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- W2069988049 abstract "Spectrographic and imaging observations of meter wave fast drift bursts are presented which imply the quasi-simultaneous particle acceleration at two different sites in the corona: one below 0.5 R⊙, where electron beams rising in the corona are produced, and one above 1.0 R⊙ from which electron beams propagate downward as revealed by reverse drift bursts. This configuration produces three groups of bursts with a similar spatial brightness distribution during 2.5 hours, demonstrating the overall stability of the large-scale magnetic field structure. The source structure of the reverse drift bursts is consistent with particle acceleration in a coronal helmet streamer neutral sheet. The same kind of high coronal acceleration sites is necessary for explaining the energy spectrum observed in interplanetary electron events." @default.
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- W2069988049 date "1993-09-01" @default.
- W2069988049 modified "2023-09-23" @default.
- W2069988049 title "Observation of electron acceleration at widely separated altitudes in the solar corona" @default.
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- W2069988049 doi "https://doi.org/10.1016/0273-1177(93)90493-u" @default.
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