Decameter radio emission from Jupiter and solar activity
β Scribed by Ch.V. Sastry
- Publisher
- Elsevier Science
- Year
- 1968
- Tongue
- English
- Weight
- 458 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0032-0633
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π SIMILAR VOLUMES
## Abstract Decameter wavelength radio emission is finely structured in solar bursts. For their research it is very important to use a sufficient sensitivity of antenna systems. In this paper we study an influence of the radiotelescopeβantenna effective area on the results of decameter solar radio
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