The next generation of earth based large telescopes, such the European Extremely Large Telescope (E-ELT) targeted for 2024, will boost the space exploration and the search for other life in the universe. The primary mirror of the E-ELT will reach up to 39 metres of aperture. It will be composed by hundreds of 1.5 m corner to corner hexagonal mirror segments. The surface from of these segments need to be manufactured at nanometre level. The bottleneck on the manufacturing process of these segments is the figuring. Indeed, the iterative measurements and correction is extremely time consuming. To address the measurement issue, the Precision Engineering Institute of Cranfield University has developed a unique Optical Test System (OTS) for metre...
The mirror segments for the E-ELT and TLT are nearly equal in size and shape (hexagonal, 1.2 m over ...
The manufacture of the next generation of large astronomical telescopes, the extremely large telesco...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
The next generation of earth based large telescopes, such the European Extremely Large Telescope (E-...
The work focuses on the structural design and performances of a unique optical test system (OTS) use...
The work focuses on the structural design and performances of a unique optical test system (OTS) use...
Ground-based optical-infrared 10m-class telescopes, such as Keck, Gemini, and Very Large Telescopes ...
Ground-based optical-infrared 10m-class telescopes, such as Keck, Gemini, and Very Large Telescopes ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
\u3cp\u3eThe preparations for the design and construction of the Extremely Large Telescope (ELT) are...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
This dissertation describes the development, calibration, and testing of the adaptive optics system ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The mirror segments for the E-ELT and TLT are nearly equal in size and shape (hexagonal, 1.2 m over ...
The manufacture of the next generation of large astronomical telescopes, the extremely large telesco...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
The next generation of earth based large telescopes, such the European Extremely Large Telescope (E-...
The work focuses on the structural design and performances of a unique optical test system (OTS) use...
The work focuses on the structural design and performances of a unique optical test system (OTS) use...
Ground-based optical-infrared 10m-class telescopes, such as Keck, Gemini, and Very Large Telescopes ...
Ground-based optical-infrared 10m-class telescopes, such as Keck, Gemini, and Very Large Telescopes ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
\u3cp\u3eThe preparations for the design and construction of the Extremely Large Telescope (ELT) are...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
This dissertation describes the development, calibration, and testing of the adaptive optics system ...
The preparations for the design and construction of the Extremely Large Telescope (ELT) are in full ...
The mirror segments for the E-ELT and TLT are nearly equal in size and shape (hexagonal, 1.2 m over ...
The manufacture of the next generation of large astronomical telescopes, the extremely large telesco...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...