《美国三十米望远镜主镜计量框架已制造完毕》

  • 来源专题:天文仪器与技术信息
  • 编译者: zwg@niaot.ac.cn
  • 发布时间:2020-06-12
  • ASADENA, CA – The first TMT primary mirror (M1) metrology frame has been built and delivered to TMT’s technical laboratory near Pasadena. TMT will use the metrology frames, which are auxiliary equipment tools, to accurately locate the M1 mirror segments during installation.

    Before the installation of TMT’s Primary Mirror (M1) segments, each fixed frame that supports the segment must be placed in the correct location. Four hundred and ninety-two individual dummy masses, mimicking the weight of each segment, will be placed on the fixed frames to induce the same deflection that will be caused by the mirror segments themselves.

    The metrology frames are located on the fixed frames using precision alignment pins, and hold retroreflectors that the laser tracker alignment system can locate. The laser trackers will then measure accurately the alignment of each segment fixed frame position relative to its neighbors, enabling precise positioning of the entire 492 fixed frames. The fixed frames will then be permanently bolted to the mirror cell, maintaining all segments in the correct place.

    “The initial metrology frame has been delivered, inspected and tested at the lab, and nine additional metrology frames will be produced,” says Alastair Heptonstall, TMT Senior Opto-Mechanical Engineer. “A total of ten metrology frames are planned to be used during the installation of the telescope mirror cell. They will be placed in clusters to align ten M1 fixed frames at the same time. They will then be moved on to the next ten fixed frames.”

    The metrology frame, made of a special type of carbon fiber material, is ultra-precisely built with a few thousandths of an inch accuracy. It needs to be light, stiff, and durable with an extremely low thermal expansion coefficient to provide a stable structure for the required measurements. Laser trackers, widely used in aerospace industry and high-tech military applications, will be used to accurately measure the position of the TMT fixed frames.

    For TMT to achieve the design optical performance, it is crucial to have all the telescope optics accurately aligned. Considering the unprecedented large size of TMT, the laser tracker system will allow fast, high precision and automated measurements of each mirror positioning relative to its neighbors. A coordinate system for the observatory will give the reference position of M1, M2, M3, the instruments, as well as the telescope structure and enclosure, and the Global Metrology System (GMS) will measure the locations of all these systems as a function of the elevation angle.

    TMT will be one of the first telescope using laser trackers to perform the initial alignment during the observatory construction. In a second and final stage, the wave-front sensors and the Alignment and Phasing System will provide the final precise tip, tilt and piston control of all 492 mirror segments.

    Rock West Composites, based in San Diego, is a high-tech carbon fiber composite design company making specialized ultra-low expansion carbon composites. For more information on Rock West Composites, you may click: https://www.rockwestcomposites.com.

  • 原文来源:https://www.tmt.org/news/463
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  • 《美国三十米望远镜圆顶准备制造》

    • 来源专题:天文仪器与技术信息
    • 编译者:zwg@niaot.ac.cn
    • 发布时间:2020-06-12
    • Pasadena, CA – TMT’s Enclosure System has achieved its final design milestone, successfully passing a series of Production Readiness Reviews (PRR) in March 2020. Over the last several years, the enclosure design has progressed through its final design phase followed by the completion of the models, drawings and specifications required for procurement and fabrication. Completion of the PRR sets the stage for effectively starting the procurement and fabrication of the enclosure parts, which will be followed by factory assembly, testing, and shipment of the enclosure components to the TMT construction site. The TMT Enclosure calotte design, selected after extensive trade studies, is a spherically shaped building that surrounds and protects the telescope and instrumentation during non-observing time and in severe weather conditions. During science operations, the enclosure aperture opens to allow the telescope a clear and unobstructed view of the sky. Fundamental features of this calotte design include: A minimum size due to its spherical form. The clearance between the inside of the enclosure and some telescope parts is as small as 0.5 meters in some places. A minimum aperture opening that provides maximum protection to the telescope from windshake, critical for maximizing telescope image quality performance. A very low mass for a structure of its size due to the structurally-efficient calotte shape. The enclosure can be repositioned to any point in the sky very quickly with reasonable drive power demands. The TMT enclosure has been designed to minimize its mass and size, with enhanced control and performances during scientific observations. This unique design will enable rapid changes of pointing direction, while providing a maximum protection from wind-induced vibrations and dome-seeing degradation, which could otherwise impact the performances and image quality of the telescope. “TMT’s enclosure is unique among the Extremely Large Telescopes being built today,” says Luc Simard, Director General of the Herzberg Astronomy and Astrophysics Research Centre. “It will facilitate the observations of astronomical phenomena requiring a rapid response and will deliver optimal conditions for Adaptive Optics observations at an unprecedented spatial resolution. TMT's enclosure design will be key to the scientific success of TMT.” The PRR focused primarily on the structural and mechanical fabrication drawings, electrical schematics, specifications, and special processes for fabrication of TMT enclosure components and assemblies. However, additional independent assessments of compliance to the enclosure design requirements, management, safety and risk were also completed as a part of the review. The review board unanimously agreed that the fabrication data package for the enclosure structural, mechanical, electrical and control systems is now complete and ready for the enclosure fabrication phase. TMT’s enclosure design was completed by Empire Dynamic Structures of Port Coquitlam, BC, Canada as a Canadian in-kind contribution to the TMT Project, managed by the Canadian National Research Council (NRC). The work was conducted through a contract between Dynamic Structures and the Canadian Commercial Corporation (CCC) on behalf of the NRC. Dynamic Structures assembled an excellent and dedicated team of structural, mechanical, electrical, systems, controls and CAD engineers to complete the work. TMT Enclosure Design Overview The TMT calotte style enclosure consists of 3 major structural components; the base, cap and shutter. The base is the lower portion of the enclosure and it rotates about the azimuth axis. The cap and shutter upper sections rotate in a plane tilted 32.5 degrees from horizon. Through combined motion of the base, cap and shutter, the shutter aperture can be positioned anywhere within the viewing range of the telescope. Relative motion of the cap and shutter is used to either close and seal the enclosure or open the shutter aperture during science observations. The shutter structure is located directly inside the cap structure. It consists of an open steel framework supporting a steel plug structure. The shutter rotates about 180° around the same axis as the cap, enabling opening and closing of the telescope aperture. The cap also includes a set of deployable external flaps designed to divert incoming air flow and provide wind protection for TMT secondary mirror. There are a total of 88 inner and outer ventilation doors which are used to provide controlled ventilation of the enclosure during astronomical observations. These vents can be opened or closed to modulate the amount of outside ambient air flowing through the enclosure and maintain a steady flow and air temperature within the optical path. Calculations using Computational Fluid Dynamics modeling have shown good wind flushing properties inside the TMT dome and around the telescope to eliminate thermal effects on the seeing. The telescope enclosure, which is 66 meters in diameter (about the width of a soccer field), has a height of approximately 56 meters above the surrounding ground and a total mass of 2900 metric tons. It is able to open its 31.25 meter diameter aperture in less than 2 minutes and will allow the telescope to point an astronomical object in under 3 minutes. The enclosure is equipped with 3 crane systems to facilitate the maintenance and technical operations of the telescope and instrumentation systems. The enclosure safety requirements are fully defined and provide adequate safety for the observatory personnel and visitors, including local emergency stop buttons, sensors and wiring that interface with the observatory safety system.
  • 《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.