首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Pitch angle distribution analysis of radiation belt electrons based on Combined Release and Radiation Effects Satellite Medium Electrons A data
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Pitch angle distribution analysis of radiation belt electrons based on Combined Release and Radiation Effects Satellite Medium Electrons A data

机译:螺旋角的辐射分布分析基于联合释放和带电子卫星介质电子辐射影响数据

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摘要

Using data from the Medium Electrons A instrument on the Combined Release and Radiation Effects Satellite (CRRES), a survey of pitch angle distributions (PADs) of energetic electrons is performed. The distributions are classified into three categories: 90°-peaked, flattop, and butterfly. The categorizations are examined as a function of L-shell and orbit number and at electron energies of 153, 510, and 976 keV. The 90°-peaked distributions dominate at the lowest energy channel, and butterfly distributions are more prevalent at higher L values. The PADs on the dayside are predominately 90°-peaked distributions, while butterfly distributions become more common on the nightside at higher L-shells. Fitting the PADs to a sin n α form, where α is the local pitch angle, a profile of the parameter n versus L-shell is produced for local times corresponding to postnoon and midnight sectors for the 510-keV channel. We then compare the 510-keV data during times of moderate disturbance to the less disturbed case and the average case, and show an increase in butterfly distributions, which occurs at L > 6 for the nightside case and 3.5 1 before and after the great storm on 24 March 1991, we find that there are significant differences before and after this event, the latter orbits being during a time of higher observed geomagnetic activity. Considering only those PADs with a calculated n > 1, the variation of the 90°-peaked distributions versus L-shell and orbit shows increased steepness at lower L-shell. For the lowest energy channel, the low L-shell variation of the steepness of the distributions visually correlates with the average 2-day minimum plasmapause location calculated from a model based on the D st index over the same time period. For the 510-keV electrons, a correlation can be seen with the development of flattop distributions inside of the calculated minimum plasmapause location.
机译:使用数据从媒介的电子仪器合并后的释放和辐射效应卫星(crr)、螺旋角的调查高能电子的分布(垫)执行。三类:90°达到顶峰,航空母舰蝴蝶。l层和轨道数和函数电子能量的153、510和976 keV。90°的峰值分布控制在最低能源通道,蝴蝶分布在较高的L值更普遍。昼主要90°达到顶峰分布,而蝴蝶分布变得越来越普遍在阴面更高L-shells。其中α是当地的螺旋角,一个概要文件的参数n和l层产生当地乘以相应postnoon和午夜行业510 kev通道。比较温和的510 kev数据时期更少的干扰情况和干扰一般情况下,并展示蝴蝶的增加分布,发生在L > 6阴面案例和3.5 L 1, 90°的变化峰值分布与l层和轨道显示增加较低的l层陡度。通道,低l层的变化视觉陡度的分布与平均为期两天的最低等离子体层顶位置计算模型基于D st指数在同一时间时期。可以看到随着航空母舰的发展分布在计算最低等离子体层顶位置。

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