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Unifying repeating fast radio bursts
Science, 2022Mysterious high-energy radio bursts are found to share certain ...
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Nature Astronomy, 2021
The annual Fast Radio Bursts conference was again held entirely online this year, from 28 July to 5 August 2021. It included plenary talks, posters, lightning talks, late-breaking news and discussion sessions.
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The annual Fast Radio Bursts conference was again held entirely online this year, from 28 July to 5 August 2021. It included plenary talks, posters, lightning talks, late-breaking news and discussion sessions.
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Nature Astronomy, 2020
The annual Fast Radio Burst conference was held as an entirely virtual event on 6–9 July inclusive, with talks spread over three time zones and an online communication channel for discussions.
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The annual Fast Radio Burst conference was held as an entirely virtual event on 6–9 July inclusive, with talks spread over three time zones and an online communication channel for discussions.
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2004
Nonthermal radio bursts in the interplanetary medium indicate the far-reaching effect of solar eruptions that inject energetic particles, plasmas and shock waves into the inner heliosphere. More than half a century of ground-based observations and subsequent space-based observations exist on this phenomena.
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Nonthermal radio bursts in the interplanetary medium indicate the far-reaching effect of solar eruptions that inject energetic particles, plasmas and shock waves into the inner heliosphere. More than half a century of ground-based observations and subsequent space-based observations exist on this phenomena.
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Science, 2013
Observations of radio bursts that appear to originate from outside the Milky Way may suggest the existence of a large and exotic source population. [Also see Report by Thornton et al. ]
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Observations of radio bursts that appear to originate from outside the Milky Way may suggest the existence of a large and exotic source population. [Also see Report by Thornton et al. ]
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Publications of the Astronomical Society of Australia, 1974
Like the strong non-thermal radio bursts from the solar corona and from the earth’s magnetosphere, the Jupiter radio bursts are characterized by their duration which may be from milliseconds to seconds, and by their complex structure on the frequency-time plane.
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Like the strong non-thermal radio bursts from the solar corona and from the earth’s magnetosphere, the Jupiter radio bursts are characterized by their duration which may be from milliseconds to seconds, and by their complex structure on the frequency-time plane.
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