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Observations of the beaming of Jupiter's radio emission at 620 and 2650 Mc/sec

โœ Scribed by J.A. Roberts; R.D. Ekers


Book ID
107760096
Publisher
Elsevier Science
Year
1968
Tongue
English
Weight
380 KB
Volume
8
Category
Article
ISSN
0019-1035

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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