期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 504, 期 4, 页码 4706-4715出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab1156
关键词
scattering; turbulence; radio continuum: transients
资金
- ERC [247295]
- Netherlands Organisation for Scientific Research [184.033.109]
- European Research Council (ERC) [247295] Funding Source: European Research Council (ERC)
The study reports the discovery of bright, fast, radio flashes near Earth caused by plasma in the ionosphere, occurring either in isolation or large clusters in the densest parts of the ionosphere. Distinguishing these events from genuine astrophysical transients is crucial for future surveys searching for low frequency radio transients.
We report the discovery of bright, fast, radio flashes lasting tens of seconds with the AARTFAAC high-cadence all-sky survey at 60MHz. The vast majority of these coincide with known, bright radio sources that brighten by factors of up to 100 during such an event. We attribute them to magnification events induced by plasma near the Earth, most likely in the densest parts of the ionosphere. They can occur both in relative isolation, during otherwise quiescent ionospheric conditions, and in large clusters during more turbulent ionospheric conditions. Using a toy model, we show that the likely origin of the more extreme (up to a factor of 100 or so) magnification events likely originate in the region of peak electron density in the ionosphere, at an altitude of 300-400 km. Distinguishing these events from genuine astrophysical transients is imperative for future surveys searching for low frequency radio transient at time-scales below a minute.
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