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A SuperDARN radar site located in Saskatoon, Canada. The Super Dual Auroral Radar Network (SuperDARN) is an international scientific radar network [1] [2] consisting of 35 [3] high frequency (HF) radars located in both the Northern and Southern Hemispheres.
Canadian Forces Station Dana (CFS Dana) was a military radar station 35 miles east of Saskatoon, Saskatchewan, in the Rural Municipality of Bayne No. 371. RCAF Station Dana (also known as Sagehill) was opened in 1962 as part of the Pinetree Line of NORAD radar stations. The station was later renamed CFS Dana when the military branches were merged.
A new radar, owned and operated by ECCC, has been installed in Blainville (near Montreal) to replace the use of the McGill radar. As well, a new radar will be installed in the Lower Athabasca area. [12] The new radars are the Leonardo METEOR 1700S (formerly marketed by Selex ES) which is fully Doppler and dual polarized: [2] [13]
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On 1 May 1964 radar operations at 57 Squadron were automated by the Semi Automatic Ground Environment (SAGE) system, and the station became a long-range radar site. It would no longer guide interceptors but only look for enemy aircraft, feeding data to the Spokane Air Defense Sector SAGE DC-15 Direction Center of the 25th NORAD Region at Larson ...
Diagram of AN/SPY-3 vertical electronic pencil beam radar conex projections. X band functionality (8 to 12 GHz frequency range) is optimal for minimizing low-altitude propagation effects, narrow beam width for best tracking accuracy, wide frequency bandwidth for effective target discrimination, and the target illumination for SM-2 and Evolved Sea Sparrow Missiles (ESSM).
The Unwin Radar array at Awarua. The Unwin Radar is a scientific radar array at Awarua, near Invercargill, New Zealand. Unwin is part of the Super Dual Auroral Radar Network (SuperDARN), an international radar network for studying the upper atmosphere and ionosphere that operates in the High Frequency (HF) bands between 8 and 22 MHz.
A novel drift scan telescope, which consists of four 100 × 20 meter 5 m focal length cylinders, with an array of 256 dual-polarized radio receivers along the focus. Will map the 21 cm line of neutral hydrogen over the cosmological redshift range of 0.8 to 2.5. Collected its first light in September 2017. [49]