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メッセンジャー (MESSENGER) は,水星の磁気圏における磁気再接続の観測を行った
James A Slavin1, Mario H Acuña, Brian J Anderson
1Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. james.a.slavin@nasa.gov
まとめ
水星の磁気圏は太陽風のエネルギー伝送に非常に反応し,磁気再接続は地球の約10倍の速度で起こります. これは,宇宙天候に対する惑星のより大きな感受性を示している.
科学分野:
- 惑星科学は惑星科学である.
- 宇宙物理学 宇宙物理学
- マグネトヒドロダイナミクス
背景:
- 惑星の磁気圏への太陽風のエネルギー転送は,磁気再接続によって制御されます.
- 磁気再接続は,惑星間磁場 (IMF) と惑星の磁場との接続性を決定する.
研究 の 目的:
- MESSENGERミッション中に水星における磁気再接続の速度と効果を調査する.
- IMFの変動に対する水星の磁気圏反応と地球の磁気圏反応を比較する.
主な方法:
- メッセンジャー号の水星の第2回フライトバイのデータ分析.
- 惑星間磁場 (IMF) と水星の磁気圏の観測.
主要な成果:
- 安定した南向きのIMFと,強い磁場による磁気断絶が観測されました.
- 水星での再接続率は,地球で典型的なものより約10倍高いと推定されました.
- 大量の流量移転イベント,プラズモイド,移動圧縮領域を含む再接続製品の証拠は,水星の磁気尾に検出されました.
結論:
- 水星の磁気圏は,地球の磁気化惑星や他の磁気化惑星よりも,IMFの方向性に著しく反応します.
- 惑星の磁気圏は,磁気再接続の効果によって支配されています.
- 水星は,再接続が強化されたため,より高い太陽風エネルギー転送を経験します.
関連する概念動画
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:
Magnetic Fields
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...
A magnetic field is defined by the force that a charged particle experiences...
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 Flux
The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
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...
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Potential Due to a Magnetized Object
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The vector...
The vector...