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In April 2007, a rotational lightcurve Wachmann was obtained at the U.S. Sandia View Observatory in New Mexico . Lightcurve analysis gave a well-defined rotation period of 3.314 ± 0.001 hours with a brightness variation of 0.40 magnitude ( U=3 ).
Sandia Crest, also known locally as Sandia Peak or simply as the Crest, [2] is a mountain ridge that, at 10,679 feet (3,255 m), is the highpoint of the Sandia–Manzano Mountains, and is located in the Sandia Mountains of Bernalillo County, New Mexico, United States. Instead of a true summit or topographic peak, this range climbs to a long ...
One of Sandia's first permanent buildings (Building 800) was completed in 1949. Sandia National Laboratories' roots go back to World War II and the Manhattan Project.Prior to the United States formally entering the war, the U.S. Army leased land near an Albuquerque, New Mexico airport known as Oxnard Field to service transient Army and U.S. Navy aircraft.
The telescope is in Sardinia, 35 kilometres (22 mi) north of Cagliari, [1] and is the largest [2] of a set of three telescopes operated by INAF, along with telescopes at the Medicina Radio Observatory and the Noto Radio Observatory. It operates as a stand-alone instrument and as part of global networks of telescopes.
Starfire Optical Range (SOR - Pronounced as an initialism) is a United States Air Force research laboratory on the Kirtland Air Force Base in Albuquerque, New Mexico.Its primary duty, according to the official website, is to "develop and demonstrate optical wavefront control technologies."
Educational observatory This is a partial list of astronomical observatories ordered by name, along with initial dates of operation (where an accurate date is available) and location. The list also includes a final year of operation for many observatories that are no longer in operation.
It is suggested it would integrate Sandia's latest designs using LTDs. Sandia Labs recently proposed a conceptual 1 petawatt (10 15 watts) LTD Z-pinch power plant, where the electric discharge would reach 70 million amperes. [27] As of 2012, fusion shot simulations at 60 to 70 million amperes are showing a 100 to 1000 fold return on input energy.
URA has helped develop the Tevatron at Fermilab. Its early activities are related to the Superconducting Supercollider, the Pierre Auger Observatory, the Long-Baseline Neutrino Facility (LBNF), and the associated Deep Underground Neutrino Experiment (DUNE), and involvement in the Honeywell International-led National Technology and Engineering Solutions at Sandia (NTESS) that manages and ...