in)“ pull}! .1.) 4A. ammo. Hf z. .w 2 . has. .i . . :1 runs :22...“ :5hnr: I; 7.. 1...)».wli ii ”4:532... .... I b 1.1.5.. 1 132.3... v95\ ‘9‘, I. . .’. Kt tufu ris. (‘15.... 433;... s . in: r! ....:!r: ......,.;.|,‘:..!. 3.! 74?. . , . . - Air. :3:. :E E. ......5.m..-......s. ekgkfinwgwuai a .91.... 11 y e. :32: 21.5.9.3:2... a. J L: . . . . .. 5w uenmes lllllllll\lllllllll lllllll LIBRARY Michigan State University This is to certify that the thesis entitled EXPERIMENTAL DESIGN AND TECHNIQUES FOR MEASUREMENT OF CVD DIAMOND FILM THERMAL CONDUCTIVITY USING INFRARED THERMOGRAPHY presented by SCOTT ALLEN HERR has been accepted towards fulfillment of the requirements for MRS—degree in MECHANICAL ENGINEERING Q/wo V!» é Major professor D... @615 12/1973 0-7639 MS U is an Affirmative Action/Equal Opportunity Institution PLACE. IN RETURN BOX to remove this checkout from your record. TO AVOID FINES return on or before date due. F DATE DUE DATE DUE DATE DUE . JIL MSU Io An Affirmative Action/Equal Opportunity Institution ammo-n1 EXPERIMENTAL DESIGN AND TECHNIQUES FOR MEASUREMENT OF CVD DIAMOND FILM THERMAL CONDUCTIVITY USING INFRARED THERMOGRAPHY By Scott Allen Herr A Thesis Submitted to Michigan State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Department of Mechanical Engineering 1993 ABSTRACT EXPERIMENTAL DESIGN AND TECHNIQUES FOR MEASUREMENT OF CVD DIAMOND FILM THERMAL CONDUCTIVITY USING INFRARED THERMOGRAPHY By Scott Allen Herr Experimental design and techniques were developed for the measurement of the thermal conductivity of doped CVD diamond films. Three solutions were derived, one each for one dimensional, two dimensional and radial heat flow. A sensitivity analysis revealed that the radial heat flow model was most sensitive to the measurement of the thermal conductivity. Sample parameters such as characteristic length, thickness of doped diamond and resistivity were chosen from the model to reduce convective effects, obtain the desired temperature rise and minimize the uncertainty in the estimation of the thermal conductivity. Two diamond film samples were made according to the specifications determined by the analytical analysis. Both samples consisted of doped and nondoped layers on the topside and were chemically etched from the backside, leaving a free standing diamond diaphragm 3 mm in diameter. The thickness of the doped and nondoped films were approximately 5.6 pm and 1.0 pm, respectively, for'both samples. A new experimental setup was designed and constructed. An infrared imaging temperature acquisition system was implemented to improve on the spatial, temporal and mechanical limitations of contact sensors such as thermocouples and resistance thermometers. Preliminary results for the thermal conductivity of a semiconducting diamond film were obtained from five experiments using the method of least squares to minimize the error between the measured temperatures recorded by the infrared temperature acquisition system and the calculated temperatures determined by the optimal radial heat flow model. The thermal conductivity along with the experimental uncertainty was determined to be 249 i 13 W/m K. These are the fast reported values for a semiconducting diamond film. The mean value falls within the range reported for undoped diamond films (190-1350 W/m K). The experimental uncertainty for this method (approximately 5%) is also the first to be determined utilizing uncertainties in all measured experimental parameters. to my parents Jack and Jan iv Acknowledgments I would like to thank my co-advisors, Professor J. V. Beck and Professor J. J. McGrath for their guidance in the present work. I am greatful for the opportunity to learn from their example as both researchers and engineers. I would like to personally thank Professor J. V. Beck for the opportunities he has extended to me as his research assistant in the Thermal Properties Measurement Laboratory over the past two years. This opportunity has presented several rewarding experiences; one of which was working with Dr. Bertrand Gamier from Laboratoire de Thermocinetique-ISITEM, Nantes, France. Dr. Gamier’s creative thinking, meticulous explanations and exceptional experimental talents have been an important influence in my own laboratory techniques. I would also like to thank Professor C. W. Somerton for his review of the present work. I believe Professor Somerton to be an exceptional teacher and consider the time spent in his classroom to be an accelerated learning experience. Many thanks go out to Professor M. Aslam and S. Sahli for their expertise in diamond deposition and microstructural fabrication; their help was crucial in designing the optimal diamond semiconductor for our experiments. I wish to also thank C. Mindock for her involvement in the chemical etching process. A special thanks goes out to my undergraduate advisor and friend Professor H. M. Dixon who’s inspiration throughout the years has elevated my understanding of physics and engineering. Professor Dixon is a most remarkable scientist and educator and I am greatful for his continual interest and involvement in my education. Last but not least, I want to thank my family for the support and encouragement they have given me throughout my life. Table of Contents List of Tables List of Figures Nomenclature Chapter 1 Introduction 1.1 Objectives 2 Background and Literature Review 2.1 CVD Diamond Films 2.2 General Experimental Methods Determining Thermal Properties 2.3 Special Experimental Methods for CVD Diamond Films 3 Problem Description 3.1 Mathematical Modeling 3.1.1 One Dimensional Heat Conduction Model 3.1.2 Two Dimensional Heat Conduction Model 3.1.3 Radial Heat Conduction Model vii xi XV 21 21 25 28 32 Design of the Diamond Film Sample 4.1 Determining the Best Experimental Model 4.2 Special Requirements for the Desired Temperature Rise 4.2.1 Volumetric Heat Generation in Diamond 4.2.2 D0ping Requirements for the Diamond Film 4.3 Limiting Natural Convection 4.4 Analytical Results 4.5 Topside Sample Fabrication 4.6 Bottomside Sample Fabrication Experimental Techniques 5.1 The Data Acquisition System 5.1.1 The Inframetrics Model 6OOL IR Imaging Radiometer 5.1.2 Thermal Image Processing System 5.1.3 The Omega 880 Digital Multimeter 5.2 System Calibration Check 5.3 Experimental Setup 5.3.1 Preparation of the Sample Setup Procedures and Results for One Dimensional Radial Experiments 6.1 Determining the Emissivity 6.2 Measuring the Electrical Power 6.3 Radiometer Settings viii 35 36 50 50 52 56 61 63 69 73 73 74 77 78 79 84 84 86 86 89 91 6.4 Surface Temperature Measurements 6.4.1 Capturing Images Using the Thermal Image Processor 6.4.2 Temperature Acquisition 6.5 Measurement of the Thermal Conductivity 6.5.1 The Simplified Experimental Model 6.5.2 Estimation of the Thermal Conductivity 6.6 Experimental Uncertainty 7 Summary and Conclusions Suggestions for future work List of References Appendices Appendix A Calibration of the Inframetrics 600L Radiometer for Rapid Transient Thermal Events Appendix B Temperature Distribution for Experiments 1-5 Appendix C Program NLIN Appendix D NLIN Output File for Experiment #5 93 93 98 98 99 100 111 115 118 120 123 123 132 137 143 Table 2.1: Table 2.2: Table 4.1: Table 6.1: Table 6.2: Table 6.3: List of Tables Thermal conductivity of diamond film evaluated at different thicknesses at room temperature (Morelli et al., 1988). Thermal conductivity parallel to the film surface as a function of film thickness (Graebner et al., 1992). Optimum sample design parameters assuming a thermal conductivity of 1000 W/m K. Temperature vs. resistance for sample A. The thermal conductivity estimated by NLIN for each of the five experiments at different power levels. Experimental parameters. their uncertainties and the corresponding contributions to the uncertainty of the thermal conductivity. 11 14 62 90 110 112 Figure 2.1: Figure 2.2: Figure 2.3: Figure 2.4: Figure 2.5: Figure 2.6: Figure 2.7: Figure 3.1: Figure 3.2: Figure 3.3: Figure 3.4: Figure 3.5: Figure 3.6: Figure 4.1: Figure 4.2: Figure 4.3: List of Figures The diamond cubic unit cell. Schematic of a deposited diamond film sample. Microscopic view of CVD diamond film prepared by the hot filament method. Microscopic view of CVD diamond film prepared by the microwave method. Thermal conductivity parallel and perpendicular to the film surface. A block diagram of the type of experimental setup used by Albin, Winfree and Crews ( 1990) to determine thermal diffusivity. Schematic of the experimental setup for the photothennal laser beam deflection technique (Machlab et al., 1991). Ratio of the diamond film thickness to the silicon substrate thickness in the z direction. Schematic of the one dimensional model. Schematic of the two dimensional diamond film sample etched from the backside. Schematic of the two dimensional model. One of the symmetric quadrants for the two dimensional model. Schematic of the radial heat conduction model. The non-dimensional sensitivity coefficient as a function of characteristic length for different film thicknesses, 1D case. The non-dimensional sensitivity coefficient as a function of characteristic length for different temperature rises, 1D case. The non-dimensional sensitivity coefficient as a function of characteristic length for different film thicknesses, 2D case. 10 18 19 24 26 29 30 31 33 39 40 42 Figure 4.4: Figure 4.5: Figure 4.6: Figure 4.7: Figure 4.8: Figure 4.9: Figure 4.10: Figure 4.11: Figure 4.12: Figure 4.13: Figure 4.14: Figure 4.15: Figure 4.16: Figure 4.17: Figure 4.18: Figure 4.19: Figure 4.20: Figure 4.21: Figure 4.22: Comparison of the non-dimensional sensitivity coefficient between the one dimensional and two dimensional cases at the same characteristic length The non-dimensional sensitivity coefficient as a function of characteristic length for different temperature rises, 2D case. The non-dimensional sensitivity coefficient as a function of characteristic length for sample widths of 1.0, 0.50 and 0.25 cm, 2D case. The non-dimensional sensitivity coefficient as a function of diameter for different film thicknesses, radial case. The non-dimensional sensitivity coefficient as a function of diameter for different temperature rises, radial case. Comparison of the non-dimensional sensitivity coefficient as a function of characteristic length between the 1D, 2D and radial cases. Schematic of a sample with 3 doped diamond film, a layer of SiO2 and a silicon substrate. Schematic of a samme with doped and undoped diamond films, a layer of SiO2 and a silicon substrate. Schematic of the electrical circuit. Temperature rise as a function of applied voltage for different film thicknesses. The non-dimensional sensitivity coefficient as a function of (tnf * characteristic length) for the 1D, 2D and radial cases. Ratio of natural convection to the total heat generated in the doped film as a function of diameter for different film thicknesses. The non-dimensional sensitivity coefficient as a function of diameter for different doped and undoped film thicknesses. Photograph of the hot filament CVD diamond deposition chamber. Thickness of the undoped film on sample A measured in A by the SEM. Thickness of the undoped film on sample B measured in A by the SEM. Thickness of the doped film on sample A measured in A by the SEM. Thickness of the doped film on sample B measured in A by the SEM. The front side of sample A. xii 43 45 47 48 49 51 51 53 55 57 59 65 65 66 68 69 70 Figure 4.23: Figure 5.1: Figure 5.2: Figure 5.3: Figure 5.4: Figure 5.5: Figure 5.6: Figure 5.7: Figure 5.8: Figure 6.1: Figure 6.2: Figure 6.3: Figure 6.4: Figure 6.5: Figure 6.6: Figure 6.7: Figure 6.8: Figure 6.9: Figure 6.10: Figure 6.11: Figure 6.12: Figure 6.13: Figure 6.14: The diamond mask pattemed on the back side of sample A. Schematic of the data acquisition system. The 600L Infiared Radiometer. The 6" close-up lens and the 3x telescope lens used to increase the spatial resolution of the radiometer. The Omega 880 Digital Multimeter. Corrected temperature of the thermocouple as a function of measured temperature of the radiometer. Heater surface temperature as a function of surface location. Schematic view of the sample afier experimental preparation. Photograph of the sample after experimental preparation. Setup used to determine the emissivity of the diamond film for sample A. The relationship between the temperature measured by the radiometer and the temperature measured by the thermocouple at an emissivity setting of 0.63. Sample setup viewed from the front side. Sample setup viewed from the back side. Image 1 from experiment #1 at 0.40 watts. Image 2 from experiment #2 at 0.62 watts. Image 3 from experiment #3 at 0.88 watts. Image 4 from experiment #4 at 0.40 watts. Image 5 from experiment #5 at 0.88 watts. Measured and calculated temperature distribution for experiments 1, 2 and 3. Measured and calculated temperature distribution for experiments 4 and 5. Residual distribution for experiment #1, 107 pts. Residual distribution for experiment #2, 107 pts. Residual distribution for experiment #3, 107 pts. xiii 71 74 75 77 79 80 83 85 85 87 88 94 95 97 97 97 97 97 102 102 103 104 104 Figure 6.15: Figure 6.16: Figure 6.17: Figure 6.18: Figure 6.19: Figure 6.20: Figure 6.21: Figure A.1: Figure A.2: Figure A.3: Figure A.4: Residual distribution for experiment #4, 121 pts. Residual distribution for experiment #5, 121 pts. Sequential estimation of the thennal conductivity for experiment #1, 107 pts. Sequential estimation of the thermal conductivity for experiment #2, 107 pts. Sequential estimation of the thermal conductivity for experiment #3, 107 pts. Sequential estimation of the thermal conductivity for experiment #4, 121 pts. Sequential estimation of the thermal conductivity for experiment #5, 121 pts. Setup used to calibrate the infrared radiometer to record transient events. Vertical refresh signals resembling legitimate line scans. Thermocouple termperature as a frmction of radiometer voltage for the six different calibration runs. Radiometer voltage recorded in fast line scan mode during calibration. xiv 105 105 107 107 108 108 109 124 129 130 131 ”@300 Nomenclature Thermal Conductivity Emissivity Thermal Diffusivity Specific Heat Density Temperature Thickness of Doped Film Thickness of Undoped Film Convection Coefficient Temperature Difference Relative Temperature Rise Area Volume Least Squares Function Sensitivity Coefficient Matrix Voltage Electrical Resistance Thermal Resistance Time Volumetric Heat Generation Convective Fin Term Eigenvalue Cylindrical Coordinate XV DU‘IQ'D“[‘- k u but were unable to positively conclude this due to experimental enors associated with each method. Graebner, Jin, Kammlott, Herb and Gardinier (1992) used a similar setup to determine the thermal conductivity parallel to the film surface (k u) using two thin film heaters which were evaporated directly onto the sample, one near each end. The temperature distribution was measured again by a row of four very fine thermocouples. Measurements were performed on several samples prepared by the microwave CVD method. The samples having different thicknesses were placed in a vacuum where the effects of convection and radiation were neglected. From their study Graebner, Jin and Kammlott also concluded that the thermal conductivity was a function of the film thickness. Graebner, Mucha, Seibles and Kammlott (1992) determined the thermal conductivity using a technique that involved etching a window of free standing diamond 2x4 mmz, similar to the Morelli, Beetz and Perry (1988) procedure. The remaining silicon served as a rugged platform to support the film as well as a heat sink and a referenced temperature boundary. The flow of heat from a heater in the center of the window was monitored with thermocouples. The thin film heater and the chromel and constantan thermocouples were deposited on the surface of the diamond by standard l3 evaporation techniques. The steady state temperature distribution, detected by the thermocouples, was then compared with a numerical simulation to extract the thermal conductivity parallel to the surface (k u)- Their efforts yielded values for k n in the range of 200-600 W/m°C. The choice of window dimensions was made to reduce the effects of radiation. To predict the thermal influence from radiation they developed the ratio, km, ~ Zoeszg 2 1 kcond K t where km is the conductance of heat along the film of thickness t, km is the effective conductance due to radiation between the film and its surroundings, 0' is the Stefan- Boltzman constant and K is the thermal conductivity. By evaluating this ratio under unfavorable conditions 8=1, To=300 K, t = 2pm and x = 300 W/m K and varying the width (w), they were able to neglect the effects of radiation when the ratio became significantly small. The effects of convection were not considered in their study. The results of their study are presented in the Table 2.2. 14 Thickness (pm) 2.8 3.8 7.0 l 7.3 7.5 7.8 7.8 10.6 11.6 13.1 Table 2.2. Thermal conductivity parallel to the film surface (k [I) as a function of film thickness presented by Graebner, Mucha, Seibles and Kammlott (1992) Baba et al. (1991) concluded that the thermal conductivity for diamond films was also dependent on the amount of hydrogen impurity deposited from the methane (CPL) gas mixture. In this study an experimental method termed the "ac calorimetric" method was employed. Here, one end of the diamond samples was periodically heated by a halogen lamp. The temperature amplitude (TAG) at a distance (x) away from the heat source was monitored by a thermocouple which was attached to the sample’s surface. A relation between TAC and distance (x) is given by 15 = _q__ - 32‘ lanacl ln<4rtfdcp) ( a )x 2.2 where q is heat quantity, f is the heating frequency, and C,, d and or are the specific heat, thickness and the thermal diffusivity of the film. The thermal conductivity was extracted from the diffusivity of two samples and evaluated from the slope of the above equation by varying x. The thermal conductivity of the film prepared with 1% CH4 concentration reached 1200 W/m K but the thermal conductivity of the film prepared with 5% CH4 concentration decreased to less than 200 W/m K. Both samples were hot-filament CVD films. Laser Pulse Technique: While it is relatively straightforward to measure It" using surface instrumentation, it is much more difficult to measure k L perpendicular to the film surface due to the small thermal resistance in this direction. For this reason a non-contact method which uses laser pulses to heat the face of the film and fast thermometry to monitor the arrival of the thermal wave at the opposite face is employed. The thermal conductivity can then be related to the short duration thermal shock applied by the laser. Graebner, Jin, Kammlott, Bacon and Seibles (1992) utilized this laser pulse technique to help determine whether any anisotropic behavior existed in their CVD diamond films. In their study the thermal conductivity parallel to the surface kn was determined using standard surface instrumentation procedures previously discussed and the thermal conductivity perpendicular to the surface k l was determined by using a Q- switched Nd:YAG laser as a heat source. The sample was glued with silver paste over 16 a hole to a temperature controlled copper plate. Germanium lenses were used to collect thermal radiation and measure the temperature on the back side of the sample. The heat from each laser pulse conducted laterally through the sample to thermal ground at its edges. The temperature rise on the back surface and the rapid transient after each pulse were recorded by the system. The thermal jump AT(t) was calculated fiom the analytical expression presented by Parker et al. (1961) AT(t) =A[1+22 (-l)”exp( '12:"2atn, 2.3 n=1 where A=q/ng and a=kjlpCP; q is the absorbed enery per unit area and a is the thermal diffusivity. Equation 2.3 is used to solve a system of equations where A and or, are the unknown quantities. By solving for the thermal diffusivity and measuring both the thermal response and the characteristic length of the film. the thermal conductivity, k l, was calculated assuming a value for pCp. A conductivity k L of 800 and 1210 W/m K was found for two different samples with thicknesses of 234 and 144 pm respectively. Values for k L were observed to be at least 50% greater than values obtained for kII . Later the same year Graebner, J in, Kammlott, Herb and Gardinier utilized a similar setup to determine k L as a function of thickness. Here the film surface was heated using a periodic laser pulse. The temperature at the top surface was monitored using a high speed infrared detector. Four samples, 0.5 x 1.0 cm2 in area, with average thicknesses ranging between 28-408 pm were evaluated. Their results concluded that the average k i through the film increased from 1000 to 2100 W/m K as the thickness increased. 17 Infrared Thermography: Ono, Baba, Tunomoto and Nishikawa (1986) utilized this non-contact method to determine the thermoconductivity parallel to the film surface. Using a long diamond film sample suspended by heated supports in a vacuum, the temperature distribution along the length was measured by an infrared thermograph. The surface area of the samples analyzed was 20 mm x 5 mm while the thicknesses varied between 7-30 pm. Measurements were made between 100 °C and 130 °C on microwave plasma CVD diamond. From the results of this study, the thermal conductivity of the diamond films increases rapidly with decreasing concentration of methane. The highest value for It" was approximately 1000 W/m K. A significant study deterrrrining the kll of diamond films using IR thermography was later done by Albin, Winfiee and Crews (1990). The thermal conductivity was extracted from the measurement of the thermal diffusivity. Periodic heating was provided by a 20W, 1.064 pm Nd:YAG laser and the time dependent surface temperature was measured by a 8-12 pm infrared camera. A diagram of the set-up is displayed in Figure 2.6. 18 - \ In Gamma I \ I Focusing Mlnor Sm” ImageProcessor Figure 2.6. A block diagram of the type of experimental setup used by Albin, Winfree and Crews determining thermal diffusivity. Temperature measurements between 25-35 °C were made on the back side of the sample using the infrared camera. The camera scanned a single horizontal line which passed through the center of the sample and the heating area. An image processor was used to digitize 128 successive images. Each image was compressed into a single temperature profile resulting in a sampling rate of 1/30 of a second. The IR camera allowed for a temperature resolution of less than 0.02 °C and a spatial resolution of better than 1 mm. In this study k.' for two samples of thickness 16 and 32 pm were determined to be 1350 and 1328 W/m K respectively. The advantage of this technique is that the thermal diffusivity and the thermal conductivity of diamond films can be determined without special sample preparation. 19 Photothermal Laser Beam Deflection: The technique known as photothermal laser beam deflection was introduced by Machlab, McGahan and Woolham (1991) as an alternate method of determining k. in diamond films. This technique also known as the "mirage effect" uses the assistance of two separate laser beams. A diagram of the experimental setup used by Machlab, McGahan and Woolham is displayed in Figure 2.7. Figure 2.7 . Schematic of the experimental setup for the Phototlrermal Laser Beam Deflection Technique, Machlab et al., 1991. One beam generates heat pulses within the sample producing heat pulses in the air above. The thermal pulse in the air results in an optical index of refraction gradient. The second beam passes through the index of refraction gradient and is deflected with components 20 both in the plane and perpendicular to the plane of the sample. Since the heating beam is periodic, the wavelength of these propagating waves can be detected. Because the wavelength of these thermal waves depends on the frequency of the heating beam and on the thermal properties, the thermal conductivity kll can be obtained. Although their study did not include experimental results for diamond films, they were successful in determining kII for aluminum. This method like the laser pulse technique and IR radiation thermography offers a non-destructive experimental evaluation of the thermal properties in CVD diamond films. Although there have been several studies on the thermal conductivity of diamond films in recent years, they have focused on non-doped films for heat sink applications. Presently, very little is known about the effects boron doping will have on the properties of diamond. As a result, the author was unable to find information concerning the thermal characteristics of doped diamond films. Without an understanding of how the doping process affects the thermal properties of CVD diamond films, applications as a semiconductor could be restricted and unreliable. As a result, experimental methods and analytical tools are presented in the present work to aid in the determination of the thermal conductivity of doped diamond films. Chapter 3 Problem Description In the area of inverse heat conduction, which includes the estimation of the thermal properties of a material from the relative temperature distribution and temperature rise, it is imperative that an accurate mathematical model of the system be developed. The mathematical model is used to describe the experimental setup such that the thermal behavior of the experiment can be predicted analytically. Without such a model, the thermal properties cannot be determined and without an accurate description fiom the model, any results are meaningless. Since there is a certain amount of error and uncertainty associated with different experimental setups, the role of the mathematical model can also become instrumental in pre-determining the overall success of an experiment. This section is dedicated to the discussion of three different mathematical models considered in the present work. The models will later be analyzed in Chapter 4 to determine the "best" experimental setup. 3.1 Mathematical Modeling The phenomenon of heat conduction is described by the energy of motion between adjacent molecules. In nonmetallic solids, molecules having greater energy and 21 22 motion translate their energy to adjacent molecules at lower energy levels. In a solid body with a temperature gradient, Fourier’s Law is used to relate the heat flux (q) to the g(r, t) =-k(r, t)VT(I, t) 3-1 temperature (T) where the tensor k [W/m K] is the effective thermal conductivity of the material, the temperature gradient VT [“C/m] is a vector normal to the isothermal surface and the heat flux vector q [W/m’] is the heat flow per unit time and unit area. The minus sign is inserted in accordance with the second law of thermodynamics. For example, if heat flows in a positive direction, the temperature must decrease in that direction. The three components of q in the x, y and 2 directions are given by __ 6T 6T __ kaT qx" xTxlqy= -ky'-_ yay IM-qz ‘kzg- 3’2 for an orthotropic solid (Carslaw and Jaeger, 1959). The accurate estimation of the thermal conductivity k, involves a solution to the heat conduction equation, fans. (‘Q’D) dA+fc.v_g(r’ t) dV=fM PC p g—gdv 3.3 which is derived from the conservation of energy (Beck et a1. 1992). The first term represents the net heat flux rate into the control volume; g(r,t) is the rate of internal volumetric heat generation; and the right side of the equation represents the energy storage rate. The solution of the equation in this study is solved for the following general assumptions: 23 1) heat dissipated through natural convection, 2) insulated at edges 3) radiation neglected 4) no energy storage (steady state condition), 5) isothermal in the z direction; q2 = 0, 6) diamond film is isotropic. Under these assumptions, general steady state heat conduction reduces to, fans. ('Q‘D) dA+f g(r' t) dV=0 3.4 GOV. Steady state experiments were chosen to be modeled instead of transient experiments due to the performance limitations of the experimental equipment. Although the data acquisition system, comprised of the infrared camera and the image processor, had excellent spatial resolution when viewing still thermal images, the image processor software is not equiped for imaging transient events. In light of this, another data- acquisition system, comprised of the infrared camera and the National Instruments AT- MIO-16F5 AID board, was developed by the author. Using this system transient thermal events can be acquired, however, the spatial resolution is poor since the infrared camera’s sampling rate is nearly ten times that of the fastest allowable sampling rate on the available A/D board. A detailed description of both data acquisition systems is given later in Chapter 5 and Appendix A. Significant amounts of heat dissipated through convection and radiation can cause 24 severe problems in the estimation of the thermal conductivity of microstructures such as CVD diamond films. For this reason, analytical tools are presented later in Chapter 4 to help aid in the minimization of these errors and to better define what "significant" means in regards to the experimental results. In order to improve our experimental results to determine the thermal conductivity k“, which is the effective thermal conductivity parallel to the diamond film surface, we must maximize the heat conduction in the film and minimize the heat conduction in the silicon substrate parallel to the film surface, see Figure 3.1. Figure 3.1. Ratio of the diamond film thickness to the silicon thickness in the z direction. By comparing the thermal resistance of the diamond to the silicon in the parallel plane we see that, Rd = ksibsi 35 R91 kdbd 25 where Rt] is the thermal resistance and 8” is the thickness of each layer. With k,, = 150 W/mK, k“ = 1000 W/m K, d = 400 pm and 5,, = 10 pm, which are normal values for the thermal conductivity and the thickness, the thermal resistance in the diamond will be approximately six times that of the silicon substrate, R,, = 6R,,. Under these conditions, the thermal conductivity of the silicon is determined instead of the diamond film. For this reason, the silicon substrate must be etched from the backside of the sample leaving a window of free-standing diamond. An explanation of the etching process will be given later in Chapter 4. 3.1.1 One Dimensional Heat Conduction Model The one dimensional heat conduction model was chosen because its solution is readily derived. The solution is also in a form that results in quicker and easier analytical analysis. However, the analytical advantage presents several experimental disadvantages. One disadvantage is the extensive sample preparation that must be done to ensure one dimensional heat flow. The top and bottom of the sample must be patterned and etched to get a channel of free standing diamond film. The sample is also very fragile due to the necessary geometry. For the one dimensional case, we make the special assumption that the temperature gradient occurs only in the x direction. This can be done experimentally by making the characteristic length much greater than the width. With this additional assumption, the governing heat conduction equation reduces to the partial differential equation, 62T_§ (T—T,) +g=0 3.6 1‘52? a 26 where h is the convection coefficient [W/m2 K] on both sides, 8 is the thickness of the film, T. is the temperature of the surroundings and g is the volumetric heat generation [W/m’] in the diamond film. A schematic diagram of the one dimensional model is displayed in Figure 3.2. Figure 3.2. Schematic of the one dimensional model. The free standing film behaves as a fin suspended in air. As heat is generated in the film a temperature distribution on the surface of the film forms about the center while the silicon maintains a constant temperature condition at the ends. Because equation 3.6 is of second order, two boundary conditions are required for 27 the solution. Since the temperature profile from x = 0 to x = L is assumed to be a mirror image of the temperature from x = 0 to x = -L we can effectively describe the temperature distribution over the entire length by modeling one half of the exposed film. Therefore, we pick the first boundary condition at x = O. This is a boundary condition of the second kind (Beck et al., 1992) and is described by, 61’ -k-a—J{ lat-0:0 3.7 The boundary condition at x = L is of the first kind and is described by, T (x=L) =cons cant 3.8 The assumption of this boundary condition is made due to the silicon substrate that remains at the edges of the sample, see Figure 3.2. The silicon which is more than 40 times the thickness of the diamond film and having a thermal conductivity of 150 W/m K acts as a thermal heat sink. The increased thermal mass at the edges is assumed to increase the temperature gradient across the film and allow the temperature at this boundary to remain at a lower constant value compared to the exposed surface of the film at steady state. Using the boundary conditions at x = 0 and x = L yields the exact one dimensional solution, fl] cosh(m,x) + gb +1,“ 3.9 T(X)=[(Tsi-T°')-2h cosh(mrL) 2h where T,i is the temperature of the silicon at x = L and 28 [17:1, R 3.10 3.1.2 Two Dimensional Heat Conduction Model A two dimensional heat conduction model in cartesian coordinates was chosen to reduce some of the experimental challenges characteristic of the one dimensional model. This two dimensional model allows for less sample preparation, heat conduction throughout the plane of the film and a stronger film sample. Although this model is experimentally much friendlier, it is more difficult analytically. In the two dimensional model, the coordinate system is defined parallel to the mutually perpendicular directions of the heat conduction so that the geometry is said to be orthotropic. The heat conduction equation for orthotropic bodies is assumed not to contain cross-derivatives. In addition, the thermal conductivity is considered to be the same in the x and y directions which is known as an isotropic condition. In the two dimensional model, heat is free to flow in the plane of the film, in directions x and y. By applying this special assumption, the two dimensional heat equation for this case is, kfl-I-k—afl-Eg (T—T”) +g=o 3_11 6x3 6y2 5 where the thermal conductivity is assumed to be constant throughout the film. For this model special design considerations are also needed for the sample. Although detailed information on the design and fabrication of the actual diamond sample is given in 29 Chapter 4, a schematic of the physical design of the sample for the two dimensional model is displayed in Figure 3.3. diamond fllm \ etched region Side 4’ Back b Figure 3.3. Schematic of the two dimensional diamond lem sample, etched from the backside. Here, the sample is etched from the backside resulting in a rectangular window of free standing diamond at the center. Such a sample would still have the silicon substrate at the edges to maintain the temperature boundary condition. By designing the sample in this way, we can solve the governing two dimensional equation using a model which has volumetric heat generation g [W/m’], constant temperature boundary conditions, and two axes of symmetry. A schematic of the model is displayed in Figure 3.4. 3O T-constant I. / . T-W diamond l \ film | | a i x-O I l "L I >conm y f _. T-constent a y-0 b Figure 3.4. Schematic of the two dimensional model. Since the model has four symmetric quadrants, we can effectively determine the temperature distribution on the entire face of the film by mathematically describing the temperature distribution in just one of the quadrants. A diagram of one of the symmetric quadrants is displayed in Figure 3.5. 31 T-constant . / l l diamond film q(y-O)-0 I T-eonstant \: a / ML | y o +——7————4b th-Oi-O Figure 3.5. One of the symmetric quadrants for the two dimensional model. With a boundary condition of the second kind at x = 0 and y = 0 and a boundary condition of the fast kind at x = a and y = b, we turn to the Green’s functions, GM and GY21 , to obtain the solution, 4 - - cos(l3mg)cos(pn%)(-1)m-1(_1),,_1 T(X’Y)="kgzz (3 13 +2"... 3.12 m-ln-l pmpn[(-f)2+(—5n)2+mf2] where [in = rt(m-1/2) and [5,, = 1t(n- 1/2), (Beck et al., 1992). 32 3.1.3 Radial Heat Conduction Model The radial heat conduction model was chosen as a compromise between the analytical simplicity of the one dimensional model and the experimental advantages of the two dimensional model. The steady state solution for this model is well known and easily obtained for different conditions. Although the heat conduction would be restricted to one direction, it would also spread throughout the plane of the film, as in the two dimensional case. For the one dimensional radial heat flow model, we make the special assumption that heat conduction is restricted to the radial direction. The physical design of the sample would be similar to the two dimensional case, but would have an exposed diamond window which is circular instead of rectangular, see Figure 3.6 For the one dimensional radial model the governing equation becomes, dzT 1 d1" 21: ——- — = 3.13 kdzz+krdr T(T T,)+g O A schematic drawing of the one dimensional model for radial heat flow is displayed in Figure 3.6. 33 T - constant diamond film Figure 3.6. Schematic of the radial heat conduction model. The general solution for the one dimensional radial heat flow is described by, T(r) =ClIo(m,.z') +C2Ko (mtr) +—L +21", 3,14 mfzk where I0 and K0 are the Bessel functions (Beck et al., 1992). Since the temperature at r = 0 is finite, Q must be zero, and we are left with a boundary condition of the first kind, T| r=b= cons tan t: 3.15 34 By applying this boundary condition to the general solution and solving for C1 we obtain, T(r) =__i_ [1- 10mg) —— +T, 3.16 mgr. I.2" . at . ‘ t ‘ . . . . z-x. , ~ A. ~ . " l ' _ 4:. -I~..o:. ;. A ' ' ‘ ' ' I .- ' - ‘ ' I. v . r l > e e v t. I . . . . , » -: .\ .‘ ‘ : .~'..” '. ‘. . t ' ’3 . .- - .. a ‘ ’ l . . . . . . , w . , '.. ‘ . . ' .‘ .. ' ‘ .1”, ' .. .. J '.. ¢_ . '1; .r. ~ .- .. _ , . . . .z, . ' r e "'. . 4 '\ .. '.- t ‘ .. .. V , . ‘ ‘ .'.'\'.. ”r. . . - .. fl 3 ~ ‘ ‘2 ' 1 ‘ ‘ ‘ . ‘ ..'. "I not. .24 a, _: . . i- 4 a . . ,. ~ "r. ‘I . . . .. .- .x-..- . . .. . - . . ,. :~. .n . . s p ., u ,. .. ' ' ~'..\' A; ‘ ‘: 'c‘ -. is; ' '-'.\':’= :v’..- 3" 1' - .' ' . ~. ‘ -:- .-:;r . .M. .' A'.’ . . ' -,. .p - .' u . . -\\l/ \ ’ '3 ‘ ' \ ' " '. -, ." ~ . - . w -. . ' v . I _ . . . . r . . A , J , . _ . . .. k . - _ . ' u '- J‘; 1. .. w \' . . A . ' x a .'. ...¢ . A v 'v, _“.- -_,'_ ' ._ . ' .... . :4 i - . .l‘ \ 1 - .- . ; . .~ - :~ . . a . .4‘. . . . El 2:!" ' "t :10". , cl": = . , ".1 . ,‘. n, can: sneeze at 972m 906' HT" 56191.5 a P1 CUH= 55:96.0 R Ii 1’992ul’1 'SLOFIN DEKTRK II Figure 4.20. Thickness of the doped film on sample A measured in A by the SEM. Figure 4.20 shows a thickness of approximately 56,000 A (5.6 pm) for the doped diamond layer on sample A, while Figure 4.21 shows an increasing thickness of nearly 60,000 A (6 pm) for the doped region on sample B. 69 at. 2.3a: q ' H. :2: tamer he” ._ieaiffl%p it i ' Xvi") ‘:':-."_' 3198’" ’“w‘fi 1%3'.’ 5} "' ? i-ee.m 7'23: ' 23m 2 ‘0 5.: (20.909 a cum 04.816 9 a 7.3230" ‘ ‘ "HUG-’HT- B34:?9.:':9.. l‘1 CURz 87.19? A (I B. 933.0" . SLOGN DEKTfiK I! Figure 4.21. Thickness of the doped diamond film on sample B measured in A by the SEM. 4.6 Bottomside Sample Fabrication When designing a sample that has a free standing circular diamond window 5 1 cm in diameter, specialized fabrication techniques must be used on the bottom of the sample. For instance, in order to remove the silicon backing in the area of interest and maintain the sample’s structural integrity by retaining silicon in other areas, the diamond must first be patterned on the backside. Patterning, commonly known as masking, is a technique which enables diamond to be deposited and grown in precise surface configurations. To pattern the samples, a mask is first designed. The mask is used to block UV 70 rays which bombard the photoresist after it has adhered to the back of the sample. By exposing the photoresist to UV radiation, diamond growth occurs in the regions shielded by the mask and is eliminated in the exposed regions. After the back has been patterned, the undoped diamond deposition process is again repeated. Unlike the top layers of diamond, the thiclmess of the bottom layer has no significant effects on the results. However, the layer needs to be continuous to guard against excessive removal of the silicon during etching. Pictures of one of the diamond samples made by the Microstructures Fabrication Laboratory is displayed in Figures 4.22 and 4.23. Figure 4.22. Deposited doped diamond film on the front side of sample A. 71 Figure 4.23. Diamond mask patterned on the back side of sample A. With the diamond deposition completed on the backside, the sample can now be etched. To etch the sample a solution consisting of 25 ml of hydrofluoric acid (HF), 50 ml of nitric acid (HNO3), and 25 ml of acetic acid (CH3COOH) is prepared. The solution is then carefully deposited (using a micro pipette) inside the circular region on the backside of the sample where it attacks the exposed silicon. Since the solution is applied to the silicon substrate in small amounts, the acid and its potency tend to evaporate rather quickly. In light of this, the solution is periodically deposited to the silicon surface until it has penetrated through to the undoped layer of diamond on the topside of the sample. This process, however, is a tedious one and takes several days to complete. With the 72 silicon completely removed in the circular region inside the diamond mask, the top layers of diamond are now free standing and exposed on both front and back sides. Chapter 5 Experimental Techniques Experimentally, diamond films are one of the most challenging materials to analyze thermally. Their microstructural size and rapid thermal response pose both spatial and temporal problems for experimental techniques utilizing surface mounted temperature sensors such as thermocouples and resistance thermometers. For this reason an optical, non-contact technique was implemented for temperature acquisition. This technique detects the thermal radiation emitted by an object and calculates the temperature. The experimental techniques developed for the steady state temperature measurements of doped diamond films are described in this chapter. Included are subsections detailing the data-acquisition system and the experimental setup. 5.1 The Data Acquisition System The data acquisition system is comprised of three primary components: 1) the Model 600L Infrared Imaging Radiometer, 2) the Thermal Image Processing System and 3) a digital multimeter. The first two components, the infrared radiometer and the image processor, comprised the temperature measurement system, while the digital multimeter 73 74 is used to measure the power generated in the electrical circuit. A diagram of the data acquisition system is displayed in Figure 5.1. lieutenant-d 00mm WW ¥ I --:I=- l l - out-rum Germanium terrain-W — mm mm Figure 5.1. Diagram of the data acquisition system. 5.1.1 The Inframetrics Model 600L Infrared Imaging Radiometer The Inframetrics Model 600L Infrared Imaging Radiometer, consisting of an infrared scanner and an electronic control unit, is designed for applications requiring real- time analysis of static or dynamic thermal patterns. The high performance system combines superior image quality and thermal sensitivity with true temperature measurement display and background correction. The system can also be linked with a video cassette recorder or a thermal image processor to store thermal events. The Model 75 600L IR Radiometer complete with scanner, RGB monitor, control unit and VCR is displayed in Figure 5.2. Figure 5.2. The Inframetrics 600L IR Radiometer. The scanner incorporates two independent electromechanical servos (galvanometers) which perform horizontal and vertical scanning. Attached to these servos are scanning mirrors which are contained in a sealed, evacuated module for increased efficiency. Horizontal scanning is performed at the very high rate of 8 kHz in a resonant sinusoidal mode. Vertical scanning is performed in a sawtooth pattern consistent with standard TV formats at 60 Hz. The thermal radiation entering the scanner through a germanium window is 76 deflected by the horizontal and vertical scanning mirrors and is focused on a HngTe detector. Motorized focus and zoom mechanisms are operated within the scanner by remote control. With the HngTe detector cooled by liquid nitrogen to approximately 77 K, maximum thermal sensitivity is obtained. The signal generated by the HngTe detector is processed, digitized, reformatted and prepared for visual display by the control unit. A microprocessor within this unit accesses such functions as background temperature, temperature range and emittance settings, image averaging, fast line scanning, focusing and zooming. The microprocessor also performs internal calibrations as the temperature of the scanner changes and when filters or lenses are connected to the scanner. The control unit accesses individual picture elements, then calculates temperatures according to calibration curves which were measured at the factory and stored in a read-only-memory. Due to variations to spectral response, every system has a unique calibration curve. The output from the control unit is a standard RS-170 format with 8 bit resolution, providing 256 pixels/line. In order to increase the spatial resolution when imaging smaller objects, two additional lenses are installed on the front of the scanner. One lens in a 3x telescopic lens which is connected directly to the scanner. Attached to the telescopic lens, however, is a 6" closeup lens which can resolve objects smaller than 100 pm. A photograph of the two lenses is displayed in Figure 5.3. 77 6' close-up lens 3x telescopic lens Figure 5.3. The 6" close-up lens and the 3x telescopic lens used to increase the spatial resolution of the radiometer. 5.1.2 Thermal Image Processing System The Thermal Image Processing System is primarily used to capture and store entire thermal patterns and access temperatures corresponding to any or all digitized picture elements (pixels) which make up the thermal field. Each field consists of 365 x 280 pixels, totaling over 102,000 accessible surface temperature measurements. Temperature measurements are individually calculated from the radiant intensity 78 of each pixel, which is digitized and saved in an 8 bit format. When the minimal 5 °C temperature range is activated on the control unit of the Radiometer, a maximum thermal resolution of 0.03 °C is attained. By using the external optics previously discussed and seen in Figure 5.4 and by zooming in at the minimum field of view allowed by the radiometer, the spatial resolution shrinks to approximately 1 pixel / 10 pm. With this type of spatial resolution, the smallest area that can be fully imaged is approximately 4 mm x 3 mm. The Thermal Image Processing System resides in an Epson 286, 16 M2 PC. Since the computer is only used to run the driver software for the image processor, access its functions and store images, the 286 is an adequate machine. 5.1.3 The Omega 880 Digital Multimeter In order to simplify the experimental setup and resulting experimental procedures, the Omega 880 Digital Multimeter is used to measure the power supplied to the electrical circuit to calculate the internal heat generation within the doped diamond film region. A picture of the multimeter is displayed in Figure 5.4. 79 altimeter. The multimeter is used to check and measure the applied voltage and determine the current flowing through the circuit usually by measuring the voltage across a known resistance, see Figure 5.1. 5.2 System Calibration Check Since the radiometer uses inaccessible internal calibration curves which were measured by the supplier to calculate temperature, it is important that the performance of these tables be calibrated versus a known temperature in order to validate this temperature measurement system. The radiometer was calibrated using a vertically mounted "black" 80 aluminum plate which was uniformly heated from the backside and had a thermocouple attached to the center of the frontside. The thermocouple was used to measure the temperature of the plate. Assuming the emissivity of the plate to be 0.98, the temperature measured by the radiometer was the same as the temperature measmed by the thermocouple. In this case, the emissivity that is input into the control unit of the radiometer merely acts as a calibration factor which initializes the "actual" temperature of the thermocouple and measured temperature of the radiometer. As the temperature of the plate increased, the corresponding temperature measured by the radiometer was recorded. The calibration covered a temperature range from 25- 100 °C and the results are presented in Figure 5.5. 110 I I T I f — Tgcorrected) - 1.00801(meaeured) - 0.307 100- - 80- - 70- ~ 60- - 50- - corrected temperature [ C] ISO-I .. 20 f H I I T i I I 20 30 4D 50 60 70 80 90 1 00 1 l 0 measured temperature [ C] Figure 5.5. Corrected temperature of thermocouple vs. measured temperature of radiometer. 81 In Figure 5.5 the thermocouple temperature (assumed to be the true temperature) is plotted as a function of the temperature measured by the radiometer. A linear curve fit was performed on the data resulting in the equation, Tcm=1 . 008*ng-0 . 307 5.1 where Tom is the corrected temperature measured by the thermocouple and Tm is the temperature measured by the radiometer in °C. Although the constant term, ~O.307, creates a difference between the actual temperatme and the measured temperature, it has no effect on the relative temperature rise, which is the quantity needed to determine the thermal conductivity of the diamond film. Since the relative temperature rise is quantified as the difference between the initial temperature and the steady state temperature, the constant drops out and we are left with AT cczA T 5.2 111968 Even though the exact value for the emissivity of the plate must be assumed to measure the temperature of the plate with the radiometer, the internal calibrations used by the control unit are assumed to be valid since the calibration is linear and has a slope of 1.008, which is less than 1% different from one. The recorded temperature range of 25- 80 °C extends beyond the expected relative temperature rise of the experiment. The biggest challenge in using this type of temperature acquisition system, however, involves the emissivity. In order to measure the absolute temperature or the relative temperature rise of a material, the emissivity must be known or determined. Unlike thermocouples and resistance thermometers, the temperature measured by the 82 radiometer is a function of the radiant intensity. For a simplified illustration, the emissive power of a grey body is expressed as, E=80T4 5.3 where e is the emissivity, o is the Stefan-Boltzmann constant and T is the temperature in Kelvin (Siegel and Howell 1981). The radiometer internally calculates temperature from the measured emissive power E. From equation 5.3 it is evident that the emissivity must be used to determine the absolute temperature and we find that the same holds true for the relative temperature rise. Using equation 5.3, the relative temperature rise of a grey body is calculated to be 1 a a 80 cult-s ) 5.4 where T and E are the temperature and the radiosity at a certain state and T. and E. are the temperature and radiosity, respectively, of the surroundings. From equation 5.4 we also see that the relative temperature rise is a function of the emissivity. In order to check the assumption that the relative temperature rise is a function of the emissivity, the radiometer was used to record the temperature of a heater at two different power levels. At each level, temperatures were measured using two different assumed emissivities. Since the change in the radiosity (AB) is the same in each case, the temperature difference at each emissivity is compared. Figure 5.6 is a plot of the surface temperature of the heater for both high and low radiosity levels using emissivities of 1.0 and 0.80. 83 100 flava) - 05.4 “ f~ r'\ l" 90" .1 85- _ Heater Temperature [ C] Location on Surface of Heater Figure 5.6. Heater surface temperature vs. location At each level the average temperature across the surface of the heater was determined. The small peaks correspond to the heater element locations across the surface. If the temperature rise is a function of emissivity, we should get different AT’s at each emissivity setting, which is the case. The temperature temperature difference at e = 0.80 (95.4-74.4) equals 21 °C whereas the temperature difference at e = 1.0 equals only (76.0- 58.6) 17.4 °C. These values of 21.0 and 17.4 are quite different, hence, it is evident that in order to accurately determine the relative temperature rise across the surface of the sample we must carefully determine the emissivity of the doped diamond film. Procedures involving the determination of the emissivity are discussed later in Chapter 6. 84 5.3 Experimental Setup A series of steady state experiments was conducted on one of the diamond film samples (sample A) which was prepared by the Microstructues Laboratory. Because of the special design considerations of the samples, the sample setup consists of only four items: I the diamond film sample, I electrical conducting adhesive tape, I electrical lead wires and I an adjustable clamp to suspend the sample in a vertical position. 5.3.1 Preparation of the Sample Setup Each of the two setups for each sample is constructed in exactly the same manner starting with cutting the electrical conducting tape into two strips approximately 2 cm x 0.45 cm. It is important that the tape contact only the surface of the doped diamond film and not the silicon substrate. Since good contact between the tape and the film surface is imperative silver paint was added to the diamond-tape interface. A schematic and photograph of sample A after experimental sample preparation are displayed in Figure 5.7 and Figure 5.8. 85 Figure 5.7. Schematic view of sample setup. silicon substrate electrical ey . - nnfiimflnn Figure 5.8. Photograph of the sample setup. Chapter 6 Procedures and Results for One Dimensional Radial Experiments This chapter presents the experimental procedures and preliminary results for the measurement of the thermal conductivity for a doped diamond film sample prepared by the Microstructures Laboratory at Michigan State University. As described in Chapter 4, the one dimensional radial heat flow model was designed to decrease the relative error in the measurements and to obtain a more symmetrical temperature distribution. By choosing a diameter of less than 0.003 m for this model, convection, which becomes less than 1% of the total heat generated, can be neglected, further simplifying experimental procedures. Issues concerning the determination of diamond film emissivity, electrical power, optimal radiometer settings and temperature acquisition are also discussed in this chapter. 6.1 Determining the emissivity As explained in Chapter 5, the emissivity of the diamond film must be determined in order to accurately convert the emissive power measured by the radiometer to surface 86 87 temperature. The emissivity of the diamond film sample was determined by adjusting the emissivity value input required by the radiometer such that the temperature calculated by the radiometer matched that of a thermocouple attached to the surface of the diamond film. The setup used to determine the emissivity of the diamond film is presented in Figure 6.1. Figure 6.1. Setup used to determine the emissivity of the diamond film for sample A. The area mode on the control unit of the radiometer was activated allowing for a real time averaged temperature measurement over a small surface area anywhere within the imaged field of view. With the small area positioned on the junction of the thermocouple itself, the radiometer measured the temperature of the thermocouple as the sample was 88 heated over a temperature range from 25-55 °C. The temperatures matched when using an emissivity of 0.63 as input into the control unit. The correspondence between the temperature measured by the thermocouple and the temperature measured by the radiometer using an emissivity of 0.63 is presented in Figure 6.2. 2 I t-temperoture meaeured by Wale 2 55‘. — r - 1.00M - 0.277 1 I — e-O.” ‘ Temperetweolmdiometedcl ‘7’ a 114 IAAJ‘JIIAL AIAA N U N O Temperature of thermocouple [ C] Figure 6.2. The relationship between the temperature measmed by the radiometer and the thermocouple at an emissive setting of 0.63. By performing a linear curve fit on the data, we see that there is a slope of 1.007 for a temperature range between 25-55 °C, refer to Figure 6.2. The correlation coefficient for this linear curve fit was determined to be 0.998. Since there is less than 1% error in assuming a slope of 1.000 and since the constant offset is cancelled out when taking differences, we are confident in assuming the emissivity of the diamond film to be 0.63 over the temperature range of interest here. 89 Ideally, we would like to determine the emissivity with the junction of the thermocouple attached to the free-standing diamond film, since it is the temperature distribution in this region which will be recorded. However, attempting to apply and attach a thermocouple to this fragile area proved to be disastrous for sample B. Upon first attempting this procedure using sample B, the free-standing diamond window was subsequently broken when thermocouple wires (approximately 100 pm in diameter) were pushed through this region. With just one other sample to work with, sample A, every precaution was taken to ensure its structural integrity not only in this procedure but in the ones that followed. 6.2 Measurement of the Electrical Power Measuring the electrical power in the designed circuit is imperative in determining the volumetric heat generated in the doped diamond film region. Without knowing the volumetric heat generation it is impossible in the present experiment for us to determine the thermal conductivity of the CVD doped diamond film. However, due to the rapid thermal response of diamond during heating, the Omega digital multimeter can have difficulty tracking the electrical current flowing through the circuit. This problem is further compounded by the fact that electrical power generated within the doped region of the film was found to be a function of temperature. For this reason, the electrical power is calculated by determining the electrical resistance of the doped film as a function of temperature, rather than the standard method of measuring the voltage across a known resistance. In order to measure the resistance as a function of temperature the sample was placed in an oven where the electrical resistance was measured using the 90 digital multimeter and the temperature was measured by the thermocouple used to determine the emissivity. The temperature of the oven was varied over a range from 25- 55 °C. The results of the measured resistance at different temperatures are presented in Table 6.1. Temperature (°C) Resistance ((2) 25 1184 30 1 173 35 1 157 i 40 1 144 45 1 124 50 l 101 55 1075 i Table 6.1. Temperature versus resistance for sample A. Notice that the resistance decreases with increasing temperature, which is characteristic of semiconductors. About a 10% reduction in the electrical resistance is noted over a temperature rise of 30 °C. 91 Hence, instead of measuring the current through a known resistor and calculating the power using V*I, where V is the voltage and I is the current, the electrical power can be more accurately determined in this case from the V2/R relationship, where V is the voltage and R is the electrical resistance. 6.3 Radiometer Settings After the emissivity (e) and the resistance of the diamond film have been detemrined, the radiometer is now prepared for thermal image acquisition. Using an emissivity of 0.63, the thermal sensitivity was maximized by using the smallest temperature range of 5 °C. Four images were averaged in real time to improve the signal- to-noise ratio. Image averaging is an attractive option for two main reasons. First and foremost, the signal-to—noise ratio alone is increased by a factor of two in this case and second the amount of data is compressed by a factor of four. However, when using this real time image averager, one must be certain that the displayed thermal field, a composite image averaged from fom separate fields, does not contain any thermal information of the relative temperature rise of the diamond window in its transient state. Since the averaged image is being scanned at a 0.07 sec interval (60/4 Hz), we need to capture the image at least 0.07 sec after the relative temperature rise is at a steady state condition or transient effects would be averaged into the results. The time constant of the film can be approximated by the relation, tel”: , 6.1 a (Carslaw and Jeager 1959) where at is the thermal diffusivity of the diamond film, b is 92 the radius of the etched region and t is the approximate time in which the relative temperature rise reaches steady state. Assuming a thermal conductivity of 200 W/m K, a density (p) of 3500 kg/m3 and a specific heat (CI) of 509 J/kg K, the thermal diffusivity (0t) is calculated to be 112.3 x 10 ‘ m2/sec for this case where b = 0.003 m. A thermal conductivity of 200 W/m K, which is on the low end of the published values for the thermal conductivity of diamond films, was used to give us a "worst case" scenario for the time constant. The larger the time constant, the more limiting is the use of the image averager. From equation 6.1, the time constant of the diamond film is calculated to be approximately 0.02 sec using a radius (b) of 1.5 mm. Hence, as long as we capture the image 0.10 see after the film has started to heat, the composite thermal field averaged over four images should represent the relative temperature rise in its steady state condition. It should be noted that although the relative temperature rise of the etched diamond window reaches a steady state condition, the surface temperatures continue to rise as the sample is heated. This condition is termed a quasi-steady state and it is this condition that describes the global heating of the diamond-silicon specimen. Because the heating of the sample is described by a quasi-steady state condition and not entirely by the steady state condition modeled, it is important to determine the amount of energy lost due to the heat capacity of the diamond sample. The effective volumetric heat capacity gm, of the diamond film which is the energy absorbed in the film itself is given by BT ghcap= P C335; 6-2 93 Using the density (p) and the specific heat (CI) for diamond, as previously determined, and typical experimental data where aT/at = (30-22)°C/ 2 secs, gm, ~ 891le W/m’. We now need to compare the volumetric heat capacity, gm with the measured volumetric heat generation, gd. For an experiment corresponding to the particular temperature rise used to calcuate gm, , g,l as 1.75x109 W/m’. By determining the ratio (ng/gd), we see that the energy needed to increase the temperature of the exposed diamond film in its quasi-steady state represents less than 0.1% of the total volumetric heat generation (g) in the film. 6.4 Surface Temperature Measurements Acquiring surface temperature measurements when using the thermal image processor consists of two main processes: 1) capturing the desired thermal field and 2) acquiring the surface temperatures, respectively. 6.4.1 Capturing Images Using the Thermal Image Processor Before the actual thermal images are acquired, the sample must be aligned and focused within the desired field of view (FOV). Because the focal distance between the sample and the scanner is approximately 15 cm, the minimum FOV could not be used because the scanner aperture reflected back off of the sample. This reflection shows up as a black dot, which is present in the center of the image at close range and is magnified when decreasing the FOV. As a result, the FOV and the position of the sample were adjusted to avoid this reflection. In the experiments that follow two different FOV’s were utilized. 94 Once the optics are adjusted and the scanner focused, the sample was connected to the electrical circuit and a constant voltage is applied. The temperature of the sample immediately increases and as it enters into the user defined range (e.g. 25-30 °C) the image is captured and stored using the freeze frame on the image processor. It is this image which contains the desired temperature distribution across the film. During this procedure, the radiometer was first focused on the front side of the sample. However, in this position the boundary temperature at the silicon-diamond interface was difficult to determine. Since the chemical etches the silicon at an angle, the thickness of the silicon at this interface is relatively thin, making it difficult to locate when imaging through the diamond on the front side. A photograph of the sample setup viewed from the front side is presented in Figure 6.3. silver paint diamond ' w1ndow electrical conducting tape Figure 6.3. Sample setup viewed from the front side. 95 As seen in Figure 6.3, silver paint was used on the sample to increase electrical contact between the electrical conducting tape and the doped diamond surface, resulting in increased uniform heating. The paint was not essential. In order to locate the boundary of the free-standing diamond window 3 mm in diameter with greater precision, the sample was simply rotated 180° such that the back side of the sample was imaged. A photograph of the sample setup in this position is presented in Figure 6.4. etched diamond window Figure 6.4. Sample setup viewed from the back side. 96 In this position the diamond-silicon interface can be determined more accurately in the infrared image. Since there is a negligible temperature gradient across the thickness of the diamond film and since the sample is symmetric on both faces, the temperature distribution on both sides of the sample is assumed to be equivalent. Hence, our results should not be adversely affected by positioning the sample in this manner. Before acquiring the thermal images, the precise location of the diamond- silicon interface in the FOV is determined. By using the electronic ruler provided by the image processor software, the coordinates for the diameter of the free standing diamond film are located. After the diameter is located, the x,y coordinates which are displayed by the RGB monitor are recorded such that the appropriate temperature distribution can later be extracted from the acquired thermal field. After the diameter of the free standing film has been located in the FOV, the thermal fields can now be acquired. With the power settings set at approximately 0.40, 0.62 and 0.88 watts five thermal images were captured using two different FOVs. These images can be viewed in Figures 6.5-6.9. 97 ,(‘mez-ei 23911 f. a 4+ "i; ‘53..»35 (13:35 :24; a.vg=-.;-¢, 2'3 NEE-E Fez: Figure 6.5. Image 1 from Figure 6.6. Image 2 from experiment #1 at 0.40 watts. experiment #2 at 0.62 watts. '2‘? E“: 1’51».th ”SEE ElfITT'J’aiE— £7 *3} 157‘): Figure 6.7. Image 3 from experiment #3 at 0.88 watts. 24 out Erl-‘I‘JE 2x35: Emmi-:5: r53 .39 etc as 57-: raw-.55 m3; 3.... .. . Figure 6.8. Image 4 from Figure 6.9. Image 5 from experiment #4 at 0.40 watts. experiment #5 at 0.88 watts. 98 6.4.2 Temperature Acquisition After the thermal images have been acquired using the appropriate control unit settings on the radiometer, the temperatures can be determined from the thermal field using the File_Access program run by the GWBASIC interpreter. This program, which is part of the thermal image processor software, extracts data from a particular line in the thermal field and converts the individual pixel intensity to temperature using calibration tables stored in the ROM of the radiometer’s microprocessor. To extract the temperature distribution, File_Access simply prompts the user for the image filename and the line number. With the location of the diameter already determined, the line number is entered and the temperatures corresponding to the pixel location across the entire thermal field are then written to a data file. After the temperatures have been determined across the designated line from the thermal field, the next step is to extract only those temperatures associated with the temperature distribution across the diameter of the diamond window. Since the coordinates of the diameter were already determined by using the electronic ruler, the temperature distribution across the 3 mm diameter free-standing diamond window for each of the five experiments can be located and extracted from the line temperature data extending across the entire horizontal FOV. The temperature distribution for each of the five experiments can be seen in Appendix B. 6.5 Measurement of the Thermal Conductivity Quantifying the thermal conductivity after acquiring the temperature distribution across the diamond film requires two steps. The first step is to develop a mathematical 99 model for the problem; and the second step is to use the temperature data and the model together to estimate the thermal conductivity (k, I)° 6.5.1 The Simplified Experimental Model Because the temperature difference between the smface of the film and the surroundings is small (within 10 °C), it is reasonable to assume that radiation can be neglected. The validity of this assumption is demonstrated below through acquired experimental data. Heat transferred by radiation is described by grad=2Aeo (T‘-T,,‘) 6.3 where e is the emissivity, 0‘ is the Stefan-Boltzmann constant, T is the temperature of the film, T. is the temperature of the surroundings and 2A (21:11) represents both sides of the surface area of the exposed diamond window. With 8 = 0.63, 0' = 5.67 x 10" W/m2 K‘, r = 0.0015 m, T = 305 K (32 °C) and T, = 295 K (22 °C), qml = 0.00054 W. Since the temperature difference used in this calculation simulates experiments for the largest heat dissipation (q = 0.88 W) radiation represents less than 0.1% of the total heat generated within the film and, therefore, can be neglected. Since the diamond window was etched to only a diameter of 0.003 m to aid in the strength of the sample, the effects of convection, discussed in detail in Chapter 4, can also be neglected With a characteristic length of 0.003 m convection S 1% of the total heat generated within the film, when assuming a thermal conductivity between 250-1000 W/m K, which is the expected range for the thermal conductivity of doped diamond. Tire 100 percentage of heat lost due to convection is, again, calculated from equation 4.19. By neglecting convection, the former mathematical description of the experiment, described by equation 4.10, is further simplified to = gdbd 2_ 2 0(1) 4k(0u+6d) (b r) 6.4 where V2 = 6.5 9" 12wa d and 6(1) =T(I) -Tb 6.6 Equation 6.6 represents the difference between the temperature at the boundary (r=b=0.0015 m) and the temperature at a particular radial position. 6.5.2 Estimating the Thermal Conductivity Now that the appropriate temperature distributions have been acquired and the governing equation simplified, the program NLIN (Beck 1993) is used to analyze the data and estimate the thermal conductivity. NLIN uses the method of least squares N 5:; [Yj-Tj12 6.7 =1 where N is the number of data points, Yj is the measured temperature and T1 is the calculated temperature represented by 101 Tj=Tb+HK[1-(—Ig)3] 6.8 where H = (gd84b2)/4(5,,+84) and K = Me. Using the method of least squares the program simultaneously estimates both T, and k to calculate Tj such that the error in S is minimized. In order to minimize the error in S, NLIN uses the system of equations as =_2" ”41:0 6.9 '33) g; r j and _a§=_ N - .. £1 2 = 6.10 6k 2; [Y1 leHtl (bH 0 Actually, NLIN is a sequential nonlinear estimation program that has more complex calculations than indicated by equations 6.9 and 6.10 but these equations form the basis of its estimation process for this linear problem. By inputting H = V2b2/4RLW(5,,+84) for each case where L = 0.0045 m, W = 0.02 m, b = 0.0015 m and V is measured and R is determined from Table 6.1, Tj is calculated for each of the five experiments. The measured temperature distribution (Y1) and the corresponding calculated temperature distribution TJ across the surface of the diamond window are displayed together in Figures 6.10 and 6.11. The largest temperature rise is approximately 3 °C. 102 343 I I I I I I I 4 '5' 5 g a-OAO eette S 25.0- 24.0- - 22.0 I 1 I I I I I --l.00 -.75 -.50 ~25 0.00 0.25 0.50 0.75 r/b 1 .00 Figure 6.10. Measured and calculated temperature distribution for experiments 1,2 and 3. q-OAO eatte Temperature [ C] 24.0- 34.0 I I I I I I I i 32.0- ”-0... -' 30.0- - 28.0- 26.0- all «i J 1 22" I I I I I -1.00 -.75 -.50 -.25 0.00 0.25 r/b I 0.50 I 0.75 1.30 Figure 6.11. Measured and calculated temperature distribution for experiments 4 and 5. 103 NLIN not only fits the mathematical model, equation 6.4, to the data but it also calculates the residuals which are the differences between the measmed and calculated temperatures [Yj-Tj]. The residual distribution for each of the five experiments can be seen in Figures 6.12-6.16. The standard deviations are approximately 0.18 °C, compared to about a 2 °C temperature rise. 0.8 I l I T I I I ~ experiment It. q-O.4D watts r 0.6-e .. 0.4- -- '8 0.2- .E o 0.0- s . 1 3. -.2- . a 1 -.4-' -I -.6- - - J ’3 I I I I I I I -1.00 -.75 -.50 -.25 0.00 0.25 0.50 0.75 1.00 r/b Figure 6.12. Residual distribution for experiment #1, 107 pts. 104 0.0 I I I I I I I - experiment '2. tar-0.62 watts ' 0.0-I - 0.4- - '5' 0.2- H '1 q ‘3’ 00- - g -.2- -r 1 -.4-1 - 1 I -.6- - “'8 I I I I I I I -1.00 -.75 -.50 -.25 0.00 0.25 0.50 0.75 1. 30 r/b Figure 6.13. Residual distribution for experiment #2, 107 pts. 0-3 I I I I I I m < experiment '3. a-0.88 matte - 0.6- .. 0.4-1 - 4 '8 0.2 '1 _. "" 1 g 00- - :3 2° - .. 3 -2. . -.4- d ‘ 1 -.6- - ‘3 I I I r I I I - 1 .00 -.75 -.50 -.25 0.00 0.25 0.50 0.75 1 .00 r/b Figure 6.14. Residual distribution for experiment #3, 107 pts. 105 0.8 I I I I I I I - experiment [4. q-0.40 watts . 0.0- .. 0.4- - q 8' 0.21 . 2:; . ‘ g 00- .. i ‘ ‘ -1. .. -.4‘ - -.0-1 -I ”-8 I I I I I I I -1.m -.75 -.50 -.25 0.“) 0.25 0.50 0.75 1.00 r/b Figure 6.15. Residual distribution for experiment #4, 121 pts. 0.0 I I I I I I I experiment '5. q-0.88 eatte - 0.0-1 .. 0.4- -I '5' 0.2-1 -- A 0 'g 0.0- - 29 . . é —.2~ - -.4- e --6-' -l I J '5 I I I I I I I —1.00 -.75 -.50 -.25 0.00 0.25 0.50 0.75 1.130 r/b Figure 6.16. Residual distribution for experiment #5, 121 pts. 106 Across most of the diameter, the residual pattern is unique for each of the five experiments, representing a random rather than a systematic error. However, in the region 0.75“)') DO 6 IP=1,NP READ(8,*)(PS(IP,KP),KP=1,NP) WRITE(7,'(5D16.5)') (PS(IP,KP),KP=1,NP) CONTINUE BLOCK 4 DO 88 IP=1,NP 8 PS(IP,IP)=B(IP)*B(IP) READ(8,*)IEXTRA IEXTRA-O FOR NO EXTRA INPUT WHICH COULD BE FOR CONSTANTS IN MODELS 81 FOR ONE INPUT, NAMELY: EXTRA(I), ETC. WRITE(7,*) WRITE(7,*)'BLOCK 4' WRITE(7,*)'IEXTRA - NO. OF EXTRA(I) PARAMETERS, 0 IF NONE' WRITE(7,*) WRITE(7,'(10X,"IEXTRA - ",IlO)')IEXTRA IF(IEXTRA .LT. 1) GOTO 21 WRITE(7,*) WRITE(7,*)'BLOCK 5' WRITE(7,*)'EXTRA(1),... ARE EXTRA CONSTANTS USED AS DESIRED’ WRITE(7,*) READ(8,*)(EXTRA(IE),IE=1,IEXTRA) WRITE(7,'("EXTRA(",I2,") - ",F16.5)') (IE,EXTRA(IE),IE=1 1,IEXTRA) 21 CONTINUE m OQOOOOOON 000 C C --- ADD BLANK CARD AFTER LAST INPUT CARD C ---END INPUT WRITE(7,*)'END INPUT QUANTITIES - - BEGIN OUTPUT CALCULATIONS' WRITE(7,*) WRITE(7,*)'SY = SUM OF SQUARES FOR PRESENT PARAMETER VALUES' WRITE(7,*)'SYP = SUM OF SQUARES FOR GAUSS PARAMETER VALUES, SHOULD 1 BE SMALLER THAN SY' WRITE(7,*)' SYP DECREASES TOWARD A POSITIVE CONSTANT’ WRITE(7,*)'G = MEASURE OF THE SLOPE, SHOULD BECOME SMALLER AS lITERATIONS PROCEED' 18 19 99 c _-- CCCC 20 29 30 4o 50 41 51 52 139 WRITE(7,*)' G SHOULD APPROACH ZERO AT CONVERGENCE' WRITE(7,*)'H - FRACTION OF THE GAUSS STEP, AS GIVEN BY THE lBOX-KANEMASU METHOD' WRITE(7,*) WRITE(7,*) DO 18 IL=1,NP BS(IL)-B(IL) CG(IL) - 0 CONTINUE DO 19 IP=1,NP XTY(IP)=0.0D+0 DO 19 KP=1,NP P(KP,IP) = PS(KP,IP) XTX(IP,KP)=0.0D+0 CONTINUE I - 0 MAX - 0 MAX = MAX + l START BASIC LOOP GIVES B(I) AND SY SY - 0.0D+0 DO 100 13=1,N I - I3 CALL MODEL CALL SENS CALL MODEL RISD - Y(I)-ETA SY - SY + RISD*RISD/SIGZ(I) SUMX- 0.0D+O DO 20 K=I,NP XTY(K)-XTY(K)+Z(K)*RISD/$IG2(I) DO 20 L=1,NP SUMX= SUMX+ Z(L)*P(K,L)*Z(K) XTx(K,L)= XTX(K,L) + Z(L)*Z(K)/SIGZ(I) CONTINUE DELTA - SIGZ(I) + SUMX DO 29 JJ=1,NP A(JJ) = 0.0D+0 CONTINUE DO 30 JA=1,NP DO 30 KA-1,NP A(JA) - A(JA) + Z(KA)*P(JA,KA) CONTINUE CS - 0.0D+0 DO 40 JC=1,NP CS - CS + Z(JC)*(B(JC)-BS(JC)) CG(JC) s CG(JC) + 2(JC)*RISD/SIGZ(I) CONTINUE C - Y(I) - CS - ETA DO 50 IB-1,NP B(IB) - B(IB) + (A(IB)*C)/DELTA CONTINUE DO 41 ISV=1,NP DO 41 JSV-1,NP PSV(JSV,ISV) - P(JSV,ISV) CONTINUE DO 52 Iv-1,NP DO 52 IU=Iv,NP SUMP - 0.0D+0 DO 51 KP=1,NP DO 51 JP=1,NP IF(KP-IV.EQ.0.0R.JP-IU.EQ.0) GOTO 51 P501 - PSV(KP,JP)*PSV(IU,IV) P802 - PSV(IU,KP)*PSV(IV,JP) PSQ = PSQl - PSQZ IF(DABS(PSQl)+DABS(PSQZ).LT.1.D-15) THEN RP = PSQ * 1.D15 ELSE RP - PSQ / (DABS(PSQl)+DABS(PSQZ)) END IF RP a ABS(RP) RPP = RP - 1.00-12 IF(RPP.LE.0.0D+O) THEN PSQ - 0.0D+0 END IF SUMP = SUMP + Z(JP)*Z(KP)*PSQ CONTINUE P(IU,IV) = (P$V(IU,IV)*SIGZ(I)+SUMP)/DELTA CONTINUE 140 D0 53 IV=2,NP IVM = IV - 1 DO 53 IU - 1,IVM P(IU,IV)- P(IV,IU) 53 CONTINUE IF(IPRINT.GT.0) THEN IF(I.EQ.1) THEN WRITE(7,*) WRITE(7,*)'SEQUENTIAL ESTIMATES OF THE PARAMETERS GIVEN BELOW' WRITE(7,'(//,3X,"I",6X,"ETA",3X,"RES.",2X, lllB(1)II'7X'IOB(2)'0’7X'IIB(3)II'7x’llB(4)00)!) END IF C WRITE(7,'(I4,6E12.5)')I,ETA,RISD,(B(JC),JC=1,NP) WRITE(7,'(I3,F10.2,F8.3,5E11.4)')I,ETA,RISD,(B(JC),JC=1,NP) END IF 100 CONTINUE C --- END BASIC LOOP, GIVES B(I) AND SY C --- START BOX-KANEMASU MODIFICATION C C START BOX-KANEMASU MODIFICATION IF(MAX-1)104,104,103 103 ss-SY/2.0D+0 IF(ss-SYP)104,104,105 105 DO 210 IBS=1,NP B(IBS)= BSV(IBS) 210 CONTINUE WRITE(IOUT,212) 212 FORMAT(7X,'USE BSV(IBS)’) GOTO 211 104 CONTINUE DO 102 IBS=1,NP BSS(IBS)= BS(IBS) 102 CONTINUE ALPHA= 2.0D+0 AA= 1.1D+0 110 ALPHA= ALPHA/2.0D+0 DO 116 IBs-1,NP BS(IBS)- BSS(IBS) + ALPHA*( B(IBS)-BSS(IBS) ) BSV(IBS)= BS(IBS) 116 CONTINUE INDEX-0 G= 0.0D+O DO 115 IP=1,NP DELB= BS(IP)-BSS(IP) G- G + DELB*CG(IP) RATIO- DELB/( BSS(IP)+EPS ) RATIO= ABS(RATIO) IF(RATIO-EPSS)113,113,114 113 INDEX= INDEX+1 WRITE(IOUT,314) 314 FORMAT(7X,’MAX',8X,’NP’,5X,'INDEX',8X,’IP’) WRITE(7,'(7IlO)') MAX,NP,INDEX,IP 114 CONTINUE C WRITE(7,122) I,Y(I),ETA,RISD,Z(IP),XYP,DELB,SIG2(I) 115 CONTINUE SYP= 0.0D+0 DO 117 I3=1,N I=I3 CALL MODEL RISD= Y(I)-ETA SYP= SYP + RISD*RISD/SIGZ(I) 117 CONTINUE IF(NP-INDEX)106,106,107 106 H=1.0D+0 GOTO 132 107 CONTINUE SYN= SYP*0.999D+0 IF(SYN-SY)112,112,111 111 IF(ALPHA-0.01D+0)109,109,110 109 WRITE(7,108) ALPHA,SYP,SY 108 FORMAT(3X,'ALPHA TOO SMALL,ALPHA=',F12.6,2X,'SYP=',E15.6,2X, l'SY',E15.6) WRITE(7,1001) 1001 FORMAT(8X,'Z(1)’,10X,'Z(2)',10X,'Z(3)',10X,'Z(4)',10X,'Z(5)') 1002 FORMAT(6E13.4) DO 1003 I=1,N CALL SENS WRITE(7,1002) (Z(IBB),IBB=1,NP) 1003 CONTINUE GOTO 1000 141 112 CONTINUE SKSUM= SY - ALPHA*G*( 2.0D+0-1.0D+0/AA ) IF(SYP—SKSUM)131,131,130 130 H= ALPHA * ALPHA*G/( SYP-SY+2.0D+O*ALPHA*G ) GOTO 132 131 CONTINUE Ha ALPHA*AA 132 CONTINUE DO 118 IBN- 1,NP B(IBN)= BSS(IBN) + H * ( B(IBN)-BSS(IBN) ) 118 CONTINUE 211 CONTINUE WRITE(IOUT,121) WRITE(*,121) 121 FORMAT(5X,'MAX',10X,'H',13X,’G',12X, 1'5Y’,11X,'SYP') WRITE(7,122) MAX,H,G,SY,SYP WRITE(*,122) MAX,H,G,SY,SYP 122 FORMAT(I8,1F13.6,4E14.6) WRITE(7,'(10X,"B(",Il,") - ",E16.6)') (I,B(I),I=1,NP) WRITE(*,'(10X,"B(",Il,") = ",E16.6)') (I,B(I),I=1,NP) C END BOX-KANEMASU MODIFICATION WRITE(7,'(/,5X,"P(1,KP)",9X,”P(2,KP)",9X,"P(3,KP)",9X, 1"P(4,KP)",9X,"P(S,KP)")') DO 206 IP=1,NP WRITE(7,207) (P(IP,KP),KP=1,NP) 206 CONTINUE 207 FORMAT(5015.7) WRITE(7,135) 135 FORMAT(5X,'CORRELATION MATRIX') DO 136 IR=1,NP DO 136 IR2=1,IR AR= P(IR,IR) * P(IR2,IR2) R(IR,IR2)= P(IR,IR2)/SQRT(AR) 136 CONTINUE DO 137 IR-1,NP WRITE(7,'(5E15.7)') (R(IR,III),III=1,IR) 137 CONTINUE DO 126 IPS=1,NP PS(IPS,IPS)= (1.0E+7) * P(IPS,IPS) 126 CONTINUE WRITE(7,*)’XTX(I,K),K=1,NP' DO 220 K=1,NP 220 WRITE(7,'(SE15.7)’)(XTX(K,III),III=1,NP) WRITE(7,*)'XTY(I),I=1,NP, WHERE Y IS RESID’ WRITE(7,’(5E15.7)')(XTY(I),I=1,NP) 127 FORMAT(3X,'IPS=',IQ,3X,’PS(IPS,IPS)=',DlS.8) WRITE(7,*)'XTY(I),I=1,NP, Y IS Y, NOT RESID' WRITE(7,'(5E15.7)')(SUM(I),I=1,NP) Do 119 IP=1,NP XTY(IP)=0.0D+0 DO 119 KP=1,NP P(IP.KP)- PS(IP,KP) XTX(IP,KP)=0.0D+0 119 CONTINUE DO 120 IP=1,NP BS(IP)= B(IP) CG(IP)= 0.0D+0 120 CONTINUE WRITE(7,314) WRITE(7,'(7I10,4F10.4)') MAX,NP,INDEX,IP IF(NP-INDEX)101,101,123 123 CONTINUE M=ITMAX IF(MAX-M)99,99,101 101 CONTINUE IF(IPRINT)133,133,134 133 IPRINT=IPRINT+1 GOTO 99 134 CONTINUE C 1000 CONTINUE CLOSE(IIN) CLOSE (IOUT) C C********************************************‘k‘k*‘k‘k**************‘k*c C C CECCCCCCCC ERROR MESSAGES BLOCK 0900 C C C C 142 C********i**itiiiit*******ii*i************t***********************C C C CFCCCCCCCC FORMAT STATEMENTS BLOCK 9000 C C C C c*******t**********iiii**********t***************************i****C C STOP END SUBROUTINE MODEL C THIS SUBROUTINE IS FOR CALCULATING ETA, THE MODEL VALUE IMPLICIT REAL*8 (A-H,O-Z) DIMENSION T(500,5),Y(500),SIGZ(500),B(5),Z(5),BET(50,2), +A(5),BS(5),VINV(5,5),EXTRA(20) DIMENSION P(5,5),PS(5,5),SUM(5) COMMON T,N,Z,BS,I,ETA,PS,P,B,A,Y,SIGZ,MODL,VINV,NP,EXTRA COMMON/MOD/AA,TL,SUM,BET,IH,CONST C WRITTEN BY JAMES V. BECK PI=4.0D+0*DATAN(1.0D+0) C IF(MODL .EQ. 1) GOTO 800 800 CONTINUE TR=T(I,1)/EXTRA(2) ETA=BS(1)+BS(2)*EXTRA(1)*(1.0D+0-TR*TR) 1000 CONTINUE C WRITE(*,*)'I,T(I,1),ETA,Z(1)',I,T(I,1),ETA,Z(1) RETURN END SUBROUTINE SENS C THIS SUBROUTINE IS FOR CALCULATING THE SENSITIVITY COEFFICIENTS IMPLICIT REAL*8 (A-H,O-Z) DIMENSION T(500,5),Y(500),SIGZ(500),B(5),BET(50,2), +Z(5),A(5),BS(5),VINV(5,5),EXTRA(20) DIMENSION P(S,S),PS(5,5),SUM(5) COMMON T,N,2,85,I,ETA,PS,P,B,A,Y,SIGZ,MODL,VINV,NP,EXTRA COMMON/MOD/AA,TL,SUM,BET,IH,CONST PI=4.0D+0*DATAN(1.0D+O) z(1)=1.0D+0 TR=T(I,1)/EXTRA(2) Z(2)=EXTRA(1)*(l.0D+0-TR*TR) DO 312 IPP=1,NP 312 SUM(IPP)-0.0D+0 313 CONTINUE 800 CONTINUE C IF(I .LT. N)GOTO 2000 DO 1001 JPP-1,NP C TZ=? TRY ETA FOR NOW TZ=ETA 1001 SUM(JPP)=SUM(JPP)+Z(JPP)*(Y(I)-TZ)/SIG2(I) 2000 CONTINUE RETURN END 143 Appendix D. NLIN Output File for Experiment #5 BEGIN LISTING INPUT QUANTITIES BLOCK 1 N I NO. DATA POINTS, NP I NO. PARAMETERS NT I NO. OF INDEPENDENT VARIABLES ITMAX I MAXIMUM NO. OF ITERATIONS MODEL I MODEL NUMBER, IF SEVERAL MODELS IN SUBROUTINES: MODEL AND SENS IPRINT I 1 FOR USUAL PRINTOUTS, 0 FOR LESS N NP NT ITMAX MODEL IPRINT 121 2 1 5 l 1 BLOCK 2 B(1),B(2),..,B(NP) ARE INITIAL PARAMETER ESTIMATES B(1) = .27SOOE+02 8(2) = .40000E-02 BLOCK 3 J = DATA POINT INDEX, Y(J) I MEASURED VALUE SIGMA(J) = STANDARD DEVIATION OF Y(J) T(J,1) I FIRST INDEPENDENT VARIABLE J Y(J) SIGMA(J) T(J,1) T(J,2) 1 27.55979 1.00000 -1.00000 2 27.55979 1.00000 -.98333 3 27.59168 1.00000 -.96667 4 27.71942 1.00000 -.95000 5 27.81519 1.00000 -.93333 6 28.10010 1.00000 -.91667 7 28.22287 1.00000 -.90000 8 28.28427 1.00000 -.88333 9 28.13077 1.00000 -.86667 10 28.06940 1.00000 -.85000 11 28.19217 1.00000 —.83333 12 28.40708 1.00000 -.81667 13 28.56055 1.00000 -.80000 14 28.71405 1.00000 -.78333 15 28.86878 1.00000 -.76667 16 28.93265 1.00000 -.75000 17 29.02844 1.00000 -.73333 18 29.09094 1.00000 -.71667 19 28.99649 1.00000 -.70000 20 28.99649 1.00000 -.68333 21 29.18421 1.00000 -.66667 22 29.33969 1.00000 -.65000 23 29.46405 1.00000 -.63333 24 29.52625 1.00000 -.61667 25 29.46405 1.00000 -.60000 26 29.43295 1.00000 -.58333 27 29.49515 1.00000 -.56667 28 29.46405 1.00000 -.55000 29 29.84625 1.00000 -.53333 30 30.23493 1.00000 -.51667 31 30.39688 1.00000 -.50000 32 30.20255 1.00000 -.48333 33 30.04059 1.00000 -.46667 34 29.91104 1.00000 -.45000 35 30.23493 1.00000 -.43333 36 30.42798 1.00000 -.41667 37 30.45908 1.00000 -.40000 38 30.45908 1.00000 -.38333 39 30.52127 1.00000 -.36667 40 30.49017 1.00000 -.35000 41 30.55237 1.00000 -.33333 42 30.67676 1.00000 -.31667 43 30.67676 1.00000 -.30000 44 30.67676 1.00000 -.28333 1 1 l 1 1 1 1 l 1 1 l 1 1 1 1 1 BLOCK 4 IEXTRA I NO. OF EXTRA(I) PARAMETERS, 06 07 08 09 10 11 12 13 14 15 16 17 18 19 20 21 30.67676 30.67676 30.70783 30.77002 30.83222 31.01877 31.01877 30.86328 30.67676 30.55237 30.58344 30.83222 30.95661 30.86328 30.61453 30.61453 30.61453 30.67676 30.70783 30.73892 30.83222 30.83222 30.80112 30.64566 30.67676 30.77002 30.89441 31.04987 31.04987 30.86328 30.70783 30.61453 30.67676 30.73892 30.73892 30.64566 30.58344 30.45908 30.39688 30.52127 30.55237 30.49017 30.49017 30.13776 29.91104 29.97580 30.10538 30.10538 29.94342 29.81387 29.78146 29.74909 29.71668 29.71668 29.74909 29.68430 29.61951 29.58844 29.49515 29.37079 29.21530 29.09094 28.86878 28.65268 28.37637 28.25357 28.22287 28.28427 28.13077 28.03870 27.97482 28.03870 28.10010 28.13077 27.97482 27.75134 27.49591 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 1.00000 144 -.26667 -.25000 -.23333 -.21667 -.20000 -.18333 -.16667 -.15000 -.13333 -.11667 .10000 .08333 .06667 .05000 .03333 .71667 .73333 .75000 .76667 .78333 .80000 .81667 .83333 .85000 .86667 .88333 .90000 .91667 .93333 .95000 .96667 .98333 1.00000 0 IF NONE 145 IEXTRA = 2 BLOCK 5 EXTRA(I),... ARE EXTRA CONSTANTS USED AS DESIRED EXTRA( 1) I 831.86000 EXTRA( 2) I 1.00000 END INPUT QUANTITIES - - BEGIN OUTPUT CALCULATIONS SY = SUM OF SQUARES FOR PRESENT PARAMETER VALUES SYP I SUM OF SQUARES FOR GAUSS PARAMETER VALUES, SHOULD BE SMALLER THAN SY SYP DECREASES TOWARD A POSITIVE CONSTANT G I MEASURE OF THE SLOPE, SHOULD BECOME SMALLER AS ITERATIONS PROCEED G SHOULD APPROACH ZERO AT CONVERGENCE H = FRACTION OF THE GAUSS STEP, AS GIVEN BY THE BOX-KANEMASU METHOD SEQUENTIAL ESTIMATES OF THE PARAMETERS GIVEN BELOW I ETA RES. 8(1) 8(2) 8(3) 8(4) 1 27.50 .060 .2756E+02 .4000E-02 2 27.61 -.050 .2751E+02 .39768-02 3 27.72 -.126 .2746E+02 .3921E-02 4 27.82 -.105 .2745E+02 .3883E-02 5 27.93 -.114 .2744E+02 .3844E-02 6 28.03 .069 .2746E+02 .39748-02 7 28.13 .091 .2747E+02 .4105E-02 8 28.23 .053 .2747E+02 .4171E-02 9 28.33 -.197 .2747E+02 .3973E-02 10 28.42 -.354 .2747E+02 .3669E-02 11 28.52 -.325 .2748E+02 .3473E-02 12 28.61 -.201 .2748E+02 .34448-02 13 28.70 -.137 .274BE+02 .34858-02 14 28.79 -.072 .2747E+02 .35748-02 15 28.87 -.003 .27468+02 .3698E-02 16 28.96 -.023 .274SE+02 .3782E-02 17 29.04 -.010 .2744E+02 .3857E-02 18 29.12 -.027 .2744E+02 .3906E-02 19 29.20 -.201 .2744E+02 .3854E-02 20 29.27 -.277 .274SE+02 .3777E-02 21 29.35 -.164 .27468+02 .37708-02 22 29.42 -.082 .2745E+02 .38008-02 23 29.49 -.029 .2744E+02 .3848E—02 24 29.56 -.O36 .2744E+02 .38848-02 25 29.63 -.166 .2744E+02 .38708-02 26 29.70 -.262 .2745E+02 .3827E-02 27 29.76 -.264 .2745E+02 .3792E-02 28 29.82 -.357 .2747E+02 .3737E-02 29 29.88 -.035 .2746E+02 .378OE-02 30 29.94 .296 .2743E+02 .3901E—02 31 30.00 .401 .2740E+02 .4031E-02 32 30.05 .152 .2739E+02 .4084E-02 33 30.10 -.062 .2739E+02 .40828-02 34 30.15 -.243 .274OE+02 .40428-02 35 30.20 .032 .2740E+02 .4062E-02 36 30.25 .178 .2739E+02 .41078-02 37 30.30 .164 .2738E+02 .4144E-02 38 30.34 .121 .2737E+02 .4168E-02 39 30.38 .141 .2736E+02 .41928-02 40 30.42 .070 .2736E+02 .4203E-02 41 30.46 .095 .27368+02 .421SE-02 42 30.49 .183 .2735E+02 .4239E-02 43 30.53 .149 .273SE+02 .42558-02 44 30.56 .116 .2735E+02 .4264E-02 45 30.59 .086 .2734E+02 .4269E-02 46 30.62 .057 .2734E+02 .4270E-02 47 30.65 .062 .2734E+02 .4270E—02 48 30.67 .099 .2734E+02 .427SE-02 49 30.69 .138 .2734E+02 .4283E-02 50 30.72 .303 .2733E+02 .43088-02 51 30.74 .284 .2733E+02 .43298-02 52 30.75 .111 .2733E+02 .433OE-02 53 30.77 -.092 .2733E+02 .4313E-02 54 30.78 -.230 .2734E+02 .4284E-02 55 30.79 -.211 .2735E+02 .4259E-02 56 30.80 .028 .273SE+02 .42568-02 57 30.81 .144 .2735E+02 .4263E-02 58 59 60 61 62 63 65 66 67 68 70 71 72 73 74 75 76 77 78 79 80 82 83 84 86 87 89 90 91 92 93 94 95 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 .4726766D-01 -.70922OSD-04 CORRELATION MATRIX 30.82 .044 30.82 - 209 30.83 -.212 30.83 -.213 30.83 - 150 30.82 -.116 30.82 -.080 30.81 .020 30.80 .028 30.79 .007 30.78 -.136 30.77 -.092 30.75 .017 30.74 .159 30.72 .334 30.69 .356 30.67 .192 30.65 .062 30.62 -.005 30.59 .086 30.56 .179 30.53 211 30.49 .152 30.46 .126 30.42 .039 30.38 .017 30.34 .183 30.30 .257 30.25 .240 30.20 .288 30.15 - 016 30.10 -.192 30.05 -.074 30.00 .110 29.94 .166 29.88 .062 29.82 -.007 29.76 022 29.70 .054 29.63 .087 29.56 .155 29.49 .256 29.42 .263 29.35 .271 29.27 .315 29.20 .298 29.12 .252 29.04 .177 28.96 .135 28.87 -.003 28.79 -.133 28.70 - 322 28.61 -.355 28.52 -.294 28.42 -.139 28.33 -.197 28.23 -.192 28.13 -.157 28.03 .007 27.93 .171 27.82 .306 27.72 .257 27.61 .141 27.50 -.004 MAX H 1 1.006253 8(1) I 8(2) = P(1,KP) -.70922050-04 .1289619D-06 .1000000E+01 -.9083821E+00 .1000000E+01 XTX(I,K),K=1,NP .1210000E+03 .6654418E+05 .6654418E+05 .4428743E+08 XTY(I),I=1,NP, WHERE Y IS RESID .2434174E+01 .2460668E+04 146 .2735E+02 .4261E-02 .2735E+02 .4240E-02 .2736E+02 .4221E-02 .2737E+02 .4203E-02 .2737E+02 .4190E-02 .2737E+02 .4181E-02 .2737E+02 .4174E-02 .2737E+02 .41748-02 .2737E+02 .41758-02 .2737E+02 .4174E-02 .27388+02 .4166E-02 .2738E+02 .41608-02 .2738E+02 .41618-02 .2738E+02 .4168E-02 .2737E+02 .4183E-02 .2737E+02 .4197E-02 .2737E+02 .42048-02 .2737E+02 .4205E-02 .2737E+02 .4204E-02 .2737E+02 .4206E-02 .2737E+02 .42118-02 .27368+02 .4217E-02 .27368+02 .4221E-02 .27368+02 .4223E-02 .2736E+02 .4223E-02 .27368+02 .4223E-02 .2736E+02 .42268-02 .2736E+02 .4230E-02 .27368+02 .4233E-02 .2737E+02 .4236E-02 .2737E+02 .42368-02 .27368+02 .42358-02 .273GE+02 .4234E-02 .2736E+02 .4234E-02 .2737E+02 .42348—02 .2737E+02 .4234E-02 .2737E+02 .4234E-02 .2737E+02 .4234E-02 .2737E+02 .4233E-02 .2737E+02 .42318-02 .2737E+02 .42288-02 .2738E+02 .42218-02 .2739E+02 .42148-02 .2740E+02 .42068-02 .2741E+02 .41958-02 .274ZE+02 .4183E-02 .2742E+02 .4173E-02 .2743E+02 .4165E-02 .2744E+02 .41588-02 .2744E+02 .4158E-02 .2743E+02 .41648-02 .274ZE+02 .41818-02 .2741E+02 .4199E-02 .2739E+02 .42148-02 .2739E+02 .4219E-02 .2738E+02 .4227E-02 .2738E+02 .4235E-02 .273SE+02 .42408-02 .273BE+02 .42338-02 .2739E+02 .4215E-02 .274lE+02 .4187E-02 .2743E+02 .4164E-02 .2744E+02 .4149E-02 .2744E+02 .4145E-02 G SY .211317E+00 .387968E+01 .274402E+02 .414560E-02 P(2.KP) P(3oKP) SYP .366705E+01 P(4.KP) P(5,KP) XTY(I),I=1,NP, Y IS Y, NOT RESID -.409000OE-02 SEQUENTIAL ESTIMATES OF THE PARAMETERS GIVEN BELOW HFJFIHrJFJH (hUhthNFACDwCD~JanhHAN)H I MAX 1 ETA 27.44 27.55 27.67 27.78 27.88 27.99 28.10 28.20 28.30 28.40 28.49 28.59 28.68 28.77 28.86 28.95 29.03 29.12 29.20 29.28 29.36 29.43 29.51 29.58 29.65 29.72 29.78 29.85 29.91 29.97 30.03 30.08 30.14 30.19 30.24 30.29 30.34 30.38 30.43 30.47 30.51 30.54 30.58 30.61 30.64 30.67 30.70 30.73 30.75 30.77 30.79 30.81 30.83 30.84 30.85 30.86 30.87 30.88 30.88 30.89 30.89 30.89 30.88 30.88 30.87 30.86 30.85 30.84 30.83 30.81 30.79 .0000000E+00 NP INDEX 2 0 RES. .120 .006 -.075 -.057 -.069 .109 .127 .086 -.168 -.328 -.302 -.182 -.121 -.059 .007 -.016 -.006 -.027 -.202 -.282 —.172 -.092 -.041 -.051 -.183 -.282 -.286 -.381 -.062 .267 .370 .119 -.097 -.279 -.006 .138 .122 .077 .096 .024 .047 .134 .098 .065 .033 .004 .007 .043 .081 .246 .226 .052 -.151 -.289 -.271 -.033 .083 -.017 -.270 -.273 -.274 -.211 -.177 —.141 -.041 -.033 -.053 -.196 -.151 -.041 .101 8(1) .2756E+02 .27563+02 .27SSE+02 .27538+02 .2751E+02 .2747E+02 .2744E+02 .2743E+02 .2747E+02 .2752E+02 .2754E+02 .2753E+02 .27SZE+02 .27SOE+02 .27488+02 .274GE+02 .274SE+02 .2744E+02 .274SE+02 .27468+02 .2746E+02 .27462+02 .27458+02 .2744E+02 .2744E+02 .27453+02 .27463+02 .2747E+02 .274GE+02 .2743E+02 .27403+02 .273QE+02 .2739E+02 .274OE+02 .27408+02 .273SE+02 .27388+02 .2737E+02 .27362+02 .27368+02 .2736E+02 .273SE+02 .2734E+02 .2734E+02 .273dE+02 .2734E+02 .27348+02 .2734E+02 .2734E+02 .2733E+02 .27323+02 .273ZE+02 .2733E+02 .2734E+02 .273SE+02 .273SE+02 .2734B+02 .2734E+02 .273SE+02 .2736E+02 .27368+02 .2737E+02 .2737E+02 .2737E+02 .2737E+02 .2737E+02 .2737E+02 .273BE+02 .27388+02 .27388+02 .273SE+02 147 IP 3 8(2) .4146E-02 .8494E-05 .58508-03 .1882E-02 .2492E-02 .3844E-02 .4442E-02 .45468-02 .3930E-02 .3288E-02 .3009E-02 .3061E-02 .32018-02 .3383E-02 .35858-02 .3714E-02 .3819E-02 .3885E-02 .38258-02 .3739E-02 .3735E-02 .3774E-02 .3830E-02 .3872E-02 .3857E-02 .3812E-02 .3775E-02 .3718E—02 .3765E-02 .3895E-02 .40338-02 .4088E-02 .4086E-02 .4044E-02 .4065E-02 .4112E-02 .4149E-02 .4174E-02 .4199E-02 .4209E-02 .4222E-02 .42468-02 .4262E-02 .4272E-02 .4276E-02 .4276E-02 .4277E-02 .42818-02 .4290E-02 .43158-02 .43358-02 .4337E-02 .4319E-02 .4289E-02 .4264E-02 .4261E-02 .4267E-02 .4266E-02 .4244E-02 .4225E-02 .4206E-02 .4193E-02 .41838-02 .4177E-02 .4177E-02 .4177E-02 .4177E-02 .4168E-02 .41638-02 .4163E-02 .4170E-02 8(3) 8(4) XTY(I),I=1,NP, WHERE Y IS RESID -.1530085E-01 -.6287375E+01 XTY(I),I=1,NP, Y IS Y, NOT RESID .55739718-01 .0000000E+00 MAX NP 2 2 2 INDEX 148 72 30.77 .277 .2737E+02 .4185E-02 73 30.75 .299 .2737E+02 .4200E-02 74 30.73 .136 .2737E+02 .4207E-02 75 30.70 .007 .2736E+02 .4208E-02 76 30.67 -.059 .2737E+02 .4207E-02 77 30.64 .033 .273GE+02 .4209E-02 78 30.61 .127 .27368+02 .4214E-02 79 30.58 .161 .27368+02 .42208-02 80 30.54 .103 .2736E+02 .4223E-02 81 30.51 .078 .273GE+02 .42268-02 82 30.47 -.007 .2736E+02 .4226E-02 83 30.43 -.028 .2736E+02 .4226E-02 84 30.38 .139 .2736E+02 .4229E-02 85 30.34 .215 .2736E+02 .42338-02 86 30.29 .200 .2736E+02 .4236E-02 87 30.24 .249 .2736E+02 .4239E-02 88 30.19 -.053 .2736E+02 .4239E-02 89 30.14 -.227 .27368+02 .4238E-02 90 30.08 -.107 .2736E+02 .4237E-02 91 30.03 .079 .27368+02 .4237E-02 92 29.97 .137 .27368+02 .4237E-02 93 29.91 .036 .2736E+02 .4237E-02 94 29.85 —.032 .273SE+02 .4237E-02 95 29.78 .000 .2736E+02 .4237E-02 96 29.72 .034 .2737E+02 .4236E-02 97 29.65 .069 .2737E+02 .4234E-02 98 29.58 .139 .2737E+02 .4231E-02 99 29.51 .244 .2738E+02 .4224E-02 100 29.43 .253 .2739E+02 .4217E-02 101 29.36 .263 .2739E+02 .4208E-02 102 29.28 .310 .274OE+02 .4197E-02 103 29.20 .296 .2741E+02 .4186E-02 104 29.12 .253 .274ZE+02 .41758-02 105 29.03 .181 .2743E+02 .4167E-02 106 28.95 .142 .2743E+02 .416OE-02 107 28.86 .007 .2744E+02 .4160E-02 108 28.77 -.120 .2743E+02 .4166E—02 109 28.68 -.305 .274ZE+02 .4183E-02 110 28.59 -.335 .2740E+02 .4201E-02 111 28.49 -.271 .2739E+02 .4216E-02 112 28.40 -.113 .2739E+02 .4221E-02 113 28.30 -.168 .2738E+02 .42308-02 114 28.20 -.159 .273BE+02 .4237E-02 115 28.10 -.121 .2737E+02 .4242E-02 116 27.99 .048 .2738E+02 .42358-02 117 27.88 .215 .2739E+02 .4217E-02 118 27.78 .354 .274lE+02 .4189E-02 119 27.67 .309 .2743E+02 .4165E-02 120 27.55 .197 .2744E+02 .4150E-02 121 27.44 .056 .2744E+02 .41468-02 MAX NP INDEX IP 2 2 1 1 MAX NP INDEX IP 2 2 2 2 H G 1.000000 .2523258-05 8(1) .274399E+02 8(2) I .4145888-02 P(1.KP) P(2.KP) P(3.KP) .4758757D-01 -.7150281D-04 -.71502810-04 .1300165D-06 CORRELATION MATRIX .1000000E+01 -.90902788+00 .1000000E+01 XTX(I,K),K=1,NP .1210000E+03 .6654418E+05 .6654418E+05 .4428743E+08 SY .366704E+01 SYP .366704E+01 P(4.KP) P(5,KP)