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相关概念视频

Atomic Nuclei: Magnetic Resonance01:05

Atomic Nuclei: Magnetic Resonance

The number of nuclear spins aligned in the lower energy state is slightly greater than those in the higher energy state. In the presence of an external magnetic field, as the spins precess at the Larmor frequency, the excess population results in a net magnetization oriented along the z axis. When a pulse or a short burst of radio waves at the Larmor frequency is applied along the x axis, the coupling of frequencies causes resonance and flips the nuclear spins of the excess population from the...
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

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. This...
NMR Spectrometers: Radiofrequency Pulses and Pulse Sequences01:17

NMR Spectrometers: Radiofrequency Pulses and Pulse Sequences

A pulse is a short burst of radio waves distributed over a range of frequencies that simultaneously excites all the nuclei in the sample. Upon passing a radio frequency pulse along the x-axis, the nuclei absorb energy corresponding to their Larmor frequencies and achieve resonance. This shifts the net magnetization vector from the z-axis toward the transverse plane. This angle of rotation of the magnetization vector, or the flip angle, is proportional to the duration and intensity of the pulse.
Motional Emf01:22

Motional Emf

Magnetic flux depends on three factors: the strength of the magnetic field, the area through which the field lines pass, and the field's orientation with respect to the surface area. If any of these quantities vary, a corresponding variation in magnetic flux occurs. If the area through which the magnetic field lines are passing changes, then the magnetic flux also changes. This change in the area can be of two types: the flux through the rectangular loop increases as it moves into the magnetic...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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. Nichols...
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...

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相关实验视频

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Hyperpolarized Xenon for NMR and MRI Applications
16:20

Hyperpolarized Xenon for NMR and MRI Applications

Published on: September 6, 2012

来自磁星的短暂脉冲无线电辐射.

Fernando Camilo1, Scott M Ransom, Jules P Halpern

  • 1Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, New York 10027, USA. fernando@astro.columbia.edu

Nature
|August 25, 2006
PubMed
概括

异常X射线脉冲星 (AXP) 或磁星已经被证明可以发射无线电脉冲,这是这些天体的首次. 这一发现将磁星与普通脉冲星联系起来,并为研究它们的磁场和冠状云开辟了新的途径.

科学领域:

  • * 天文学和天体物理学
  • * 高能天体物理学
  • * 中子星物理学

背景情况:

  • *异常X射线脉冲星 (AXP) 是具有超强磁场 (>10^14 G) 的中子星,称为磁星.
  • *磁星表现出明亮的,可变的X射线发射,但从未观察到发射无线电脉冲,与普通脉冲星不同.
  • *XTE J1810-197,一个AXP,在2003年显示出显著的X射线爆发,随后检测到无线电源.

研究的目的:

  • * 为了研究异常X射线脉冲星XTE J1810-197.7的无线电发射特性.
  • * 为了确定磁星是否可以表现出无线电脉冲星行为.
  • *将磁星观测与普通无线电脉冲星的观测联系起来.

主要方法:

  • *使用射电望远镜观测XTE J1810-197的无线电脉冲.
  • *分析检测到的无线电脉冲的特征,包括偏振和流量.
  • *将无线电发射特性与平常脉冲星和磁星在静止状态中的特性进行比较.

主要成果:

  • * 检测到XTE J1810-197在每次旋转时都会发出明亮,狭窄和高度线性偏振的无线电脉冲.
  • * 在2003年X-ray爆发之前,没有观察到XTE J1810-197的无线电辐射.

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A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
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A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

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Last Updated: May 8, 2026

Hyperpolarized Xenon for NMR and MRI Applications
16:20

Hyperpolarized Xenon for NMR and MRI Applications

Published on: September 6, 2012

How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters
08:42

How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters

Published on: April 16, 2015

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

A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

  • * XTE J1810-197的无线电流量每天都在变化,并且在无线电频率上几乎是恒定的,成为已知的20 GHz以上最亮的中子星.
  • 结论:

    • *磁星确实可以作为无线电脉冲星,弥合磁星和普通无线电脉冲星之间的差距.
    • *这些发现排除了AXP的其他基于积累的模型.
    • * 这些观测为磁星的磁层冠状提供了至关重要的见解.