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Foundations of Newtonian Dynamics: an Axiomatic Approach For
Foundations of Newtonian Dynamics: 1 An Axiomatic Approach for the Thinking Student C. J. Papachristou 2 Department of Physical Sciences, Hellenic Naval Academy, Piraeus 18539, Greece Abstract. Despite its apparent simplicity, Newtonian mechanics contains conceptual subtleties that may cause some confusion to the deep-thinking student. These subtle- ties concern fundamental issues such as, e.g., the number of independent laws needed to formulate the theory, or, the distinction between genuine physical laws and deriva- tive theorems. This article attempts to clarify these issues for the benefit of the stu- dent by revisiting the foundations of Newtonian dynamics and by proposing a rigor- ous axiomatic approach to the subject. This theoretical scheme is built upon two fun- damental postulates, namely, conservation of momentum and superposition property for interactions. Newton’s laws, as well as all familiar theorems of mechanics, are shown to follow from these basic principles. 1. Introduction Teaching introductory mechanics can be a major challenge, especially in a class of students that are not willing to take anything for granted! The problem is that, even some of the most prestigious textbooks on the subject may leave the student with some degree of confusion, which manifests itself in questions like the following: • Is the law of inertia (Newton’s first law) a law of motion (of free bodies) or is it a statement of existence (of inertial reference frames)? • Are the first two of Newton’s laws independent of each other? It appears that -
Industrial Noise Control and Acoustics
Industrial Noise Control and Acoustics Randall F. Barron Louisiana Tech University Ruston, Louisiana, U.S.A. Marcel Dekker, Inc. New York • Basel Copyright © 2001 by Marcel Dekker, Inc. All Rights Reserved. Copyright © 2003 Marcel Dekker, Inc. LibraryofCongressCataloging-in-PublicationData AcatalogrecordforthisbookisavailablefromtheLibraryofCongress. ISBN:0-8247-0701-X Thisbookisprintedonacid-freepaper. Headquarters MarcelDekker,Inc. 270MadisonAvenue,NewYork,NY10016 tel:212-696-9000;fax:212-685-4540 EasternHemisphereDistribution MarcelDekkerAG Hutgasse4,Postfach812,CH-4001Basel,Switzerland tel:41-61-260-6300;fax:41-61-260-6333 WorldWideWeb http://www.dekker.com The publisher offers discounts on this book when ordered in bulk quantities, For more information, write to Special Sales/Professional Marketing at the headquarters address above. Copyright # 2003 by Marcel Dekker, Inc. All Rights Reserved. Neither this book nor any part may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying, microfilming, and recording, or by any information storage retrieval system, without permission in writing from the publisher. Current printing (last digit): 10987654321 PRINTED IN THE UNITED STATES OF AMERICA Copyright © 2003 Marcel Dekker, Inc. Preface Since the Walsh-Healy Act of 1969 was amended to include restrictions on the noise exposure of workers, there has been much interest and motivation in industry to reduce noise emitted by machinery. In addition to concerns about air and water pollution by contaminants, efforts have also been direc- ted toward control of environmental noise pollution. In response to these stimuli, faculty at many engineering schools have developed and introduced courses in noise control, usually at the senior design level. It is generally much more effective to design ‘‘quietness’’ into a product than to try to ‘‘fix’’ the noise problem in the field after the product has been put on the market. -
Definition and Measurement of Sound Energy Level of a Transient Sound Source
J. Acoust. Soc. Jpn. (E) 8, 6 (1987) Definition and measurement of sound energy level of a transient sound source Hideki Tachibana,* Hiroo Yano,* and Koichi Yoshihisa** *Institute of Industrial Science , University of Tokyo, 7-22-1, Roppongi, Minato-ku, Tokyo, 106 Japan **Faculty of Science and Technology, Meijo University, 1-501, Shiogamaguti, Tenpaku-ku, Nagoya, 468 Japan (Received 1 May 1987) Concerning stationary sound sources, sound power level which describes the sound power radiated by a sound source is clearly defined. For its measuring methods, the sound pressure methods using free field, hemi-free field and diffuse field have been established, and they have been standardized in the international and national stan- dards. Further, the method of sound power measurement using the sound intensity technique has become popular. On the other hand, concerning transient sound sources such as impulsive and intermittent sound sources, the way of describing and measuring their acoustic outputs has not been established. In this paper, therefore, "sound energy level" which represents the total sound energy radiated by a single event of a transient sound source is first defined as contrasted with the sound power level. Subsequently, its measuring methods by two kinds of sound pressure method and sound intensity method are investigated theoretically and experimentally on referring to the methods of sound power level measurement. PACS number : 43. 50. Cb, 43. 50. Pn, 43. 50. Yw sources, the way of describing and measuring their 1. INTRODUCTION acoustic outputs has not been established. In noise control problems, it is essential to obtain In this paper, "sound energy level" which repre- the information regarding the noise sources. -
Overview of the CALET Mission to the ISS 1 Introduction
32ND INTERNATIONAL COSMIC RAY CONFERENCE,BEIJING 2011 Overview of the CALET Mission to the ISS SHOJI TORII1,2 FOR THE CALET COLLABORATION 1Research Institute for Scinece and Engineering, Waseda University 2Space Environment Utilization Center, JAXA [email protected] DOI: 10.7529/ICRC2011/V06/0615 Abstract: The CALorimetric Electron Telescope (CALET) mission is being developed as a standard payload for the Exposure Facility of the Japanese Experiment Module (JEM/EF) on the International Space Station (ISS). The instrument consists of a segmented plastic scintillator charge measuring module, an imaging calorimeter consisting of 8 scintillating fiber planes with a total of 3 radiation lengths of tungsten plates interleaved with the fiber planes, and a total absorption calorimeter consisting of crossed PWO logs with a total depth of 27 radiation lengths. The major scientific objectives for CALET are to search for nearby cosmic ray sources and dark matter by carrying out a precise measurement of the electron spectrum (1 GeV - 20 TeV) and observing gamma rays (10 GeV - 10 TeV). CALET has a unique capability to observe electrons and gamma rays in the TeV region since the hadron rejection power is larger than 105 and the energy resolution better than 2 % above 100 GeV. CALET has also the capability to measure cosmic ray H, He and heavy nuclei up to 1000 TeV.∼ The instrument will also monitor solar activity and search for gamma ray transients. The phase B study has started, aimed at a launch in 2013 by H-II Transfer Vehicle (HTV) for a 5 year observation period on JEM/EF. -
Chapter 11.Pdf
Chapter 11. Kinematics of Particles Contents Introduction Rectilinear Motion: Position, Velocity & Acceleration Determining the Motion of a Particle Sample Problem 11.2 Sample Problem 11.3 Uniform Rectilinear-Motion Uniformly Accelerated Rectilinear-Motion Motion of Several Particles: Relative Motion Sample Problem 11.5 Motion of Several Particles: Dependent Motion Sample Problem 11.7 Graphical Solutions Curvilinear Motion: Position, Velocity & Acceleration Derivatives of Vector Functions Rectangular Components of Velocity and Acceleration Sample Problem 11.10 Motion Relative to a Frame in Translation Sample Problem 11.14 Tangential and Normal Components Sample Problem 11.16 Radial and Transverse Components Sample Problem 11.18 Introduction Kinematic relationships are used to help us determine the trajectory of a snowboarder completing a jump, the orbital speed of a satellite, and accelerations during acrobatic flying. Dynamics includes: Kinematics: study of the geometry of motion. Relates displacement, velocity, acceleration, and time without reference to the cause of motion. Fdownforce Fdrive Fdrag Kinetics: study of the relations existing between the forces acting on a body, the mass of the body, and the motion of the body. Kinetics is used to predict the motion caused by given forces or to determine the forces required to produce a given motion. Particle kinetics includes : • Rectilinear motion: position, velocity, and acceleration of a particle as it moves along a straight line. • Curvilinear motion : position, velocity, and acceleration of a particle as it moves along a curved line in two or three dimensions. Rectilinear Motion: Position, Velocity & Acceleration • Rectilinear motion: particle moving along a straight line • Position coordinate: defined by positive or negative distance from a fixed origin on the line. -
Particle Motions Caused by Seismic Interface Waves
Prodeedings of the 37th Scandinavian Symposium on Physical Acoustics 2 - 5 February 2014 Particle motions caused by seismic interface waves Jens M. Hovem, [email protected] 37th Scandinavian Symposium on Physical Acoustics Geilo 2nd - 5th February 2014 Abstract Particle motion sensitivity has shown to be important for fish responding to low frequency anthropogenic such as sounds generated by piling and explosions. The purpose of this article is to discuss the particle motions of seismic interface waves generated by low frequency sources close to solid rigid bottoms. In such cases, interface waves, of the type known as ground roll, or Rayleigh, Stoneley and Scholte waves, may be excited. The interface waves are transversal waves with slow propagation speed and characterized with large particle movements, particularity in the vertical direction. The waves decay exponentially with distance from the bottom and the sea bottom absorption causes the waves to decay relative fast with range and frequency. The interface waves may be important to include in the discussion when studying impact of low frequency anthropogenic noise at generated by relative low frequencies, for instance by piling and explosion and other subsea construction works. 1 Introduction Particle motion sensitivity has shown to be important for fish responding to low frequency anthropogenic such as sounds generated by piling and explosions (Tasker et al. 2010). It is therefore surprising that studies of the impact of sounds generated by anthropogenic activities upon fish and invertebrates have usually focused on propagated sound pressure, rather than particle motion, see Popper, and Hastings (2009) for a summary and overview. Normally the sound pressure and particle velocity are simply related by a constant; the specific acoustic impedance Z=c, i.e. -
Chapter 3 Motion in Two and Three Dimensions
Chapter 3 Motion in Two and Three Dimensions 3.1 The Important Stuff 3.1.1 Position In three dimensions, the location of a particle is specified by its location vector, r: r = xi + yj + zk (3.1) If during a time interval ∆t the position vector of the particle changes from r1 to r2, the displacement ∆r for that time interval is ∆r = r1 − r2 (3.2) = (x2 − x1)i +(y2 − y1)j +(z2 − z1)k (3.3) 3.1.2 Velocity If a particle moves through a displacement ∆r in a time interval ∆t then its average velocity for that interval is ∆r ∆x ∆y ∆z v = = i + j + k (3.4) ∆t ∆t ∆t ∆t As before, a more interesting quantity is the instantaneous velocity v, which is the limit of the average velocity when we shrink the time interval ∆t to zero. It is the time derivative of the position vector r: dr v = (3.5) dt d = (xi + yj + zk) (3.6) dt dx dy dz = i + j + k (3.7) dt dt dt can be written: v = vxi + vyj + vzk (3.8) 51 52 CHAPTER 3. MOTION IN TWO AND THREE DIMENSIONS where dx dy dz v = v = v = (3.9) x dt y dt z dt The instantaneous velocity v of a particle is always tangent to the path of the particle. 3.1.3 Acceleration If a particle’s velocity changes by ∆v in a time period ∆t, the average acceleration a for that period is ∆v ∆v ∆v ∆v a = = x i + y j + z k (3.10) ∆t ∆t ∆t ∆t but a much more interesting quantity is the result of shrinking the period ∆t to zero, which gives us the instantaneous acceleration, a. -
Sound Power Measurement What Is Sound, Sound Pressure and Sound Pressure Level?
www.dewesoft.com - Copyright © 2000 - 2021 Dewesoft d.o.o., all rights reserved. Sound power measurement What is Sound, Sound Pressure and Sound Pressure Level? Sound is actually a pressure wave - a vibration that propagates as a mechanical wave of pressure and displacement. Sound propagates through compressible media such as air, water, and solids as longitudinal waves and also as transverse waves in solids. The sound waves are generated by a sound source (vibrating diaphragm or a stereo speaker). The sound source creates vibrations in the surrounding medium. As the source continues to vibrate the medium, the vibrations propagate away from the source at the speed of sound and are forming the sound wave. At a fixed distance from the sound source, the pressure, velocity, and displacement of the medium vary in time. Compression Refraction Direction of travel Wavelength, λ Movement of air molecules Sound pressure Sound pressure or acoustic pressure is the local pressure deviation from the ambient (average, or equilibrium) atmospheric pressure, caused by a sound wave. In air the sound pressure can be measured using a microphone, and in water with a hydrophone. The SI unit for sound pressure p is the pascal (symbol: Pa). 1 Sound pressure level Sound pressure level (SPL) or sound level is a logarithmic measure of the effective sound pressure of a sound relative to a reference value. It is measured in decibels (dB) above a standard reference level. The standard reference sound pressure in the air or other gases is 20 µPa, which is usually considered the threshold of human hearing (at 1 kHz). -
A Uniformly Moving and Rotating Polarizable Particle in Thermal Radiation Field: Frictional Force and Torque, Radiation and Heating
A uniformly moving and rotating polarizable particle in thermal radiation field: frictional force and torque, radiation and heating G. V. Dedkov1 and A.A. Kyasov Nanoscale Physics Group, Kabardino-Balkarian State University, Nalchik, 360000, Russia Abstract. We study the fluctuation-electromagnetic interaction and dynamics of a small spinning polarizable particle moving with a relativistic velocity in a vacuum background of arbitrary temperature. Using the standard formalism of the fluctuation electromagnetic theory, a complete set of equations describing the decelerating tangential force, the components of the torque and the intensity of nonthermal and thermal radiation is obtained along with equations describing the dynamics of translational and rotational motion, and the kinetics of heating. An interplay between various parameters is discussed. Numerical estimations for conducting particles were carried out using MATHCAD code. In the case of zero temperature of a particle and background radiation, the intensity of radiation is independent of the linear velocity, the angular velocity orientation and the linear velocity value are independent of time. In the case of a finite background radiation temperature, the angular velocity vector tends to be oriented perpendicularly to the linear velocity vector. The particle temperature relaxes to a quasistationary value depending on the background radiation temperature, the linear and angular velocities, whereas the intensity of radiation depends on the background radiation temperature, the angular and linear velocities. The time of thermal relaxation is much less than the time of angular deceleration, while the latter time is much less than the time of linear deceleration. Key words: fluctuation-electromagnetic interaction, thermal radiation, rotating particle, frictional torque and tangential friction force 1. -
Acoustic Particle Velocity Investigations in Aeroacoustics Synchronizing PIV and Microphone Measurements
INTER-NOISE 2016 Acoustic particle velocity investigations in aeroacoustics synchronizing PIV and microphone measurements Lars SIEGEL1; Klaus EHRENFRIED1; Arne HENNING1; Gerrit LAUENROTH1; Claus WAGNER1, 2 1 German Aerospace Center (DLR), Institute of Aerodynamics and Flow Technology (AS), Göttingen, Germany 2 Technical University Ilmenau, Institute of Thermodynamics and Fluid Mechanics, Ilmenau, Germany ABSTRACT The aim of the present study is the detection and visualization of the sound propagation process from a strong tonal sound source in flows. To achieve this, velocity measurements were conducted using particle image velocimetry (PIV) in a wind tunnel experiment under anechoic conditions. Simultaneously, the acoustic pressure fluctuations were recorded by microphones in the acoustic far field. The PIV fields of view were shifted stepwise from the source region to the vicinity of the microphones. In order to be able to trace the acoustic propagation, the cross-correlation function between the velocity and the pressure fluctuations yields a proxy variable for the acoustic particle velocity acting as a filter for the velocity fluctuations. The temporal evolution of this quantity indicates the propagation of the acoustic perturbations. The acoustic radiation of a square rod in a wind tunnel flow is investigated as a test case. It can be shown that acoustic waves propagate from emanating coherent flow structures in the near field through the shear layer of the open jet to the far field. To validate this approach, a comparison with a 2D simulation and a 2D analytical solution of a dipole is performed. 1. INTRODUCTION The localization of noise sources in turbulent flows and the traceability of the acoustic perturbations emanating from the source regions into the far field are still challenging. -
Particle Acceleration at Interplanetary Shocks
PARTICLE ACCELERATION AT INTERPLANETARY SHOCKS G.P. ZANK, Gang LI, and Olga VERKHOGLYADOVA Institute of Geophysics and Planetary Physics (IGPP), University of California, Riverside, CA 92521, U.S.A. ([email protected], [email protected], [email protected]) Received ; accepted Abstract. Proton acceleration at interplanetary shocks is reviewed briefly. Understanding this is of importance to describe the acceleration of heavy ions at interplanetary shocks since wave excitation, and hence particle scattering, at oblique shocks is controlled by the protons and not the heavy ions. Heavy ions behave as test particles and their acceler- ation characteristics are controlled by the properties of proton excited turbulence. As a result, the resonance condition for heavy ions introduces distinctly di®erent signatures in abundance, spectra, and intensity pro¯les, depending on ion mass and charge. Self- consistent models of heavy ion acceleration and the resulting fractionation are discussed. This includes discussion of the injection problem and the acceleration characteristics of quasi-parallel and quasi-perpendicular shocks. Keywords: Solar energetic particles, coronal mass ejections, particle acceleration 1. Introduction Understanding the problem of particle acceleration at interplanetary shocks is assuming increasing importance, especially in the context of understanding the space environment. The basic physics is thought to have been established in the late 1970s and 1980s with the seminal papers of Axford et al. (1977); Bell, (1978a,b), but detailed interplanetary observations are not easily in- terpreted in terms of the simple original models of particle acceleration at shock waves. Three fundamental aspects make the interplanetary problem more complicated than the typical astrophysical problem: the time depen- dence of the acceleration and the solar wind background; the geometry of the shock; and the long mean free path for particle transport away from the shock. -
Derivation of the Sabine Equation: Conservation of Energy
UIUC Physics 406 Acoustical Physics of Music Derivation of the Sabine Equation: Conservation of Energy Consider a large room of volume V = HWL (m3) with perfectly reflecting walls, filled with a uniform, steady-state (i.e. equilibrium) acoustic energy density wrtfa ,, at given frequency f (Hz) within the volume V of the room. Uniform energy density means that a given time t: 3 waa r,, t f w t , f constant (SI units: Joules/m ). The large room also has a small opening of area A (m2) in it, as shown in the figure below: H V A I rt,, f ac nAˆˆ, An W L In the steady-state, the rate of acoustical energy Wa input e.g. by a point sound source within the large room equals the rate at which acoustical energy is “leaking” out of the room through the hole of area A, i.e. the acoustical power input by the sound source in the room into the room = the acoustical power leaving the room through the hole of area A. In this idealized model of a room with perfectly reflecting walls, the hole of area A thus represents absorption of sound in a real room with finite reflectivity walls, i.e. walls that have some absorption associated with them. Suppose at time t = 0 the sound source in the room {located far from the hole} is turned off. Since the sound energy density is uniform in the room, the sound energy contained in the room Wtf,,,, wrtfdrwtf 33 drwtfV , will thus decrease with time, since aaVV a a acoustical energy is (slowly) leaking out of the room through the opening of area A.