地球磁层顶通量传输事件的轴向研究
[Abstract]:The magnetopause flux transmission event (Flux Transfer Event,FTE) is considered to be a phenomenon related to the reconnection of the magnetic field, which is marked by the bipolar variation of the normal component of the magnetic field measured by the satellite at the top of the magnetopause. So far, there are still some debates about the essence, formation mechanism and location of FTE. It is necessary to determine the axial direction of FTE not only to study the geometric structure of FTE and to understand the plasma dynamics, but also to help us distinguish the different formation mechanism and generation position of FTE. In this paper, the axial research of FTE is taken as the main line, and the main contents and conclusions are summarized as follows: (1) A new multi-point analysis method is developed to determine the axial direction of FTE. This method is based on the pure geometric assumption that the structure is left and right symmetry. For the FTE structure embedded in the magnetopause current sheet, regardless of its physical properties, it basically satisfies this symmetry condition, so the new method has a wide range of applications. The model test and practical application show that, The new method is more effective and reliable in determining the axial direction than the traditional methods such as Grad-Shafranov (GS) method and magnetic field minimum variance analysis method, as well as the closer method based on cylindrical symmetry. (2) the axial and coincidence of FTE are determined. Under the suitable multi-satellite configuration, A new method is designed to reconstruct the spatial distribution of FTE magnetic field. The application of this method to the two FTE observed by THEMIS and Cluster respectively shows that it can reconstruct the magnetic field spatial distribution of the structure quickly and effectively, thus helping us to speculate the magnetic field configuration of the structure. Understand the time variation of satellite measurement data and obtain the spatial distribution characteristics of other physical quantities relative to the structural magnetic field. (3) the first statistical analysis of FTE axis is carried out by using the new FTE axial determination method. The results show that although most of the FTE observed in the low latitudes of the fainting side have an axial direction close to the north and south, the source is still the subsolar component reconnection line. Different from the traditional understanding that the Japanese and lower point component reconnection line is a separation line with almost unchanged direction, the actual diurnal point component reconnection line has considerable curvature at the top of the magnetosphere. (4) for the first time, it is found that the magnetic field signal of FTE is formed by multi-X-ray reconnection. GS reconstruction results show that there are multiple substructures in events with such magnetic signals, which is consistent with the pattern of multiple flux tubes formed by reconnection of multiple X-rays. However, the substructures are arranged sequentially from large to small on the top of the magnetosphere, which is not predicted by the traditional multi-X-ray reconnection model. In order to explain this phenomenon, we propose a new model to describe the formation process of FTE: reconnection continues to occur at the top of the magnetosphere and forms a cuneiform configuration in the magnetic field near the main X-ray; The reconnection rate changes periodically, and a continuous number of small island structures are formed by tearing mode instability in the cuneiform magnetic field line as it grows. These small magnetic island structures merge with each other, and due to the limitation of the cuneiform magnetic field, they form a number of FTE, arranged in order by size. Finally, under the action of magnetic sheath flow pressure and magnetic tension, the reconnection position is left. (5) A series of continuous FTE. of "abnormal" diurnal motion measured in the low latitude magnetopause of the fainting side are analyzed. By comparing the velocity of the event with the FTE motion model, it can be found that the magnetic tension of the actual reconnected magnetic field is much larger than that given by the model in order to counter the larger wake magnetic sheath velocity near the dizzy side magnetopause at this time. This shows that when the magnetohydrodynamic effect may play an important role, the existing model can not accurately describe the magnetic field and plasma environment, so it needs to be modified.
【学位授予单位】:中国科学院国家空间科学中心
【学位级别】:博士
【学位授予年份】:2017
【分类号】:P353
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