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相关概念视频

Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

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...
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.
Thomson's e/m Experiment01:19

Thomson's e/m Experiment

In a beam of charged particles created by a heated cathode, the particles move at different speeds. However, many applications need a beam with uniform particle speeds. An arrangement known as a velocity selector uses electric and magnetic fields to pick particles with a particular speed from the beam.
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The magnetic...
Atomic Absorption Spectroscopy: Lab01:21

Atomic Absorption Spectroscopy: Lab

For AAS measurements, samples must be introduced as clear solutions, often requiring extensive preliminary treatment to dissolve materials like soils, animal tissues, and minerals. Common methods for sample preparation include treatment with hot mineral acids, wet ashing, combustion in closed containers, high-temperature ashing, or fusion with reagents.
 Solutions containing organic solvents, such as low-molecular-mass alcohols, esters, or ketones, enhance absorbances by increasing nebulizer...
Vibrating Concrete01:19

Vibrating Concrete

Mechanical vibrators are instrumental in compacting newly poured concrete within formwork and around reinforcements. This process is essential to eliminate trapped air pockets and establish a dense concrete mass. One widely used method is vibrating by internal vibrators, often referred to as a poker vibrator or immersion vibrator. It is rapidly inserted through the full depth of the freshly laid concrete and slightly extends into the layer below it (which remains in a plastic state). Consistent...
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.
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相关实验视频

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

阿波罗14号活动地震实验

J S Watkins, R L Kovach

    Science (New York, N.Y.)
    |March 17, 1972
    PubMed
    概括

    地震数据显示,阿波罗14号地点有一个8.5米高的 regolith层覆盖了Fra Mauro形成. 这个地下结构显示出明显的压缩波速度,没有检测到永久土.

    科学领域:

    • 月球地质学 月球地质学
    • 地震学 地震学
    • 星球科学 星球科学

    背景情况:

    • 了解月球着陆地点的地下结构对于解释地质历史和资源潜力至关重要.
    • 阿波罗14号的Fra Mauro形成是理解月球撞击过程的关键地质单元.

    研究的目的:

    • 用地震折射数据来描述阿波罗14号着陆地点的浅地地下结构.
    • 为了确定 regolith 和底层形成的厚度和地震特性.
    • 为了调查潜在的永久土的存在.

    主要方法:

    • 分析在阿波罗14号站点收集的爆炸地震折射数据.
    • 从地震行程时间计算压缩波速度和层厚度.

    主要成果:

    • 确定了一个厚度为8.5米,压缩波速度为104m/s的月球规律层.
    • 发现底层的弗拉莫罗岩层厚度在16至76米之间,压缩波的速度为299米/秒.
    • 检测到一个速度超过370米/秒的更深层,没有发现永久土的证据.

    结论:

    • 地震数据提供了阿波罗14号站点浅层地下的详细模型.

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  • 已识别的层和它们的地震特性与对弗拉莫罗岩层的地质预期一致.
  • 永久土的缺失表明地震数据采集时的特定热或地质条件.