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| Titel |
Why do the Solar Type III Burst emit the maximum of their radio energy around 1 MHz ? |
| VerfasserIn |
Milan Maksimovic, Vratislav Krupar, Eduard Kontar, Arnaud Zaslavsky, Louis Pascal, Hamish Reid, Alain Lecacheux, Xavier Bonnin, Ondrej Santolik, Nicole Vilmer |
| Konferenz |
EGU General Assembly 2014
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| Medientyp |
Artikel
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| Sprache |
Englisch
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 16 (2014) |
| Datensatznummer |
250095675
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| Publikation (Nr.) |
 EGU/EGU2014-14136.pdf |
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| Zusammenfassung |
| We present a statistical survey of a few hundred of Type III bursts observed from about 100 KHz up to about 400 MHz. When displayed as a function of the frequency, the radio flux exhibits a clear maximum at about 1 MHz. This property, already reported in previous studies, will be described in more details and possible explanations about its origin will be discussed. |
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