and altocumulus of the species stratiformis, castellanus, and floccus, and with stratocumulus of the species stratiformis and castellanus.
It is possible for some species to show combined varieties at one time, especially if one variety is opacity-based and the other is pattern-based. An example of this would be an opaque layer of altocumulus stratiformis arranged in seemingly converging rows. The full technical name of a cloud in this configuration would be altocumulus stratiformis opacus radiatus, which would identify respectively its genus, species, and two combined varieties.
Accessory clouds and supplementary features
Supplementary features are not further subdivisions of cloud types below the species and variety level. Rather, they are either hydrometeors or special cloud formations with their own Latin names that form in association with certain cloud genera, species, and varieties. Supplemenary features, whether in the form of clouds or precipitation, are directly attached to the main genus-cloud. Accessory clouds, by contrast, are generally detached from the main cloud.
Precipitation-based supplementary features
One group of supplementary features are not actual cloud formations but rather precipitation that falls when water droplets that make up visible clouds have grown too heavy to remain aloft. Virga is a feature seen with clouds producing precipitation that evaporates before reaching the ground, these being of the genera cirrocumulus, altocumulus, altostratus, nimbostratus, stratocumulus, cumulus, and cumulonimbus.
When the precipitation reaches the ground without completely evaporating, it is designated as the feature praecipitatio. This normally occurs with altostratus opacus, which can produce widespread but usually light precipitation, and with thicker clouds that show significant vertical development. Of the latter, upward-growing cumulus mediocris produces only isolated light showers, while downward growing nimbostratus is capable of heavier, more extensive precipitation. Towering vertical clouds have the greatest ability to produce intense precipitation events, but these tend to be localized unless organized along fast-moving cold fronts. Showers of moderate to heavy intensity can fall from cumulus congestus clouds. Cumulonimbus, the largest of all cloud genera, has the capacity to produce very heavy showers. Low stratus clouds usually produce only light precipitation, but this always occurs as the feature praecipitatio due to the fact this cloud genus lies too close to the ground to allow for the formation of virga.
Cloud-based supplementary features
Incus is the most type-specific supplementary feature, seen only with cumulonimbus of the species capillatus. A cumulonimbus incus cloud top is one that has spread out into a clear anvil shape as a result of rising air currents hitting the stability layer at the tropopause where the air no longer continues to get colder with increasing altitude.
The mamma feature forms on the bases of clouds as downward-facing bubble-like protuberances caused by localized downdrafts within the cloud. It is also sometimes called mammatus, an earlier version of the term used before a standardization of Latin nomenclature brought about by the World Meterorological Organization during the 20th century. The best-known is cumulonimbus with mammatus, but the mamma feature is also seen occasionally with cirrus, cirrocumulus, altocumulus, altostratus, and stratocumulus.
A tuba feature is a cloud column that may hang from the bottom of a cumulus or cumulonimbus. A newly formed or poorly organized column might be comparatively benign, but can quickly intensify into a funnel cloud or tornado.
An arcus feature is a roll cloud with ragged edges attached to the lower front part of cumulus congestus or cumulonimbus that forms along the leading edge of a squall line or thunderstorm outflow. A large arcus formation can have the appearance of a dark menacing arch.
There are some arcus-like clouds that form as a consequence of interactions with specific geographical features rather than with a parent cloud. Perhaps the strangest geographically specific cloud of this type is the Morning Glory, a rolling cylindrical cloud that appears unpredictably over the Gulf of Carpentaria in Northern Australia. Associated with a powerful "ripple" in the atmosphere, the cloud may be "surfed" in glider aircraft. It has been officially suggested that roll clouds of this type that are not attached to a parent cloud be reclassified as a new species of stratocumulus, possibly with the Latin name volutus.
Supplementary cloud formations detachewd from the main cloud are known as accessory clouds. The heavier precipitating clouds, nimbostratus, towering cumulus (cumulus congestus), and cumulonimbus, typically see the formation in precipitation of the pannus feature, low ragged clouds of the genera and species cumulus fractus or stratus fractus.
After the pannus types, the remaining accessory clouds comprise formations that are associated mainly with upward-growing cumuliform and cumulonimbiform clouds of free convection. Pileus is a cap cloud that can form over a cumulonimbus or large cumulus cloud, whereas a velum feature is a thin horizontal sheet that sometimes forms like an apron around the middle or in front of the parent cloud.
Under conditions of strong atmospheric wind-shear and instability, wave-like undulatus formations may break into regularly spaced crests. This variant has no separate WMO Latin designation, but is sometimes known informally as Kelvin-Helmholtz wave cloud. This phenominum has also been observed in cloud formations over other planets and even in the sun's atmosphere. It has been formally suggested that this wave cloud be classified as supplementary feature, possibly with the Latin name fluctus. Another wave-like cloud feature that is distinct from the variety undulatus has been dubbed with the Latin name asperatus. It has been recommended for formal classification as a supplementary feature using it's suggested Latin name.
A circular fall-streak hole occasionally forms in a thin layer of supercooled altocumulus or cirrocumulus. Fallstreaks consisting of virga or wisps of cirrus are usually seen beneath the hole as ice crystals fall out to a lower altitude. This type of hole is usually larger than typical lacunosus holes, and a formal recommendation has been made to classify it as a supplementary feature, possibly with the Latin name cavus.
Clouds initially form in clear air or become clouds when fog rises above surface level. The genus of a newly formed cloud is determined mainly by air mass characteristics such as stability and moisture content. If these characteristics change over time, the genus tends to change accordingly. When this happens, the original genus is called a mother cloud. If the mother cloud retains much of its original form after the appearance of the new genus, it is termed a genitus cloud. One example of this is stratocumulus cumulogenitus, a stratocumulus cloud formed by the partial spreading of a cumulus type when there is a loss of convective lift. If the mother cloud undergoes a complete change in genus, it is considered to be a mutatus cloud.
It has been officially recommended that the genitus category be expanded to include certain types that do not originate from pre-existing clouds or as the result of any natural atmospheric processes. Among vertically developed clouds, these may include flammagenitus for cumulus congestus or cumulonimbus that are formed by large scale fires or volcanic eruptions. Smaller low-étage "pyrocumulus" or "fumulus" clouds formed by contained industrial activity could be classified as cumulus homogenitus. Contrails formed from the exhaust of aircraft flying in the high étage can persist and spread into formations resembling any of the high cloud genus-types. These variants have no special WMO designations, but are sometimes given the faux-Latin name Aviaticus. Persistent contrails have been identified as candidates for possible inclusion in the genitus category as cirrus, cirrostratus, or cirrocumulus homogenitus
Stratocumulus clouds can be organized into "fields" that take on certain specially classified shapes and characteristics. In general, these fields are more discernable from high altitudes than from ground level. They can often be found in the following forms:
- Actinoform, which resembles a leaf or a spoked wheel.
- Closed cell, which is cloudy in the center and clear on the edges, similar to a filled honeycomb.
- Open cell, which resembles an empty honeycomb, with clouds around the edges and clear, open space in the middle.
Reporting and mapping cloud types
The international synoptic code (or SYNOP) is used to report weather conditions at regular intervals by professionally trained staff at major weather stations. It provides for reporting of cloud types in any of the three basic étages for tropospheric clouds, but makes no special provision for vertical or multi-level clouds that can occupy more than one étage at a particular time. Consequently, cloud genera with significant vertical development are coded as low when they form in the low étage of the troposphere and achieve vertical extent by growing upward into the middle or high étage, as is the case with cumulus and cumulonimbus. Conversely, nimbostratus is coded as middle because it usually initially forms in the middle étage of the troposphere and becomes vertically developed by growing downward into the low étage, and ofter upward in to the high étage as well. Although the SYNOP code has no separate formal group classification for vertical or multi-level clouds, the observer procedure for selecting numerical codes is designed to give high reporting priority to those genera or species that show significant vertical development. Cloud codes are translated into symbols and plotted on weather maps along with other meteorological data that make up a complete synoptic message.
Formation: how the air becomes saturated
Cooling air to its dew point
This process occurs when one or more of three possible lifting agents, cyclonic/frontal, convective, and oragraphic, causes air containing invisible water vapor to rise and cool to its dew point, the temperature at which the air becomes saturated. The main mechanism behind this process is adiabatic cooling. Atmospheric pressure decreases with altitude, so the rising air expands in a process that expends energy and causes the air to cool, which reduces its capacity to hold water vapor. If the air is cooled to its dew point and becomes saturated, it normally sheds vapor it can no longer retain which condenses into cloud.
The altitude at which this begins to happen is called the lifted condensation level (LCL), which roughly determines the height of the cloud base. Water vapor in saturated air is normally attracted to condensation nuclei such as salt particles that are small enough to be held aloft by normal circulation of the air. If the condensation process occurs below the freezing level in the troposphere, the nuclei help transform the vapor into very small water droplets. Clouds that form just above the freezing level are composed mostly of supercooled liquid droplets, while those that condense out at higher altitudes where the air is much colder generally take the form of ice crystals. An absence of sufficient condensation particles at and above the condensation level causes the rising air to become supersaturated and the formation of cloud tends to be inhibited.
Frontal and cyclonic lift
Frontal and cyclonic lift occur in their purist manifestations when stable air, which has been subjected to little or no surface heating, is forced aloft at weather fronts and around centers of low pressure producing mostly stratiform cloud types. Visible cloud droplets form when the air is lifted beyond the condensation level where water vapor condenses on so-called nuclei; (small particles) that grow to a radius of typically 0.002 mm (0.00008 in). In a cloud the droplets collide to form larger droplets. These larger droplets remain aloft as long as the drag force of the air dominates over the gravitational force for small particles.
Another agent is the buoyant convective upward motion caused by significant daytime solar heating at surface level, or by relatively high absolute humidity. Incoming short-wave radiation generated by the sun is re-emitted as long-wave radiation when it reaches Earth's surface. This process warms the air closest to ground and increases air mass instability by creating a steeper temperature gradient from warm or hot at surface level to cold aloft. This causes it to rise and cool until temperature equilibrium is achieved with the surrounding air aloft. Free convective clouds generally form at the altitude of the convective condensation level (CCL). Moderate instability allows for the formation of cumuliform clouds of moderate size that can produce light showers if the airmass is sufficiently moist. Typical convection upcurrents may allow the droplets to grow to a radius of about 0.015 mm (15 microns or 0.0006 in) before precipitating as showers. The equivalent diameter of these droplets is about 0.03 mm. (30 microns or 0.0012 in). If air near the surface becomes extremely warm and unstable, its upward motion can become quite explosive resulting in towering cumulonimbiform clouds that can cause severe weather.
Convective lift can occur in an unstable air mass well away from any fronts. However very warm unstable air can also be present around fronts and low-pressure centers, often producing cumuliform and cumulonimbiform clouds in heavier and more active concentrations because of the combined frontal and convective lifting agents. As with non-frontal convective lift, increasing instability promotes upward vertical cloud growth and raises the potential for severe weather. On comparatively rare occasions, convective lift can be powerful enough to penetrate the tropopause and push the cloud top into the stratosphere.
A third source of lift is wind circulation forcing air over a physical barrier such as a mountain (orographic lift). If the air is generally stable, nothing more than lenticular cap clouds will form. However, if the air becomes sufficiently moist and unstable, orographic showers or thunderstorms may appear.
Along with adiabatic cooling that requires a lifting agent, there are three other main mechanisms for lowering the temperature of the air to its dew point, all of which occur near surface level and do not require any lifting of the air. Conductive, radiational, and evaporative cooling can cause condensation at surface level resulting in the formation of fog. Conductive cooling takes place when air from a relatively mild source area comes into contact with a colder surface, as when mild marine air moves across a colder land area. Radiational cooling occurs due to the emission of infrared radiation, either by the air or by the surface underneath. This type of cooling is common during the night when the sky is clear. Evaporative cooling happens when moisture is added to the air through evaporation, which forces the air temperature to cool to its wet-bulb temperature, or sometimes to the point of saturation.
Adding moisture to the air
There are five main ways water vapor can be added to the air. Increased vapor content can result from wind convergence over water or moist ground into areas of upward motion. Precipitation or virga falling from above also enhances moisture content. Daytime heating causes water to evaporate from the surface of oceans, water bodies or wet land. Transpiration from plants is another typical source of water vapor. Lastly, cool or dry air moving over warmer water will become more humid. As with daytime heating, the addition of moisture to the air increases its heat content and instability and helps set into motion those processes that lead to the formation of cloud or fog.
Distribution: variable global prevalence and association with organized weather systems
Convergence along low-pressure zones
Although the local distribution of clouds can be significantly influenced by topography, the global prevalence of cloud cover tends to vary more by latitude. It is most prevalent globally in and along low pressure zones of surface atmospheric convergence which encircle the Earth close to the equator and near the 50th parallels of latitude in the northern and southern hemispheres. Convergence is a process that involves the horizontal inflow and accumulation of air at a given location, as well as the rate at which this happens. Near the equator, increased cloudiness is due to the presence of the low-pressure Intertropical Convergence Zone (ITCZ) where very warm and unstable air promotes mostly cumuliform and cumulonimbiform clouds. Clouds of virtually any type can form along the mid-latitude convergence zones depending on the stability and moisture content of the air. These extratropical convergence zones are occupied by the polar fronts where air masses of polar origin meet and clash with those of tropical or subtropical origin. This leads to the formation of weather-making extratropical cyclones composed of cloud systems that may be stable or unstable to varying degrees according to the stability characteristics of the various airmasses that are in conflict.
Warm fronts associated with extratropical cyclones tend to generate mostly cirriform and stratiform clouds over a wide area unless the approaching warm airmass is unstable, in which case cumulus congestus or cumulonimbus clouds will usually be embedded in the main precipitating cloud layer. Cold fronts are usually faster moving and generate a narrower line of clouds which are mostly stratocumuliform, cumuliform, or cumulonimbiform depending on the stability of the warm air mass just ahead of the front.
Divergence along high pressure zones
Divergence is the opposite of convergence. In the Earth's atmosphere, it involves the horizontal outflow of air from the upper part of a rising column of air, or from the lower part of a subsiding column often associated with an area or ridge of high pressure. Cloudiness tends to be least prevalent near the poles and in the subtropics close to the 20th parallels, north and south. The latter are sometimes referred to as the horse latitudes. The presence of a large-scale high-pressure subtropical ridge on each side of the equator reduces cloudiness at these low latitudes. Similar patterns also occur at higher latitudes in both hemispheres. After the passage of a cold front or other organized weather disturbance, the sky usually clears as high pressure builds in behind the system, although significant amounts of cumulus or stratocumulus, often in the form of long bands called cloud streets may persist if the air mass behind the front remains humid. Small and unchanging amounts of cumulus or cirrus clouds in an otherwise clear sky are usually indications of continuing fair weather as long as the barometric pressure remains comparatively high.
Determination of properties
Data sets regarding cloud properties are gathered using satellites, such as MODIS, POLDER, CALIPSO or ATSR The instruments measure the radiances of the clouds, from which the relevant parameters can be retrieved. This is usually done by using inverse theory.
The method of detection is based on the fact that the clouds tend to appear brighter and colder than the land surface. Because of this, difficulties rise in detecting clouds above bright (highly reflective) surfaces, such as oceans and ice.
The value of a certain parameter is more reliable the more satellites are measuring the said parameter. This is due to the fact that the range of errors and neglected details varies from instrument to instrument. Thus, if the analysed parameter has similar values for different instruments, it is accepted that the true value lies in the range given by the corresponding data sets.
The Global Energy and Water Cycle Experiment uses the following quantities in order to compare data quality from different satellites in order to establish a reliable quantification of the properties of the clouds:
- the Cloud Amount with values between 0 and 1
- the cloud temperature at top ranging from 150 to 340 K
- the cloud pressure at top 1013 - 100 hPa
- the cloud height, measured above sea level, ranging from 0 to 20 km
- the cloud IR emissivity, with values between 0 and 1, with a global average around 0.7.
- the effective cloud amount is the cloud amount weighted by the cloud IR emissivity, with a global average of 0.5
- the cloud (visible) optical depth varies within a range of 4 and 10.
- the cloud water path for the liquid and solid (ice) phases of the cloud particles
- the cloud effective particle size for both liquid and ice, ranging from 0 to 200 μm
Another vital property is the icing characteristic of various cloud genus types at various altitudes, which can have great impact on the safety of flying. The methodologies used to determine these characteristics include using CloudSat data for the analysis and retrieval of icing conditions, the location of clouds using cloud geometric and reflectivity data, the identification of cloud types using cloud classification data, and finding vertical temperature distribution along the CloudSat track (GFS)
The range of temperatures that can give rise to icing conditions is defined according to cloud types: Low stratocumulus and stratus can cause icing at a temperature range of 0 to -10 degrees C. For middle etage altocumulus and altostratus, the range is 0 to -20 degrees C. Vertical or multi-etage cumulus, cumulonimbus, and nimbostatus, create icing at a range of 0 to -25 degrees C. High etage cirrus, cirrocumulus, and cirrostratus generally cause no icing because they are made mostly of ice crystals colder that -25 degrees C.
Polar stratospheric clouds show little variation in structure and are limited to a single very high range of altitude of about 15,000–25,000 m (49,200–82,000 ft), so they are not classified into étages, genus types, species, or varieties in the manner of tropospheric clouds. Instead, the classification is alpha-numeric and is based on chemical makeup rather than variations in physical appearance.
Types and subtypes
Nacreous and non-nacreous (very high cirriform)
- Type 1 (Non-nacreous): This type contains frozen or supercooled nitric acid and water droplets and lacks any special coloration. It is dividable into subtype 1A which is mostly made up of water ice crystals and frozen nitric acid, 1B which consists of supercooled droplets of nitric and sulfuric acid, and subtype 1C which comprises small particles of nitric acid. Nacreous type 2 is sometimes associated or embedded.
- Type 2 (Nacreous): Nacreous polar stratospheric cloud consists of ice crystals only and generally shows mother-of-pearl colors.
Formation and distribution
Polar stratospheric clouds form in the lowest part of the statosphere during the winter, at the altitude and during the season that produces the coldest temperatures and therefore the best chances of triggering condensation caused by adiabatic cooling. They are typically very thin with an undulating cirriform appearance. Moisture is scarce in the stratosphere, so nacreous and non-nacreous cloud at this altitude range is rare and is usually restricted to polar regions in the winter where the air is coldest.
Polar mesospheric clouds form at a single extreme altitude range of about 80 to 85 km (50 to 53 mi) and are consequently not classified into more than one étage. They are given the Latin name Noctilucent because of their illumination well after sunset and before sunrise. An alpha-numeric classification is used to identify variations in physical appearance.
Types and subtypes
Noctilucent (extremely high cirriform)
- Type 1: The first type is characterized by very tenuous filaments resembling cirrus fibratus.
- Type 2: This type comprises bands in the form of long streaks, often in groups or interwoven at small angles, similar to cirrus intortus. It is dividable into two subtypes; 2A where the streaks have diffuse, blurred edges, and 2B where they have sharply defined edges.
- Type 3: Billows in the form of short streaks can be seen that are clearly spaced and roughly parallel. Subtype 3A has short, straight, narrow streaks while 3B has wave-like streaks similar to cirrus undulatus.
- Type 4: This shows whirls in the form of partial or rarely complete rings with dark centers. With subtype 4A, the whirls are of small angular radius and have a similar appearance to surface water ripples. 4B is characterized by simple curves of medium angular radius with one or more bands. Subtype 4C has whirls with large-scale ring structure.
Formation and distribution
Polar mesospheric clouds are the highest in the atmosphere and form near the top of the mesosphere at about ten times the altitude of tropospheric high clouds. From ground level, they can occasionally be seen illuminated by the sun during deep twilight. Ongoing research indicates that convective lift in the mesophere is strong enough during the polar summer to cause adiabatic cooling of small amount of water vapour to the point of saturation. This tends to produce the coldest temperatures in the entire atmosphere just below the mesopause. These conditions result in the best environment for the formation of polar mesospheric clouds. There is also evidence that smoke particles from burnt-up meteors provide much of the condensation nuclei required for the formation of noctilucent cloud.
Distribution in the mesosphere is similar to the stratosphere except at much higher altitudes. Because of the need for maximum cooling of the water vapor to produce noctilucent clouds, their distribution tends to be restricted to polar regions of Earth. A major seasonal difference is that convective lift from below the mesosphere pushes very scarce water vapor to higher colder altitudes required for cloud formation during the respective summer seasons in the northern and southern hemispheres. Sightings are rare more than 45 degrees south of the north pole or north of the south pole.
Clouds throughout the homosphere
Cohesion and dissolution
There are forces throughout the homosphere (which includes the troposphere, stratosphere, and mesophere) that can impact the structural integrity of a cloud. However, as long as the air remains saturated, the natural force of cohesion that hold the molecules of a substance together acts to keep the cloud from breaking up. Dissolution of the cloud can occur when the process of adiabatic cooling ceases and upward lift of the air is replaced by subsidence. This leads to at least some degree of adiabatic warming of the air which can result in the cloud droplets or crystals turning back into invisible water vapor. Stronger forces such as wind shear and downdrafts can impact a cloud, but these are largely confined to the troposphere where nearly all the Earth's weather takes place.
Luminance and reflectivity
The luminance or brightness of a cloud is determined by how light is reflected, scattered, and transmitted by the cloud's particles. Its brightness may also be affected by the presence of haze or photometeors such as halos and rainbows. In the troposphere, dense, deep clouds exhibit a high reflectance (70% to 95%) throughout the visible spectrum. Tiny particles of water are densely packed and sunlight cannot penetrate far into the cloud before it is reflected out, giving a cloud its characteristic white color, especially when viewed from the top. Cloud droplets tend to scatter light efficiently, so that the intensity of the solar radiation decreases with depth into the gases. As a result, the cloud base can vary from a very light to very-dark-grey depending on the cloud's thickness and how much light is being reflected or transmitted back to the observer. High thin tropospheric clouds reflect less light because of the comparatively low concentration of constituent ice crystals or supercooled water droplets which results in a slightly off-white appearance. However, a thick dense ice-crystal cloud appears brilliant white with pronounced grey shading because of its greater reflectivity.
As a tropospheric cloud matures, the dense water droplets may combine to produce larger droplets. If the droplets become too large and heavy to be kept aloft by the air circulation, they will fall from the cloud as rain. By this process of accumulation, the space between droplets becomes increasingly larger, permitting light to penetrate farther into the cloud. If the cloud is sufficiently large and the droplets within are spaced far enough apart, a percentage of the light that enters the cloud is not reflected back out but is absorbed giving the cloud a darker look. A simple example of this is one's being able to see farther in heavy rain than in heavy fog. This process of reflection/absorption is what causes the range of cloud color from white to black.
Striking cloud colorations can be seen at many altitudes in the homosphere. The color of a cloud is usually the same as the incident light.
During daytime when the sun is relatively high in the sky, clouds generally appear bright white on top with varying shades of grey underneath. Thin clouds may look white or appear to have acquired the color of their environment or background. Other colors occur naturally in tropospheric clouds that can tell much about what is going on inside the cloud. Bluish-grey is the result of light scattering within the cloud. In the visible spectrum, blue and green are at the short end of light's visible wavelengths, whereas red and yellow are at the long end. The short rays are more easily scattered by water droplets, and the long rays are more likely to be absorbed. The bluish color is evidence that such scattering is being produced by rain-size droplets in the cloud.
A cumulonimbus cloud that appears to have a greenish/bluish tint is a sign that it contains extremely high amounts of water; hail or rain which scatter light in a way that gives the cloud a blue color. A green colorization occurs mostly late in the day when the sun is comparatively low in the sky and the incident sunlight has a reddish tinge that appears green when illuminating a very tall bluish cloud. Supercell type storms are more likely to be characterized by this but any storm can appear this way. Coloration such as this does not directly indicate that it is a severe thunderstorm, it only confirms its potential. Since a green/blue tint signifies copious amounts of water, a strong updraft to support it, high winds from the storm raining out, and wet hail; all elements that improve the chance for it to become severe, can all be inferred from this. In addition, the stronger the updraft is, the more likely the storm is to undergo tornadogenesis and to produce large hail and high winds.
Yellowish clouds may occur in the late spring through early fall months during forest fire season. The yellow color is due to the presence of pollutants in the smoke. Yellowish clouds caused by the presence of nitrogen dioxide are sometimes seen in urban areas with high air pollution levels.
Within the troposphere, red, orange, and pink clouds occur almost entirely at sunrise/sunset and are the result of the scattering of sunlight by the atmosphere. When the angle between the sun and the horizon is less than 10 percent, as it is just after sunrise or just prior to sunset, sunlight becomes too red due to refraction for any colors other than those with a reddish hue to be seen. The clouds do not become that color; they are reflecting long and unscattered rays of sunlight, which are predominant at those hours. The effect is much like if one were to shine a red spotlight on a white sheet. In combination with large, mature thunderheads, this can produce blood-red clouds. Clouds look darker in the near-infrared because water absorbs solar radiation at those wavelengths. When the sun is just below the horizon, low-etage clouds are gray, middle clouds appear rose-colored, and high-etage clouds are white or off-white.
Clouds at night are black or dark grey in a moonless sky, or whitish when illuminated by the moon. They may also reflect the colors of large fires, city lights, or auroras that might be present.
In high latitude regions of the stratosphere, nacreous clouds occasionally found there during the polar winter tend to display quite striking displays of mother-of-pearl colorations. This is due to the refraction and diffusion of the sun's rays through thin clouds with supercooled droplets that often contain compounds other than water. At still higher altitudes up in the mesospere, noctilucent clouds made of ice crystals are sometimes seen in polar regions in the summer. They typically have a bluish or silvery white coloration that can resemble brightly illuminated cirrus. Noctilucent clouds may occasionally take on more of a red or orange hue.
Effects on climate and the atmosphere
The role of tropospheric clouds in regulating weather and climate remains a leading source of uncertainty in projections of global warming. This uncertainty arises because of the delicate balance of processes related to clouds, spanning scales from millimeters to planetary. Hence, interactions between the large-scale (synoptic meteorology) and clouds becomes difficult to represent in global models. The complexity and diversity of clouds, as outlined above, adds to the problem. On the one hand, white-colored cloud tops promote cooling of Earth's surface by reflecting short-wave radiation from the sun. Most of the sunlight that reaches the ground is absorbed, warming the surface, which emits radiation upward at longer, infrared, wavelengths. At these wavelengths, however, water in the clouds acts as an efficient absorber. The water reacts by radiating, also in the infrared, both upward and downward, and the downward long-wave radiation results in some warming at the surface. This is analogous to the greenhouse effect of greenhouse gases and water vapor.
High-étage tropospheric genus-types, cirrus, cirrocumulus, and cirrostratus, particularly show this duality with both short-wave albedo cooling and long-wave greenhouse warming effects. On the whole though, ice-crystal clouds in the upper troposphere tend to favor net warming. However, the cooling effect is dominant with low-étage stratocumuliform and stratiform clouds made of very small water droplets that have an average radius of about 0.002 mm (0.00008 in)., especially when they form in extensive sheets that block out more of the sun. These include middle-étage layers of altocumulus and altostratus as well as low stratocumulus, and stratus. Small-droplet aerosols are not good at absorbing long-wave radiation reflected back from Earth, so there is a net cooling with almost no long-wave effect. This effect is particularly pronounced with low-étage clouds that form over water. Low and vertical heaps of cumulus, towering cumulus, and cumulonimbus are made of larger water droplets ranging in radius from 0.005 to about 0.015 mm. Nimbostratus cloud droplets can also be quite large, up to 0.015mm radius. These larger droplets associated with vertically developed clouds are better able to trap the long-wave radiation thus migitating the cooling effect to some degree. However, these large often precipitating clouds are variable or unpredictable in their overall effect because of variations in their concentration, distribution, and vertical extent. Measurements taken by NASA indicate that on the whole, the effects of low and middle étage clouds that tend to promote cooling are outweighing the warming effects of high layers and the variable outcomes associated with multi-level or vertically developed clouds.
As difficult as it is to evaluate the effects of current cloud cover characteristics on climate change, it is even more problematic to predict the outcome of this change with respect to future cloud patterns and events. As a consequence, much research has focused on the response of low and vertical clouds to a changing climate. Leading global models can produce quite different results, however, with some showing increasing low-étage clouds and others showing decreases.
In the stratosphere, Type I non-nacreous clouds are known to have harmful effects over the polar regions of Earth. They become catalysts which convert relatively benign man-made chlorine into active free radicals like chlorine monoxide which are destructive of the stratospheric ozone layer.
Polar mesospheric clouds are not common or widespread enough to have a significant effect on climate. However, an increasing frequency of occurrence of noctilucent clouds since the 19th century may be the result of climate change.
New research indicates a global brightening trend. The details are not fully understood, but much of the global dimming (and subsequent reversal) is thought to be a consequence of changes in aerosol loading in the atmosphere, especially sulfur-based aerosol associated with biomass burning and urban pollution. Changes in aerosol burden can have indirect effects on clouds by changing the droplet size distribution or the lifetime and precipitation characteristics of clouds.
Cloud cover has been seen on most other planets in the solar system. Venus's thick clouds are composed of sulfur dioxide and appear to be almost entirely stratiform. They are arranged in three main layers at altitudes of 45 to 65 km that obscure the planet's surface and can produce virga. No embedded cumuliform types have been identified, but broken stratocumuliform wave formations are sometimes seen in the top layer that reveal more continuous layer clouds underneath. On Mars, cirrus, cirrocumulus and stratocumulus composed of water-ice have been detected mostly near the poles. Water-ice fogs have also been detected on this planet.
Both Jupiter and Saturn have an outer cirriform cloud deck composed of ammonia, an intermediate stratiform haze-cloud layer made of ammonium hydrosulfide, and an inner deck of cumulus water clouds. Embedded cumulonimbus are known to exist near the Great Red Spot on Jupiter. The same category-types can be found covering Uranus, and Neptune, but are all composed of Methane. Saturn's moon Titan has cirrus clouds believed to be composed largely of methane. The Cassini–Huygens Saturn mission uncovered evidence of a fluid cycle on Titan, including lakes near the poles and fluvial channels on the surface of the moon.
In October 2013, the detection of high altitude optically thick clouds in the atmosphere of Kepler-7b was announced, and, in December 2013, also in the atmospheres of GJ 436 b and GJ 1214 b.
- "Weather Terms". National Weather Service. Retrieved 21 June 2013.
- Harper, Douglas (2012). "Cloud". Online Etymology Dictionary. Retrieved 2014-11-13.
- "Cloud". The Free Dictionary. Farlex. Retrieved 2014-11-13.
- Garry Toth and Don Hillger, ed. (2007). "Ancient and pre-Renaissance Contributors to Meteorology". Colorado State University. Retrieved 2014-11-30.
- World Meteorological Organization, ed. (1975). International Cloud Atlas, preface to the 1939 edition. I. pp. IX–XIII. ISBN 92-63-10407-7. Retrieved 6 December 2014.
- John D. Cox (2002). Storm Watchers. John Wiley & Sons, Inc. pp. 13–17. ISBN 0471444863.
- Met Office (U.K.) (2013). "Fact sheet No. 1 - Clouds". Met Office (U.K.). Retrieved 21 November 2013.
- "Cumulus". The Free Dictionary. Farlex. Retrieved 2014-12-13.
- Colorado State University Dept. of Atmospheric Science, ed. (2014). "Cloud Art: Cloud Classification". Retrieved 13 December 2014.
- Henry Glassford Bell, ed. (1827). Constable's miscellany of original and selected publications XII. p. 320.
- Mark J. Laufersweiler and Hampton N. Shirer (March 1995). Theoretical model of multi-regime convection in a stratocumulus-topped boundary layer. 73, issue=4. pp. 373–409. Retrieved 26 November 2014.
- E.C. Barrett and C.K. Grant (1976). "The identification of cloud types in LANDSAT MSS images". NASA. Retrieved 22 August 2012.
- World Meteorological Organization, ed. (1975). Noctilucent, International Cloud Atlas I. p. 66. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1975). Nacreous, International Cloud Atlas I. p. 65. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- NASA, ed. (2014). "TIROS". Retrieved 5 December 2014.
- JetStream, ed. (8 October 2008). "Cloud Classifications". National Weather Service. Retrieved 23 November 2014.
- JetStream (5 January 2010). "Cloud Classifications". National Weather Service. Retrieved 31 January 2011.
- World Meteorological Organization, ed. (1975). Étages, International Cloud Atlas I. pp. 15–16. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- Clouds Online (2012). "Cloud Atlas". Retrieved 1 February 2012.
- Jim Koermer (2011). "Plymouth State Meteorology Program Cloud Boutique". Plymouth State University. Retrieved 31 January 2011.
- World Meteorological Organization, ed. (1975). Cirrus, International Cloud Atlas I. pp. 25–27. ISBN 92-63-10407-7. Retrieved 28 November 2014.
- "Cumulus clouds". Weather (USA Today). 16 October 2005. Retrieved 16 October 2012.
- Stommel 1947, p. 91
- Mossop & Hallett 1974, pp. 632–634
- Elementary Meteorology Online (2013). "Humidity, Saturation, and Stability". vsc.edu. Retrieved 18 November 2013.
- NASA, ed. (2015). "Stratiform or Stratus Clouds". Retrieved 23 January 2015.
- JetStream (2008). How to read weather maps. National Weather Service. Retrieved on 2007-05-16.
- Vincent J. Schaefer (October 1952). Cloud Forms of the Jet Stream. General Electric Research Laboratory. Retrieved 27 November 2014.
- World Meteorological Organization, ed. (1975). Cirrostratus, International Cloud Atlas I. pp. 29–31. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1995). "WMO cloud classifications". Retrieved 1 February 2012.
- World Meteorological Organization, ed. (1975). Cirrocumulus, International Cloud Atlas I. pp. 27–29. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- Miyazaki et al. 2001, p. 364
- World Meteorological Organization, ed. (1975). Altostratus, International Cloud Atlas I. pp. 35–37. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1975). Altocumulus, International Cloud Atlas I. pp. 31–35. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1975). Nimbostratus, International Cloud Atlas I. pp. 37–39. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1975). Stratocumulus, International Cloud Atlas I. pp. 39–42. ISBN 92-63-10407-7. Retrieved 28 November 2014.
- World Meteorological Organization, ed. (1975). Stratus, International Cloud Atlas I. pp. 43–45. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- World Meteorological Organization, ed. (1975). Cumulus, International Cloud Atlas I. pp. 45–48. ISBN 92-63-10407-7. Retrieved 28 November 2014.
- "cloud: Classification of Clouds". Infoplease.com.
- Becca Hatheway (2009). "Cloud Types". Windows to the Universe, US National Earth Science Teachers Association (NESTA). Retrieved 15 September 2011.
- UXL, ed. (2002). "clouds. UXL Encyclopedia of Science". Retrieved 23 November 2014.
- Paul de Valk, Rudolf van Westhrenen, and Cintia Carbajal Henken (2010). "Automated CB and TCU detection using radar and satellite data: from research to application". Retrieved 15 September 2011.
- Robert A. Houze (1994). Cloud Dynamics. Retrieved 21 November 2013.
- American Meterological Society (2012). "Glossary of Meteorology". Retrieved 9 January 2014.
- Steven A. Ackerman (2011). Meteorology:Precipitating Clouds. Published by Jones & Bartlett. Retrieved 22 October 2013.
- World Meteorological Organization, ed. (1975). Cumulonimbus, International Cloud Atlas I. pp. 48–50. ISBN 92-63-10407-7. Retrieved 28 November 2014.
- Scott, A (2000). "The Pre-Quaternary history of fire". Palaeogeography Palaeoclimatology Palaeoecology 164 (1–4): 281. doi:10.1016/S0031-0182(00)00192-9.
- National Center for Atmospheric Research (2008). "Hail". University Corporation for Atmospheric Research. Retrieved 18 July 2009.
- Ted Fujita (1985). "The Downburst, microburst and macroburst". SMRP Research Paper 210, 122 pp.
- Nilton O. Renno (August 2008). "A thermodynamically general theory for convective vortices" (PDF). Tellus A 60 (4): 688–99. Bibcode:2008TellA..60..688R. doi:10.1111/j.1600-0870.2008.00331.x.
- Lee M. Grenci and Jon M. Nese (2001). A World of Weather: Fundamentals of Meteorology: A Text / Laboratory Manual (3 ed.). Kendall/Hunt Publishing Company. pp. 207–212. ISBN 978-0-7872-7716-1. OCLC 51160155.
- World Meteorological Organization, ed. (1975). Species, International Cloud Atlas I. pp. 17–20. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- Morris (2008). "Clouds – Species and Varieties". University of Minnesota. Retrieved 4 February 2012.
- World Meteorological Organization, ed. (1975). Varieties, International Cloud Atlas. pp. 20–22. Retrieved 26 August 2014.
- Aerographer/Meteorology (2012). "Cloud Variety". meteorologytraining.tpub.com. Retrieved 2 July 2012.
- "Sculpting La Silla’s Skies". www.eso.org. ESO. Retrieved 23 August 2014.
- Cumulus-skynews (2013). "Clouds: Their curious natures". Retrieved 26 August 2014.
- Pretor-Pinney 2007, p. 20
- World Meteorological Organization, ed. (1975). Features, International Cloud Atlas I. pp. 22–24. ISBN 92-63-10407-7. Retrieved 26 August 2014.
- Dunlop 2003, pp. 77–78
- "Cumulonimbus Incus". Universities Space Research Association. 5 August 2009. Retrieved 23 October 2012.
- Aerographer/Meteorology (2012). "Roll cloud formation on cumulonimbus". Retrieved 5 July 2012.
- Dunlop 2003, p. 79
- Ludlum 2000, p. 473
- Task Team On Revision of the International Cloud Atlas (2013). "Final Report, pp 15-18". World Meteorological Organization. Retrieved 6 October 2014.
- Garret, et al. 2006, p. i
- Fox, Karen C. "NASA's Solar Dynamics Observatory Catches "Surfer" Waves on the Sun". NASA-The Sun-Earth Connection: Heliophysics. NASA.
- Ilan Koren & Graham Feingold (2013). "Adaptive behavior of marine cellularclouds". Retrieved 1 October 2013.
- "Cloud Formations off the West Coast of South America". NASA Earth Observatory. Retrieved 29 March 2013.
- NOAA, ed. (September 3, 2007). Federal Meteorological Handbook (FMH) Number 2. NOAA. p. C-17. Retrieved 26 November 2014.
- R. Nave (2013). "Adiabatic Process". gsu.edu. Retrieved 18 November 2013.
- Steve Horstmeyer (2008). "Cloud Drops, Rain Drops". Retrieved 19 March 2012.
- E. Freud and D. Rosenfeld (January 2012). "Linear relation between convective cloud drop number concentration and depth for rain initiation". American Geophysical Union. Retrieved 9 November 2014.
- Long,Michael J.; Hanks,Howard H.; Beebe,Robert G. (June 1965). "TROPOPAUSE PENETRATIONS BY CUMULONIMBUS CLOUDS". Retrieved 9 November 2014.
- Pidwirny, M. (2006). "Cloud Formation Processes", chapter 8 in Fundamentals of Physical Geography, 2nd ed.
- Steven A. Ackerman (2011). Meteorology:Fog Formation. Published by Jones & Bartlett. Retrieved 22 October 2013.
- Glossary of Meteorology (2009). "Radiational cooling". American Meteorological Society. Retrieved 27 December 2008.
- Robert Fovell (2004). "Approaches to saturation". University of California in Los Angeles. Retrieved 7 February 2009.
- Robert Penrose Pearce (2002). Meteorology at the Millennium. Academic Press. p. 66. ISBN 978-0-12-548035-2.
- National Weather Service Office, Spokane, Washington (2009). "Virga and Dry Thunderstorms". National Oceanic and Atmospheric Administration. Retrieved 2 January 2009.
- Bart van den Hurk and Eleanor Blyth (2008). "Global maps of Local Land-Atmosphere coupling". KNMI. Retrieved 2 January 2009.
- H. Edward Reiley, Carroll L. Shry (2002). Introductory horticulture. Cengage Learning. p. 40. ISBN 978-0-7668-1567-4.
- JetStream (2008). "Air Masses". National Weather Service. Retrieved 2 January 2009.
- Kirill Iakovlevich Kondratʹev (2006). Atmospheric aerosol properties: formation, processes and impacts. Springer. p. 403. ISBN 978-3-540-26263-3.
- Leung Wei-hung (2010). "Meteorology Basics: Convergence and Divergence". Hong Kong Observatory. Retrieved 8 December 2014.
- "Inter-Tropical Convergence Zone". JetStream - Online School for Weather. NOAA. 2007-10-24. Retrieved 2009-06-04.
- Yochanan Kushnir (2000). "The Climate System: General Circulation and Climate Zones". Retrieved 13 March 2012.
- Jack Williams (27 June 1997). "Extratropical storms are major weather makers". USA Today. Retrieved 13 March 2012.
- "Mackerel sky". Weather Online. Retrieved 21 November 2013.
- Weston 1980, pp. 437–438
- Stubenrauch, C. J.; Rossow, W. B.; Kinne, S.; Ackerman, S.; Cesana, G.; Chepfer, H; Di Girolamo, L.; Getzewich, B.; Guignard, A.; Heidinger, A.; Maddux, B. C.; Menzel, W.P; Minnis, P.; Pearl, C.; Platnick, S.; Poulsen, C.; Reidi, J.; Sun-Mack, S; Walther, A.; Winker, D.; Zeng, S.; Zhao, G. (2013). "Assessment of global cloud datasets from satellites: Project and Database initiated by GEWEX Radiation Panel" (pdf). Bulletin of the American Meteorological Society 94: 1031–1049. doi:10.1175/BAMS-D-12-00117.1.
- NOAA/ESRL/GSD Forecast Verification Section (2009). "Verification of WAFS Icing Products". Retrieved 11 November 2014.
- Les Cowley (2011). "Nacreous and polar stratospheric clouds". Atmospheric optics, atoptics.co.uk. Retrieved 7 November 2014.
- Turco, R. P.; Toon, O. B.; Whitten, R. C.; Keesee, R. G.; Hollenbach, D. (1982). "Noctilucent clouds: Simulation studies of their genesis, properties and global influences". Planetary and Space Science 30 (11): 1147. doi:10.1016/0032-0633(82)90126-X.
- Karen C. Fox (2013). "NASA Sounding Rocket Observes the Seeds of Noctilucent Clouds". Retrieved 1 October 2013.
- American Heritage Science Dictionary (2010). "cohesion science definition". Retrieved 25 July 2012.
- The Westminster review (2013). attraction cohesive cloud droplets. Retrieved 1 October 2013.
- UCAR Center for Science Education, ed. (2011). "The Troposphere - overview". Retrieved 15 January 2015.
- World Meteorological Organization, ed. (1975). Luminance, International Cloud Atlas I. pp. 9–10. ISBN 92-63-10407-7. Retrieved 13 January 2015.
- Increasing Cloud Reflectivity, Royal Geographical Society, 2010.
- Bette Hileman (1995). "Clouds absorb more solar radiation than researchers previously thought". Chemical & Engineering News 73 (7): 33. doi:10.1021/cen-v073n007.p033.
- World Meteorological Organization, ed. (1975). Coloration, International Cloud Atlas I. pp. 10–11. ISBN 92-63-10407-7. Retrieved 13 January 2015.
- emereo publishing (March 2014). "Cloud Coloration". Emereo Publishing. Retrieved 8 November 2014.
- University of Wisconsen-Madison-News, ed. (2007). "Curiosities-Green sky before tornado". Retrieved 17 January 2015.
- Cities and Air Pollution, Nature, 1998, chapter 10
- Frank W. Gallagher, III. (October 2000). "Distant Green Thunderstorms – Frazer's Theory Revisited". Journal of Applied Meteorology (American Meteorological Society) 39 (10): 1754–1757. Bibcode:2000JApMe..39.1754G. doi:10.1175/1520-0450-39.10.1754.
- "Cloud Fraction : Global Maps". nasa.gov. Retrieved 26 October 2014.
- D. Randall, R. Wood, S. Bony, R. Colman, T. Fichefet, J. Fyfe, V. Kattsov, A. Pitman, J. Shukla, J. Srinivasan, R. Stouffer, A. Sumi, and K. Taylor (2007) "Climate models and their evaluation" in S. Solomon, D. Qin, M. Manning, Z. Chen, M. Marquis, K. Averyt, M.Tignor, and H. Miller (eds.) Climate Change 2007: The Physical Science Basis. Contribution of Working Group I to the Fourth Assessment Report of the Intergovernmental Panel on Climate Change. Cambridge University Press, Cambridge, United Kingdom and New York, NY, USA.
- "Will Clouds Speed or Slow Global Warming?". National Science Foundation. Retrieved 23 October 2012.
- "Cloud Climatology". International Satellite Cloud Climatology Program. National Aeronautics and Space Administration. Retrieved 12 July 2011.
- Steven A. Ackerman (2011). Meteorology:Clouds and the Greenhouse Effect. Published by Jones & Bartlett. Retrieved 23 October 2013.
- Franks F. (2003). "Nucleation of ice and its management in ecosystems" (PDF). Philosophical Transactions of the Royal Society A 361 (1804): 557–574. Bibcode:2003RSPTA.361..557F. doi:10.1098/rsta.2002.1141. PMID 12662454.
- T. Okita (1961). "Size Distribution of Large Droplets in Precipitating Clouds". tellusa. Retrieved 24 November 2013.
- S. Bony and J.-L. Dufresne (2005). "Marine boundary layer clouds at the heart of tropical cloud feedback uncertainties in climate models". Geophysical Research Letters 32 (20). Bibcode:2005GeoRL..3220806B. doi:10.1029/2005GL023851.
- B. Medeiros, B. Stevens, I.M. Held, M. Zhao, D.L. Williamson, J.G. Olson, and C.S. Bretherton (2008). "Aquaplanets, Climate Sensitivity, and Low Clouds". Journal of Climate 21 (19): 4974. Bibcode:2008JCli...21.4974M. doi:10.1175/2008JCLI1995.1.
- Martin Wild, Hans Gilgen, Andreas Roesch, Atsumu Ohmura, Charles N. Long, Ellsworth G. Dutton, Bruce Forgan, Ain Kallis, Viivi Russak, and Anatoly Tsvetkov (2005). "From Dimming to Brightening: Decadal Changes in Solar Radiation at Earth's Surface". Science 308 (5723): 847–50. Bibcode:2005Sci...308..847W. doi:10.1126/science.1103215. PMID 15879214.
- Costantino, L. and F.-M. Bréon (2010). "Analysis of aerosol-cloud interaction from multi-sensor satellite observations". Geophysical Research Letters 37 (11): n/a. Bibcode:2010GeoRL..3711801C. doi:10.1029/2009GL041828.
- S. A. Twomey (1974). "Pollution and the planetary albedo". Atmospheric Environment (1967) 8 (12): 1251. doi:10.1016/0004-6981(74)90004-3.
- B. Stevens and G. Feingold (2009). "Untangling aerosol effects on clouds and precipitation in a buffered system". Nature 461 (7264): 607–13. Bibcode:2009Natur.461..607S. doi:10.1038/nature08281. PMID 19794487.
- Bougher & Phillips 1997, pp. 127–129
- Franck Montmessin (2013). "Clouds in the terrestrial planets". Retrieved 5 November 2013.
- David Shiga (2006). "Mysterious waves seen in Venus's clouds". New Scientist. Retrieved 5 November 2013.
- "Clouds Move Across Mars Horizon". Phoenix Photographs. National Aeronautics and Space Administration. 19 September 2008. Retrieved 15 April 2011.
- "NASA SP-441: Viking Orbiter Views of Mars". National Aeronautics and Space Administration. Retrieved 26 January 2013.
- Phillips, Tony (20 May 2010). "Big Mystery: Jupiter Loses a Stripe". Nasa Headline News – 2010. National Aeronautics and Space Administration. Retrieved 15 April 2011.
- Dougherty & Esposito 2009, p. 118
- A.P. Ingersoll, T.E. Dowling, P.J. Gierasch, G.S. Orton, P.L. Read, A. Sanchez-Lavega, A.P. Showman, A.A. Simon-Miller, A.R. Vasavada. "Dynamics of Jupiter’s Atmosphere" (PDF). Lunar & Planetary Institute. Retrieved 1 February 2007.
- Monterrey Institute for Research in Astronomy (11 August 2006). "Saturn". Retrieved 31 January 2011.
- "Thunderheads on Jupiter". Jet Propulsion Laboratory. National Aeronautics and Space Administration. Retrieved 26 January 2013.
- Minard, Anne (14 October 2008). "Mysterious Cyclones Seen at Both of Saturn's Poles". National Geographic News (National Geographic). Retrieved 26 January 2013.
- Nola Taylor Redd (2012). "Neptune's Atmosphere: Composition, Climate, & Weather". Space.com. Retrieved 5 November 2013.
- Boyle, Rebecca (18 October 2012). "Check Out The Most Richly Detailed Image Ever Taken Of Uranus". Popular Science. Retrieved 26 January 2013.
- Irwin 2003, p. 115
- "Uranus". Scholastic. Archived from the original on 24 July 2011. Retrieved 16 April 2011.
- Lunine, Jonathan I. (September 1993). "The Atmospheres of Uranus and Neptune". Annual Review of Astronomy and Astrophysics 31: 217–263. Bibcode:1993ARA&A..31..217L. doi:10.1146/annurev.aa.31.090193.001245.
- Linda T. Elkins-Tanton (2006). Uranus, Neptune, Pluto, and the Outer Solar System. New York: Chelsea House. pp. 79–83. ISBN 0-8160-5197-6.
- Athéna Coustenis and F.W. Taylor (2008). Titan: Exploring an Earthlike World. World Scientific. pp. 154–155. ISBN 978-981-270-501-3.
- "Surprise Hidden in Titan's Smog: Cirrus-Like Clouds". Mission News. National Aeronautics and Space Administration. 3 February 2011. Retrieved 16 April 2011.
- Chu, Jennifer (2 October 2013). "Scientists generate first map of clouds on an exoplanet". MIT. Retrieved 2 January 2014.
- Demory, Brice-Olivier et al. (30 September 2013). "Inference of Inhomogeneous Clouds in an Exoplanet Atmosphere". arXiv. arXiv:1309.7894. Retrieved 2 January 2014.
- Harrington, J.D.; Weaver, Donna; Villard, Ray (31 December 2013). "Release 13-383 - NASA's Hubble Sees Cloudy Super-Worlds With Chance for More Clouds". NASA. Retrieved 1 January 2014.
- Moses, Julianne (1 January 2014). "Extrasolar planets: Cloudy with a chance of dustballs". Nature (journal) 505: 31–32. doi:10.1038/505031a. Retrieved 1 January 2014.
- Knutson, Heather et al. (1 January 2014). "A featureless transmission spectrum for the Neptune-mass exoplanet GJ 436b". Nature (journal) 505: 66–68. doi:10.1038/nature12887. Retrieved 1 January 2014.
- Kreidberg, Laura et al. (1 January 2014). "Clouds in the atmosphere of the super-Earth exoplanet GJ 1214b". Nature (journal) 505: 69–72. doi:10.1038/nature12888. Retrieved 1 January 2014.
- Hamblyn, Richard The Invention of Clouds – How an Amateur Meteorologist Forged the Language of the Skies Picador; Reprint edition (3 August 2002). ISBN 0-312-42001-3
- Could Reducing Global Dimming Mean a Hotter, Dryer World?
Find more about
at Wikipedia's sister projects
|Definitions from Wiktionary|
|Media from Commons|
|News stories from Wikinews|
|Quotations from Wikiquote|
|Source texts from Wikisource|
|Textbooks from Wikibooks|
|Learning resources from Wikiversity|
- BadMeteorology's explanation of why clouds form
- Monthly maps of global cloud cover, from NASA's Earth Observatory
- Introduction to Clouds: Sky Watcher Chart National Oceanic and Atmospheric Administration and National Aeronautics and Space Administration
- Cloud Appreciation Society Aesthetics of clouds
- Shuttle Views the Earth: Clouds from Space
- Details of main cloud types and sub types
- USA Today Understanding clouds and Fog
- clouds that look as if they were sculpted out of the sky
- Clouds 365 Project Year-long photographic experiment shooting clouds everyday
- The Function of Clouds
- The short film Know Your Clouds (1 January 1967) is available for free download at the Internet Archive