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'High Elevation' Bilder und Clips Suchergebnisse page 91 of 2

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Bilder zu 'High Elevation' gefunden, 107

 
Hubbard Glacier - Alaska - Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672485

Hubbard Glacier - Alaska - Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672485

 
Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

PIX4583494

Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

PIX4583494

 
Hubbard Glacier - Alaska - Wide view of Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America leading to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672493

Hubbard Glacier - Alaska - Wide view of Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America leading to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672493

 
Glacier Hubbard - Alaska - Close up view face of Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America leading to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672500

Glacier Hubbard - Alaska - Close up view face of Hubbard Glacier - Alaska - The Hubbard Glacier is the longest glacier in North America leading to the sea. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672500

 
Savannah Landscape, Chobe National Park, Botwana (photo)

Sergi Reboredo

SRB1202604

Savannah Landscape, Chobe National Park, Botwana (photo)

Sergi Reboredo

SRB1202604

 
Disenchantment Bay - Alaska - Overview of Disenchantment Bay - Alaska - Right, Hubbard Glacier, left Turner Glacier. Overview of Disenchantment Bay, Hubbard Glacier right, Turner/Haenke Glacier left, Wrangell - St. Elias Mountain peaks in background. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672519

Disenchantment Bay - Alaska - Overview of Disenchantment Bay - Alaska - Right, Hubbard Glacier, left Turner Glacier. Overview of Disenchantment Bay, Hubbard Glacier right, Turner/Haenke Glacier left, Wrangell - St. Elias Mountain peaks in background. Hubbard Glacier, the largest tidewater glacier in the world. The Hubbard and Turner/Haenke Glaciers extend out into Disenchantment Bay (discovered and named by Captain Alejandro Malaspina in 1791, who was disappointed to find the inlet was a dead end). The face of Hubbard Glacier extends 6 1/2 miles in length. The towering ice peaks making up the face of the glacier are 400 to 500 feet high! To give some perspective the Wrangell - St. Elias mountain peaks in the background are all between 14,000 and 18,000 feet in elevation, the tallest coastal mountains in the world

R. Gendler

PIX4672519

 
Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the nor

PIX4616037

Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the nor

PIX4616037

 
Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

 
Zusätzliche Genehmigungen
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
A general view, seen from the portico of the chapel, and looking north-east down the tree-lined walk towards the Monument of British Liberty in the background , Gibside Chapel, Whickham, Gateshead, UK, c.1955-80 (b/w photo)

EHT5667963

A general view, seen from the portico of the chapel, and looking north-east down the tree-lined walk towards the Monument of British Liberty in the background , Gibside Chapel, Whickham, Gateshead, UK, c.1955-80 (b/w photo)

EHT5667963

 
La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Brittany, 27 September 2008

Laurent Laveder

PIX4637852

La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Brittany, 27 September 2008

Laurent Laveder

PIX4637852

 
La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer

PIX4632280

La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer

PIX4632280

 
Impact Crater Kara - Kul seen from space - Kara - Kul impact crater, Tajikistan - The 25 km-diameter lake Kara - Kul (or Qarokul) is located at 3900 metres above sea level in Tajikistan's Pamir Mountains. This lake is located in a 45 km wide impact crater formed by the fall of a meteorite 25 million years ago. Image obtained from shuttle Atlantis on May 20, 2000. The mountain lake Kara - Kul, located in eastern Tajikistan, high in the Pamir Mountain Range near the Afghan border is a 25 - kilometer (16 - mile) diameter lake sitting at an elevation of about 4,000 meters (about 12,000 feet) above sea level. Kara - Kul was formed from a meteorite impact approximately 25 million years ago, leaving a crater with a rim diameter of 45 kilometers (28 miles). Islands formed from the central uplift can be seen in the northern and southern parts of the lake. Image taken from the space shuttle Atlantis on May 20, 2000

PIX4630871

Impact Crater Kara - Kul seen from space - Kara - Kul impact crater, Tajikistan - The 25 km-diameter lake Kara - Kul (or Qarokul) is located at 3900 metres above sea level in Tajikistan's Pamir Mountains. This lake is located in a 45 km wide impact crater formed by the fall of a meteorite 25 million years ago. Image obtained from shuttle Atlantis on May 20, 2000. The mountain lake Kara - Kul, located in eastern Tajikistan, high in the Pamir Mountain Range near the Afghan border is a 25 - kilometer (16 - mile) diameter lake sitting at an elevation of about 4,000 meters (about 12,000 feet) above sea level. Kara - Kul was formed from a meteorite impact approximately 25 million years ago, leaving a crater with a rim diameter of 45 kilometers (28 miles). Islands formed from the central uplift can be seen in the northern and southern parts of the lake. Image taken from the space shuttle Atlantis on May 20, 2000

PIX4630871

 
La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne,

Laurent Laveder

PIX4637858

La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne,

Laurent Laveder

PIX4637858

 
Kara impact crater - Kul seen from space - Kara - Kul impact crater - The 25 km diameter lake Kara - Kul (or Qarokul) is located at 3900 metres above sea level in the Pamir Mountains of Tajikistan. This lake is located in a 45 km wide impact crater formed by the fall of a meteorite 25 million years ago. Image obtained from the International Space Station (ISS) on 25 June 2003. The mountain lake Kara - Kul, located in eastern Tajikistan, high in the Pamir Mountain Range near the Afghan border is a 25 - kilometer (16 - mile) diameter lake sitting at an elevation of about 4,000 meters (about 12,000 feet) above sea level. Kara - Kul was formed from a meteorite impact approximately 25 million years ago, leaving a crater with a rim diameter of 45 kilometers (28 miles). Islands formed from the central uplift can be seen in the northern and southern parts of the lake. Image taken from the International Space Station (ISS) on June 25, 2003

PIX4630809

Kara impact crater - Kul seen from space - Kara - Kul impact crater - The 25 km diameter lake Kara - Kul (or Qarokul) is located at 3900 metres above sea level in the Pamir Mountains of Tajikistan. This lake is located in a 45 km wide impact crater formed by the fall of a meteorite 25 million years ago. Image obtained from the International Space Station (ISS) on 25 June 2003. The mountain lake Kara - Kul, located in eastern Tajikistan, high in the Pamir Mountain Range near the Afghan border is a 25 - kilometer (16 - mile) diameter lake sitting at an elevation of about 4,000 meters (about 12,000 feet) above sea level. Kara - Kul was formed from a meteorite impact approximately 25 million years ago, leaving a crater with a rim diameter of 45 kilometers (28 miles). Islands formed from the central uplift can be seen in the northern and southern parts of the lake. Image taken from the International Space Station (ISS) on June 25, 2003

PIX4630809

 
Saturn rings seen by Cassini - Saturn's rings from Cassini - Image obtained by the Cassini probe on January 21, 2007 at a distance of 1.6 million km from the planet. This view in natural colors shows Saturn's ring system. The planet, overexposed on this image, has been deliberately erased from the image but its shadow decouts the rings on the right. Some satellites are visible: Epimethee (at 1 hour), Pandora (at 5 o'clock) and Janus (at 10 o'clock). Mosaic of 27 images. The ring system is composed from closest to Saturn to outermost by ring D, then C, B, the division of Cassini, A with division of Encke, F, G and E. The Cassini spacecraft, flying high above Saturn, captured this view of an alien copper - colored ring world. The overexposed planet has deliberately been removed to show the unlit rings alone, seen from an elevation of 60 degrees. The view is a mosaic of 27 images - - nine separate sets of red, green and blue images - - taken over the course of about 45 minutes, as Cassini

PIX4625026

Saturn rings seen by Cassini - Saturn's rings from Cassini - Image obtained by the Cassini probe on January 21, 2007 at a distance of 1.6 million km from the planet. This view in natural colors shows Saturn's ring system. The planet, overexposed on this image, has been deliberately erased from the image but its shadow decouts the rings on the right. Some satellites are visible: Epimethee (at 1 hour), Pandora (at 5 o'clock) and Janus (at 10 o'clock). Mosaic of 27 images. The ring system is composed from closest to Saturn to outermost by ring D, then C, B, the division of Cassini, A with division of Encke, F, G and E. The Cassini spacecraft, flying high above Saturn, captured this view of an alien copper - colored ring world. The overexposed planet has deliberately been removed to show the unlit rings alone, seen from an elevation of 60 degrees. The view is a mosaic of 27 images - - nine separate sets of red, green and blue images - - taken over the course of about 45 minutes, as Cassini

PIX4625026

 
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Urban Hanlon Broughton (1857-1929)

Birley, Oswald Hornby Joseph (1880-1952)

USB1159931

Urban Hanlon Broughton (1857-1929)

Birley, Oswald Hornby Joseph (1880-1952)

USB1159931

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