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  • Measuring Surface Slope Error on Precision Aspheres (.pdf)
    . Controlling the errors at cycles of. 10-12 per aperture ensures that the mirrors will be smooth enough for the instrument to work correctly, and help limit the. potential roll-off that may occur on the final 10% of the mirror aperture. 2.2. Off-axis generalized aspheric and conic mirrors for ozone
  • Applying Taguchi Designs to EMMAQUA Weathering Experiments
    solar image on the target. A blower forces air across the target to cool test specimens. The optical system is often described as a Fresnel reflecting solar concentrator with mirrors positioned as tangents to an imaginary parabolic trough. The test specimen's optical properties (solar reflectance
  • Wavelength-scalable hollow optical
    losses while increas-. spectra were measured with a Fourier-transform infrared (FTIR). ing robustness. spectrometer (Nicolet Magna 860), using a parabolic mirror to. To achieve high index contrast in the layered portion of the. couple light into the fibre and an external detector. The results

Engineering Web Search: 12 Parabolic Mirrors Top