Investigations on Type III/V Bursts of Solar Radio Emission. Part II: Relation to the Flare Event

✍ Scribed by H. Daene; A. KrÜGER

• Publisher: John Wiley and Sons
• Year: 2007
• Tongue: English
• Weight: 712 KB
• Volume: 289
• Category: Article
• ISSN: 0004-6337
• DOI: 10.1002/asna.19662890303

✦ Synopsis

With 5, figurcs. (lieccived 1965 July 22)

Decameter type 111 and type III/V bursts observed during more than five years are investigated statistically concerning their association with microwavc bursts and chroinospheric flares. The effects of starting times, morphology, and spectrum of associated microwave bursts are discussed a 5 well as the importances and positions of the correlated flares. Distributions of starting frequencies of some classes of type I11 bursts have been taken into account.

The primary origin of type I11 bursts has been supposed to be within or a little above those levels of the solar atmosphere, where the bursts of the lower decimeter range originate. The occurrence of type V bursts is not characteristic for the frequency of disappearance of type 111 bursts as a consideration of the "ending" frequencies of type 111 bursts shows.