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Long and Active Magnetopause Reconnection X-Lines During Changing IMF Conditions

机译:长和主动磁重联x轴在不断变化的国际货币基金组织的条件

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The magnetic reconnection process at the Earth's magnetopause is observed at various times and places as either anti-parallel or component reconnection. The two scenarios are combined in a model known as the Maximum Magnetic Shear model, which predicts the location of long and continuous reconnection X-lines across the dayside magnetopause along the ridge of maximum magnetic shear. This study investigates a Magnetospheric Multiscale Mission (MMS) magnetopause encounter where the spacecraft had repeated contact with the boundary layers for about 40 min. While in contact with the magnetopause boundary layers, the Interplanetary Magnetic Field (IMF) slowly and continuously rotated,magnetically connecting the MMS spacecraft to different sections along an extended dayside reconnection X-line. These magnetic connection points slide along component reconnection tilted X-lines and also connect several times to the anti-parallel section of the magnetopause X-line. Despite the continuously changing IMF conditions, each magnetopause boundary layer encounter shows accelerated ion beams,indicating an active reconnection X-line at the magnetopause that covers a length of about 20 R_E.
机译:地球的磁场重联过程磁层观察到在不同时期作为反平行或组件的地方重新连接。模型被称为最大磁剪切模型,预测长期的位置在哪里吗连续重联的x轴沿着山脊的光面磁层的最大值磁剪切。磁性层的多尺度任务(MMS)磁层遇到的航天器重复接触层的边界大约40分钟。而在接触磁层边界层,星际慢慢地、不断地磁场(IMF)旋转,磁连接MMS沿着一个航天器不同部分扩展的光面重新连接x轴。磁连接点滑动组件重新连接倾斜x轴连接几次的反并行的部分磁层x轴。国际货币基金组织环境变化,每个磁层边界层遇到显示加速离子梁,表明一个活跃的重新连接x轴磁层覆盖的长度约为20R_E。

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