1986年7月8日のマグニチュード5.9のパームスプリングス北部地震の地震磁気観測
まとめ
1986年のノース・パームスプリングス地震の後に地震磁気偏移が観測されました. これらの永久磁場の変化は,難解な地震磁気効果の最初の直接的な証拠を提供します.
科学分野:
- 地質物理学 地質物理学とは地質物理学です.
- 地震学 地震学とは
- 地磁気学とは地磁気学である.
背景:
- サンアンドレアス断層は磁気計配列によって監視され,地震磁気効果を検出します.
- 地震磁気効果,または地震による磁場の変化は,長い間予期されてきましたが,めったに観測されていません.
研究 の 目的:
- 地震磁気偏移の最初の直接観測を報告する.
- 観測された地震磁気オフセットの特性を分析し,地震モデルと比較する.
主な方法:
- サンアンドレアス断層に沿って動作する24個の陽子磁気計の微分的に接続された配列を利用した.
- 1986年のノース・パームスプリングス地震の前と後の磁場データを記録した.
主要な成果:
- 観測された地震磁気偏移は,それぞれ3kmと9kmの震源距離で1.2と0.3ナノテスラであった.
- 観測されたオフセットは,バンニング断層の右側20cmの破裂を含む地震磁気モデルと一致しています.
- 観測された磁気変化は恒常的で,20分以内に完了した.
結論:
- この研究は,地震磁気効果の最初の直接的な証拠を提供します.
- このデータは,地震による磁場変化の物理モデルを裏付けている.
- 観測された永久磁場の変化の説明は,電動力学的な効果ではありそうにない.
関連する概念動画
Magnetostatic Boundary Conditions
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...
Magnetic Susceptibility and Permeability
In linear magnetic materials, like paramagnets and diamagnets, magnetization is proportional to the magnetic field intensity. The constant of proportionality, a dimensionless number, is called magnetic susceptibility. The value of the susceptibility depends on the type of material.
When diamagnetic materials are placed under an external magnetic field, the moments opposite to the field are induced. Hence, the susceptibility for diamagnets has a minimal negative value of 10-5–10-6. Since...
When diamagnetic materials are placed under an external magnetic field, the moments opposite to the field are induced. Hence, the susceptibility for diamagnets has a minimal negative value of 10-5–10-6. Since...
Magnetic Declination
Magnetic declination is the angle between true north, which aligns with the Earth's rotational axis, and magnetic north, which follows the direction of the Earth's magnetic field. This discrepancy exists because the magnetic poles do not coincide with the geographic poles. The value of magnetic declination depends on the observer's location on Earth and is subject to changes over time due to the dynamic nature of the Earth's magnetic field.The declination is called eastern when magnetic north...
Magnetic Damping
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...
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...
Magnetic Force
In addition to the electric forces between electric charges, moving electric charges exert magnetic forces on each other. A magnetic field is created by a moving charge or a group of moving charges known as the electric current. A magnetic force is experienced by a second current or moving charge in response to this magnetic field. Fundamentally, interactions between moving electrons in the atoms of two bodies produce magnetic forces between them.
The magnetic force acting on a moving charge...
The magnetic force acting on a moving charge...
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:
Magnetic field lines follow several hard-and-fast rules:

