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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...
Shock Waves01:16

Shock Waves

While deriving the Doppler formula for the observed frequency of a sound wave, it is assumed that the speed of sound in the medium is greater than the source's speed through it. When this condition is breached, a shock wave occurs.
When the source's speed approaches the speed of sound, constructive interference between successive wavefronts emitted by the source occurs immediately behind it. Initially, scientists believed that this constructive interference would result in such high pressures...
Magnetostatic Boundary Conditions01:28

Magnetostatic Boundary Conditions

An electric field suffers a discontinuity at a surface charge. Similarly, a magnetic field is discontinuous at a surface current. The perpendicular component of a magnetic field is continuous across the interface of two magnetic mediums. In contrast, its parallel component, perpendicular to the current, is discontinuous by the amount equal to the product of the vacuum permeability and the surface current. Like the scalar potential in electrostatics, the vector potential is also continuous...
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...
Electrostatic Boundary Conditions01:16

Electrostatic Boundary Conditions

Consider an external electric field propagating through a homogeneous medium. When the electric field crosses the surface boundary of the medium, it undergoes a discontinuity. The electric field can be resolved into normal and tangential components. The amount by which the field changes at any boundary is given by the difference between the field components above and below the surface boundary.
The surface integral of an electric field is given by Gauss's law in integral form and is related to...
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...

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関連する実験動画

Updated: Jul 4, 2026

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

非対称的な太陽風の終結ショック.

Edward C Stone1, Alan C Cummings, Frank B McDonald

  • 1California Institute of Technology, Pasadena, California 91125, USA. ecs@srl.caltech.edu

Nature
|July 4, 2008
PubMed
まとめ

ボイジャー2号は,太陽風の終結ショックで,ボイジャー1号よりも高いエネルギーを持つ陽子の強度を検出しました. これは,衝撃の衝撃の違いを示唆しています.

科学分野:

  • ヘリオフィジックス ヘリオフィジックス
  • 天体物理学 天体物理学
  • プラズマ物理学 プラズマ物理学

背景:

  • ボイジャー2号は83.7アウで太陽風の終結ショックを横断し,ボイジャー1号より10アウ近くでした.
  • この近接差は,非対称なヘリオスフィアの存在を示唆している.
  • 潜在的な原因には,星間磁場圧力,衝撃運動,または太陽風圧などがあります.

研究 の 目的:

  • 太陽風の終結ショックの非対称性を調査する.
  • ボイジャー1号とボイジャー2号の衝撃交差点におけるエネルギー粒子の強度を比較する.
  • 異常な宇宙線と銀河系宇宙線グラデーションの源を決定する.

主な方法:

  • 終結ショック時のボイジャー2によるインシトゥ測定.
  • ヴォイジャー1号のデータと4~5MVの陽子強度の比較.
  • 銀河宇宙線ヘリウム強度グラデーションの分析.

主要な成果:

  • ボイジャー2号は,ボイジャー1号よりも3倍高い4〜5 MeVのプロトン強度を観測した.
  • 異常な宇宙線源は,ボイジャー2号による衝撃時に発見されなかった.
  • 銀河宇宙線ヘリウムの小さな強度グラデーションが検出されました.

さらに関連する動画

Surface Renewal: An Advanced Micrometeorological Method for Measuring and Processing Field-Scale Energy Flux Density Data
09:55

Surface Renewal: An Advanced Micrometeorological Method for Measuring and Processing Field-Scale Energy Flux Density Data

Published on: December 12, 2013

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing
08:54

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing

Published on: February 13, 2018

関連する実験動画

Last Updated: Jul 4, 2026

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

Surface Renewal: An Advanced Micrometeorological Method for Measuring and Processing Field-Scale Energy Flux Density Data
09:55

Surface Renewal: An Advanced Micrometeorological Method for Measuring and Processing Field-Scale Energy Flux Density Data

Published on: December 12, 2013

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing
08:54

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing

Published on: February 13, 2018

結論:

  • 終結ショックは非対称であり,陽子の強度が異なることが証明されています.
  • 異常な宇宙線の源は,衝撃交差点の位置ではない可能性が高い.
  • 銀河の宇宙線グラデーションは,ヘリオシートにさらに深く広がり,予想より低くなることもあります.