Random Vibration – A Brief History

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Random Vibration – A Brief HistoryThomas L. Paez, Thomas Paez Consulting, Durango ColoradoIn 1827, upon observing the motion of particles of pollen in afluid suspension, Robert Brown, a Scottish botanist, speculated thatparticle motions were due, not to some vitality in the particles, butto molecular-kinetic motion in the fluid. That is, he speculated thatunobservable particles in the fluid were impacting the particlesfrom the pollen to excite their motion. The motion became knownas Brownian motion.In 1905, Albert Einstein wrote the first paper on random vibration,1,2 “On the Movement of Small Particles Suspended in aStationary Liquid Demanded by the Molecular-Kinetic Theory ofHeat.” (Einstein wrote several other famous papers in 1905, amongthem, his paper on the special theory of relativity and his paperon the photoelectric effect. He won the Nobel Prize in Physics forthe latter work.) He developed equations governing the distribution of motions of a particle suspended in a fluid in a derivationunderstandable to most undergraduate students of thermodynamics. Along the way, he developed a way of understanding randomprocesses because the theory of random processes did not existat that date, at least, in the form it exists today. Einstein’s workspawned a flurry of activity in random vibration.This article summarizes the work of Einstein and some of thosewho followed in his footsteps. It summarizes the milestones inrandom vibration from 1905 to the present, including developmentof an alternate to Einstein’s technique for analysis of random vibration, definition of the spectral density of a stationary random process,development of the fundamental relation of random vibration in scalarand matrix forms, estimation of spectral density, specification of nonstationary random processes, random vibration of random structures, andmany others. Many examples are provided.Einstein’s Introduction of Random VibrationBy the start of the twentieth century the idea that gases and fluidsmight be composed of molecules that move freely and energetically was well established. In fact, Robert Brown had speculatedas early as 1827 that that the motion of inert particles in a fluidmedium is caused by the molecular-kinetic effect, the impingementof unobservable particles in a fluid medium upon a microscopic,observable, particle. If we were to observe the Brownian motionof a particle suspended in a fluid, we would see a sequence likethat shown in Figure 1.Through 1905 a mathematical theory for the so-called Brownian movement had not been developed. In 1905 Albert Einstein1,2developed a mathematical theory to describe Brownian movement.Einstein did not use a direct approach to solve the problem. (Adirect approach would write the equation governing motion of theparticle in Brownian motion, and then find the probabilistic response character from the character of the input.) Rather, he arguedthat if the molecular-kinetic theory of heat is applicable in describing the Brownian motion of particles, then pressures on Brownianparticles can be established. Those pressures would cause the diffusion of small particles in a suspension. (He assumed the particlesto be spherical.) He developed a diffusion equation governing theprobability density function (PDF) of a collection of Brownian52SOUND & VIBRATION/JANUARY 20120yHumans have observed and experienced dynamic randomphenomena for millennia through our contact with earthquakes,winds, ocean waves, rough roads and trails. Before people couldeasily conceptualize harmonic motions, they observed randomvibration. Today, random vibration is thought of as the randommotion of a structure excited by a random input. The mathematicaltheory of random vibration is essential to the realistic modelingof structural dynamic systems. This article summarizes the workof some key contributors to the theory of random vibration fromits inception in 1905, with the work of Einstein, to the present.Several graphical examples are included.–2–4–20x2Figure 1. The locations of a Brownianparticle on the x-y plane, observed ata fixed interval of time, and on a preestablished length scale. The particlestarts at the origin (red circle), andends at the tenth observation (greencircle).particles. During developmentof the diffusion equation, hemade assumptions that wouldlater characterize the molecular excitation as an ideal whitenoise, an excitation with signalcontent over a very broad bandof frequencies. (See the following section for descriptionof white noise.) The diffusionequation Einstein obtained is(for a single, one-dimensionalcomponent of motion): f 2 f D 2 t xf ( x, 0) d ( x ) (1)where f(x,t), – x , t 0is the PDF of particle displacement at displacement locationx and at time t and D is the coefficient of diffusion. The initial condition at t 0 specifies that the PDF starts as a Dirac delta function;that is, there is complete certainty that displacement motion startsat the origin. For Einstein’s formulation the coefficient of diffusionis D (RT/N)(1/6pcf r) where R is the universal gas constant, T isthe absolute temperature, N is Avagadro’s number, cf is the coefficient of viscosity of the fluid, and r is the radius of the sphere.The solution to Eq. 1 is:f x (t ) ( x ) Êx2 ˆexp Á (2p )(2Dt )Ë 2(2Dt ) 1- x , t 0 (2a)where the subscript on f indicates that we are interested in thedisplacement random variable, X(t), at time t. Note that the standarddeviation of the response is:s X (t ) 2Dtt 0(2b)The standard deviation of the displacement response grows,without bound, as the square root of time. The reason is thatthere is no force applied to the system (a spring) that causes thedisplacements to oscillate about the origin. If we were interestedin characterizing the response of a Brownian particle we woulduse Eq. 2 to answer questions regarding the unfolding of randomparticle response in time.However, structural dynamicists are interested in consideringstructural response. The simple mechanical system equivalent tothe one Einstein considered is the structure shown in Figure 2; itis a mass tied to ground with a damper (and no spring). Let m andc be the mass and damping constant of the structure with unitsof lb-sec2/in and lb-sec/in, and let Sww, be the two-sided spectraldensity of the white noise excitation with units of lb2/(rad/sec).Equivalence between the mechanical system and the Brownianparticle is established when D Swwm2/2c2. Figure 3 shows fivemarginal PDFs of the displacement response at normalized timest 2Dt 0.1,1,4,7,10 and the minus/plus one standard deviationcurves. The mechanical system parameters are arbitrary and theresponse depends only on the coefficient of diffusion D.Einstein did not consider explicitly the time-domain response ofthe system of interest; however, we can do so, easily. The equationgoverning motion of the system in Figure 2 is:mx cx w (t )x (0) x0 , x (0) n0 , t 0(3)where x(t), t 0 is the displacement response, dots denote differentiation with respect to time, the initial conditions specifythe response, and w(t), t 0 is a white noise realization from arandom source. (The response x(t) is not capitalized, here, bewww.SandV.com

xxkcmW(t)W(t)mcFigure 2. The structural dynamic system equivalent to the system analyzedby Einstein.Figure 3. Five separate marginal PDFs of the displacement response of thesystem in Figure 2 at normalized times t 2Dt 0.1,1,4,7,10. (Blue, Eq. 2a,plotted above the t – x plane) Standard deviation of the response. (Red, Eq.2b, plotted in the t – x plane).Figure 5. Single-degree-of-freedom (SDOF) structure with mass m stiffnessk and damping c excited by input force W(t).excites. (The excitation must approximate the ideal white noisewith band-limited white noise.) Figure 4a shows a realization ofband-limited white noise excitation with signal content in thefrequency band [–50,50] Hz and two-sided spectral density Sww 1 lb2 / (rad/sec). Figure 4b is the velocity response of a systemwith mass, m 1 lb-sec2/in, and damper, c 1 lb-sec/in. Figure4c is the displacement response of the same system. Note that theinput is simply one excitation from an infinite ensemble of possibilities; therefore, additional trials would yield other inputs andcorresponding responses.Because the problem Einstein solved yields the probabilisticdescription of the motion of a mass attached via a viscous damperto a fixed boundary and excited with white noise, his development can be thought of as the first solution to a random vibrationproblem and the dawning of the era of random vibration analysis.However, the fact is that structural dynamicists are more interested in structures that are supported on resilient elements; suchstructures usually display oscillatory responses. The simplest formof oscillatory structure is the single-degree-of-freedom (SDOF)structure shown in Figure 5. This is the fundamental model ofstructural dynamics, one whose response is treated in practicallyevery text on random vibration. (See, for example, the fundamentaltexts,4,5 the intermediate texts,3,6 or the more advanced texts.7,8)The first successful treatments of such a structure were by Smoluchowski9 and Furth10, independently in 1916 and 1917. Theydeveloped a form of the diffusion equation for the SDOF structurethat would, eventually, become known as the Fokker-Planck equation. Interestingly, the case they considered is the over-damped(non-oscillatory) system. They referred to the system we call theSDOF structure as the “harmonically bound particle.”The limitation of over-damping would eventually be overcome,but in the short term, Ornstein11 developed the idea of analyzingrandom vibrations, directly, based on the governing equation ofmotion. The equation governing motion of the SDOF structure is cX kX WmXFigure 4. (a) Sample excitation from a band-limited random source withtwo-sided spectral density, Sww 1 lb2/(rad/sec), with frequency content in[–50,50) Hz; (b) velocity response of structure of Figure 2, with m 1 lb-sec2/in, and c 1 lb-sec/in, to the input in Figure 4a. (c) displacement responseof the structure of Figure 2, with m 1 lb-sec2/in, and c 1 lb-sec/in, tothe input in Figure 4a.cause we consider the exciting force to be a sample of the inputrandom process, not the random process, itself.) We can generatea sample excitation3 from the white noise random process, andthen compute the velocity and displacement responses the inputwww.SandV.com(4)where m, c, X and W are defined as before, and k denotes the stiffness of the spring that attaches the SDOF mass to ground. (Theexcitation and response, W(t) and X(t) are capitalized, here becausethey are formally considered to be random processes.) The initialconditions on this equation must involve the joint probabilitydistribution of displacement and velocity. The method Ornsteindeveloped forms the basis for the method we use today to performrandom vibration analysis.Uhlenbeck and Ornstein12 wrote a paper that elaborated onOrnstein’s solution to Eq. 4. In that paper they described the excitation and response in terms of their moments (averages). Thisuse of moments was an extremely important innovation; to a greatdegree, it constructed a foundation for the framework most randomvibration analysts use today for the solution of random vibrationproblems. Specifically, to start, they described the input excitationas having zero mean and autocorrelation function (a term not inuse at the time) defined:E ÈÎW (t1 )W (t2 ) Rww (t1, t2 ) 2p Sww d (t1 - t2 )- t1, t2 (5)45TH ANNIVERSARY ISSUE53

random processes; i.e., random processes in a statistical steadystate whose realizations extend from the infinite past to the infinitefuture. No such random source actually exists; however, manyrandom phenomena realize steady-state signals over relatively longperiods of time. Those are the sources we seek to model. Weiner’sdefinition of spectral density is based on the idea of autocorrelationfunction. The autocorrelation function of a random process is theaverage value, over all time, of the product of the process at timet, times the process at time t t. For a stationary random process,this average is a function of t, only. The mathematical definition is:RXX (t ) E [X (t )X (t t )] limt Æ Figure 6. Six marginal PDFs of the displacement response of an SDOFstructure developed by Uhlenbeck and Ornstein.12where Sww is the constant spectral density of an ideal white noiserandom process, and d ( ) is the Dirac delta function. (The paperformally defining spectral density appeared in 1930, but Uhlenbeckand Ornstein were, apparently, not aware of it. Therefore, theydid not use it specifically in their definition of the coefficient onthe right hand side.) They proceeded to show that the responserandom process, X(t), – t , has zero mean and mean square:p SwwE È X 2(t ) s x2 (t ) Î 2zw 3 m2nÏÔ-2zw ntÌ1 - eÓÔÈ Ô2zzsin (2wdt ) sin2 (wdt ) Í1 221 -z1-zÍÎ Ô2t 0 (6)and they specified that the response has a Gaussian probability distribution. In this expression, w n k / m is the naturalfrequency of the SDOF structure, z 0.5c / mk is the systemdamping factor (zŒ [0,1]), and wd w n 1 - z 2 is its damped naturalfrequency. Their result demonstrates the practical result that thestandard deviation of displacement response approaches a finitelimit, s X ( ) (p Sww ) / 2zw n3 m2 , as t Æ . The limit is reachedwithin one percent when (0.18/z) cycles of response have beenexecuted. Though Uhlenbeck and Ornstein did not express theresponse autocorrelation function, and they did not refer to inputor response spectral density, their presentation must be consideredthe first to use “modern” techniques of random vibration analysis.An example that shows the result developed by Uhlenbeck andOrnstein is provided in Figure 6. Six separate marginal PDFs of thedisplacement response of an SDOF structure excited by ideal whitenoise are shown, plotted above the normalized time versus normalized displacement plane. In the graph, time, t wnt, is normalizedby the natural frequency of the SDOF structure. Displacement, x x/sX ( ), is normalized by the root-mean-square response at t Æ ,and the PDF is normalized as s X ( ) fX (t /w n ) (s X ( )x ), where fx(t)( )is the PDF of displacement response.Many more contributions have been made to the theory ofrandom vibration, and some of them will be summarized later, inthe section titled “Random Vibration in Engineering StructuralDynamics.”()Weiner and the Definition of Spectral DensityIt is quite unlikely that the mathematical theory of random vibration would have realized the widespread use it enjoys, today, ifNorbert Weiner had not developed the idea of spectral density.13(He named it spectral intensity. Today, it is also called mean squarespectral density, power spectral density, and by other descriptivenames.) His paper is a 242-page, mathematically dense, presentation that formally defines spectral density and pursues manyother topics including a definition of cross-spectral density, andother spectral quantities. He attributed his inspiration to papers bySchuster.14-16 Schuster had made several efforts to define a formof spectral density, but had never defined it using a limit as didWeiner, and as we do today.Strictly speaking, the spectral density exists only for stationary54SOUND & VIBRATION/JANUARY 20121 TÚ -T x (t )x (t t )dt2T- t (7)where x,(t), – t is a random process realization, i.e., a signalthat comes from a stationary random source. The definition makesthe assumption that a realization of a stationary random processrepresentative of all other realizations is used; the assumptionamounts to an assumption that the random source is ergodic.The autocorrelation function, while indispensible in manyframeworks, is a blunt tool for the interpretation of the character ofa random process. For example, Figures 7a and 7b show a segmentof a finite duration realization of a structural acceleration responserandom process and its estimated autocorrelation function. Thetime history of Figure 7a does not clearly reveal the character ofthe random source, and neither does the estimated autocorrelationfunction of Figure 7b. Weiner defined the spectral density as theFourier transform of the autocorrelation function.SXX (w ) 1 - iwtdtÚ - RXX (t )e2p- w (8a)where w is circular frequency in units of rad/sec, and i -1 is theimaginary unit. (This formula defines the two-sided spectral density, usedin random vibration analysis. The one-sided spectral density is used topresent experimental results, and most frequently, to plot spectral densities; it is written as a function of cyclic frequency, with units of cycles/sec Hertz.) Weiner then proceeded to develop many of its features. Amongother things, the spectral density is non-negative. The autocorrelationfunction is recoverable from the spectral density because the operationof Fourier transformation is invertible.iwtRXX (t ) Ú dw- SXX (w )e- t (8b)Because of this and because the autocorrelation function isdefined (see Eq. 7), RXX (t) E[X(t)X(t t)], it follows that:RXX (0) E È X 2(t ) Ú (8c)- SXX (w )dwÎ That is, the area under the spectral density curve equals the meansquare of the random process. Beyond this preliminary conclusion,Eq. 8c also shows that the mean square is built up from componentsin different frequency ranges, and this fact can be used to drawimportant conclusions about a random motion. (See, for example,the following paragraph.)Figure 7c shows the estimated spectral density of the randomprocess that is the source of the time history shown in Figure 7a.The area under the spectral density curve is the mean square of the2 1.23g 2 , and the value of the autocorrelationrandom process, s Xfunction at t 0. The graph of the spectral density is a sequence ofpeaks. Because the signal upon which the spectral density estimateis based is the acceleration response of a structure, the peaks indicate mean square response signal content at the modal frequenciesof the structure. The spectral density is easily interpretable; thecontribution to total mean square response by each mode can bedirectly approximated.An important historical note that relates to spectral density involves, so-called, ideal white noise. Ideal white noise is a randomprocess that possesses a spectral density that is constant over allfrequencies (equal energy per unit frequency), from minus infinityto infinity. (The terminology comes from a reference to the spectrumof light.) Of course, such a random process has spectral densitywith infinite area, and therefore, infinite mean square signal content; it cannot exist, in nature. It does excite measures of responsein some structures with finite signal content, therefore, it is oftenused in simple modeling applications.3www.SandV.com

Figure 7. (a) Realization of a stationary random process; (b) estimatedautocorrelation function of the source of the random signal in Figure 7a;(c) estimated spectral density function of the source of the random signalin Figure 7a.Weiner developed many other measures of stationary randomprocess behavior and many more features of those measures andstationary random processes, themselves. Some will be mentioned,briefly, in the following section. Is should be noted that in 1934Khintchine17 published a paper in which he independently defined spectral density. For that reason, Eqs. 8a and 8b are calledthe Weiner-Khintchine relations.Random Vibration in Engineering Structural DynamicsThe modern field of random vibrations of mechanical systemsand probabilistic structural dynamics, in general, has gained importance as the awareness that real mechanical environments arestochastic has broadened. Today random vibration analyses areperformed frequently and in practical settings, usually within theframework of a commercial finite element code. Commercial finitee

vibration. Today, random vibration is thought of as the random motion of a structure excited by a random input. The mathematical theory of random vibration is essential to the realistic modeling of structural dynamic systems. This article summarizes the work of some key contributors to the theory of random vibration from

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