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Kinematic MHD Models of Collapsing MagneticTraps: Extension to 3D

机译：折叠函数的运动MHD模型：扩展到3D

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We show how fully 3D kinematic MHD models of collapsing magnetic traps (CMTs) canbe constructed, thus extending previous work on 2D trap models. CMTs are thought to form in therelaxing magnetic field lines in solar flares and it has been proposed that they play an important rolein the acceleration of high-energy particles. This work is a first step to understanding the physics ofCMTs better.

机译：我们展示了完全3D运动MHD模型的折叠磁阱（CMTS）建造，从而在2D陷阱模型上延伸了先前的工作。 CMTS被认为在太阳光晕的其上形成的磁场线，并且已经提出了它们在高能量颗粒的加速度发挥重要作用。这项工作是了解物理学的第一步。

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《Cambridge Workshop on Cool Stars, Stellar Systems and the Sun 》|2009年||共4页
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Keith J. Grady; Thomas Neukirch;
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中图分类 P151-532;
关键词
Acceleration of particles; Sun: flares;

机译：粒子加速;太阳：耀斑;

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Kinematic MHD Models of Collapsing MagneticTraps: Extension to 3D

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