The 11
year sunspot cycle roughly corresponds with Jupiter's orbital period.
Not exact matches
The sun's magnetic activity waxes and wanes
roughly every 11
years, generating more dark
sunspots at the peak of the
cycle and fewer at the trough.
The number of
sunspots varies as solar magnetic activity does — the change in this number, from a minimum of none to a maximum of
roughly 250
sunspots or clusters of
sunspots and then back to a minimum, is known as the solar
cycle, and averages about 11
years long.
Because of the variations of
sunspots and faculae on the sun's surface, the total solar irradiance (TSI), also called the solar constant, varies on a
roughly 11 -
year cycle by about 0.07 %, which has been measured by orbiting satellites since 1978 [Lean, 1987, 1991; Wilson et al., 1981].
Typically, a
cycle takes
roughly 5.5
years to move from a solar minimum, when there are few
sunspots, to the solar maximum, during which
sunspot activity is amplified.