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Switzerland Coca-Cola Squad (b/w photo)

Switzerland Coca-Cola Squad (b/w photo)

Nandor Nagy

KES6251607

A row of Canberra 5 fuselages, being tested, Preston, 1956

A row of Canberra 5 fuselages, being tested, Preston, 1956

UIS5073822

Allied navies bombard the French coast at Provence

Allied navies bombard the French coast at Provence

IMW6287793

Metal spinning a section for a Canberra aircraft, English Electric, 1956

Metal spinning a section for a Canberra aircraft, English Electric, 1956

UIS5073824

May 05, 1953 - Flying Over The North Pole: Two Hastings aircraft of the Royal Air Force Flying College at Manby, Lines., have just returned with these photograph taken by an Air Ministry photographer on flights over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour flights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic Circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigation over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron Leader H.D. Archer, D.F.C., and Flight Lieut. R.W. Firmin, D.F.C., the aircraft which carried two staff navigators and five students, with other air and ground crew

May 05, 1953 - Flying Over The North Pole: Two Hastings aircraft of the Royal Air Force Flying College at Manby, Lines., have just returned with these photograph taken by an Air Ministry photographer on flights over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour flights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic Circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigation over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron Leader H.D. Archer, D.F.C., and Flight Lieut. R.W. Firmin, D.F.C., the aircraft which carried two staff navigators and five students, with other air and ground crew

ZUM4842226

May 11, 1953 - Flying Over The North Pole: Two hastings aircraft of the Royal Air Force Flying College at Manby, Linos., have just returned with these photographs taken by an Air Ministry photographer on flights over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour flights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic Circle (position: 74 degrees 50 minutes North, 95 degrees West) The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigation over featureless areas, where magnetic compasse are unrealible, using special techniques. Captained by Squadron Lesder H.D. Archer, D.F.C., and Flight Lieut. R.W. Firmin, D.F.C., the aircraft wach carried two staff navigators and five students, with other air and ground crew

May 11, 1953 - Flying Over The North Pole: Two hastings aircraft of the Royal Air Force Flying College at Manby, Linos., have just returned with these photographs taken by an Air Ministry photographer on flights over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour flights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic Circle (position: 74 degrees 50 minutes North, 95 degrees West) The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigation over featureless areas, where magnetic compasse are unrealible, using special techniques. Captained by Squadron Lesder H.D. Archer, D.F.C., and Flight Lieut. R.W. Firmin, D.F.C., the aircraft wach carried two staff navigators and five students, with other air and ground crew

ZUM4846123

Edelweiss Squadron, 1940.

Edelweiss Squadron, 1940.

LCS7223901

The first attempt to reach the stratosphere January 30 1934. Scientists, physicians and Soviet space program pioneers in laboratories performing experiments, first rocket launch.

The first attempt to reach the stratosphere January 30 1934. Scientists, physicians and Soviet space program pioneers in laboratories performing experiments, first rocket launch.

FLM2598281

May 05, 1953 - FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Ranby, Lines., have just returned with these photographs taken by an air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which is within the Arctic circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H. D. Archer, D.F.C., and Flight Lieutenant R. W. Firmin, the aircraft each carried two staff navigators and five students, with other air and ground crew. BRITISH OFFICIAL PHOTO SHOWS: On returning from the North Pole, the two Hastings were inspected and serviced, and special engine covers were used.

May 05, 1953 - FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Ranby, Lines., have just returned with these photographs taken by an air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which is within the Arctic circle (position: 74 degrees 50 minutes North, 95 degrees West). The flights, which involved flying 10,115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H. D. Archer, D.F.C., and Flight Lieutenant R. W. Firmin, the aircraft each carried two staff navigators and five students, with other air and ground crew. BRITISH OFFICIAL PHOTO SHOWS: On returning from the North Pole, the two Hastings were inspected and serviced, and special engine covers were used.

ZUM4841627

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

Earth observed at night by satellite. Mosaic of hundreds of images obtained by four satellites DMSP (Defense Meteorological Satellite Program) from October 1994 to March 1995 - The image is a composite of hundreds of pictures made by the Defense Meteorological Satellite Program (DMSP) currently operates four satellites carrying the Operational Linescan System (OLS) in low-altitude polar orbits. Three of these satellites record nighttime data. The DMSP-OLS has a unique capability to detect low levels of visible-near infrared (VNIR) radiance at night. With the OLS 'VIS' band data it is possible to detect clouds illuminated by moonlight, plus lights from cities, towns, industrial sites, gas flares, and ephemeral events such as fires and lightning-illuminated clouds. October 1994 - March 1995 DMSP nighttime data collected when moonlight was low. Using the OLS thermal infrared band, areas containing clouds were removed and the remaining area used in the time series: Earth by night

PIX4669194

Velle / Denkste, 2010 (plaster)

Velle / Denkste, 2010 (plaster)

Schlothauer, Cornelia (21st Century)

STF452341

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. - 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. - 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

May 05, 1953 - British Official Photograph (Air Ministry) Crown Copyright Reserved. FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Manby, Lines., have just returned with these photographs taken by an Air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic circle (position: 74 degrees 50 minutes north, 95 degrees West) The flights, which involved flying 10, 115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H.D. Archer, D.F.C. and Flight Lieutenant H.W. Firmin, D.F.C., the aircraft carried two staff navigators and five students, with other air and ground crew. British Official Photo Shows: Pack ice and open water between Devon Island, in the North-West

May 05, 1953 - British Official Photograph (Air Ministry) Crown Copyright Reserved. FLYING OVER THE NORTH POLE: Two Hastings aircraft of the Royal Air Force Flying College at Manby, Lines., have just returned with these photographs taken by an Air Ministry photographer on fly over and near the North Pole. Each aircraft circled the Geographical Pole on two 11-hour fights from the Royal Canadian Air Force base at Resolute Bay, which lies within the Arctic circle (position: 74 degrees 50 minutes north, 95 degrees West) The flights, which involved flying 10, 115 miles, gave practical training in high-altitude navigational work over featureless areas, where magnetic compasse are unreliable, using special techniques. Captained by Squadron leader H.D. Archer, D.F.C. and Flight Lieutenant H.W. Firmin, D.F.C., the aircraft carried two staff navigators and five students, with other air and ground crew. British Official Photo Shows: Pack ice and open water between Devon Island, in the North-West

ZUM4841681

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

Jul 07, 1953 - First Picture Released Of Bomber Command's New Rapier: The Handley Page Victor 4-jet crescent-wing bomber - more powerful than 25 express locomotives - makes its public debut before the Queen next Wednesday at the R.A.F. Coronation Review. Since its Maiden flight last Christmas Eve it has been carrying out an exhaustive test-flying programme and was airborne no less than six times in one day recently. The Victor was ordered in quantity from the drawing-board and is now in super-priority production for R.A.F. Bomber Command. Its revolutionary crescent wing enables it to cruise at high altitude with near-sonic speed. It flies so fast that it is protected by the sound-barrier; conditions near the speed of sound render attacking fighters ineffective. The Victor is the outstanding example of the modern concept of a bomber as a rapier - an atomically hard-hitting and accurate weapon able to paralyse an enemy's nerve-centres and yet, by outstanding performance, avoid intercepti

Jul 07, 1953 - First Picture Released Of Bomber Command's New Rapier: The Handley Page Victor 4-jet crescent-wing bomber - more powerful than 25 express locomotives - makes its public debut before the Queen next Wednesday at the R.A.F. Coronation Review. Since its Maiden flight last Christmas Eve it has been carrying out an exhaustive test-flying programme and was airborne no less than six times in one day recently. The Victor was ordered in quantity from the drawing-board and is now in super-priority production for R.A.F. Bomber Command. Its revolutionary crescent wing enables it to cruise at high altitude with near-sonic speed. It flies so fast that it is protected by the sound-barrier; conditions near the speed of sound render attacking fighters ineffective. The Victor is the outstanding example of the modern concept of a bomber as a rapier - an atomically hard-hitting and accurate weapon able to paralyse an enemy's nerve-centres and yet, by outstanding performance, avoid intercepti

ZUM4863605

LINE CADORNA Forte at Dossaccio di Oga, part of the North Frontier, the defensive system

LINE CADORNA Forte at Dossaccio di Oga, part of the North Frontier, the defensive system

Elena Piccini

FGL6203230

LINE CADORNA Forte at Dossaccio di Oga, part of the North Frontier, the defensive system

LINE CADORNA Forte at Dossaccio di Oga, part of the North Frontier, the defensive system

Elena Piccini

FGL6203229

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Rainer Krack

PFH1774274

Nepal: Hashish-smoking sadhu, Pashupatinath, Kathmandu

Nepal: Hashish-smoking sadhu, Pashupatinath, Kathmandu

Rainer Krack

PFH1774271

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Rainer Krack

PFH1774272

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Chaweewan Chuchuay

PFH1774273

Nepal: Sadhu (Holy Man) near Durbar Square, Kathmandu

Nepal: Sadhu (Holy Man) near Durbar Square, Kathmandu

Chaweewan Chuchuay

PFH1774326

Nepal: Sadhu holy men in Kathmandu

Nepal: Sadhu holy men in Kathmandu

Chaweewan Chuchuay

PFH2562481

Nepal: Hashish-smoking sadhu with his shankha (ritual conch shell), a symbol of Vishnu, Pashupatinath, Kathmandu

Nepal: Hashish-smoking sadhu with his shankha (ritual conch shell), a symbol of Vishnu, Pashupatinath, Kathmandu

Rainer Krack

PFH2562480

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck, Durbar Square, Kathmandu

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck, Durbar Square, Kathmandu

Rainer Krack

PFH2562483

Nepal: Sadhu with Shiva's trident (trishula) and a necklace made of rudraksha (seeds used for prayer beads in Hinduism), Pashupatinath, Kathmandu

Nepal: Sadhu with Shiva's trident (trishula) and a necklace made of rudraksha (seeds used for prayer beads in Hinduism), Pashupatinath, Kathmandu

Chaweewan Chuchuay

PFH2562340

Nepal: Shiva Avatari Lama, Pashupatinath, Kathmandu

Nepal: Shiva Avatari Lama, Pashupatinath, Kathmandu

Rainer Krack

PFH1773697

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Nepal: Sadhu (Holy Man) wearing rudraksha (seeds used for prayer beads in Hinduism) around his neck and as a hat, Pashupatinath, Kathmandu

Chaweewan Chuchuay

PFH1774275

Nepal: Hashish-smoking sadhu with Shiva's trident (trishula), Pashupatinath, Kathmandu

Nepal: Hashish-smoking sadhu with Shiva's trident (trishula), Pashupatinath, Kathmandu

Rainer Krack

PFH2562479

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

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

HMAS Sydney's fight with a Zeppelin in the North Sea, 1918 (oil on canvas)

HMAS Sydney's fight with a Zeppelin in the North Sea, 1918 (oil on canvas)

Bryant, Charles David Jones (1883-1937)

MEM1268327

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

PIX4625231

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

PIX4625211

The Orion MPVC module - artist view - Orion spacecraft exploded view - Ecorchee view of the module lives in Orion. This module is intended to take a crew to the Moon where asteroides will also be used to commute with the space station. An artist's impression of the Orion spacecraft and its components including ESA's service module. The Crew Module sits atop the service module and can hold four astronauts and cargo. This the only part of Orion designed to reenter Earth's atmosphere: the heatshield protects it against the intense heat of reentry at 32,000 km/h. The European Service Module (ESM) provides electricity, propulsion, air and water, and forms part of the vehicle's structure, like a car chassis. More information about the module is given on separate pages to the left. A Crew Module Adapter (CMA) connects the capsule to the ESM. It houses electronic equipment for communications, power and control, and includes a bridge that connects electrical, data and fluid systems between the

The Orion MPVC module - artist view - Orion spacecraft exploded view - Ecorchee view of the module lives in Orion. This module is intended to take a crew to the Moon where asteroides will also be used to commute with the space station. An artist's impression of the Orion spacecraft and its components including ESA's service module. The Crew Module sits atop the service module and can hold four astronauts and cargo. This the only part of Orion designed to reenter Earth's atmosphere: the heatshield protects it against the intense heat of reentry at 32,000 km/h. The European Service Module (ESM) provides electricity, propulsion, air and water, and forms part of the vehicle's structure, like a car chassis. More information about the module is given on separate pages to the left. A Crew Module Adapter (CMA) connects the capsule to the ESM. It houses electronic equipment for communications, power and control, and includes a bridge that connects electrical, data and fluid systems between the

PIX4603537

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

PIX4565787

Andes, Chile - Bolivia - Volcano Licancabur/ASTER - The high - altitude, volcanic, arid terrain at the border of Bolivia and Chile has been described as the best Earth - based analog for conditions on Mars billions of years ago - - a time when scientists think it's possible that the surface of Mars harbored icy lakes and rivers. A team of scientists led by Nathalie Cabrol of NASA Ames Research Center believes the similarities are so compelling that in late October 2003, they arrived at the Licancabur Volcano to explore what life is able to exist in such an extreme environment - - as well as to test diving and other high - tech equipment like bodysuits that one day might be used to monitor the physiology (breathing rates, heartbeat, etc) of Mars explorers. Among the most interesting sites are the lakes - - the one in the caldera of the volcano itself and the one at the base of the volcano. Pictured here in this false - color image from the Advanced Spaceborne Thermal Emission and Reflec

Andes, Chile - Bolivia - Volcano Licancabur/ASTER - The high - altitude, volcanic, arid terrain at the border of Bolivia and Chile has been described as the best Earth - based analog for conditions on Mars billions of years ago - - a time when scientists think it's possible that the surface of Mars harbored icy lakes and rivers. A team of scientists led by Nathalie Cabrol of NASA Ames Research Center believes the similarities are so compelling that in late October 2003, they arrived at the Licancabur Volcano to explore what life is able to exist in such an extreme environment - - as well as to test diving and other high - tech equipment like bodysuits that one day might be used to monitor the physiology (breathing rates, heartbeat, etc) of Mars explorers. Among the most interesting sites are the lakes - - the one in the caldera of the volcano itself and the one at the base of the volcano. Pictured here in this false - color image from the Advanced Spaceborne Thermal Emission and Reflec

PIX4675943

Cuban Missile Crisis 1962

Cuban Missile Crisis 1962

BOF6283648

Not For Conquest 2of3

Not For Conquest 2of3

BOF6285240

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