Planetary gear train with dual sun and planet gear sets
This block represents a planetary gear train with dual sun and planet gear sets. The two sun gears are centrally located and separated longitudinally along a common rotation axis. The smaller of these gears engages an inner planet gear set, which in turn engages an outer planet gear set. The outer planet gear set, whose length spans the distance between the two sun gears, engages both the larger sun gear and the ring gear.
A carrier holds the planet gear sets in place at different radii. The carrier, which rigidly connects to a drive shaft, can spin as a unit with respect to the sun and ring gears. Revolute joints, each located between a planet gear and the carrier, enable the gears to spin about their individual longitudinal axes.
The relative angular velocities of the sun, planet, and ring gears follow from the kinematic constraints between them. For more information, see Ravigneaux Gear Model.
This block is a composite component with four underlying blocks:
The figure shows the connections between the blocks.
Ratio gRSL of the ring gear wheel radius to the large sun gear wheel radius. This gear ratio must be strictly greater than 1. The default is 2.
Ratio gRSS of the ring gear wheel radius to the small sun gear wheel radius. This gear ratio must be strictly greater than the ring-large sun gear ratio. The default is 3.
Select how to implement friction losses from nonideal meshing of gear teeth. The default is No meshing losses.
No meshing losses — Suitable for HIL simulation — Gear meshing is ideal.
Constant efficiency — Transfer of torque between gear wheel pairs is reduced by a constant efficiency η satisfying 0 < η ≤ 1. If you select this option, the panel changes from its default.
Vector of viscous friction coefficients [μLS μSS μLSP μSSP] for the large sun-carrier, small sun-carrier, large sun planet-carrier, and small sun planet-carrier gear motions, respectively. The default is [0 0 0 0].
From the drop-down list, choose units. The default is newton-meters/(radians/second) (N*m/(rad/s)).
Ravigneaux imposes four kinematic and four geometric constraints on the four connected axes and the two internal wheels (inner and outer planets):
rCiωC = rSSωSS + rPiωPi , rCi = rSS + rPi ,
rCoωC = rSLωSL + rPoωPo , rCo = rSL + rPo ,
(rCo – rCi)ωC = rPiωPi + rPoωPo , rCo – rCi= rPo + rPi ,
rRωR = rCoωC + rPoωPo , rR = rCo + rPo .
The ring-small sun ratio gRSS = rR/rSS = NR/NSS and ring-large sun gear ratio gRSL = rR/rSL = NR/NSL. N is the number of teeth on each gear. In terms of these ratios, the key kinematic constraints are:
(gRSS – 1)ωC = gRSSωR – ωSS ,
(gRSL + 1)ωC = gRSLωR + ωSL .
The six degrees of freedom reduce to two independent degrees of freedom. The gear pairs are (1,2) = (LS,P), (SS,P), (P,R), and (P,P).
Warning The gear ratio gRSS must be strictly greater than the gear ratio gRSL. The gear ratio gRSL must be strictly greater than one.
The torque transfers are:
gRSSτSS + τR – τloss(SS,R) = 0 , gRSLτSL + τR – τloss(SL,R) = 0 ,
with τloss = 0 in the ideal case.
In the nonideal case, τloss ≠ 0. See Model Gears with Losses.
Gear inertia is negligible. It does not impact gear dynamics.
Gears are rigid. They do not deform.
Coulomb friction slows down simulation. See Adjust Model Fidelity.
C — Rotational conserving port representing the planet gear carrier.
R — Rotational conserving port representing the ring gear.
SL — Rotational conserving port representing the large sun gear.
SS — Rotational conserving port representing the small sun gear.