OSU0907_Fig8a
OSU0907_Fig8a

Figure 8:
(a) Steady state RMS of dynamic planet rotation versus mesh frequency Ω when tooth separation is considered. The parameters are as in Figure 3 with ε=0.3. Circles (o) indicate increasing speed Ω and crosses (x) indicate decreasing Ω. (b) Sun-planet tooth separation (ksp=0) occurs for Ω=4.5kHz≈2ω5.