A History of Engineering and Science in the Bell System

Total Page:16

File Type:pdf, Size:1020Kb

A History of Engineering and Science in the Bell System A History of Engineering and Science in the Bell System Physical Sciences (1925-1980) Prepared by Members of the Technical Staff, AT&T Bell Laboratories. S. Millman, Editor. AT&T Bell Laboratories Credits for figm·es taken from other than Bell System sources appear on page 641. Copyright c 1983 Bell Telephone Laboratories, Incorporated All rights r•eserved f-1( e ; '/C, 1-' l / 'i ·~­ ''' First Printing, 1983 International Standard Book Number: 0-932764-03-7 Library of Congress Catalog Card Number: 83-62738 Printed in the United States of America Contents Foreword xiii Acknowledgments xxiii Part I. Research in Physics Overview .. 1 1. Magnetism and Magnetic Resonance . 19 I. The Physics of Magnetic Solids, 19. Ferromagnetic Metals and Alloys, 20. Ferromagnetic Domains, 22. Magnetic Oxides­ Ferrimagnetic Garnets, 26. Magnetic Moments and Interatomic Magnetic Interactions, 31. II. Magnetic Resonance and Solid State Spectroscopy-The Gyrator and Paramagnetic Amplifier, 35. Nuclear Magnetic Resonance, 36. Electron Paramagnetic Resonance, 39. Ferromagnetic Resonance, 46. Electron Orbital Resonance, 50. Resonance Experiments in the Far-Infrared, 52. III. Mossbauer Spectroscopy, 53. Hyperfine Structure Studies in Magnetic Materials, 53. Layer-Structure Compounds, 57. Amorphous Materials, 58. Studies of Electroplating, 58. References, 60. 2. Semiconductor Physics and Electronics- The Transistor . 71 I. Semiconductor Research up to 1948-The Point-Contact Transistor, 72. II. The Junction Transistor and Other Semiconductor Amplifiers, 74. The p-n Junction, 74. p-n Junction Transistors, 74. Field Effect Transistors, 76. The Read Diode, 78. Acoustic-Wave Amplifiers, 79. III. The Bell Solar Photovoltaic Cell, 79. IV. Transport Properties, 80. Phonon Drag and Thermal Transport, 81. V. Semiconductor Spectroscopy, 83. Band Structure in Semiconductors, 83. Pair Spectra, 87. Light Emitting Diodes, 89. Thin Layers, 90. Deep Levels, 91. Electron-Hole Liquids, 92. VI. Molecular Beam Epitaxy, 93. VII. Semiconductor Research Supplement-The Story of the "Genesis of the Transistor," 96. "The Genesis of the Transistor," 97. J. B. Fisk's Letter to Ralph Bown, 101. Walter H. Brattain's Personal Reminiscences, Recorded by Brattain in 1975, 101. References, 102. v vi Engineering and Science in the Bell System 3. Surface Physics- Wave Nature of the Electron . 109 I. The Davisson-Germer Experiment, 109. Quotations from Davisson's Nobel Lecture, December 13, 1937, 111. Davisson's "Well-Known Accident," 112. Quotations from Karl K. Darrow's "The Scientific Work of C. J. Davisson," 112. Observation of Spin Polarization Effe·cts, 113. II. Electron Emission from Solids, 114. Primary Emission, 114. Secondary Emission, 115. Au~;er Electron Emission Spectroscopy of Solids, 115. Field Emission, 116. III. Semiconductor Surface Research During 1948-1960, 119. Surface Charge, Contact Potential, and Surface Voltage, 119. Surface Photovoltage and Surface State·s, 120. Semiconductors in an Electrolyltic Ambient, 122. IV. Modern Surface Research- Controlled Surface int Ultra-High Vacuum, 122. Surface Crystallography-Low Energy JBlectron Diffraction, 124. Surface Electronic Structure, 125. MultiJPl•e Experiments in One Apparatus, 131. References, 133. 4. Electronic Band Structu:rE~ of Metals ...... 139 I. Fermi Surfaces, 139. II. Cyclotron Resonance, 141. Ill. Hi~;h-Field Galvanomagnetic Effects, 143. IV. The Oscillatory Effects, 145. deHaas-vanAlphen Effect, 145:. Magnetothermal Effect, 146. Magnetoacoustic Effects, 147. V. Band Structure Calculations, 147. References, 147. 5. Quantum Electronics-The Laser ............ 151 I. Microwave Spectroscopy andl Masers, 151. II. Physical Priinciples and Conditions for Laser Actio1n ·-The He-Ne Laser, 152. Earlly Solid State Lasers, 156. Modes of Oscillation in the Laser Resonating System, 158. Mode Locking and Pulse Generation, 161. Temporal Coherence of Laser Radiation, 163. III. La:sers for Optical Communication, 164. The Heterojunction Semiconductor Laser, 165. HeterostructurE! Lasers and Optical Fibers, 167. IV. Latiiers for Industrial Applic:ation!O- The 168. Yttrium Aluminum Garnet (YAG) Laser, 172. V. C02 Laser, Other Laser Types, 172. Lasers Based on Atomic Transitions, 172. Lasers Involving Vibrational-:Rotational Molecular Transitions, 173. Optically Pumped Molecular Ga:s l.asers, 174. Dye Lasers, 174. Color­ Center Lasers, 175. VI. Laserli in Physical Research, 176. High­ Resolution Spectroscopy, 176. R~tman and Brillouin Scattering, 178. Coherent Optical Effects, 181. Radiation Pressure and Optical Levitation, 184. VII. Nonlim~a1r Optics, 185. Second Hatrmonic Generation, 186. Optical Parametric Amplification, 192. Stimulated Raman Scattering and Lasers, 19':1,. References, 196. Contents vii 6. Atoms, Molecules, and Plasmas ............ 211 I. Atomic and Molecular Physics, 211. Lamb Shift in Hydrogenic Ions, 211. The Hydrogen Molecular Ion Hyperfine Structure, 212. Optical Pumping of States with Nonzero Orbital Angular Momentum, 213. Radiation from Low-Energy, Ion-Atom, and Ion-Molecule Collisions, 215. Anticrossing Spectroscopy, 215. Laser Spectroscopy, 218. Opto­ Acoustic Spectroscopy of Gases and Pollution Detection, 221. II. Plasma Physics, 223. Gas Discharges and the Arc Plasma, 224. The Collective Modes of Plasmas, 230. Plasma Instabilities, 237. Highly Nonlinear Plasma States, 242. III. Molecular Biophysics, 246. Nuclear Magnetic Relaxation of Water Protons in DNA, 247. Optical Studies of DNA and Other Molecules, 247. Physical Transport of Biomolecules, 249. Nuclear Magnetic Resonance, 249. Paramagnetic Resonance in Metalloenzymes, 251. Translation of the Genetic Code, 252. Extended X-Ray Absorption Spectroscopy in Biomolecules, 253. Fluorometric Screening Test for Lead Poisoning, 254. References, 258. 7. Astrophysics and Magnetospheric Physics- Cosmic Background Radiation . 269 I. Astrophysics, 269. Radio Astronomy-Early Observation of Galactic Radio Noise, 270. Microwave Background Noise Studies-Impact on Cosmology, 271. Application of Sensitive Receivers to the Study of Molecules in Interstellar Space, 274. Statistical Study of Galaxies, 276. Gravity Waves, 277. Gamma-Ray Line Astronomy, 277. The Indium Solar Neutrino Spectrometer, 278. II. The Magnetosphere, 279. Study of Electrons and Protons in the Van Allen Belts with Detectors in the Telstar Satellite, 279. Outer Zone Studies with Synchronous Altitude Satellites, 280. Effect of Solar Flares on Particles in Interplanetary Space, 281. Ground-Based Magnetometers in Antarctica and at High Northern Latitudes, 282. References, 284. 8. Ion Beams, X-Rays, Electrons, and Neutrons in Solids-Channeling and Ion Implantation ... 289 I. Particle Detectors, Nuclear Physics, and Ion Beam Research, 289. Semiconductor Particle Detectors, 290. The Rutgers University-Bell Laboratories Accelerator Laboratory, 294. Particle Channeling, 298. Ion Implantation, 305. Ion Scattering, 310. Sputtering, 314. II. X-Ray Scattering and Spectroscopy, 317. X-Ray Diffraction, 317. Inelastic X­ Ray Spectroscopy, 319. Extended X-Ray Absorption Fine Structure Spectroscopy, 325. III. X-Ray Photoelectron Spectroscopy, 328. Ionic and Covalent Bonding, 328. Core Electron and Conduction Electron Spectroscopy, 329. Rare Earth Ion Spectroscopy. 330. Application to viii En~ri111eering and Science in the BeU System Surface Studies, 330. IV. Neutr•3n. Scattering, 331. Phase Transition in Magnetic Systems, 333. Electronk Structure of Magnetic Systems, 334. References, 335. 9. Ordered Phases of Matte1r and Phase Transitions . • • . 0 .347 I. Superconductivity-Superc(Jinductive Tunneling, 347. Contri­ butions to Fundamental The011y,. 348. Quantized Flux Lin•es, 349. Strong Coupling Theory, 349. The Proximity Effect, 351. The Josephson Effect and Tunnel Ju.ndions, 351. II. Ferroelectricity, 354. BaTi03 Experiments, 355. Ferroelectric Domains in Triglycine Sulfate and Guanidine Aluminum Sulfate Hexahydrate, 357. Lattice Dynamics and Ferroelectricity, 358. III. Liquid Crystals, 359. The Nematic Phase, 359. The Smectic Phase, 359. The Cholesteric Phase, 360. Liquid Crystal Display Devices, 361. IV. Physics at Low Temperatures, 361. Vortex Rings in Superfluid Helium, 363. Phonons in Helium, 364. Surface Electrons on Sup•er:fluid Helium, 364. Superfluiidity in 3He, 367. V. Physics at High :Pressures, 370. Phase Diagrams in Electronic Transitions, 370. Metal-Insulator Transitions, 371. Transitions in Mixed-Valence Compounds, 372. VI. Phase Transitions and Critical Phenomena, 372. Calorimetric Investigations, 373. The Effect of Dimensionality of Space, 373. Critical Dynamic:s, 374. Structural Transitions, 374. Impad on Other Fields, 376. Reft~rences, 377. 10. The Role of Theoretical P'hysics at Bell Laboratories . .. .. .. 387 I. Nature of Theoretical Physi.cs, 387. II. The Buildup of the Theoretical Physics Effort, 389. Il[I. The Increasing Role of Quantum Mechanics-Physics of Ordered States, 390. IV. Extension to Localized States and Random Systems, 392. V. Many-Body Theory-­ Broken Symmetry and Superconductivity, 395. VI. Statistical Mechanics and Phase Transitions, 397. VII. Concluding Contmenbl, 398. References, 398. Part II. Resear•ch in Materials Overview . • . 40~l 11. Semiconductors-Silicon, Germanium, and III-V Compounds .••.................. 411 I. Compound Semiconductors for Thermistors and Varistor's, 411.. Thermistors, 412. Varistors, 413. II. Silicon and Germanium in Contents ix Point-Contact Rectifiers, 414. Silicon Rectifiers, 415. Germanium Rectifiers, 416. III. Silicon and Germanium Studies
Recommended publications
  • What Made Bell Labs Special? Ley in Recent Years, the High Pay and Excellent Working Conditions at Bell Labs Attracted Many Who Might Look Elsewhere Today
    physicsworld.com Christmas books Andrew Gelman What made Bell Labs special? ley in recent years, the high pay and excellent working conditions at Bell Labs attracted many who might look elsewhere today. Second, there was nothing to do at the labs all day but work. I have known lots of middle-aged profes- sors who don’t spend much time teaching but don’t do any research either. At Bell Labs it was harder to be deadwood. Located as it was in the middle of nowhere, the Murray Hill campus was not a place to relax, and if you were going into the lab every weekday anyhow, you might as well work – there was nothing better to do. Several researchers, including Shannon and Shockley, had sharp mid-career productivity declines – but after they left Murray Hill. In my own experience working at Bell Labs for three summers during Bell Laboratories/Alcatel-Lucent USA/AIP Emilio Segrè Visual Archives, Hecht Collection the 1980s, I vividly recall a general feeling of comfort and well-being, Innovation central Bell Labs was a legendary place, an Idea Factory. I say this not at all as a along with the low-level intensity Ali Javan (left) and industrial lab in the outer suburbs of criticism of its author, the journalist that comes from working eight-hour Donald R Herriott New York where thousands of scien- Jon Gertner; rather, there was just so days, week after week after week. work with a helium- tists, working nine to five, changed much going on at Bell that it cannot I did the research underlying my neon optical gas the world’s technological history.
    [Show full text]
  • Controlling Phonons and Photons at the Wavelength-Scale: Silicon Photonics Meets Silicon Phononics
    1 Controlling phonons and photons at the wavelength-scale: silicon photonics meets silicon phononics AMIR H. SAFAVI-NAEINI1,D RIES VAN THOURHOUT2,R OEL BAETS2, AND RAPHAËL VAN LAER1,2 1Department of Applied Physics and Ginzton Laboratory, Stanford University, USA 2Photonics Research Group (INTEC), Department of Information Technology, Ghent University–imec, Belgium .Center for Nano- and Biophotonics, Ghent University, Belgium Compiled October 9, 2018 Radio-frequency communication systems have long used bulk- and surface-acoustic-wave de- vices supporting ultrasonic mechanical waves to manipulate and sense signals. These devices have greatly improved our ability to process microwaves by interfacing them to orders-of- magnitude slower and lower loss mechanical fields. In parallel, long-distance communications have been dominated by low-loss infrared optical photons. As electrical signal processing and transmission approaches physical limits imposed by energy dissipation, optical links are now being actively considered for mobile and cloud technologies. Thus there is a strong driver for wavelength-scale mechanical wave or “phononic” circuitry fabricated by scalable semiconduc- tor processes. With the advent of these circuits, new micro- and nanostructures that combine electrical, optical and mechanical elements have emerged. In these devices, such as optomechan- ical waveguides and resonators, optical photons and gigahertz phonons are ideally matched to one another as both have wavelengths on the order of micrometers. The development of phononic circuits has thus emerged as a vibrant field of research pursued for optical signal pro- cessing and sensing applications as well as emerging quantum technologies. In this review, we discuss the key physics and figures of merit underpinning this field.
    [Show full text]
  • Robotics/Principles of Technology (Semester Course)
    Robotics/Principles of Technology (Semester Course) Course Description Robotics/Principles of Technology is aligned with the NGSS standards and was developed based upon the interest of students. Through the use of technology, engineering and robotics, the course stresses problem‐solving skills in a real world setting. Students will be given tasks and will need to design and construct various projects. Students will work independently as well as in pairs, small groups and large groups. Both verbal and written communication of ideas will be emphasized. The course is designed to motivate the student of all ability levels to participate in real‐world scenarios utilizing engineering and robotic concepts to problem solve through hand on activities. Robotics/Principles of Technology encompass STEM principles in a variety of in‐class and out‐of‐class learning activities designed to teach the student about careers in technology, engineering, robotics and science. Suggested Course Sequence: History of Robotics (2 weeks) Careers in STEM (1 week) Design in Engineering & Technology (2‐3 weeks) Getting Started in Robotics (3‐4 weeks) Space Exploration Robotics (6‐7 weeks) Design & Build a Robot (3 weeks) ENGAGING STUDENTS • FOSTERING ACHIEVEMENT • CULTIVATING 21st CENTURY GLOBAL SKILLS Unit Overview Content Area: Robotics/Principles of Technology Unit Title: History of Robots Grade Level: 11‐12 Unit Summary: This unit will cover the development of robotics over time. Students will research how robotics has evolved over time. Interdisciplinary Connections: History 6.1.4.C.17 6.1.4.C.16 English RT.11‐12.9 RT.11‐12.10 WHST.11‐12.2B Technology 8.1.12.E.1 8.2.12.A.3 8.2.12.C.2 21st Century Themes and Skills: ‐ CRP2 Apply appropriate academic and technical skills.
    [Show full text]
  • G.W.A.T.T. (Global 'What If' Analyzer of Network Energy Consumption)
    G.W.A.T.T. New Bell Labs application able to measure the impact of technologies like SDN & NFV on network energy consumption WHITE PAPER Increased energy consumption is a key challenge for the Information and Communications Technologies (ICT) industry. Network energy bills represent more than 10 percent of operators’ operational expenses. With the advent of the Internet of Things era, and the inexorable consumption of video and cloud services promising to drive massively increased traffic across networks, it is even more important for operators to have a complete view of the energy impact of different technology and architectural evolution options. G.W.A.T.T. (Global “What if” Analyzer of NeTwork Energy ConsumpTion) has been built to allow operators and industry stakeholders to better understand these challenges. This application visualizes the current and future communication networks and forecasts key trends in energy consumption, energy efficiency, cost and carbon emissions based on a wide variety of traffic growth scenarios and technology evolution choices. It is intended as a mind-sharing tool to grasp the importance of the energy challenge and how innovation and new technologies can help address these issues in the future. EXECUTIVE SUMMARY The explosion of the Internet traffic volume resulting from both the worldwide broadband subscriber base extension and the increasing number and diversity of available applications and services require a relentless deployment of new technologies and infrastructures to deliver the expected user-experience. At the same time, it also raises the issue of the energy consumption and energy cost of the Internet and more generally of the Information and Communication Technologies (ICT).
    [Show full text]
  • DTMF Control System
    P a g e | 38 Vol. 10 Issue 11 (Ver. 1.0) October 2010 Global Journal of Computer Science and Technology A2Z Control System- DTMF Control System Er. Zatin Gupta1, Payal Jain2 , Monika3 GJCST Classification (FOR) H.4.3 Abstract-Dual Tone Multi Frequency (DTMF) technique for c) Microcontroller (At89s52) controlling the domestic and industrial appliances is being presented in this paper. A simple mobile phone which works on Microcontroller is the control unit of this system. We have DTMF tone, used to control the domestic as well as industrial used AT89S52. It is low power, high performance CMOS 8- electrical appliances which with the control system which we Bit controller with 4K bytes of ROM and 128 bytes of RAM. have designed here for experimental study. In recent state of affairs, domestic, military and industrial applications use this d) Dtmf Signal technique because it can be operated from remote location. Radio frequency (RF) is also used for wireless communication but DTMF is most widely known method of Multi Frequency DTMF is an alternate for RF. Mobile phone is used to send the Shift Keying (MSFK) data transmission technique. DTMF DTMF code from remote location to the control system. The was developed by Bell Labs to be used in the telephone blocks of system are mobile phone, Microcontroller (AT89S52), system. Most telephones today uses DTMF dialing (or “tone” DTMF Decoder (MT8870D), Relays and power supply. This dialing). paper shows the working areas where the system is applicable and how it has advantages over RF. 1209 1336 1477 1633 Hz Hz Hz Hz I.
    [Show full text]
  • Electrical Engineering Engineering
    College of Electrical Engineering Engineering The undergraduate electrical engineering degree program seeks to produce gradu- Second Semester ates who are trained in the theory and practice of electrical and computer engineering EE 468G Introduction to Engineering Electromagnetics ........................................ 4 and are well prepared to handle the professional and leadership challenges of their Elective EE Laboratory [L] ...................................................................................... 2 careers. The program allows students to specialize in high performance and embed- Engineering/Science Elective [E] ............................................................................ 3 ded computing, microelectronics and nanotechnology, power and energy, signal Technical Elective [T] ............................................................................................. 3 processing and communications, high frequency circuits and fields, and control UK Core – Citizenship - USA .................................................................................. 3 systems, among others. Senior Year Degree Requirements The following curriculum meets the requirements for a B.S. in Electrical Engineering, First Semester Hours provided the student satisfies UK Core requirements and graduation requirements EE/CPE 490 ECE Capstone Design I† ..................................................................... 3 of the College of Engineering. EE Technical Elective* ...........................................................................................
    [Show full text]
  • Nanotechnology, Ethics and Policy Education: Research and Pedagogy: Selected Bibliography
    Association for Practical and Professional Ethics Conference Presentation, March 2013 NSF Nanotechnology Undergraduate Education grant (#EEC-1138257) focused on creating interdisciplinary modules about the social, ethical, environmental, and economic impact of nanotechnology for all students at the Colorado School of Mines. (For an overview of the project plan, see NanoSTEP: Nano-Science, Technology, Ethics and Policy Poster Presentation to NSF EEC conference March 2012 ) Dr. Corinne Packard, a professor in the department of Metallurgical and Materials Engineering who works with solar cell nanomaterials, was the PI. The team of Co-PIs and Senior Personnel were drawn from the multidisciplinary Liberal Arts and International Studies department which is responsible for delivering core courses in humanities and social sciences. The first part of the project was a module for the freshman ethics and writing course, Nature and Human Values, which included a common lecture and reading assignments and different course activates and discussions about the risks and benefits of the technology. (See Workshop and Module Design—Part 1—Nature and Human Values). The second part of the project was a module for the sophomore-level course, Human Systems, a history of sociological, religious, political, and economic systems. For this course, the focus of the module was on policy and international relations in technology development. (See Workshop and Module Design—Part 2—Human Systems). We disseminated our work at several conferences and to universities in China and Spain, but most notably contributed a panel discussion with several team members at APPE 2013 in San Antonio (See Association for Practical and Professional Ethics 2013 Conference Presentations).
    [Show full text]
  • Measurement of the Cosmic Microwave Background Radiation at 19 Ghz
    Measurement of the Cosmic Microwave Background Radiation at 19 GHz 1 Introduction Measurements of the Cosmic Microwave Background (CMB) radiation dominate modern experimental cosmology: there is no greater source of information about the early universe, and no other single discovery has had a greater impact on the theories of the formation of the cosmos. Observation of the CMB confirmed the Big Bang model of the origin of our universe and gave us a look into the distant past, long before the formation of the very first stars and galaxies. In this lab, we seek to recreate this founding pillar of modern physics. The experiment consists of a temperature measurement of the CMB, which is actually “light” left over from the Big Bang. A radiometer is used to measure the intensity of the sky signal at 19 GHz from the roof of the physics building. A specially designed horn antenna allows you to observe microwave noise from isolated patches of sky, without interference from the relatively hot (and high noise) ground. The radiometer amplifies the power from the horn by a factor of a billion. You will calibrate the radiometer to reduce systematic effects: a cryogenically cooled reference load is periodically measured to catch changes in the gain of the amplifier circuit over time. 2 Overview 2.1 History The first observation of the CMB occurred at the Crawford Hill NJ location of Bell Labs in 1965. Arno Penzias and Robert Wilson, intending to do research in radio astronomy at 21 cm wavelength using a special horn antenna designed for satellite communications, noticed a background noise signal in all of their radiometric measurements.
    [Show full text]
  • The Evolution of Engineering Materials
    Paper ID #20611 The Evolution of Engineering Materials Dr. Amber L. Genau, University of Alabama at Birmingham Dr. Amber Genau is an assistant professor in the Materials Science and Engineering Department at the University of Alabama at Birmingham. She received her B.S. and M.S. from Iowa State University and Ph.D. from Northwestern University, all in materials engineering. Before coming to UAB, Dr. Genau spent two years as a guest scientist at the German Aerospace Center in Cologne, Germany, working on metal solidification and microstructural characterization. She is particularly interested in broadening participation in engineering and providing international experiences and perspectives to undergraduate students. c American Society for Engineering Education, 2017 The Evolution of Engineering Materials Abstract This paper describes the development of an upper level engineering elective entitled “The Evolution of Engineering Materials.” The course considers how the discovery of new materials and the ability of process materials in new ways has influenced the course of history, shaping both human societies and their surrounding environments, from the Stone Age to the Modern Era. Students become familiar with a variety of still-relevant technical content through the consideration of historical activity, from smelting and coking to polymerization reactions and cross linking. The course addresses a variety of ABET outcomes while also supporting the development of global competency through an increased appreciation of world history. Although this course was developed for and taught in the context of a three-week study abroad trip to Europe, the engaging and accessible nature of the content could also make it valuable as a service course for non-engineering majors.
    [Show full text]
  • Chemical & Biological Engineering Department History (PDF)
    Chemical & Biological Engineering The University of Alabama A Century of Excellence and Quality A Legacy of Leadership 1910 – 2010 By Gary C. April University Research Professor & Head (Emeritus) A Century of Excellence and Quality A Legacy of Leadership 1910-2010 Gary C. April University Research Professor & Head Emeritus Chemical & Biological Engineering The University of Alabama October 2010 ii Dedication The author would like to dedicate this brief history of the Chemical Engineering Department at The University of Alabama to Lynne, his wife, partner and soul mate of 48 years, to his children, Andrew, Brian and Elizabeth, who lived most of their lives while he was a professor there, and to his granddaughters, Andrea, Abigail, Caroline and Olivia who continue to provide him with encouragement by sharing a vision for the future that is filled with hope and opportunities. iii Table of Contents Preface ..................................................................................................................... v 1. The Beginning of Engineering Education at The University of Alabama 1 ................................................................................................................. 1 2. The Emergence of the Chemical Engineering Profession ........................... 7 3. Chemical Engineering at the University of Alabama – A Century of Excellence and Quality – A Legacy of Leadership 5 ....................................... 11 4. The Significance of Who We Are .................................................................
    [Show full text]
  • Displacement and Equilibrium: a Cultural History of Engineering in America Before Its “Golden Age”
    Displacement and Equilibrium: A Cultural History of Engineering in America Before Its “Golden Age” A DISSERTATION SUBMITTED TO THE FACULTY OF UNIVERSITY OF MINNESOTA BY David M. Kmiec IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY Bernadette Longo, Adviser August 2012 Table of Contents Introduction ............................................................................................................. 1 1 Using historical context to contextualize history: The ideology of cultural history ........................................................................... 12 Motivation and methodology for a cultural history of American engineering ......................................................................................... 16 2 National service and public work: Military education and civilian engineering ......................................................... 23 Early modern France and the origins of military engineering ................................ 24 Military engineering and the American Revolution ................................................ 30 Civilian engineering as rationale for maintaining a military in peacetime .............................................................................................. 37 Engineering union in sectionalist America .............................................................. 51 3 The self-made engineer goes to school: Institutionalized education(s) for engineers ......................................................... 59 Colleges at the
    [Show full text]
  • I : the Discovery of the Cosmic Microwave Background
    Class 19 : The cosmic microwave background and the “Hot Big Bang” theory Discovery of the cosmic microwave background Basic idea of the Hot Big Bang I : The discovery of the cosmic microwave background Penzias & Wilson (Bell-Labs) 1 Arno Penzias & Robert Wilson (1964) Were attempting to study radio emissions from our Galaxy using sensitive antenna built at Bell-Labs Needed to characterize and eliminate all sources of noise They never could get rid of a certain noise source… noise had a characteristic temperature of about 3 K. They figured out that the noise was coming from the sky, and was approximately the same in all directions… The COBE mission Built by NASA-Goddard Space Flight Center Launched Nov. 1989 Purpose was to survey infra-red and microwave emission across the whole sky. Primary purpose – to characterize the CMB. Had a number of instruments on it: FIRAS (Far infra-red absolute spectrophotometer) DMR (Differential Microwave Radiometer) DIRBE (Diffuse Infrared background Experiment) 2 Our Galaxy observed by the DIRBE instrument on COBE 3 Almost uniform intensity of microwaves in all directions (isotropic 2.7K black body radiation) 4 Subtracting off the mean level leaves with a “dipole” pattern… what is this?? Subtracting off the dipole finally reveals the emission from the Galaxy that Penzias and Wilson were looking for! 5 Subtracting contribution from Galaxy reveals fluctuations in the CMB WMAP (2004) 6 II : The hot big bang model Penzias & Wilson had discovered radiation left over from the early universe… The hot big bang model… Independently developed by James Peebles and George Gamov They suggested that the universe started off in an extremely hot state.
    [Show full text]