首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Comparisons between ion distributions retrieved from ENA images of the ring current and contemporaneous, multipoint ion measurements recorded in situ during the major magnetic storm of 15 May 2005
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Comparisons between ion distributions retrieved from ENA images of the ring current and contemporaneous, multipoint ion measurements recorded in situ during the major magnetic storm of 15 May 2005

机译:从环电流的ENA图像中检索到的离子分布与2005年5月15日的大磁暴期间现场记录的同期多点离子测量结果之间的比较

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The Neutral Atom Detector Unit (NUADU) aboard the TC-2 spacecraft recorded energetic neutral atom (ENA) image data for >3 h during part of the main and recovery phases of a major magnetic storm on 15 May 2005. A custom designed, constrained linear inversion method was applied to retrieve ring current ion distributions in the ENA records out to L = 6.6. Comparisons were then made between the ion fluxes retrieved from these ENA data (energy ranges 50-81 keV and 81-158 keV) and complementary, contemporaneous particle fluxes measured in situ by Synchronous Orbit Particle Analyzer (SOPA) instruments aboard a series of geosynchronous satellites that were launched to encircle the equatorial plane at L ~ 6.6 by the Los Alamos National Laboratory (LANL), The ENA data revealed the development of two emission peaks during the main phase of the storm which corresponded to the arrival from the magnetotail of a pair of particle injections. These injections reached, in each case, maximum value before the corresponding AL index amplitude peak was attained. The main phase of the storm concluded (Dst≈-256 nT) in the aftermath of this event pair, and the ring current ion fluxes thereafter gradually decayed over several hours (the storm recovery phase), This is the first time that the linear inversion method developed for NUADU data has been globally validated using multipoint in situ measurements made at different magnetic local times. It was found that the higher the derived flux values were on the dusksideightside, the closer they were to the in situ measurements. The retrieved fluxes obtained on the dusksideightside tended, however, to be still somewhat underestimated since the ENA measurements concerned were made around the outer edge of the ring current at an altitude where the magnetic field in the inner magnetosphere deviates from that dipole configuration assumed in the inversion procedure to pertain there. The two methods utilized to study ions during a large magnetic storm are complementary in that the retrieved ion fluxes provide high time resolution information concerning the changing, large-scale structure of ring current events, whereas in situ flux sampling presents "measurement truth" at particular locations within individual ring currents.
机译:TC-2航天器上的中性原子探测器单元(NUADU)在2005年5月15日的一次大磁暴的主要阶段和恢复阶段记录了大于3小时的高能中性原子(ENA)图像数据。应用线性反演方法检索ENA记录中的环电流离子分布,得出L = 6.6。然后,对从这些ENA数据(能量范围50-81 keV和81-158 keV)中检索到的离子通量与由一系列地球同步卫星上的同步轨道粒子分析仪(SOPA)仪器现场测量的互补,同期粒子通量之间进行了比较。洛斯阿拉莫斯国家实验室(LANL)发射了L〜6.6环绕赤道平面的卫星,ENA数据显示,在风暴的主要阶段出现了两个发射峰的发展,这对应于一对磁尾的到达粒子注射。在每种情况下,在达到相应的AL指数振幅峰值之前,这些注入均达到最大值。在该事件对之后,风暴的主要阶段结束(Dst≈-256nT),此后环流离子通量在几个小时内逐渐衰减(风暴恢复阶段),这是线性反转第一次为NUADU数据开发的方法已使用在不同磁性当地时间进行的多点原位测量得到了全球验证。已发现,在黄昏/夜晚获得的通量值越高,它们与现场测量值越接近。但是,在黄昏/夜晚获得的恢复通量往往仍被低估了,因为有关ENA的测量是在内部磁层中的磁场偏离假定偶极子构型的高度上,在环流的外边缘附近进行的。在反演程序中涉及到。在大磁暴期间用于研究离子的两种方法是互补的,因为检索到的离子通量提供了有关环流事件的变化的大规模结构的高分辨率信息,而原位通量采样特别提供了“测量真相”单个环流中的位置。

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