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August 30, 2018 - NREL scientist Jordan Macknick and Jake Janski, from Minnesota Native Landscapes survey
a pollinator test plot ( planted) underneath the PV array
at the Chisago (spelled correctly) Solar Site, part of the Aurora Solar Project in Minnesota. NREL scientist Jordan Macknick is researching the economical and ecological impact of pollinator plants planted underneath the PV array
. (Photo by Dennis Schroeder / NREL)
is one of my favorite places in New Mexico. I was there several times and I'm fascinated by this place in the middle of nowhere.
The Very Large Array (VLA) is a radio astronomy observatory located on the Plains of San Agustin, between the towns of Magdalena and Datil, some fifty miles (80 km) west of Socorro, New Mexico, USA. U.S. Route 60 passes through the complex, which is adjacent to the Boy Scout Double H High Adventure Base. The VLA stands at an elevation of 6970 ft (2124 m) above sea level. It is a component of the National Radio Astronomy Observatory (NRAO).
ist einer meiner Lieblingsorte in New Mexico. Ich war mehrere Male dort und ich bin fasziniert von diesem Ort mitten im Nichts.
Das Very Large Array (VLA) ist ein Interferometer für astronomische Beobachtungen im Radiobereich. Die Anlage befindet sich auf der Ebene von San Agustin zwischen den Städten Magdalena und Datil in New Mexico in den Vereinigten Staaten, etwa 80 Kilometer westlich von Socorro. Das Teleskop befindet sich auf 2.124 m ü. NN und ist Teil der amerikanischen National Radio Astronomy Observatory.
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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.
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.