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Related Concept Videos

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...
Fluorescence and Phosphorescence: Instrumentation01:25

Fluorescence and Phosphorescence: Instrumentation

Fluorometers and spectrofluorometers are two types of instruments used for measuring molecular fluorescence. These instruments differ in how they select excitation and emission wavelengths and the type of light sources they utilize. Fluorometers use absorption interference filters to choose excitation and emission wavelengths. The excitation source in a fluorometer is typically a low-pressure mercury vapor lamp that emits intense lines distributed throughout the ultraviolet and visible regions.
Spectrophotometry: Introduction01:16

Spectrophotometry: Introduction

Spectrophotometry is the quantitative measurement of the absorption, reflection, diffraction, or transmission of electromagnetic radiation through a material as a function of the intensity and wavelength of the radiation. A spectrophotometer is a device used to measure the change in the radiation intensity caused by its interaction with the material.
The essential components of a spectrophotometer include a source of electromagnetic radiation, a slot for placing a material to be analyzed, and a...
UV–Vis Spectroscopy: Beer–Lambert Law01:09

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The Beer-Lambert law describes the relationship between absorbance and concentration, which combines the principles established by scientists Johann Heinrich Lambert and August Beer. Lambert's law states that when light passes through a medium, the loss in intensity is directly proportional to the original intensity and the path length of the light. Beer's law proposed that the transmittance of a solution remains constant if the product of concentration and path length is constant. The modern...

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Related Experiment Video

Updated: Jun 16, 2026

Evaluation of Photosynthetic Behaviors by Simultaneous Measurements of Leaf Reflectance and Chlorophyll Fluorescence Analyses
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Evaluation of Photosynthetic Behaviors by Simultaneous Measurements of Leaf Reflectance and Chlorophyll Fluorescence Analyses

Published on: August 9, 2019

Photometer for submillimeter measurements.

P Grenier, A Langlet, B Talureau

    Applied Optics
    |February 4, 2010
    PubMed
    Summary
    This summary is machine-generated.

    We developed a new photometer and blackbody calibrator for measuring submillimeter sky emissions. These instruments enable precise observations of cosmic background radiation at wavelengths greater than 500 micrometers.

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    Area of Science:

    • Astronomy and Astrophysics
    • Cosmology

    Background:

    • Understanding the cosmic microwave background (CMB) and other large-scale sky emissions is crucial for cosmology.
    • Submillimeter wavelengths probe early universe phenomena and interstellar medium properties.

    Purpose of the Study:

    • To introduce a novel photometer system for submillimeter astronomical observations.
    • To present a low-temperature calibration blackbody designed for accurate sky emission measurements.

    Main Methods:

    • Development of a specialized photometer for detecting faint submillimeter signals.
    • Construction of a stable, low-temperature blackbody source for instrument calibration.
    • Measurement of sky background emission at wavelengths exceeding 500 micrometers.

    Main Results:

    • The designed photometer and blackbody are functional and suitable for submillimeter measurements.
    • Initial measurements demonstrate the capability to characterize sky background emission.

    Conclusions:

    • The new instrumentation facilitates precise measurements of submillimeter sky background.
    • This work contributes to improved observational capabilities in submillimeter astronomy.