Table 1:
Synodic and siderial rotation periods and
corresponding siderial frequencies. Sunspot rotation
periods are calculated from
determined by Balthasar et al. (1986).
The value for the solar interior is the one just below the
tachocline taken from Eff-Darwich et al. (2002).
determined by Balthasar et al. (1986).
The value for the solar interior is the one just below the
tachocline taken from Eff-Darwich et al. (2002).