Abstract:We present an experimental study of the motion of a circular disk spun onto a table. With the help of a high speed video system, the temporal evolutions of (i) the inclination angle α, (ii) the angular velocity ω and (iii) the precession rate Ω are studied. The influence of the mass of the disk and the friction between the disk and the supporting surface are considered. The inclination angle α and the angular velocity are observed to decrease according to a power law. We also show that the precession rate Ω di… Show more
“…The experimental results agree with values of n between 1 2 and 2 3 . Measurements on a torus are believed in [5] to confirm the supposition of van den Engh et al [23] that air drag is only of minor importance.…”
Section: Introductionsupporting
confidence: 66%
“…Caps et al [5] present a rather detailed experimental study of various rolling disks using a high-speed video camera (125-500 fps) and a laser beam during about 10 s. The inclination angle, precession rate and angular velocity around the axis of symmetry of the disk are each measured with a different experimental setup during a different run and, therefore, have not been obtained simultaneously. The experimental results agree with values of n between 1 2 and 2 3 .…”
Section: Introductionmentioning
confidence: 99%
“…There exists a tremendous amount of literature on the dynamics of the rolling disk, e.g. [1][2][3][4][5][6][7][8][11][12][13][17][18][19][20][21][22][23][24] but this list is far from complete. Here, we will only give an overview of the literature on dissipation mechanisms which explain the finite-time singularity and of the literature reporting measurements of this phenomenon.…”
This paper is concerned with the dominant dissipation mechanism for a rolling disk in the final stage of its motion. The aim of this paper is to present the various dissipation mechanisms for a rolling disk which are used in the literature in a unified framework. Furthermore, new experiments on the 'Euler disk' using a high-speed video camera and a novel image analysis technique are presented. The combined experimental/theoretical approach of this paper sheds some more light on the dominant dissipation mechanism on the time-scale of several seconds.Keywords Euler disk · Spinning · Finite-time singularity · Rolling friction · Non-smooth dynamics with the exponent n = 1 3 . The viscous air drag model of Moffatt was extended by Bildsten [3] to account for boundary layer effects which are expected to occur for larger values of the inclination angle. The derivations of Bildsten reveal an exponent of n = 4 9 . Observations of spinning coins in vacuum led van den Engh et al.[23] to suppose that air viscosity is not the dominant dissipation mechanism during the final stage of motion. Moffatt [19] replies that air viscosity is rather insensitive to the pressure and, therefore, that these observations R. I. Leine (B)
“…The experimental results agree with values of n between 1 2 and 2 3 . Measurements on a torus are believed in [5] to confirm the supposition of van den Engh et al [23] that air drag is only of minor importance.…”
Section: Introductionsupporting
confidence: 66%
“…Caps et al [5] present a rather detailed experimental study of various rolling disks using a high-speed video camera (125-500 fps) and a laser beam during about 10 s. The inclination angle, precession rate and angular velocity around the axis of symmetry of the disk are each measured with a different experimental setup during a different run and, therefore, have not been obtained simultaneously. The experimental results agree with values of n between 1 2 and 2 3 .…”
Section: Introductionmentioning
confidence: 99%
“…There exists a tremendous amount of literature on the dynamics of the rolling disk, e.g. [1][2][3][4][5][6][7][8][11][12][13][17][18][19][20][21][22][23][24] but this list is far from complete. Here, we will only give an overview of the literature on dissipation mechanisms which explain the finite-time singularity and of the literature reporting measurements of this phenomenon.…”
This paper is concerned with the dominant dissipation mechanism for a rolling disk in the final stage of its motion. The aim of this paper is to present the various dissipation mechanisms for a rolling disk which are used in the literature in a unified framework. Furthermore, new experiments on the 'Euler disk' using a high-speed video camera and a novel image analysis technique are presented. The combined experimental/theoretical approach of this paper sheds some more light on the dominant dissipation mechanism on the time-scale of several seconds.Keywords Euler disk · Spinning · Finite-time singularity · Rolling friction · Non-smooth dynamics with the exponent n = 1 3 . The viscous air drag model of Moffatt was extended by Bildsten [3] to account for boundary layer effects which are expected to occur for larger values of the inclination angle. The derivations of Bildsten reveal an exponent of n = 4 9 . Observations of spinning coins in vacuum led van den Engh et al.[23] to suppose that air viscosity is not the dominant dissipation mechanism during the final stage of motion. Moffatt [19] replies that air viscosity is rather insensitive to the pressure and, therefore, that these observations R. I. Leine (B)
“…Since then, results on the dynamics of a rigid body have been reported in a tremendous body of literature [2][3][4][5]. Owing to Moffatt's recent work [6], this classical problem has recently revived interest for studying the energy dissipation in the motion of a 'Euler's disc', namely a circular (homogeneous) metal disc spinning on a flat surface [7][8][9][10][11][12][13][14]. In this system, while its mechanical energy is dissipating, paradoxically, the speed of the disc's rolling increases rapidly.…”
Section: Introductionmentioning
confidence: 99%
“…Easwar et al [9] reported an exponent n = 3 through experiments using a single high-speed camera to measure the precession rate. Caps [8] performed a series of experiments to separately measure the inclination angle, precession rate and angular velocity around the symmetric axis of the disc, and presented the exponent with a value varying between n = 3 and 4. Leine [10] adopted a high-speed camera to synchronically measure the inclination angle and the precession rate, and suggested that the exponent is either n = 4 or 3.…”
This paper presents the results of both experimental and theoretical investigations for the dynamics of a steel disc spinning on a horizontal rough surface. With a pair of high-speed cameras, a stereoscopic vision method is adopted to perform omnidirectional measurements for the temporal evolution of the disc's motion. The experiment data allow us to detail the dynamics of the disc, and consequently to quantify its energy. From our experimental observations, it is confirmed that rolling friction is a primary factor responsible for the dissipation of the energy. Furthermore, a mathematical model, in which the rolling friction is characterized by a resistance torque proportional to the square of precession rate, is also proposed. By employing the model, we perform qualitative analysis and numerical simulations. Both of them provide results that precisely agree with our experimental findings.
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