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Thermal analysis for the Thirty Meter Telescope (TMT) structure was performed using finite element analysis in ANSYS and I-DEAS. In the thermal analysis, the telescope structural parts with simplifi...
The primary mirror segment aberrations after shape corrections with warping harness have been identified as the single largest error term in the Thirty Meter Telescope (TMT) image quality error...
Analysis of normalized point source sensitivity as a performance metric for large telescopes.
Dynamic disturbance sources affecting the optical performance of the Thirty Meter Telescope (TMT) include unsteady wind forces inside the observatory enclosure acting directly on the telescope ...
This presentation describes a strategy for assessing the performance of the Thirty Meter Telescope (TMT). A Monte Carlo Simulation Framework has been developed to combine optical modeling with Compu...
The optical systems of TMT have stringent requirements to achieve scientific goals. The M2M support system was optimized to meet the requirements defined in “TMT Image Size and Wavefront Error Budge...
A large ground-based astronomical telescope project, like the Thirty Meter Telescope (TMT), is rivaling space projects in technical complexity, design and construction time span, budget, as well as ...
Thermal analysis for the Thirty Meter Telescope (TMT) optics (the primary mirror segment, the secondary mirror, and the tertiary mirror) was performed using finite element analysis in ANSYS and I-DE...
Mirror and dome seeing are critical effects influencing the optical performance of ground based telescopes. The Thirty Meter Telescope project has been utilizing a combination of optical simulations...
The performance requirements of the Thirty Meter Telescope (TMT) dictate, among others, a thorough understanding of the flow field inside and around the observatory. Mirror and dome seeing as well a...
We consider high-resolution optical modeling of the Thirty Meter Telescope for the purpose of error budget and instrumentation trades utilizing the Modeling and Analysis for Controlled Optical System...
We investigate a new metric, Normalized Point Source Sensitivity (PSSN), for characterizing the seeing limited performance of the Thirty Meter Telescope. As the PSSN metric is directly related to the...
Wind loads on ground-based telescopes.
University of California Observatories.
TMT Early Light Adaptive Optics     TMT  Adaptive Optics       2015/5/12
TMT Early Light Adaptive Optics.

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