Abstract
Assuming various types of the excitation functions of the polar wobble, simulated polar orbits are calculated for the respective excitation functions. About these polar orbits, the rotational periods and the mean square radii for respective examples are compared with the values calculated basing on the theory developed in the author's previous paper (SEKIGUCHI, 1990). The results are likely to support the validity of the present theory. In the case of harmonic oscillator, a parallel reasoning is also possible, and the similar simulations are performed.
