Johann Von Lamont (1805-1879): a Pioneer in Geomagnetism

Total Page:16

File Type:pdf, Size:1020Kb

Johann Von Lamont (1805-1879): a Pioneer in Geomagnetism Inside... Visiting Fellow Reports 2 Current Abstracts 4 new Visiting Fellows 7 IRM news 11 Winter 2004-5, Vol. 14, No. 4 Johann von Lamont (1805-1879): A pioneer in geomagnetism In 2005 we can commemorate the 200th Heinrich Soffel birthday of Johann von Lamont (Fig. 1), Prof. Emeritus a pioneer in geomagnetism in the middle University of of the 19th century. He belonged to the München group around Gauss, von Humboldt, Sabine, Angström and others (forming the Göttingen Magnetic Union) who established within a few years an international network of geomagnetic observatories around the word (Barraclough et al., 1992) upon which much of our present day knowledge about the geomagnetic field rests. Johann von Lamont was born as John Lamont on 15 December 1805 in Corriemulzie near Braemar in Central Fig. 1. Portrait of Johann von Lamont from 1856 showing him at the age of 50. of Johann von Lamont from Fig. 1. Portrait Scotland. His father, Robert Lamont, was a forester and administrator to James, the second Earl of Five. When Robert engineering which helped him later in the the Observatory in 1835 at the age of 29. Lamont died suddenly in 1816 from an construction and production of instru- More details about the Lamont family, accident with his horse the family had to ments for observatory and field work. the life and the scientific career of search for a sponsor who could take care Since 1827 he spent most of the time of Johann von Lamont can also be taken of the education of the bright 12 year old his vacations as a student in the Royal from Wienert (1966) and Beblo & Soffel boy John. In 1817, Father Gallus Astronomical Observatory which had (1991). Robertson, the dean of the Scottish been built in 1816-1817 in Bogenhausen, The early 1830’s were very Monastery St. James from Regensburg in at that time a small village close to important for geomagnetism due to the Bavaria visited Scotland in search of Munich. In 1828 he was appointed as an initiatives of Carl Friedrich Gauss and talented students for his monastery assistant in the observatory and in 1830 Alexander von Humboldt. During his school. John received a fellowship and he got a PhD at the University of expeditions, which led him to remote was taken to Regensburg for an educa- Munich. Due to the bad health of the parts of our globe, von Humboldt had tion in theology and sciences. However, director of the observatory, Georg von recognised that the origin of the spatial the main interests of the boy were not in Soldner, Lamont was soon in charge of and temporal variations of the geomag- theology but in mathematics and natural doing all the astronomical routine work. netic field could only be investigated by sciences. This was soon recognized by When von Soldner died in 1833 Lamont world-wide simultaneous and permanent Father Benedict Deasson, one of his was on his own and entirely responsible. observations in a global network of teachers, and John was trained in these He was finally appointed as director of Lamont disciplines including also mechanical 1 continued on p. 8... Visiting Fellows’ Reports decreased sharply in passing through the reduce or partially remove the internal Magnetic Memory in MD strains and stresses produced by crystal Morin transition (TM). At TM, 97% of the Hematite original SIRM is demagnetized with the defects. A large single crystal of Özden Özdemir disappearance of spin-canting and the hematite (6 mm) was heated in zero field University of Toronto In previous years at the IRM, I onset of c-axis antiferromagnetism. in air at 600°C for 3 and 5 hours. I used [email protected] a Schoenstedt thermal demagnetizer to studied low-temperature demagnetization Between TM and 20 K, there was no of TRM and SIRM of natural single further demagnetization. The residual 3% anneal the crystal in zero field. The crystals of hematite with grain sizes of the original remanence remained sequence of the annealing experiments between 1-6 mm. The zero-field cooling constant. In warming back though the was: (1) thermally demagnetize the and warming curves of SIRM for a 4 mm Morin transition, 43% of the original crystal at 705°C, anneal for 3 hours; (2) hematite crystal are shown in Figure 1. remanence was recovered. This value is produce 0.1 mT TRM and measure M ; (3) LTD by cooling the crystal to In cooling from 300 K, the remanence much higher than the SIRM memory TR ratios of 30-32% measured for SD 77 K in liquid N2 and measure the TRM hematites with grain sizes memory; (4) repeat (1) to (4) for 5-hour 1.0 between 0.12-0.23 µm. annealing experiments. The intensity of TRM decreased 7% At TM, as spins rotate from the (0001) plane to the c-axis, after 3-hours annealing. However, the 0.8 intensity of the TRM memory was α -Fe O the magnetocrystalline 23 anisotropy constant passes reduced much more. After 3-hours (300) Single crystal through zero and changes sign. annealing, the crystal had a 30% lower 0.6 In MD hematite, domain walls TRM memory. Five hours annealing HSIRM // (0001) blocked by magnetocrystalline had further effect on the memory: about controlled pinning become free 2/3 of the initial memory was retained. 0.4 to jump and lead to demagneti- It appears that annealing reduced the SIRM SIRM zation of a large fraction of the number of strain centers but did not M/M original SIRM. The remaining completely remove all of them. The 0.2 43% of the room-temperature memory must be due to strongly pinned SIRM was not destroyed by domain walls, probably pinned magneto- cycling through T . strictively by dislocations or other 0 M 0 50 100150 200 250 300 This year at the IRM, I crystal defects. investigated the effect of I would like to thank Mike, Peat, Temperature, T (K) annealing on the TRM Ramon and Thelma for their help and memory. Annealing could hospitality. Normalized zero-field cooling and warming curves of SIRM for a 4 mm single crystal of hematite. Field is applied along (0001). Guillaume Plenier However, complex fabrics (those that fraction of super paramagnetic (SP) grains. Cooling the sample below the IPGP and CNRS Origin of complex magnetic differ significantly from the normal case) SP-blocking temperature would lead to [email protected] appear to be more prevalent than is fabrics an increase in the fraction of single and generally accepted. Indeed, entire sites can yield a single well-defined complex domain grains that would, in turn, Jonathan Glen The aim of our visit was to determine fabric. As a result, independent flow change the sample’s AMS fabric U. S. Geological Survey what factors control complex fabrics in indicators (e.g., vesicle orientation or (driving it towards an inverse fabric) and [email protected] igneous rocks, and to assess whether petrofabric studies) are needed to allow one to infer the flow direction. magma flow directions could be confidently infer magma flow directions. To test this idea, we applied an recovered from them. Interestingly, some of the most existing high-field method (Ferré et al., commonly observed complex fabrics are 2000; Thill et al. 2000; Kelso et al. Introduction ones that mimic the normal case, in that 2002), for the first time, at low tempera- Until recently, studies of the the AMS axes are aligned with the flow tures. In addition we performed anisotropy of magnetic susceptibility coordinates but are flipped with respect to magnetic mineral identification, based (AMS) of dikes and lavas have largely each other (Figure 1). One of the most on low-temperature crystallographic assumed a simple relation between the compelling explanations for these transitions using an MPMS, and principal AMS directions and magma “permuted” fabrics involves mixtures of determination of magnetic grain size, flow. In the so-called “normal” magnetic single domain and multidomain grain with the use of hysteresis curves, FORC fabric case, the magnetic foliation sizes (Rochette et al., 1992; Ferré, 2002). distribution analyses, and low-tempera- mimics the flow plane (i.e., the AMS Assuming grain size mixtures are ture AC-susceptibility measurements, to minimum — Kmin, which is the normal responsible for these permuted fabrics, assess the actual factors responsible for to the foliation plane, lies perpendicular one might be able to recover the true flow the permuted fabrics. to a dike’s walls or to a lava’s bottom) direction by isolating the influence of the Two sets of samples yielding and the magnetic lineation (given by the different grain size fractions on the permuted fabrics were studied: mid- AMS maximum — Kmax) parallels the magnetic fabric. It might be particularly Miocene dikes from the Roberts magma flow direction. Mountains, NV (eastern Northern 2 appropriate for samples containing some Normal flow coordinates Kmax flow Kmin direction K1 K3 LTHFASR - small cube Kint K2 K1 Max Specimen 0110 N AMS paleomag specimen dike walls or flow top and bottom K2 Int (parallel to flow plane) K3 Min Normal Flat Normal Fin MD 300a K2-K3 flip 200 175 np + ip: Rochette et al. , 1992 100 300b 25 AMS 200 300a AMS 300b 175 Intermediate Flat Intermediate Fin K1-K2 flip 3-axis flip 100 25 100 200 25 Inverse Parallel Inverse Perpendicular 175 300a 300b 3-axis flip K1-K3 flip AMS Figure 2: Comparison of the LTHFASR measurements (in color) at different temperatures no + ip: Rochette et al. , 1992 (in °K) with the low-field room-temperature AMS (black) fabric for the specimen 0110 from the Black Butte locality (Oregon).
Recommended publications
  • Goodman, Matthew (2018) from 'Magnetic Fever' to 'Magnetical Insanity': Historical Geographies of British Terrestrial Magnetic Research, 1833- 1857
    Goodman, Matthew (2018) From 'magnetic fever' to 'magnetical insanity': historical geographies of British terrestrial magnetic research, 1833- 1857. PhD thesis. https://theses.gla.ac.uk/30829/ Copyright and moral rights for this work are retained by the author A copy can be downloaded for personal non-commercial research or study, without prior permission or charge This work cannot be reproduced or quoted extensively from without first obtaining permission in writing from the author The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given Enlighten: Theses https://theses.gla.ac.uk/ [email protected] From ‘magnetic fever’ to ‘magnetical insanity’: historical geographies of British terrestrial magnetic research, 1833-1857 Matthew Goodman Submitted in fulfilment of the requirements for the Degree of Doctor of Philosophy (PhD) School of Geographical and Earth Sciences College of Science and Engineering University of Glasgow Contents Abstract................................................................................................................................................................ 5 List of Figures .................................................................................................................................................... 6 Acknowledgements .........................................................................................................................................
    [Show full text]
  • Fischer, the Scots in Germany
    The Scots in Germany http://studienstelleog.de/download/ScotsGermany_Fischer.pdf The Scots in Germany - Preface http://studienstelleog.de/download/ScotsGermany_Fischer.pdf The Scots in Germany The Scots in Germany Being a contribution towards the history of the Scot abroad Preface by Th A Fischer (first published in 1902) My thanks for Gregory Lauder-Frost for making this book available to us. WHEN I several years ago commenced to write this book, voices were not wanting advising me to abandon the idea, chiefly on account of the vast area from which the material had to be gathered and the almost total want of preparatory inquiry into this particular branch of Scottish History. l Preface l Commerce and Trade - Part 1 When I nevertheless persevered in my task, though experiencing to the full the truth of those l Commerce and Trade - Part 2 Cassandra voices, it was owing not only to an interest which warmed with the increasing difficulties, l The Army - Part 1 but to the very kind and active help that friends of historical research both in Scotland and in l The Army - Part 2 Germany have afforded me in supplying copies of records or other sources of information, or in l The Church - Part 1 reading proofs, or in acting as guides through the labyrinths of their libraries. It would be too long to l The Church - Part 2 mention their names; my thanks are due to them all, in particular to the librarians and keepers of records in Edinburgh, Glasgow, Aberdeen, St Andrews, Fort Augustus, Dundee, and in half a l Statesman and Scholar hundred places in Sweden, Germany and Austria.
    [Show full text]
  • From William Hyde Wollaston to Alexander Von Humboldt
    This article was downloaded by: [Deutsches Museum] On: 15 February 2013, At: 08:42 Publisher: Taylor & Francis Informa Ltd Registered in England and Wales Registered Number: 1072954 Registered office: Mortimer House, 37-41 Mortimer Street, London W1T 3JH, UK Annals of Science Publication details, including instructions for authors and subscription information: http://www.tandfonline.com/loi/tasc20 From William Hyde Wollaston to Alexander von Humboldt - Star Spectra and Celestial Landscape Jürgen Teichmann a & Arthur Stinner b a Deutsches Museum and Ludwig-Maximilians-University, München, Germany b University of Manitoba, Winnipeg, Canada Version of record first published: 13 Feb 2013. To cite this article: Jürgen Teichmann & Arthur Stinner (2013): From William Hyde Wollaston to Alexander von Humboldt - Star Spectra and Celestial Landscape, Annals of Science, DOI:10.1080/00033790.2012.739709 To link to this article: http://dx.doi.org/10.1080/00033790.2012.739709 PLEASE SCROLL DOWN FOR ARTICLE Full terms and conditions of use: http://www.tandfonline.com/page/terms-and- conditions This article may be used for research, teaching, and private study purposes. Any substantial or systematic reproduction, redistribution, reselling, loan, sub-licensing, systematic supply, or distribution in any form to anyone is expressly forbidden. The publisher does not give any warranty express or implied or make any representation that the contents will be complete or accurate or up to date. The accuracy of any instructions, formulae, and drug doses should be independently verified with primary sources. The publisher shall not be liable for any loss, actions, claims, proceedings, demand, or costs or damages whatsoever or howsoever caused arising directly or indirectly in connection with or arising out of the use of this material.
    [Show full text]
  • NASA News National Aeronautics and Space Administration Washington, D.C
    NASA News National Aeronautics and Space Administration Washington, D.C. 20546 AC 202 755-8370 CN r* IT! w to r^ For Release IMMEDIATE I i-f r~ o o =r CD c «- O O Press Kit PrOJGCt Solar Maximum Mission RELEASE NO: 80-16 CM O i-H IH (C «~. H O O W-H -H W +> -P (C (d •* S5 (j «! W SB pq-H EH C Contents M -H e VO r- I 0 as 0) General Release 1-7 cc o I Mission Objectives 8-9 (P K O. W PS tn The Spacecraft 9 (0 < CM jj 1^3 Mission Operations 9-10 i—i fe C Scientific Investigations 10-13 ^ (0 P3 B5 The Sun 13-15 1 rt w Sun-Earth Relationship 16 w ^ u > O -H Launch Vehicle 16-17 Q; co •*-> Launch Operations 17 l a: to Launch Support 17 «c U es in a o Major Launch Events. 18 rt » U }3^ f4 CU Solar Maximum Mission Team 19-20 — i-? rt Contractors 21 February 6, 1980 WNSANews National Aeronautics and Space Administration Washington, D.C. 20546 AC 202 755-8370 Nicholas Panagakos For Release: Headquarters, Washington, D.C. IMMEDIATE (Phone: 202/755-3680) James Lacy Goddard Space Flight Center, Greenbelt, Md. (Phone: 301/344-5565) RELEASE NO: 80-16 NASA SET TO LAUNCH SOLAR FLARE SATELLITE NASA is preparing to place in Earth orbit the first spacecraft designed specifically for the study of solar flares. The mission represents a major step toward a better understanding of the violent nature of the Sun and its effects on Earth.
    [Show full text]
  • How Astronomical Objects Are Named
    How Astronomical Objects Are Named Jeanne E. Bishop Westlake Schools Planetarium 24525 Hilliard Road Westlake, Ohio 44145 U.S.A. bishop{at}@wlake.org Sept 2004 Introduction “What, I wonder, would the science of astrono- use of the sky by the societies of At the 1988 meeting in Rich- my be like, if we could not properly discrimi- the people that developed them. However, these different systems mond, Virginia, the Inter- nate among the stars themselves. Without the national Planetarium Society are beyond the scope of this arti- (IPS) released a statement ex- use of unique names, all observatories, both cle; the discussion will be limited plaining and opposing the sell- ancient and modern, would be useful to to the system of constellations ing of star names by private nobody, and the books describing these things used currently by astronomers in business groups. In this state- all countries. As we shall see, the ment I reviewed the official would seem to us to be more like enigmas history of the official constella- methods by which stars are rather than descriptions and explanations.” tions includes contributions and named. Later, at the IPS Exec- – Johannes Hevelius, 1611-1687 innovations of people from utive Council Meeting in 2000, many cultures and countries. there was a positive response to The IAU recognizes 88 constel- the suggestion that as continuing Chair of with the name registered in an ‘important’ lations, all originating in ancient times or the Committee for Astronomical Accuracy, I book “… is a scam. Astronomers don’t recog- during the European age of exploration and prepare a reference article that describes not nize those names.
    [Show full text]
  • Johann Von Lamont and His Magnetotelluric Experiment in 1862
    26. Schmucker-Weidelt-Kolloquium Dassel, 21.–25. September 2015 Johann von Lamont and his magnetotelluric experiment in 1862 Volker Haak, Blankenfelde SUMMARY Earth currents were first observed in the middle of the 19th century, closely related to magnetic field variations. Particularly the magnetic storms of 1859, which belong to the strongest ones ever experienced, destroying telegraphic constructions in the USA, Europe and Australia, made Johann von Lamont start with experiments about the nature and origin of earth currents. Among these experiments he presented for the first time a method to calculate the thickness of a high conductivity layer in southern Germany. Keywords: earth-electric current, magnetic storms, Lamont INTRODUCTION The geophysical sounding method “magnetotellurics” was formulated and published by Louis Cagniard in 1953, in particular in Western Europe. Later on it became known that even before in 1950 A.N. Tikhonov published an equivalent theory in Eastern Europe, in Russian. Both were henceforth appreciated as the discoverers of magnetotellurics. However, a few years ago we could read that a Japanese author, M.H.Hiramaya, published an equivalent theory already in 1934. Quite recently the question came up somewhere in the MT community whether Johann von Lamont could have been the very first who “invented” the magnetotelluric method. He actually published in 1862 a book about earth currents. There he describes an experiment to measure electrical currents in the earth and the corresponding magnetic field. He then uses the ratio of the amplitudes to calculate the depth range of the sediments beneath his geomagnetic observatory close to the capital of Bavaria, now known as Fürstenfeldbruck (FUR).
    [Show full text]
  • Litir Do Luchd-Ionnsachaidh Le Ruairidh Macilleathain
    Litir do Luchd-ionnsachaidh le Ruairidh MacIlleathain A special programme, in the form of a “letter”, designed for Gaelic learners who already have some knowledge of the language. A short vocabulary and comments on points of grammar and figures of speech are included with the text. If you have comments, Ruairidh can be contacted at [email protected]. This is Litir 436. Note that there is also a simplified version called An Litir Bheag which is likewise available on the BBC website. Litir Bheag 132 corresponds to Litir 436. A bharrachd air a bhith na shàr-reuladair, bha Johann von Lamont, a rugadh ann an Gàidhealtachd Siorrachd Obar Dheathain, aithnichte mar eòlaiche air iùil-tharraing agus dealan. Chruthaich e uidheamachd a ghabhadh cleachdadh airson neart na h-iùil-tharraing air uachdar na talmhainn a thomhas. Rinn e fhèin obair mhòr ann a bhith a’ tomhas a leithid ann am Babhàiria. Às dèidh sin, fhuair e cùmhnantan bho riaghaltasan grunn dùthchannan Eòrpach eile airson an aon rud a dhèanamh dhaibhsan. Sgrìobh e mu bhuaidh na gealaich air gluasad snàthad iùil-tharraingeach, agus mhothaich e gun robh neart na h-iùil-tharraing air uachdar na talmhainn a’ gluasad ann an cuairtean deicheadach. Bha sin gu math faisg air cuairt spotan na grèine a chaidh a lorg le Heinrich Schwabe. Agus sgrìobh von Lamont tràchdas air a’ cheangal eadar comharraidhean dealain na Talmhainn agus iùil-tharraing na planaid. Bha e gu math ainmeil ann an saoghal saidheans – air feadh an t-saoghail. Ann an ochd ceud deug, seachdad ’s a trì (1873) chaidh Iarla Crawford, a bha na reuladair neo-dhreuchdail, gu ruige Munich airson bruidhinn ri von Lamont, agus comhairle fhaighinn bhuaithe mu uidheamachd.
    [Show full text]
  • The CL Gerling and JM Gilliss Correspondence (1847–1856)
    JHA0010.1177/0021828620919536Journal for the History of AstronomySanhueza-Cerda and Valderrama 919536research-article2020 Article JHA Journal for the History of Astronomy 2020, Vol. 51(2) 187 –208 Finding a Point of Observation © The Author(s) 2020 Article reuse guidelines: in the Global South: The sagepub.com/journals-permissions https://doi.org/10.1177/0021828620919536DOI: 10.1177/0021828620919536 C. L. Gerling and J.M. Gilliss journals.sagepub.com/home/jha Correspondence (1847–1856) Carlos Sanhueza-Cerda Universidad de Chile, Chile Lorena B. Valderrama University Alberto Hurtado, Chile Abstract Historians of science have amply demonstrated the transnational character of science; however, they have not sufficiently attended to how several scientific projects were coordinated as part of global initiatives. Our research – based on the unpublished, written correspondence between Christian Ludwig Gerling in Germany and James M. Gilliss in the United States, from 1847 to 1856 – examines the issues that were being discussed in the search for an observation point in Chile that could be linked to the various astronomical research projects happening in the global north. This article shows that the building of this network had to navigate communicational and language barriers, financial uncertainty, lack of adequate scientific instruments, and the influence of intermediaries. In fact, the intermediaries involved affected the formulation of questions and objectives, as well as the choice of methods and instruments to be used (such as Alexander von Humboldt and Friedrich Gauss), and directly impacted on how these things were brought to bear (for example, instrument manufacturers, diplomats, and translators). Keywords Astronomy in the nineteenth century, Christian Ludwig Gerling, James M.
    [Show full text]
  • A Collection of Biographies Geophysics
    A Collection of Biographies with special emphasis on Geophysics by Wolfgang A. Lenhardt Lenhardt – Biographies 1 Foreword This presentation of biographies is far from complete and kept very brief for each person relevant to geophysics. Most texts are taken from Wikipedia and respective links are stated at the bottom of each page. The biographies are sorted in chronological order according respective years of birth and show pictures (when possible from their haydays) of these scientists and engineers. Their countries of birth and death are given in historical context (England <> G.B. >> U.K., Prussia <> Germany, Austro-Hungarian Empire >> Austria, Yugoslavia <> Serbia, Croatia, etc.) thus might to appear erratic, but are deemed to be correct. It seems appropriate to mention the many achievements in geophysics which were not accomplished by a single person alone – as it happens in all other scientific disciplines. Therefore, collaborations are briefly addressed in some slides. In addition, the sequence of biographies is supplemented by slides describing two significant natural events, which altered almost immediately the course of geophysical understanding of our planet. Each person has been allocated a specific main achievement or topic related to geophysics. Sometimes, these allocations are incomplete, like for e.g. Gauss, Laplace or Young, which were truly multi-talented. Hence, some of the headlines might be considered not to the point by some readers. I apologize for that. Please let me know, where I did very wrong. [email protected]
    [Show full text]
  • Stars and Satellites Mary Brück
    Mary Brück Women in Early British and Irish Astronomy Stars and Satellites 123 Women in Early British and Irish Astronomy Mary Brück Women in Early British and Irish Astronomy Stars and Satellites Mary Brück ISBN 978-90-481-2472-5 e-ISBN 978-90-481-2473-2 DOI 10.1007/978-90-481-2473-2 Springer Dordrecht Heidelberg London New York Library of Congress Control Number: 2009931554 c Springer Science+Business Media B.V. 2009 No part of this work may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, microfilming, recording or otherwise, without written permission from the Publisher, with the exception of any material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) For my sisters (nees´ Conway) Eithne, Meadhbh and Aoife Foreword The role of women in the growth of science has become an important area of modern historical scholarly research. And as far as the study of the role of women in astron- omy is concerned, Dr. Mary Br¨uck is an established and illustrious pioneer, with an international reputation and acclaimed books and articles already to her credit. Her present book, Stars and Satellites, brings together many figures who worked over a 300-year time scale, and whose relationship with astronomy ranged from informed assistants to independent researchers to major writers and interpreters of contem- porary astronomy to, eventually, paid professionals.
    [Show full text]
  • LAMONT's SEED: GEORG VON Neumayer's INTEREST IN
    CSIRO Publishing The Royal Society of Victoria, 127, 98, 2015 www.publish.csiro.au/journals/rs 10.1071/RS15010 LAMONT’S SEED: GEORG VON NEuMAyER’S INTEREST IN MAGNETISM, METEOROLOGy AND ASTRONOMy Cornelia lüdeCke* Center for History of Science and Technology, university of Hamburg, Hamburg, Germany Correspondence: [email protected] ABSTRACT: From 1835 Johann von Lamont (1805– about Lamont’s different interests and how he dealt with 1879) was director of the observatory at the village them. Although Neumayer only stayed a few months at of Bogenhausen, north-east of Munich (today part of the observatory, Lamont’s input determined Neumayer’s Munich). He was a scholar with varied interests and the future life as a scientist, referring to the construction and ability to achieve something excellent with sparse funding. calibration of instruments and astronomical observations Although he started his astronomical research with a brand and timing, as well as magnetic and meteorological new Fraunhofer refractor, he mostly had to work with older measurements and magnetic surveys, and instilled in him instruments until his death in 1879. For instance, he used the importance of promptly publishing his results. When a Reichenbach meridian circle not only to determine the Neumayer decided on a career path, his main aim was to positions of more than 37,500 stars but also to determine the continue Ross’s magnetic measurements in the south polar exact time at noon. He also was involved in the project of region. A starting point was Hobart, where Ross had set up the European arc measurement.
    [Show full text]
  • Journal the Future of the City Observatory
    10/07/2018 ASE Journal No. 49 Astronomical Society of Edinburgh Journal No. 49 - October 2005 Nora Jenkinson with Harperdean Astronomical Society members, c. 1990. The future of the City Observatory http://www.astronomyedinburgh.org/publications/journals/49/all.shtml 1/12 10/07/2018 ASE Journal No. 49 For some time the Society has been anxious about the state of the Playfair Building which houses the Cooke refractor and also the other Building in which we have our monthly meetings. The buildings are leased from the City Council. The buildings are deteriorating and may become unfit for any use in the not too distant future. The City has plans to redevelop Calton Hill, including the buildings of astronomical interest. To review progress towards the completion of these plans myself and Alan Ellis met with City Council officials on 13th September 2005. Chairing the meeting was Lynne Halfpenny, Head of Museum and Arts, City of Edinburgh Council. We were informed that the Council has appointed architects and hopes to set up a management group within the next six months which will develop a plan. Once the plan is completed funding will be secured (hopefully) and work can commence. Work on the whole site may not be completed until 2010/2011. The ASE will be invited to be represented on the management group. The ASE now has the choice of two possible scenarios. One scenario is separating ourselves from the City Observatory because of its deteriorating state and because its upkeep is expensive. Rates and electricity are significant costs which result in our relatively high membership fee.
    [Show full text]