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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...
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 Absorption Spectroscopy: Instrumentation01:22

Atomic Absorption Spectroscopy: Instrumentation

An atomic absorption spectrophotometer (AAS) comprises several components: a radiation source, an atomizer, a monochromator, and a detector. The radiation source can be a hollow-cathode lamp (HCL) or an electrodeless-discharge lamp (EDL), both of which provide a narrow emission line of the required wavelength. However, some instruments use continuum sources and high-resolution monochromators to achieve a narrow range of radiation.
The atomizer used in AAS can be either a flame atomizer or an...
UV–Vis Spectrum01:30

UV–Vis Spectrum

When light passes through a substance, a portion of the light is absorbed while the remaining light is reflected or transmitted. If the molecule absorbs light between the wavelengths of 180–400 nm range, the UV spectrum is obtained, and if it absorbs light in the 400–780 nm wavelength range, the visible spectrum is obtained.     
The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
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...
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.

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Related Experiment Video

Updated: Jul 7, 2026

In Situ Monitoring of the Accelerated Performance Degradation of Solar Cells and Modules: A Case Study for Cu(In,Ga)Se2 Solar Cells
09:19

In Situ Monitoring of the Accelerated Performance Degradation of Solar Cells and Modules: A Case Study for Cu(In,Ga)Se2 Solar Cells

Published on: October 3, 2018

GaN-Based Solar-Ultraviolet Detection Instrument.

E Monroy, F Calle, C Angulo

    Applied Optics
    |February 21, 2008
    PubMed
    Summary
    This summary is machine-generated.

    We developed a solar-ultraviolet (UV) monitoring system using gallium nitride (GaN)-based photodetectors. Schottky photodiodes demonstrated optimal performance, enabling a reliable UV detection head.

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    Published on: November 9, 2015

    Area of Science:

    • Materials Science
    • Semiconductor Physics
    • Optoelectronics

    Background:

    • Gallium nitride (GaN)-based materials are crucial for optoelectronic devices due to their wide bandgap properties.
    • Accurate solar-UV monitoring is essential for applications ranging from environmental science to human health.
    • Developing robust and sensitive UV detectors is an ongoing challenge in semiconductor research.

    Purpose of the Study:

    • To fabricate and characterize a solar-UV monitoring system utilizing GaN-based photodetectors.
    • To evaluate different GaN photodetector structures (photoconductors, p-n junction, Schottky barrier) for UV sensing capabilities.
    • To assess the performance of Al(x)Ga(1-x)N detectors and integrate GaN Schottky diodes into a complete UV detection head.

    Main Methods:

    • Fabrication of GaN photoconductors, p-n junction photodiodes, and Schottky barrier photodiodes.
    • Characterization of fabricated devices for UV sensing performance, including responsivity, linearity, and noise.
    • Preliminary investigation of Al(x)Ga(1-x)N detectors with varying aluminum compositions.
    • Assembly and evaluation of a complete solar-UV detection head using optimized GaN Schottky diodes.

    Main Results:

    • Schottky barrier photodiodes exhibited the best performance among the tested GaN structures.
    • Optimized Schottky photodiodes demonstrated a linear response, flat responsivity (100 mA/W), and high visible rejection ratio (>10^3).
    • A noise-equivalent power of 1 nW/Hz(-1/2) was achieved for the Schottky photodiodes.
    • Preliminary data on Al(x)Ga(1-x)N detectors showed potential for tailored UV detection.

    Conclusions:

    • GaN-based Schottky photodiodes are highly suitable for solar-UV monitoring applications.
    • The developed GaN Schottky diode-based detection head offers a promising solution for accurate UV sensing.
    • Further research into Al(x)Ga(1-x)N alloys could lead to advanced UV detector designs.