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Infrared (IR) Spectroscopy: Overview01:09

Infrared (IR) Spectroscopy: Overview

When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
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...
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for electronic transitions. As a result...
Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

The instrumentation of atomic emission spectrometry (AES) involves various components, including atomization devices that convert samples into gas-phase atoms and ions. There are two main types of atomization devices: continuous and discrete atomizers.  Continuous atomizers, like plasmas and flames, introduce samples in a constant stream, while discrete atomizers inject individual samples using syringes or autosamplers. The most common discrete atomizer is the electrothermal atomizer.
Flame Photometry: Lab01:16

Flame Photometry: Lab

In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
UV–Vis Spectrometers01:14

UV–Vis Spectrometers

The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...

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Related Experiment Video

Updated: Jun 16, 2026

Automated Charting of the Visual Space of Housefly Compound Eyes
08:34

Automated Charting of the Visual Space of Housefly Compound Eyes

Published on: March 31, 2022

Versatile nebular insect-eye fabry-perot spectrograph.

J Meaburn

    Applied Optics
    |February 6, 2010
    PubMed
    Summary
    This summary is machine-generated.

    A novel insect-eye spectrograph for the Isaac Newton telescope offers versatile astronomical observation. Its design features an optically contacted etalon and image tube detector for enhanced performance.

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    Area of Science:

    • Astronomy and Astrophysics
    • Optical Instrumentation

    Background:

    • Astronomical spectroscopy requires advanced instrumentation for detailed analysis.
    • The Isaac Newton telescope is a key facility for astrophysical research.

    Purpose of the Study:

    • To present the design and performance of a new insect-eye spectrograph.
    • To highlight the instrument's adaptability as a nebular filter camera.

    Main Methods:

    • Development of an insect-eye spectrograph with an optically contacted etalon.
    • Integration of an image tube as a detector.
    • Testing performance on the 249-cm Isaac Newton telescope.

    Main Results:

    • The spectrograph demonstrates effective performance on the Isaac Newton telescope.
    • The instrument's novel features, including pressure control, were successfully implemented.
    • Conversion to a nebular filter camera capability was achieved.

    Conclusions:

    • The insect-eye spectrograph is a valuable addition to astronomical observation tools.
    • The instrument's design offers flexibility and advanced detection capabilities.
    • This technology enhances the observational capacity of the Isaac Newton telescope.