Radio Photo


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The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars Radio telescope antenna, part of the Very Long Baseline Array (VLBA). The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO). These ten radio antennas work together as an array that forms the longest system in the world that uses very long baseline interferometry, Big Pine, California This photo is the top of a stack of similar images, click to see them all. The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars This photo is the top of a stack of similar images, click to see them all.
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Radio Photo.
Image ID: 28796  
Location: Big Pine, California, USA
Pano dimensions: 7153 x 11978
 
Radio telescope antenna, part of the Very Long Baseline Array (VLBA). The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO). These ten radio antennas work together as an array that forms the longest system in the world that uses very long baseline interferometry. Radio Picture.
Image ID: 28787  
Location: Big Pine, California, USA
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Stock Photography of Radio.
Image ID: 28793  
Location: Big Pine, California, USA
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Photograph of Radio.
Image ID: 28788  
Location: Big Pine, California, USA
Pano dimensions: 5954 x 12875
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Radio Photos.
Image ID: 28790  
Location: Big Pine, California, USA
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Radio Image.
Image ID: 28789  
Location: Big Pine, California, USA
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Professional stock photos of Radio.
Image ID: 28791  
Location: Big Pine, California, USA
 
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars Radio City Music Hall, neon lights, night, New York City Radio City Music Hall, neon lights, night, New York City
The OVRO 40 meter Telescope, part of the Owens Valley Radio Observatory located near Big Pine, California, USA. The telescope is used to conduct interferometric observations along with the other telescopes in the observatory, as a Very Long Baseline Interferometry (VLBI) station and as a single dish instrument. Its main focus today is on the monitoring of blazars. Pictures of Radio.
Image ID: 28794  
Location: Big Pine, California, USA
 
Radio City Music Hall, neon lights, night. Radio Photo.
Image ID: 11174  
Location: Radio City Music Hall, New York City, USA
 
Radio City Music Hall, neon lights, night. Radio Picture.
Image ID: 11176  
Location: Radio City Music Hall, New York City, USA
 
Radio City Music Hall, neon lights, night, New York City Radio City Music Hall, neon lights, night, New York City Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night. Stock Photography of Radio.
Image ID: 11173  
Location: Radio City Music Hall, New York City, USA
 
Radio City Music Hall, neon lights, night. Photograph of Radio.
Image ID: 11175  
Location: Radio City Music Hall, New York City, USA
 
Radio City Music Hall, neon lights, night. Radio Photos.
Image ID: 11177  
Location: Radio City Music Hall, New York City, USA
 
Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming Antenna towers atop San Miguel Mountain, aerial view.  San Miguel Mountain reaches an altitude of 2565 feet, and hosts commercial radio and television antennas for the San Diego region, east of downtown San Diego Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Radio Image.
Image ID: 13093  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 
Antenna towers atop San Miguel Mountain, aerial view. San Miguel Mountain reaches an altitude of 2565 feet, and hosts commercial radio and television antennas for the San Diego region, east of downtown San Diego. Professional stock photos of Radio.
Image ID: 22141  
Location: San Miguel Mountain, San Diego, California, USA
 
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Pictures of Radio.
Image ID: 13091  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 
Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Radio Photo.
Image ID: 13092  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Radio Picture.
Image ID: 13094  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Stock Photography of Radio.
Image ID: 13095  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 
Coyote, Lamar Valley.  This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear, Canis latrans, Yellowstone National Park, Wyoming
Coyote, Lamar Valley. This coyote bears not only a radio tracking collar, so researchers can follow its daily movements, but also a small green tag on its left ear. Photograph of Radio.
Image ID: 13096  
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming, USA
 


Natural History Photography Blog posts (14) related to Radio



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Categories Appearing Among These Images:
Animal  >  Mammal  >  Coyote
Gallery  >  California
Gallery  >  Landscape Astrophotography
Gallery  >  Milky Way
Gallery  >  New Work September 2013
Gallery  >  Night
Gallery  >  Panorama
Gallery  >  Travel
Location  >  Protected Threatened and Significant Places  >  National Parks  >  Yellowstone National Park (Wyoming)
Location  >  Protected Threatened and Significant Places  >  World Heritage Sites  >  Yellowstone National Park (USA)
Location  >  USA  >  California  >  Big Pine
Location  >  USA  >  New York City
Location  >  USA  >  Wyoming  >  Yellowstone National Park
Subject  >  Technique  >  Landscape Astrophotography
Subject  >  Technique  >  Night / Time Exposure
Subject  >  Technique  >  Panoramic Photo

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Canis latrans

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Updated: November 19, 2019