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The first preview was released on December 16, 2015. The final release was made available to Windows Insiders on July 18, 2016, followed by a public release on August 2.
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View from the Earth's north pole, showing the field of view of the main DSN antenna locations. Once a mission gets more than 30,000 km (19,000 mi) from Earth, it is always in view of at least one of the stations. Tracking vehicles in deep space is quite different from tracking missions in low Earth orbit (LEO). Deep space missions are visible ...
The main antenna is a 32-meter Deep Space Antenna. The wheel and track 32 m antenna is a state-of-the-art system that supported the Chandrayaan-1 and later the Mars Orbiter Mission mission operations. [4] It is currently supporting the Chandrayaan-2 orbiter and the Aditya-L1 mission as well as actively tracking the Chandrayaan-3 Propulsion ...
The DSN Switching Subsystem consists of multifunction, stand-alone tandem, end office, and remote switching units. Using the transmission, timing, and control elements of the DISN, they interconnect all military locations worldwide and provide end-to-end long-distance common user and dedicated voice, secure voice, data, and video services ...
The station is one of three [5] satellite communication stations in the NASA Space Communications and Navigation (SCaN) program’s Deep Space Network (DSN), whose mission is to provide the vital two-way communications link that tracks and controls interplanetary spacecraft and receives the images and scientific information they collect.
The beam waveguide antenna addresses these problems by locating the feed antenna in a "feed house" at the base of the antenna, instead of in front of the dish. The radio waves collected by the dish are focused into a beam and reflected by metal surfaces in a path through the supporting structure to the stationary feed antenna at the base.
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