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Observational studies of the angular structure of the radio galaxy 3C 234 at decameter wavelengths

✍ Scribed by A. V. Megn; S. Ya. Braude; S. L. Rashkovskiy; N. K. Sharykin; V. A. Shepelev; G. A. Inyutin; R. V. Vashchishin; A. I. Brazhenko; V. G. Bulatsen

Book ID
110137263
Publisher
Springer
Year
2003
Tongue
English
Weight
250 KB
Volume
47
Category
Article
ISSN
1063-7729

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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