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- W2809670667 abstract "Three types of low-frequency nonthermal radio bursts are associated with coronal mass ejections (CMEs): Type III bursts due to accelerated electrons propagating along open magnetic field lines, type II bursts due to electrons accelerated in shocks, and type IV bursts due to electrons trapped in post-eruption arcades behind CMEs. This paper presents a summary of results obtained during solar cycle 23 primarily using the white-light coronagraphic observations from the Solar Heliospheric Observatory (SOHO) and the WAVES experiment on board Wind." @default.
- W2809670667 created "2018-06-29" @default.
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- W2809670667 date "2011-01-01" @default.
- W2809670667 modified "2023-09-27" @default.
- W2809670667 title "Coronal Mass Ejections and Solar Radio Emissions (invited)" @default.
- W2809670667 doi "https://doi.org/10.1553/pre7s325" @default.
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