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関連する概念動画

Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Scanning Electron Microscopy01:07

Scanning Electron Microscopy

A scanning electron microscope (SEM) is used to study the surface features of a sample by using an electron beam that scans the sample surface in a two-dimensional manner. Typically, areas between ~1 centimeter to 5 micrometers in width can be imaged. SEM can be used to image bacteria, viruses, tissues as well as larger samples like insects. Conventional SEM gives a magnification ranging from 20X to 30,000X and spatial resolution of 50 to 100 nanometers.
Fundamental Principles
Accelerated...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

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,...
Interference and Diffraction02:18

Interference and Diffraction

Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...

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関連する実験動画

Updated: Jul 11, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

ウエスト彗星と彗星塵の散射機能

E P Ney, K M Merrill

    Science (New York, N.Y.)
    |December 3, 1976
    PubMed
    まとめ

    研究者は,赤外線観測を用いて,西彗星の塵の性質を研究した. 粉塵粒子はおそらく1ミクロンの介電粒子であり,前向きに散乱する性質は,その大きさと組成を示している.

    科学分野:

    • 彗星科学 彗星科学
    • 塵の物理学 塵の物理
    • 赤外線天文学の天文学

    背景:

    • 彗星の塵は,太陽系の形成を理解する上で重要な役割を果たしています.
    • 以前の研究では,彗星の塵の組成と大きさの分布を特徴づけた.
    • ウエスト彗星 (1975n) は,塵の性質を研究するためのユニークな機会を提供します.

    研究 の 目的:

    • 彗星ウエストの塵の散乱相関数を決定する.
    • 彗星の塵粒子の大きさと組成を推測する.
    • 塵の振る舞いを彗星の断片化イベントと相関させるため.

    主な方法:

    • 0.5〜18マイクロンの波長で西彗星の赤外線観測.
    • 彗星コマからの散乱光と熱放射の分析.
    • 観測データに基づく散乱相関数のモデリング.

    主要な成果:

    • 西彗星の塵の散乱相関は,前向きに強くピークする.
    • 粉塵粒子は,半径約1ミクロンの介電粒子として識別されます.
    • コマの明るさの突然の上昇は,彗星の断片化時間の予測と相関しています.

    さらに関連する動画

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay
    05:55

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay

    Published on: August 23, 2024

    Controlled Synthesis and Fluorescence Tracking of Highly Uniform Poly(N-isopropylacrylamide) Microgels
    11:34

    Controlled Synthesis and Fluorescence Tracking of Highly Uniform Poly(N-isopropylacrylamide) Microgels

    Published on: September 8, 2016

    関連する実験動画

    Last Updated: Jul 11, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay
    05:55

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay

    Published on: August 23, 2024

    Controlled Synthesis and Fluorescence Tracking of Highly Uniform Poly(N-isopropylacrylamide) Microgels
    11:34

    Controlled Synthesis and Fluorescence Tracking of Highly Uniform Poly(N-isopropylacrylamide) Microgels

    Published on: September 8, 2016

    結論:

    • 彗星ウエスト彗星の彗星塵の粒子は,1ミクロンの介電粒子と一致する前方散射特性を示しています.
    • 観測された明るさの変動は,粉砕イベントが塵の放出とコマ特性に影響したことを示唆しています.
    • この研究は,彗星の塵の動力学と進化の理解を深める.