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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...
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...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
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:
Electromagnetic Waves in Matter01:30

Electromagnetic Waves in Matter

Electromagnetic waves can travel in the vacuum as well as in matter. For example light, which is an electromagnetic wave, can travel through air, water, or glass.
Consider the electromagnetic wave passing through a dielectric medium. In such a case, Maxwell's equations get modified. In Ampere's law, ε0 , the dielectric permittivity of free space is replaced with ε, the permittivity of dielectric. Also, the vacuum permeability μ0 is replaced by the permeability of the medium, μ.
Furthermore, the...

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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

太陽系物質における宇宙線記録

R C Reedy, J R Arnold, D Lal

    Science (New York, N.Y.)
    |January 14, 1983
    PubMed
    まとめ

    太陽系物体と相互作用する宇宙線は,その歴史を明らかにする. 核酸と粒子の軌跡の分析は,何百万年にもわたる宇宙線流の過去の変動を示しています.

    科学分野:

    • 宇宙線物理学 宇宙線物理学
    • 惑星科学は惑星科学である.
    • 核天体物理学は,核天体物理学である.

    背景:

    • 宇宙線におけるエネルギー核は,隕石,月,惑星などの太陽系天体と相互作用する.
    • これらの相互作用は,標的材料内のヌクリドと重核の軌跡を生成します.

    研究 の 目的:

    • 宇宙線で生成された核酸と軌跡に含まれる情報を調査する.
    • 太陽系オブジェクトの歴史と粒子フローの変動を理解するために.
    • 月面のサンプルと隕石の複雑な宇宙線被曝履歴を分析する.

    主な方法:

    • 地球外物質におけるヌクリドと重核の痕跡の分析.
    • 宇宙線被曝歴の再構築. 宇宙線被曝歴の再構築.
    • サンプルに影響する侵食,ガーデニング,断片化,軌道変化の調査.

    主要な成果:

    • 宇宙線相互作用は,太陽系天体の詳細な歴史的記録を提供します.
    • 証拠は,宇宙線粒子フローの時間的および空間的な変動を示唆しています.
    • 複雑な曝露歴は,様々なプロセスによる月面サンプルや隕石で一般的です.

    さらに関連する動画

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells
    10:16

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells

    Published on: August 20, 2019

    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

    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

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells
    10:16

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells

    Published on: August 20, 2019

    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

    結論:

    • 宇宙線曝露の歴史は,太陽系の進化を理解するために不可欠です.
    • 過去の太陽粒子フローは,10^4年から10^7年の時間スケールで変動を示しています.
    • 銀河の宇宙線流の変動に関するさらなる研究が必要である.