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Radio identification and continuum spectra of decameter-wavelength sources

✍ Scribed by O. V. Verkhodanov; N. V. Verkhodanova; H. Andernach

Book ID
110133622
Publisher
Springer
Year
2003
Tongue
English
Weight
353 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