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Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

230
Inductively coupled plasma (ICP) is the common plasma source used in atomic emission spectroscopy (AES), a technique that detects and analyzes various elements in a sample. This method is often called inductively coupled plasma atomic emission spectroscopy (ICP-AES).
There are three main types of inductively coupled plasma atomic emission spectroscopy  (ICP-AES) instruments: sequential, simultaneous multichannel, and Fourier transform instruments, with the latter being less commonly used....
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Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

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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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Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

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Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
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Atomic Emission Spectroscopy: Lab01:29

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AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
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UV–Vis Spectrometers01:14

UV–Vis Spectrometers

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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.
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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...
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Atmospheric-pressure Molecular Imaging of Biological Tissues and Biofilms by LAESI Mass Spectrometry
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露西热发射光谱仪 (L'TES) 仪器仪表.

P R Christensen1, V E Hamilton2, G L Mehall1

  • 1School of Earth and Space Exploration, Arizona State University, Tempe, AZ USA.

Space science reviews
|December 22, 2023
PubMed
概括
此摘要是机器生成的。

露西热发射光谱仪 (L'TES) 将测量特洛伊小行星的热物理特性. 这个仪器是OTES的副本,它使用福里埃变形光谱仪进行远程测量,验证其在太空中的性能.

关键词:
一个小行星.路西路西路西路西路西路西路热辐射光谱仪热辐射光谱仪这是一个特洛伊木马.

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科学领域:

  • 行星科学 行星科学
  • 天体物理学 天体物理学
  • 频谱学是一种光谱学.

背景情况:

  • 露西任务的目标是特洛伊木马小行星,需要遥感能力.
  • 了解小行星的热物理特性对于行星形成研究至关重要.
  • 以前的仪器,如OSIRIS-REx上的OTES,为新的任务硬件提供了基础.

研究的目的:

  • 详细介绍露西热发射光谱仪 (L'TES) 的设计和功能.
  • 概述仪器能够远程测量特洛伊小行星的热物理性质的能力.
  • 通过校准和初始空间数据来确认仪器的准备和性能.

主要方法:

  • 使用福里埃变换光谱仪 (FTS) 覆盖5.71-100微米.
  • 使用一个Cassegrain望远镜,其光圈为15.2厘米.
  • 采用DLATGS火电探测器和计量干扰仪进行精确的控制.

主要成果:

  • L'TES仪器是OTES仪器的构建打印副本.
  • 它为不同的光谱分辨率提供可变的采集时间 (0.5,1,2秒).
  • 放射测量精度为≤2.2 × 10−8 W cm−2 sr−1/cm−1,绝对温度误差为<2 K,用于>75 K的场景.

结论:

  • L'TES是一个完全特色的仪器,为其任务目标做好了准备.
  • 最初的太空数据证实了仪器的放射和空间性能.
  • 该仪器准备好提供有关特洛伊木马小行星的关键热物理数据.