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Photographs from 'Alex-Tudorica' found, 117

 
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

Alex Tudorica

PIX4671636

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

Alex Tudorica

PIX4671636

 
Raufarholshellir cave - Iceland - Raufarhollshellir cellar - Exploration of lava tunnels. April 2016. Inside the lava tubes of Raufarhollshellir cave, South Iceland

Alex Tudorica

PIX4666417

Raufarholshellir cave - Iceland - Raufarhollshellir cellar - Exploration of lava tunnels. April 2016. Inside the lava tubes of Raufarhollshellir cave, South Iceland

Alex Tudorica

PIX4666417

 
Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. Milky way above Cerro Tololo observatory, Chile

Alex Tudorica

PIX4652865

Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. Milky way above Cerro Tololo observatory, Chile

Alex Tudorica

PIX4652865

 
Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657504

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657504

 
Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Alex Tudorica

PIX4657511

Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Alex Tudorica

PIX4657511

 
La Palma Observatory - La Palma observatory - The Roque de Los Muchachos Observatory is located at the top of the island of La Palma, in the Spanish Canary Islands. At 2400 m above sea level, this European Boreal Observatory is one of the largest astronomical centres in the world. In the foreground on the right, the 1.2m telescope Mercator Roque de Los Muchachos observatory is located at the top of La Palma island, in Canary islands. This is one of the largest astronomical centre in the world. Foreground is the 1.2 meter telescope Mercator

Alex Tudorica

PIX4654387

La Palma Observatory - La Palma observatory - The Roque de Los Muchachos Observatory is located at the top of the island of La Palma, in the Spanish Canary Islands. At 2400 m above sea level, this European Boreal Observatory is one of the largest astronomical centres in the world. In the foreground on the right, the 1.2m telescope Mercator Roque de Los Muchachos observatory is located at the top of La Palma island, in Canary islands. This is one of the largest astronomical centre in the world. Foreground is the 1.2 meter telescope Mercator

Alex Tudorica

PIX4654387

 
La Palma Observatory - La Palma observatory - The Roque de Los Muchachos Observatory is located at the top of the island of La Palma, in the Spanish Canary Islands. At 2400 m above sea level, this European Boreal Observatory is one of the largest astronomical centres in the world. In the foreground the 1.2m telescope Mercator Roque de Los Muchachos observatory is located at the top of La Palma island, in Canary islands. This is one of the largest astronomical centre in the world. Foreground is the 1.2 meter telescope Mercator

Alex Tudorica

PIX4654388

La Palma Observatory - La Palma observatory - The Roque de Los Muchachos Observatory is located at the top of the island of La Palma, in the Spanish Canary Islands. At 2400 m above sea level, this European Boreal Observatory is one of the largest astronomical centres in the world. In the foreground the 1.2m telescope Mercator Roque de Los Muchachos observatory is located at the top of La Palma island, in Canary islands. This is one of the largest astronomical centre in the world. Foreground is the 1.2 meter telescope Mercator

Alex Tudorica

PIX4654388

 
La Palma Observatory: Gamma ray telescope MAGIC - La Palma Observatory: The MAGIC Gamma ray telescope - The Major Atmospheric Gamma - ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC - I is a telescope of 17 meters in diameter. MAGIC - II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). MAGIC (Major Atmospheric Gamma - ray Imaging Cherenkov Telescope) is a Imaging Atmospheric Cherenkov telescope situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. It detects particle showers released by cosmic gamma - rays, using the Cherenkov radiation. With a diameter of 17 meters for the reflecting surface, it is the largest in the world. A second MAGIC telescope (MAGIC 2) at a distance of 85 m from the first one has started taking data in July 2009

Alex Tudorica

PIX4654526

La Palma Observatory: Gamma ray telescope MAGIC - La Palma Observatory: The MAGIC Gamma ray telescope - The Major Atmospheric Gamma - ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC - I is a telescope of 17 meters in diameter. MAGIC - II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). MAGIC (Major Atmospheric Gamma - ray Imaging Cherenkov Telescope) is a Imaging Atmospheric Cherenkov telescope situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. It detects particle showers released by cosmic gamma - rays, using the Cherenkov radiation. With a diameter of 17 meters for the reflecting surface, it is the largest in the world. A second MAGIC telescope (MAGIC 2) at a distance of 85 m from the first one has started taking data in July 2009

Alex Tudorica

PIX4654526

 
La Palma Observatory: Gamma ray telescope MAGIC - La Palma Observatory: The MAGIC Gamma ray telescope - The Major Atmospheric Gamma - ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC - II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). MAGIC (Major Atmospheric Gamma - ray Imaging Cherenkov Telescope) is a Imaging Atmospheric Cherenkov telescope situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. It detects particle showers released by cosmic gamma - rays, using the Cherenkov radiation. With a diameter of 17 meters for the reflecting surface, it is the largest in the world. Here is the second MAGIC telescope (MAGIC 2) at a distance of 85 m from the first one

Alex Tudorica

PIX4654531

La Palma Observatory: Gamma ray telescope MAGIC - La Palma Observatory: The MAGIC Gamma ray telescope - The Major Atmospheric Gamma - ray Imaging Cherenkov Telescope (MAGIC telescope) is a telescope located at the Roque de los Muchachos de La Palma, in the Canary Islands. MAGIC - II is a second telescope of 17 m in diameter located 85 meters from the first telescope (in operation since April 2009). MAGIC (Major Atmospheric Gamma - ray Imaging Cherenkov Telescope) is a Imaging Atmospheric Cherenkov telescope situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. It detects particle showers released by cosmic gamma - rays, using the Cherenkov radiation. With a diameter of 17 meters for the reflecting surface, it is the largest in the world. Here is the second MAGIC telescope (MAGIC 2) at a distance of 85 m from the first one

Alex Tudorica

PIX4654531

 
Telescope geant Grantecan - La Palma Observatory - Grantecan - La Palma observatory - The Grantecan telescope (Gran Telescopio Canarias) is the largest telescope in the world (2008). Its hexagonal mirror measures 10.4 m in diameter. It is located at 2400 m above sea level, at the Roque de Los Muchachos Observatory, located at the top of the island of La Palma, in the Spanish archipelago of the Canary Islands. The Gran Telescopio Canarias (GTC), called GranteCAN, is a 10.4 m reflecting telescope and is undertaking commissioning observations at the Observatorio del Roque de los Muchachos on the island of La Palma, Spain

Alex Tudorica

PIX4654541

Telescope geant Grantecan - La Palma Observatory - Grantecan - La Palma observatory - The Grantecan telescope (Gran Telescopio Canarias) is the largest telescope in the world (2008). Its hexagonal mirror measures 10.4 m in diameter. It is located at 2400 m above sea level, at the Roque de Los Muchachos Observatory, located at the top of the island of La Palma, in the Spanish archipelago of the Canary Islands. The Gran Telescopio Canarias (GTC), called GranteCAN, is a 10.4 m reflecting telescope and is undertaking commissioning observations at the Observatorio del Roque de los Muchachos on the island of La Palma, Spain

Alex Tudorica

PIX4654541

 
Lujiazui - Shanghai: The skyscrapers of the financial and commercial area of Lujiazui in Pudong District. 10 December 2016. Lujiazui District. December 10 2016

Alex Tudorica

PIX4660034

Lujiazui - Shanghai: The skyscrapers of the financial and commercial area of Lujiazui in Pudong District. 10 December 2016. Lujiazui District. December 10 2016

Alex Tudorica

PIX4660034

 
Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Alex Tudorica

PIX4660042

Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Alex Tudorica

PIX4660042

 
Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Alex Tudorica

PIX4660054

Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Alex Tudorica

PIX4660054

 
Halo and Light Column- Ice halos near Zeel am See, Austria - A light column is created by the reflection of a light source on the horizontal faces of ice crystals. So it takes a fairly stable atmosphere to keep these crystals parallel to the horizon. Lunar halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. A paraselene consists of light spots located on the left and right at the height of the Moon. Austria, January 2016. A light pillar is created by the reflection of light on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

Alex Tudorica

PIX4671758

Halo and Light Column- Ice halos near Zeel am See, Austria - A light column is created by the reflection of a light source on the horizontal faces of ice crystals. So it takes a fairly stable atmosphere to keep these crystals parallel to the horizon. Lunar halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. A paraselene consists of light spots located on the left and right at the height of the Moon. Austria, January 2016. A light pillar is created by the reflection of light on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

Alex Tudorica

PIX4671758

 
Stars on the Matterhorn - Photographic pose on the star sky above the Matterhorn. Long exposure photograph on starry sky above Matterhorn

Alex Tudorica

PIX4624263

Stars on the Matterhorn - Photographic pose on the star sky above the Matterhorn. Long exposure photograph on starry sky above Matterhorn

Alex Tudorica

PIX4624263

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