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Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

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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...
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Maxwell-Boltzmann Distribution: Problem Solving01:20

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Individual molecules in a gas move in random directions, but a gas containing numerous molecules has a predictable distribution of molecular speeds, which is known as the Maxwell-Boltzmann distribution, f(v).
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Consider the electric field of an oppositely charged, parallel-plate system and an imaginary box between those plates. Let the bottom face of the box be ABCD, and the top face be FGHK. The electric field between the plates is uniform and points from the positive plate toward the negative plate. The calculation of this field's flux through the box's various faces shows that the net flux through the box is zero. Why does the flux cancel out here?
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Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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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.
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Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

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Magnetic dipoles in magnetic materials are aligned when placed under an external magnetic field. For paramagnets and ferromagnets, dipole alignment occurs in the direction of the magnetic field. However, the dipoles align opposite to the field in the case of diamagnets. This state of magnetic polarization due to the external field is called magnetization. Magnetization is defined as the dipole moment per unit volume. It plays a similar role to polarization in electrostatics.
The vector...
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Potential Due to a Polarized Object01:29

Potential Due to a Polarized Object

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A neutral atom consists of a positively charged nucleus surrounded by a negatively charged electron cloud. When placed in an external electric field, the external electric force pulls the electrons and nucleus apart, opposite to the intrinsic attraction between the nucleus and the electrons. The opposing forces balance each other with a slight shift between the center of masses of the nucleus and the electron cloud, resulting in a polarized atom. On the other hand, a few molecules, like water,...
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相关实验视频

Updated: Dec 13, 2025

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一种基于物理学的方法可以预测即将发生的大型太阳耀斑

Kanya Kusano1, Tomoya Iju2, Yumi Bamba3,4

  • 1Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan. kusano@nagoya-u.jp.

Science (New York, N.Y.)
|August 1, 2020
PubMed
概括
此摘要是机器生成的。

一个新的基于物理的模型, κ-scheme,通过识别关键磁动力不稳定性,准确地预测了大型太阳耀斑. 这种模型使用磁扭流密度来确定耀斑的发生,位置和大小,从而改善太空天气预报.

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科学领域:

  • * 太阳物理
  • * 太空天气
  • *等离子体物理

背景情况:

  • * 太阳耀斑是对地球太空天气产生影响的有活力的冠状体事件.
  • *目前的太阳耀斑预测依赖于经验方法,
  • 了解火焰触发器对于改善预测能力至关重要.

研究的目的:

  • * 引入基于物理的模型, κ-方案,用于预测大型太阳耀斑.
  • * 调查磁动力不稳定性和磁重新连接在爆发的作用.
  • * 确定确定耀斑发生,位置和大小的关键参数.

主要方法:

  • * 基于物理学的预测模型 κ-scheme 的开发.
  • 分析2008年至2019年的X级太阳耀斑 (太阳周期24).
  • * 检查极性反转线附近的磁扭流密度.

主要成果:

  • * κ模式成功预测了即将发生的大型太阳耀斑.
  • * 一些有限的耀斑是模型预测的例外.
  • * 极性逆变线附近的磁扭流密度是一个关键预测因素.

结论:

  • 这是一个基于物理的方法来预测太阳耀斑.
  • * 磁扭流密度是决定太阳耀斑特征的关键因素.
  • 这项研究有助于我们更好地了解太阳耀斑的机制和预测.