The observed correlations between X-ray and type III radio emissions from solar bursts are described by means of a bivariate distribution function. Procedures for determining the form of this distribution are described using a sample of data analyzed by Kane (1981). With the help of this distributio
Relationship between type III-V radio and hard X-ray bursts
β Scribed by R. T. Stewart
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 502 KB
- Volume
- 58
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
With 13 figurcs. (Keccived 1965 July 15) Thc phenomenological features of type V radiation arc discussed a t the basis of fine structure rccords taken a t the Astrophysical Observatory Potsdam since 1958. A phenomenological subclassification is derived from the various forms of appearance. It is bel
Observations of impulsive solar flare X-rays > 10 keV made with the OGO-5 satellite are compared with ground based measurements of type III solar radio bursts in 10-580 MHz range. It is shown that the times of maxima of these two emissions, when detectable, agree within ~ 18 s. This maximum time dif