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Heavily (over) processed New Horizons false color image of Pluto from a few days ago, arranged as a grid of Plutos.
The Lenten array here is very good, and it is highly unusual to find it in a Forward in Faith church. This is St Oswald's Chapel
Trying the array modifier having generated a huge array of cubes… And then getting lost in it with a camera (and two lights grouped with it).
Some mist was added as well so that we cannot see the end of the array (it is 25³-ish by the way…)
U-Boats, B-Boats, SD45s, and 2nd-generation Geeps all come together at Blue Island Yard. 12/28/78--Tom Golden photo.
Four antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) gaze up at the star-filled night sky, in anticipation of the work that lies ahead. The Moon lights the scene on the right, while the band of the Milky Way stretches across the upper left. ALMA is being constructed at an altitude of 5000 m on the Chajnantor plateau in the Atacama Desert in Chile. This is one of the driest places on Earth and this dryness, combined with the thin atmosphere at high altitude, offers superb conditions for observing the Universe at millimetre and submillimetre wavelengths. At these long wavelengths, astronomers can probe, for example, molecular clouds, which are dense regions of gas and dust where new stars are born when a cloud collapses under its own gravity. Currently, the Universe remains relatively unexplored at submillimetre wavelengths, so astronomers expect to uncover many new secrets about star formation, as well as the origins of galaxies and planets, when ALMA is operational. The ALMA project is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile. This panorama was taken by ESO Photo Ambassador José Francisco Salgado. Links ESO Photo Ambassadors webpage.
Solar Array Clean Low cost power. We see more of these in the future or maybe there will be no future.
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White Sands Missile Range Museum
This is an array element module from the MOTR radar antenna. There are 8359 of these in the antenna, all phased, hence the name Phased Array Radar. On each end of this element is a dipole antenna, one to receive and the other to transmit data.
As its name implies, MOTR phased array radar can track 40 objects at once. It was designed by and for WSMR engineers for instrumentation tracking. There are two MOTRs here at WSMR.