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41223 Search Results for The Graphic

Russia / Soviet Union: 'Productive Propaganda', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'Productive Propaganda', Vladimir Lebedev (1891-1967), c. 1920

PFH2642408: Russia / Soviet Union: 'Productive Propaganda', Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Russia / Soviet Union: A British ship in St Petersburg Harbour, Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: A British ship in St Petersburg Harbour, Vladimir Lebedev (1891-1967), c. 1920

PFH2642430: Russia / Soviet Union: A British ship in St Petersburg Harbour, Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Study for 'Her First Born, Horsham Churchyard (Funeral of the First Born)', 1874 (w/c on paper)
Study for 'Her First Born, Horsham Churchyard (Funeral of the First Born)', 1874 (w/c on paper)

MAA2956906: Study for 'Her First Born, Horsham Churchyard (Funeral of the First Born)', 1874 (w/c on paper), Holl, Frank (1845-88) / Bridgeman Images

Russia / Soviet Union: 'One Must Work, the Rifle is Right Here', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'One Must Work, the Rifle is Right Here', Vladimir Lebedev (1891-1967), c. 1920

PFH2642414: Russia / Soviet Union: 'One Must Work, the Rifle is Right Here', Vladimir Lebedev (1891-1967), c. 1920, Lebedev, Vladimir Vasilevic (1891-1967) / Bridgeman Images

Russia / Soviet Union: 'Against White Militarism', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'Against White Militarism', Vladimir Lebedev (1891-1967), c. 1920

PFH2642415: Russia / Soviet Union: 'Against White Militarism', Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Russia / Soviet Union: 'A Bourgeois Tearing His Hair Because of the Second Meeting of the International Congress', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'A Bourgeois Tearing His Hair Because of the Second Meeting of the International Congress', Vladimir Lebedev (1891-1967), c. 1920

PFH2642419: Russia / Soviet Union: 'A Bourgeois Tearing His Hair Because of the Second Meeting of the International Congress', Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Russia / Soviet Union: 'A Woman Worker', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'A Woman Worker', Vladimir Lebedev (1891-1967), c. 1920

PFH2642426: Russia / Soviet Union: 'A Woman Worker', Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Queen Victoria at the Tomb of Napoleon, 24 August 1855
Queen Victoria at the Tomb of Napoleon, 24 August 1855

HRP5246078: Queen Victoria at the Tomb of Napoleon, 24 August 1855 / Bridgeman Images

Russia / Soviet Union: 'Workers Must Unionize', c.1920 (litho)
Russia / Soviet Union: 'Workers Must Unionize', c.1920 (litho)

PFH2642416: Russia / Soviet Union: 'Workers Must Unionize', c.1920 (litho), Lebedev, Vladimir Vasilevic (1891-1967) / Bridgeman Images

Russia / Soviet Union: 'A Worker Controlling Nationalised Enterprises', Vladimir Lebedev (1891-1967), c. 1920
Russia / Soviet Union: 'A Worker Controlling Nationalised Enterprises', Vladimir Lebedev (1891-1967), c. 1920

PFH2642418: Russia / Soviet Union: 'A Worker Controlling Nationalised Enterprises', Vladimir Lebedev (1891-1967), c. 1920 / Bridgeman Images

Advertisement for Hungary as tourist destination
Advertisement for Hungary as tourist destination

XLF3784814: Advertisement for Hungary as tourist destination / Bridgeman Images

View of debris in orbit around the Earth - Graphic computer of objects around the earth - View of debris in low orbit and geostationary orbit (35,785 km) around the Earth, from then a genere point above the north pole. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. This image is generated from a vantage point above the north pole, showing the concentrations of objects in Low Earth Orbit and in the geosynchronous region. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions
View of debris in orbit around the Earth - Graphic computer of objects around the earth - View of debris in low orbit and geostationary orbit (35,785 km) around the Earth, from then a genere point above the north pole. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. This image is generated from a vantage point above the north pole, showing the concentrations of objects in Low Earth Orbit and in the geosynchronous region. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions

PIX4642723: View of debris in orbit around the Earth - Graphic computer of objects around the earth - View of debris in low orbit and geostationary orbit (35,785 km) around the Earth, from then a genere point above the north pole. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. This image is generated from a vantage point above the north pole, showing the concentrations of objects in Low Earth Orbit and in the geosynchronous region. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions / Bridgeman Images

Graphic computer of objects around the earth - View of debris in geostationary orbit (35,785 km) around the Earth. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. The GEO images are images generated from a distant oblique vantage point to provide a good view of the object population in the geosynchronous region (around 35,785 km altitude). Note the larger population of objects over the northern hemisphere is due mostly to Russian objects in high - inclination, high - eccentricity orbits. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions
Graphic computer of objects around the earth - View of debris in geostationary orbit (35,785 km) around the Earth. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. The GEO images are images generated from a distant oblique vantage point to provide a good view of the object population in the geosynchronous region (around 35,785 km altitude). Note the larger population of objects over the northern hemisphere is due mostly to Russian objects in high - inclination, high - eccentricity orbits. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions

PIX4642695: Graphic computer of objects around the earth - View of debris in geostationary orbit (35,785 km) around the Earth. Approximately 11,000 objects over 10 cm have been identified. Most of these debris is in low orbit. The number of debris between 10 cm and 1 cm in diameter, greater than 100,000; particles less than 1 cm must exceed 10 million. The GEO images are images generated from a distant oblique vantage point to provide a good view of the object population in the geosynchronous region (around 35,785 km altitude). Note the larger population of objects over the northern hemisphere is due mostly to Russian objects in high - inclination, high - eccentricity orbits. Approximately 11,000 objects larger than 10 cm are known to exist. The estimated population of particles between 1 and 10 cm in diameter is greater than 100,000. The number of particles smaller than 1 cm probably exceeds tens of millions / Bridgeman Images

Seville, 1914 (litho)
Seville, 1914 (litho)

LBI6340713: Seville, 1914 (litho), Steiner-Prag, Hugo (1880-1945) / Bridgeman Images

The Attack on Cronje’s Force at Vedute Drift near Paardeberg, 1900 (oil on canvas)
The Attack on Cronje’s Force at Vedute Drift near Paardeberg, 1900 (oil on canvas)

NAM5919926: The Attack on Cronje’s Force at Vedute Drift near Paardeberg, 1900 (oil on canvas), Giles, Godfrey Douglas (1857-1941) / Bridgeman Images

LLoyds Bank, Baker Street, September 1971
LLoyds Bank, Baker Street, September 1971

MPX5141360: LLoyds Bank, Baker Street, September 1971 / Bridgeman Images

Patient Heroes, a Royal Horse Artillery Gun Team in action, 1882 circa (oil on canvas)
Patient Heroes, a Royal Horse Artillery Gun Team in action, 1882 circa (oil on canvas)

NAM5925037: Patient Heroes, a Royal Horse Artillery Gun Team in action, 1882 circa (oil on canvas), Butler, Lady (Elizabeth Southerden Thompson) (1846-1933) / Bridgeman Images

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The color of the Martian surface and ice was estimated from MRO HiRise color images of other Martian craters and the polar ice caps. The buried ice in these craters as measured by SHARAD is ~ 250 meter thick on the upper crater and ~ 300 and 450 meters on the middle and lower levels respectively. Each image is 20 km (12.8 mi.) across and extends to 50 km (32 mi) in the distance. Recent measurements from the Mars Reconnaissance Orbiter SHARAD radar sounder have detected large amounts of water ice in such deposits over widespread areas, arguing for the flow of glacial - like structures on Mars in the relatively recent geologic past. This suggests that snow and ice accumulated on higher topography, flowed downhill and is now protected from sublimation by a layer of rock debris and dust. Furrows and ridges on the surface were caused by deforming ice
Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The color of the Martian surface and ice was estimated from MRO HiRise color images of other Martian craters and the polar ice caps. The buried ice in these craters as measured by SHARAD is ~ 250 meter thick on the upper crater and ~ 300 and 450 meters on the middle and lower levels respectively. Each image is 20 km (12.8 mi.) across and extends to 50 km (32 mi) in the distance. Recent measurements from the Mars Reconnaissance Orbiter SHARAD radar sounder have detected large amounts of water ice in such deposits over widespread areas, arguing for the flow of glacial - like structures on Mars in the relatively recent geologic past. This suggests that snow and ice accumulated on higher topography, flowed downhill and is now protected from sublimation by a layer of rock debris and dust. Furrows and ridges on the surface were caused by deforming ice

PIX4616544: Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The color of the Martian surface and ice was estimated from MRO HiRise color images of other Martian craters and the polar ice caps. The buried ice in these craters as measured by SHARAD is ~ 250 meter thick on the upper crater and ~ 300 and 450 meters on the middle and lower levels respectively. Each image is 20 km (12.8 mi.) across and extends to 50 km (32 mi) in the distance. Recent measurements from the Mars Reconnaissance Orbiter SHARAD radar sounder have detected large amounts of water ice in such deposits over widespread areas, arguing for the flow of glacial - like structures on Mars in the relatively recent geologic past. This suggests that snow and ice accumulated on higher topography, flowed downhill and is now protected from sublimation by a layer of rock debris and dust. Furrows and ridges on the surface were caused by deforming ice / Bridgeman Images

Muscovite ambassadors to the Empire Diete has rawed, July 18, 1576, 1576-1606 (watercolour on paper)
Muscovite ambassadors to the Empire Diete has rawed, July 18, 1576, 1576-1606 (watercolour on paper)

FIA5409565: Muscovite ambassadors to the Empire Diete has rawed, July 18, 1576, 1576-1606 (watercolour on paper), Unknown Artist, (17th century) / Bridgeman Images

Christ and his disciples in the Garden of Gethsemane, c.1634 (watercolour on paper)
Christ and his disciples in the Garden of Gethsemane, c.1634 (watercolour on paper)

FIA5409605: Christ and his disciples in the Garden of Gethsemane, c.1634 (watercolour on paper), Rembrandt Harmensz. van Rijn (1606-69) / Bridgeman Images

Advertising Poster For The Glass And, c.1921-23 (chromolitho)
Advertising Poster For The Glass And, c.1921-23 (chromolitho)

FIA5403503: Advertising Poster For The Glass And, c.1921-23 (chromolitho), Anonymous / Bridgeman Images

In front of the mirror - Before the Mirror, 1913 (gouache on paper)
In front of the mirror - Before the Mirror, 1913 (gouache on paper)

FIA5404963: In front of the mirror - Before the Mirror, 1913 (gouache on paper), Schiele, Egon (1890-1918) / Bridgeman Images

Poster for the theatre play The flea by E. Zamyatin, 1925 (lithograph)
Poster for the theatre play The flea by E. Zamyatin, 1925 (lithograph)

FIA5405425: Poster for the theatre play The flea by E. Zamyatin, 1925 (lithograph), Kustodiev, Boris Mikhailovich (1878-1927) / Bridgeman Images

The Third Partition Of Poland, 1795 (etching, watercolour)
The Third Partition Of Poland, 1795 (etching, watercolour)

FIA5405757: The Third Partition Of Poland, 1795 (etching, watercolour), Thomson, John (1778-1840) / Bridgeman Images

Movie Poster City Lights (the Lights of the City) By Charlie Chaplin, 1936 (colour lithograph)
Movie Poster City Lights (the Lights of the City) By Charlie Chaplin, 1936 (colour lithograph)

FIA5405438: Movie Poster City Lights (the Lights of the City) By Charlie Chaplin, 1936 (colour lithograph), Vasilyev, Anatoli (1917-1994) / Bridgeman Images

Ladies Fashion, 1840s (watercolour on paper)
Ladies Fashion, 1840s (watercolour on paper)

FIA5410058: Ladies Fashion, 1840s (watercolour on paper), Sadovnikov, Vasili Semenovich (1800-79) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409433: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409451: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409439: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409448: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409449: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Before A Tavern, 1842-45 (lithograph, watercolour)
Before A Tavern, 1842-45 (lithograph, watercolour)

FIA5405772: Before A Tavern, 1842-45 (lithograph, watercolour), Zhukovsky, Rudolf Kasimirovich (1814-1886) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409441: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409431: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)
Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph)

FIA5409443: Equestrian Portrait of Nicholas II of Russia, 1896 (colour lithograph), Bakmanson, Hugo Karlovich (1860-1953) / Bridgeman Images

Set design for the opera ernani, 19th century (watercolour on paper)
Set design for the opera ernani, 19th century (watercolour on paper)

FIA5407275: Set design for the opera ernani, 19th century (watercolour on paper), Conti, M. (1810-1886) / Bridgeman Images


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