Collaborative Research: Super-Alfvenic propagation of energy released during magnetic reconnection in the Earth's magnetotail

合作研究：地球磁尾磁重联过程中释放的能量的超亚芬尼传播

• 批准号: 1219369
• 负责人: James Drake
• 金额: $ 10.09万
• 依托单位: University of Maryland, College Park
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2013
• 资助国家: 美国
• 起止时间: 2013-09-01 至 2016-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1219369&HistoricalAwards=false
• 关键词: Collaborative; Research; Super; Alfvenic; propagation

Magnetic reconnection plays a fundamental role in magnetotail dynamics, reconfiguring magnetic topology to release stored magnetic energy. The nature of the energy propagating away from the reconnection site has implications for our understanding of transient magnetotail phenomena such as bursty bulk flows, dipolarization fronts and substorms. While bulk ion flows accelerated by reconnection have been measured directly by spacecraft and have been linked to the generation of aurora the propagation speed of this energy is limited to the Alfvén speed and there is evidence that energy must propagate faster than the Alfvén speed to account for substorm onset. Less well understood, however, are super-Alfvénic flows of energy associated with kinetic electron dynamics which tend to occur near the magnetic separatrices. The quadrupolar magnetic fields in this region associated with Hall dynamics have been shown to be the manifestation of a kinetic Alfvén wave (KAW) that propagates super-Alfvénically parallel to the magnetic field and generates substantial Poynting flux associated with energetic electron streams. This investigation will study the basic physics mechanisms controlling the super-Alfvénic propagation of reconnection energy with focus roughly on the mid-tail region. The study will use kinetic particle-in-cell simulations (PIC) and satellite observations of reconnection from the Cluster and THEMIS spacecraft. This should be a significant step towards understanding the causal relationships between reconnection onset and transient magnetotail phenomena such as bursty bulk flows, dipolarization fronts, and substorm onset. However the potential benefit of this research extends beyond magnetotail research because propagation of reconnection energy is an important problem for a wide range of natural plasmas and laboratory plasmas.

磁重联在磁尾动力学中起着重要的作用，重新配置磁拓扑以释放储存的磁能。从重连点传播的能量的性质对我们理解瞬变磁尾现象，如突发性整体流动，偶极锋和亚暴有影响。虽然宇宙飞船直接测量了重连加速的大量离子流，并将其与极光的产生联系起来，但这种能量的传播速度仅限于阿尔文速度，而且有证据表明，能量的传播速度必须快于阿尔文速度，才能解释亚暴的发生。然而，人们对超阿尔夫文能流的了解较少，它与倾向于发生在磁分界线附近的动力学电子动力学有关。与霍尔动力学相关的该区域中的四极磁场已被证明是动力学阿尔文波（KAW）的表现，其平行于磁场超阿尔文传播，并产生与高能电子流相关的大量坡印廷通量。本研究将研究控制重联能量超阿尔夫文传播的基本物理机制，重点大致集中在中尾区域。这项研究将使用动力学粒子模拟（PIC）和来自星团和THEMIS航天器的重连卫星观测。这应该是一个重要的一步，了解之间的因果关系的重联发病和瞬态磁尾现象，如突发散装流量，偶极锋，亚暴发病。然而，这项研究的潜在好处超出了磁尾研究，因为重联能量的传播是一个重要的问题，为广泛的自然等离子体和实验室等离子体。