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Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

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...
Magnetism01:30

Magnetism

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...
Magnetic Vector Potential01:15

Magnetic Vector Potential

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...
Energy In A Magnetic Field01:24

Energy In A Magnetic Field

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 negligible.
The energy...
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:
Potential Due to a Polarized Object01:29

Potential Due to a Polarized Object

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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Updated: Jun 6, 2026

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

来自一个巨大的原恒星的磁性喷气.

Carlos Carrasco-González1, Luis F Rodríguez, Guillem Anglada

  • 1Instituto Astrofísica Andalucía, Consejo Superior de Investigaciones Científicas (CSIC), Camino Bajo de Huétor 50, E-18008 Granada, Spain. charly@iaa.es

Science (New York, N.Y.)
|November 27, 2010
PubMed
概括

研究人员在年轻的恒星物体喷射中发现了极化同步子辐射,类似于活跃的银河系核喷射. 这表明所有天体物理喷气的共同起源,为喷气形成和磁场提供了新的见解.

科学领域:

  • 天体物理学 天体物理学
  • 等离子体物理学的物理学

背景情况:

  • 同步子发射是一种已知的现象,来自活跃星系核 (AGN) 和微类星体的喷射.
  • 从年轻的恒星天体 (YSOs) 喷射中出现同步子发射的存在以前没有得到证实.

研究的目的:

  • 为了提供YSO喷气中极化同步子发射的证据.
  • 为了研究YSO喷气体内的磁场特性和配置.
  • 将YSO喷气机的特性与AGN喷气机的特性进行比较.

主要方法:

  • 使用极化测量的观测天文学.
  • 对同步发射辐射特性进行分析.
  • 磁场强度和方向的确定.

主要成果:

  • 在YSO喷气中检测到极化同步子发射的证据.
  • 表面磁场强度大约为0.2毫瓦斯,与喷气轴对齐.
  • 向喷射边缘增加极化度,与螺旋式磁场一致.

结论:

  • 这些发现为YSO喷气式飞机中的同步子发射提供了第一个证据.
  • 观察到的特征类似于AGN喷气的特征,这表明天体物理喷气的统一模型.

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Cryogenic Liquid Jets for High Repetition Rate Discovery Science
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Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

Simultaneous Synthesis of Single-walled Carbon Nanotubes and Graphene in a Magnetically-enhanced Arc Plasma
09:48

Simultaneous Synthesis of Single-walled Carbon Nanotubes and Graphene in a Magnetically-enhanced Arc Plasma

Published on: February 2, 2012

相关实验视频

Last Updated: Jun 6, 2026

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
11:47

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

Cryogenic Liquid Jets for High Repetition Rate Discovery Science
08:34

Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

Simultaneous Synthesis of Single-walled Carbon Nanotubes and Graphene in a Magnetically-enhanced Arc Plasma
09:48

Simultaneous Synthesis of Single-walled Carbon Nanotubes and Graphene in a Magnetically-enhanced Arc Plasma

Published on: February 2, 2012

  • 这意味着所有天体物理喷射的形成和演变背后有一个共同的物理机制.