Octaves and inharmonicity in piano tuning

Similar documents
y = log b Exponential and Logarithmic Functions LESSON THREE - Logarithmic Functions Lesson Notes Example 1 Graphing Logarithms

MAT120 Supplementary Lecture Notes

PHY-2464 Physical Basis of Music

SUPPLEMENTARY MATERIAL FOR THE PAPER "A PARAMETRIC MODEL AND ESTIMATION TECHNIQUES FOR THE INHARMONICITY AND TUNING OF THE PIANO"

MCAT Physics Problem Solving Drill 13: Sound

1) The K.E and P.E of a particle executing SHM with amplitude A will be equal to when its displacement is:

Harmonic Motion: The Pendulum Lab Advanced Version

Physics 9 Fall 2009 Homework 12 - Solutions

What does the speed of a wave depend on?

Unit 4 Waves and Sound Waves and Their Properties

Sound. Speed of Sound

HW Set 2 Solutions. Problem 1

Reflection & Transmission

Equal Temperament and Pythagorean Tuning: a geometrical interpretation in the plane

Chapter 18 Solutions

Chapter 16: Oscillatory Motion and Waves. Simple Harmonic Motion (SHM)

FOURIER ANALYSIS. (a) Fourier Series

Superposition and Standing Waves

Homework #4 Reminder Due Wed. 10/6

Fourier Analysis. David-Alexander Robinson ; Daniel Tanner; Jack Denning th October Abstract 2. 2 Introduction & Theory 2

-Electromagnetic. Waves - disturbance that propagates through space & time - usually with transfer of energy -Mechanical.

Chapter 8: Wave Motion. Homework #4 Reminder. But what moves? Wave properties. Waves can reflect. Waves can pass through each other

Physics 202 Homework 7

To prepare for this lab, you should read the following sections of the text: Sections 3.4, 11.3, and 12.1 OVERVIEW

Consonance of Complex Tones with Harmonics of Different Intensity

Math and Music Part II. Richard W. Beveridge Clatsop Community College

7-6. nth Roots. Vocabulary. Geometric Sequences in Music. Lesson. Mental Math

arxiv: v1 [physics.pop-ph] 10 Aug 2015

Physical Modeling Synthesis

Wave Phenomena Physics 15c. Lecture 9 Wave Reflection Standing Waves

arxiv: v3 [physics.pop-ph] 14 Nov 2015

Nicholas J. Giordano. Chapter 13 Sound

KEY TERMS. compression rarefaction pitch Doppler effect KEY TERMS. intensity decibel resonance KEY TERMS

Applying Root-Locus Techniques to the Analysis of Coupled Modes in Piano Strings

Lecture 14 1/38 Phys 220. Final Exam. Wednesday, August 6 th 10:30 am 12:30 pm Phys multiple choice problems (15 points each 300 total)

Physics 25 Section 2 Exam #1 February 1, 2012 Dr. Alward

Producing a Sound Wave. Chapter 14. Using a Tuning Fork to Produce a Sound Wave. Using a Tuning Fork, cont.

Physics 6B. Practice Midterm #1 Solutions

Additive Numbering Systems and Numbers of Different Bases MAT 142 RSCC Scott Surgent

-Electromagnetic. Waves - disturbance that propagates through space & time - usually with transfer of energy -Mechanical.

Chapter 20: Mechanical Waves

DOING PHYSICS WITH MATLAB WAVE MOTION STANDING WAVES IN AIR COLUMNS

General Physics I Spring Oscillations

Time-Frequency Analysis

arxiv: v2 [physics.class-ph] 12 Jul 2016

Quiz on Chapters 13-15

Chapters 11 and 12. Sound and Standing Waves

CHAPTER 1 REVIEW Section 1 - Algebraic Expressions

Origin of Sound. Those vibrations compress and decompress the air (or other medium) around the vibrating object

Weber Fechner s law, uncertainty, and Pythagorean system

Einstein Classes, Unit No. 102, 103, Vardhman Ring Road Plaza, Vikas Puri Extn., Outer Ring Road New Delhi , Ph. : ,

Pythagoras Πυθαγόρας. Tom Button

Physics Worksheet Sound and Light Section: Name:

Chapter 15 Mechanical Waves

Worksheet #12 Standing waves. Beats. Doppler effect.

Audio Features. Fourier Transform. Fourier Transform. Fourier Transform. Short Time Fourier Transform. Fourier Transform.

3 THE P HYSICS PHYSICS OF SOUND

Convention e-brief 473

Uniform circular motion, angular variables, and the equations of motion for angular

Physics 202 Quiz 1. Apr 8, 2013

STATISTICAL APPROACH FOR SOUND MODELING

Lecture 6: Differential Equations Describing Vibrations

Work. Work and Energy Examples. Energy. To move an object we must do work Work is calculated as the force applied to the object through a distance or:

Fall 2010 RED barcode here Physics 123 section 2 Exam 2

PHYSICS 220. Lecture 21. Textbook Sections Lecture 21 Purdue University, Physics 220 1

Math Circles Intro to Complex Numbers Solutions Wednesday, March 21, Rich Dlin. Rich Dlin Math Circles / 27

Name Date Credit. Homework #48: Direct Variation and Proportion Read p

Section 2.7 Solving Linear Inequalities

University of Colorado at Boulder ECEN 4/5532. Lab 2 Lab report due on February 16, 2015

Music Synthesis. synthesis. 1. NCTU/CSIE/ DSP Copyright 1996 C.M. LIU

Physics 106 Group Problems Summer 2015 Oscillations and Waves

A Quantitative Study of Relationships Between Interval-width Preference and Temperament Conditions in Classically-trained Musicians Byron Pillow

Einstein Classes, Unit No. 102, 103, Vardhman Ring Road Plaza, Vikas Puri Extn., Outer Ring Road New Delhi , Ph. : ,

PHY205H1F Summer Physics of Everyday Life Class 7: Physics of Music, Electricity

Robert Hooke De Potentia Restitutiva, Introduction

Part I Multiple Choice (4 points. ea.)

The Role of Continued Fractions in Rediscovering a Xenharmonic Tuning

arxiv: v1 [cs.sd] 14 Nov 2017

Oscillations - AP Physics B 1984

LAST NAME First Name(s) Student Number Practical Group as on student card as on student card Code

LAST NAME First Name(s) Student Number Practical Group as on student card as on student card Code

Marketed and Distributed By FaaDoOEngineers.com

1 Hz = 1 1. f = 2L. WENDY S XENHARMONIC KEYBOARD

PLEASE NOTE THAT YOU MUST BE ABLE TO DO THE FOLLOWING PROBLEMS WITHOUT A CALCULATOR!

APMTH 105 Final Project: Musical Sounds

Superposition & Interference

Chapter 8 Review, Understanding pages Knowledge

PHY 103: Standing Waves and Harmonics. Segev BenZvi Department of Physics and Astronomy University of Rochester

string is V. If a second weight W is added without stretching the string, the speed of pulses on this string will now become

Seminary 10 SOUND WAVES 2

Laboratory 4: Wave Motion and Resonance

Answer: 101 db. db = 10 * log( 1.16 x 10-2 W/m 2 / 1 x W/m 2 ) = 101 db

KEY SOLUTION. 05/07/01 PHYSICS 223 Exam #1 NAME M 1 M 1. Fig. 1a Fig. 1b Fig. 1c

Normal modes. where. and. On the other hand, all such systems, if started in just the right way, will move in a simple way.

42 TRAVELING WAVES (A) (B) (C) (D) (E) (F) (G)

Study Guide: Semester Two ( )

Physics 107: Ideas of Modern Physics

12.1 Homework Set 1a Solutions

Final Practice Problems

2. Limits at Infinity

Transcription:

Octaves and inharmonicity in piano tuning Kees van den Doel January 11, 2013 Abstract I show that equal beating 4:2/6:3 octaves (called 4:2+ octaves) results in an approximately equal beating 2:1 octave as well as long as the inharmonicity is increasing when going up, i.e., above the break. The consequences for 4:1 and 8:1 double and triple octave beat rates is also analysed. 1 Partials, beats, and cents Let s start by reviewing some basic formulae and definitions. Suppose we have two single frequencies (sine waves) x and y, measured in Hertz (or any other units). The cent distance c between y and x is per definition c = 1200 log(y/x), (1) log 2 with log the natural logarithm. If x and y are very close we will hear a beat with frequency (beatrate) b = y x. The beatrate is given very accurately in terms of the cent difference by b = log 2 cx. (2) 1200 For example is x = 440Hz and c = 1 we get b 1/4, i.e., one beat every 4 seconds for a 1 cent detuned A4 unison. A real piano tone is composed of not just a single frequency but a set of partials. In the absense of inharmonicity the partial frequencies are x, 2x, 3x,... with x the fundamental frequency. In terms of cents the distance of the i-th partial from the fundamental is given by c(i) = 1200 log(i), i = 1, 2, 3,... (3) log 2 1

2 In a real piano the partials are all shifted up by a small amount, and effect called inharmonicity. We consider here the Young model [2] and a more realistic modification thereof based on piano data by Robert Scott as implemented in Tunelab [1]. According to this model each partial i is offset by an amount B(a i 1) where B is the inharmonicity constant of the note and the coefficients a i are given by in the Young model and are given by a i = i 2 (4) a 1 = 1 a 2 = 4 a 3 = 8.45 a 4 = 13.18 a 5 = 19.72 a 6 = 27.27 a 7 = 35.53 a 8 = 46.25 (5) by the Tunelab model. Values for higher partials can be found in the Tunelab manual. Formula (3) is thus modified to c(i) = 1200 log 2 log(i) + B(a i 1). (6) 2 Tuning the octave by partial matching Consider tuning a note N 2 an octave above a note N 1. Both notes have a partial structure given by (6), but will have different inharmonicity constants B which we call B 1 and B 2. Above the break B 2 will be about twice the value of B 1. Let s measure all the partials in cents relative to the fundamental of N 1. Also, let s assume we first tune N 2 so that its fundamental is exactly 1200 cents above the fundamental of N 1 and then adding a stretch of s 2 cents, where the value of s 2 is to be determined later. The cent values of the i-th partials of both notes (w.r.t the fundamental of N 1 ) are now given by c 1 (i) = 1200 log 2 log(i) + B 1(a i 1) c 2 (i) = 1200 + 1200 log 2 log(i) + B 2(a i 1) + s 2. (7) As a warm-up excercise, let s compute the stretch s 2 first for a 2:1 octave. We want the second partial of N 1 to match the first partial of N 2, so the equation to solve for

3 s 2 is c 1 (2) = c 2 (1) which reads 1200 + B 1 (a 2 1) = 1200 + s 2, (8) where we have used a 1 = 1. We thus get for a 2:1 octave the stretch s 2 [2 : 1] = B 1 (a 2 1). (9) For example if N 1 = C4 and using a typical value B 1 = 0.404 we get a stretch of 1.21 cents. We can calculate the theoretical stretch for the 4:2 and 6:3 octaves in the same manner by solving c 1 (4) = c 2 (2) and c 1 (6) = c 2 (3) which gives and s 2 [4 : 2] = B 1 (a 4 1) 3B 2 (10) s 2 [6 : 3] = B 1 (a 6 1) B 2 (a 3 1). (11) We see that the larger B 2 is, i.e., the steeper the inharmonicity curve is, the less stretch is required for these octaves. Taking the average values for C4 and C5 from the Tunelab sample data, B 1 = 0.404 and B 2 = 1.116 this gives stretches of s 2 [4 : 2] = 1.57 and s 2 [6 : 3] = 2.3 cents. 3 Tuning the octave by equal beating 4:2 and 6:3 Next we will compute the stretch required for the 4:2+ octave, which has equal beating 4:2 and 6:3, with 4:2 being wide, and 6:3 narrow. First we need the cent difference (i) between partial i of N 2 and partial 2i of note N 1. Using (7) we get (i) = c 2 (i) c 1 (2i) = B 2 (a i 1) B 1 (a 2i 1) + s 2. (12) A positive (i) means the 2i : i octave is wide, a negative means it is narrow. The beat rate b(i) of this difference according to (2) is given by b(i) = log 2 1200 (i)2if 0 (13) where f 0 is the frequency of the fundamental of N 1. Note that the frequency of partial 2i is not exactly 2if 0 but the difference is very small and lies beyond the threshold of hum beat speed discrimination. The beat frequency (or rate) of the 2i : i octave as given by (13) is positive if the octave is wide, and negative if narrow. We now want to find s 2 such that b(2) = b(3), i.e., the 4:2 beats wide at the same speed the 6:3 beat narrow. Using (13) and (12) we obtain the stretch s 2 b(2) + b(3) = 0 2 (2) + 3 (3) = 0 2B 2 (a 2 1) 2B 1 (a 4 1) + 2s 2 + 3B 2 (a 3 1) 3B 1 (a 6 1) + 3s 2 = 0 s 2 [4 : 2+] = (B 1 (2a 4 + 3a 6 5) B 2 (2a 2 + 3a 3 5))/5. (14)

4 If we use the numbers as after (11) we obtain a stretch of 2 cents. However if we used Young s model the stretch would come out to be about 4.2 cents, which is more than twice as much! With the 4:2+ stretch (14) in had we can now compute the beat rates of the various octave partial matches by using (12) and (13). After some algebra we get the 4:2+ octave 2i:i beat rates b(i) = f 0 log 2 3000 [B 1(2a 4 + 3a 6 5a 2i ) B 2 (2a 2 + 3a 3 5a i )]i. (15) For the Tunelab model this comes out to be for 4:2 as b(2) = b 4:2 = f 0 log 2 1200 (33.82B 1 10.7B 2 ). (16) Of course be have b(2) = b(3) which is easy to check. The big question is now, what about 2:1? So let s compute the beat rate difference between 4:2 and 2:1, i.e., b(2) b(1) using (15). We get b(2) b(1) = f 0 log 2 3000 [B 1(2a 4 + 3a 6 + 20 10a 4 ) B 2 (2a 2 + 3a 3 35)]. (17) Remarkably, for Young s model a i = i 2 the coefficients of B 1 and B 2 are both zero so we have 2:1 beating at exactly the same speed as 4:2 and 6:3. For the tunelab model, plugging in in the table values we obtain instead b(2) b(1) = f 0 log 2 3000 [1.65B 2 3.63B 1 ]. (18) So if B 2 = 2.2B 1 we have 2:1 equal beating, and this relation is almost satisfied on most piano scales. Even if it were not and we had B 2 = B 1 or B 2 = 4B 1 which are extreme values probably not found on any real piano, we still have a beat speed difference of only 0.1 and 0.14 Hz (or beats per second if you like): virtually equal beating! For comparison the 4:2 (and 6:3) beat speed in this example is 0.5 Hz. On the other hand, the 8:4 octave is quite narrow and beats at 6.4 Hz. 4 Double and triple octaves Let us now imagine tuning N 2 to N 1 as a 4:2+ octave, and next N 3 to N 2 and N 4 to N 3 with the same method. What will the double octaves (4:1) and triple octave (8:1) be like? To analyze this we extend (7) for the notes N 1,..., N 4, measuring all frequencies in cents relative to the fundamental of N 1 for analysis purposes. As the octave stretches are cumulative we now obtain the following expression for the i-th partial of octave k c k (i) = 1200(k 1) + 1200 log 2 log(i) + B k(a i 1) + k s j. (19) j=1

5 where s j is the stretch of octave N j N j 1 for j > 1 and for notational convenience we define s 1 = 0. The individual octave stretches are obtained from (14) as s k = [B k 1 (2a 4 + 3a 6 5) B k (2a 2 + 3a 3 5)]/5, k > 1, (20) where B k is the inharmonicity constant of note N k. To simplify notation let s write (20) as with s k = q 1 B k 1 q 2 B k, k > 1, (21) q 1 = (2a 4 + 3a 6 5)/5 = 20.634 (27) q 2 = (2a 2 + 3a 3 5)/5 = 5.67 (6), (22) where the numerical values are according to the Tunelab model and the parenthesized values according to Young s model. It is now easy to obtain the 4:1 beat rate (of N 1 versus N 3 ) as b 4:1 = log 2 300 f 0[c 1 (4) c 3 (1)] = log 2 300 f 0[s 2 + s 3 B 1 (a 4 1)]. (23) Substituing the values from (21) gives b 4:1 = log 2 300 f 0[c 1 (4) c 3 (1)] = log 2 300 f 0[(q 1 + 1 a 4 )B 1 + (q 1 q 2 )B 2 q 2 B 3 ]. (24) Numerically using the Tunelab model this gives b 4:1 = f 0 log 2 1200 (33.82B 1 + 59.9B 2 22.7B 3 ) (25) to be compared with for example the 4:2 beat rate of the N 2 N 3 single octave given by (16) which gives b 4:2 = f 0 log 2 1200 2(33.82B 2 10.7B 3 ). (26) (Note the extra factor 2 as we are considering the second single octave.) Let s take (B 1, B 2, B 3 ) = (0.404, 1.116, 2.12) from the Tunelab average tuning file, corresponding to C4-C5-C6. Unfortunately both C5-C6 4:2 and the C4-C6 4:1 beat rates are about 9 Hz (both wide) which is much too high to be acceptable. The C4-C5 4:2 beat rate remains good of course, about 0.5 Hz. The reason is that the steeper the slow of the inharmonicity curve, the better the 4:2 octave is as follows from (26), up to a limit of B3 3B2 where both 4:2 and 6:3 become pure (at the expense of 2:1). As a second example let us consider the octaves F3F4F5F6 tuned according to 4:2+ for the case of a Kawai K3 for which I have the inharmonicity constants which are (0.372, 0.566.1.56, 3.6). Plugging in the numbers we get an F3F4 4:2 beat rate of 0.5 Hz, an F4F5 4:2 beat rate of 5.7 Hz, and 33Hz for F5F6. The 4:1 beat rates are 1 Hz for F3F5 and 6 Hz for F4F6.

6 5 Conclusions The equal beating 4:2/6:3 octave (4:2+) leads to virtual identical beating rates of also the 2:1 octave. Whenever the beat rate is slow in the absolute sense the theory therefore support the notion that this is the aurally purest octave size. However, this seems to apply only to the temperament octave, as outside the temperament octave as it leads to much too fast beating 4:2 octaves and 4:1 double octaves. Above this area the stretch has to be reduced, sacrificing the 6:3 octave (which rapidly becomes too high pitched to be relevant anyways) for a slower 4:2 beat. References [1] Robert Scott. Tunelab piano tuning software. http://www.tunelab-world.com. [2] Robert W. Young. Inharmonicity of Plain Wire Piano Strings. The Journal of the Acoustical Society of America, 24(3), 1952.