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- W1534854082 abstract "Radio bursts in the solar atmosphere and interplanetary space come from energetic non-maxwellian electron populations. Since the radio emission is a non collisional process, it traces electrons also in dilute plasmas, where hard X-rays and gamma-rays are undetectable. Radio waves are therefore a probe of energetic electrons from the low corona to the interplanetary medium. This review outlines how radio signatures can be used to infer sites in flares and to visualize the magnetic structures which guide particles from the low corona to interplanetary space. Electron at coronal shock waves is then discussed. These are seen to accelerate less electrons than the impulsive processes operating in the low corona. The ability to determine onset times of SEP events to within a few minutes has recently revived the comparison with radio bursts as tracers of processes in the corona. Remarkable discrepancies in the timing of the escaping and interacting particles were ascribed to different processes of these particle populations (i.e. CME shock of the escaping particles), transport processes (delayed particle transport in interplanetary space) or a combination of time-extended in the magnetically stressed corona and transport to space along several diverging magnetic flux tubes. The different interpretations are confronted and discussed. It is concluded that particle at the Sun is not adequately described by a bimodal picture of flare acceleration of very short duration in very small volumes on the one hand and CME shock over large volumes on the other hand." @default.
- W1534854082 created "2016-06-24" @default.
- W1534854082 date "2006-01-01" @default.
- W1534854082 modified "2023-09-23" @default.
- W1534854082 title "Radio Bursts and Solar Energetic Particle Events" @default.
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- W1534854082 doi "https://doi.org/10.1029/165gm22" @default.
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