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相关概念视频

Magnetic Field Lines01:19

Magnetic Field Lines

4.1K
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:
4.1K
Magnetic Field of a Solenoid01:18

Magnetic Field of a Solenoid

3.8K
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...
3.8K
Magnetic Field due to Moving Charges01:23

Magnetic Field due to Moving Charges

8.5K
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...
8.5K
Magnetic Field Of A Current Loop01:16

Magnetic Field Of A Current Loop

4.4K
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.
4.4K
Magnetic Vector Potential01:15

Magnetic Vector Potential

573
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...
573
Magnetic Field Due To A Thin Straight Wire01:28

Magnetic Field Due To A Thin Straight Wire

4.8K
Consider an infinitely long straight wire carrying a current I. The magnetic field at point P at a distance a from the origin can be calculated using the Biot-Savart law.
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相关实验视频

Updated: Jun 13, 2025

Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures
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使用齐曼效应绘制太阳冠状磁场的地图.

Thomas A Schad1, Gordon J D Petrie2, Jeffrey R Kuhn3

  • 1National Solar Observatory, 22 'Ōhi'a Kū Street, Makawao, HI 96768, USA.

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|September 11, 2024
PubMed
概括

科学家们使用先进的冠状图学创建了太阳在冠冕中的磁场的新地图. 这些前所未有的测量为太阳风,冠状热和太空天气预报提供了关键的见解.

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科学领域:

  • * 太阳物理 太阳物理
  • * 天体物理学 * 天体物理学
  • * 太空天气 * 太空天气

背景情况:

  • * 太阳冠状磁场的遥感有限,阻碍了对冠状热,太阳风发电和能量释放事件的研究.
  • *了解太阳的磁场对于预测太阳耀斑和喷发现象至关重要.

研究的目的:

  • * 开发和演示一种用于绘制太阳冠冕磁场的新方法.
  • * 为太阳冠状的磁动力学 (MHD) 模型提供观测约束.
  • * 改进太空天气研究和预报.

主要方法:

  • *利用了大光圈太阳光冠冕仪的进展.
  • * 测量了在1074nm时被Fe+12离子在活跃的冠状状体中发射的偏光谱.
  • * 检测到的泽曼效应信号表明冠状磁场.

主要成果:

  • *从活跃的太阳冠冕生成了前所未有的极化光谱图.
  • * 确定了泽曼效应的明确特征,与冠状磁场直接相关.
  • *为验证和限制全球MHD模型提供了有价值的观测数据.

结论:

  • *这项新技术提供了一种强大的工具,用于对冠状磁场的遥感.
  • *这些测量显著提升了我们研究冠状热和太阳风的能力.
  • *根据这些发现改进的冠状模拟将增强空间天气预报能力.