Case Study

Unlocking Efficient Panel Manufacturing for the ngVLA

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ngvlaAssembly

Case Studies

SteelMoldStructure

Summary The Large Fiber Array Spectroscopic Telescope (LFAST) is a large telescope concept designed to be scalable. The telescope array

PanelBeingMeasured

Summary We hate to admit it, but accidents happen. When they do, what you do next is most critical. In

1E9A6561

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Summary

The next-generation Very Large Array (ngVLA) radio telescope aims to produce 250, 18-meter aperture telescope in the next decade. This telescope will be able to resolve objects in the sky, like black holes, in a way that has never been seen before. This telescope is bound to advance humanity’s understanding of fundamental physics. Building this many telescopes in such a short time is no easy feat. With each panel sizing up at roughly 2-2.5 m, the entire array will consist of about 18,000 total panels. This means that for the next decade, nearly 10 panels per working day need to be made to stay on schedule. With CMMs taking hours to perform a single measurement on these panels, a new method was needed to avoid the process bottleneck

FringeScan-3m

In November 2024 we delivered our largest system yet to mtex Antenna Technology Gmbh: FringeScan-3m. The system utilized 6 cameras (three cameras pairs) and an installation-caliber projector that all work in unison to cover the entire 3 meter area with a measurement time of just a few minutes.

Layout diagram of the 3-meter system

Installation Photos and Videos

Calibration data collection example

Application

Steel molds

Application

Damage Analysis

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