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関連する概念動画

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...
Mutations01:35

Mutations

Mutations are changes in the sequence of DNA. These changes can occur spontaneously or they can be induced by exposure to environmental factors. Mutations can be characterized in a number of different ways: whether and how they alter the amino acid sequence of the protein, whether they occur over a small or large area of DNA, and whether they occur in somatic cells or germline cells.
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
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...

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関連する実験動画

Updated: Jul 12, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

月面サンプルにおける太陽放射線の影響

B W Hapke, A J Cohen, W A Cassidy

    Science (New York, N.Y.)
    |January 30, 1970
    PubMed
    まとめ

    粉砕されたアポロ11号の結晶岩は,月面の土と異なる光学特性を示しています. 放射線と加熱によりこれらの性質が変化し,土壌のアルベドとスペクトルが予想値から著しく偏差した.

    科学分野:

    • 地質学 地質学 地質学
    • 惑星科学は惑星科学である.
    • マテリアルサイエンス 材料科学

    背景:

    • 月面のレゴリティの光学特性は,表面の過程を理解する上で極めて重要です.
    • アポロ11号のサンプルは,月の地質学と物質進化の洞察を提供します.

    研究 の 目的:

    • 粉砕されたアポロ11号の結晶岩の光学特性を調査するために.
    • これらの光学特性に対する環境要因の影響を決定する.
    • 岩石と土壌の光学特性を比較するために.

    主な方法:

    • 結晶岩粉末の光学特性 (アルベド,スペクトル) の分析.
    • サンプルの紫外線およびX線照射への暴露.
    • 熱処理 (加熱) を適用する.
    • 月の天然の土壌特性との比較.

    主要な成果:

    • 粉砕された結晶岩は,月面の土壌と比較して独特の光学特性を示す.
    • 放射線と加熱により,サンプルの光学特性が大幅に変化した.
    • 処理された土壌の観測されたアルベドとスペクトル値は,予測から著しく逸脱した.

    さらに関連する動画

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    関連する実験動画

    Last Updated: Jul 12, 2026

    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
    06:14

    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

    Published on: July 30, 2020

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    結論:

    • 放射線と熱などの環境要因は,月の岩の光学特性を変更することができます.
    • これらの改変は,月面の土壌の予想と観測の光学行動の間の不一致を説明する.
    • これらの変化を理解することは,正確なリモートセンシングと表面解釈に不可欠です.