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相关概念视频

Magnetic Fields01:28

Magnetic Fields

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...
Magnetic Field Lines01:19

Magnetic Field Lines

The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
Magnetic Field of a Solenoid01:18

Magnetic Field of a Solenoid

A solenoid is a conducting wire coated with an insulating material, wound tightly in the form of a helical coil. The magnetic field due to a solenoid is the vector sum of the magnetic fields due to its individual turns. Therefore, for an ideal solenoid, the magnetic field within the solenoid is directly proportional to the number of turns per unit length and the current. Conversely, the magnetic field outside the solenoid is zero.
Consider a solenoid with 100 turns wrapped around a cylinder of...
Atomic Nuclei: Nuclear Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

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...
Magnetic Flux01:19

Magnetic Flux

The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Magnetic Field Of A Current Loop01:16

Magnetic Field Of A Current Loop

Consider a circular loop with a radius a, that carries a current I. The magnetic field due to the current at an arbitrary point P along the axis of the loop can be calculated using the Biot-Savart law.

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相关实验视频

Updated: Jul 11, 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

土星的磁场和磁层.

E J Smith, L Davis, D E Jones

    Science (New York, N.Y.)
    |January 25, 1980
    PubMed
    概括

    开拓者土星磁力表显示,土星的磁场比预期的要弱,其磁轴和旋转轴之间几乎是完美的对齐. 这表明行星核心较小,并提供了关于土星磁层动态的见解.

    科学领域:

    • 行星科学 行星科学
    • 磁层物理 磁层物理
    • 空间物理 空间物理

    背景情况:

    • 在开拓者任务之前,土星的磁层和内部磁场属性并没有得到很好的理解.
    • 以前对土星磁场强度的估计是基于地球和木星的缩放.

    研究的目的:

    • 为了准确地描述土星的行星磁场,使用开拓者土星矢量磁仪的数据.
    • 研究土星磁层的结构和动态及其与太阳风的相互作用.

    主要方法:

    • 通过先土星矢量磁仪进行现场测量.
    • 磁场数据的球体波分析.
    • 观察到的场状特征与理论模型和来自其他行星的数据进行比较.

    主要成果:

    • 探测土星的弓冲击和磁停止.
    • 测量到的赤道表面磁场为0.20高斯,比预期弱3-5倍.
    • 观察到双极轴倾斜角度<1度,表明与旋转轴的异常对齐.
    • 球体波分析显示四极与二极矩比率<10%,表明更均的场和更小的核心.
    • 从外部磁层的纯二极子场系统偏差,包括在中午附近的压缩和黎明附近的赤道电流板.
    • 证据表明,水磁波可能是由泰坦与磁层相互作用引起的.

    更多相关视频

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    相关实验视频

    Last Updated: Jul 11, 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

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    结论:

    • 土星的磁场比预测的要弱得多,而且比预测的更加均,这意味着它的核心相对较小.
    • 磁层表现出复杂的结构和动态,包括与泰坦等卫星的相互作用.
    • 开拓者的发现为改进行星磁场和磁层模型提供了至关重要的数据.