《美国三十米望远镜TMT主镜部件的辅助质量监测》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2019-09-20
  • Pasadena, CA – September 12, 2019 – New developments within the TMT Quality Assurance program include the acquisition of an advanced metrology system to measure to very high precision the telescope primary mirror assemblies.

    “We now have a Portable Coordinate Measuring Machine (CMM), which is a great tool for analyzing our assemblies and ensuring we meet the required high-tolerances for the TMT primary mirror. The TMT Optics team and Quality Assurance group have been trained this summer to use this CMM to test the M1 aluminum segment and its support assembly,” says Dr. Alastair Heptonstall, TMT Senior Opto-Mechanical Engineer.

    The mirror cell test-platform, also called the Multi-Segment Integration & Test (MSIT) facility*, installed in the TMT Laboratory is used to verify the functionality of all TMT primary mirror system components and assemblies.

    TMT Engineers are already working with real, full-size components of the primary mirror to see how they fit and work together when assembled. Engineers must precisely measure the geometry of these parts by sensing various points on their surface with an optical and tactile probe to ensure they perform correctly.

    Parts are measured in three dimensions, and compared directly to the original dimensions and tolerances given by the Computer-Aided-Design (CAD) model. Engineers will be able to verify the technical specifications of the telescope’s machined parts and processes.

    The accuracy of the measurements provided by the metrology arm is in the range of 25 microns, which is about a third of the diameter of a human hair!

    Some tests and study of the mirror cell ergonomics will include:

    - Verifying the process for the removal and installation of segments using a lifting jack device, as the segments will be taken out for recoating,

    - Inspecting parts such as segment sensor edges,

    - Testing the dust boots that cover and keep clean the edge sensors, and

    - Assessing the alignment of segments.

    These exact same tests will be required and performed at the TMT telescope when it is built and integrated. All material, equipment, parts, components and processes supplied to the telescope will be inspected on arrival to verify and certify their conformity in comparison to their technical requirements. These measuring procedures and the equipment tests used to perform them will assure the accuracy needed for the TMT to perform as expected.

    "When parts of the telescope come in, engineers will be able to check them and ensure that the product complies with the specifications and drawings of the CAD model” added Dr. Heptonstall. “Every time we take a segment out to be re-coated we will measure where the edges of the segment are compared to its support structure. This is required to protect every part of the segments, especially the corners of each segment that are particularly vulnerable. As the gap between segments is very narrow, the corners could touch the nearby segments if it is incorrectly positioned. Once mirror segments are placed together, there is a very small and uniform gap of 2.5 millimeter between them. The gap separation is necessary to prevent contact and allow continuous control and maintenance of the segments."

    The goal of the upcoming tests is to verify the positional accuracy of the segment during the actions of docking and undocking, for instance when a segment is removed and replaced at the time of mirror recoating, or during upgrades or maintenance exercises.

    The software used by the measuring device is identical to the software TMT will use for the initial alignment of the telescope during its construction. The same metrology and process control will be applied to align the TMT Telescope Optics during the important phase of assembly, installation and verification of the major sub-systems, as well as during operations. This new measuring hardware will be used to ensure and verify the alignment and positioning of all telescope optics: the M1 segments, the primary mirror with the secondary mirror, and the tertiary mirror with the science instruments.

  • 原文来源:https://www.tmt.org/news/431
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  • 《美国三十米望远镜(TMT)主镜进入加工》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2017-11-08
    • Marking a major production milestone, TMT has entered into a contract with Coherent Inc., one of the world’s leading providers of lasers and laser-based technology for scientific, commercial and industrial customers, to polish its U.S. manufactured primary mirrors (M1) segments. TMT, with its thirty-meter diameter primary mirror, and a collecting area greater than all other optical telescopes on Maunakea combined, is the largest optical/near-infrared telescope planned for the northern hemisphere. Under the terms of the contract, Coherent will precisely contour and polish the optical surfaces of 230 mirror segments to the accuracy of less than 1/50th of the width of a human hair. The remaining segments, including spare segments, are being provided by TMT’s international partners Japan, China and India. Coherent will use a unique “Stressed Mirror Polishing” (SMP) technique, a process refined jointly with TMT, for the production of the polished mirror segments. The Stressed Mirror Polishing uses specially designed fixtures that apply precise forces to the mirrors during their fabrication. The Ohara ClearCeram™ blank is warped into an aspheric shape, then accurately polished into a smooth spherical surface using a conventional polishing technique. The forces are released after polishing, and the mirror relaxes into the desired aspheric shape. SMP methodology was originally developed for the construction of the Keck telescope primary mirror, led by the late TMT Project Scientist, Jerry Nelson. This process both reduces the cost of polishing and improves the smoothness of the resulting optical surfaces. Nelson’s revolutionary concept of segmented mirrors replacing a single large collecting aperture has been used worldwide for several large telescopes that cannot be created using a single optical element, including the James Webb Space Telescope. About TMT: The Thirty Meter Telescope (TMT) Project has been developed as collaboration among Caltech, the University of California (UC), the Association of Canadian Universities for Research in Astronomy (ACURA), and the national institutes of Japan, China, and India with the goal to design, develop, construct, and operate a thirty-meter class telescope and observatory on Maunakea in cooperation with the University of Hawaii (TMT Project). The TMT International Observatory LLC (TIO), a non-profit organization, was established in May 2014 to carry out the construction and operation phases of the TMT Project. The Members of TIO are Caltech, UC, the National Institutes of Natural Sciences of Japan, the National Astronomical Observatories of the Chinese Academy of Sciences, the Department of Science and Technology of India, and the National Research Council (Canada); the Association of Universities for Research in Astronomy (AURA) is a TIO Associate. Major funding has been provided by the Gordon & Betty Moore Foundation. About COHERENT: Founded in 1966, Coherent, Inc. one of the world’s leading providers of lasers and laser-based technology for scientific, commercial and industrial customers. Our common stock is listed on the Nasdaq Global Select Market and is part of the Russell 2000 and Standard & Poor’s MidCap 400 Index. For more information about Coherent, visit the company’s website at www.coherent.com for product and financial updates.
  • 《美国三十米望远镜(TMT)72块主镜子镜坯验收》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2017-05-04
    • April 24, 2017 Pasadena, CA - The TMT project has accepted 72 mirror blanks produced by OHARA, a Japanese optical glass manufacturer in Sagamihara near Tokyo, and polished by CANON Inc., under the direction of the National Astronomical Observatory of Japan (NAOJ). This official acceptance confirms the excellent quality of the blanks and is based on stringent verification of the technical specifications set for all 492 TMT primary segment blanks (plus an additional 82 spare units) that will ultimately make TMT’s 30-meter diameter primary mirror. To receive this acceptance, the blanks were tested against many requirements such as the lack of flaws, cracks and non-uniformity in the glass which could be caused by machining or grinding. The chemical resistance, stability and coefficient of thermal expansion of the material were also tested under various conditions. A set of 70 blanks will be delivered to the U.S. later this year and stored in northern California waiting for the next steps in processing. The other two blanks will be sent to Nanjing Institute of Astronomical Optics and Technology (NIAOT), where TMT Chinese partners will start their trial polishing activities to develop a robust industrial base for TMT mirror segment production in Nanjing, China. The acceptance of the first mirror blanks produced by Japan represents a milestone for the TMT project. Japan will produce the entire stock of 574 meniscus blanks and perform surface polishing of 174 of them. The rest of the blanks will be polished within China, India and the United States, first as roundels, next hexagonal cut and further processed into the mirror segments that will comprise the TMT primary mirror. Mirror fabrication within the partnerships An efficient manufacturing process is required for the fabrication of TMT primary mirror segments: Mirror production starts with casting of the CLEARCERAM®-Z material, a special glass ceramic that is an ideal material for telescope mirrors due to a nearly zero coefficient of thermal expansion and excellent polishability. OHARA has produced 213 blanks as of March 2017. The flat blanks are first ground into a meniscus shaped blank, with a concave surface called the “segment optical surface.” To date, Okamoto, a company contracted by Canon, has manufactured 166 meniscus blanks, stored at the Canon’s Utsunomyia facility in Japan. Using a conventional polishing machine, meniscus blanks are accurately polished into a smooth aspherical shape and are then referred to as ‘roundels’. Canon has polished 12 roundels so far in Japan. In the U.S., Coherent Inc. will be the supplier responsible for polishing blanks and transforming them into roundels. After these first polishing steps, each roundel is cut and shaped into a hexagon; some pockets and reference features are ground into the back surface to mount the segment to the Segment Support Assembly (SSA), a mechanism that enables precise adjustments to ensure proper positioning of each mirror segment. The processes of roundel polishing, hexagonal cutting and segment support assembly mounting are developed in Japan, China, India and the United States. Harris Precision Optics in New York will receive U.S. roundels to create the polished mirror assemblies. The polished mirror assemblies receive a final verification of their optical surface quality and ultra-fine correction is applied using precise bombardment from an ion source, also known as Ion Beam Figuring. Harris Precision Optics will gather all hexagons produced by partners and be responsible to apply the final figuring process of ion figuring. About blanks and segments Weighing 185 kilograms each, with a diameter of 1.52 meters and a thickness of 46.1 millimeters, each blank is identified by a unique serial number which is linked to a data package containing information such as the batch identification number, date of melt, coefficient of thermal expansion, and compliance with mechanical and quality requirements. Each segment, when mounted to the telescope, will be separated from its neighbor by a narrow and uniform gap of 2.5mm. Once in operations, the position and orientation of the 1.44-meter wide hexagonal segments will be controlled so that the array functions as a single, highly accurate 30-m diameter mirror. Although each of the segments will have approximately the same thickness, their optical figure will be slightly different to account for the overall hyperboloidal shape of TMT’s primary mirror. The layout of the 492 segments is made of six identical sectors, each of them composed of 82 segments with a unique hexagonal shape and optical surface configuration. An additional set of 82 spare segments will be manufactured, each segment unit being used during a two-year recoating cycle. Molten glass ceramic poured into a mold for TMT primary mirror blank production. The first cast of blanks took place in 2013. TMT primary mirror blanks prior to being ground to a meniscus shape. TMT blank being polished into a smooth aspherical shape at Canon Inc. in Utsunomiya, Japan.