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The array consists of 27 dishes, 9 on each of 3 tracks radiating from a central point. One of the tracks crosses US route 60, so even when the facility is closed to the public (as it is right now) you can sometimes get a close look at one. Each dish is 25 meters in diameter.
An array of microham array modules - these control radios, the antenna/amplifier switching matrix and rotators.
The Measurements of Aerosols, Radiation, and Clouds over the Southern Ocean (MARCUS) field campaign of 2017 and 2018 used several ARM instruments such as the laser disdrometer (LDIS, right) to capture the variability in aerosol and cloud properties across the Southern Ocean (SO) from spring to autumn. Such measurements help scientists correct uncertainties in simulations of SO clouds, aerosols, precipitation and radiative transfer.
Terms of Use: Our images are freely and publicly available for use with the credit line, “Image courtesy of the U.S. Department of Energy Atmospheric Radiation Measurement (ARM) user facility.”
Amazing Tiles Floor Collection for Kitchen and Bathroom Tiles Design Daily Kitchen Interior Design Info
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 photovoltaic array system at IAAAP
captures solar energy to create electricity, thus
reducing power costs for the administration
building. Together with a geothermal system,
the photovoltaic system allows IAAAP to heat
and cool its administration building exclusively
with renewable energy sources. (Photo by Linda
K. Loebach, JMC Public Affairs)
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.