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Wind buffeting of large telescopes.

Douglas G MacMynowski1, Torben Andersen

  • 1Control and Dynamical Systems, California Institute of Technology, 1200 East California Boulevard, Pasadena, California 91125, USA. macmardg@cds.caltech.edu

Applied Optics
|February 2, 2010
PubMed
Summary
This summary is machine-generated.

Turbulent wind loads cause significant image jitter in ground-based telescopes. A simplified model accurately predicts this wind response and its sensitivity to telescope design parameters.

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Area of Science:

  • Optical engineering
  • Aerodynamics
  • Structural dynamics

Background:

  • Ground-based optical telescopes face significant dynamic disturbances from unsteady wind loads.
  • Turbulence within telescope enclosures is a primary source of wind-induced vibrations.
  • Minimizing wind response is crucial for telescope enclosure, structure, and control system design.

Purpose of the Study:

  • To develop and validate a simplified model for predicting telescope image jitter caused by wind.
  • To analyze the sensitivity of image jitter to various telescope design parameters.

Main Methods:

  • Utilized detailed integrated modeling to capture relevant wind physics.
  • Verified a proposed simplified model against a more complex, detailed model.
  • Investigated the influence of design elements on wind response.

Main Results:

  • The simplified model effectively captures the essential physics of wind-induced image jitter.
  • Identified key telescope design elements that significantly influence wind response.
  • Quantified the sensitivity of image jitter to a broad spectrum of design parameters.

Conclusions:

  • A simplified modeling approach is effective for understanding and predicting wind effects on optical telescopes.
  • The model provides valuable insights for optimizing telescope designs to mitigate wind disturbances.
  • This work aids in minimizing image jitter for improved astronomical observations.