Rotational Double Inverted Pendulum
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Inverted Pendulum System Introduction This Lab Experiment Consists of Two Experimental Procedures, Each with Sub Parts
Inverted Pendulum System Introduction This lab experiment consists of two experimental procedures, each with sub parts. Experiment 1 is used to determine the system parameters needed to implement a controller. Part A finds the hardware gains in each direction of motion. Part B requires calculation of system parameters such as the inertia, and experimental verification of the calculations. Experiment 2 then implements a controller. Part A tests the system without the controller activated. Part B then activates the controller and compares the stability to Part A. Part C then has a series of increasing step responses to determine the controller’s ability to track the desired output. Finally Part D has an increasing frequency input into the system to determine the system’s frequency response. Hardware Figure 1 shows the Inverted Pendulum Experiment. It consists of a pendulum rod which supports the sliding balance rod. The balance rod is driven by a belt and pulley which in turn is driven by a drive shaft connected to a DC servo motor below the pendulum rod. There are two series of weights included that affect the physical plant: brass counter weights connected underneath the pivot plate with adjustable height and weight and brass “donut” weights attached to both ends of the balance rod. Figure 1: Model 505 ECP Inverted Pendulum Apparatus 1 Safety - Be careful on the step where students are asked to physically turning the equipment upside-down. Make sure the device is not on the edge of the table after it is inverted. - Make sure the pendulum, when released, will not hit anyone or anything. -
Hamiltonian Chaos
Hamiltonian Chaos Niraj Srivastava, Charles Kaufman, and Gerhard M¨uller Department of Physics, University of Rhode Island, Kingston, RI 02881-0817. Cartesian coordinates, generalized coordinates, canonical coordinates, and, if you can solve the problem, action-angle coordinates. That is not a sentence, but it is classical mechanics in a nutshell. You did mechanics in Cartesian coordinates in introductory physics, probably learned generalized coordinates in your junior year, went on to graduate school to hear about canonical coordinates, and were shown how to solve a Hamiltonian problem by finding the action-angle coordinates. Perhaps you saw the action-angle coordinates exhibited for the harmonic oscillator, and were left with the impression that you (or somebody) could find them for any problem. Well, you now do not have to feel badly if you cannot find them. They probably do not exist! Laplace said, standing on Newton’s shoulders, “Tell me the force and where we are, and I will predict the future!” That claim translates into an important theorem about differential equations—the uniqueness of solutions for given ini- tial conditions. It turned out to be an elusive claim, but it was not until more than 150 years after Laplace that this elusiveness was fully appreciated. In fact, we are still in the process of learning to concede that the proven existence of a solution does not guarantee that we can actually determine that solution. In other words, deterministic time evolution does not guarantee pre- dictability. Deterministic unpredictability or deterministic randomness is the essence of chaos. Mechanical systems whose equations of motion show symp- toms of this disease are termed nonintegrable. -
Problem Set 26: Feedback Example: the Inverted Pendulum
26 Feedback Example: The Inverted Pendulum Recommended Problems P26.1 Consider an inverted pendulum mounted on a movable cart as depicted in Figure P26.1. We have modeled the pendulum as consisting of a massless rod of length L, with a mass m attached at the end. The variable 0(t) denotes the pendulum's angular deflection from the vertical, g is gravitational acceleration, s(t) is the position of the cart with respect to some reference point, a(t) is the acceleration of the cart, and x(t) represents the angular acceleration resulting from any disturbances, such as gusts of wind. NIM L L I x(t) 0(t) N9 a(t) s(t) Figure P26.1 Our goal in this problem is to analyze the dynamics of the inverted pendulum and more specifically to investigate the problem of balancing the pendulum by judi cious choice of the cart acceleration a(t). The differential equation relating 0(t), a(t), and x(t) is d20(t) L dt = g sin [(t)] - a(t) cos [(t)] + Lx(t) (P26.1-1) This relation merely equates the actual acceleration of the mass along a direction perpendicular to the rod and the applied accelerations (gravity, the disturbance acceleration due to x(t), and the cart acceleration) along this direction. Note that eq. (P26.1-1) is a nonlinear differential equation relating 0(t), a(t), and x(t). The detailed, exact analysis of the behavior of the pendulum therefore requires that we examine this nonlinear equation; however, we can obtain a great deal of insight into the dynamics of the inverted pendulum by performing a linear analysis. -
Annotated List of References Tobias Keip, I7801986 Presentation Method: Poster
Personal Inquiry – Annotated list of references Tobias Keip, i7801986 Presentation Method: Poster Poster Section 1: What is Chaos? In this section I am introducing the topic. I am describing different types of chaos and how individual perception affects our sense for chaos or chaotic systems. I am also going to define the terminology. I support my ideas with a lot of examples, like chaos in our daily life, then I am going to do a transition to simple mathematical chaotic systems. Larry Bradley. (2010). Chaos and Fractals. Available: www.stsci.edu/~lbradley/seminar/. Last accessed 13 May 2010. This website delivered me with a very good introduction into the topic as there are a lot of books and interesting web-pages in the “References”-Sektion. Gleick, James. Chaos: Making a New Science. Penguin Books, 1987. The book gave me a very general introduction into the topic. Harald Lesch. (2003-2007). alpha-Centauri . Available: www.br-online.de/br- alpha/alpha-centauri/alpha-centauri-harald-lesch-videothek-ID1207836664586.xml. Last accessed 13. May 2010. A web-page with German video-documentations delivered a lot of vivid examples about chaos for my poster. Poster Section 2: Laplace's Demon and the Butterfly Effect In this part I describe the idea of the so called Laplace's Demon and the theory of cause-and-effect chains. I work with a lot of examples, especially the famous weather forecast example. Also too I introduce the mathematical concept of a dynamic system. Jeremy S. Heyl (August 11, 2008). The Double Pendulum Fractal. British Columbia, Canada. -
Lecture Notes on Classical Mechanics for Physics 106Ab Sunil Golwala
Lecture Notes on Classical Mechanics for Physics 106ab Sunil Golwala Revision Date: September 25, 2006 Introduction These notes were written during the Fall, 2004, and Winter, 2005, terms. They are indeed lecture notes – I literally lecture from these notes. They combine material from Hand and Finch (mostly), Thornton, and Goldstein, but cover the material in a different order than any one of these texts and deviate from them widely in some places and less so in others. The reader will no doubt ask the question I asked myself many times while writing these notes: why bother? There are a large number of mechanics textbooks available all covering this very standard material, complete with worked examples and end-of-chapter problems. I can only defend myself by saying that all teachers understand their material in a slightly different way and it is very difficult to teach from someone else’s point of view – it’s like walking in shoes that are two sizes wrong. It is inevitable that every teacher will want to present some of the material in a way that differs from the available texts. These notes simply put my particular presentation down on the page for your reference. These notes are not a substitute for a proper textbook; I have not provided nearly as many examples or illustrations, and have provided no exercises. They are a supplement. I suggest you skim them in parallel while reading one of the recommended texts for the course, focusing your attention on places where these notes deviate from the texts. ii Contents 1 Elementary Mechanics 1 1.1 Newtonian Mechanics .................................. -
Instructional Experiments on Nonlinear Dynamics & Chaos (And
Bibliography of instructional experiments on nonlinear dynamics and chaos Page 1 of 20 Colorado Virtual Campus of Physics Mechanics & Nonlinear Dynamics Cluster Nonlinear Dynamics & Chaos Lab Instructional Experiments on Nonlinear Dynamics & Chaos (and some related theory papers) overviews of nonlinear & chaotic dynamics prototypical nonlinear equations and their simulation analysis of data from chaotic systems control of chaos fractals solitons chaos in Hamiltonian/nondissipative systems & Lagrangian chaos in fluid flow quantum chaos nonlinear oscillators, vibrations & strings chaotic electronic circuits coupled systems, mode interaction & synchronization bouncing ball, dripping faucet, kicked rotor & other discrete interval dynamics nonlinear dynamics of the pendulum inverted pendulum swinging Atwood's machine pumping a swing parametric instability instabilities, bifurcations & catastrophes chemical and biological oscillators & reaction/diffusions systems other pattern forming systems & self-organized criticality miscellaneous nonlinear & chaotic systems -overviews of nonlinear & chaotic dynamics To top? Briggs, K. (1987), "Simple experiments in chaotic dynamics," Am. J. Phys. 55 (12), 1083-9. Hilborn, R. C. (2004), "Sea gulls, butterflies, and grasshoppers: a brief history of the butterfly effect in nonlinear dynamics," Am. J. Phys. 72 (4), 425-7. Hilborn, R. C. and N. B. Tufillaro (1997), "Resource Letter: ND-1: nonlinear dynamics," Am. J. Phys. 65 (9), 822-34. Laws, P. W. (2004), "A unit on oscillations, determinism and chaos for introductory physics students," Am. J. Phys. 72 (4), 446-52. Sungar, N., J. P. Sharpe, M. J. Moelter, N. Fleishon, K. Morrison, J. McDill, and R. Schoonover (2001), "A laboratory-based nonlinear dynamics course for science and engineering students," Am. J. Phys. 69 (5), 591-7. http://carbon.cudenver.edu/~rtagg/CVCP/Ctr_dynamics/Lab_nonlinear_dyn/Bibex_nonline.. -
The Stability of an Inverted Pendulum
The Stability of an Inverted Pendulum Mentor: John Gemmer Sean Ashley Avery Hope D’Amelio Jiaying Liu Cameron Warren Abstract: The inverted pendulum is a simple system in which both stable and unstable state are easily observed. The upward inverted state is unstable, though it has long been known that a simple rigid pendulum can be stabilized in its inverted state by oscillating its base at an angle. We made the model to simulate the stabilization of the simple inverted pendulum. Also, the numerical analysis was used to find the stability angle. Introduction The model of the simple pendulum problem is one the most well studied dynamical systems. Imagine a weight attached to the end of weightless rod that is freely swinging back and forth about some pivot without friction. The governing equation for this idealized mathematical model is given as d 2θ 2 + glsinθ = 0, where g is gravitational acceleration, � is the length of the pendulum, and � is the dt angular displacement about downward vertical. If the pendulum starts at any given angle, we can expect € € to see one of the following happen: the pendulum will oscillate about the downward angle,θ = 0; it will continue to rotate around the pivot; or it will stay still, atθ = 0,π , but atθ = π any slight disturbance will € cause the pendulum to swing downward. € € Separatrix Rotations Oscillations The phase portrait above shows that the stability points for the simple pendulum are atθ = πn, for n = 0,±1,±2,.... For even n‘s,θ is a stable point and if given some angular velocity,ω , the pendulum € will always oscillate around it, but for odd n’s,θ is an unstable point, so even the smallest angular € € € € velocity will knock the pendulum off it and it will swing down toward its stable point. -
Chaos Theory and Robert Wilson: a Critical Analysis Of
CHAOS THEORY AND ROBERT WILSON: A CRITICAL ANALYSIS OF WILSON’S VISUAL ARTS AND THEATRICAL PERFORMANCES A dissertation presented to the faculty of the College of Fine Arts Of Ohio University In partial fulfillment Of the requirements for the degree Doctor of Philosophy Shahida Manzoor June 2003 © 2003 Shahida Manzoor All Rights Reserved This dissertation entitled CHAOS THEORY AND ROBERT WILSON: A CRITICAL ANALYSIS OF WILSON’S VISUAL ARTS AND THEATRICAL PERFORMANCES By Shahida Manzoor has been approved for for the School of Interdisciplinary Arts and the College of Fine Arts by Charles S. Buchanan Assistant Professor, School of Interdisciplinary Arts Raymond Tymas-Jones Dean, College of Fine Arts Manzoor, Shahida, Ph.D. June 2003. School of Interdisciplinary Arts Chaos Theory and Robert Wilson: A Critical Analysis of Wilson’s Visual Arts and Theatrical Performances (239) Director of Dissertation: Charles S. Buchanan This dissertation explores the formal elements of Robert Wilson’s art, with a focus on two in particular: time and space, through the methodology of Chaos Theory. Although this theory is widely practiced by physicists and mathematicians, it can be utilized with other disciplines, in this case visual arts and theater. By unfolding the complex layering of space and time in Wilson’s art, it is possible to see the hidden reality behind these artifacts. The study reveals that by applying this scientific method to the visual arts and theater, one can best understand the nonlinear and fragmented forms of Wilson's art. Moreover, the study demonstrates that time and space are Wilson's primary structuring tools and are bound together in a self-renewing process. -
Model-Based Proprioceptive State Estimation for Spring-Mass Running
Model-Based Proprioceptive State Estimation for Spring-Mass Running Ozlem¨ Gur¨ and Uluc¸Saranlı Abstract—Autonomous applications of legged platforms will [18] limit their utility for use with fully autonomous mobile inevitably require accurate state estimation both for feedback platforms. Visual state estimation methods by themselves often control as well as mapping and planning. Even though kinematic do not offer sufficient measurement bandwith and accuracy models and low-bandwidth visual localization may be sufficient for fully-actuated, statically stable legged robots, they are in- and when they do, they entail high computational loads that are adequate for dynamically dexterous, underactuated platforms not feasible for autonomous operation [17]. As a consequence, where second order dynamics are dominant, noise levels are a combination of both proprioceptive and exteroceptive sensors high and sensory limitations are more severe. In this paper, we are often used within filter based sensor fusion frameworks to introduce a model based state estimation method for dynamic combine the advantages of both approaches. running behaviors with a simple spring-mass runner. By using an approximate analytic solution to the dynamics of the model within In this paper, we show how the use of an accurate analytic an Extended Kalman filter framework, the estimation accuracy of motion model and additional cues from intermittent kinematic our model remains accurate even at low sampling frequencies. events can be utilized to achieve accurate state estimation for We also propose two new event-based sensory modalities that dynamic running even with a very limited sensory suite. To further improve estimation performance in cases where even this end, we work with the well-established Spring-Loaded the internal kinematics of a robot cannot be fully observed, such as when flexible materials are used for limb designs. -
Moon-Earth-Sun: the Oldest Three-Body Problem
Moon-Earth-Sun: The oldest three-body problem Martin C. Gutzwiller IBM Research Center, Yorktown Heights, New York 10598 The daily motion of the Moon through the sky has many unusual features that a careful observer can discover without the help of instruments. The three different frequencies for the three degrees of freedom have been known very accurately for 3000 years, and the geometric explanation of the Greek astronomers was basically correct. Whereas Kepler’s laws are sufficient for describing the motion of the planets around the Sun, even the most obvious facts about the lunar motion cannot be understood without the gravitational attraction of both the Earth and the Sun. Newton discussed this problem at great length, and with mixed success; it was the only testing ground for his Universal Gravitation. This background for today’s many-body theory is discussed in some detail because all the guiding principles for our understanding can be traced to the earliest developments of astronomy. They are the oldest results of scientific inquiry, and they were the first ones to be confirmed by the great physicist-mathematicians of the 18th century. By a variety of methods, Laplace was able to claim complete agreement of celestial mechanics with the astronomical observations. Lagrange initiated a new trend wherein the mathematical problems of mechanics could all be solved by the same uniform process; canonical transformations eventually won the field. They were used for the first time on a large scale by Delaunay to find the ultimate solution of the lunar problem by perturbing the solution of the two-body Earth-Moon problem. -
Chapter 8 Nonlinear Systems
Chapter 8 Nonlinear systems 8.1 Linearization, critical points, and equilibria Note: 1 lecture, §6.1–§6.2 in [EP], §9.2–§9.3 in [BD] Except for a few brief detours in chapter 1, we considered mostly linear equations. Linear equations suffice in many applications, but in reality most phenomena require nonlinear equations. Nonlinear equations, however, are notoriously more difficult to understand than linear ones, and many strange new phenomena appear when we allow our equations to be nonlinear. Not to worry, we did not waste all this time studying linear equations. Nonlinear equations can often be approximated by linear ones if we only need a solution “locally,” for example, only for a short period of time, or only for certain parameters. Understanding linear equations can also give us qualitative understanding about a more general nonlinear problem. The idea is similar to what you did in calculus in trying to approximate a function by a line with the right slope. In § 2.4 we looked at the pendulum of length L. The goal was to solve for the angle θ(t) as a function of the time t. The equation for the setup is the nonlinear equation L g θ�� + sinθ=0. θ L Instead of solving this equation, we solved the rather easier linear equation g θ�� + θ=0. L While the solution to the linear equation is not exactly what we were looking for, it is rather close to the original, as long as the angleθ is small and the time period involved is short. You might ask: Why don’t we just solve the nonlinear problem? Well, it might be very difficult, impractical, or impossible to solve analytically, depending on the equation in question. -
The Strengths and Weaknesses of Inverted Pendulum
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by University of Salford Institutional Repository THE STRENGTHS AND WEAKNESSES OF INVERTED PENDULUM MODELS OF HUMAN WALKING Michael McGrath1, David Howard2, Richard Baker1 1School of Health Sciences, University of Salford, M6 6PU, UK; 2School of Computing, Science and Engineering, University of Salford, M5 4WT, UK. Email: [email protected] Keywords: Inverted pendulum, gait, walking, modelling Word count: 3024 Abstract – An investigation into the kinematic and kinetic predictions of two “inverted pendulum” (IP) models of gait was undertaken. The first model consisted of a single leg, with anthropometrically correct mass and moment of inertia, and a point mass at the hip representing the rest of the body. A second model incorporating the physiological extension of a head‐arms‐trunk (HAT) segment, held upright by an actuated hip moment, was developed for comparison. Simulations were performed, using both models, and quantitatively compared with empirical gait data. There was little difference between the two models’ predictions of kinematics and ground reaction force (GRF). The models agreed well with empirical data through mid‐stance (20‐40% of the gait cycle) suggesting that IP models adequately simulate this phase (mean error less than one standard deviation). IP models are not cyclic, however, and cannot adequately simulate double support and step‐ to‐step transition. This is because the forces under both legs augment each other during double support to increase the vertical GRF. The incorporation of an actuated hip joint was the most novel change and added a new dimension to the classic IP model.