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関連する概念動画

Electromagnetic Waves01:30

Electromagnetic Waves

James Clerk Maxwell formulated a single theory combining all the electric and magnetic effects scientists knew during that time, calling the phenomena his theory predicted “Electromagnetic waves”. He brought together all the work that had been done by brilliant physicists such as Oersted, Coulomb, Gauss, and Faraday and added his own insights to develop the overarching theory of electromagnetism. Maxwell’s equations, combined with the Lorentz force law, encompass all the laws of electricity and...
Propagation of Waves01:07

Propagation of Waves

When a wave propagates from one medium to another, part of it may get reflected in the first medium, and part of it may get transmitted to the second medium. In such a case, the interface of the two mediums can be considered as a boundary that is neither fixed nor free.
Consider a scenario where a wave propagates from a string of low linear mass density to a string of high linear mass density. In such a case, the reflected wave is out of phase with respect to the incident wave, however the...
Standing Waves01:17

Standing Waves

Sometimes waves do not seem to move; rather, they just vibrate in place. Unmoving waves can be seen on the surface of a glass of milk kept in a refrigerator, which is one example of standing waves. Vibrations from the refrigerator motor create waves on the milk that oscillate up and down but do not seem to move across the surface. These waves are formed or created by the superposition of two or more identical moving waves in opposite directions. The waves move through each other, with their...
Electromagnetic Wave Equation01:24

Electromagnetic Wave Equation

Maxwell's equations for electromagnetic fields are related to source charges, either static or moving. These fields act on a test charge, whose trajectory can thus be determined using suitable boundary conditions. The objective of electromagnetism is thus theoretically complete.
However, although electric and magnetic fields were first introduced as mathematical constructs to simplify the description of mutual forces between charges, a natural question emerges from Maxwell's equations: What...
Equations of Wave Motion01:02

Equations of Wave Motion

Mathematically, the motion of a wave can be studied using a wavefunction. Consider a string oscillating up and down in simple harmonic motion, having a period T. The wave on the string is sinusoidal and is translated in the positive x-direction as time progresses. Sine is a function of the angle θ, oscillating between +A and −A and repeating every 2π radians. To construct a wave model, the ratio of the angle θ and the position x is considered.
Standing Waves in a Cavity01:28

Standing Waves in a Cavity

A household microwave and lasers are examples of standing electromagnetic waves in a cavity. When two conducting metal plates are placed parallel at the nodal planes, it creates a cavity where standing waves are formed. The cavity between the two planes is analogous to a stretched string held at the points x = 0 and x = L. Here, the distance 'L' between the two planes must be an integer multiple of half of the wavelength. The wavelengths that satisfy this condition are given by:

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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

アルフヴェン波は太陽のコロナにある.

S Tomczyk1, S W McIntosh, S L Keil

  • 1High Altitude Observatory (HAO), National Center for Atmospheric Research (NCAR), Post Office Box 3000, Boulder, CO 80307-3000, USA. tomczyk@ucar.edu

Science (New York, N.Y.)
|September 1, 2007
PubMed
まとめ

アルフヴェン波は太陽のコロナで検出されましたが,観測された波は,冠状熱を説明するには弱すぎるようです. 未解明の波は,太陽の冠状の加熱メカニズムを理解する鍵を握っているかもしれない.

科学分野:

  • 太陽物理 太陽物理学
  • プラズマ天体物理学とは
  • ヘリオフィジックス ヘリオフィジックス

背景:

  • 太陽のコロナは数百万度に達し,現在のモデルでは完全に説明できない現象です.
  • アルフヴェン波は,光球からコロナにエネルギーを輸送し,潜在的にこの加熱を誘導することを提案されています.
  • 冠状熱の理解は,宇宙天候と地球への影響の予測に不可欠です.

研究 の 目的:

  • 太陽のコロナにおけるアルフヴェン波を検知し,特徴づけること.
  • 観測されたアルフヴェン波のエネルギー輸送能力を評価するため.
  • 太陽の大気エネルギーバランスにおけるアルフヴェン波の役割を調査する.

主な方法:

  • 国立太陽光天文台の冠状多チャンネル偏極計 (CoMP) を使いました.
  • 太陽のコロナの強度,視線速度,線形極化データを分析した.
  • FeXIII 1074.7ナノメートルの冠状放射線に焦点を当てました.

主要な成果:

  • 太陽のコロナで,上向きに広がるアルフヴェン波が検出されました.
  • 測定された波の相速度は,毎秒1〜4メガメートルの範囲です.

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

Published on: February 13, 2018

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

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

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

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

  • 推論された波の軌道は,極化測定から得られた磁場方向と一致する.
  • 結論:

    • 検出された空間的に解明されたアルフヴェン波は,太陽のコロナを温めるのに不十分なエネルギーを運んでいます.
    • 未解明のアルフヴェン波またはより小規模なアルフヴェン波が,冠状熱に必要なエネルギーを供給する可能性は残っています.
    • 未解明の波群に関するさらなる調査は,冠状のエネルギー輸送を完全に理解するために必要である.