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相关概念视频

Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

348
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.
348
Emission Spectra02:39

Emission Spectra

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When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

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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...
151
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

1.7K
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...
1.7K
Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

200
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....
200
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

175
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,...
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相关实验视频

Updated: Jun 14, 2025

In situ Grazing Incidence Small Angle X-ray Scattering on Roll-To-Roll Coating of Organic Solar Cells with Laboratory X-ray Instrumentation
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太阳爆发整体场光谱仪 太阳爆发整体场光谱仪

Vicki L Herde1,2, Phillip C Chamberlin1,2, Don Schmit3

  • 1University of Colorado Boulder, Boulder, CO 80303 USA.

Solar physics
|September 2, 2024
PubMed
概括
此摘要是机器生成的。

太阳喷发近场整体场光谱仪 (SNIFS) 将以高分辨率观察太阳的染色层和过渡区域. 这次NASA探测火箭任务将为动态太阳现象提供前所未有的细节.

关键词:
染色体,活跃的染色体.发射火焰,可以发射火焰.仪器仪表和数据管理.探测火箭 探测火箭 探测火箭谱写仪的光谱学图刺 (Spicules) 是一种刺.

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科学领域:

  • 太阳物理 太阳物理
  • 天文学 天文学
  • 频谱学是一种光谱学.

背景情况:

  • 太阳染色层和过渡区域是理解太阳活动的关键领域.
  • 以前的仪器缺乏必要的空间和光谱分辨率来观测快速太阳事件.

研究的目的:

  • 为了引入太阳喷发近场整体场光谱仪 (SNIFS) 仪器.
  • 详细说明科学目标和仪器设计,用于观察动态太阳现象.

主要方法:

  • 使用格雷戈里亚式反射望远镜和专门的镜子阵列.
  • 实现高节奏 (1s) 的空间 () 和光谱 (33mÅ) 观测.
  • 聚焦于莱曼α (1216 Å),Si iii (1206 Å) 和O v (1218 Å) 周围的波长.

主要成果:

  • SNIFS仪器是为高频率,高分辨率的太阳观测而设计的.
  • 仪器及其子系统的集成前测试已经完成.
  • 该仪器计划在2025年夏天进行NASA探测火箭飞行.

结论:

  • SNIFS将提供关于太阳螺纹,纳米耀斑和潜在的太阳耀斑的新见解.
  • 该仪器的独特设计使得能够详细研究快速变化的太阳特征.
  • 这个任务将推动我们对太阳大气中的能量传输的理解.