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相关概念视频

Magnetism01:30

Magnetism

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Magnets are commonly found in everyday objects, such as toys, hangers, elevators, doorbells, and computer devices. Experimentation on these magnets shows that all magnets have two poles: one is labeled north (N) and the other south (S). Magnetic poles repel if they are alike and attract if unlike. Moreover, both poles of a magnet attract unmagnetized pieces of iron.
An individual magnetic pole cannot be isolated. No matter how small, every piece of a magnet contains a north pole and a south...
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Magnetic Field Lines01:19

Magnetic Field Lines

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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:
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Energy In A Magnetic Field01:24

Energy In A Magnetic Field

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If a magnetic field is sustained, there must be a current in a closed circuit or loop, implying some energy has been spent in creating the field. If this energy is not dissipated via the circuit's resistance, it is stored in the field.
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus...
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Divergence and Curl of Magnetic Field01:26

Divergence and Curl of Magnetic Field

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The magnetic field due to a volume current distribution given by the Biot–Savart Law can be expressed as follows:
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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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Magnetic Vector Potential01:15

Magnetic Vector Potential

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In electrostatics, the electric field can be written as the negative gradient of the potential. In magnetostatics, the zero divergence of the magnetic field ensures that the magnetic field can be expressed as the curl of a vector potential. This potential is known as the magnetic vector potential.
Consider an ideal solenoid with n turns per unit length and radius R. If I is the current through the solenoid, the magnetic field inside the solenoid is expressed as the product of vacuum...
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相关实验视频

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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来自一个进化的恒星的磁性聚合喷气.

Wouter H T Vlemmings1, Philip J Diamond, Hiroshi Imai

  • 1Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK. wouter@jb.man.ac.uk

Nature
|March 3, 2006
PubMed
概括
此摘要是机器生成的。

观察到磁场与来自一个进化的恒星的喷气相结合,解释了行星星云的不对称形状. 这项研究提供了磁场对恒星喷射的影响的第一个直接证据.

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科学领域:

  • 天文学和天体物理学
  • 恒星进化 恒星进化
  • 磁动力学是一种磁动力学.

背景情况:

  • 行星星云往往表现出不对称的形状,这种现象不易被对称的祖先恒星解释.
  • 理论模型表明,进化恒星的聚合喷射可能导致这些不对称性.
  • 假设磁场是这些喷射的首要结合机制,类似于它们在活跃的星系核和原恒星外流中的作用.

研究的目的:

  • 为磁场在恒星喷射的结合中的作用提供直接的观测证据.
  • 为了研究非对称巨型分支恒星W43A.的预处理喷气中的磁场特性.

主要方法:

  • 测量水蒸气质量仪极化被用来探测磁场.
  • 观察集中在位于W43A.喷射的尖端的巨星星团上.
  • 该研究分析了喷气体内的磁场的方向和强度.

主要成果:

  • 这项研究成功地测量了W43A恒星喷射中水蒸气质子的极化.
  • 这些巨星被发现在两个星团中,位于相反的喷射尖端,距离恒星大约有1000天文单位.
  • 数据表明存在显著的磁场,并对齐以聚合喷气.

结论:

  • 这些发现提供了第一个直接的观测证据,证明磁场与天体物理喷气相结合.
  • 这证实了磁场在行星星云形成过程中发挥关键作用的假设.
  • 这项研究促进了我们对恒星进化的后期阶段和进化恒星流出的物理学的理解.