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'Cirrus' images et/ou videos résultats page 1 of 1

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86 médias trouvés pour 'Cirrus'

Study of Cirrus Clouds, c.1822 (oil on canvas)
Altitude Cloud/Cirrus
Study of Cirrus, 1822 (oil on canvas)
Cirrus clouds in deep blue sky
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Cirrus clouds drift across blue sky in timelapse, showing cirrus fibratus streaks.
BLUNT/CLOUDS/CIRRUS/PL98
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Cirrus clouds over a seascape. Coloured lithograph 1845.
Clouds: fibrous cirrus puffs
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Light cirro-cumulus beneath cirrus, 1803-1811
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Cirrus clouds - floccus species against a pale blue sky
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Lacunosis variety of cirrus clouds in a deep blue sky above.
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Cirrus cloud in the form of a mares tail in a deep blue sky.
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Thin and wispy Cirrus clouds in a blue sky, the most common type of high-level clouds found at heights greater than 6,000 metres, usually occurring in fair weather.
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Natural history of clouds: cirrus, cirrostratus, cirrocumulus, nimbus, etc. Handcoloured copperplate engraving from Friedrich Johann Bertuch's Bilderbuch fur Kinder (Picture Book for Children), Weimar, 1823.
Natural history of clouds: cirrostratus, cirrus, cumulus, cumulostratus, etc. Handcoloured copperplate engraving from Friedrich Johann Bertuch's Bilderbuch fur Kinder (Picture Book for Children), Weimar, 1823.
Stratocumulus, white and grey clouds characterised by large dark, rounded masses, thin and wispy cirrus catching sunlight, sun brightening and illuminating white areas, blue sky seen in patches, fields below.
Norway; Svalbard Islands; cirrus clouds over North-western coast
(photo)
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Single cirrus cloud drifts over beach and sea in a minimalist timelapse coastal scene.
Traditional homes dot a snowy valley beneath cirrus clouds, creating a quiet highland scene.
Clouds: segmented, fibrous cirrus cloud and a high cirro-cumulus cloud in the process of freezing
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Timelapse storm clouds and cirrus drift across blue sky, revealing fast changing weather.
New Zealand mountains show cirrus clouds above untouched mixed forest and clear sky.
Dense cloud sea from plane window with cirrus fragments drifting above white layers.
1960s: farmer on tractor pulls farm equipment in field, blue sky filled with cirrus clouds
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Timelapse cirrus clouds drift above treeless rocky mountain range forming a dramatic cliff barrier.
Condensation Trains - Contrails - Aircraft Condensation Trainees whose shadow is projected on the lower cirrus sail
Fishes: Perciformes Centracanthidae -  Picarel (Spicara smaris), Curled picarel (Centracanthus cirrus), Blotched picarel (Spicara maena) illustration
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Wispy cirrus stretch above alpine forest and green hills, opening toward distant mountain ridges.
Wispy cirrus stretch above alpine forest and green hills, opening toward distant mountain ridges.
Panoramic view of Setif, Algeria
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Cirrus clouds spreading out in long line downwind from the contrail in a blue sky, small airfield below, aeroplane in foreground.
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Portugal, Algarve, Portimao, traditional painted wooden boat on Arade River, with modern Arade River Bridge in background, close-up
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Great Bear Lake timelapse shows cirrus clouds across blue white sky in Northwest Territories.
Wispy cirrus stretch above alpine forest and green hills, opening toward distant mountain ridges.
Norway; Svalbard Islands; North-western coast
(photo)
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High thin cirrus clouds, ripening field of wheat and lone oil pump jack, rural Alberta, Canada, 2007
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Logos of different credit card companies (photo)
1960s: farmer on tractor steers with one hand, works equipment behind him with the other hand, blue sky filled with cirrus clouds
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Post-war period: French soldiers during manoeuvre in Germany
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Post-war period: French soldiers build Rhine bridge during manoeuvre in Germany
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Illustrations showing different types of clouds as described by the author.
a,a, represents different appearances of the cirrus: b, a regular cumulus: c, a stratus occupying a valley at sun-set, in the midst of which is supposed a spot of higher ground, with trees etc.
Post-war period: French soldiers during manoeuvre in Germany
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Post-war period: French soldiers during manoeuvre in Germany
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Cloud formations, 1 Cumulus, 2 Stratus, 3 Cirrocumulus, 4 Cirrus, 5 Nimbus, lithograph by Salvatore Puglia from Poliorama Pittoresco, n 43, June 3, 1843
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Post-war period: French soldiers during manoeuvre in Germany
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Post-war period: French soldiers during manoeuvre in Germany
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Post-war period: French soldiers during manoeuvre in Germany
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Post-war period: French soldiers during manoeuvre in Germany
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Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Earth. Unlike cirrus clouds on Earth however, which are composed of crystals of water ice, Neptune's cirrus clouds are made up of crystals of frozen methane. Neptune's clouds are driven by winds of 1,200 mph, the fastest winds of any planet in the Solar System
Lunar Halo - Lunar Halo - Lunar Halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. Lunar halos are caused by moonlight being refracted by cirro - stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter
Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. This image obtained by a 50 cm amateur telescope, in February 2010 for 23 hours of poses, shows gas filaments whose origin is uncertain. Located about 12 million light - years from our planet, M81 (NGC 3031) together with M82 (NGC 3034), NGC 3077 and NGC 2976 forms one of the most iconic groups of interacting galaxies. The M81 group has also been the subject of many studies searching for and analyzing evidence of strong interactions among its components. In 1965, Halton Arp detected an unusual looping feature near M81 while examining photographic plates produced with the 48 - inch Schmidt on Mount Palomar. Traditionally, ARP's loop has been interpreted as a tail resulting from the tidal interaction between M81 and M82. However, since its discovery that explanation has been doubted by many researchers. Interestingly, the region of the sky containing the M81 group of galaxies is filled with Galactic cirrus and ARP's loop exhibits colors and emission properties similar to those observed in Galactic cirrus clouds. This optical image suggests that the light observed at optical wavelengths is a combination of emissions from: recent star forming regions situated near M81, the extended disk of M81 and scattered light from the same Galactic cirrus that is responsible for the bulk of the far infrared emissions. Although our observations cannot exclude the presence of some material stripped from the disk of M81 (NGC 3031) and/or M82 (NGC 3034) that is chance located in our line of sight to and far behind this intruiging structure, our findings suggest that ARP's Loop is situated between the observer and M81 (
Earth's atmosphere and night clouds - Earth's atmosphere, noctilucent clouds and Moon - View of the Earth's atmosphere and a crescent moon photographs from the International Space Station on July 27, 2003. Night clouds are also visible. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Noctilucent clouds are very high clouds that look like cirrus clouds, but are much higher (75 - 90 km above the Earth's surface) than clouds that we observe every day. They are optically thin and can only be observed during twilight hours, when the sun is just below the horizon and only shines on the uppermost atmosphere. In this image, the limb of the Earth at the bottom transitions into the orange - colored troposphere, the lowest and most dense portion of the Earth's atmosphere. The troposphere ends abruptly at the tropopause, which appears in the image as the sharp boundary between the orange - and blue - colored atmosphere. The silvery - blue noctilucent clouds are far above this boundary. This image was taken July 27, 2003 when the International Space Station was over central Asia. June and July is the season for noctilucent clouds in the northern hemisphere - - they form in the polar mesosphere, generally above 50 degrees latitude
Neptune from Triton - Illustration - Neptune from the surface of Triton - Neptune seen from the icy surface of his Triton satellite. White cirrus clouds race across a crescent Neptune as it presides over Triton's bleak and frozen south polar region. Sheets of frozen nitrogen ice with traces of other substances, including frozen methane and carbon monoxide, overlie Triton's darker material. The ice has turned pink due to the interaction with ultraviolet light from the distant Sun. Further south all of the surface of Triton is covered by such ices
Tropical Tempete Sam seen from Shuttle Columbia. - Tropical Storm Sam, Eastern Indian Ocean - Tropical Tempete Sam seen by Shuttle Columbia over the Indian Ocean in January 1990. Tropical Storm Sam, Eastern Indian Ocean, exact location unknown, was begining to decay when this photograph was taken. The storm was mostly at sea for its entire duration and had little effect on land. The eye of the storm is still visible with the gyre of swirling clouds rotating clockwise. Winds aloft have begun to shear the tops of the thunderstorms associated with the storm forming a high cirrus cloud cover over the center of the storm
Earth's atmosphere and noctiluque clouds - Earth's atmosphere and noctilucent clouds - View of the Earth's atmosphere with night clouds photographs from the International Space Station on July 22, 2008. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Polar Mesospheric Clouds (also known as noctilucent clouds) are transient, upper atmospheric phenomena observed usually in the summer months at high latitudes (greater than 50 degrees) of both the Northern and Southern Hemispheres. They are bright and cloudlike in appearance while in deep twilight. They are illuminated by sunlight when the lower layers of the atmosphere are in the darkness of the Earth's shadow. This image was acquired at an altitude of just over 200 miles in the pre - dawn hours of July 22, 2008 as the International Space Station was passing over western Mongolia in central Asia. The dark horizon of the Earth appears below with some layers of the lower atmosphere already illuminated. The higher, bluish - colored clouds look much like wispy cirrus clouds which can be found in the troposphere as high as 60,000 feet. However noctilucent clouds, as seen here, are observed in the mesosphere at altitudes of 250,000 to 280,000 feet. Astronaut observations of Polar Mesospheric Clouds (PMC) over northern Asia in June and July are not uncommon
Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet
Halo around the Moon - Lunar Halo - Halo around the Moon observes a few hours before the full Moon on January 10, 2009. The paper pencil-shaped ice crystals present in the cirrus form the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give birth to this large coloured circle (red inside and blue outside). Lunar halos are caused by moonlight being refracted by cirro - stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter. January 10 2009
Lebanon Mediterranean coastline timelapse shows drifting clouds, misty water, sunlit horizon.
Cloud study by Luke Howard, c 1808-1811
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Condensation trains over Brittany - Airplane contrails over Brittany, France - A multitude of condensation trains caused by air traffic appear on this image obtained by the Terra satellite on 25 April 2004. This true - color Moderate Resolution Imaging Spectroradiometer (MODIS) image, acquired on April 25, 2004 by the Terra satellite, shows a web of contrails over northwestern Europe. These contrails are straight lines of ice crystals that form in the wake of jet liners where air temperatures at altitude are lower than about 40* C. Newer contrails are thin whereas older trails have widened with time as a result of light winds. The problem with contrails is that they can spread into extensive high, thin cirrus clouds, which tend to warm the Earth because they reflect less sunlight back to space than the amount of heat they trap
Halo and Light Column- Ice halos near Zeel am See, Austria - A light column is created by the reflection of a light source on the horizontal faces of ice crystals. So it takes a fairly stable atmosphere to keep these crystals parallel to the horizon. Lunar halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. A paraselene consists of light spots located on the left and right at the height of the Moon. Austria, January 2016. A light pillar is created by the reflection of light on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter
Neptune - Voyager 2 - Image of the Great Dark Spot on Neptune obtained by the Voyager 2 probe on August 23, 1989. The Great Dark Spot is the size of the Earth and winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Date: 08/23/89 Range: 2.8 million km. (1.7 million miles) Smallest Resolvable Feature: 50 km or 31 miles This Voyager 2 image shows the last face on view of the Great Dark Spot that Voyager 2 will take with the narrow angle camera. It was made 45 hours before the closest approach to Neptune. the image shows feathery white clouds that overlie the boundary of the dark and light blue regions. the pinwheel (spiral) structure of both the dark boundary and the white cirrus suggest a storm system rotating counterclockwise. Periodic, small - scale patterns in the white clouds, possibly waves, are short - lived and do not persist from one Neptunian rotation to the next. This color composite was made from the clear and green filter images
Feather Stars, Crinoids
Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the first evidence that the GDS lies lower in the atmosphere than these bright clouds, which have remained in its vicinity for several months. Increasing detail in global banding, and the south polar can also be seen. A smaller dark spot at high southern latitudes is dimly visible near the limb at lower left
Total Moon Eclipse and Lactee Track, Namibia 2018
Types of cloud, 1803
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