Maxwell Discovers That Light Is Electromagnetic Waves in 1862
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On the First Electromagnetic Measurement of the Velocity of Light by Wilhelm Weber and Rudolf Kohlrausch
Andre Koch Torres Assis On the First Electromagnetic Measurement of the Velocity of Light by Wilhelm Weber and Rudolf Kohlrausch Abstract The electrostatic, electrodynamic and electromagnetic systems of units utilized during last century by Ampère, Gauss, Weber, Maxwell and all the others are analyzed. It is shown how the constant c was introduced in physics by Weber's force of 1846. It is shown that it has the unit of velocity and is the ratio of the electromagnetic and electrostatic units of charge. Weber and Kohlrausch's experiment of 1855 to determine c is quoted, emphasizing that they were the first to measure this quantity and obtained the same value as that of light velocity in vacuum. It is shown how Kirchhoff in 1857 and Weber (1857-64) independently of one another obtained the fact that an electromagnetic signal propagates at light velocity along a thin wire of negligible resistivity. They obtained the telegraphy equation utilizing Weber’s action at a distance force. This was accomplished before the development of Maxwell’s electromagnetic theory of light and before Heaviside’s work. 1. Introduction In this work the introduction of the constant c in electromagnetism by Wilhelm Weber in 1846 is analyzed. It is the ratio of electromagnetic and electrostatic units of charge, one of the most fundamental constants of nature. The meaning of this constant is discussed, the first measurement performed by Weber and Kohlrausch in 1855, and the derivation of the telegraphy equation by Kirchhoff and Weber in 1857. Initially the basic systems of units utilized during last century for describing electromagnetic quantities is presented, along with a short review of Weber’s electrodynamics. -
A Beautiful Approach: Transformational Optics
A beautiful approach: “Transformational optics” [ several precursors, but generalized & popularized by Ward & Pendry (1996) ] warp a ray of light …by warping space(?) [ figure: J. Pendry ] Euclidean x coordinates transformed x'(x) coordinates amazing Solutions of ordinary Euclidean Maxwell equations in x' fact: = transformed solutions from x if x' uses transformed materials ε' and μ' Maxwell’s Equations constants: ε0, μ0 = vacuum permittivity/permeability = 1 –1/2 c = vacuum speed of light = (ε0 μ0 ) = 1 ! " B = 0 Gauss: constitutive ! " D = # relations: James Clerk Maxwell #D E = D – P 1864 Ampere: ! " H = + J #t H = B – M $B Faraday: ! " E = # $t electromagnetic fields: sources: J = current density E = electric field ρ = charge density D = displacement field H = magnetic field / induction material response to fields: B = magnetic field / flux density P = polarization density M = magnetization density Constitutive relations for macroscopic linear materials P = χe E ⇒ D = (1+χe) E = ε E M = χm H B = (1+χm) H = μ H where ε = 1+χe = electric permittivity or dielectric constant µ = 1+χm = magnetic permeability εµ = (refractive index)2 Transformation-mimicking materials [ Ward & Pendry (1996) ] E(x), H(x) J–TE(x(x')), J–TH(x(x')) [ figure: J. Pendry ] Euclidean x coordinates transformed x'(x) coordinates J"JT JµJT ε(x), μ(x) " ! = , µ ! = (linear materials) det J det J J = Jacobian (Jij = ∂xi’/∂xj) (isotropic, nonmagnetic [μ=1], homogeneous materials ⇒ anisotropic, magnetic, inhomogeneous materials) an elementary derivation [ Kottke (2008) ] consider× -
J Ames Clerk Maxwell and His Equations
GENERAL I ARTICLE James Clerk Maxwell and his Equations B N Dwivedi This article presents a brief account of life and work of James Clerk Maxwell and his equations. James Clerk Maxwell James Clerk Maxwell was a physicists' physicist, the prime author of the modern theory of colour vision, the principal B N Dwivedi does creator of statistical thermodynamics, and above all the author research in solar physics of the classical electromagnetic theory, with its identification of and teaches physics in light and electromagnetic waves. Maxwell's electromagnetic Banaras Hindu University. theory is acknowledged as one of the outstanding achievements He has over twenty two years of teaching of nineteenth century physics. If you wake up a physicist in the experience and broad middle of the night and say 'Maxwell', I am sure he will say experience in solar 'electromagnetic theory'. Einstein described the change brought research with involvement about by Maxwell in the conception of physical reality as "the in almost all the major solar space experiments, most profound and the most fruitful that physics has experi including Sky lab, Yohkoh, enced since the time of Newton". Maxwell's description of SOHO, and TRACE. The reality is represented in his double system of partial differential Max-Planck-Institut fur equations in which the electric and magnetic fields appear as Aeronomie recently awarded him the 'Gold dependent variables. Since Maxwell's time physical reality has Pin' in recognition of his been thought of as represented by continuous fields governed by outstanding contribution partial differential equations. The advent of quantum mechan to the SOHO/Sumer ics, rather than the theory of relativity, has produced a situation experiment. -
Notizen Zur Schweizerischen Kulturgeschichte
Notizen zur schweizerischen Kulturgeschichte. Von FERDINAND RUDIO und CARL SCHRÖTER. 29. Die Eulerausgabe (Fortsetzung 1). Im Anschluss an unsern letztjährigen Bericht geben wir zunächst den Bericht der Eulerkommission für das Jahr 1909/10 wieder, wie er am . 5. September 1910 der. 93. Jahresversammlung der Schweize- rischen Naturforschenden Gesellschaft in Basel vorgelegt worden ist. Er lautet: Bericht der Eulerkommission für das Jahr 1909/10. • Um die Beschlüsse der Gesellschaft vom 6. September 1909 aus- zuführen, versammelte sich die Kommission am 19. Dezember in Bern; vom Zentralkomitee nahmen • die Herren Dr. Fritz Sarasin und Dr. P. Chappuis an der Sitzung teil. Die Kommission konstituierte sich und bestellte ihre Organe wie folgt: Herr Professor Rudio übernimmt als Präsident des Redaktions- komitees die wissenschaftliche Leitung des ganzen Unternehmens. Als Mitredakteure stehen ihm zur Seite die Herren Geheimräte A. Krazer und P. Stäckel, Professoren an der technischen Hoch- schule in Karlsruhe. Zum Präsidenten der Eulerkommission wird der Unterzeichnete gewählt, zum Schriftführer Herr Professor R. Fueter, zum Mitglied an Stelle von Herrn Professor Geiser Herr Professor Dr. Heinrich Ganter in Aarau. Zur Besorgung der Finanzen wird ein Schatzmeister und ein Finanzausschuss von drei Mitgliedern bestellt: zum Schatzmeister wird gewählt Herr Eduard His-Schlumberger in Firma Ehinger & Co., 1) Siehe die Notizen Nr. 26 (1909), 24 (1908) und 22 (1907). 542 Ferdinand Rudio und Carl Schröter. Basel, zum dritten Mitglied des Finanzausschusses neben dem Präsi- denten und dem Schatzmeister Herr Dr. P. C h a p p u i s. Auf Antrag von Herrn Professor Rudio wird die Firma B. G. Teubner in Leipzig mit dem Druck und Verlag des Werkes betraut. -
1.1. Galilean Relativity
1.1. Galilean Relativity Galileo Galilei 1564 - 1642 Dialogue Concerning the Two Chief World Systems The fundamental laws of physics are the same in all frames of reference moving with constant velocity with respect to one another. Metaphor of Galileo’s Ship Ship traveling at constant speed on a smooth sea. Any observer doing experiments (playing billiard) under deck would not be able to tell if ship was moving or stationary. Today we can make the same Even better: Earth is orbiting observation on a plane. around sun at v 30 km/s ! ≈ 1.2. Frames of Reference Special Relativity is concerned with events in space and time Events are labeled by a time and a position relative to a particular frame of reference (e.g. the sun, the earth, the cabin under deck of Galileo’s ship) E =(t, x, y, z) Pick spatial coordinate frame (origin, coordinate axes, unit length). In the following, we will always use cartesian coordinate systems Introduce clocks to measure time of an event. Imagine a clock at each position in space, all clocks synchronized, define origin of time Rest frame of an object: frame of reference in which the object is not moving Inertial frame of reference: frame of reference in which an isolated object experiencing no force moves on a straight line at constant velocity 1.3. Galilean Transformation Two reference frames ( S and S ) moving with velocity v to each other. If an event has coordinates ( t, x, y, z ) in S , what are its coordinates ( t ,x ,y ,z ) in S ? in the following, we will always assume the “standard configuration”: Axes of S and S parallel v parallel to x-direction Origins coincide at t = t =0 x vt x t = t Time is absolute Galilean x = x vt Transf. -
International Year of Light Blog James Clerk Maxwell, the Man Who
12/7/2015 James Clerk Maxwell, the man who changed the world forever II | International Year of Light Blog International Year of Light Blog James Clerk Maxwell, the man who changed the world forever II JUNE 15, 2015JUNE 11, 2015 LIGHT2015 LEAVE A COMMENT A Dynamical Theory of the Electromagnetic Field Maxwell left us contributions to colour theory, optics, Saturn’s rings, statics, dynamics, solids, instruments and statistical physics. However, his most important contributions were to electromagnetism. In 1856, he published On Faraday’s lines of force; in 1861, On physical lines of force. In these two articles he provided a mathematical explanation for Faraday’s ideas on electrical and magnetic phenomena depending on the distribution of lines of force in space, definitively abandoning the classical doctrine of electrical and magnetic forces as actions at a distance. His mathematical theory included the aether, that «most subtle spirit», as Newton described it. He studied electromagnetic interactions quite naturally in the context of an omnipresent aether. Maxwell stood firm that the aether was not a hypothetical entity, but a real one and, in fact, for physicists in the nineteenth century, aether was as real as the rocks supporting the Cavendish Laboratory. http://light2015blog.org/2015/06/15/james-clerk-maxwell-the-man-who-changed-the-world-forever-ii/ 1/6 12/7/2015 James Clerk Maxwell, the man who changed the world forever II | International Year of Light Blog (https://light2015blogdotorg.files.wordpress.com/2015/06/figure_3.jpg) http://light2015blog.org/2015/06/15/james-clerk-maxwell-the-man-who-changed-the-world-forever-ii/ -
Research Papers-Mechanics / Electrodynamics/Download/7797
The Full Significance of the Speed of Light Frederick David Tombe, Northern Ireland, United Kingdom, [email protected] 15th June 2019 Abstract. In the year 1855, German physicists Wilhelm Eduard Weber and Rudolf Kohlrausch performed a landmark experiment of profound significance. By discharging a Leyden jar (a capacitor), they linked the speed of light to the ratio between electrostatic and electrodynamic units of charge. This experiment was electromagnetism’s Rosetta Stone because the result can be used to, (i) identify the speed of light as the speed of circulation of electric current, (ii) identify the speed of light as the speed of electromagnetic waves through a dielectric solid that pervades all of space, while noting that inertial centrifugal force and dipole fields share in common an inverse cube law in distance. The result can also be used to, (iii) identify magnetic repulsion as a centrifugal force, and hence to establish the double helix pattern that characterizes magnetic lines of force. Weber’s Interpretation I. Weber and Kohlrausch’s 1855 experiment involved discharging a Leyden jar (a capacitor) that had been storing a known amount of charge in electrostatic units, and then seeing how long it took for a unit of electric current, as measured in electrodynamic units, to produce the same deflection in a galvanometer [1]. From these readings they discovered that the ratio of the two systems of units was equal to c√2 where c is the directly measured speed of light, although it’s not clear that they immediately noticed the numerical value of c explicitly. Had they however used electromagnetic units instead of electrodynamic units for the electric current, the result would have stood out as c exactly. -
Christa Jungnickel Russell Mccormmach on the History
Archimedes 48 New Studies in the History and Philosophy of Science and Technology Christa Jungnickel Russell McCormmach The Second Physicist On the History of Theoretical Physics in Germany The Second Physicist Archimedes NEW STUDIES IN THE HISTORY AND PHILOSOPHY OF SCIENCE AND TECHNOLOGY VOLUME 48 EDITOR JED Z. BUCHWALD, Dreyfuss Professor of History, California Institute of Technology, Pasadena, USA. ASSOCIATE EDITORS FOR MATHEMATICS AND PHYSICAL SCIENCES JEREMY GRAY, The Faculty of Mathematics and Computing, The Open University, UK. TILMAN SAUER, Johannes Gutenberg University Mainz, Germany ASSOCIATE EDITORS FOR BIOLOGICAL SCIENCES SHARON KINGSLAND, Department of History of Science and Technology, Johns Hopkins University, Baltimore, USA. MANFRED LAUBICHLER, Arizona State University, USA ADVISORY BOARD FOR MATHEMATICS, PHYSICAL SCIENCES AND TECHNOLOGY HENK BOS, University of Utrecht, The Netherlands MORDECHAI FEINGOLD, California Institute of Technology, USA ALLAN D. FRANKLIN, University of Colorado at Boulder, USA KOSTAS GAVROGLU, National Technical University of Athens, Greece PAUL HOYNINGEN-HUENE, Leibniz University in Hannover, Germany TREVOR LEVERE, University of Toronto, Canada JESPER LU¨ TZEN, Copenhagen University, Denmark WILLIAM NEWMAN, Indiana University, Bloomington, USA LAWRENCE PRINCIPE, The Johns Hopkins University, USA JU¨ RGEN RENN, Max Planck Institute for the History of Science, Germany ALEX ROLAND, Duke University, USA ALAN SHAPIRO, University of Minnesota, USA NOEL SWERDLOW, California Institute of Technology, USA -
Lessons from Faraday, Maxwell, Kepler and Newton
Science Education International Vol. 26, Issue 1, 2015, 3-23 Personal Beliefs as Key Drivers in Identifying and Solving Seminal Problems: Lessons from Faraday, Maxwell, Kepler and Newton I. S. CALEON*, MA. G. LOPEZ WUI†, MA. H. P. REGAYA‡ ABSTRACT: The movement towards the use of the history of science and problem-based approaches in teaching serves as the impetus for this paper. This treatise aims to present and examine episodes in the lives of prominent scientists that can be used as resources by teachers in relation to enhancing students’ interest in learning, fostering skills about problem solving and developing scientific habits of mind. The paper aims to describe the nature and basis of the personal beliefs, both religious and philosophical, of four prominent scientists—Faraday, Maxwell, Kepler and Newton. P atterns of how these scientists set the stage for a fruitful research endeavor within the context of an ill-structured problem situation a re e x a m i n e d and how their personal beliefs directed their problem-solving trajectories was elaborated. T h e analysis of these key seminal works provide evidence that rationality and religion need not necessarily lie on opposite fences: both can serve as useful resources to facilitate the fruition of notable scientific discoveries. KEY WORDS: history of science; science and religion; personal beliefs; problem solving; Faraday; Maxwell; Kepler; Newton INTRODUCTION Currently, there has been a movement towards the utilization of historical perspectives in science teaching (Irwin, 2000; Seker, 2012; Solbes & Traver, 2003). At the same time, contemporary science education reform efforts have suggested that teachers utilize problem-based instructional approaches (Faria, Freire, Galvão, Reis & Baptista, 2012; Sadeh & Zion, 2009; Wilson, Taylor, Kowalski, & Carlson, 2010). -
Wilhelm Weber Und Maxwells Elektromagnetische Lichttheorie '
Wilhelm Weber und Maxwells elektromagnetische Lichttheorie ' Karl Heinrich Wiederkehr Summary This essay aims at demonstrating a possih/y decisive impu/se ic/iich induced J. CZ. MaxweZZ to create /lis e/ectromagneticaZ t/ieory o/ Zig/it. Pkïth their experi- ment in 7855 77. 7AohZrausch and hi Pkéber had come across the re/ocily o/Zight when determining the re/afion between the absoZute e/ectrostatic and the absoZute eZectromagnetic quantity 0/ eZectricity which they had measured. 7n V/anceZ/'s treatise "On PhysicaZ Lines 0/ Force" 77867/62/ that reZation is exact/y identi- caZ with the reZocity 0/ transmission 0/po.ssib/e transversa/ waves in /V/axu-eZZ'.s hypotheticaZ medium 7etherg The e.i/>erimeuf 0/ 7855, a masterpiece, is described in detaiZ. The "v-determinations" tv/tich were Zater carried out by some physicists — among them Maxwe/Z himseZ/ and h i Thomson — veri/ied the convergency ivit/i the more accurate measurements 0/the ve/ocity o/ Zight. Thus the va/idity 0/ the e/ectromagneticaZ theory 0/Zight was secured. Zusammenfassung Diese HbhandZung ici// an einen vieZZeicht entscheidenden /f ustoss erinnern, der J. CZ. Marice// zur Schalung seiner eZektromagnetischen Lichttheorie bewogen hat. 77.7<io/i/rausc7i und PL. Pkéber ivaren bei ihrem Experiment von 7855 au/ die /a'chtgesc/iwindig/ceit gestossen, a/s sie das kerhä/tnis von abso/ut e/ehtrostatisch und abso/ut eZe/ctromagnetisch gemessener EZektrizitäfsmenge bestimmten. 7n der MaxweZZschen Hrbeif «[/her PhysikaZische /Ara/f/inien» /7867/Ö2/ ist gerade jenes kerhä/tnis identisch mit der /vwfp//anzung.sgese/i u:indig/.:eit mög/i- eher TransversaZweZZen in \/a.TueZZs hypothetischem Medium 7/lt/ierJ. -
Speed of Light
Speed of light From Wikipedia, the free encyclopedia The speed of light in vacuum, commonly denoted c, is a universal physical constant important in many areas of physics. Its precise value is 299792458 metres per second (approximately 3.00×108 m/s), since the length of the metre is defined from this constant and the international standard for time.[1] According to special relativity, c is the maximum speed at which all matter and information in the universe can travel. It is the speed at which all massless particles and changes of the associated fields (including electromagnetic radiation such as light and gravitational waves) travel in vacuum. Such particles and waves travel at c regardless of the motion of the source or the inertial reference frame of the observer. In the theory of relativity, c interrelates space and time, and also appears in the famous equation of mass–energy equivalence E = mc2.[2] Speed of light Sunlight takes about 8 minutes 17 seconds to travel the average distance from the surface of the Sun to the Earth. Exact values metres per second 299792458 Planck length per Planck time 1 (i.e., Planck units) Approximate values (to three significant digits) kilometres per hour 1080 million (1.08×109) miles per second 186000 miles per hour 671 million (6.71×108) Approximate light signal travel times Distance Time one foot 1.0 ns one metre 3.3 ns from geostationary orbit to Earth 119 ms the length of Earth's equator 134 ms from Moon to Earth 1.3 s from Sun to Earth (1 AU) 8.3 min one light year 1.0 year one parsec 3.26 years from nearest star to Sun (1.3 pc) 4.2 years from the nearest galaxy (the Canis Major Dwarf Galaxy) to 25000 years Earth across the Milky Way 100000 years from the Andromeda Galaxy to 2.5 million years Earth from Earth to the edge of the 46.5 billion years observable universe The speed at which light propagates through transparent materials, such as glass or air, is less than c; similarly, the speed of radio waves in wire cables is slower than c. -
James Clerk Maxwell 1831-1879
James Clerk Maxwell 1831-1879 lems too. In particular, it is not clear Earlier this year saw the centenary 1 3 June 1 831, but soon went to live whether many of the nice results of of the birth of Albert Einstein. It is at Glenlair. At the age of ten, he the MIT bag for hadronic properties highly apt that 1979, which has returned to Edinburgh to begin his will be lost. A great deal of challeng been marked by further consolida formal schooling, where his unfash ing work lies ahead for both experi tion of the unified theory of weak ionable clothes and rustic manner mentalists and theorists. At question and electromagnetic interactions were mocked by his schoolfellows. is the whole understanding of and its recognition in the award of The genius who was to shape much atomic nuclei at the microscopic the Nobel Prize to Glashow, Salam of physics apparently earned the level, but that is the sort of question and Weinberg, is also the centenary name 'Dafty'. that Weisskopf and de Shalit had in of the death of the great Scottish By fourteen, he had developed a mind when they instituted this series physicist who first formulated a method for constructing geometrical of Conferences. unified theory of electric and mag figures which was read as a paper to netic fields. We are grateful to the Royal Society of Edinburgh. His Abdus Salam for drawing our at evident interest in physics led his tention to the Maxwell anniversary. uncle to introduce him to William Nicol, of prism fame.