Abstract
Short time periodicities of 3, 6, and 12 months have been found by analysis of the coefficient of atmospheric activity of Jupiter for the time period 1963–1967.
These periodicities have been attributed to seasonal variations of the Jovian atmosphere, and could be related to similar periodicities observed in solar flares and in the high velocity solar wind streamers.
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Xanthakis, J., Petropoulos, B., Banos, C. et al. Short time periodicities of the atmospheric activity of Jupiter. Earth Moon Planet 49, 211–219 (1990). https://doi.org/10.1007/BF00055175
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DOI: https://doi.org/10.1007/BF00055175