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関連する概念動画

Magnetic Fields01:27

Magnetic Fields

6.0K
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...
6.0K
Magnetic Field Lines01:19

Magnetic Field Lines

5.4K
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:
5.4K
Magnetic Field due to Moving Charges01:23

Magnetic Field due to Moving Charges

11.3K
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...
11.3K
Magnetic Field of a Solenoid01:18

Magnetic Field of a Solenoid

5.6K
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...
5.6K
Magnetostatic Boundary Conditions01:28

Magnetostatic Boundary Conditions

1.9K
An electric field suffers a discontinuity at a surface charge. Similarly, a magnetic field is discontinuous at a surface current. The perpendicular component of a magnetic field is continuous across the interface of two magnetic mediums. In contrast, its parallel component, perpendicular to the current, is discontinuous by the amount equal to the product of the vacuum permeability and the surface current. Like the scalar potential in electrostatics, the vector potential is also continuous...
1.9K
Magnetic Damping01:17

Magnetic Damping

1.3K
Eddy currents can produce significant drag on motion, called magnetic damping. For instance, when a metallic pendulum bob swings between the poles of a strong magnet, significant drag acts on the bob as it enters and leaves the field, quickly damping the motion.
If, however, the bob is a slotted metal plate, the magnet produces a much smaller effect. When a slotted metal plate enters the field, an emf is induced by the change in flux; however, it is less effective because the slots limit the...
1.3K

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

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太陽風の終結ショックにおける磁場

L F Burlaga1, N F Ness, M H Acuña

  • 1NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA. Leonard.F.Burlaga@nasa.gov

Nature
|July 4, 2008
PubMed
まとめ

ボイジャー2号は,終結ショックの複雑で波紋状の構造を観察し,そのダイナミックな再構成を明らかにした. この発見は,この境界を形作る上で,イオン化された恒星間原子,またはピックアップ陽子の重要な役割を強調しています.

科学分野:

  • ヘリオフィジックスと宇宙物理学
  • プラズマ物理学 プラズマ物理学
  • マグネトヒドロダイナミクス

背景:

  • ボイジャー1号は以前,超音速の太陽風から亜音速の太陽風への移行を観測した.
  • ヘリオスフィアの終結ショック (TS) はこの境界をマークしますが,データギャップのため,ボイジャー1によって直接観測されませんでした.

研究 の 目的:

  • ヘリオスフィアの終結ショックの磁場構造と動態を調査するために.
  • 詳細なin-situ測定を用いて,TSの交差点の性質を理解する.

主な方法:

  • ヴォイジャー2号からの磁場データの分析.
  • 観測期間:2007年8月31日~9月1日,太陽から83.7天文学単位 (au) 離れた場所.

主要な成果:

  • ヴォイジャー2号は,複雑な波紋状,準垂直の超臨界磁気水力ダイナミックショックに遭遇した.
  • 終結ショックは,安定した境界の期待とは対照的に,数時間のスケールでリフォームを示した.
  • 観測された衝撃構造は,イオン化された恒星間原子 (ピックアップ陽子) が有意な影響を及ぼすことを示唆しています.

結論:

さらに関連する動画

Optimizing Magnetic Force Microscopy Resolution and Sensitivity to Visualize Nanoscale Magnetic Domains
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Optimizing Magnetic Force Microscopy Resolution and Sensitivity to Visualize Nanoscale Magnetic Domains

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Author Spotlight: Simulation and Analysis of the Temperature Rise of Ring Main Unit Equipment
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Author Spotlight: Simulation and Analysis of the Temperature Rise of Ring Main Unit Equipment

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関連する実験動画

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

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Optimizing Magnetic Force Microscopy Resolution and Sensitivity to Visualize Nanoscale Magnetic Domains
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Optimizing Magnetic Force Microscopy Resolution and Sensitivity to Visualize Nanoscale Magnetic Domains

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Author Spotlight: Simulation and Analysis of the Temperature Rise of Ring Main Unit Equipment
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Author Spotlight: Simulation and Analysis of the Temperature Rise of Ring Main Unit Equipment

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  • ヘリオスフィアの終端ショックは,動的で複雑な構造であり,安定した境界線ではありません.
  • ピックアッププロトンは,衝撃のリフォームと全体的な構造において重要な役割を果たします.
  • これらの発見は,太陽風と恒星間介質の相互作用に関する重要な洞察を提供します.