Radio Photos

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.
Location: Big Pine, California
Image ID: 28796  
Panorama 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, Big Pine, California
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.
Location: Big Pine, California
Image ID: 28787  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36023  
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.
Location: Big Pine, California
Image ID: 28788  
Panorama 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.
Location: Big Pine, California
Image ID: 28793  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36021  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36024  
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.
Location: Big Pine, California
Image ID: 28790  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36019  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36020  
Radio Tower Rock at Sunset, Page, Arizona
Radio Tower Rock at Sunset, Page, Arizona.
Location: Page, Arizona
Image ID: 36022  
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.
Location: Big Pine, California
Image ID: 28789  
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.
Location: Big Pine, California
Image ID: 28791  
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.
Location: Big Pine, California
Image ID: 28792  
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.
Location: Big Pine, California
Image ID: 28794  
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
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.
Location: Big Pine, California
Image ID: 28795  
Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night.
Location: Radio City Music Hall, New York City
Image ID: 11174  
Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night.
Location: Radio City Music Hall, New York City
Image ID: 11176  
Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night.
Location: Radio City Music Hall, New York City
Image ID: 11173  
Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night.
Location: Radio City Music Hall, New York City
Image ID: 11175  
Radio City Music Hall, neon lights, night, New York City
Radio City Music Hall, neon lights, night.
Location: Radio City Music Hall, New York City
Image ID: 11177  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13093  
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
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.
Location: San Miguel Mountain, San Diego, California
Image ID: 22141  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13091  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13092  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13094  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13095  
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.
Species: Coyote, Canis latrans
Location: Lamar Valley, Yellowstone National Park, Wyoming
Image ID: 13096  
All photographs copyright © Phillip Colla / Oceanlight.com, all rights reserved worldwide.