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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
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

PIX4671730: 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 / Bridgeman Images

ID: PIX4671730

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

Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia
Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia

PIX4671634: Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia / Bridgeman Images

ID: PIX4671634

Noctulescent clouds - Noctilucent clouds - Noctilucent clouds, very high altitude clouds, photographs in July 2009 in Russia. These rare clouds are called noctilucent or “” night shining” as they seem to glow in the dark. They are caused by ice crystals at about 80 km altitude. These crystals reflect sunlight when the sun is well below the horizon. They are properly known as polar mesospheric clouds and are under intense study as it remains a mystery as to how they are formed. Image taken in july 2009 in Russia

Lunar crown - Lunar corona - A lunar crown is due to the diffraction of the light of the Moon by drops of water in medium-altitude clouds. Lunar corona is caused by the diffraction of the moonlight by water droplets
Lunar crown - Lunar corona - A lunar crown is due to the diffraction of the light of the Moon by drops of water in medium-altitude clouds. Lunar corona is caused by the diffraction of the moonlight by water droplets

PIX4671739: Lunar crown - Lunar corona - A lunar crown is due to the diffraction of the light of the Moon by drops of water in medium-altitude clouds. Lunar corona is caused by the diffraction of the moonlight by water droplets / Bridgeman Images

ID: PIX4671739

Lunar crown - Lunar corona - A lunar crown is due to the diffraction of the light of the Moon by drops of water in medium-altitude clouds. Lunar corona is caused by the diffraction of the moonlight by water droplets

Corona around the Moon - Corona around the Moon - When the light of the Moon passes through thin clouds of water droplets, it can create a moon crown of color. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud
Corona around the Moon - Corona around the Moon - When the light of the Moon passes through thin clouds of water droplets, it can create a moon crown of color. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud

PIX4671779: Corona around the Moon - Corona around the Moon - When the light of the Moon passes through thin clouds of water droplets, it can create a moon crown of color. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud / Bridgeman Images

ID: PIX4671779

Corona around the Moon - Corona around the Moon - When the light of the Moon passes through thin clouds of water droplets, it can create a moon crown of color. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud

Clouds Altostratus undulatus - Altostratus undulatus clouds - Medium clouds, between 2000m and 5000 m. These undulated clouds are low altostratus
Clouds Altostratus undulatus - Altostratus undulatus clouds - Medium clouds, between 2000m and 5000 m. These undulated clouds are low altostratus

PIX4671804: Clouds Altostratus undulatus - Altostratus undulatus clouds - Medium clouds, between 2000m and 5000 m. These undulated clouds are low altostratus / Bridgeman Images

ID: PIX4671804

Clouds Altostratus undulatus - Altostratus undulatus clouds - Medium clouds, between 2000m and 5000 m. These undulated clouds are low altostratus

Colored crown around the Moon and irizations - Corona around the Moon with irisation - Provoked by the microscopic drops of water that form these clouds, the crowns are colored blue as close to the Moon, then degrade from yellow to brick red. In the distance, on the edge of the cloud strip, another luminous phenomene is noticeable: these are colourful irisations such as those seen sometimes on some puddles. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud
Colored crown around the Moon and irizations - Corona around the Moon with irisation - Provoked by the microscopic drops of water that form these clouds, the crowns are colored blue as close to the Moon, then degrade from yellow to brick red. In the distance, on the edge of the cloud strip, another luminous phenomene is noticeable: these are colourful irisations such as those seen sometimes on some puddles. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud

PIX4671856: Colored crown around the Moon and irizations - Corona around the Moon with irisation - Provoked by the microscopic drops of water that form these clouds, the crowns are colored blue as close to the Moon, then degrade from yellow to brick red. In the distance, on the edge of the cloud strip, another luminous phenomene is noticeable: these are colourful irisations such as those seen sometimes on some puddles. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud / Bridgeman Images

ID: PIX4671856

Colored crown around the Moon and irizations - Corona around the Moon with irisation - Provoked by the microscopic drops of water that form these clouds, the crowns are colored blue as close to the Moon, then degrade from yellow to brick red. In the distance, on the edge of the cloud strip, another luminous phenomene is noticeable: these are colourful irisations such as those seen sometimes on some puddles. In meteorology, a lunar corona is produced by the diffraction of light from the Moon by small water droplets in a cloud

Clouds and sunset of Solei
Clouds and sunset of Solei

PIX4671894: Clouds and sunset of Solei / Bridgeman Images

ID: PIX4671894

Clouds and sunset of Solei

Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.
Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.

TEC4672111: Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95. / Bridgeman Images

ID: TEC4672111

Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.

Crepuscular rays - Crepuscular rays - Crepuscular rays seen on November 6, 2006. Crepuscular rays. November 6 2006
Crepuscular rays - Crepuscular rays - Crepuscular rays seen on November 6, 2006. Crepuscular rays. November 6 2006

PIX4672131: Crepuscular rays - Crepuscular rays - Crepuscular rays seen on November 6, 2006. Crepuscular rays. November 6 2006 / Bridgeman Images

ID: PIX4672131

Crepuscular rays - Crepuscular rays - Crepuscular rays seen on November 6, 2006. Crepuscular rays. November 6 2006

Dawn - Dawn - Micocoulier at sunrise. 30 December 2004. Celtis seen at dawn. December 30 2004
Dawn - Dawn - Micocoulier at sunrise. 30 December 2004. Celtis seen at dawn. December 30 2004

PIX4672224: Dawn - Dawn - Micocoulier at sunrise. 30 December 2004. Celtis seen at dawn. December 30 2004 / Bridgeman Images

ID: PIX4672224

Dawn - Dawn - Micocoulier at sunrise. 30 December 2004. Celtis seen at dawn. December 30 2004

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. 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
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. 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

PIX4671060: 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. 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 / Bridgeman Images

ID: PIX4671060

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. 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

Sunray on the Pyrenees - Sunray on the Pyrenees - Sunray through the clouds seen from the Pic du Midi Observatory. Sun ray between clouds seen from Pic du Midi observatory
Sunray on the Pyrenees - Sunray on the Pyrenees - Sunray through the clouds seen from the Pic du Midi Observatory. Sun ray between clouds seen from Pic du Midi observatory

PIX4671967: Sunray on the Pyrenees - Sunray on the Pyrenees - Sunray through the clouds seen from the Pic du Midi Observatory. Sun ray between clouds seen from Pic du Midi observatory / Bridgeman Images

ID: PIX4671967

Sunray on the Pyrenees - Sunray on the Pyrenees - Sunray through the clouds seen from the Pic du Midi Observatory. Sun ray between clouds seen from Pic du Midi observatory

Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.
Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.

TEC4672100: Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95. / Bridgeman Images

ID: TEC4672100

Les sculptures habitacles d'Andre Bloc (1896-1966) à Meudon (Hauts de Seine). Plastic intervention 1964-1966. Photography 10/06/95.

Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. The parhely is clearly off the halo of 22* radius when the Sun is 21* high. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals
Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. The parhely is clearly off the halo of 22* radius when the Sun is 21* high. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals

PIX4671367: Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. The parhely is clearly off the halo of 22* radius when the Sun is 21* high. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals / Bridgeman Images

ID: PIX4671367

Parhely - Sun dog - Parhelies are optical phenomena due to the interaction of solar light on ice crystals. The parhely is clearly off the halo of 22* radius when the Sun is 21* high. Sundogs appear generally when the sun is low, and the atmosphere is filled with ice crystals forming cirrus clouds; they are caused by the refraction of sunlight passing through ice crystals

Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo
Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo

PIX4671379: Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under angles between 30 and 45* around the antisolar point (at the opposite of the Sun). Then the colors mixe and one can see a white light bow, with sometime blue in the interior and red in the exterior, larger than a rainbo / Bridgeman Images

ID: PIX4671379

Arc de fog - Fogbow - Arc de fog observed in Brittany on 5 May 2006. A haze arc is formed in the way of a rainbow. The light of the Sun is reflected in the water drops of the mist, but unlike raindrops, the mist droplets are much smaller: about a millimetre for the rain versus a few centiemes for the mist. As a result, the diffraction in the mist droplets is preponderant, which results in colour refracting at random angles, between 30 and 45* around the anti-sun point (opposite the Sun). Thus, all colours blend and one sees a white arch of light, sometimes slightly bluish on the inside and red on the outside, wider than a rainbow. Fogbow seen in Brittany on May 5, 2006. A fogbow is forming like a rainbow. The sunlight reflects in the fog droplets, but thoses droplets are much more smaller than the raindrops: about hundredths millimeters for the fog instead of about one millimeter for the rain. Thus, the diffraction in the fog droplets is leading, then the colors are refracted under ang

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center left). Moraines - - accumulations of soil and rock debris - - form along the edges of a glacier as it flows downhill across the landscape (much like a snowplow builds ridges of snow along the roadside). Glaciers flowing downslope through adjacent valleys merge when they encounter each other, and debris entrained along their sides becomes concentrated in the central portion of the new combined ice mass, much as small streams join to form a river.Crevasse fields are also visible in the image. The crevasse - - small, but potentially quite deep fissures - - form as a result of stress between slower - and faster - moving ice within the glacier. Crevasse fields on Tyndall Glacier are most evident near rock promontories extending into the glacier; these rock outcrops cause the ice to slow as it flows around the obstruction
Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center left). Moraines - - accumulations of soil and rock debris - - form along the edges of a glacier as it flows downhill across the landscape (much like a snowplow builds ridges of snow along the roadside). Glaciers flowing downslope through adjacent valleys merge when they encounter each other, and debris entrained along their sides becomes concentrated in the central portion of the new combined ice mass, much as small streams join to form a river.Crevasse fields are also visible in the image. The crevasse - - small, but potentially quite deep fissures - - form as a result of stress between slower - and faster - moving ice within the glacier. Crevasse fields on Tyndall Glacier are most evident near rock promontories extending into the glacier; these rock outcrops cause the ice to slow as it flows around the obstruction

PIX4675989: Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center left). Moraines - - accumulations of soil and rock debris - - form along the edges of a glacier as it flows downhill across the landscape (much like a snowplow builds ridges of snow along the roadside). Glaciers flowing downslope through adjacent valleys merge when they encounter each other, and debris entrained along their sides becomes concentrated in the central portion of the new combined ice mass, much as small streams join to form a river.Crevasse fields are also visible in the image. The crevasse - - small, but potentially quite deep fissures - - form as a result of stress between slower - and faster - moving ice within the glacier. Crevasse fields on Tyndall Glacier are most evident near rock promontories extending into the glacier; these rock outcrops cause the ice to slow as it flows around the obstruction / Bridgeman Images

ID: PIX4675989

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

Ratification of the Treaty of Ardres between King Henry VIII of England (1491-1547)
Ratification of the Treaty of Ardres between King Henry VIII of England (1491-1547)

JLJ4676067: Ratification of the Treaty of Ardres between King Henry VIII of England (1491-1547) / Bridgeman Images

ID: JLJ4676067

Ratification of the Treaty of Ardres between King Henry VIII of England (1491-1547)

Laguna Miniques, Chile - The Miniques volcano dominating the Laguna Miniques. Cerro Miniques is a 5900 meter stratovolcano
Laguna Miniques, Chile - The Miniques volcano dominating the Laguna Miniques. Cerro Miniques is a 5900 meter stratovolcano

PIX4676179: Laguna Miniques, Chile - The Miniques volcano dominating the Laguna Miniques. Cerro Miniques is a 5900 meter stratovolcano / Bridgeman Images

ID: PIX4676179

Laguna Miniques, Chile - The Miniques volcano dominating the Laguna Miniques. Cerro Miniques is a 5900 meter stratovolcano

Student accommodation in Paris 75018.
Student accommodation in Paris 75018.

TEC4676307: Student accommodation in Paris 75018. / Bridgeman Images

ID: TEC4676307

Student accommodation in Paris 75018.

Starry sky above Moais on Easter island - The Clouds of Magellan and the Star Canopus above the Moais of Easter Island. Ahu Tongariki. September 2009. Magellanic Clouds with the bright star Canopus above Moais on Easter island. Ahu Tongariki. September 2009
Starry sky above Moais on Easter island - The Clouds of Magellan and the Star Canopus above the Moais of Easter Island. Ahu Tongariki. September 2009. Magellanic Clouds with the bright star Canopus above Moais on Easter island. Ahu Tongariki. September 2009

PIX4676397: Starry sky above Moais on Easter island - The Clouds of Magellan and the Star Canopus above the Moais of Easter Island. Ahu Tongariki. September 2009. Magellanic Clouds with the bright star Canopus above Moais on Easter island. Ahu Tongariki. September 2009 / Bridgeman Images

ID: PIX4676397

Starry sky above Moais on Easter island - The Clouds of Magellan and the Star Canopus above the Moais of Easter Island. Ahu Tongariki. September 2009. Magellanic Clouds with the bright star Canopus above Moais on Easter island. Ahu Tongariki. September 2009

Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai volcano is an active volcano located in Tanzania in the valley of the Great Rift. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite
Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai volcano is an active volcano located in Tanzania in the valley of the Great Rift. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite

PIX4676439: Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai volcano is an active volcano located in Tanzania in the valley of the Great Rift. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite / Bridgeman Images

ID: PIX4676439

Ol Doinyo Lengai - Volcano Ol Doinyo Lengai - Ol Doinyo Lengai volcano is an active volcano located in Tanzania in the valley of the Great Rift. Ol Doinyo Lengai is the only volcano in the world to emit carbonatite. Volcano Ol Doinyo Lengai is an active volcano located in Tanzania in the great rift valley. It is the only known volcano producing carbonatite

In the lava lake of Erta Ale - In Erta Ale lava lake - Lava lake of Erta Ale. Erta Ale is a shield volcano in Ethiopia located in the Afar Triangle. Erta Ale lava lake. Erta Ale is an active shield volcano located in Ethiopia, in the Afar Triangle
In the lava lake of Erta Ale - In Erta Ale lava lake - Lava lake of Erta Ale. Erta Ale is a shield volcano in Ethiopia located in the Afar Triangle. Erta Ale lava lake. Erta Ale is an active shield volcano located in Ethiopia, in the Afar Triangle

PIX4676522: In the lava lake of Erta Ale - In Erta Ale lava lake - Lava lake of Erta Ale. Erta Ale is a shield volcano in Ethiopia located in the Afar Triangle. Erta Ale lava lake. Erta Ale is an active shield volcano located in Ethiopia, in the Afar Triangle / Bridgeman Images

ID: PIX4676522

In the lava lake of Erta Ale - In Erta Ale lava lake - Lava lake of Erta Ale. Erta Ale is a shield volcano in Ethiopia located in the Afar Triangle. Erta Ale lava lake. Erta Ale is an active shield volcano located in Ethiopia, in the Afar Triangle

Social housing, ZAC Seine Rive Gauche in Paris 75013. Realisation 1993-1997. architects Eric Saunier and Jerome Brunet. Photography 1998.
Social housing, ZAC Seine Rive Gauche in Paris 75013. Realisation 1993-1997. architects Eric Saunier and Jerome Brunet. Photography 1998.

TEC4676788: Social housing, ZAC Seine Rive Gauche in Paris 75013. Realisation 1993-1997. architects Eric Saunier and Jerome Brunet. Photography 1998. / Bridgeman Images

ID: TEC4676788

Social housing, ZAC Seine Rive Gauche in Paris 75013. Realisation 1993-1997. architects Eric Saunier and Jerome Brunet. Photography 1998.

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.
Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

PIX4676925: Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption. / Bridgeman Images

ID: PIX4676925

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

Semeru - Semeru volcano eruption - Semeru volcano eruption in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Volcanic eruption of Semeru in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java
Semeru - Semeru volcano eruption - Semeru volcano eruption in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Volcanic eruption of Semeru in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java

PIX4676989: Semeru - Semeru volcano eruption - Semeru volcano eruption in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Volcanic eruption of Semeru in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java / Bridgeman Images

ID: PIX4676989

Semeru - Semeru volcano eruption - Semeru volcano eruption in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Volcanic eruption of Semeru in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java

Loft a Paris 75020. Photography 1998.
Loft a Paris 75020. Photography 1998.

TEC4676902: Loft a Paris 75020. Photography 1998. / Bridgeman Images

ID: TEC4676902

Loft a Paris 75020. Photography 1998.

Volcanic bomb - Japan - Lava Bomb - Japan - Volcanic bomb measuring 1 metre in diameter. Volcano Aso, January 2010. 1 meter diameter lava bomb. Volcano Aso, January 2010
Volcanic bomb - Japan - Lava Bomb - Japan - Volcanic bomb measuring 1 metre in diameter. Volcano Aso, January 2010. 1 meter diameter lava bomb. Volcano Aso, January 2010

PIX4676914: Volcanic bomb - Japan - Lava Bomb - Japan - Volcanic bomb measuring 1 metre in diameter. Volcano Aso, January 2010. 1 meter diameter lava bomb. Volcano Aso, January 2010 / Bridgeman Images

ID: PIX4676914

Volcanic bomb - Japan - Lava Bomb - Japan - Volcanic bomb measuring 1 metre in diameter. Volcano Aso, January 2010. 1 meter diameter lava bomb. Volcano Aso, January 2010

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.
Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

PIX4676920: Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption. / Bridgeman Images

ID: PIX4676920

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.
Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

PIX4676930: Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption. / Bridgeman Images

ID: PIX4676930

Anak Krakatau volcano eruption - Anak Krakatau volcano - Anak Krakatau volcano eruption in May 2008. This explosive-type active volcano is located in Indonesia on the Pacific belt of fire. The Anak Krakatau (the “son of Krakatoa”) appeared in 1927 on the remains of the terrible explosion of Krakatoa in 1883. Volcanic eruption of Anak Krakatau in May 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. Anak Krakatau, which means child of Kratatau,””” emerged from the sea in 1928 replacing the Krakatau craters destroyed in the 1883 eruption.

Semeru volcanic eruption at night with lighting - Semeru volcanic eruption during the eruption of Semeru volcano in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Lightning during volcanic eruption of Semeru seen at night in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java
Semeru volcanic eruption at night with lighting - Semeru volcanic eruption during the eruption of Semeru volcano in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Lightning during volcanic eruption of Semeru seen at night in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java

PIX4677031: Semeru volcanic eruption at night with lighting - Semeru volcanic eruption during the eruption of Semeru volcano in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Lightning during volcanic eruption of Semeru seen at night in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java / Bridgeman Images

ID: PIX4677031

Semeru volcanic eruption at night with lighting - Semeru volcanic eruption during the eruption of Semeru volcano in June 2008. This explosive active volcano is 3676 metres from the highest point of the island of Java in Indonesia. It's a stratovolcano located on the Pacific belt of fire. Lightning during volcanic eruption of Semeru seen at night in june 2008. This active volcano is located in Indonesia on the Pacific Ring of fire. With an elevation of 3676 meters, this stratovolcano is the tallest mountain on the island of Java

Lava lake of Puu Oo -Kilauea -Hawaii - Puu Oo lava lake -Kilauea -Hawaii - Lava lake in the crater of Puu Oo, an event of the volcano shield Kilauea -Hawaii. Lava lake in Puu Oo crater, an active cone on the shield volcano Kilauea, in Hawaii
Lava lake of Puu Oo -Kilauea -Hawaii - Puu Oo lava lake -Kilauea -Hawaii - Lava lake in the crater of Puu Oo, an event of the volcano shield Kilauea -Hawaii. Lava lake in Puu Oo crater, an active cone on the shield volcano Kilauea, in Hawaii

PIX4677235: Lava lake of Puu Oo -Kilauea -Hawaii - Puu Oo lava lake -Kilauea -Hawaii - Lava lake in the crater of Puu Oo, an event of the volcano shield Kilauea -Hawaii. Lava lake in Puu Oo crater, an active cone on the shield volcano Kilauea, in Hawaii / Bridgeman Images

ID: PIX4677235

Lava lake of Puu Oo -Kilauea -Hawaii - Puu Oo lava lake -Kilauea -Hawaii - Lava lake in the crater of Puu Oo, an event of the volcano shield Kilauea -Hawaii. Lava lake in Puu Oo crater, an active cone on the shield volcano Kilauea, in Hawaii

Volcano Fuego - Guatemala - Volcanic eruption - Volcano Fuego - Guatemala - Ash eruption of Fuego volcano in Guatemala. Ash eruption at volcano Fuego in Guatemala
Volcano Fuego - Guatemala - Volcanic eruption - Volcano Fuego - Guatemala - Ash eruption of Fuego volcano in Guatemala. Ash eruption at volcano Fuego in Guatemala

PIX4677364: Volcano Fuego - Guatemala - Volcanic eruption - Volcano Fuego - Guatemala - Ash eruption of Fuego volcano in Guatemala. Ash eruption at volcano Fuego in Guatemala / Bridgeman Images

ID: PIX4677364

Volcano Fuego - Guatemala - Volcanic eruption - Volcano Fuego - Guatemala - Ash eruption of Fuego volcano in Guatemala. Ash eruption at volcano Fuego in Guatemala

Eruption of the volcano Santa Maria -Guatemala - Volcanic eruption - volcano Santa Maria - Guatemala - eruption of the Santiaguito, the active lava dome of the volcano Santa Maria in Guatemala. Ash eruption at lava dome of Santiaguito, an active part of volcano Santa Maria in Guatemala
Eruption of the volcano Santa Maria -Guatemala - Volcanic eruption - volcano Santa Maria - Guatemala - eruption of the Santiaguito, the active lava dome of the volcano Santa Maria in Guatemala. Ash eruption at lava dome of Santiaguito, an active part of volcano Santa Maria in Guatemala

PIX4677383: Eruption of the volcano Santa Maria -Guatemala - Volcanic eruption - volcano Santa Maria - Guatemala - eruption of the Santiaguito, the active lava dome of the volcano Santa Maria in Guatemala. Ash eruption at lava dome of Santiaguito, an active part of volcano Santa Maria in Guatemala / Bridgeman Images

ID: PIX4677383

Eruption of the volcano Santa Maria -Guatemala - Volcanic eruption - volcano Santa Maria - Guatemala - eruption of the Santiaguito, the active lava dome of the volcano Santa Maria in Guatemala. Ash eruption at lava dome of Santiaguito, an active part of volcano Santa Maria in Guatemala

Lava - Pacaya Volcano - Lava - Volcano Pacaya - Pacay volcano
Lava - Pacaya Volcano - Lava - Volcano Pacaya - Pacay volcano

PIX4677361: Lava - Pacaya Volcano - Lava - Volcano Pacaya - Pacay volcano / Bridgeman Images

ID: PIX4677361

Lava - Pacaya Volcano - Lava - Volcano Pacaya - Pacay volcano

Eruption of the Soufriere-Ile of Montserrat - Soufriere volcanic eruption - Montserrat - Eruption of the volcano of the Soufriere. Montserrat Island. February 2010. February 2010
Eruption of the Soufriere-Ile of Montserrat - Soufriere volcanic eruption - Montserrat - Eruption of the volcano of the Soufriere. Montserrat Island. February 2010. February 2010

PIX4677519: Eruption of the Soufriere-Ile of Montserrat - Soufriere volcanic eruption - Montserrat - Eruption of the volcano of the Soufriere. Montserrat Island. February 2010. February 2010 / Bridgeman Images

ID: PIX4677519

Eruption of the Soufriere-Ile of Montserrat - Soufriere volcanic eruption - Montserrat - Eruption of the volcano of the Soufriere. Montserrat Island. February 2010. February 2010

Lava entry into the OCEAN-kilauea -Hawaii - Lava sea Entry-kilauea -Hawaii - Entering a flow of Pahoehoe lava into the Pacific Ocean. It is a type of fluid basaltic lava characteristic of the volcano shield Kilauea to Hawaii. Pahoehoe (fluid and smooth basaltic lava) sea entry from the shield volcano Kilauea, in Hawaii
Lava entry into the OCEAN-kilauea -Hawaii - Lava sea Entry-kilauea -Hawaii - Entering a flow of Pahoehoe lava into the Pacific Ocean. It is a type of fluid basaltic lava characteristic of the volcano shield Kilauea to Hawaii. Pahoehoe (fluid and smooth basaltic lava) sea entry from the shield volcano Kilauea, in Hawaii

PIX4677264: Lava entry into the OCEAN-kilauea -Hawaii - Lava sea Entry-kilauea -Hawaii - Entering a flow of Pahoehoe lava into the Pacific Ocean. It is a type of fluid basaltic lava characteristic of the volcano shield Kilauea to Hawaii. Pahoehoe (fluid and smooth basaltic lava) sea entry from the shield volcano Kilauea, in Hawaii / Bridgeman Images

ID: PIX4677264

Lava entry into the OCEAN-kilauea -Hawaii - Lava sea Entry-kilauea -Hawaii - Entering a flow of Pahoehoe lava into the Pacific Ocean. It is a type of fluid basaltic lava characteristic of the volcano shield Kilauea to Hawaii. Pahoehoe (fluid and smooth basaltic lava) sea entry from the shield volcano Kilauea, in Hawaii


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