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相关概念视频

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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Electronic Distance Measuring Instruments (EDMs) are essential tools in modern surveying, offering precise distance measurements by emitting electromagnetic signals and calculating the time required for these signals to travel to a target and return. Two primary types of signals are used in EDMs — light waves and microwaves — each suited to specific environmental and distance requirements. Light-wave-based EDMs utilize either infrared or laser light, providing high accuracy over short...
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The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
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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).
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星球激光干扰测量地震声学天文台

Grigory Dolgikh1, Sergey Budrin1, Stanislav Dolgikh1

  • 1V.I. Il'ichev Pacific Oceanological Institute FEB RAS, 690041 Vladivostok, Russia.

Sensors (Basel, Switzerland)
|January 11, 2025
PubMed
概括

一个新的行星激光干扰测量地震声学天文台可以精确地确定全球范围内超声波干扰的来源. 该系统识别信号分歧和传播期间的能量损失,增强地震和声学监测能力.

关键词:
吸收系数 的吸收系数.不同的差异,不同的差异.激光压力计激光压力计.星球观测台行星观测台三角测量是三角测量的方法.

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科学领域:

  • 地质物理学 地质物理学
  • 声学 声学 在声学方面
  • 激光干扰计是指激光干扰计.

背景情况:

  • 地震声学监测依赖于检测和定位干扰.
  • 星球范围内的超声波探测在信号定位和特征化方面提出了重大挑战.

研究的目的:

  • 描述行星激光干扰测量地震声学天文台的发展和能力.
  • 建立在行星距离处的超声波干扰的方向查找和信号分析方法.

主要方法:

  • 使用一个六个静止激光压力计的网络与不平等的手臂.
  • 采用三角测量方法,用于查找超声波干扰的方向.
  • 集成一个高精度计时系统 (TRIMBLE 5700) 进行同步测量.

主要成果:

  • 开发了基本方法,用于在任何行星距离处发现超声波干扰的方向.
  • 证明了使用空间分离压力计来确定信号分歧和传播期间的能量损失的能力.
  • 在0-1000 Hz频率范围内,实现了10 pm的位移记录准确度.

结论:

  • 已建立的行星激光干扰测量地震声学天文台可以确定全球变形超声波干扰的主要来源.
  • 该系统可以对信号特征进行详细分析,包括分歧和能量减弱.
  • 这个天文台增强了监测和理解行星规模地震声学现象的能力.