A Nanosecond-duration Radio Pulse Originating from the Defunct Relay 2 Satellite

C. W. James, A. T. Deller, T. Dial, M. Glowacki, S. J. Tingay, K. W. Bannister, A. Bera, N. D. R. Bhat, R. D. Ekers, V. Gupta, A. Jaini, J. Morgan, J. N. Jahns-Schindler, R. M. Shannon, M. Sukhov, J. Tuthill and Z. Wang
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Abstract

We report the detection of a burst of emission over a 695.5–1031.5 MHz bandwidth by the Australian Square Kilometre Array Pathfinder. The burst was localized through analysis of near-field time delays to the long-decommissioned Relay 2 satellite and exhibited a dispersion measure of 2.26 × 10−5 pc cm−3—69.7 total electron content units, consistent with expectations for a single pass through the ionosphere. After coherent dedispersion, the burst was determined to be less than 30 ns in width, with an average flux density of at least 300 kJy. We consider an electrostatic discharge (ESD) or plasma discharge following a micrometeoroid impact to be plausible explanations for the burst. ESDs have previously been observed with the Arecibo radio telescope, but on 1000 times longer timescales. Our observation opens new possibilities for the remote sensing of ESD, which poses a serious threat to spacecraft, and reveals a new source of false events for observations of astrophysical transients.
从失效中继2号卫星发出的纳秒级无线电脉冲
我们报告澳大利亚平方公里阵列探路者探测到695.5-1031.5 MHz带宽上的发射爆发。通过对长期退役的中继2号卫星的近场时间延迟分析,确定了该爆发的位置,并显示出2.26 × 10−5 pc cm−3-69.7总电子含量单位的色散测量,与单次通过电离层的预期一致。经相干去色散后,确定爆发宽度小于30 ns,平均通量密度至少为300 ky。我们认为静电放电(ESD)或等离子体放电后的微流星体的影响是合理的解释爆发。以前用阿雷西博射电望远镜也曾观测到静电场,但时间尺度要长1000倍。我们的观测为ESD遥感提供了新的可能性,它对航天器构成了严重威胁,并揭示了天体物理瞬变观测的新假事件来源。
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