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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. -
Weberˇs Planetary Model of the Atom
Weber’s Planetary Model of the Atom Bearbeitet von Andre Koch Torres Assis, Gudrun Wolfschmidt, Karl Heinrich Wiederkehr 1. Auflage 2011. Taschenbuch. 184 S. Paperback ISBN 978 3 8424 0241 6 Format (B x L): 17 x 22 cm Weitere Fachgebiete > Physik, Astronomie > Physik Allgemein schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. Weber’s Planetary Model of the Atom Figure 0.1: Wilhelm Eduard Weber (1804–1891) Foto: Gudrun Wolfschmidt in der Sternwarte in Göttingen 2 Nuncius Hamburgensis Beiträge zur Geschichte der Naturwissenschaften Band 19 Andre Koch Torres Assis, Karl Heinrich Wiederkehr and Gudrun Wolfschmidt Weber’s Planetary Model of the Atom Ed. by Gudrun Wolfschmidt Hamburg: tredition science 2011 Nuncius Hamburgensis Beiträge zur Geschichte der Naturwissenschaften Hg. von Gudrun Wolfschmidt, Geschichte der Naturwissenschaften, Mathematik und Technik, Universität Hamburg – ISSN 1610-6164 Diese Reihe „Nuncius Hamburgensis“ wird gefördert von der Hans Schimank-Gedächtnisstiftung. Dieser Titel wurde inspiriert von „Sidereus Nuncius“ und von „Wandsbeker Bote“. Andre Koch Torres Assis, Karl Heinrich Wiederkehr and Gudrun Wolfschmidt: Weber’s Planetary Model of the Atom. Ed. by Gudrun Wolfschmidt. Nuncius Hamburgensis – Beiträge zur Geschichte der Naturwissenschaften, Band 19. Hamburg: tredition science 2011. Abbildung auf dem Cover vorne und Titelblatt: Wilhelm Weber (Kohlrausch, F. (Oswalds Klassiker Nr. 142) 1904, Frontispiz) Frontispiz: Wilhelm Weber (1804–1891) (Feyerabend 1933, nach S. -
History (From Wikipedia)
History (from Wikipedia) November 13, 2019 There’s a reason math things are named after physicists: 1. Friedrich Wilhelm Bessel was a German astronomer, mathematician, physicist and geodesist. He was the first astronomer who determined reliable values for the distance from the sun to another star by the method of parallax. A special type of mathematical functions were named Bessel functions after Bessel’s death, though they had originally been discovered by Daniel Bernoulli and then generalised by Bessel. 2. Pierre-Simon, marquis de Laplace: was a French scholar whose work was important to the devel- opment of engineering, mathematics, statistics, physics, astronomy, and philosophy. He summarized and extended the work of his predecessors in his five-volume Mécanique Céleste (Celestial Mechanics) (1799–1825). This work translated the geometric study of classical mechanics to one based on calculus, opening up a broader range of problems. In statistics, the Bayesian interpretation of probability was developed mainly by Laplace. 3. Adrien-Marie Legendre: Whoops, he’s a mathemetician. But much of his work was completed by Gauss. Legendre is known for the Legendre transformation, which is used to go from the Lagrangian to the Hamiltonian formulation of classical mechanics. In thermodynamics it is also used to obtain the enthalpy and the Helmholz and Gibbs (free) energies from the internal energy. He is also the namesake of the Legendre polynomials, solutions to Legendre’s differential equation, which occur frequently in physics and engineering applications, e.g. electrostatics. 4. Carl Gottfried Neumann, while in Königsberg, studied physics with his father, and later as a working mathematician, dealt almost exclusively with problems arising from physics. -
Weber Quoting Maxwell
Weber quoting Maxwell Zur Anseinandcrsetzun!!; zwit;chen der Weberschen Theorie del" Elektrizitat lind der emfkommenden lVIaxwelIschen Elektrodynaillik Andf(~ Koch Torres Assis, Campinas, Sao Paulo, Brasil, and Karl Heinrich \Vicdcrkehr, Hamburg Zusamrnenfassung Die Abhandlllllg spt7:t sidl mit del' Ablos\lll!-\ der iilterPIl Ekktrodynamik vou \Vilhdill \Ve bef und Fran;. Npumunll durch die .\laxwf'lJschr Theoric im lebten Drittel des 19. .lahr h\llldf'rt~ aus!'inClIHirr. AuflliingrT fiir die Darst.ellllng der Pl'oblcl11<Jtik sind <iiI" w€nigen i':ltatp, dk sidl bci VI/ilhe]m \Ve!wr findcn. Di(' Diskuf'sioll wUrci(' daIllals h,mpt~iicblich (lurch Carl Nculllanu lind Johann Karl Friedrich Z;ii1hwr gcfUhrt" Ikidc warell cngagienE' und !eidpIIschaftlidlP AnhiiTlger lind Vertei<iiger (\r-~r \\"f'bcr~dlPII Sieht uml Darstl'lluIlg der Thl'orie von d('r ElekLrb:iUit" Streit,pnnkte waf(~n (1) dk N<l,hwirkungHtlH'orie, die mit dem \laxwell~c1wn Feldkoll7Ppt identiHch illt unci 1m Gegel1H<l,tz zur FermvirkUllg-~theorie (Pro toLyp: ~ewtonscheH Gravitati()lI~gesetz) c,t,anli, und (2) die Annalilne der ExiSlenz piner ~ub~tant.iellen EkktrizitiiL \V("\H'r beharrte his ;;ulpt7.t auf scinPHl Konzept nnt! entwickeite ein ,\t,omnH)(\ell, d,u.; ab Vor~tufe des Jlutherford-Hohr~chE'n At()lllIllOdcJl~ angesehen wer den kalln. Konsen~ bestand Lei den absoluten eiektrischpn :'\,Ia.i;sYHt,emen. J_ Cl. lvI~wel1 Ii\..'; au~ d('lll Kohlransch-\VclwT-E::qJPrinwnt die LirhtgeHthwindigkeit heraU'" die flir ~eine ('lektnJInagnl'tiHthc l .. ichttheorie cine wiehtige Stiitze war. Da.s absolnte elektrornagneLi~che I\IaJ~SVHr,em (\icnLe <lh Crul1dlagp fur die InternaLionalen 'l\Iar~einheiten 1881. -
Maxwell Discovers That Light Is Electromagnetic Waves in 1862
MAXWELL DISCOVERS LIGHT IS ELECTROMAGNETIC WAVES James Clerk Maxwell was a Scottish scientist. He worked in the mid-nineteenth century in Scotland and England. At that time, electricity and magnetism had been extensively studied, and it was known since 1831 that electric current produces magnetism. Maxwell added the idea that changing magnetism could produce electricity. The term that Maxwell added to the known equations (called Ampere's law) for magnetism allowed Maxwell to see that there were wave-like solutions, that is, solutions that look like a sine wave (as a function of time). The numbers in Maxwell's equations all came from laboratory experiments on electric- ity and magnetism. There was nothing in those equations about light, and radio waves were completely unknown at the time, so the existence of electromagnetic waves was also completely unknown. But mathematics showed that Maxwell's equations had wave-like solutions. What did that mean? Maxwell proceeded to calculate the speed of those waves, which of course depended on the numbers that came from lab experiments with electricity and magnetism (not with light!). He got the answer 310,740,000 meters per second. Maxwell must have had an \aha moment" when he recognized that number. He did recognize that number: it was the speed of light! He was lecturing at King's College, London, in 1862, and there he presented his result that the speed of propagation of an electromagnetic field is approximately that of the speed of light. He considered this to be more than just a coincidence, and commented: \We can scarcely avoid the conclusion that light consists in the transverse undulations of the same medium which is the cause of electric and magnetic phenomena." 1 2 MAXWELL DISCOVERS LIGHT IS ELECTROMAGNETIC WAVES He published his work in his 1864 paper, A dynamical theory of the electromagnetic field. -
The Double Helix Theory of the Magnetic Field
The Double Helix Theory of the Magnetic Field Frederick David Tombe Belfast, Northern Ireland, United Kingdom [email protected] 15th February 2006, Philippine Islands Abstract. The historical linkage between optics and electromagnetism can be traced back to a paper published in the year 1856 by Wilhelm Eduard Weber and Rudolf Kohlrausch. By discharging a Leyden Jar (a capacitor), they showed that the ratio of the electromagnetic and electrostatic units of charge is numerically equal to the directly measured speed of light. Weber interpreted this result as meaning that the speed of light is a kind of escape velocity for electricity in motion, such as would enable the associated magnetic force to overcome the electrostatic force. An alternative interpretation was advanced a few years later by James Clerk-Maxwell who connected the result to the elasticity in an all pervading solid medium that serves as the carrier of light waves. As a consequence, he concluded that light waves are electromagnetic undulations. These two perspectives can be reconciled by linking the speed of light to the circumferential speed of the molecular vortices which Maxwell believed to be the constituent particles of the solid luminiferous medium. If we consider these molecular vortices to be tiny electric current circulations, magnetic repulsion can then be explained in terms of centrifugal force. And if these molecular vortices should take the form of an electron and a positron in mutual orbit, we can then also explain magnetic attraction in terms of the more fundamental electrostatic force being channeled through space along double helix chains that constitute magnetic lines of force. -
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. -
Applied Electromagnetics
Dan Sievenpiper - UCSD, 858-822-6678,[email protected] Applied Electromagnetics Dan Sievenpiper, 2018-10-29 1 Dan Sievenpiper - UCSD, 858-822-6678,[email protected] History: A Few of the Early Pioneers in Electromagnetics Andre-Marie Ampere Michael Faraday James C. Maxwell Heinrich Hertz Invented telegraph Invented electric motor Unified electricity, magnetism Proved existence of (among many other things) (among many other things) and light into one theory electromagnetic waves Guglielmo Many, many others: Nicola Tesla Marconi • Alessandro Volta • James Prescott Joule • Georg Simon Ohm • Charles William Siemens • Charles-Augustin Coulomb • Joseph Henry • Wilhelm Eduard Weber • Hans Christian Orsted Invented AC, wireless Invented radio • … communication 2 power transfer Dan Sievenpiper - UCSD, 858-822-6678,[email protected] Courses in Applied Electromagnetics • Undergrad Courses – ECE107 – Electromagnetism – ECE123 – Antenna Systems Engineering – ECE166 – Microwave Systems and Circuits – ECE182 – Electromagnetic Optics, Guided-wave and Fiber Optics • Graduate Courses – ECE221 – Magnetic Materials Principles and Applications – ECE222A – Antennas and their System Applications – ECE222B – Electromagnetic Theory – ECE222C – Computational Methods for Electromagnetics – ECE222D – Advanced Antenna Design 3 Dan Sievenpiper - UCSD, 858-822-6678,[email protected] ECE107 Electromagnetism • Electrostatics, magnetostatics • Vector analysis • Maxwell’s equations • Plane waves, reflection, refraction • Electromagnetic -
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 -
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. -
– by Julia Cipo, Holger Kersten –
THE GAS DISCHARGE PHYSICS IN THE 19th CENTURY (PART I) – by Julia Cipo, Holger Kersten – Sir Vasily Humphry Petrov * July 19th, 1761 in Oboyan, Russia Davy † August 5th, 1834 in Saint Petersburg, Russia * December 17th, 1778 in Penzance, Cornwall in England Vasily Vladimirovich Petrov was a russian physicist and member of the Russian † May 29th, 1829 in Genf, Switzerland *4 Academy of Sciences. After A.Volta introduced his voltaic battery in the year *1 1800, Petrov began constructing a larger battery by using 4200 copper and zinc Sir Humphry Davy was an english chemist, inventor and presi- discs, stowed in four huge boxes. The boxes were about 3 m long and placed dent of the Royal Society. Unaware of Petrov’s work, Davy con- parallel to each other. They alternately ended with zinc and copper, so when structed a larger voltaic battery with an electrode area of 80 m2. connected they could be used as a serial circuit of Using his huge battery in 1807 he could decompose potash and 4200 electric cells. The motivation of building an soda by gaining the metals potassium and sodium. Later he could “enormous” battery as called by Petrov was the obtain barium, calcium, strontium and magnesium. During these observation of new effects. In his report of the experiments he experienced new gas discharge phenomena such year 1803 “Announcements on Galvano-Volta- as continuous arcs, which he presented often in front of a large ic experiments” he describes the observation of aristocratic audience. In his Bakerian Lecture he writes: “By the ar- *5 the fi rst continuous arc discharge.