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Anik-E1 and E2 satellite failures of January 1994 revisited

机译:回顾1994年1月的Anik-E1和E2卫星故障

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The consecutive failures of the geosynchronous Anik-El communication satellite on January 20, 1994, and Anik-E2 about nine hours later on January 21 (both incidents occurred on January 20 local time) received considerable publicity because the malfunctions of the satellites disrupted television and computer data transmissions across Canada, as well as telephone services to remote northern communities for hours. This often-cited event is revisited here with materials not covered before. Using publicly available information, Anik-E failure details, media coverage, recovery effort and cost incurred are first presented. This is then followed by scrutiny of space weather conditions pertinent to the occurrences of the Anik-E upsets. We trace the space weather episode's inception on the Sun, propagation through interplanetary medium, and manifestation in magnetic field variations as well as in energetic electron flux increases, and its eventual impact on the Anik-Es. The genesis of the energetic electron enhancements that have been blamed for the satellite malfunctions is thus traceable via high-speed solar wind stream with Alfven wave fluctuations to a longitudinally wide coronal hole on the Sun. Furthermore, strong magnetic pulsations preceding electron flux peaks indicate Pc5 ULF (Ultra Low Frequency) waves as a probable acceleration mechanism for the energetic electron flux enhancement that resulted in the internal charging of the Anik-Es. The magnetic fluctuations may even be possible triggers for the subsequent discharge that caused the satellites to malfunction. This incident illustrates that satellite operators should be on alert for elevated high-energy electron environment that is above established thresholds, as specifications in satellite design may not render a satellite immune from internal charging.
机译:1994年1月20日地球同步Anik-El通信卫星和Anik-E2连续故障约1小时(9月20日在当地时间1月21日)发生了9个小时,这引起了广泛的关注,因为卫星的故障扰乱了电视和电视。整个加拿大的计算机数据传输,以及到偏远北部社区的电话服务都需要数小时。在此重新讨论了这个经常被引用的事件,之前没有涉及到这些材料。首先使用公开的信息显示Anik-E故障详细信息,媒体报道,恢复工作和产生的成本。然后,检查与Anik-E异常有关的太空天气情况。我们追踪太空天气事件在太阳上的开始,通过行星际介质的传播以及磁场变化以及高能电子通量增加的表现,以及最终对Anik-Es的影响。因此,可以归因于卫星故障的高能电子增强的起源可以通过带有阿尔夫文波起伏的高速太阳风流追踪到太阳上纵向宽的日冕孔中来进行。此外,在电子通量峰值之前的强磁脉冲表明,Pc5 ULF(超低频)波是能量电子通量增强的可能加速机制,导致Anik-Es内部充电。电磁波动甚至可能是导致卫星故障的后续放电​​的触发因素。该事件表明,卫星运营商应警惕高能电子环境高于已建立的阈值,因为卫星设计中的规范可能无法使卫星免受内部充电的影响。

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