Abstract
Prompted by recent moves to ask the International Astronomical Union to redefine the System III rotation period, we have used all available dekametric observations from 1951 to 1975 and new analysis methods in an attempt to improve our estimate of the Jovian dekametric rotation period.
Publisher
Cambridge University Press (CUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
2 articles.
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