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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...
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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.
The atomizer used in AAS can be either a flame atomizer or an...

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Updated: Jul 12, 2026

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

アポロ14号のアクティブ地震実験

J S Watkins, R L Kovach

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

    地震データによると,アポロ14号の遺跡には,フラ・マウロ・フォーメーションを覆う8.5メートルのレゴリット層がある. この地下構造は,明確な圧縮波速度を示しており,永久凍土は検出されていません.

    科学分野:

    • 月面地質学 月面地質学
    • 地震学 地震学とは
    • 惑星科学は惑星科学である.

    背景:

    • 月面着陸地点の地下構造を理解することは,地質の歴史と資源の可能性を解釈するために不可欠です.
    • アポロ14号のフラ・マウロ・フォーメーションは,月面での衝突過程を理解するための重要な地質学的な単位である.

    研究 の 目的:

    • 地震屈折データを用いて,アポロ14号の着陸地点の浅い地下構造を特徴づけるために.
    • 規則石と基礎構造の厚みと地震特性を決定する.
    • 潜在的な永久凍土の存在を調査するために.

    主な方法:

    • アポロ14号の遺跡で収集された爆発地震折射データの分析.
    • 地震の移動時間から圧縮波の速度と層の厚さの計算.

    主要な成果:

    • 厚さ8.5メートルで圧縮波の速度が104m/sの月のレゴリット層が特定されました.
    • 根底にあるフラ・マウロ岩層は16~76メートルの厚さで,圧縮波の速度は299m/sであった.
    • 370m/s以上の速度を持つより深い層が検出され,永久凍土の証拠は見つかりませんでした.

    結論:

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    06:14

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    Published on: July 30, 2020

    Atom Probe Tomography Analysis of Exsolved Mineral Phases
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    Simulation of the Planetary Interior Differentiation Processes in the Laboratory
    06:04

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    Published on: November 15, 2013

    • 地震データは,アポロ14号の遺跡の浅い地下の詳細なモデルを提供します.
    • 特定された層とその地震特性は,フラ・マウロ・フォーメーションの地質学的な期待と一致しています.
    • 永久凍土の欠如は,地震データ収集の時点での特定の熱的または地質的条件を示唆しています.