This paper studies sensitivity of compound planetary gear natural frequencies and vibration modes to system parameters. Based on a lumped parameter model of general compound planetary gears and their distinctive modal properties [1], the eigensensitivities to inertias and stiffnesses are calculated and expressed in compact formulae. Analysis reveals that eigenvalue sensitivities to stiffness parameters are directly proportional to modal strain energies, and eigenvalue sensitivities to inertia parameters are proportional to modal kinetic energies. Furthermore, the eigenvalue sensitivities to model parameters are determined by inspection of the modal strain and kinetic energy distributions. This provides an effective way to identify those parameters with the greatest impact on tuning certain natural frequencies. The present results, combined with the modal properties of general compound planetary gears, show that rotational modes are independent of translational bearing/shaft stiffnesses and masses of carriers/central gears, translational modes are independent of torsional bearing/shaft stiffnesses and moment of inertias of carriers/central gears, and planet modes are independent of all system parameters of other planet sets, the shaft/bearing stiffness parameters of carriers/rings, and the mass/moment of inertia parameters of carriers/central gears.

1.
Kiracofe, D. R., and Parker R. G., 2006, “Structured Vibration Modes of General Compound Planetary Gear Systems,” in press, ASME J. Vibr. Acoust.
2.
Peter Lynwander, “Gear Drive Systems: Design and Applications”, 1983
3.
Kahraman
A.
,
2001
, “
Free Torsional Vibration Characteristics of Compound Planetary Gear Sets
,”
Mechanism and Machine Theory
, Vol
36
, pp.
953
971
.
4.
Botman, M., 1976, “Epicyclic gear vibations,” ASME J. Engineering Indu., pp. 811–815.
5.
Kahraman
A.
,
1994
, “
Natural modes of planetary gear trains
,”
ASME J. Sound Vib.
,
173
, pp.
125
130
.
6.
Saada
A.
, and
Velex
P.
,
1995
, “
An extended model for the analysis of the dynamic behavior of planetary trains
,”
ASME J. Mech. Desd
117
, pp.
241
247
.
7.
Lin
J.
, and
Parker
R. G.
,
1999
, “
Analytical characterization of the unique properties of planetary gear free vibration
,”
ASME J. Vibr. and Acoust.
,
121
, pp.
316
321
.
8.
Lin
J.
and
Parker
R. G.
,
1999
, “
Sensitivity of Planetary Gear Natural Frequencies and Vibration Modes to Model Parameters
,”
Journal of Sound and Vibration
, vol.
228
, pp.
109
128
.
9.
Fox
R. L.
, and
Kapoor
M. P.
,
1968
, “
Rates of change of eigenvalues and eigenvetors
,”
AIAA Journal
6
, pp.
2426
2429
.
10.
Courant, R. and Hilbert, D., 1953, “Methods of Mathematical Physics,” New York: Interscience Publishers.
11.
Nelson
R. B.
,
1976
, “
Simplified calculation of eigenvector derivatives
,”
AIAA Journal
14
, pp.
1201
1205
.
12.
Mills-Crran
W. C.
,
1988
, “
Calcuation of eigenvector derivatives for structures with repeated eigenvalues
,”
AIAA Journal
26
, pp.
867
871
.
13.
Friswell
M. I.
,
1996
, “
The derivatives of repeated eigenvalues and their associated eigenvectors
,”
ASME J. Vibr. Acoust.
,
118
, pp.
390
397
.
14.
Lin
J.
, and
Parker
R. G.
,
2000
, “
Structured Vibration Characteristics of Planetary Gears with Unequally Spaced Planets
,”
ASME J. Sound Vib.
,
233
(
5)
, pp.
921
928
.
15.
Lin
J.
and
Parker
R. G.
,
2001
, “
Natural Frequency Veering in Planetary Gears
,”
Mechanics of Structures and Machines
,
29
(
4)
, pp.
411
429
.
16.
Kahraman, A., and Blankenship, G. W., 1994, “Planet Mesh Phasing in Epicyclic Gear Sets,” Proceedings of International Gearing Conference Newcastle, pp. 99–104.
17.
Seager
D. L.
,
1975
, “
Conditions for the Neutralization of Excitation by the Teeth in Epicyclic Gearing
,”
ASME J. of Mechanical Engineering Science.
17
(
5)
, pp
293
298
.
18.
Cunliffe, F., Smith, J. D., and Welbourn, D. B., 1974, “Dynamic Tooth Loads in Epicyclic Gears,” ASME J. of Engineering Indust, pp. 578–584.
19.
Pierre
C.
,
1988
, “
Mode localization and eigenvalue loci veering phenomena in disordered structures
,”
ASME J. Sound Vib.
,
126
, pp.
485
502
.
This content is only available via PDF.
You do not currently have access to this content.