Albert Abraham Michelson 1852-1931
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Selected Bibliography of American History Through Biography
DOCUMENT RESUME ED 088 763 SO 007 145 AUTHOR Fustukjian, Samuel, Comp. TITLE Selected Bibliography of American History through Biography. PUB DATE Aug 71 NOTE 101p.; Represents holdings in the Penfold Library, State University of New York, College at Oswego EDRS PRICE MF-$0.75 HC-$5.40 DESCRIPTORS *American Culture; *American Studies; Architects; Bibliographies; *Biographies; Business; Education; Lawyers; Literature; Medicine; Military Personnel; Politics; Presidents; Religion; Scientists; Social Work; *United States History ABSTRACT The books included in this bibliography were written by or about notable Americans from the 16th century to the present and were selected from the moldings of the Penfield Library, State University of New York, Oswego, on the basis of the individual's contribution in his field. The division irto subject groups is borrowed from the biographical section of the "Encyclopedia of American History" with the addition of "Presidents" and includes fields in science, social science, arts and humanities, and public life. A person versatile in more than one field is categorized under the field which reflects his greatest achievement. Scientists who were more effective in the diffusion of knowledge than in original and creative work, appear in the tables as "Educators." Each bibliographic entry includes author, title, publisher, place and data of publication, and Library of Congress classification. An index of names and list of selected reference tools containing biographies concludes the bibliography. (JH) U S DEPARTMENT Of NIA1.114, EDUCATIONaWELFARE NATIONAL INSTITUTE OP EDUCATION THIS DOCUMENT HAS BEEN REPRO DUCED ExAC ICY AS RECEIVED FROM THE PERSON OR ORGANIZATIONORIGIN ATING IT POINTS OF VIEW OR OPINIONS STATED DO NOT NECESSARILYREPRE SENT OFFICIAL NATIONAL INSTITUTEOF EDUCATION POSITION OR POLICY PREFACE American History, through biograRhies is a bibliography of books written about 1, notable Americans, found in Penfield Library at S.U.N.Y. -
A Basic Michelson Laser Interferometer for the Undergraduate Teaching Laboratory Demonstrating Picometer Sensitivity Kenneth G
A basic Michelson laser interferometer for the undergraduate teaching laboratory demonstrating picometer sensitivity Kenneth G. Libbrechta) and Eric D. Blackb) 264-33 Caltech, Pasadena, California 91125 (Received 3 July 2014; accepted 4 November 2014) We describe a basic Michelson laser interferometer experiment for the undergraduate teaching laboratory that achieves picometer sensitivity in a hands-on, table-top instrument. In addition to providing an introduction to interferometer physics and optical hardware, the experiment also focuses on precision measurement techniques including servo control, signal modulation, phase-sensitive detection, and different types of signal averaging. Students examine these techniques in a series of steps that take them from micron-scale sensitivity using direct fringe counting to picometer sensitivity using a modulated signal and phase-sensitive signal averaging. After students assemble, align, and characterize the interferometer, they then use it to measure nanoscale motions of a simple harmonic oscillator system as a substantive example of how laser interferometry can be used as an effective tool in experimental science. VC 2015 American Association of Physics Teachers. [http://dx.doi.org/10.1119/1.4901972] 8–14 I. INTRODUCTION heterodyne readouts, and perhaps multiple lasers. Modern interferometry review articles tend to focus on complex optical Optical interferometry is a well-known experimental tech- configurations as well,15 as they offer improved sensitivity and nique for making precision displacement measurements, stability over simpler designs. While these advanced instru- with examples ranging from Michelson and Morley’s famous ment strategies are becoming the norm in research and indus- aether-drift experiment to the extraordinary sensitivity of try, for educational purposes we sought to develop a basic modern gravitational-wave detectors. -
Detector Description and Performance for the First Coincidence
ARTICLE IN PRESS Nuclear Instruments and Methods in Physics Research A 517 (2004) 154–179 Detector description and performance for the first coincidence observations between LIGO and GEO B. Abbotta, R. Abbottb, R. Adhikaric, A. Ageevao,1, B. Allend, R. Amine, S.B. Andersona, W.G. Andersonf, M. Arayaa, H. Armandulaa, F. Asiria,2, P. Aufmuthg, C. Aulberth, S. Babaki, R. Balasubramaniani, S. Ballmerc, B.C. Barisha, D. Barkeri, C. Barker-Pattonj, M. Barnesa, B. Barrk, M.A. Bartona, K. Bayerc, R. Beausoleill,3, K. Belczynskim, R. Bennettk,4, S.J. Berukoffh,5, J. Betzwieserc, B. Bhawala, I.A. Bilenkoao, G. Billingsleya, E. Blacka, K. Blackburna, B. Bland-Weaverj, B. Bochnerc,6, L. Boguea, R. Borka, S. Bosen, P.R. Bradyd, V.B. Braginskya,o, J.E. Brauo, D.A. Brownd, S. Brozekg,7, A. Bullingtonl, A. Buonannop,8, R. Burgessc, D. Busbya, W.E. Butlerq, R.L. Byerl, L. Cadonatic, G. Cagnolik, J.B. Campr, C.A. Cantleyk, L. Cardenasa, K. Carterb, M.M. Caseyk, J. Castiglionee, A. Chandlera, J. Chapskya,9, P. Charltona, S. Chatterjic, Y. Chenp, V. Chickarmanes, D. Chint, N. Christensenu, D. Churchesi, C. Colacinog,v, R. Coldwelle, M. Colesb,10, D. Cookj, T. Corbittc, D. Coynea, J.D.E. Creightond, T.D. Creightona, D.R.M. Crooksk, P. Csatordayc, B.J. Cusackw, C. Cutlerh, E. D’Ambrosioa, K. Danzmanng,v,x, R. Daviesi, E. Daws,11, D. DeBral, T. Delkere,12, R. DeSalvoa, S. Dhurandary,M.D!ıazf, H. Dinga, R.W.P. Dreverz, R.J. Dupuisk, C. Ebelingu, J. Edlunda, P. Ehrensa, E.J. -
Henry Andrews Bumstead 1870-1920
NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XIII SECOND MEMOIR BIOGRAPHICAL MEMOIR OF HENRY ANDREWS BUMSTEAD 1870-1920 BY LEIGH PAGE PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1929 HENRY ANDREWS BUMSTEAD BY LIUGH PAGE Henry Andrews Bumstead was born in the small town of Pekin, Illinois, on March 12th, 1870, son of Samuel Josiah Bumstead and Sarah Ellen Seiwell. His father, who was a physician of considerable local prominence, had graduated from the medical school in Philadelphia and was one of the first American students of medicine to go to Vienna to complete his studies. While the family was in Vienna, Bumstead, then a child three years of age, learned to speak German as fluently as he spoke English, an accomplishment which was to prove valuable to him in his subsequent career. Bumstead was descended from an old New England family which traces its origin to Thomas Bumstead, a native of Eng- land, who settled in Boston, Massachusetts, about 1640. Many of his ancestors were engaged in the professions, his paternal grandfather, the Reverend Samuel Andrews Bumstead, being a graduate of Princeton Theological Seminary and a minister in active service. From them he inherited a keen mind and an unusually retentive memory. It is related that long before he had learned to read, his Sunday school teacher surprised his mother by complimenting her on the ease with which her son had rendered the Sunday lesson. It turned out that his mother made a habit of reading the lesson to Bumstead before he left for school, and the child's remarkable performance there was due to his ability to hold in his memory every word of the lesson after hearing it read to him a single time. -
Josiah Willard Gibbs
GENERAL ARTICLE Josiah Willard Gibbs V Kumaran The foundations of classical thermodynamics, as taught in V Kumaran is a professor textbooks today, were laid down in nearly complete form by of chemical engineering at the Indian Institute of Josiah Willard Gibbs more than a century ago. This article Science, Bangalore. His presentsaportraitofGibbs,aquietandmodestmanwhowas research interests include responsible for some of the most important advances in the statistical mechanics and history of science. fluid mechanics. Thermodynamics, the science of the interconversion of heat and work, originated from the necessity of designing efficient engines in the late 18th and early 19th centuries. Engines are machines that convert heat energy obtained by combustion of coal, wood or other types of fuel into useful work for running trains, ships, etc. The efficiency of an engine is determined by the amount of useful work obtained for a given amount of heat input. There are two laws related to the efficiency of an engine. The first law of thermodynamics states that heat and work are inter-convertible, and it is not possible to obtain more work than the amount of heat input into the machine. The formulation of this law can be traced back to the work of Leibniz, Dalton, Joule, Clausius, and a host of other scientists in the late 17th and early 18th century. The more subtle second law of thermodynamics states that it is not possible to convert all heat into work; all engines have to ‘waste’ some of the heat input by transferring it to a heat sink. The second law also established the minimum amount of heat that has to be wasted based on the absolute temperatures of the heat source and the heat sink. -
THE MICHELSON INTERFEROMETER Intermediate ( First Part) to Advanced (Latter Parts)
THE MICHELSON INTERFEROMETER Intermediate ( first part) to Advanced (latter parts) Goal: There is a progression of goals for this experiment but you do not have to do Reading: the last goal. The first goal is to align the interferometer and calibrate it. Calibration ADC should be done both mechanically and Michelson program writeup optically with a HeNe laser. The second Stepper motors goal is a study of the sodium doublet. One measures the average wavelength of the two Good optics text lines and the separation of the lines. The Fourier transforms and FFT final experimental goal is to find interference fringes for white light and measure it’s coherence length. Homework: 1. Indicate how the standard michelson interferometer optics is the same as the Introduction: optics shown in fig. 2. Figure 1 The optics of the Michelson Interferometer. Note the light directed away from the mirrors is offset from the light directed toward the mirrors for clarity Note: The observation of fringes associated with the sodium doublet is a rather difficult Figure 2 The optics of the Michelson experiment and the observation of white Interferometer is equivalent to the that of light fringes is even more difficult. two sources S1 ans S2, that are emitting Understanding how the concept of light that is in phase. Note: source S1 is coherence length relates to this experiment movable. is almost essential to complete these goals. 2. Explain changes the optics in fig.1 and 2 required to account for the finite size of the light source Page -1- 3. For the optics shown in fig.2, at what Experimental tasks distance should the detector (eye) be There are three experimental tasks, focused? but only the first two are required. -
Increasing the Sensitivity of the Michelson Interferometer Through Multiple Reflection Woonghee Youn
Rose-Hulman Institute of Technology Rose-Hulman Scholar Graduate Theses - Physics and Optical Engineering Graduate Theses Summer 8-2015 Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection Woonghee Youn Follow this and additional works at: http://scholar.rose-hulman.edu/optics_grad_theses Part of the Engineering Commons, and the Optics Commons Recommended Citation Youn, Woonghee, "Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection" (2015). Graduate Theses - Physics and Optical Engineering. Paper 7. This Thesis is brought to you for free and open access by the Graduate Theses at Rose-Hulman Scholar. It has been accepted for inclusion in Graduate Theses - Physics and Optical Engineering by an authorized administrator of Rose-Hulman Scholar. For more information, please contact bernier@rose- hulman.edu. Increasing the Sensitivity of the Michelson Interferometer through Multiple Reflection A Thesis Submitted to the Faculty of Rose-Hulman Institute of Technology by Woonghee Youn In Partial Fulfillment of the Requirements for the Degree of Master of Science in Optical Engineering August 2015 © 2015 Woonghee Youn 2 ABSTRACT Youn, Woonghee M.S.O.E Rose-Hulman Institute of Technology August 2015 Increase a sensitivity of the Michelson interferometer through the multiple reflection Dr. Charles Joenathan Michelson interferometry has been one of the most famous and popular optical interference system for analyzing optical components and measuring optical metrology properties. Typical Michelson interferometer can measure object displacement with wavefront shapes to one half of the laser wavelength. As testing components and devices size reduce to micro and nano dimension, Michelson interferometer sensitivity is not suitable. The purpose of this study is to design and develop the Michelson interferometer using the concept of multiple reflections. -
The Holometer: a Measurement of Planck-Scale Quantum Geometry
The Holometer: A Measurement of Planck-Scale Quantum Geometry Stephan Meyer November 3, 2014 1 The problem with geometry Classical geometry is made of definite points and is based on “locality.” Relativity is consistent with this point of view but makes geometry “dynamic” - reacts to masses. Quantum physics holds that nothing happens at a definite time or place. All measurements are quantum and all known measurements follow quantum physics. Anything that is “real” must be measurable. How can space-time be the answer? Stephan Meyer SPS - November 3, 2014 2 Whats the problem? Start with - Black Holes What is the idea for black holes? - for a massive object there is a surface where the escape velocity is the speed of light. Since nothing can travel faster than the speed of light, things inside this radius are lost. We can use Phys131 to figure this out Stephan Meyer SPS - November 3, 2014 3 If r1 is ∞, then To get the escape velocity, we should set the initial kinetic energy equal to the potential energy and set the velocity equal to the speed of light. Solving for the radius, we get Stephan Meyer SPS - November 3, 2014 4 having an object closer than r to a mass m, means it is lost to the world. This is the definition of the Schwarzshild radius of a black hole. So for stuff we can do physics with we need: Stephan Meyer SPS - November 3, 2014 5 A second thing: Heisenberg uncertainty principle: an object cannot have its position and momentum uncertainty be arbitrarily small This can be manipulated, using the definition of p and E to be What we mean is that to squeeze something to a size λ, we need to put in at least energy E. -
1 Laboratory 8: Michelson Interferometer 1.1 Theory: References:Optics,E.Hecht,Sec 9.4
1051-232-20033 Imaging Systems Laboratory II Week of 5/3/2004, Writeup Due 5/18/2004 (T) 1 Laboratory 8: Michelson Interferometer 1.1 Theory: References:Optics,E.Hecht,sec 9.4 1.1.1 Division-of-Wavefront Interferometry In the last lab, you saw that coherent (single-wavelength) light from point sources two different locations in an optical beam could be combined after having traveled along two different paths. The recombined light exhibited sinusoidal fringes whose spatial frequency depended on the difference in angle of the light beams when recombined. The regular variation in relative phase of the light beams resulted in constructive interference (when the relative phase difference is 2πn,wheren is an integer) and destructive interference where the relative phase difference is 2πn + π. The centers of the “bright” fringes occur where the optical paths differ by an integer multiple of λ0. “Division-of-Wavefront” Interferometry via Young’s Two-Slit Experiment. The period of the intensity fringes at the observation plane is D Lλ . ' d 1.1.2 Division-of-Amplitude Interferometry This laboratory will introduce a second class of interferometer where the amplitude of the light is separated into two (or more) parts at the same point in space via partial reflection by a beamsplitter. The beamsplitter is the light-dividing element in several types of interferometers. This lab will demostrate the action of the Michelson interferometer for both coherent light from a laser and for white light (with some luck!). Coherence of a Light Source If two points within the same beam of light exhibit a consistent and measurable phase difference, then the light at the two points is said to be coherent, and thus 1 the light at these two locations may be combined to create interference. -
A Conversation with Richard A. Olshen 3
Statistical Science 2015, Vol. 30, No. 1, 118–132 DOI: 10.1214/14-STS492 c Institute of Mathematical Statistics, 2015 A Conversation with Richard A. Olshen John A. Rice Abstract. Richard Olshen was born in Portland, Oregon, on May 17, 1942. Richard spent his early years in Chevy Chase, Maryland, but has lived most of his life in California. He received an A.B. in Statistics at the University of California, Berkeley, in 1963, and a Ph.D. in Statistics from Yale University in 1966, writing his dissertation under the direction of Jimmie Savage and Frank Anscombe. He served as Research Staff Statistician and Lecturer at Yale in 1966–1967. Richard accepted a faculty appointment at Stanford University in 1967, and has held tenured faculty positions at the University of Michigan (1972–1975), the University of California, San Diego (1975–1989), and Stanford University (since 1989). At Stanford, he is Professor of Health Research and Policy (Biostatistics), Chief of the Division of Biostatistics (since 1998) and Professor (by courtesy) of Electrical Engineering and of Statistics. At various times, he has had visiting faculty positions at Columbia, Harvard, MIT, Stanford and the Hebrew University. Richard’s research interests are in statistics and mathematics and their applications to medicine and biology. Much of his work has concerned binary tree-structured algorithms for classification, regression, survival analysis and clustering. Those for classification and survival analysis have been used with success in computer-aided diagnosis and prognosis, especially in cardiology, oncology and toxicology. He coauthored the 1984 book Classi- fication and Regression Trees (with Leo Brieman, Jerome Friedman and Charles Stone) which gives motivation, algorithms, various examples and mathematical theory for what have come to be known as CART algorithms. -
Statement by Howard Bloch at the FAS Senate Meeting on October 15, 2020 Missed Opportunities
Statement by Howard Bloch at the FAS Senate meeting on October 15, 2020 Missed Opportunities So much of what goes into making a university great has to do with meeting and matching the moment. Science at Yale began with such a recognition. When a meteorite fell on the morning of December 14, 1807 in Weston, CT, an enterprising young Professor of Chemistry, Benjamin Silliman, and a colleague, James Kingsley, who taught Hebrew, Greek, and Latin, set off two days later to bring it back to New Haven. The paper which Silliman presented to the American Philosophical Society in Philadelphia in 1809 engendered a national debate and was probably the first scientific paper in America since those of Benjamin Franklin to attract notice in Europe. When it came to the natural sciences, Yale was unsurpassed by any American university in the nineteenth century, which began with Silliman and ended with Josiah Willard Gibbs whom Albert Einstein, leaving all relativity aside, pronounced “the greatest mind in American history.” But science lagged at Yale in the twentieth century, in part as a result of missed opportunities. Yale failed to hire Jewish scientists exiled from Germany and Hungary in the wake of the rise of Nazism in the 1930s and 40s. None of the exiled physicists who played major and supporting roles in the quantum revolution, Jewish or not, ended up in New Haven, but were welcomed at Princeton/IAS, Columbia, Harvard, MIT, Cornell, the University of Chicago, UC-Berkeley, and Caltech. When we missed the revolution in physics in the first half of the century, we were ill-suited to participate in the revolution in genetics in the second half. -
Slepian-UF-Q2-On the Nature of Time and Being-Gen Ed Syllabus
Quest 2: On the nature of time and being: an astrophysics-informed approach to the big questions Primary General Education Designation: Physical Sciences Secondary General Education Designation: International I. Course Information Quest 2 IDS2935/XXXX, Spring 2020 Meeting Day/Time: TBA Location: TBA General Education Designation: [Physical Sciences, International, WR 4000] * A minimum grade of C is required for general education credit * Instructor Zachary Slepian, PhD [email protected]; (352) 294–1851 Office Hours: Days TBD, Time TBD 302 Bryant Space Science Center Course Description What is the nature of time? What is the nature of space (and space-time)? And where do we fit in? These are hard questions, and this course will not offer final answers. Rather, in this course we will acquire the tools and language to think critically about these questions. We will thoroughly investigate some of the most interesting topics in contemporary physics— the arrow of time, irreversibility, quantum mechanics, cosmology—through the lens of these big questions. Throughout, we will attack these areas via many different channels. This class should be accessible to non-physics majors—indeed, to those with minimal technical background at all—so we will focus on the concepts, exploring the key ideas with almost no math. At the same time, we will mix in ideas from philosophy, history, and art that also bear on these questions. This will make the course relevant and exciting both for those who feel a strong affinity with the arts and humanities as well as for those for whom science resonates more. 1 Importantly, the course will also expose what the scientific method is and how science has been shaped by broader currents in history, culture, and philosophy, and in turn, how it has shaped them.