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Observations of Solar Type II bursts at frequencies 10–30 MHz

✍ Scribed by V.N. Mel'nik; A.A. Konovalenko; H.O. Rucker; A.A. Stanislavsky; E.P. Abranin; A. Lecacheux; G. Mann; A. Warmuth; V.V. Zaitsev; M.Y. Boudjada; V.V. Dorovskii; V.V. Zaharenko; V.N. Lisachenko; C. Rosolen


Book ID
111611989
Publisher
Springer
Year
2004
Tongue
English
Weight
903 KB
Volume
222
Category
Article
ISSN
0038-0938

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Type III solar radio burst storms observ
✍ Joseph Fainberg; R. G. Stone 📂 Article 📅 1970 🏛 Springer 🌐 English ⚖ 671 KB

Storms of type III solar radio bursts observed from 5.4 ot 0.2 MHz consist of a quasi-continuous production of type III events observable for half a solar rotation but persisting in some cases for well over a complete rotation (Fainberg and Stone, 1970). The observed burst drift rates are a function