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A Highly Circularly Polarized Solar Radio Emission Component Observed at Hectometric Wavelengths

โœ Scribed by M. J. Reiner; M. L. Kaiser; J. Fainberg; J. -L. Bougeret


Book ID
106532360
Publisher
Springer
Year
2006
Tongue
English
Weight
730 KB
Volume
234
Category
Article
ISSN
0038-0938

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โœ Ch. V. Sastry; K. S. Dwarkanath; R. K. Shevgaonkar; V. Krishan ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 517 KB

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