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Related Experiment Video

Updated: Jun 16, 2026

Design, Fabrication, and Administration of the Hand Active Sensation Test (HASTe)
07:54

Design, Fabrication, and Administration of the Hand Active Sensation Test (HASTe)

Published on: September 8, 2015

Dynamic Hartmann test.

L J Golden

    Applied Optics
    |February 16, 2010
    PubMed
    Summary
    This summary is machine-generated.

    The dynamic Hartmann test precisely monitors telescope alignment and optical figure using a star source. This method achieves high sensitivity, detecting aberrations at the lambda/50 to lambda/100 level.

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    Area of Science:

    • Optical engineering
    • Astronomy instrumentation

    Background:

    • Precise alignment and optical figure are critical for advanced telescope systems like the Large Space Telescope.
    • Existing testing methods may lack the required sensitivity or operational range for comprehensive system monitoring.

    Purpose of the Study:

    • To develop and validate a dynamic Hartmann test for precise monitoring of complete telescope systems.
    • To assess the test's capability in detecting low-order aberrations under laboratory conditions.

    Main Methods:

    • Utilized a real star source for in-situ testing of the complete telescope system.
    • Analyzed the dynamic Hartmann test configuration and constructed an experimental instrument.
    • Employed a wavefront error simulator to experimentally determine the instrument's aberration detection capabilities.

    Main Results:

    • The dynamic Hartmann test demonstrated high sensitivity, achieving detection levels between lambda/50 and lambda/100.
    • The test proved effective in detecting low-order aberrations under controlled laboratory conditions.

    Conclusions:

    • The dynamic Hartmann test is a suitable method for precise alignment and optical figure monitoring of large telescope systems.
    • The test offers a balance of operational range, sensitivity, and relative simplicity for astronomical applications.