The Austro-Hungarian Deep-Sea Expeditions
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Ludwig Boltzmann Was Born in Vienna, Austria. He Received His Early Education from a Private Tutor at Home
Ludwig Boltzmann (1844-1906) Ludwig Boltzmann was born in Vienna, Austria. He received his early education from a private tutor at home. In 1863 he entered the University of Vienna, and was awarded his doctorate in 1866. His thesis was on the kinetic theory of gases under the supervision of Josef Stefan. Boltzmann moved to the University of Graz in 1869 where he was appointed chair of the department of theoretical physics. He would move six more times, occupying chairs in mathematics and experimental physics. Boltzmann was one of the most highly regarded scientists, and universities wishing to increase their prestige would lure him to their institutions with high salaries and prestigious posts. Boltzmann himself was subject to mood swings and he joked that this was due to his being born on the night between Shrove Tuesday and Ash Wednesday (or between Carnival and Lent). Traveling and relocating would temporarily provide relief from his depression. He married Henriette von Aigentler in 1876. They had three daughters and two sons. Boltzmann is best known for pioneering the field of statistical mechanics. This work was done independently of J. Willard Gibbs (who never moved from his home in Connecticut). Together their theories connected the seemingly wide gap between the macroscopic properties and behavior of substances with the microscopic properties and behavior of atoms and molecules. Interestingly, the history of statistical mechanics begins with a mathematical prize at Cambridge in 1855 on the subject of evaluating the motions of Saturn’s rings. (Laplace had developed a mechanical theory of the rings concluding that their stability was due to irregularities in mass distribution.) The prize was won by James Clerk Maxwell who then went on to develop the theory that, without knowing the individual motions of particles (or molecules), it was possible to use their statistical behavior to calculate properties of a gas such as viscosity, collision rate, diffusion rate and the ability to conduct heat. -
Scientific Contributions of the First Female Chemists at the University of Vienna Mirrored in Publications in Chemical Monthly 1
Monatshefte für Chemie - Chemical Monthly (2019) 150:961–974 https://doi.org/10.1007/s00706-019-02408-4 ORIGINAL PAPER Scientifc contributions of the frst female chemists at the University of Vienna mirrored in publications in Chemical Monthly 1902–1919 Rudolf Werner Soukup1 · Robert Rosner1 Received: 29 November 2018 / Accepted: 1 March 2019 / Published online: 29 April 2019 © The Author(s) 2019 Abstract In 1897, the frst female students were admitted at the Faculty of Philosophy at Vienna University. The frst dissertation in chemistry was approved in 1902. In the following years, only one or two women were annually enrolled, while the number of male students of chemistry continuously fuctuated around 22. Whereas four women completed their doctorate in the frst year of WWI, six followed in 1917, and ten more in 1919. Strikingly, in that year the number of female students even exceeded that of male colleagues. Margarethe Furcht, the daughter of a Jewish stockbroker, was the frst female chemist with a doctoral degree certifcate in the Austro-Hungarian Empire. Her paper “Über die Veresterung von Sulfosäuren…”, which she published in 1902 together with her academic supervisor Rudolf Wegscheider, was one of the frst scientifc chemical publications of women in Austria. However, of all female graduates, only a small number worked as chemists within the next two decades. After the occupation of Austria by German Troops in March 1938, seven of the Jewish women managed to emigrate, four were murdered in the Holocaust. Given the importance of this period within the landscape of European scientifc history, we here aim to provide the frst comprehensive overview of the history of women studying chemistry at the University of Vienna. -
Light and the Electromagnetic Spectrum
© Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © JonesLight & Bartlett and Learning, LLCthe © Jones & Bartlett Learning, LLC NOTElectromagnetic FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION4 Spectrum © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALEJ AMESOR DISTRIBUTIONCLERK MAXWELL WAS BORN IN EDINBURGH, SCOTLANDNOT FOR IN 1831. SALE His ORgenius DISTRIBUTION was ap- The Milky Way seen parent early in his life, for at the age of 14 years, he published a paper in the at 10 wavelengths of Proceedings of the Royal Society of Edinburgh. One of his first major achievements the electromagnetic was the explanation for the rings of Saturn, in which he showed that they con- spectrum. Courtesy of Astrophysics Data Facility sist of small particles in orbit around the planet. In the 1860s, Maxwell began at the NASA Goddard a study of electricity© Jones and & magnetismBartlett Learning, and discovered LLC that it should be possible© Jones Space & Bartlett Flight Center. Learning, LLC to produce aNOT wave FORthat combines SALE OR electrical DISTRIBUTION and magnetic effects, a so-calledNOT FOR SALE OR DISTRIBUTION electromagnetic wave. -
Arxiv:Quant-Ph/0510180V1 24 Oct 2005 Einstein and the Quantum
TIFR/TH/05-39 27.9.2005 Einstein and the Quantum Virendra Singh Tata Institute of Fundamental Research Homi Bhabha Road, Mumbai 400 005, India Abstract We review here the main contributions of Einstein to the quantum theory. To put them in perspective we first give an account of Physics as it was before him. It is followed by a brief account of the problem of black body radiation which provided the context for Planck to introduce the idea of quantum. Einstein’s revolutionary paper of 1905 on light-quantum hypothesis is then described as well as an application of this idea to the photoelectric effect. We next take up a discussion of Einstein’s other contributions to old quantum theory. These include (i) his theory of specific heat of solids, which was the first application of quantum theory to matter, (ii) his discovery of wave-particle duality for light and (iii) Einstein’s A and B coefficients relating to the probabilities of emission and absorption of light by atomic systems and his discovery of radiation stimulated emission of light which provides the basis for laser action. We then describe Einstein’s contribution to quantum statistics viz Bose- Einstein Statistics and his prediction of Bose-Einstein condensation of a boson gas. Einstein played a pivotal role in the discovery of Quantum mechanics and this is briefly mentioned. After 1925 Einstein’s contributed mainly to the foundations of Quantum Mechanics. We arXiv:quant-ph/0510180v1 24 Oct 2005 choose to discuss here (i) his Ensemble (or Statistical) Interpretation of Quantum Mechanics and (ii) the discovery of Einstein-Podolsky-Rosen (EPR) correlations and the EPR theorem on the conflict between Einstein-Locality and the completeness of the formalism of Quantum Mechanics. -
1 Historical Background
1 Historical Background 1.1 Introduction The purpose of this chapter is to explain how and why Planck introduced his famous quantum hypothesis and the constant h. I have added a few contributions from Einstein that are relevant for this book. We shall see that results based on the wave nature of light alternate with results based on its corpuscular nature. Eventually, it will be Planck’s constant that will bridge the gap between these two viewpoints and lead to the foundation of quantum physics, unifying the two aspects of light, and much more. But first a warning! This chapter is difficult to read because we are no longer used to thinking and reasoning along the same lines as our prede- cessors. Still, I think that it is of interest to follow the chain that started with Kirchhoff’s second law and ended with Planck’s hypothesis of quan- tized emission of radiation, using the tools available in their time. It gives a flavor of what physics was at that time. It also shows how much we have progressed since then. 1.2 Kirchhoff (1859) 1.2.1 The Birth of Spectroscopy The physicist Kirchhoff1 was collaborating with the chemist Bunsen2 (Fig. 1.1). Out of this collaboration emerged the science of spectroscopy. An early discovery was the phenomenon of spectral line inversion. The experiment is displayed schematically in Fig. 1.2. 1Gustav Robert Kirchhoff (b. Königsberg, 1824; d. Berlin, 1887). 2Robert Wilhelm Bunsen (b. Göttingen, 1811; d. Heidelberg, 1899). Nonlinear Optics: An Analytic Approach. Paul Mandel Copyright © 2010 Wiley-VCH Verlag GmbH & Co. -
Ht2009-88060
Proceedings HT 2009 2009 ASME Summer Heat Transfer Conference July 19-23, 2009, San Francisco, California USA HT2009-88060 A BRIEF HISTORY OF THE T4 RADIATION LAW John Crepeau University of Idaho Department of Mechanical Engineering PO Box 440902 Moscow, ID 83844-0902 USA ABSTRACT he combined his Displacement Law with the T4 law to give a Since the 1700s, natural philosophers understood that heat blackbody spectrum which was accurate over some ranges, but exchange between two bodies was not precisely linearly diverged in the far infrared. dependent on the temperature difference, and that at high Max Planck, at the University of Berlin, built on temperatures the discrepancy became greater. Over the years, Wien’s model but, as Planck himself stated, “the energy of many models were developed with varying degrees of success. radiation is distributed in a completely irregular manner among The lack of success was due to the difficulty obtaining accurate the individual partial vibrations...” This “irregular” or discrete experimental data, and a lack of knowledge of the fundamental treatment of the radiation became the basis for quantum mechanisms underlying radiation heat exchange. Josef Stefan, mechanics and a revolution in physics. of the University of Vienna, compiled data taken by a number This paper will present brief biographies of the four of researchers who used various methods to obtain their data, pillars of the T4 radiation law, Stefan, Boltzmann, Wien and and in 1879 proposed a unique relation to model the Planck, and outline the methodologies used to obtain their dependence of radiative heat exchange on the temperature: the results. -
Chapter 1 Blackbody Radiation
Chapter 1 Blackbody Radiation Experiment objectives: explore radiation from objects at certain temperatures, commonly known as \blackbody radiation"; make measurements testing the Stefan-Boltzmann law in high- and low-temperature ranges; measure the inverse-square law for thermal radiation. Theory A familiar observation to us is that dark-colored objects absorb more thermal radiation (from the sun, for example) than light-colored objects. You may have also observed that a good absorber of radiation is also a good emitter (like dark-colored seats in an automobile). Although we observe thermal radiation (\heat") mostly through our sense of touch, the range of energies at which the radiation is emitted can span the visible spectrum (thus we speak of high-temperature objects being \red hot" or \white hot"). For temperatures below about 600◦C, however, the radiation is emitted in the infrared, and we cannot see it with our eyes, although there are special detectors (like the one you will use in this lab) that can measure it. An object which absorbs all radiation incident on it is known as an \ideal blackbody". In 1879 Josef Stefan found an empirical relationship between the power per unit area radiated by a blackbody and the temperature, which Ludwig Boltzmann derived theoretically a few years later. This relationship is the Stefan-Boltzmann law: S = σT 4 (1.1) where S is the radiated power per unit area (W=m2), T is the temperature (in Kelvins), and σ = 5:6703 × 10−8W=m2K4 is the Stefan's constant. Most hot, opaque objects can be approximated as blackbody emitters, but the most ideal blackbody is a closed volume (a cavity) with a very small hole in it. -
View/Download
SILURIFORMES (part 10) · 1 The ETYFish Project © Christopher Scharpf and Kenneth J. Lazara COMMENTS: v. 25.0 - 13 July 2021 Order SILURIFORMES (part 10 of 11) Family ASPREDINIDAE Banjo Catfishes 13 genera · 50 species Subfamily Pseudobunocephalinae Pseudobunocephalus Friel 2008 pseudo-, false or deceptive, referring to fact that members of this genus have previously been mistaken for juveniles of various species of Bunocephalus Pseudobunocephalus amazonicus (Mees 1989) -icus, belonging to: Amazon River, referring to distribution in the middle Amazon basin (including Rio Madeira) of Bolivia and Brazil Pseudobunocephalus bifidus (Eigenmann 1942) forked, referring to bifid postmental barbels Pseudobunocephalus iheringii (Boulenger 1891) in honor of German-Brazilian zoologist Hermann von Ihering (1850-1930), who helped collect type Pseudobunocephalus lundbergi Friel 2008 in honor of John G. Lundberg (b. 1942), Academy of Natural Sciences of Philadelphia, Friel’s Ph.D. advisor, for numerous contributions to neotropical ichthyology and the systematics of siluriform and gymnotiform fishes Pseudobunocephalus quadriradiatus (Mees 1989) quadri-, four; radiatus, rayed, referring to four-rayed pectoral fin rather than the usual five Pseudobunocephalus rugosus (Eigenmann & Kennedy 1903) rugose or wrinkled, referring to “very conspicuous” warts all over the skin Pseudobunocephalus timbira Leão, Carvalho, Reis & Wosiacki 2019 named for the Timbira indigenous groups who live in the area (lower Tocantins and Mearim river basins in Maranhão, Pará and -
Icilio Guareschi and His Amazing “1897 Reaction”
Icilio Guareschi and his amazing “1897 reaction” Gian Cesare Tron*1, Alberto Minassi1, Giovanni Sorba1, Mara Fausone2 and Giovanni Appendino*1 Review Open Access Address: Beilstein J. Org. Chem. 2021, 17, 1335–1351. 1Dipartimento di Scienze del Farmaco, Università degli Studi del https://doi.org/10.3762/bjoc.17.93 Piemonte Orientale, Largo Donegani 2, 28100 Novara, Italy and 2Sistema Museale di Ateneo, Archivio Scientifico e Tecnologico Received: 02 February 2021 dell'Università di Torino, C.so Massimo D'Azeglio 52, 10126 Torino, Accepted: 04 May 2021 Italy Published: 25 May 2021 Email: Associate Editor: J. S. Dickschat Gian Cesare Tron* - [email protected]; Giovanni Appendino* - [email protected] © 2021 Tron et al.; licensee Beilstein-Institut. License and terms: see end of document. * Corresponding author Keywords: Guareschi; history of chemistry; hydrocarbons; name reactions; pyridine Abstract Organic chemistry honors Icilio Guareschi (1847–1918) with three eponymic reactions, the best known ones being the Guareschi synthesis of pyridones and the Guareschi–Lustgarten reaction. A third Guareschi reaction, the so-called “Guareschi 1897 reaction”, is one of the most unusual reactions in organic chemistry, involving the radical-mediated paradoxical aerobic generation of hydro- carbons in near-neutral water solution. A discussion of the mechanism of this amazing reaction, the only metal-free process that generates hydrocarbons, and the implications of the approach in biology and geosciences mirrors the multifaceted scientific person- ality of the discoverer. Thus, Guareschi’s eclectic range of activities spans a surprising variety of topics, overcoming the bound- aries of the traditional partition of chemistry into organic, inorganic, and analytical branches and systematically crosses the divide between pure and applied science as well as between the history of chemistry and the personal contributions to its development. -
Dr. Paolo G. ALBANO, Phd Professional Profile
Dr. Paolo G. ALBANO, PhD Institutional address: Department of Paleontology, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria E-mail: [email protected] Website: http://homepage.univie.ac.at/paolo.albano/index.html ORCID identifier: 0000-0001-9876-1024; ResearchGate, Google Scholar Languages: Italian: mother tongue; English: Proficient (C2, certified 10 January 2012); German: Intermediate (B1). Number of papers: 32 (I am first or last author of 72%), h-index: 7, Total citations: 161 (Scopus extraction 6 June 2018) Professional profile Research themes Historical ecology of ecosystems affected by biological invasions Environmental assessment when pristine controls are not available Patterns of biodiversity, rarity and singularity in the Indo-Pacific province Climate change forcing on marine species distribution in the Mediterranean Sea Taxonomy of marine molluscs Education 2011 University of Bologna, Department of Experimental Evolutionary Biology. PhD in Biodiversity & Evolution. Thesis: “Molluscs of the Marine Protected Area ‘Secche di Tor Paterno’”. 2001 University of Bologna, Degree in Environmental Engineering cum laude. Experimental thesis on the “Mo.S.E.” project for the protection of the Venice Lagoon from exceptionally high tides Scientific and professional experience 2016 – Senior post-doctoral researcher, Principal Investigator University of Vienna, Department of Paleontology, Austria Project “Historical ecology of Lessepsian migration”, funded by the Austrian Science Fund 2016 Curatorial appointment Natural History Museum, Vienna, Austria Digitalization project of the invertebrate collections: taxonomic expert for Mollusca. Two month full-time contract. 2013 – 2015 Post-doctoral researcher (Marie Curie fellow) University of Vienna, Department of Paleontology, Austria Project “Conservation palaeobiology of oil-polluted tropical marine biota”, funded by the European Commission with a Marie Curie Intra-European Fellowship (scientist in charge: Prof. -
Bibliographie Nach-Linneischer Literatur Über Die Mollusken Österreichs, II
Bibliographie nach-linneischer Literatur über die Mollusken Österreichs, II. (Stand 31. Dez. 2018) Von ALEXANDER REISCHÜTZ, PETER L. REISCHÜTZ & WOLFGANG FISCHER Horn - Wien 2019. © Erste Vorarlberger Malakologische Gesellschaft, Sulzerweg 2, A-6830 Rankweil, Österreich. Januar 2019 Autoren: Alexander Reischütz, Untere Augartenstraße 7/2/24, A-1020 Wien, Österreich. Peter L. Reischütz, Puechhaimg. 52, A-3580 Horn, Österreich. Wolfgang Fischer, Martnigasse 26, A-1220 Wien, Österreich. Bibliographie nach-linneischer Literatur über die Mollusken Österreichs, II. (Stand 31. Dez. 2018). Von ALEXANDER REISCHÜTZ, PETER L. REISCHÜTZ & WOLFGANG FISCHER, Horn - Wien. Vorwort Diese Bibliographie zeigt, dass in Österreich mit minimalen Ausnahmen nie eine naturschutzrelevante Kartierung der Molluskenfauna stattgefunden hat. Zukünftige Kartierungen werden nach den Erfahrungen der Autoren bis auf wenige Ausnahmen einen erschütternden Zustand der Biotope dieser Tiergruppe aufzeigen. „Mit dem Ausscheiden von R. STURANY (gest. 1935) aus dem aktiven Dienst beendete die offizielle Malakologie ihre Beteiligung an der Vermehrung unseres Wissens über die Weichtiere Österreichs, die bis auf weiteres fast ausschließlich von Privatpersonen getragen wurde“ (W. KLEMM in einem Gespräch mit dem Seniorautor im Dezember 1973). Während unserer Arbeiten über die Mollusken Österreichs machte sich immer wieder das Fehlen einer brauchbaren Bibliographie bemerkbar, obwohl in FRAUENFELD 1855, STURANY 1900, KLEMM 1960 und 1974, FRANK 1976 und anderen zahlreiche Literaturzitate angeführt sind. Die Überprüfung aller bis dahin zitierten Arbeiten erwies sich als notwendig, weil immer wieder Arbeiten ohne Bezug zu Österreich - oft marine Literatur und häufig auch Arbeiten über andere Tiergruppen (Insekten, Krebse, Würmer, ...) - in den Molluskenbibliographien zitiert und nicht überprüft oder falsch abgeschrieben wurden. Dadurch kam es zu langen Verzögerungen durch erhöhten zeitlichen Aufwand. -
Museum of Comparative Zoölogy
SENATE. No. 252 ANNUAL REPORT OF THE TRUSTEES OF THE MUSEUM OF COMPARATIVE ZOÖLOGY, AT HARVARD COLLEGE, IN CAMBRIDGE: TOGETHER WITH THE REPORT OF THE DIRECTOR FOR 1872. BOSTON: WRIGHT & POTTER, STATE PRINTERS, 19 Province Street. 1 8 73. CmnmomDcaltl) of itlassadjiisctts. Boston, Mass., June 4, 1873. To the Hon. George B. Loring, President of the Senate. Sir .-—The Trustees of the Museum of Comparative Zoology have the honor to present to the Legislature the Annual Report of the Director, for the past year, marked [A]. The paper marked [B] contains a list of the Trustees, offi- cers and committees for 1873. Respectfully submitted, for the Trustees, MARTIN BRIMMER, Secretary. 4 COMPARATIVE ZO-OLOGY. [June, [A.] REPORT OF THE DIRECTOR OF THE MUSEUM OE COMPARATIVE ZOOLOGY, For the Year 1872. It gives me the greatest pleasure to state that my absence, though extended to nearly a year, has not in the slightest degree interfered with the progress of the Museum. Mr. Cary, the Superintendent, has directed the business of our Institution with so much ability, forethought and diligence, anticipating and providing for the needs of each working department, that there have been no unnecessary delays or interruptions. His special Report contains the details of his administration. The scientific officers of the Museum have shown the utmost zeal and fidelity, carrying on the work of the separate laboratories so efficiently that I can truly say the results of the year have far exceeded my most sanguine expectations. There is one inference to be drawn from this statement which is of great importance, though few perhaps can value it as highly as Ido myself.