Abstract
ABSTRACTPassive radio measurements of Saturn’s Rings are reviewed and new interferometric measurements at λ = 2.7 mm are presented. The brightness temperatures of the A plus B rings at a ring angle of B ⋍ 10° were found to be 17 K and 38 K in two separate experiments, the latter being the more reliable. These results are interpreted in terms of ring particle emission and scattering of the planet’s disk emission by the rings.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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