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Related Concept Videos

Interference and Diffraction02:18

Interference and Diffraction

Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
IR Spectrometers01:25

IR Spectrometers

There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
Total Internal Reflection Fluorescence Microscopy01:05

Total Internal Reflection Fluorescence Microscopy

Total internal reflection fluorescence microscopy or TIRF is an advanced microscopic technique used to visualize fluorophores in samples close to a solid surface with a higher refractive index, such as a glass coverslip. TIRF only allows fluorophores in proximity to the solid surface to be excited. When light from a medium with a lower refractive index (such as air) hits the glass coverslip at a critical angle, the light undergoes total internal reflection stead of passing through the glass.
Phase Contrast and Differential Interference Contrast Microscopy01:26

Phase Contrast and Differential Interference Contrast Microscopy

Phase-Contrast Microscopes
In-phase-contrast microscopes, interference between light directly passing through a cell and light refracted by cellular components is used to create high-contrast, high-resolution images without staining. It is the oldest and simplest type of microscope that creates an image by altering the wavelengths of light rays passing through the specimen. Altered wavelength paths are created using an annular stop in the condenser. The annular stop produces a hollow cone of...
IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration01:16

IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration

A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to the...

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Updated: Jun 9, 2026

Compact Lens-less Digital Holographic Microscope for MEMS Inspection and Characterization
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Hubble Space Telescope COSTAR asphere verification with a modified computer-generated hologram interferometer.

L Feinberg, M Wilson

    Applied Optics
    |September 8, 2010
    PubMed
    Summary

    A new, simple method was developed to verify the surface accuracy of aspheric mirrors designed to correct Hubble Space Telescope

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    Area of Science:

    • Optical engineering
    • Space telescope instrumentation

    Background:

    • Hubble Space Telescope primary mirror exhibited spherical aberration.
    • Correction required specialized anamorphic aspheric mirrors for scientific instruments.

    Purpose of the Study:

    • To develop a quick and simple method for verifying the surface figure of aspheric mirrors.
    • To ensure the accuracy of corrective optics for the Hubble Space Telescope.

    Main Methods:

    • Fabrication of five anamorphic aspheric mirrors for the Corrective-Optics Space Telescope Axial-Replacement (COSTAR) instrument.
    • Development and application of a simple verification technique during vendor acceptance tests.

    Main Results:

    • The developed technique was successfully applied to three aspheric mirrors.
    • Results confirmed that the tested aspheres meet the expected accuracy requirements for this verification method.

    Conclusions:

    • A practical and efficient method for aspheric mirror surface figure verification has been established.
    • This method aids in ensuring the quality of corrective optics for space-based observatories.