Saturn's rotation period was initially determined to be 10h 39m 24s ± 7s, based on long-wavelength radio emission. But subsequent observations revealed that this period varies by ± 6 min on a timescale of several months to years. It is shown that the periodicity of the radio waves varies systematically by ±1 percent with a characteristic timescale of 20–30 days, and it is demonstrated that these fluctuations are correlated with solar wind speed at Saturn.
- Philippe Zarka
- Laurent Lamy
- Helmut O. Rucker