Observations on the time and frequency structure of solar decameter radio bursts
β Scribed by Ch. V. Sastry
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 526 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
Solar radio bursts were observed with a 4-channel radiometer and polarization analyser at wavelenghts around 12 m. The time and frequency resolutions were 10 ms and 100 kHz respectively. Observations on the duration, time profile and frequency splitting are described.
π SIMILAR VOLUMES
observed the brightness distribution of solar radio bursts at 26 MHz \* Laboratoire Associ6 du CNRS No. 264.
It is observed that while there exists a strong correlation between the decay constant and the exciter duration for isolated type III radio bursts, it is absent for those type III radio bursts which are preceded by type IIIb radio bursts. A possible theoretical explanation for the presence of correl
We have observed the slowly varying component of solar radio emission at a frequency of 34.5 MHz with half power beam widths of 26'/40' in the east-west and north-south directions, respectively. It is found that the observed brightness temperatures vary within the limits of 0.3x 106 K to 1.5 x 106 K