Bibliography of Historical Geomagnetic Main Field Survey and Secular Variation Reports at WDC-A, 1993
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Table of Contents
Solar System Table of Contents Publisher's Note Editors' Introduction List of Contributors Complete List of Contents Archeaostronomy (new) Asteroids Auroras Big Bang Brown Dwarfs Callisto (new) Ceres (new) Comet Halley Comet Shoemaker-Levy 9 (new) Comets Coordinate Systems Coronal Holes and Coronal Mass Ejections (new) Cosmic Rays Cosmology Dwarf Planets (new) Earth-Moon Relations (new) Earth-Sun Relations Earth System Science Earth's Age Earth's Atmosphere Earth's Composition Earth's Core Earth's Core-Mantle Boundary Earth's Crust Earth's Crust-Mantle Boundary(new) Earth's Differentiation Earth's Magnetic Field: Origins Earth's Magnetic Field: Secular Variation Earth's Magnetic Field at Present Earth's Magnetosphere Earth's Mantle Earth's Oceans Earth's Origin Earth's Rotation Earth's Shape Earth's Structure Eclipses Electromagnetic Radiation: Thermal Emissions (new) Electromagnetic Radiation: Nonthermal Emissions (new) Enceladus (new) Eris and Dysnomia (new) Europa Extrasolar Planet Detection Methods (new) Extrasolar Planetary Systems Extraterrestrial Life in the Solar System Gamma-Ray Bursters Ganymede (new) General Relativity Gravity Measurement Greenhouse Effect Habitable Zones (new) Hertzsprung-Russell Diagram Iapetus (new) Impact Cratering Infrared Astronomy Interstellar Clouds and the Interstellar Medium Interplanetary Environment (new) Io Jovian Planets Jupiter's Atmosphere Jupiter's Great Red Spot Jupiter's Interior (new) Jupiter's Magnetic Field and Radiation Belts Jupiter's Ring System (new) Jupiter's Satellites Kuiper Belt -
Key and Driving Requirements for the Juno Payload Suite of Instruments
Key and Driving Requirements for the Juno Payload Suite of Instruments Randy Dodge1 and Mark A. Boyles2 Jet Propulsion Laboratory-California Institute of Technology, Pasadena, CA, 91109-8099 Chuck E. Rasbach3 Lockheed Martin-Space System Company, Denver, CO, 80201 [Abstract] The Juno Mission was selected in the summer of 2005 via NASA’s New Frontiers competitive AO process (refer to http://www.nasa.gov/home/hqnews/2005/jun/HQ_05138_New_Frontiers_2.html). The Juno project is led by a Principle Investigator based at Southwest Research Institute [SwRI] in San Antonio, Texas, with project management based at the Jet Propulsion Laboratory [JPL] in Pasadena, California, while the Spacecraft design and Flight System integration are under contract to Lockheed Martin Space Systems Company [LM-SSC] in Denver, Colorado. The payload suite consists of a large number of instruments covering a wide spectrum of experimentation. The science team includes a lead Co-Investigator for each one of the following experiments: A Magnetometer experiment (consisting of both a FluxGate Magnetometer (FGM) built at Goddard Space Flight Center [GSFC] and a Scalar Helium Magnetometer (SHM) built at JPL, a MicroWave Radiometer (MWR) also built at JPL, a Gravity Science experiment (GS) implemented via the telecom subsystem, two complementary particle instruments (Jovian Auroral Distribution Experiment, JADE developed by SwRI and Juno Energetic-particle Detector Instrument, JEDI from the Applied Physics Lab [APL]--JEDI and JADE both measure electrons and ions), an Ultraviolet Spectrometer (UVS) also developed at SwRI, and a radio and plasma (Waves) experiment (from the University of Iowa). In addition, a visible camera (JunoCam) is included in the payload to facilitate education and public outreach (designed & fabricated by Malin Space Science Systems [MSSS]). -
“The Touch of Cold Philosophy”
Edinburgh Research Explorer The Fragmentation of Renaissance Occultism and the Decline of Magic Citation for published version: Henry, J 2008, 'The Fragmentation of Renaissance Occultism and the Decline of Magic', History of Science, vol. 46, no. Part 1, No 151, pp. 1-48. <http://www.ingentaconnect.com/content/shp/histsci/2008/00000046/00000001/art00001> Link: Link to publication record in Edinburgh Research Explorer Document Version: Peer reviewed version Published In: History of Science Publisher Rights Statement: With permission © Henry, J. (2008). The Fragmentation of Renaissance Occultism and the Decline of Magic. History of Science, 46(Part 1, No 151), 1-48 General rights Copyright for the publications made accessible via the Edinburgh Research Explorer is retained by the author(s) and / or other copyright owners and it is a condition of accessing these publications that users recognise and abide by the legal requirements associated with these rights. Take down policy The University of Edinburgh has made every reasonable effort to ensure that Edinburgh Research Explorer content complies with UK legislation. If you believe that the public display of this file breaches copyright please contact [email protected] providing details, and we will remove access to the work immediately and investigate your claim. Download date: 23. Sep. 2021 The Fragmentation of Renaissance Occultism and the Decline of Magic* [History of Science, 46 (2008), pp. 1-48.] The touch of cold philosophy? At a Christmas dinner party in 1817 an admittedly drunken -
Book of Abstracts Ii Contents
2014 CAP Congress / Congrès de l’ACP 2014 Sunday, 15 June 2014 - Friday, 20 June 2014 Laurentian University / Université Laurentienne Book of Abstracts ii Contents An Analytic Mathematical Model to Explain the Spiral Structure and Rotation Curve of NGC 3198. .......................................... 1 Belle-II: searching for new physics in the heavy flavor sector ................ 1 The high cost of science disengagement of Canadian Youth: Reimagining Physics Teacher Education for 21st Century ................................. 1 What your advisor never told you: Education for the ’Real World’ ............. 2 Back to the Ionosphere 50 Years Later: the CASSIOPE Enhanced Polar Outflow Probe (e- POP) ............................................. 2 Changing students’ approach to learning physics in undergraduate gateway courses . 3 Possible Astrophysical Observables of Quantum Gravity Effects near Black Holes . 3 Supersymmetry after the LHC data .............................. 4 The unintentional irradiation of a live human fetus: assessing the likelihood of a radiation- induced abortion ...................................... 4 Using Conceptual Multiple Choice Questions ........................ 5 Search for Supersymmetry at ATLAS ............................. 5 **WITHDRAWN** Monte Carlo Field-Theoretic Simulations for Melts of Diblock Copoly- mer .............................................. 6 Surface tension effects in soft composites ........................... 6 Correlated electron physics in quantum materials ...................... 6 The -
Seabirds of Human Settlements in Antarctica: a Case Study of the Mirny Station
CZECH POLAR REPORTS 11 (1): 98-113, 2021 Seabirds of human settlements in Antarctica: A case study of the Mirny Station Sergey Golubev Papanin Institute for Biology of Inland Waters, Russian Academy of Sciences, Borok, Nekouzskii raion, Yaroslavl oblast, 152742, Russia Abstract Antarctica is free of urbanisation, however, 40 year-round and 32 seasonal Antarctic stations operate there. The effects of such human settlements on Antarctic wildlife are insufficiently studied. The main aim of this study was to determine the organization of the bird population of the Mirny Station. The birds were observed on the coast of the Davis Sea in the Mirny (East Antarctica) from January 8, 2012 to January 7, 2013 and from January 9, 2015 to January 9, 2016. The observations were carried out mainly on the Radio and Komsomolsky nunataks (an area of about 0.5 km²). The duration of observations varied from 1 to 8 hours per day. From 1956 to 2016, 13 non-breeding bird species (orders Sphenisciformes, Procellariiformes, Charadriiformes) were recorded in the Mirny. The South polar skuas (Catharacta maccormicki) and Adélie penguins (Pygoscelis adeliae) form the basis of the bird population. South polar skuas are most frequently recorded at the station. Less common are Brown skuas (Catharacta antarctica lonnbergi) and Adélie penguins. Adélie penguins, Wilson's storm petrels (Oceanites oceanicus), South polar and Brown skuas are seasonal residents, the other species are visitors. Adélie penguins, Emperor (Aptenodytes forsteri), Macaroni (Eudyptes chrysolophus) and Chinstrap penguins (Pygoscelis antarctica), Wilson's storm petrels, South polar and Brown skuas interacted with the station environment, using it for com- fortable behavior, feeding, molting, shelter from bad weather conditions, and possible breeding. -
History of Paediatric Treatment in the Reichsuniversität Straßburg (1941-1944) Aisling Shalvey
History of paediatric treatment in the Reichsuniversität Straßburg (1941-1944) Aisling Shalvey To cite this version: Aisling Shalvey. History of paediatric treatment in the Reichsuniversität Straßburg (1941-1944). His- tory. Université de Strasbourg, 2021. English. NNT : 2021STRAG002. tel-03283700 HAL Id: tel-03283700 https://tel.archives-ouvertes.fr/tel-03283700 Submitted on 12 Jul 2021 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. UNIVERSITÉ DE STRASBOURG ÉCOLE DOCTORALE 519 Sciences humaines et sociales – Perspectives européennes [ ARCHE ] THÈSE présentée par : Aisling SHALVEY soutenue le : 12 mars 2021 pour obtenir le grade de : Docteur de l’université de Strasbourg Discipline/ Spécialité : Histoire Contemporaine de la Médecine History of Paediatric Treatment in the Reichsuniversität Straßburg (1941-1944) THÈSE dirigée par : Professeur MAURER Catherine Directrice du thèse, Université de Strasbourg Professeur WEINDLING Paul Directeur du thèse, Oxford Brookes University RAPPORTEURS : Professeur VON BUELTZINGSLOEWEN Isabelle Professor, Université Lumière Lyon 2 Professeur ROELCKE Volker Professor, Justus-Liebig- Universität Gießen AUTRES MEMBRES DU JURY : Professeur BONAH Christian Professor, Université de Strasbourg 1 Do mo sheantuismitheoirí Le grá 2 Acknowledgements I am extraordinarily lucky to have so many people who have supported me throughout the process of writing my PhD thesis; too many people to list, so I will begin by saying thank you to everyone who has helped me along the way. -
Chapter 2 Tests of Magnetometer/Sun-Sensor Orbit Determination Using Flight Data*
Chapter 2 Tests of Magnetometer/Sun-Sensor Orbit Determination Using Flight Data* 2.1 Introduction Orbit determination is an old topic in celestial mechanics and is an essential part of satellite navigation. Traditional ground-based tracking methods that use range and range-rate measurements can provide an orbit accuracy as good as a few centimeters1. Autonomous orbit determination using only onboard measurements can be a requirement of military satellites in order to guarantee independence from ground facilities2. The rapid increase in the number of satellites also increases the need for autonomous navigation because of bottlenecks in ground tracking facilities3. A filter that uses magnetometer measurements provides one possible means of doing autonomous orbit determination. This idea was first introduced by Psiaki and Martel4 and has been tested by a number of researchers since then3,5-9. Magnetometers fly on most spacecraft (S/C) for attitude determination and control purposes. Therefore, successful autonomous orbit determination using magnetometer measurements can make the integration of attitude and orbit determination possible and lead to reduced mission costs. Although magnetometer-based autonomous orbit determination is unlikely to have better accuracy than ground-based tracking, a magnetometer-based system could be applied to a mission that does not need the accuracy of ground-station tracking. The Tropical Rainfall Measurement Mission * This chapter is from the published paper: Hee Jung and Mark L. Psiaki, “Tests of Magnetometer/Sun-Sensor Orbit Determination Using Flight Data,” Journal of Guidance, Control, and Dynamics, Volume 25, Number 3, pp. 582-590. [© 2002. The American Institute of Aeronautics and Astronautics, Inc]. 8 9 (TRMM), for example, requires 40 km position accuracy. -
Juno Magnetometer (MAG) Standard Product Data Record and Archive Volume Software Interface Specification
Juno Magnetometer Juno Magnetometer (MAG) Standard Product Data Record and Archive Volume Software Interface Specification Preliminary March 6, 2018 Prepared by: Jack Connerney and Patricia Lawton Juno Magnetometer MAG Standard Product Data Record and Archive Volume Software Interface Specification Preliminary March 6, 2018 Approved: John E. P. Connerney Date MAG Principal Investigator Raymond J. Walker Date PDS PPI Node Manager Concurrence: Patricia J. Lawton Date MAG Ground Data System Staff 2 Table of Contents 1 Introduction ............................................................................................................................. 1 1.1 Distribution list ................................................................................................................... 1 1.2 Document change log ......................................................................................................... 2 1.3 TBD items ........................................................................................................................... 3 1.4 Abbreviations ...................................................................................................................... 4 1.5 Glossary .............................................................................................................................. 6 1.6 Juno Mission Overview ...................................................................................................... 7 1.7 Software Interface Specification Content Overview ......................................................... -
Four Centuries of Geomagnetic Secular Variation from Historical Records
Fourcenturies of geomagnetic secular variationfrom historical records ByAndrewJackson 1,ArtR.T. Jonkers 2 andMatthewR.W alker 1 1School ofEarth Sciences, Leeds University,Leeds LS29JT, UK 2Departmentof History, V rijeUniversiteit, Amsterdam, The Netherlands Wepresent anewmodel of the magnetic eld at the core{mantle boundary for the interval 1590{1990. Themodel, called gufm1,is based on amassive newcompilation of historical observations of the magnetic eld. The greater part of the newdataset originates from unpublished observations taken by mariners engaged in merchant and naval shipping. Considerable attention is given to both correction of data for possible mislocation (originating from poor knowledge of longitude) and to proper allocation of error in the data. Weadopt astochastic model for uncorrected positional errors that properly accounts for the nature of the noise process based on aBrownian motion model. Thevariability of navigational errors as afunction of the duration of the voyages that wehave analysed isconsistent with this model. For the period before 1800, more than 83 000 individual observations of magnetic declination wererecorded at more than 64 000 locations; more than 8000 new observations are for the 17th century alone. Thetime-dependent eld model that weconstruct from the dataset is parametrized spatially in terms of spherical harmonics and temporally in B-splines, using atotal of 36 512 parameters. Themodel has improved the resolution of the core eld, and represents the longest continuous model of the eld available. However, full exploitation of the database may demand anew modelling methodology. Keywords: Earth’score; geom agneticsec ularvariation ; magnetic¯ eld;m aritimehistory 1.Intro duction TheEarth has possessed amagnetic eld for more than 4billion years, generated in the ®uid core. -
Magnetic Power Spectrum, with Application to Planetary Dynamo Radii
Earth and Planetary Science Letters 401 (2014) 347–358 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl A new model for the (geo)magnetic power spectrum, with application to planetary dynamo radii ∗ Benoit Langlais a, , Hagay Amit a, Hugo Larnier a,b, Erwan Thébault c, Antoine Mocquet a a Laboratoire de Planétologie et Géodynamique, CNRS UMR 6112, Université de Nantes, 44322 Nantes cedex 3, France b Institut de Physique du Globe de Strasbourg, UdS–CNRS UMR7516, EOST – Université de Strasbourg, 5 rue René Descartes, 67084 Strasbourg Cedex, France c Équipe de Géomagnétisme, Institut de Physique du Globe de Paris, CNRS UMR 7154, 75252 Paris cedex 5, France a r t i c l e i n f o a b s t r a c t Article history: We propose two new analytical expressions to fit the Mauersberger–Lowes geomagnetic field spectrum Received 6 November 2013 at the core–mantle boundary. These can be used to estimate the radius of the outer liquid core where the Received in revised form 23 April 2014 geodynamo operates, or more generally the radius of the planetary dynamo regions. We show that two Accepted 10 May 2014 sub-families of the geomagnetic field are independent of spherical harmonics degree n at the core–mantle Available online 9 July 2014 boundary and exhibit flat spectra. The first is the non-zonal field, i.e., for spherical harmonics order m Editor: C. Sotin different from zero. The second is the quadrupole family, i.e., n + m even. The flatness of their spectra is Keywords: motivated by the nearly axisymmetric time-average paleomagnetic field (for the non-zonal field) and the magnetic power spectrum dominance of rotational effects in core dynamics (for the quadrupole family). -
Lachlan Macquarie in Russia1
Aleksandr Massov Lachlan Macquarie in Russia1 Despite the abundance of works in Australian and British historiography devoted to the life and career of Lachlan Macquarie, there is as yet no specialist study of the ‘Russian chapter’ in his biography: his journey through Russia from Astrakhan to St Petersburg in 1807.2 At the same time, the story of the future governor’s sojourn in Russia is of interest not only for the light it casts on this little-known phase of his life; there is a sense in which it had a significant impact on the relationship between Britain’s Australian colonies and the Russian Empire in the first years of contact between the two countries. As Macquarie’s Australian biographer Robin Walsh has argued,3 the events which befell him in 1807 require closer investigation. Macquarie, at that time a 45-year-old lieutenant in the British army, undertook his Russian journey on his way home from India. He was in some haste to take up a new appointment, and also to marry his fiancée Elizabeth Campbell as soon as possible. Accompanying him were his servant George Jarvis and two fellow-officers, George William Brande, a lieutenant, and William Thomas of the Medical Corps.4 The journey, it should be said, took place at a time of international crisis: Napoleon was continuing his triumphant advance over the European continent, while the alliance of his enemies (Britain, Prussia, Russia and Sweden) sustained defeat after defeat. In October 1806 the Prussian army had been virtually annihilated at Jena and Auerstadt, while his victory over the Russians at Friedland in June 1807 had allowed Bonaparte to occupy East Prussia 1 This article was completed when the author held the post of Visiting Scholar in the School of Languages and Comparative Cultural Studies at the University of Queensland under the Australian Academy of the Humanities Visiting Scholar Programme. -
Confirmations Database
Pastor Willing’s Diarium Pastorale Confirmation Extractions © Society for German Genealogy in Eastern Europe 2013 Surname Given Event Date Year Father Mother's Mother's Given Parish Residence Page Reg Remarks Extractor Book Name(s) Surname Names Place Nr. # Abel Lydia C 8 Mar 1907 Daniel Foerster Augustine Leduc 120 born 13 Oct 1892 in Kissolowna, Russia Armbruster Johann C 28 May 1902 Valentin Schuetz Catharina 110 born 12 Jul 1888 in Sassendorf Jerry Frank 3 (Galicia); location of confirmation not indicated but probably Neudorf Armbruster Ludwig C 1906? 108 no data shown Jerry Frank 4 Armbruster Philipp C 1907 Valentin 118 born 26 Sep 1893 in Neudorf, SK Jerry Frank 4 Assmann Elisabeth C 9 Aug 1903 Carl Erbach Elisabeth 114 13 born 1 Oct 1889 in Mewnitz, Jerry Frank 3 Russia Assmann Emilie C 3 Jun 1906 Carl Erbach Elisabeth 110 born 1 May 1892 in ?? Jerry Frank 4 Ast Anna C 1900? Johann Zachmann Luise 116 born 24 Mar 1886 in Jerry Frank 2 Jstenschaegel Ast Catherine C 1900? Christian Schoenthaler Marie 114 born 20 Jun 1887 in Jllischeske Jerry Frank 2 Ast Franz C 1898 Johann Louisa 110 17 born 20 Feb 1884 in Jstan Jerry Frank 2 Szegez? Ast Jacob C 1898 Christian Maria 108 5 born 6 Sep 1884 in Jllischeske Jerry Frank 2 Baber Carolina C 28 May 1902 Carl Mueller Wilhelmine 108 born 22 Feb 1889 in Eichfeld; Jerry Frank 3 location of confirmation not indicated but probably Neudorf Batzwald Carl C 1904 Julius Weber Caroline 114 born 2 Dec 1888 in Josefufke, Jerry Frank 3 Russia Batzwald Theresia C 1904 Julius Weber Caroline 114 born 2 Sep 1890 in Josefufke, Jerry Frank 3 Russia Bauer Georg C 1 Apr 1928 Castor 118 born 18 Nov 1912 in Hague, SK Jerry Frank 5 Bender Bernhard C 3 Jun 1906 Philipp Zapp Caroline 110 born 28 Sep 1891 in Medwitz, Jerry Frank 4 Russia Bender Caroline C 31 May 1903 Phil.