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相关概念视频

Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

3.4K
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: Interference01:30

Atomic Emission Spectroscopy: Interference

555
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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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 Spectroscopy: Effects of Temperature01:27

Atomic Spectroscopy: Effects of Temperature

804
Atomization, converting samples into gas-phase atoms and ions, is essential for atomic spectroscopy. The flame temperature required for atomization affects the efficiency of the atomic spectroscopic methods by increasing the atomization efficiency and the relative population of the excited and ground states.
At thermal equilibrium, the relative populations of excited and ground state atoms can be estimated using the Maxwell–Boltzmann distribution. For example, an increase in temperature...
804
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

507
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...
507
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

2.6K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
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Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
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Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

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在太阳附近观测F-冠状体减少和K-冠状体细结构

R A Howard1, A Vourlidas2, V Bothmer3

  • 1US Naval Research Laboratory, Washington, DC, USA. Russ.Howard@nrl.navy.mil.

Nature
|December 6, 2019
PubMed
概括
此摘要是机器生成的。

新的帕克太阳探测器的观测揭示了太阳附近的无尘区域以及包括磁流绳和岛屿在内的小型太阳喷发的详细等离子体结构. 这为太阳冠状动态和进化提供了洞察力.

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科学领域:

  • 太阳物理
  • 血物理
  • 太空科学

背景情况:

  • 太阳冠状体 (K冠状体和F冠状体) 的远程观测因距离而受到限制.
  • 之前的研究并未证实太阳附近存在理论上预测的无尘区域.
  • 太阳小事件的结构和发起仍然不确定.

研究的目的:

  • 使用帕克太阳探测器在前所未有的距离 (0.16-0.25 AU) 拍摄太阳冠.
  • 调查太阳附近没有尘埃的区域的存在.
  • 解决微型太阳爆发的等离子体结构.

主要方法:

  • 在帕克太阳探测器的日圆周围时拍摄太阳冠状.
  • 在短延伸时分析F-冠状强度以推断尘埃分布.
  • 解决太阳爆发的微型等离子体结构.

主要成果:

  • 观察到F-冠状强度在短延伸, 暗示一个无尘区.
  • 解决了小型太阳爆发的微型等离子体结构,识别了磁流绳和磁岛.
  • 证实了大规模的冠状拓,并揭示了冠状流中的子流.

结论:

  • 帕克太阳探测器的观测提供了太阳附近无尘区的证据.
  • 这项研究解决了以前未被观察到的磁性结构.
  • 冠状流是由具有持续密度波动的较小子流组成的.