Olmsted, Denison
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Severe Space Weather
Severe Space Weather ThePerfect Solar Superstorm Solar storms in +,-. wreaked havoc on telegraph networks worldwide and produced auroras nearly to the equator. What would a recurrence do to our modern technological world? Daniel N. Baker & James L. Green SOHO / ESA / NASA / LASCO 28 February 2011 !"# $ %&'&!()*& SStormtorm llayoutayout FFeb.inddeb.indd 2288 111/30/101/30/10 88:09:37:09:37 AAMM DRAMATIC AURORAL DISPLAYS were seen over nearly the entire world on the night of August !"–!&, $"%&. In New York City, thousands watched “the heavens . arrayed in a drapery more gorgeous than they have been for years.” The aurora witnessed that Sunday night, The New York Times told its readers, “will be referred to hereafter among the events which occur but once or twice in a lifetime.” An even more spectacular aurora occurred on Septem- ber !, $"%&, and displays of remarkable brilliance, color, and duration continued around the world until Septem- ber #th. Auroras were seen nearly to the equator. Even after daybreak, when the auroras were no longer visible, disturbances in Earth’s magnetic fi eld were so powerful ROYAL ASTRONOMICAL SOCIETY / © PHOTO RESEARCHERS that magnetometer traces were driven off scale. Telegraph PRELUDE TO THE STORM British amateur astronomer Rich- networks around the globe experienced major disrup- ard Carrington sketched this enormous sunspot group on Sep- tions and outages, with some telegraphs being completely tember $, $()*. During his observations he witnessed two brilliant unusable for nearly " hours. In several regions, operators beads of light fl are up over the sunspots, and then disappear, in disconnected their systems from the batteries and sent a matter of ) minutes. -
Tarheel Junior Historian
Tar Heel Junior Historian Association Carolina's Mountain Region History Journal For Inquiring Students A Fall 197 tar heel junior historian Gltaitel Gltallie's QltaU The Tar Heel Junior Historian Association is making history this year by celebrating its twenty-fifth anniversary. Special plans are being made for the "biggest and best" Awards Day ever. It will be held at Meredith College in Raleigh on May 18 and 19. You can start now by making a placard on poster board paper with Placard means a notice, your club name on it. This placard should be 14 inches high usually displayed on by 22 inches wide. Use your imagination to draw a design a sign or poster. that represents either your club or the historical events associated with your community. Prizes will be given for outstanding ones. Also, newly designed membership cards and special Tar Heel Junior Historian recruiting posters will soon be sent to you. Use them to help us recruit new members in this special anniversary year! Visual history is both an exciting detective game and a learning experience for junior historians. Service to the community is its own reward. Junior historians have put many thousands of hours into such work and have received national recognition for their efforts. To help you to plan for the coming Awards Day and to remind you of all the activities of last May, be sure to read the article "Awards Day 1977" in this issue. In that article, please pay particular attention to the ideas for Recruit means to get or enlist. -
Wiki Template-1Eb7p59
Wikipedia Reader https://en.wikipedia.org/wiki/Aurora Selected by Julie Madsen - Entry 10 1 Aurora From Wikipedia, the free encyclopedia An aurora, sometimes referred to as a polar lights or north- ern lights, is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions.[1] Au- roras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (ther- mosphere/exosphere), where their energy is lost. The resulting ion- ization and excitation of atmospheric constituents emits light of varying color and complexity. The form of the aurora, occur- ring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating parti- cles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton Images of auroras from around the world, auroras are usually observed at including those with rarer red and blue lower latitudes.[2] lights Wikipedia Reader 2 May 1 2017 Contents 1 Occurrence of terrestrial auroras 1.1 Images 1.2 Visual forms and colors 1.3 Other auroral radiation 1.4 Aurora noise 2 Causes of auroras 2.1 Auroral particles 2.2 Auroras and the atmosphere 2.3 Auroras and the ionosphere 3 Interaction of the solar wind with Earth 3.1 Magnetosphere 4 Auroral particle acceleration 5 Auroral events of historical significance 6 Historical theories, superstition and mythology 7 Non-terrestrial auroras 8 See also 9 Notes 10 References 11 Further reading 12 External links Occurrence of terrestrial auroras Most auroras occur in a band known as the auroral zone,[3] which is typically 3° to 6° wide in latitude and between 10° and 20° from the geomagnetic poles at all local times (or longitudes), most clearly seen at night against a dark sky. -
7 X 11 Long.P65
Cambridge University Press 978-0-521-85349-1 - Meteor Showers and their Parent Comets Peter Jenniskens Excerpt More information Part I Introduction © Cambridge University Press www.cambridge.org Cambridge University Press 978-0-521-85349-1 - Meteor Showers and their Parent Comets Peter Jenniskens Excerpt More information 1 How meteor showers were linked to comets When we wish upon a falling star, we appeal to an ancient belief that the stars represent our souls and a meteor is one falling into the hereafter.1 In Teutonic mythology, for example, your star was tied to heaven by a thread, spun by the hands of an old woman from the day of your birth, and when it snapped, the star fell and your life had ended.2 The Greek philosophers were the first to speculate on the nature of things without regard to ancient myths. Especially the world views of Aristotle of Stagira (384–322 BC) in his 350 BC book Meteorology3 were widely quoted for over two thousand years, embraced by Christian religion, and passionately defended until into the eight- eenth century. The Greeks held that all matter in the Universe is made of the elements ‘‘earth,’’ ‘‘water,’’ ‘‘air,’’ and ‘‘fire.’’ Aristotle was of the opinion that shooting stars, because of their rapid motion, occurred relatively nearby in the realm of the element ‘‘fire’’ above the layer of ‘‘air’’ that is now called our atmosphere. He believed that shooting stars were not caused by the falling of stars, but were caused by thin streams of a warm and dry ‘‘windy exhalation’’ (a mixture of the elements fire and air) that had risen from dry land warmed by the Sun. -
GEOMAGNETISM -A HISTORICAL REVIEW Sashikanth Rapeti
GEOMAGNETISM -A HISTORICAL REVIEW Sashikanth Rapeti To cite this version: Sashikanth Rapeti. GEOMAGNETISM -A HISTORICAL REVIEW. 2020. hal-02901860 HAL Id: hal-02901860 https://hal.archives-ouvertes.fr/hal-02901860 Preprint submitted on 17 Jul 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. GEOMAGNETISM – A HISTORICAL REVIEW R. Sashikanth Assistant Professor and Head of the Department Department of Physics and Space Sciences Gandhi Institute of Technology and Management, Gangapada, Bhubhaneshwar, Odisha, India. E-mail : [email protected], [email protected] [email protected], [email protected] Abstract : This specific paper addresses the historical events that had led in the current scenario, to the development of one of the most important fundamental research areas – Geomagnetism, which might even date back to probably millions of years embedded in the core scientific aspects of even ancient civilizations. The solar wind and its associated magnetic field have their source in the Sun and their interaction with the geo-magnetic field which extends into outer space has its origin inside the earth’s core. Needless to say, the contributions of many scientific researchers on the dynamics of upper, middle and lower atmospheres of the earth is really outstanding and remarkable, but certain important aspects appear to have been missed. -
47 February 1999
HeA. D. News The Newsletter of the Historical Astronomy Division of the American Astronomical Society Number 47 February 1999 Kristv Kaiser. Manson. Iowa (original charcoal) -1- Biennial History of Persons wishing to register should contact: Astronomy, Center for ContinuingEducation, Astronomy Workshop, To Be University of Notre Dame, Notre Dame, IN Co-sponsored by the HAD 46556, E-mail: [email protected]. The registration fee of $70 includes the cost of the Steven Dick banquet. Housing is available in new air- conditioned dormitories at $27 per night for a The Fourth Biennial History of Astronomy single, $21 per night for a double. Workshop will be held July 1-4, 1999 at the University of Notre Dame. The workshop is The conference will include a book exhibit sponsored by Notre Dame's Graduate Program and display tables. Participants are welcome to in History and Philosophy of Science, Notre bring materials to display. Contact Matt Dame's Reilly Center for Science, Technol- Dowd with regard to how much space will be ogy, and Values, the History of Astronomy needed. Special Interest Group of the History of Science Society, and theHistorica1Astronomy Regarding transportation, flights come to Division of the American Astronomical South Bend from a number of major cities. Society. Persons arriving via Chicago can take the United Limo Bus, which runs from the United Steven Dick and Michael Crowe are program Terminal at 0'1-Iare Airport directly to the co-chairs. Persons wishing to present work- Notre Dame campus. Round-trip fare is $52. in-progress papers, or poster papers, should For a schedule and reservations, call United submit a title and abstract of approximately Limo at (800) 833-5555. -
Olmsted 200 Bicentennial Notes About Olmsted Falls and Olmsted Township – First Farmed in 1814 and Settled in 1815 Issue 42 November 1, 2016
Olmsted 200 Bicentennial Notes about Olmsted Falls and Olmsted Township – First Farmed in 1814 and Settled in 1815 Issue 42 November 1, 2016 Contents November Meteors Have Connection to Olmsted History 1 Sesquicentennial Coin Turns Up 7 Did Peltzes Move to California for Their Health? 8 Chestnut Grove Will Host Veterans Day Ceremony 10 Still to Come 11 November Meteors Have Connection to Olmsted History If the nighttime sky is dark enough and clear enough around the middle of November and you happen to see one or more meteors – or “shooting stars” – you might be witness to a portion of one of the best-known annual meteor showers. But maybe you didn’t know – until now – about that meteor shower’s connection to the family for whom Olmsted Falls and Olmsted Township, as well as North Olmsted, are named. Meteor showers occur when the Earth, in its orbit around the sun, encounters streams of particles. Those particles are left in the wake of comets in their trips from the edges of the solar system to close passes by the sun and then back to the outer realms. The Earth experiences several meteor showers of varied intensity each year. One of the best- known meteor showers is the Perseids, partly because they reliably provide an average of about one meteor each minute at their peak. It’s also partly because they occur in mid-August, when the weather is warm enough that it is comfortable for observers to stay outside for long periods NASA released this photo of the Leonids as in the middle of the night. -
Kenneth Raper, Elisha Mitchell And<Emphasis Type="Italic
Perspectives Kenneth Raper, Elisha Mitchell and Dictyostelium EUGENE R KATZ Department of Molecular Genetics and Microbiology, Stony Brook University, Stony Brook, NY 11794, USA (Email, [email protected]) 1. Introduction forms the fruiting body. The fruiting body, a small plant-like structure about a millimetre tall, basically consists of only Dictyostelium discoideum has become an important organism two kinds of cells, stalk cells in the stalk and spore cells con- in the study of modern cellular and developmental tained in a droplet of liquid above the stalk. Although mod- biology (Kessin 2001). The most recent International ern work has shown that there are several cellular subtypes, Dictyostelium Conference, held outside Grenoble, France Raper’s view was essentially correct. Furthermore, under a last summer, was attended by more than 150 scientists from given set of nutritional and environmental conditions, the thirteen countries. D. discoideum is a member of a group of ratio of spore cells to stalk cells in the fruiting body is fixed, organisms known as the cellular slime moulds. Cellular with spores representing about 80% of the cells and stalk slime moulds were first described in the second half of cells 20%. Since both spore cells and stalk cells derive from the nineteenth century but their potential as model organisms amoebae, Raper was interested in understanding how the only began to be appreciated with the isolation of the amoebae made the decision about which of the two cell types D. discoideum species by Kenneth Raper in 1933. Raper was, to become. He thought it could be a model for how cell fate at the time, working for the United States Department of decisions are made during the embryogenesis of higher Agriculture as a mycologist. -
Between Two Empires: the Toronto Magnetic Observatory and American Science Before Confederation"
Article "Between Two Empires: the Toronto Magnetic Observatory and American Science before Confederation" Gregory Good Scientia Canadensis: Canadian Journal of the History of Science, Technology and Medicine / Scientia Canadensis : revue canadienne d'histoire des sciences, des techniques et de la médecine , vol. 10, n° 1, (30) 1986, p. 34-52. Pour citer cet article, utiliser l'information suivante : URI: http://id.erudit.org/iderudit/800224ar DOI: 10.7202/800224ar Note : les règles d'écriture des références bibliographiques peuvent varier selon les différents domaines du savoir. Ce document est protégé par la loi sur le droit d'auteur. L'utilisation des services d'Érudit (y compris la reproduction) est assujettie à sa politique d'utilisation que vous pouvez consulter à l'URI https://apropos.erudit.org/fr/usagers/politique-dutilisation/ Érudit est un consortium interuniversitaire sans but lucratif composé de l'Université de Montréal, l'Université Laval et l'Université du Québec à Montréal. Il a pour mission la promotion et la valorisation de la recherche. Érudit offre des services d'édition numérique de documents scientifiques depuis 1998. Pour communiquer avec les responsables d'Érudit : [email protected] Document téléchargé le 14 février 2017 07:54 34 BETWEEN TWO EMPIRES: THE TORONTO MAGNETIC OBSERVATORY AND AMERICAN SCIENCE BEFORE CONFEDERATION* Gregory Good** (Received 20 November 1985. Revised/Accepted 19 May 1986) PERSPECTIVES ON THE TORONTO MAGNETIC OBSERVATORY The Magnetic Observatory was founded at Toronto in 1839 as part of the worldwide magnetic Crusade of the British Association for the Advancement of Science and the Royal Society of London.1 Although it was a focus of scientific research and of institutional development in Canada for decades, little attention has been given to it. -
Denison Olmsted (1791-1859), Scientist, Teacher, Christian: a Biographical Study of the Connection Of
AN ABSTRACT OF THE THESIS OF Gary Lee Schoepflin for the degree ofDoctor of Philosophy in General Science presented on June 17, 1977 Title:DENISON OLMSTED (1791-1859), SCIENTIST, TEACHER, CHRISTIAN: A BIOGRAPHICAL STUDY OF THE CONNECTION OF SCIENCE WITH RELIGION IN ANTEBELLUM AMERICA Redacted for Privacy Abstract approved: Danie JJ one s A biographical study of Denison Olmsted, focusing upon his own Christian world view and its connection with his various activities in science, supports the view that religion served as a significant factor in the promotion of science in America during this time period. Olmsted taught physics, meteorology and astronomy at Yale from 1826 to 1859, and from this position of influence, helped mold the minds and outlook of a new generation of scientists, of hundreds of students who came to Yale to obtain a liberal educa- tion, and of those members of society who attended his popular lectures.Olmsted's personal perspective was that science was God-ordained, that it would ever harmonize with religion, that it was indeed a means of hastening the glorious millennium. Olmsted lived in an era characterized by an unprecedented revivalism and emphasis upon evangelical Christianity. He graduated from Yale (1813) at a time when its president, Reverend Dr. Timothy Dwight, one of the most influential clergymen in New England, was at the height of his fame. Olmsted subsequently studied theology under Dwight, but before completing his prepara- tion for the ministry, Olmsted was appointed to a professorship of science at the University of North Carolina where he taught from 1818 until he was called to Yale in 1826. -
George P. Merrill Collection, Circa 1800-1930 and Undated
George P. Merrill Collection, circa 1800-1930 and undated Finding aid prepared by Smithsonian Institution Archives Smithsonian Institution Archives Washington, D.C. Contact us at [email protected] Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Historical Note.................................................................................................................. 1 Descriptive Entry.............................................................................................................. 2 Names and Subjects ...................................................................................................... 3 Container Listing ............................................................................................................. 4 Series 1: PHOTOGRAPHS, CORRESPONDENCE AND RELATED MATERIAL CONCERNING INDIVIDUAL GEOLOGISTS AND SCIENTISTS, CIRCA 1800-1920................................................................................................................. 4 Series 2: PHOTOGRAPHS OF GROUPS OF GEOLOGISTS, SCIENTISTS AND SMITHSONIAN STAFF, CIRCA 1860-1930........................................................... 30 Series 3: PHOTOGRAPHS OF THE UNITED STATES GEOLOGICAL AND GEOGRAPHICAL SURVEY OF THE TERRITORIES (HAYDEN SURVEYS), CIRCA 1871-1877.............................................................................................................. -
On the Equilibrium of Heterogeneous Substances
: TRANSACTIONS CONNECTICUT ACADEMY OF ARTS AND SCIENCES. VOX^XJJVIE III t7> NEW H AYEN PUBLISHED BY THE ACADEMY, 1874 to 1878. TulUr, Murehouse 4 Taylor, Printers, New Ha ———— CONTENTS. PAGE List of Additions to the Library,..,. v Art. I. —Report on the dredgings in the region of St. George's Banks, in 1872. By S. I. Smith and O. Harger. Plates 1 -8, 1 Art. IL—Descriptions op new and rare species of Hy- DROIDS from the NeW EnGLAND COAST. By S. F, Clark. Plates 9-10, 58 Art. III. On the Chondrodite from the Tilly-Foster IRON mine, Brewster, N. Y, By E. S. Dana, Plates 11-13, 67 Art. IV. On the Transcendental curves sin y sin iny=. a sin ic sin ??a; -|- ^''- By II. A. Newton and A. W. Philips. Plates 14-37, 97 Art. V. On the equilibrium of heterogeneous sub- stances. By J. W. Gibbs. First Part, 108 Art. VI. The Hydroids of the Pacific coast of the United States south of Vancouver Island, with a report upon those in the Museum of Yale Coixege. By S. F. Clark. Plates 38-41, 249 Art. VII. On the anatomy and habits of Nereis virens. By Y. M, Turnbull. Plates 42-44, 265 Art. VIII. Median and paired fins, a contribution to the history of vertebrate limbs. By J. K. Thacher, Plates 49-60, 281 Art. IX. Early stages op Hippa talpoida, with a note ON THE structure OF THE MANDIBLES AND MAXILLJE IN Hipp A and Remipes. By S. I. Smith. Plates 45-48, 311 Art.