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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
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
A neonate gray whale calf, born just hours before, still exhbiting embryonic folds in the skin along its side.  This baby gray whale was born in the cold waters of Big Sur, far to the north of the Mexican lagoons of Baja California where most gray whale births take place, Eschrichtius robustus, Monterey
A neonate gray whale calf, born just hours before, still exhbiting embryonic folds in the skin along its side. This baby gray whale was born in the cold waters of Big Sur, far to the north of the Mexican lagoons of Baja California where most gray whale births take place.
Species: Gray whale, Eschrichtius robustus
Location: Monterey, California
Image ID: 01135  
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  
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  
Gray whale, blow, Eschrichtius robustus, Big Sur, California
Gray whale, blow.
Species: Gray whale, Eschrichtius robustus
Location: Big Sur, California
Image ID: 01173  
Big Surf breaks on Children's Pool, harbor seals protected on the beach, La Jolla, California
Big Surf breaks on Children's Pool, harbor seals protected on the beach.
Location: La Jolla, California
Image ID: 30198  
La Jolla Cove only breaks on really big swells.  Giant surf and big waves nail Southern California, December 21, 2005
La Jolla Cove only breaks on really big swells. Giant surf and big waves nail Southern California, December 21, 2005.
Location: La Jolla Cove, California
Image ID: 14813  
La Jolla Cove only breaks on really big swells.  Giant surf and big waves nail Southern California, December 21, 2005
La Jolla Cove only breaks on really big swells. Giant surf and big waves nail Southern California, December 21, 2005.
Location: La Jolla Cove, California
Image ID: 14815  
Salt Creek surf, pretty big day, winter, morning, Laguna Niguel, California
Salt Creek surf, pretty big day, winter, morning.
Location: Salt Creek, Laguna Niguel, California
Image ID: 14851  
Salt Creek surf, pretty big day, winter, morning, Laguna Niguel, California
Salt Creek surf, pretty big day, winter, morning.
Location: Salt Creek, Laguna Niguel, California
Image ID: 14852  
Northern elephant seal,  mother and neonate pup, gulls eating placenta, Mirounga angustirostris, Piedras Blancas, San Simeon, California
Northern elephant seal, mother and neonate pup, gulls eating placenta.
Species: Elephant seal, Mirounga angustirostris
Location: Piedras Blancas, San Simeon, California
Image ID: 00945  
Gray whale, Eschrichtius robustus, Big Sur, California
Gray whale.
Species: Gray whale, Eschrichtius robustus
Location: Big Sur, California
Image ID: 01182  
Gray whale, neonate calf with embryonic folds visible, Eschrichtius robustus, Monterey, California
Gray whale, neonate calf with embryonic folds visible.
Species: Gray whale, Eschrichtius robustus
Location: Monterey, California
Image ID: 01129  
Gray whale, blow, Eschrichtius robustus, Big Sur, California
Gray whale, blow.
Species: Gray whale, Eschrichtius robustus
Location: Big Sur, California
Image ID: 01170  
Gray whale, Eschrichtius robustus, Monterey, California
Gray whale.
Species: Gray whale, Eschrichtius robustus
Location: Monterey, California
Image ID: 01190  
Gray whale, raising fluke to dive, Eschrichtius robustus, Big Sur, California
Gray whale, raising fluke to dive.
Species: Gray whale, Eschrichtius robustus
Location: Big Sur, California
Image ID: 05780  
Gray whale, raising fluke to dive, Eschrichtius robustus, Big Sur, California
Gray whale, raising fluke to dive.
Species: Gray whale, Eschrichtius robustus
Location: Big Sur, California
Image ID: 05781  
Northern elephant seal, sunset.  Scars on neck and chest are from territorial battles with other adult males. Big Sur, Mirounga angustirostris, Gorda
Northern elephant seal, sunset. Scars on neck and chest are from territorial battles with other adult males. Big Sur.
Species: Elephant seal, Mirounga angustirostris
Location: Gorda, Big Sur, California
Image ID: 10037  
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  
Bodyboarders tackle big waves at Oceanside Pier, sunset. Giant surf and big waves nail Southern California, December 21, 2005
Bodyboarders tackle big waves at Oceanside Pier, sunset. Giant surf and big waves nail Southern California, December 21, 2005.
Location: Oceanside Pier, California
Image ID: 14843  
Gray whale, Eschrichtius robustus, Monterey, California
Gray whale.
Species: Gray whale, Eschrichtius robustus
Location: Monterey, California
Image ID: 01178  
Gray whale, Eschrichtius robustus, Monterey, California
Gray whale.
Species: Gray whale, Eschrichtius robustus
Location: Monterey, California
Image ID: 01188  
Northern elephant seal, pup, Mirounga angustirostris, Piedras Blancas, San Simeon, California
Northern elephant seal, pup.
Species: Elephant seal, Mirounga angustirostris
Location: Piedras Blancas, San Simeon, California
Image ID: 00948  
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  
An enormous red cedar tree has been hit by lightning and burn through its core all the way to the ground, and still survives!  The Big Tree Trail on Meares Island, temperate rainforest home to huge red cedar and spruce trees, Meares Island Big Trees Trail, Tofino, British Columbia, Canada
An enormous red cedar tree has been hit by lightning and burn through its core all the way to the ground, and still survives! The Big Tree Trail on Meares Island, temperate rainforest home to huge red cedar and spruce trees.
Location: Meares Island Big Trees Trail, Tofino, British Columbia, Canada
Image ID: 21063