Halbert Frederick Gates candidate for the degree of Doctor of Philosophy Final examination, May 24, 1954, 1:00 P.M. room, Physics-Mathematics Building Conference Dissertation: Determination of the Ratio p/q of the Photoelastic Constants of Optical Glasses by Means of Two Different Ultrasonic Methods Outline of Studies Major subject: Minor subject: Physics Mathematics Biographical Items Born, October 30, 1919, Milwaukee, Wisconsin Undergraduate Studies, Milwaukee State Teachers College, 1936-1940 Graduate Studies, University of Wisconsin, 1940-1944, continued 1947-1948, Michigan State College, 1950-1954 Experience: Graduate Assistant, University of Wisconsin, 1941-1944; Officer in Charge, Principles of Elec­ tricity Section, Theater Signal Corps School (Germany), 1946; Assistant Professor of Physics, Berea College, 1948-1950; Special Graduate Research Assistant, Michigan State College, 1951-1954 Member of American Physical Society, American Association of Physics Teachers, Society of Sigma X i , Sigma Pi Sigma, Pi Mu Epsilon, Kappa Delta Pi DETERMINATION OP THE RATIO p/q OP THE PHOTOELASTIC CONSTANTS OP OPTICAL GLASSES BY MEANS OF TWO DIFFERENT ULTRASONIC METHODS by Halbert Frederick (Gates AN ABSTRACT Submitted to the School of Graduate Studies of Michigan State College of Agriculture and Applied Science in partial fulfillment of the requirements for the degree of DOCTOR OP PHILOSOPHY Department of Physics and Astronomy 1954 Approved ^ ProQuest Number: 10008463 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest ProQuest 10008463 Published by ProQuest LLC (2016). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code Microform Edition © ProQuest LLC. ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 4 8 1 0 6 - 1346 Halbert F. Gates ABSTRACT Mueller (l) has described, in theory, two dynamic methods for the determination of the ratio p/q of the strainoptical constants of glass. The strains are produced by ultrasonic waves in the glass, while the optical effects are observed in the diffraction patterns produced by light which has passed through the sound field. The theory of Mueller is an extension of that of Raman and Nath (2) which explains the diffraction of light by a sound wave on the basis of varia­ tions of the index of refraction of the medium traversed by the sound wave. Measurements were made on a series of thirteen American optical glasses and fused silica, following Mueller's methods ,IB" and "C11, The ultrasonic frequency was in the neighborhood of ten megacycles per second. Method "B" involves the methods of Hiedemann (3 ). Measurements are made of the polarizations in the diffraction pattern at several amplitudes. An extrapolation to zero sound amplitude leads to a value for p/q. The experimental results are In excellent agreement with the theory. Values of p/q were determined for all of the samples, the ratios ranging from 1.11 to 2.34. Halbert F. Gates Method "Cu involves the methods of Bergmann and Fues (4)• Measurements are made of intensity ratios in the diffraction patterns at several sound amplitudes* The experimental values at various sound amplitudes, while of the correct order of magnitude, do not agree with the theory. Extrapolation cannot be performed as indicated in the theory, and no value of the ratio p/q can be deter­ mined. The behavior of the data is, however, consistent and systematic and it is hoped that some significance may be attached to it. The values of the ratio p/q of the strain-optical con­ stants, as obtained by method MB", are given, together with other data on the samples. The behavior of the data as ob­ tained by method "C11 is described. Literature Cited 1. H. Mueller, Z. Kristallogr. A, 99, 122 (1938) 2. C. V. Raman and N. S. N. Nath, Proc. Indian Acad. Sci. A, 2, 406 (1935); 3, 75 (1936); 3, 459 (1936) « 3. E. Hiedemann, Z. P h y s ., 108, 592 (1938) 4. L. Bergmann and E. Fues, Naturwissenschaften, 24, 492 (1936) DETERMINATION OF THE RATIO p/q OF THE PHOTOELASTIC CONSTANTS OF OPTICAL GLASSES BY MEANS OF TWO DIFFERENT ULTRASONIC METHODS by Halbert Frederick Gates A THESIS Submitted to the School of Graduate Studies of Michigan State College of Agriculture and Applied Science in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Department of Physics and Astronomy 1954 ACKNOWLEDGMENTS The author wishes to express his sincere thanks to Dr. E. A. Hiedemann who suggested this investigation and has given valuable and helpful guidance throughout the course of its development. Greatful acknowledgment is also due to Dr. C. D. Hause for his help with the photo­ metric measurements. This work was supported by a grant from the OwensIllinois Glass Company. The author greatly appreciates the resulting Special Graduate Research Assistantship which made it financially possible for him to pursue the problem. table of contents Page INTRODUCTION 1 Definitions of Photoelastic Constants 1 Static Determination of Photoelastic Constants 2 Dynamic Determination of Photoelastic Proper­ ties of Glass by means of Ultrasonic Waves 2 Purposes of this Investigation 5 Theory of Photoelasticity in Glass 5 THEORY 7 Basis of the Mueller Theory 7 Special Conditions for this Investigation 7 Conclusions of the Mueller Theory for Standing Longitudinal Sound Waves 9 B and 0 as Functions of v and of Sound Ampli­ tude 12 Justification for Consideration of Only r = 0 Sub-components of First Diffraction Orders 15 Indication of Sound Amplitude 16 APPARATUS AND METHODOLOGY 18 Ultrasonic Generator 18 Transducer 26 Optical Arrangements and Measurements 26 Temperature 31 Glass and Fused Silica Samples 34 Page presentation of data 40 Method nB" 40 Method 11C" 42 Values of R from Other Investigations 46 SUMMARY AND CONCLUSIONS 49 APPENDIXES I Theoretical Intensity Ratios in the Diffraction Orders 52 II Sample Data and Calculation for Method "B" 56 III Sample Data and Calculation for Method "C" 59 BIBLIOGRAPHY 64 LIST OF FIGURES Page Figure 1. Theoretical variation of tan 0 and v2 -5b " with 13 2. Oscillator and power amplifier 19 3. Voltage-regulated power supplies 24 4. High voltage power supply 25 5. Transducer matching circuit 25 6. Optical system for method "B" 27 7. Optical system for method "C" 27 8. Experimental variation of tan 6 with I2 29 9. 10. 11. 12. Exoerimental variation of in BSC-1 v— with I 2 32 Experimental variation of in DBF-1 -5B" with Experimental variation of in fused silica -JB* with Experimental variation of in CF-1 -iRB with I2 32 12 33 I2 33 list of Ta b l e s Page TABLE I ELECTRICAL COMPONENTS 20 II DESCRIPTION OF GLASS SAMPLES 35 III COMPOSITION OF GLASS SAMPLES 37 NUMERICAL RESULTS 43 VALUES OF p/q GIVEN BY OTHER INVESTIGATORS 47 IV V VI VII VIII IX TOTAL INTENSITY RATIOS: ORDER, METHOD "B" THIRD ORDER TO ZERO 53 SUB-COMPONENT INTENSITY RATIOS: FIRST TO ZERO SUB-COMPONENTS, FIRST ORDER, METHOD "B" 53 TOTAL INTENSITY R a TIOS: ORDER, METHOD f,C" 54 SECOND ORDER TO ZERO SUB-COMPONENT INTENSITY R a TIOS: FIRST TO ZERO SUB-COMPONENTS, FIRST ORDER, METHOD MC" 55 INTRODUCTION Definitions of Photoelastic Constants P o c ke ls 1 strain-optical constants. Pockels (l) has given a set of thirty-six phenomenological constants which relate the general strain tensor to the optical effects which accompany it. In the case of an isotropic material these constants, p^j (the subscripts run from one through six), are reduced by symmetry considerations to two, p ^ and P 12 * Neumann's strain-optical constants. Neumann (2) de­ scribes the photoelastic behavior of an isotropic medium by means of two strain-optical constants, p and q. These constants relate a strain to the changes which it produces in the index of refraction n for light vibrating parallel and normal respectively to the direction of the strain. Equation (1) defines the Neumann constants in terms of a typical strain zz . n 3- n = 1 z.2 * d n x = n x- n = — n p z * Equation U) (2) shows the relation between the Neumann constants and the Pockels constants for an isotropic material. 2 It is assumed that the fine-annealed optical glass used in this investigation is an isotropic material, and the dis­ cussion is in terms of the Neumann strain-optical constants, p and q. Stress-optical constants* The optical effects may also be described in terms of the stress which causes them. deed, In­ in measurements beyond the elastic limit, Filon and Jessop (3) find evidence that stress is the fundamental quantity related to the optical effects. It is assumed in this investigation that the deformations are small and that H o o k e 1s Law applies and that stress and strain constants are equally significant. Static Determination of Photoelastic Constants Determinations of the photoelastic constants of glass by means of the application of steady stress have been made by Mach (4), Pockels (5), Filon (6), Twyman and Perry and Schaefer and Nassenstein (8). (7), These static methods often involve difficult optical measurements requiring large or specifically shaped samples, two "Identical11 samples, and/or precise temperature control. The samples are subject to re­ laxation or plastic flow as described by Coker and Filon Dynamic Determination of Photoelastic Properties of Glass oy means of Ultrasonic Waves The dynamic strains are produced in the glass by (9). 3 ultrasonic waves. The optical effects are observed in the diffraction of a beam of light which has passed through the sound field. Diffraction of light by ultrasonic w a ve s. Early obser­ vations of the scattering or diffraction effect of an ultra­ sonic field on a beam of light were made by Debye and Sears and by Lucas and Biquard (ll). The use of a point source of light to show the diffraction of light by many sound waves simultaneously was developed by Schaefer and Bergmann (12) (13) (14). The use of a slit source of light to show the diffraction by a single wave was developed by Hiedemann and Hoesch (15) vestigation. (16) (17). This is the method used in this in­ The slit is made parallel to the sound wave front and the light beam is normal to the sound beam. line diffraction pattern is then formed. A This investigation also makes use of the polarization techniques of Hiedemann and Hoesch (18) for the separation of the effects of longi­ tudinal and transverse sound waves. Raman and Nath (19) have given a theory of the dif­ fraction of light by a sound field. The theory is based on the phase changes in the light wave as it passes through the periodic structure of variations of index of refraction caused by the sound field. The effect on the light is the production of a "corrugated wave front11 which leads to a diffraction pattern. The theory gives the directions, in­ tensities, and frequencies of the light in the diffraction (10) 4 orders. The theory has been verified on the basis of experi- u ments by Bar / \ (20) and Sanders / (21). Determination of the ratio p/q of the strain-optical constants. theory. Mueller (23) has extended the Raman and Nath He evaluates the index variations in terms of the strain-optical constants of the medium. This leads to ex­ pressions for the directions, polarizations, frequencies, and intensities of the elements of the diffraction pattern in terms of the strain-optical constants and the sound amplitude. Many of the conclusions have been experimentally verified by Hiedemann (24) Mueller (25). (23) gives three methods for the experimental evaluation of the ratio p/q. Method "B11 involves measurements of the polarizations of the diffraction orders in the Hiedemann spectrum. of this method have been used on glasses by Vedam (26) Forms (27) and by Schaefer and Dransfeld (28). Method "C" involves measurements of the intensity ratios in the diffraction orders. A partially similar method has been used on glasses by Bergmann and Fues (29). Method "A” applies to certain crystals (but not also to glasses, as do "B" and ,?C ,f), yielding ratios of strainoptical constants. Measurements have been made on crystals by Burstein, Smith, and Henvis (30) and by Galt (31). Galt reports agree­ ment with the theory of photoelasticity in cubic crystals 5 given by Mueller (32), while Burstein and Smith (33) in­ dicate the need of some modifications. These dynamic determinations offer- some characteristic advantages. The results are obtained directly in terms of the strain-optical constants, which are, according to Mueller (23), of greater theoretical importance than the stress-optical constants. Small samples are sufficient. There are no effects due to relaxations with time constants which are long with respect to the period of the sound. Purposes of this Investigation This investigation had two purposes. The first was to determine dynamic values of the ratio p/q for a series of American optical glasses and fused silica. to compare methods The second was MB ,r and "C" as a check on the values and on the theory. These results are made more interesting by other work completed or projected in this laboratory. vestigation was in progress Barnes While this in­ (34) determined dynamic values of the elastic constants of the same set of samples. A projected problem involves static measurements leading to values of p and q for the same samples. Theory of Photoelasticity in Glass A theory of photoelasticity in amorphous solids has been given by Mueller (35). ascribed to two effects. The photoelastic behavior is The first involves elastic 6 alterations in the Lorentz-Lorenz interactions between di­ poles. The second Involves the production of artificial optical anisotropy of the atoms. Under the action of p r es ­ sure the first produces positive birefringence while the second produces negative birefringence. The second is usually the larger, but when the index of refraction reaches large values the first may surpass it. An effect due to the alignment (by deformation) of optically anisotropic molecules is discussed by Treloar (36) and Braybon (37), but is probably of significance only for long high-polymers• 7 THEORY Basis of the Mueller Theory The basic ideas in Mueller*s extension of the Raman and Nath theory are outlined in the Introduction. M ue ller’s methods f,B" and "C,r for the determination of the ratio p/q are identified. Special Conditions for this Investigation Homogeneous and isotropic m at e r i a l . It is assumed that fine-annealed optical glass is homogeneous and isotropic. Each of the samples was good enough to permit almost complete extinction when placed between crossed polarizers. Longitudinal sound w a v e s . The observed effects were entirely due to longitudinal sound waves. used was an x-cut quartz crystal The transducer (a thickness vibrator) so that the primary wave in the glass was a longitudinal wave. Frequencies were chosen at which the blocks exhibited strong resonances for the longitudinal modes and weak resonances for transverse modes. In method ,fB" the polarizer and analyzer are set at forty-five degrees to the sound wave front. Hiedemann and Hoesch (18) have shown that this arrangement eliminates the effect of transverse waves. In method "C" the absence of significant transverse waves can be checked visually since their velocity differs from that of longi­ tudinal waves and the corresponding diffraction patterns 8 have different spacing. Standing sound w a v e s . In a one inch cube of a low- absorption material like glass it would be very difficult to produce anything other than standing waves. The appear­ ance of intense diffraction patterns due to resonances as the frequency was changed gave evidence of the standing wave condition. The theory of Raman and Nath notes that each line in the diffraction pattern due to standing waves is composed of sub-components having different frequencies and polarizations. by the Index m. The diffraction orders are Identified The value zero corresponds to the central order while the index one corresponds to the first order and so on. The sub-components are identified by the index r, which may be zero or have positive integral values. Diffraction order and sub-component. component (r=0) Only the zero sub­ of the first diffraction order considered in any of the measurements. (m = l) was Justification for this will appear below. Applicability of Raman and Nath Theory. The sound frequencies used were in the neighborhood of ten megacycles per second. The optical path length in the sound field was about two centimeters. These values place this investigation In the region in which the Raman and Nath theory applies. Experimental verifications of the theory been mentioned above. involved in this work. (in liquids) have The wave lengths correspond to those A theoretical condition for 9 applicability has been given by riytov (38). (X*) It is (3) z where L is the optical path length in the sound field, is the optical wave length, Willard X XT is the acoustic wave length. (39) gives for a criterion (4) including the Baman and Neth argument v, which, work, is seldom greater than unity. in this Both of these criteria place these measurements in the province of the theory. Conclusions of the Mueller Theory for Standing Longitudinal Sound Waves Arrangement for method MB ,f. The arrangement for method trB" requires the light beam to be perpendicular to the sound propagation direction. the sound wave fronts. degrees to the slit. The slit is parallel to The polarizer is set at forty-five This optical arrangement is diagramed in Figure 6. In this case the polarization of the sub-component r of the diffraction order m of the Hiedemann spectrum is given by (5) ixn ('«w,v+ 4s'°) if bo = X S 10 where s Is zero or any positive integer. ^ iY is the angle of rotation of the analyzer from the crossed position which causes extinction of the sub-component order m . x of the diffraction J is the Bessel function of the first kind and of order indicated by the subscript. the strain-optical constants. R is the ratio p/q of v is the argument of the Bessel functions in the Raman and Nath theory, given by _ 2.TT./U-L A _ 4-TT*l_n*ci A ~ A A' . . ' where j*. is the amplitude of variation of the index of re­ fraction associated with the strain-optical constant q, L is the optical path length in the sound field, optical wave length in air, A is the A * is the acoustical wave length, n is the index of refraction of the medium, and A is the acoustical amplitude. It is to be noted that the quantity v is proportional to the amplitude A of the sound wave • In the case (used in this investigation) where r = 0 and m = l, equation 5 becomes J [Rv') T (Rv'j to.* © = t o ^ ( T 0+4-S6) = — where 9 = 0 (7) , is the experimental quantity measured in method "B11. Arrangement for method irC n . The arrangement for method "C" requires the light beam to be perpendicular to the direc­ tion of propagation of the sound. The slit is parallel to 11 the sound wave fronts. gramed in Figure 7. This optical arrangement is dia­ Natural light passes through a Wollaston double image prism which splits it into two beams of equal intensity* the polarizations of which are normal to each other and parallel and normal respectively to the slit. two beams diverge slightly (forty-two minutes in this work) and give rise to two separate diffraction patterns. ratio The The of the intensities of corresponding lines in the two patterns is given by t) — (8) xv\ = 2* S T»-* I P (p where the symbols have the same meaning as in equation 5. In the case m =1, (used in this investigation) where r - 0 and equation 8 becomes ,____ To <9> B is the experimental quantity measured in method MC M . Analytical similarity of methods irB" and "C11, A com­ parison of equations 7 and 9 indicates that "tan 6 - -0 B — ----------— “ Jo where 0 ip j is the extinction angle (10) ,t p (from crossed position) plus forty-five degrees for the sub-component r = 0 of the first diffraction order of method "B" and B is the intensity ratio 12 of the r = 0 sub-components of the first diffraction orders of method "C". Thus two experimental quantities which may be independently measured are given by the same analytical expres s ion, B and 0 as Functions of v and of Sound Amplitude B solved and 9 as functions of v . Bquation 10 cannot be to give values of R since v contains quantities which cannot be accurately measured. Neither sound amplitude nor sound field width, for example, can be precisely known. However, as v approaches zero the right hand member of equation 10 approaches the value R. Thus, letting subscript zeros indicate limiting values, equation 10 becomes "tcun 0 o = i V B e — R (n) Figure 1, drawn from equation 10 shows the mode of ap­ proach of these quantities to their limit as v approaches zero. Tan 9 and iTB are plotted against the square of v merely in order to give a relation which is very nearly linear. The straight lines are drawn to show the departure of the points from the linear relation as v increases. when v For example, is less than unity and R is less than two, a straight line is a good approximation. Thus the "best" straight line (criterion of least squares) (40) through the four points shown in Figure 1 for R equal to two, intersects the vertical axis at 1.989, giving an error of 0.55 percent. None of the 13 APPEARANCE OF SECOND ORDER 9 = EXTINCTION ANGLE B = INTENSITY RATIO R * RATIO OF PHOTOELASTIC CONSTANTS I I --------------------------- 1------------ J--------------1--------------------------- 1--------------------------- 1--------------------------0.2 0.4 _ 0.6 0.8 1.0 V2 — ► Pig. 1. Theoretical variation of tan 0 and -d B with 14 glasses examined exhibited values of R greater than 1.83. B and 8 as functions of sound amplitude. Since v is proportional to sound amplitude, a similar linear relation­ ship exists between tan 9 or and the square of the sound amplitude, provided that the latter corresponds, general, to values of v less than unity. perimental points on a plot of tan 9 or in In this case ex­ - 5b against the square of the sound amplitude can be extrapolated linearly to give a value for tan d0 or t5B0 . Such an extrapolation was used in this investigation. It is necessary to relate the experimental sound am­ plitudes to values of v in order to justify the linear extrapolation. An approximate value of v corresponding to any given sound amplitude can be obtained from a comparison of the light intensities in the diffraction orders due to that sound. It is thus possible to consider only values of sound amplitude which correspond to acceptable values of v. The relationship between values of v and Intensities in the diffraction orders is given, In the case of liquids, by the theory of Raman and Nath (19). Good agreement between experiment and theory has been obtained by Sanders (21). For solids the theory has been extended by Mueller (23) to include the effect of the photoelastic constants. Since the optics differ, the relationship is different for the arrangements for methods ,fB M and "Cfl. Appendix I gives 15 M u e l l e r !s theoretical conclusions and lists numerical values in the range of Figure 1 and of this investigation. For the special case of method 11B 11 and a glass having R equal to 1.5, values of v corresponding to the appearance of second and third diffraction orders are indicated in Mueller's Figure 3 (23) (due to Hiedemann). These approxi­ mate values are indicated by the dotted vertical lines of Figure 1. In general, the values of v at which the diffraction orders appear, decrease as R increases. all conclusions may be drawn. The following over­ For method "B", when the third order diffraction line does not appear, the sound ampli­ tude corresponds to a value of v which lies on the essentially straight portion of the appropriate curve of Figure 1. extrapolation is then in order. Linear For method "Cu , when the second diffraction order does not appear, the sound amplitude corresponds to a value of v on the linear portion of the cor­ responding curve and extrapolation is justified. An arbitrary criterion for the "appearance" of a dif­ fraction order is an intensity in that order of approximately one percent of that in the central order. gested by Sanders One criterion sug­ (21) is 0.86 percent. Justification for Consideration of Only r = 0 Sub-components of First Diffraction Orders The numerical values given in Appendix I also indicate the conditions under which it is permissable to consider only 16 the r - 0 sub-components or the first diffraction orders. In method "B", when the third diffraction order does not appear, the ratio of the intensities in the r = 0 and first sub-components of the first diffraction order is not more than a few percent. Thus the extinction of the r = 0 sub­ component causes a distinct minimum in the intensity of the line* In method "C", when the second order does not appear, the ratio of the intensities in the r = 0 and r = l sub-compo­ nents of the first diffraction order is not more than about 0*1 percent. Thus an intensity measurement of the line Is equivalent to an Intensity measurement of the r = 0 sub-com­ ponent • In this work, third order lines never appeared during measurements by method "B" and second order lines never ap­ peared during measurements by method "CTt. Indication of Sound Amplitude Since the curve of tan 0 or v Tb plotted against the square of sound amplitude is extrapolated to zero sound, it is, fortunately, not necessary to determine absolute values of sound amplitude. Values of some quantity which is pro­ portional to sound amplitude are sufficient. is quartz (transducer) Such a quantity current or the current at any point In the series transducer circuit, as long as the geometry and frequency remain constant. A relationship between acoustic intensity J and piezoelectric transducer current I is given 17 by Cady (41). T = r R s/ z R g is the (12) (constant) series resistance of the transducer equivalent network and involves frequency, piezoelectric constants, dimensions, acoustic impedances, and wave velocity. Thus for a given transducer, coupled to a constant load and driven at a constant frequency, tional to transducer current* sound amplitude is propor­ The independent variable in this investigation has been transducer current. extrapolations to and tan 90 The linear were made on that basis. 18 APPARATUS AiJD MhThODOLOGY Ultrasonic Generator The ultrasonic generator designed and constructed as a part of this investigation consists of, six main parts, connected to operate as a unit and mounted in a r e l a y rack. Oscillator and power amplifier. Figure 2 shows the cir­ cuits of the oscillator and power amplifier which are con­ structed on the same chassis* Table I identifies the com­ ponents • The oscillator is an .electron-coupled Hartley circuit, modified to give maximum stability. Its frequency range is continuous from about 5.2 megacycles per second to about 13.6 megacycles per second. The radio-frequency power amplifier can deliver from one hundred and fifty to two hundred electrical watts. Plug­ in output coils cover the ranges from 5.7 to 12 megacycles per second and from 12 to 24 megacycles per second, with the output stage doubling in the upper range. When the circuit is well warmed up it Is able to main­ tain a frequency In the neighborhood of ten megacycles per second constant within one kilocycle per second for several hours. Stability was checked by means of a General Radio Type 620-A Heterodyne Frequency Meter while the approximate 19 x .9 U-O Q u_ 0 — ouig T" rin 0 -i UJ U_ I• li­ ar C\l U_ a: a: CT~ oc Oscillator and power amplifi ■OX (SJ ci •I— 1 20 TABLE I ELECTRICAL COMPONENTS Components for Oscillator and Amplifier (Figure 2) Ll,2,3 3.5 microhenrys C14 130 mmfd mica 600 v l4 a ) 18 microhenrys c17 0.001 mfd mica 3000 v 2*6 microhenrys B1 50,000 ohm zero temp % swinging link R2 . 68,000 ohm 1 w C1 ,2> 3 13-300 mmfd R3 10,000 ohm 1 w c4 11-150 mmfd dual r 4 25,000 ohm 1 w C5 10 mmfd variable R5 500 ohm 5 w c6 0*5 mmfd variable RFC1j2 2.5 mh 100 ma C7 75 mmfd zero temp r f c 3j4 2.5 mh 100 ma ce 0*01 mfd rfc5 1 mh 200 ma Cg,10,13 0.01 mfd 500 v r f c 6j7 14 turns -J” c15,16 0.01 mfd 500 v R FC 8 8 turns -J-ff CI1 50 mmfd mica 600 v b) Components i for Voltage-regulated Power Supplies (Figure 3) R3 15,000 ohm 5 w r4 90 ohm 600 v CT 120 ma; 5a 5 v 3a; 6.3v R 5,6 1000 ohm lw 7.5 v r T-j_ 5 v T2 550 v T, T4 3 a CT 250 ma 3 a 7 470,000 ohm 2w 21 TABLE I CONTINUED Components for Voltage-regul ated Power Supplies 6.3 v 3a (Figure 3) R 8,9 100 ohm h w 6.3 v i a R 10 12,000 ohm 25 w L1 24 h 200 ma R 1 1 ,12 1 meg 1 w L2 25 h 75 ma R 13 5,000 ohm 10 w 4 mfd 1000 v oil R 14 250,000 ohm 1 w C3, 4 16 mfd 600 v R 15 100,000 ohm -J- w C5, 5 0.1 mfd 400 v r 16 390,000 ohm 2 w c7 0.2 mfd 600 v r 17 50,000 ohm 2 w C8 4 mfd 600 v oil r 18 120,000 ohm 1 w R1 72 ohm 5 w r 19 500,000 ohm 1 w «2 5,000 ohm 50 w T5 t6 Cl» 2 VH tube firing relay Components for High Voltage Power Supply (Figure 4) 2.5 v 10 a 10,000 v insulation L1 5/25 h 225 ma swinging choke 1500 v (dc) 200 ma CT L 2,3 8 h 225 ma filter choke T3 0.4 kva autotrans­ former Cl,3 4 mfd 2,000 v oil R1 50,000 ohm 50 w c2 2 mfd 2,000 v oil *1 S1 thermal delay relay 22 TABLE I COLTIBLBD Components for Matching Circuit 2'1 diameter L1 22 turns Cl 20-200 mmfd 2 M length (Figure 5) 23 frequency given for each run depends upon measurements made with a General Radio Type 566-A Wavemeter. Voltage-Regulated Power Supplies. Figure 3 shows the circuits of the voltage-regulated power supplies which are constructed on the same chassis. Table I identifies the components• The minus seventy-five volt bias supply is regulated by two 0A3 gas discharge tubes operating in parallel. The load through these tubes must be carefully balanced in order to avoid excessive current in either. A delay relay applies the firing voltage to this pair simultaneously. the firing process is photosensitive, As it is sometimes neces­ sary to illuminate one or both tubes in order to fire both. The four hundred volt plate supply is adapted from one described by Elmore and Sands (42). It uses the series re­ actance tube principle and maintains a regulation of about 0.1 percent with a ripple of about five millivolts. High voltage power supply. Figure 4 shows the circuit of the high voltage power supply. components. Table I identifies the The filtering Is good and the circuit provides voltages from zero to fifteen hundred volts at currents from zero to two hundred mllliamperes• Impedance matching circuit. Figure 5 shows the circuit of the impedance matching unit which is connected to the trans­ ducer. Table I Identifies the components. This circuit would probably require modifications for operation above fifteen -AAAHI- 11-o Voltage-regulated power supplies ■vw Fig. 3. 24 vw AA/V 25 P 9 2 0Q >"na 866A Pig* 4. High voltage power supply GENERATOR OUTPUT o--TO TRANSDUCER Pig. 5. Transducer matching circuit 26 megacycles per second. The radio-frequency ammeter is the one used to indicate sound amplitudes by means of their proportionality to transducer current. Transducer The transducer used for all measurements was an x-cut quartz crystal (thickness vibrator), driven near its funda­ mental frequency of ten megacycles per second. The crystal was one inch square. about three- Aluminum foil electrodes, quarters of an inch square provided the electrical connections. Silicone grease and the glass. provided acoustic coupling between the crystal The sandwich was held in olace against the glass block by means of light spring pressure. Optical Arrangements and Measurements Method "B". method "B". Figure 6 shows the optical system for The light source is a General Electric Type A-H4 high intensity mercury lamp. Condenser lens luminates a slit of aperture about 0.05 millimeters. il­ The Gaertner Type L 541 E monochromatic filter combination iso­ lates the Hg5461 line. Lens Lg collimates the light. The polarizing prism is set at forty-five degrees to the slit. The light beam passes through the glass block normal to the direction of propagation of the sound waves. fronts are parallel to the slit. The analyzer is initially set in the "crossed" position for extinction. field is present, The sound wave When the sound a diffraction pattern is formed in the focal 27 filter polarizer analyzer Hg arc L| quartz glass block slit L 2 Fig. 6* filter L3 eye piece Optical system for method "B11 Wollaston prism Hg arc slit L Fig. 7. quartz V glass block L Optical system for method “C" camera 28 plane of lens (focal length, twenty Inches). The dif­ fraction pattern is viewed by means of an eyepiece. analyzer is then rotated through an angle position) (from the crossed to produce extinction (or a minimum) diffraction order. The in the first Ten minimum settings were made and averaged to determine the angle. This is the condition of extinction of the r = 0 sub­ component of the first diffraction order. be computed as in equation 7. Tan 8 can then This measurement was repeated for at least four different sound amplitudes corresponding to four values of transducer current. The maximum amplitude was made at least twice the minimum, but not great enough to produce third order diffraction lines. Typical plots of tan 8 versus the square of the trans­ ducer current I are shown in Figure 8. A linear extrapolation can then be made, as shown, to give values of tan 0 O by equation 11. , which are values of R as indicated It is more convenient and accurate, however to perform the extrapolation analytically (40), using the least squares criterion of best fit. Appendix II gives a sample calculation for the borosilicate crown glass of Figure 8. The data of this investigation was obtained by analytical extrapolation. Method »C». method "C11. Figure 7 shows the optical system for The production of the collimated beam is the same as for method "B” . In this case a Wollaston double 29 2.5 2.3 2.1 BOROS ILICATE CROWN TAN 9 1.9 1.7 20 [CURRENT IN AMP] 1.5 DENSE BARIUM FLINT 1.3 1.1 2 3 4 5 6 7 8 9 [CURRENT IN AMP. ] 2 Fig. 8. Experimental variation of tan 9 with I2 1.0 30 Image prism is inserted before the glass block. Two beams are thus formed, having polarizations normal and parallel respectively to the slit and to the sound wave fronts. beams diverge at an angle of forty-two minutes. The When a sound field is present In the glass, two diffraction patterns are formed In the focal plane of lens L^. These patterns are recorded photographically, as are also, for a comparison of Intensities, the images of the slit when no sound is present. Exposures were made for four or more sound amplitudes, cor­ responding to as many values of transducer current. The maximum amplitude was made at least twice the minimum, but not great enough to produce second order diffraction lines. The ratios of the Intensities in the first order lines of the two patterns were determined photographically. Be­ fore development, an emulsion calibrating exposure was made with Hg5461 light and a rotating step-wedge to give a pat­ tern of densities corresponding to ten or twelve exposures. Each step represents an exposure of one and one half times the previous value. These densities were compared to the densities of the diffraction pattern lines by means of a Jarrel-Ash Type JA-200 Microphotometer. Assuming the re­ ciprocity relation and no intermittency effect, the ratio of intensities B of the diffraction pattern lines was cal­ culated from the ratio of exposures in the step-wedge pattern. Two or three exposures were made for each sound ampli­ tude and two or three photometer readings were made on each first order line on each exposure. A correction was applied 31 for the (small) difference in intensities of the no-sound beams due to any slight misalignment of the Wollaston prism. Plots of i5"b versus the square of the transducer current I are shown in Figures 9, 10, 11, and 12. tained by this method. The data was ob­ No correspondence with the theoreti­ cal curves of Figure 1 is evident. No value of or of R is indicated. Appendix III gives a sample calculation by this method for the crown flint glass of Figure 12 , Temperature Importance of temperature. Since a change of temperature varies both the dimensions of the glass block and the velocity of sound, it may disturb the standing wave resonance condition and so alter the proportionality between transducer current and sound amplitude. Temperature gradients in the block might produce inhomogeneities or anisotropies which would disturb the optical measurements. Harris (43) and Filon (44) report small changes in photoelastic constants with changes in temperature. Room temperature. Since the glass block was cooled by a current of air, the temperature of this air (’’room tempera­ t u r e ” ) was the nominal temperature of the block. Room temperature was measured by means of an ordinary mercury thermometer placed in the neighborhood of the block. general, In a run was not satisfactory when the room temperature varied much more than one half of a degree centigrade. 32 1.95 r | J . 1.80 1.65 1.50 1.35 15 ± .30 Fig. 9. _L _L .45 .60 .75 .9 0 i2 [CURRENT IN AMP] 1.05 Experimental variation of 12 in BSC-1. 1.20 1.35 -J"B with 1.55 1.40 V q 1.25 .10 2 Fig. 10. 3 4 5 7 6 [CURRENT IN AM P]2 x I 0 2- 8 9 Experimental variation of xiB with Id in DBF-1. 33 2.50 2 .3 5 - t 1 2.20 - 2 .0 5 1.90 .75 2 3 4 [CURRENT IN A M P ]2 x I0 2-----^ Pig. 11. Experimental variation of *\Jb " with l2 in fused silica. 2.00 V | 1.85 b _ 1.70 1.55 1.40 2 3 4 5 6 7 8 9 [CURRENT IN A M P ]2 x I 0 2 ------ ► Fig. 12. Experimental variation of t)B with l2 in C F-1. 34 Block temperature. The temper&ture difference between the surface of the block and the surrounding air was measured by means of a thermocouple in contact with the surface and insulated from the air. This measurement gives some indica­ tion of the internal temperature of the block. Data was taken only when this temperature difference was less than one quarter of a degree centigrade. Glass and Fused Silica Samples Measurements were carried out on thirteen samples of fine-annealed optical glass and one sample of fused silica. The ordinary glasses were supplied by the Bausch and Lomb Optical Company, the rare earth glasses by the Eastman Kodak Company, and the fused silica block was fabricated in Germany and secured by the Owens-Illinois Glass Company through the Hanovia Chemical Company. The Bausch and Lomb samples and the fused silica block were one inch cubes. The Eastman samples were three quarter Inch cubes or near cubes. Table II gives descriptions of the samples. B&L re­ presents Bausch and Lomb, E represents Eastman, H represents Hanovia. The densities are those determined in this labora­ tory by Barnes (34) with the exception of the value for block number nine which is the manufacturer’s nominal density, n^ Is the nominal index of refraction for Na5893 light. V is the nominal dispersion, being given by the formula V = (n^p - l)/(np - nc) In which np refers to H4861 35 TABLE II DESCRIPTION OF GLASS SAMPLES Y o u n g !s Modulus dynes cmfA xlO11 Bulk Modulus dynes -U - f. 1 cm^ xlO1! Jlock No. Mf g r . 1 B&L BSC-1 2.48 1.51100 63.5 7.64 4.39 2 B&L C-l 2.53 1.52300 58.6 7.57 4.30 3 B&L CF-1 2.69 1.52860 51.6 6.20 3.54 4 B&L LF-1 3.18 1.57250 42.5 5.91 3.50 5 B&L LBC-2 3.14 1.57250 57.4 7.55 4.85 6 B&L DBF-1 3.60 1.61700 38.5 5.98 3.64 7 B&L DF-2 3.64 1.61700 36.6 7.81 5.58 8 B&L DBC-2 3.78 1.61700 54.9 5.64 3.41 9 B&L EDF-1 3.91 1.64900 33.8 7.98 4.40 10 B&L EDF-4 4.72 1.75060 27.7 5.45 3.57 11 E EK-110 4.13 1.69680 56.15 10.24 8.04 12 E EK-330 4.57 1.75510 47.19 10.88 8.58 13 E EK-450 4.63 1.80370 41.80 11.80 9.52 14 H Fused silica 2.20 7.30 3.67 Type Dens ity gra/cm*5 nD V 56 and H q to H6565. The elastic constants are preliminary values of dynamic determinations made in this laboratory by Barnes (34) using ultrasonic waves of the same order of frequency as those used in this work* Table III gives the compositions of the samples as supplied by the manufacturers. The letters in the Bausch and Lomb designations for the glass types have the following significance: borosilicate crown; BSC, C, crown; CF, crown flint; LF, light flint, LBC, light barium crown; DF, dense flint; DBF, dense barium flint; DBG, dense barium crown; E D F , extra dense fli nt • 37 TABLE III COMPOSITION^ OF GLASB SAMPLES IK PERCENT BY WEIGHT Block No. Type Melt No. 1 BBC-1 0-9560 2 C-l 0-7763 3 CF-1 0-9841 4 LF-1 0-9447 5 LBC-2 0-8765 SlOg 70.8 71.7 67.8 54.3 49.1 K 2° 12.1 2.0 11.2 8.0 7.8 7.5 13.7 2.0 3.0 0.5 9.0 32.5 Na20 PbO 2.1 BaO 31.0 SrO CaO 1*3 9.0 b 2°3 8.0 1.1 ZnO 3.4 1*5 4.0 7.5 1.0 6.0 0.5 ZrOg TiOg Alg03 BbgO^ As 2 03 0.3 L a 203 Th02 Ta205 w o3 Al+Si+Zr+Ti (oxides) 0.1 0.2 38 Block No. Type Melt No. iii 6 DBF-1 0-9271 7 DF-2 0-9001 45*0 46.6 to O table 6.3 6.4 NagO 2.0 Si02 PbO 38.2 BaO 7.6 46.3 continued 8 DBC-2 0-8472 9 EDF-1 0-4432 10 EDF-4 0-8030 39.0 42.1 31.5 7.1 1.6 48.8 64.5 0.2 0.1 1.6 42.7 SrO CaO 4.7 b 2°3 ZnO 0.8 0.4 5.4 0.5 ZrOg 1.5 TiOg 5.1 Alg03 0.3 Sbg03 ^■s 2^3 0.1 L a 203 ThOg Ta ^05 W03 A1+Si+Zr+Ti (oxides) 2.0 0.8 0.2 0.3 0.3 39 TABLE III CONTINUED Block No. Type 11 EK-110 12 EK-330 13 EK-450 Si02 100 K 20 N a 20 PbO BaO 14 SrO 6 12 }• CaO B 2°3 40 30 22 20 28 40 20 12 6 18 11 ZnO Zr02 Ti02 a i 2°3 Sb203 AS2O3 ThO, 2 Ta2°5 4 W03 Al+Si+Zr+Ti 14 Fused silica (oxides) 11 40 PRESENTATION OF D a TA Method "B" Only method "B" led to data which agreed with the theory and permitted extrapolation. Therefore values of R were ob­ tained only by this method. Accuracy of d ata. Figure 1 shows the departure of the theoretical points from a straight line. As is mentioned above, an analytical straight line extrapolation for the case in which R equals two and v is not greater than unity leads to an error of 0.55 percent in the value of R. Since all glasses tested exhibited values of R less than 1.83* the "theoretical" error introduced by linear extrapolation is certainly less than 0.5 percent. The linearity of typical experimental data is shown in Figure 8. Since the result is obtained by extrapolation to zero transducer current, absolute accuracy of current determina­ tion is unnecessary. readings. In one case Linearity is sufficient for the meter (block number’eight) successive de­ terminations were made with different ammeters. The re­ sulting values for R differed by 0.31 percent, less than the average percent of difference between runs using the same meter. Although the analytical extrapolation method (40) assumes deviations only in the values of the ordinates, errors 41 in abscissa (current) values must also reflect in the "probable error" of the y-intercept. Although only four or five points were involved in each determination, a formal value of the probable error pR in the value of R due to the deviation of the data points from the straight line was cal­ culated (as in Appendix II) for each determination. In every determination of R for a glass sample p_ was less than 0.3 R percent. This gives some indication of the effect of any non-linearity in the ammeter and of errors in the scale rea d i n g s • Each valu£ of extinction angle used in the calculations was an average of ten settings and readings of the analyzer circle. Each value of the "crossed" position of the analyzer was an average of ten settings and readings. Angle determina­ tions are most difficult for the faint lines corresponding to low sound amplitudes and for materials of large R which require a greater analyzer rotation and consequently permit more background illumination. Since p^ was less than 0.3 percent for all glass determinations, it appears that the contributions of errors in angle measurements to non-linearity must be smaller than that. Two Independent determinations of R were made for each glass sample. They agree, in every case, to within about one percent. Fused silica requires some special consideration. Be­ cause of the large value of R it is especially necessary to 42 use small values of current in this case. (low sound amplitude, small v) Thus the extrapolation was made from only three points, not including a doubling of sound amplitude. Be­ cause of this narrow base for extrapolation the uncertainty in R is greater. for fused silica. Therefore four determinations were made Each differs from the average by less than 0.8 percent. It seems safe to conclude that the average values for R are correct to within two percent. Numerical r e s u l t s . Table IV lists the individual de­ terminations with corresponding temperatures and approximate frequencies, together with the final average values for R, the ratio p/q of the Neumann strain-optical constants. Method "C" Accuracy of d a t a . The remarks about the measurement of transducer current which were made in regard to method '^B11 apply also in this case.' Some idea of the dependability of the photographic method can be gained from an examination of the spread of experi­ mentally determined values. this experimental spread. Figures 9, 10, 11, and 12 show This check is especially signifi­ cant for the case of block number one (borosilicate crown) for which the experimental spread at each current includes four determinations. The spreads for block number six in­ clude two values while those for block number three include two or three v a l u e s . 43 TABLE IV NUMERICAL RESULTS Freq. me/sec Room Temp. °C Points for Extrapolat ion R p/q PR 1 BSC -1 9.8 24.0 5 1.827 .0025 1 BSC-1 9.8 25.0 4 1.816 .0011 2 C-l 10.2 25.0 4 1.823 .0004 2 C-l 10.0 25.0 4 1.819 .0004 3 CP -1 9.4 to o • Block No. Type 5 1.672 .0014 3 CP -1 10.0 26.0 5 1.689 .0010 4 LF-1 9.9 26.5 4 1.440 .0038 4 LF-1 10.0 26.0 4 1.452 .0004 5 LBC-2 10.1 25.5 4 1.625 .0003 1.618 .0009 Aver. R 1.82 CJ1 1.82 1.68 1.45 1.62 5 LBC-2 9.8 25.0 4 6 DBF-1 10.5 26.0 5 1.366 .0009 .0004 1.36 6 DBF-1 10.2 24.5 4 1.361 7 DF -2 10.2 28.0 4 1.456 .0010 7 DF -2 9.9 27.0 4 1.459 .0003 8 DBG-2 9.8 26.0 5 1.281 .0010 8 DBC-2 10.2 22.5 4 1.285 .0006 9 EDF-1 H . o H 25.0 4 1.459 .0010 9.4 25.0 5 1.464 .0007 1.46 9 EDF-1 1.28 1.46 44 TABLE IV CONTINUED Block No. Type Freq* mc/sec Room Temp. °C Points for Extrapolation Aver. R p/q Pr 10 EDF-4 9.6 25.0 5 1.109 .0045 10 EDF-4 10.5 26.0 4 1.113 .0013 11 EK-110 9.9 24.0 4 1.530 .0017 11 EK-110 10.2 26.5 4 1.536 .0017 12 EK-450 10.2 27.5 4 1.548 .0016 12 EK-450 o • o i —1 27.0 4 1.554 .0016 13 EK-330 10.1 30.0 4 1.595 .0007 13 EK-330 9.8 27.5 4 1.596 .0007 14 Fused silica 10.1 27.0 3 2.343 Fused s ilica 10.4 27.0 3 2.349 k 1.11 1.53 1.55 1.60 14 2.34 14 14 Fused silica 10.1 26.5 3 2.318 Fused silica 10.0 25.5 3 2.334 45 Multiple diffraction cannot have caused trouble* for only the first order lines appeared. Transverse waves cannot have caused trouble since the frequencies used were non-resonant for them* and* since their diffraction pattern has a different spacing than that due to the longitudinal waves* their presence would have been obvious. Due to the action of the Wollaston prism* the beams of light are not quite normal to the sound beam but have an obliquity of twenty-one minutes, Parthasarathy (45) (46) has investigated the asymmetrical intensity distribution in the diffraction pattern due to oblique incidence of light on progressive waves in liquids. He reports an effect only at wave lengths shorter than those involved in this work. In addition* since the two beams from the Wollaston prism are symmetrical In incidence and since the sound field con­ sists of standing waves* any effect should disappear when the two first order intensities in each pattern are averaged in the calculation. Further* an examination of the data in­ dicates no significant intensity asymmetry. There is thus no apparent reason to doubt the experi­ mental values. Numerical r e s u l t s . Since the experimental points do not follow the linear pattern indicated by the theory they do not lead to values of R. The values of the intensity ratios for various currents are the only numerical results of method 11C 11. These values are shown on the curves of 46 Figures 9, 10 , 11 , and 12. Values of R from Other Investigations It is well known that glasses of similar composition or even ’’identical1’ samples may differ significantly in their properties. (35). See, for example, Coker and Filon (9 ) and Mueller In addition, effects of aging on photoelastic properties and temperature dependence are reported by Harris Filon (44). (43 ) and So it is with grave reservations as to its signi­ ficance that the data in Table V is given. The glass types are merely similar, identified on the basis of incomplete data on density, composition. index of refraction, elastic constants, or The parenthesis In the Table indicate that the similarity of types is quite doubtful. to Pockels (5), to Twyman and Perry (7), and to Schaefer and Nassenstein (8 ) are by static methods. (26) The measurements due Those due to Vedam (27) are by Mueller!s method "B” with sound intensities inferred from input voltage to the power amplifier. Those due to Schaefer and Dransfeld (28) are by Mueller!s method ”B ” with sound amplitudes inferred from intensities in the diffraction pattern and extrapolation from two points giving an announced accuracy of five percent. Bergmann and Fues (29) used the intensity ratio method without extrapolation, being content with sound amplitudes low enough to avoid second order lines. ficance. Their results are, therefore, of doubtful signi­ Bergmann has since remarked on the necessity of extrapolation (47). It is to be noted that Schaefer and 47 TABLE V VALUES OP p/q GIVEN BY OTHER INVESTIGATORS (Glass types compared in this table are merely sirrilar, with parenthesis indicating especially doubtful similarity) This Investigation Block No. Type p/ q 1 BSC -1 1.82 3 CP-1 1.68 4 LF-1 1.45 5 LBC -2 1.62 6 DBF-1- 1.36 7 DF-2 1.46 9 EDF-1 1.46 10 EDF-4 1.11 14 Fused Silica 2.34 Other Investigations Type Reference p/q BK-1 BK -1 BK-1 2 BK-1 2 KF-7 KF-7 (LF-1 ) (LF-1) LF-4 LF-4 0,8154 (x) (10 ) BaK-4 BaK-4 (9) BaSF -1 BaSF -1 (12 ) (0.1571) (14) (SF-2 ) (SF-2 ) (SF-9) (SF-9) (SF-4) (3F-4) 0.500 (16) (17) Fused Silica (8 ) (28) (8 ) (28) (8 ) (28) (8 ) (28) (8 ) (28) (5) (7) (27) (8 ) (28) (27) (e> (28) (27) (5) (27) (8 ) (28) (8 ) (28) (8 ) (28) (5) (27) (27) 1.76 1.73 1.82 1.89 1.64 1.64 (1.45) (1.50) 1.32 1.39 1.44 (1.51) (1.70) 1.73 1.75 (1.84) 1.29 1.29 (1.50) (1.27) (1.41) (1.18) (1.26) (1 .20 ) (1 .22 ) (1.07) (1.07) 1.11 1.05 (1.18) (26) 2.85 48 Nassenstein used the same set of glasses as Schaefer and Dransfeld. 49 SUMMARY AND CONCLUSIONS Mueller has described, In theory, two methods for the determination of the ratio p/q of the strain-optical constants of glass. Both methods Involve the diffraction of light by means of ultrasonic waves. Method "B" involves measurements of the polarization of the diffraction orders. involves measurements Method HC" of ratios of intensities in the dif­ fraction orders. The appropriate experimental arrangement was provided for each method. Data was taken, by both methods, on three glass samples and on a fused silica sample. The data given by method "B” was in excellent agreement with the theory. This method was then applied to a set of thirteen American optical glasses, glasses, and to fused silica. including three rare earth The ratio of the strain-optical constants was calculated for each sample for dynamic harmonic strains having a frequency in the neighborhood of ten mega­ cycles per second. The data given by method "Cn did not agree with the theory and did not lead to values for the ratio of the strain-optical constants. The data followed a definite pattern, however, and the pattern was consistent among the four sarples tested. It may be concluded that method "B" Is applicable as de­ scribed and leads to dynamic values of the ratio of the strain- 50 optical constants. It may also be concluded that method "C" does not apply as described. However, on the basis of the pattern and consistency of the data obtained by method "C 11 it is hoped that it may be shown to have significance. 51 APPENDIXES 52 APPENDIX I Theoretical Intensity Ratios in the Diffraction Orders Arrangement of MuellerT3 Method "B11. The optical system for M u e l l e r ^ method nB ,! (23) is shown in Figure 6 , For the case of standing longitudinal waves in glass, incident light polarized at forty-five degrees to the slit, crossed analyzer, and unit incident intensity, the intensity I 1 7 0 m,r in the r subcomponent of the m diffraction order Is given by the Mueller theory as I where the quantities are the same as those in equation 5. The total intensity I in the order of index m Is J m given by (1-2 ) 1 Numerical substitutions for R and v give the following ratios of the total intensity in the third order to the total intensity In the zero or central order. 53 TABLE VI TOTAL INTENSITY RATIOS: THIRD ORDER TO ZERO ORDER, METHOD "B" v R 1.5 R 2.0 R 2.5 0.8 .0136 .0206 .0292 1.0 .0221 .0327 .0464 Numerical substitutions for R and v give the following ratios of the intensity in the first sub-component to the intensity in the zero sub-component for the case of the first diffraction order. TABLE VII SUB-COMPONENT INTENSITY RATIOS: FIRST TO ZERO SUB-COMPONENTS, FIRST ORDER, M e T s OD "B" v R 1.5 R 2.0 R 2.5 0.8 .0223 .0591 .156 1.0 .0460 .155 .610 Arrangement of MuellerTs Method uC n . The optical system for M u e ller1s method UC ” (23) is shown in Figure 7 . For the case of standing longitudinal waves in glass, incident light polarized parallel to the slit, and unit incident intensity, the intensity I in the r sub-component of the m difm, r fraction order is given by the Mueller theory as 54 I ’v < ’ [7^)j^mx if (i-3 where the quantities are the same as those in equation 5 . The total intensity in the m order is given by equation 1-2. Numerical substitutions for R and v give the following ratios of the total intensity in the second order to the total intensity in the zero or central order. TABLE VIII TOTAL INTENSITY RATIOS: SECOND ORDER TO ZERO ORDER, METHOD "C,! V R 1.5 R 2.0 R 2.5 0.4 .000788 .00256 .00650 0.6 .00420 .0141 .0368 0.8 .0155 .0487 .127 1.0 .0368 .127 .299 Numerical substitutions for R and v give the following ratios of the intensity in the first to that in the zero sub-component of the first diffraction order. 55 TABLE IX BUB-COMPONENT INTENSITY RATIOS: FIRST TO ZERO SUB-COMPONENTS, FIRST ORDER, METHOD 11C" 0 •4 .000122 .000429 .00106 0.6 .000697 .00229 .00602 .00229 .00805 .0226 o • H o • 03 R 1.5 CO • o R 2.5 V .00602 .0226 .0702 56 APPENDIX II Sample Data and Calculation for Method "B" Glass; Block number 1 , type BSC -1 Frequency: 9.8 megacycles Room temperature: 24° (oscillator dial 20.36) centigrade Thermocouple thermometer scale reading maintained less than 2.5 (temperature difference: less than one quarter degree centigrade) Maximum permissable transducer current: no third order at 1.5 amperes Analyzer angle readings in degrees: (for extinction or a minimum) No sound ("crossed") .50 amp .73- amp .92 amp 1.10 amp 1.50 amp 44.75 44.80 44.85 44 .85 44.80 44.75 44.80 44.80 44.85 44.80 60.8 61.6 61.3 60.5 61.3 61.2 61.0 60.8 61.0 60.0 60.2 60.8 60.0 61.0 60.3 (59.4) 60.9 60.9 61.0 60.6 60.2 60.6 60.5 60.3 60.3 59.6 60.3 60.1 59.5 60.5 60.3 59.1 59.8 60.2 60.7 60.1 59.5 59.5 59.7 60.1 60.1 59.0 60.0 59.5 59.1 59.0 59.4 59.2 59.2 59.4 60.63 60.19 59.90 59.39 Analyzer angle averages: 44.80 60.90 57 Values of © i (9 = minimum setting minus plus forty-five degrees. Tan 0 "crossed" setting See equation 7 ) .50 amp .71 amp .92 amp 61.10 60.83 60.39 60.10 59.59 1.811 1,791 1.759 1.739 1.704 : 1.10 amp 1.50 amp For linear extrapolation assume a curve of form y - a + b x , 2 where x = I and y = 10(tan9 -1 .6 ), which gives best fit in sense of least squares. The y-intercept y Q is given by the value of the coefficient a which is, in turn given (40) by y nZx--(Z*r Evaluating a: X y .250 .504 .846 .21 .69 4.50 2.11 1.91 1.59 1.39 1.04 8.04 xy X2 .5275 .9625 1.345 1.6825 1.755 6.2725 .0625 .2540 .7140 1.464 2 •856 5.3505 Substituting In equation II-l, yQ — a — 2.2729 Evalutating R: R = tan 0O R = 1.827 = 1.6 + y 0/lO Evaluating ppj; If the data points are assumed to have a random dis­ tribution about a theoretical straight line, the probable error ppj in the y-intercept is given formally by (40) 56 (II-2) where (II-3) In this work the data points do not follow a relation which is, theoretically, perfectly linear. (See Figure 1 ). Nevertheless, this calculation is carried through formally to give some indication of the reliability of the data. For this sample, b = -0.7394 pa = 0.0254 PR ~ 0.0025 59 APPENDIX III Sample Data and Calculation for Method "C" Glass : Block number 3, type CP -1 Frequency: 9.4 megacycles Room temperature: (oscillator dial 20.06) 23° centigrade Thermocouple thermometer scale reading maintained less than 2 > (temperature difference: less than one quarter degree centigrade) Maximum permissable transducer current: no second order at 300 milliamperes Emulsion sensitivity exposure: rotating step-wedge with step to step exposure ratio of 1.5 Diffraction pattern exposure: Exposure number 1 2 3 4 5 6 7 8 9 10 11 12 13 Exposure time ____ (s e c )____ 1/2 1/2 1 1/2 1/2 1/2 1/2 1/2 1/5 1/5 1/5 1/2 1/5 Transducer current (ma_)________ no sound 100 100 150 150 200 200 250 250 300 300 100 250 60 Photometer readings on successive sector steps: 1) 2) 3) 4) 5) 6) 7) 8) 9) 10 ) 11 ) 12 ) 13) 2.0 4.5 10.3 19.9 35.3 50.2 64.5 75.5 80.7 86.7 90.9 93.8 95.6 1.5 4.7 10.3 20.3 35.5 48.8 63.0 75.4 80.3 86.5 91.0 93.8 95.8 1.5 4.8 10.5 19.5 36.0 50.0 62.8 75.6 81.2 86.6 90.8 93.4 95.4 Average: 1.67 4.67 10.37 19.90 35.60 50.00 63.43 75.50 80.73 86.60 90.90 93.67 95.60 The average photometer readings are plotted against the logarithm (to the base 1.5) of the rotating sector ex­ posures. A standard s-shaped emulsion sensitivity curve results * Pairs of photometer readings on the two lines of exposure 1 (no s o u n d ) : 63.4 64.7 65.0 66.0 65.8 67.0 64.6 65.6 Average difference: 66.9 1.22 Difference in log exposure curve): 65.8 (read from sensitivity 0.084 This diffrence, due to the inequality of the two beams from the Wollaston prism, will be applied below as a correction. Photometer readings L on diffraction lines and calculations: and L ? ; photometer readings on the diffraction lines of one beam. (Light polarized normal to slit). L 3 and L a ; photometer readings on the lines of the other beam. diffraction 61 A 12 average of L^ and L^. A34 average of Lg and L 4 . Bkg photometer reading on background near lines. Bkg Cor Correction to A due to presence of back­ ground. Bkg Cor Bkg (100 - A)/ 100. Ac Corrected average photometer readings on lines. G_ Logarithm of average exposure of dif­ fraction lines of one beam. G is de­ termined from A c by means of sensitivity curve. G2 Logarithm of average exposure of diffrac­ tion lines of the other beam. D^Gg-Gi Logarithm of ratio of exposures of dif­ fraction lines of the two beams. Since the exposures are made simultaneously, D is the logarithm of the ratio of the in­ tensities of the diffraction lines of the two b e a m s • Da Average value of three determinations of D. Dac = Da -*.08 Da corrected for beam inequality. B = X.5^D a c ^ Intensity ratio of the diffraction lines. 62 Exp L1 L2 A12 2 2 2 4 4 4 5 5 5 6 6 6 7 7 7 8 8 8 9 9 9 10 10 10 11 11 11 12 12 12 13 13 13 15 *4 13.9 13.1 28.8 25.3 21.3 28.1 25.5 22.1 47.2 42.8 36.0 47.0 42.0 34.9 61.2 56.4 51.0 6.1 4.7 5.8 13.7 11.6 14.5 11.6 9.9 9.7 13.4 12.9 12.3 6.1 4.7 6.3 15.9 14.0 12.5 28.9 25.2 22.0 29.2 25.2 22.2 49.0 43.4 37.5 48.0 43.3 35.8 61.6 56.8 51.7 6.4 4.3 6.0 14.6 12.2 15.2 12.5 11.2 9.4 13.1 13.0 12.3 6.2 5.4 7.6 15.65 13.95 12.80 28.85 25.25 21.65 28.65 25.35 22.15 48.10 43.10 36.74 47.50 42.65 35.35 61.40 56.60 51.35 6.25 4.50 5.90 14.15 11.90 14.85 12.05 10.55 9.55 13.25 12.95 12.30 6.15 5.05 6.95 Bkg Bkg Cor 2 2 2 1 2 3 2 2 3 2 2 2 1 1 2 3 2 2 0 0 0 0 0 0 0 0 0 1 2 2 0 0 0 1.7 1.7 1.7 0.7 1.5 2.3 1.4 1.5 2.3 1.0 1.1 1.3 0.5 0.6 1.3 1.3 0.9 1.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.9 1.7 1.8 0.0 0.0 0.0 Ac G1 L3 L4 13.95 12.25 11.10 28.15 23.75 19.35 27.25 23.85 19.85 47.10 42.00 35.45 47.00 42.05 34.05 60.10 55.70 50.35 6.25 4.50 5.90 14.15 11.90 14.85 12.05 10.55 9.55 12.35 11.25 10.50 6.15 5.05 6.95 3.43 3.24 3.11 4.53 4.23 4.00 4.47 4.25 3.93 5.84 5.49 5.04 5.83 5.50 4.94 6.75 6.44 6.07 2.34 1.95 2.28 3.47 3.20 3.52 3.21 3.02 2.88 3.25 3.13 3.02 2.31 2.08 2.45 41.2 36.4 32.2 67.6 60.2 54.0 65.1 59.4 54.4 81.6 77.0 72.2 81.0 76.4 70.7 87.0 84.4 81.4 39.7 35.0 38.0 59.2 56.3 59.7 58.0 52.3 50.0 37.3 35.7 33.1 41.5 35 .6 43.8 40.2 35.4 31.2 66.4 59.4 54.3 65.0 58.8 53.5 81.9 77,4 73.0 81.4 77.4 71.2 87.0 84.4 81.4 39.8 34.7 39.0 59.9 56.0 60.3 57.6 52.9 50.6 36.8 35.6 31.3 42.0 36.7 43.3 63 2 2 2 4 4 4 5 5 5 6 6 6 7 7 7 8 8 8 9 9 9 10 10 10 11 11 11 12 12 12 13 13 13 A 34 40 •70 35 •90 31 •70 67 .00 59.80 54.15 65.05 59.10 53.95 81.75 77.20 72.60 81.20 76.90 70.95 87.00 84.40 81.40 39.75 34.85 38.50 59.55 56.15 60.00 57.80 52.60 50.30 37.05 35.65 32.20 41.75 36.15 43.55 6kg Bkg Cor 1 2 2 1 2 2 1 1 1 1 1 1 1 1 2 2 2 2 0 0 0 0 0 0 0 0 0 1 1 2 0 0 0 The values of 0.6 1.3 1.4 0.6 0.8 0.9 0.3 0.4 0.5 0.2 0.2 0.3 0.2 0.2 0.6 0.3 0.3 0.4 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.6 0.6 1.4 0.0 0.0 0.0 Ac G2 40.10 5.36 34.60 4.98 30.30 4.68 66.40 7.18 6.67 59.00 6.27 53.25 7.06 64.75 58.70 6.65 53.45 6.29 81.55 9.00 77.00 8.21 72.30 7.70 81.00 8.92 76.70 8.24 7.51 70.35 86.70 10.00 9.47 84.10 8.91 81.00 5.34 39.75 4.99 34.85 5.25 38.50 6.71 59.55 56.15 6.48 6.74 60.00 57.80 6.59 6.22 52.60 50.30 6.06 5.10 36.45 5.00 35.05 30.80 4.71 5.48 41.75 5.08 36 •15 5.60 43.55 D 1.93 1.74 1.57 2.65 2.44 2.27 2.59 2.41 2.36 3.16 2.72 2.66 3.09 2.74 2.57 3.25 3.03 2.84 3.00 3.04 2.97 3.24 3.28 3.22 3.38 3.20 3.18 1.85 1.87 1.69 3.17 3.00 3.15 Gac -5b ~ 1.75 1.67 1.40 2.45 2.37 1.62 2.45 2.37 1.62 2.85 2.77 1.75 O CO • c\i Exp 2.72 1.74 3.04 2.96 1.82 3.00 2.92 1.81 3.25 3.17 1.90 3.28 3.20 1.91 1.80 1.72 1.42 3.11 3.03 1.85 Da from the last column are plotted aga: the square of trie transducer current in Eigure 12 . 64 BIBLIOGRAPHY 1. 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