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Immagini di 'U Bend' trovate, 13

Triptych May-June 1973

Triptych May-June 1973

Bacon, Francis (1909-92)

XJL169810

RL 27835 Rounding a Bend on the Mississippi Steamboat Queen of the West (litho)

RL 27835 Rounding a Bend on the Mississippi Steamboat Queen of the West (litho)

Currier, N. (1813-88) and Ives, J.M. (1824-95)

BAL32898

Kitchen (oil on canvas)

Kitchen (oil on canvas)

Andrist, Alice (b.1902)

MNS488169

The Letter U (colour litho)

The Letter U (colour litho)

English School, (20th century)

LLM3642900

A Chinese office worker reads today's edition of the Yangcheng evening news featuring a picture of U.., 1999-04-04 (photo)

A Chinese office worker reads today's edition of the Yangcheng evening news featuring a picture of U.., 1999-04-04 (photo)

Natalie Behring

REU7613347

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenithal arc, very colorful. October 28, 2006 Quimper (France) — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenitha

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenitha

Laurent Laveder

PIX4670932

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenithal arc, very colorful. October 28, 2006 Quimper (France) — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenitha

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele”” to the halo of 22* radius, the arc of Parry. - near the zenith, the arc cirucmzenithal, very colourful. Quimper Halos are caused by sunlight being refracted by cirro-stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenitha

Laurent Laveder

PIX4670923

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the right of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenithal arc, very colorful. -, tangent to it, the inconspicuous supralateral arc — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Laurent Laveder

PIX4670921

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the right of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc (a splayed U shape). - above it, “” parallel”” to the 22* halo, the Parry arc. - near the zenith, the cirucmzenithal arc, very colorful. -, tangent to it, the inconspicuous supralateral arc — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Laurent Laveder

PIX4670979

Valley towards Saltillo, From near the base of "Palace Hill," at Monterey. [Looking to the S. West.]... [No. 3.] [with the rear guard and wagon train of the U. S. Army coming into the Castle after its capitulation]., 1847 (lithograph)

Valley towards Saltillo, From near the base of "Palace Hill," at Monterey. [Looking to the S. West.]... [No. 3.] [with the rear guard and wagon train of the U. S. Army coming into the Castle after its capitulation]., 1847 (lithograph)

Parsons, Charles (1821-1910)

HST2634499

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parry arc. - near the zenith, the circumzenithal arc. October 28, 2006 — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Laurent Laveder

PIX4670954

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parry arc. - near the zenith, the circumzenithal arc. October 28, 2006 — Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Laurent Laveder

PIX4670945

Kittanning Point, "Horse-Shoe Bend". USA

Kittanning Point, "Horse-Shoe Bend". USA

American School, (19th century)

LZT1005559

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