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相关概念视频

Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

682
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
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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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Atomic Nuclei: Nuclear Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

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All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
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Magnetic Fields01:27

Magnetic Fields

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A moving charge or a current creates a magnetic field in the surrounding space, in addition to its electric field. The magnetic field exerts a force on any other moving charge or current that is present in the field. Like an electric field, the magnetic field is also a vector field. At any position, the direction of the magnetic field is defined as the direction in which the north pole of a compass needle points.
A magnetic field is defined by the force that a charged particle experiences...
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Magnetic Field due to Moving Charges01:23

Magnetic Field due to Moving Charges

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A stationary charge creates and interacts with the electric field, while a moving charge creates a magnetic field.
Consider a point charge moving with a constant velocity. Like the electric field, the magnetic field at any point is directly proportional to the magnitude of the charge and inversely proportional to the square of the distance between the source point and the field point. However, unlike the electric field, the magnetic field is always perpendicular to the plane containing the line...
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Updated: Jul 23, 2025

Scattering And Absorption of Light in Planetary Regoliths
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宇宙射线和随机的磁陷

Devika Tharakkal1, Andrew P Snodin1, Graeme R Sarson1

  • 1School of Mathematics, Statistics and Physics, Newcastle University, Newcastle upon Tyne, NE1 7RU, United Kingdom.

Physical review. E
|July 19, 2023
PubMed
概括
此摘要是机器生成的。

在星际介质 (ISM) 中宇宙射线 (CR) 的分布受到磁场的影响. 模拟显示源变化和能量损失产生持久的CR团,影响天体物理解释.

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Last Updated: Jul 23, 2025

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科学领域:

  • 天体物理学 天体物理学
  • 无线电天文学 无线电天文学

背景情况:

  • 在星际介质 (ISM) 中宇宙射线 (CR) 的分布对射电天文学和理论天体物理学至关重要.
  • 当地磁场变化影响CR粒子动力学和扩散性.
  • 磁陷可以在CR空间分布中创建持久特征.

研究的目的:

  • 研究宇宙射线粒子在各种磁场配置中的空间分布.
  • 了解磁场结构对CR粒子行为的影响.
  • 分析CR源不均质和能量损失对其分布的影响.

主要方法:

  • 使用了试验粒子模拟.
  • 研究了质子和电子的组合.
  • 采用各种磁场配置,从理想化的陷到随机场.

主要成果:

  • 证明了CR源不均性和能量损失导致局部CR分布不均性的持续性.
  • 展示了质子和电子的独特空间分布.
  • 突出了磁陷在塑造CR分布中的作用.

结论:

  • 磁场结构和粒子特性对CR空间分布有很大的影响.
  • 这些发现对解释同步子发射及其波动有影响.
  • 该研究提供了关于CR和ISM之间的复杂相互作用的见解.