北部尖顶重叠双离子能量弥散事件的统计分析

D. E. da Silva, L. J. Chen, S. Fuselier, S. Petrinec, K. Trattner, G. Cucho-Padin, H. K. Connor, B. L. Burkholder, A. J. Huntenburg
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引用次数: 0

摘要

本文介绍了对北侧尖顶重叠的双重离子能量散布事件("双重散布")的统计分析。任一尖顶的双扩散现象都与日侧磁层与多变的太阳风不断相互作用而发生的多次重新连接有关。利用低地球轨道(LEO)国防气象卫星计划(DMSP)卫星的观测数据,我们分析了从以前的工作中扩展的自动算法选出的 138 个日侧事件。我们对检测到的双扩散事件数量与以下两个因素进行了相关性研究:1)年份月份,以分析尖顶的季节性响应;2)太阳风行星际磁场(IMF)成分和时钟/圆锥角,以研究其与磁重联的关系。我们发现,频散事件更频繁地发生在北部夏季(即偶极子向太阳倾斜时),以及行星际磁场的By分量为正时。此外,我们还提供了一份机器可读的事件列表以及用于自动检测事件的代码。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Statistical analysis of overlapping double ion energy dispersion events in the northern cusp
This article presents a statistical analysis of overlapping double ion-energy dispersion events in the northern cusp (“double dispersion”). Double dispersion in either cusp is a phenomenon associated with multiple reconnections occurring on the dayside magnetosphere as a result of its constant interaction with the variable solar wind. Using observations from a low Earth orbiting (LEO) Defense Meteorological Satellite Program (DMSP) satellite, we analyze 138 dayside events selected by the automatic algorithm extended from our previous work. We conducted a correlation study between the number of detected double dispersion events and 1) the month of the year to analyze the seasonal response of the cusp, and 2) solar wind interplanetary magnetic field (IMF) components and clock/cone angles to investigate its relationship with magnetic reconnection. We found that dispersion events occur more frequently during the northern summer months (i.e., when the dipole is tilted Sunward) and when the By component of IMF is positive. In addition, we provide a machine-readable list of the events and the code used to automatically detect the events.
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