View allAll Photos Tagged arrays!!!
April 18th - I was out for a walk again. Nice weather and the wind of the previous outing wasn't blowing everything around. I'll be posting a new blog entry today. In the meantime, if anyone should ask, I was not photographing a government communication array when I took this shot. I was photographing the crow that was sitting on top of the dish!
Post of the outing with 30+ photos: Am I on the right track?
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I love this hulking yet elegant edifice located at the southwest corner of Adelaide & Peter streets ... as seen from the northwest corner's rooftop patio ...
- Toronto, Canada
Taken with Asahi Pentax S1a Super Takumar 1:2 / 55 on Fuji Superia ISO 200
Comprises twenty-eight 25-meter radio telescopes deployed in a Y-shaped array and all the equipment, instrumentation, and computing power to function as an interferometer. Each of the massive telescopes is mounted on double parallel railroad tracks, so the radius and density of the array can be transformed to adjust the balance between its angular resolution and its surface brightness sensitivity.
Astronomers using the VLA have made key observations of black holes and protoplanetary disks around young stars, discovered magnetic filaments and traced complex gas motions at the Milky Way's center, probed the Universe's cosmological parameters, and provided new knowledge about the physical mechanisms that produce radio emission.
The Combined Array for Research in Millimeter-wave Astronomy (CARMA) was an astronomical instrument comprising 23 radio telescopes. These telescopes formed an astronomical interferometer where all the signals are combined in a purpose-built computer (a correlator) to produce high-resolution astronomical images. The telescopes ceased operation in April 2015 and were relocated to the Owens Valley Radio Observatory for storage.
The Combined Array for Research in Millimeter-wave Astronomy (CARMA) was an astronomical instrument comprising 23 radio telescopes. These telescopes formed an astronomical interferometer where all the signals are combined in a purpose-built computer (a correlator) to produce high-resolution astronomical images. The telescopes ceased operation in April 2015 and were relocated to the Owens Valley Radio Observatory for storage.