Clark Lake Radio Observatory
USA /
California /
Borrego Springs /
World
/ USA
/ California
/ Borrego Springs
World / United States / California
observatory, abandoned / shut down, interesting place, historic ruins
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Although the observatory, built in 1966, has been removed, the below passage explains what it did while operational:
"A new, fully steerable, decametric array for radio astronomy has been built at the Clark Lake Radio Observatory near Borrego Springs, California. This array is a “T” of 720 conical spiral antennas (teepee-shaped antennas), 3.0 km by 1.8 km. It is capable of operating between 15 and 125 MHz but has best sensitivity in the 25 to 75 MHz range. Both its operating frequency and beam position are adjustable in ∼ ms.
A 1024 channel digital correlator has been built and attached to the array. This permits the simultaneous measurement of the complex visibility functions on 512 interferometer baselines between various portions of the array. After Fourier transformation these visibility data yield a 32 × 32 resolution element picture of the area of sky under observation, with frequency-dependent angular resolution ranging from 20′ to 2.7′ and a sensitivity of 1 Jy per beam. The system is described, and some initial observations are presented."
www.aspbooks.org/a/volumes/article_details/?paper_id=28...
"A new, fully steerable, decametric array for radio astronomy has been built at the Clark Lake Radio Observatory near Borrego Springs, California. This array is a “T” of 720 conical spiral antennas (teepee-shaped antennas), 3.0 km by 1.8 km. It is capable of operating between 15 and 125 MHz but has best sensitivity in the 25 to 75 MHz range. Both its operating frequency and beam position are adjustable in ∼ ms.
A 1024 channel digital correlator has been built and attached to the array. This permits the simultaneous measurement of the complex visibility functions on 512 interferometer baselines between various portions of the array. After Fourier transformation these visibility data yield a 32 × 32 resolution element picture of the area of sky under observation, with frequency-dependent angular resolution ranging from 20′ to 2.7′ and a sensitivity of 1 Jy per beam. The system is described, and some initial observations are presented."
www.aspbooks.org/a/volumes/article_details/?paper_id=28...
Nearby cities:
Coordinates: 33°19'59"N 116°16'49"W
- Mount Palomar Observatory 55 km
- Kitt Peak National Observatory 462 km
- Kitt Peak National Observatory 464 km
- Owens Valley Radio Observatory (OVRO) 472 km
- Anderson Mesa Station 479 km
- McDonald Observatory 1193 km
- Prude Ranch / Texas Star Party 1202 km
- LIGO Hanford Observatory 1489 km
- Dominion Astrophysical Observatory 1793 km
- LIGO Livingston Observatory 2419 km
- Clark Dry Lake 1.2 km
- Borrego Springs, California 11 km
- Camp Ensign Cantonment Area 12 km
- Borrego Spring Resort & Spa 12 km
- Rockhouse Canyon 14 km
- Ram's Hill Golf Club 16 km
- Borrego Valley Manuever Area 17 km
- Truck Haven OHV 22 km
- Coachella Valley 42 km
- Salton Sea 42 km