2019 APS/CNM USERS MEETING Program and Abstracts
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UC Irvine UC Irvine Previously Published Works
UC Irvine UC Irvine Previously Published Works Title Astrophysics in 2006 Permalink https://escholarship.org/uc/item/5760h9v8 Journal Space Science Reviews, 132(1) ISSN 0038-6308 Authors Trimble, V Aschwanden, MJ Hansen, CJ Publication Date 2007-09-01 DOI 10.1007/s11214-007-9224-0 License https://creativecommons.org/licenses/by/4.0/ 4.0 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Space Sci Rev (2007) 132: 1–182 DOI 10.1007/s11214-007-9224-0 Astrophysics in 2006 Virginia Trimble · Markus J. Aschwanden · Carl J. Hansen Received: 11 May 2007 / Accepted: 24 May 2007 / Published online: 23 October 2007 © Springer Science+Business Media B.V. 2007 Abstract The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe) and others of which there are always many, like meteors and molecules, black holes and binaries. Keywords Cosmology: general · Galaxies: general · ISM: general · Stars: general · Sun: general · Planets and satellites: general · Astrobiology · Star clusters · Binary stars · Clusters of galaxies · Gamma-ray bursts · Milky Way · Earth · Active galaxies · Supernovae 1 Introduction Astrophysics in 2006 modifies a long tradition by moving to a new journal, which you hold in your (real or virtual) hands. The fifteen previous articles in the series are referenced oc- casionally as Ap91 to Ap05 below and appeared in volumes 104–118 of Publications of V. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Lunar Impact Basins Revealed by Gravity Recovery and Interior
Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, Sean Solomon, David Smith, Frank Lemoine, Erwan Mazarico, Terence Sabaka, et al. To cite this version: Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, et al.. Lunar im- pact basins revealed by Gravity Recovery and Interior Laboratory measurements. Science Advances , American Association for the Advancement of Science (AAAS), 2015, 1 (9), pp.e1500852. 10.1126/sci- adv.1500852. hal-02458613 HAL Id: hal-02458613 https://hal.archives-ouvertes.fr/hal-02458613 Submitted on 26 Jun 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. RESEARCH ARTICLE PLANETARY SCIENCE 2015 © The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. Distributed Lunar impact basins revealed by Gravity under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). Recovery and Interior Laboratory measurements 10.1126/sciadv.1500852 Gregory A. Neumann,1* Maria T. Zuber,2 Mark A. Wieczorek,3 James W. Head,4 David M. H. Baker,4 Sean C. Solomon,5,6 David E. Smith,2 Frank G. -
Patterning and Characterization of Graphene Nano-Ribbon by Electron Beam Induced Etching Sébastien Linas
Patterning and characterization of graphene nano-ribbon by electron beam induced etching Sébastien Linas To cite this version: Sébastien Linas. Patterning and characterization of graphene nano-ribbon by electron beam induced etching. Materials Science [cond-mat.mtrl-sci]. Université Paul Sabatier - Toulouse III, 2012. English. NNT : 2012TOU30323. tel-01025043 HAL Id: tel-01025043 https://tel.archives-ouvertes.fr/tel-01025043 Submitted on 17 Jul 2014 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. 5)µ4& &OWVFEFMPCUFOUJPOEV %0$503"5%&-6/*7&34*5²%&506-064& %ÏMJWSÏQBS Université Toulouse 3 Paul Sabatier (UT3 Paul Sabatier) 1SÏTFOUÏFFUTPVUFOVFQBS LINAS Sébastien le mercredi 19 décembre 2012 5JUSF Fabrication et caractérisation de nano-rubans de graphène par gravure électronique directe. ²DPMF EPDUPSBMF et discipline ou spécialité ED SDM : Nano-physique, nano-composants, nano-mesures - COP 00 6OJUÏEFSFDIFSDIF Centre d'Elaboration de Matériaux et d'Etudes Structurales. CEMES CNRS UPR8011 %JSFDUFVS T EFʾÒTF DUJARDIN Erik Jury : BANHART Florian (IPCMS, Strasbourg), Rapporteur BOUCHIAT Vincent (Inst. Néel, Grenoble), Rapporteur SERP Philippe (LCC, Toulouse), Président MLAYAH Adnen (CEMES, Toulouse), Examinateur PAILLET Matthieu (L2C-UM2, Montpellier), Examinateur Remerciements. Mes premiers remerciements vont à mon amoureuse Céline et notre Paul qui ont sup‐ porté mes absences ces trois années durant. -
Shock Vaporization of Silica and the Thermodynamics of Planetary Impact Events R
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E09009, doi:10.1029/2012JE004082, 2012 Shock vaporization of silica and the thermodynamics of planetary impact events R. G. Kraus,1 S. T. Stewart,1 D. C. Swift,2 C. A. Bolme,3 R. F. Smith,2 S. Hamel,2 B. D. Hammel,2 D. K. Spaulding,4 D. G. Hicks,2 J. H. Eggert,2 and G. W. Collins2 Received 15 March 2012; revised 17 August 2012; accepted 18 August 2012; published 28 September 2012. [1] The most energetic planetary collisions attain shock pressures that result in abundant melting and vaporization. Accurate predictions of the extent of melting and vaporization require knowledge of vast regions of the phase diagrams of the constituent materials. To reach the liquid-vapor phase boundary of silica, we conducted uniaxial shock-and-release experiments, where quartz was shocked to a state sufficient to initiate vaporization upon isentropic decompression (hundreds of GPa). The apparent temperature of the decompressing fluid was measured with a streaked optical pyrometer, and the bulk density was inferred by stagnation onto a standard window. To interpret the observed post-shock temperatures, we developed a model for the apparent temperature of a material isentropically decompressing through the liquid-vapor coexistence region. Using published thermodynamic data, we revised the liquid-vapor boundary for silica and calculated the entropy on the quartz Hugoniot. The silica post-shock temperature measurements, up to entropies beyond the critical point, are in excellent qualitative agreement with the predictions from the decompressing two-phase mixture model. Shock-and-release experiments provide an accurate measurement of the temperature on the phase boundary for entropies below the critical point, with increasing uncertainties near and above the critical point entropy. -
Modeling Polarimetric Radar Scattering from the Lunar Surface: Study on the Effect of Physical Properties of the Regolith Layer Wenzhe Fa, Mark Wieczorek, Essam Heggy
Modeling polarimetric radar scattering from the lunar surface: Study on the effect of physical properties of the regolith layer Wenzhe Fa, Mark Wieczorek, Essam Heggy To cite this version: Wenzhe Fa, Mark Wieczorek, Essam Heggy. Modeling polarimetric radar scattering from the lunar sur- face: Study on the effect of physical properties of the regolith layer. Journal of Geophysical Research. Planets, Wiley-Blackwell, 2011, 116 (E3), pp.E03005. 10.1029/2010JE003649. hal-02458568 HAL Id: hal-02458568 https://hal.archives-ouvertes.fr/hal-02458568 Submitted on 26 Jun 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. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03005, doi:10.1029/2010JE003649, 2011 Modeling polarimetric radar scattering from the lunar surface: Study on the effect of physical properties of the regolith layer Wenzhe Fa,1 Mark A. Wieczorek,1 and Essam Heggy1,2 Received 10 May 2010; revised 21 November 2010; accepted 15 December 2010; published 5 March 2011. [1] A theoretical model for radar scattering from the lunar regolith using the vector radiative transfer theory for random media has been developed in order to aid in the interpretation of Mini‐SAR data from the Chandrayaan‐1 and Lunar Reconnaissance Orbiter missions. -
Monday Morning, October 19, 2015 Atom Probe Tomography Focus Topic Complex Device Such As Solar Cells and Batteries Is the Need of the Hour
Monday Morning, October 19, 2015 Atom Probe Tomography Focus Topic complex device such as solar cells and batteries is the need of the hour. Here we report on laser assisted atom probe tomography of energy storage Room: 230A - Session AP+AS+MC+MI+NS-MoM and conversion devices to identify the spatial distribution of the elements comprising the various layers and materials. Recent progress and significant Atom Probe Tomography of Nanomaterials challenges for preparation and study of perovskite solar cells and battery materials using laser assisted atom probe tomography will be discussed. Moderator: Daniel Perea, Pacific Northwest National This opens up new avenues to understand complex mutli-layer systems at Laboratory the atomic scale and provide a nanoscopic view into the intricate workings of energy materials. 8:20am AP+AS+MC+MI+NS-MoM1 Correlative Multi-scale Analysis of Nd-Fe-B Permanent Magnet, Taisuke Sasaki, T. Ohkubo, K. Hono, 10:00am AP+AS+MC+MI+NS-MoM6 Atom Probe Tomography of Pt- National Institute for Materials Science (NIMS), Japan INVITED based Nanoparticles, Katja Eder, P.J. Felfer, J.M. Cairney, The (Nd,Dy)–Fe–B based sintered magnets are currently used for traction University of Sydney, Australia motors and generators of (hybrid) electric vehicles because of their Pt nanoparticles are commonly used as catalysts in fuel cells. There are a lot excellent combination of maximum energy product and coercivity. of factors which influence the activity of a catalyst, including the surface However, there is a strong demand to achieve high coercivity without using structure and geometry [1], d-band vacancy of the metal catalyst [2], the Dy due to its scarce natural resources and high cost. -
Arxiv:1403.6528V1 [Astro-Ph.IM] 25 Mar 2014
25 Years of Self-Organized Criticality: Solar and Astrophysics Markus J. Aschwanden Lockheed Martin, Solar and Astrophysics Laboratory (LMSAL), Advanced Technology Center (ATC), A021S, Bldg.252, 3251 Hanover St., Palo Alto, CA 94304, USA; e-mail: [email protected] Norma Crosby Belgian Institute for Space Aeronomy, Ringlaan-3-Avenue Circulaire, B-1180 Brussels, Belgium Michaila Dimitropoulou Kapodistrian University of Athens, Dept. Physics, 15483, Athens, Greece Manolis K. Georgoulis Research Center Astronomy and Applied Mathematics, Academy of Athens, 4 Soranou Efesiou St., Athens, Greece, GR-11527. Stefan Hergarten Institute f¨ur Geo- und Umweltnaturwissenschaften, Albert-Ludwigs-Universit¨at Freiburg, Albertstr. 23B, 79104 Freiburg, Germany James McAteer Dept. Astronomy, P.O.Box 30001, New Mexico State University, MSC 4500, Las Cruces, USA Alexander V. Milovanov Associazione EURATOM-ENEA sulla Fusione, Italian National Agency for New Technologies, Frascati Research Centre, Via E. Fermi 45, C.P.-65, I-00044 Frascati, Rome, Italy; Space Research Institute, Russian Academy of Sciences, Profsoyuznaya str. 84/32, 117997 Moscow, Russia; Max Planck Institute for the Physics of Complex Systems, Noethnitzer Str. 38, 01187 Dresden, Germany Shin Mineshige Dept. Astronomy, Kyoto University, Kyoto 606-8602, Japan arXiv:1403.6528v1 [astro-ph.IM] 25 Mar 2014 Laura Morales Canadian Space Agency, Space Science and Technology Branch, 6767 Route de l’Aeroport, Saint Hubert, Quebec, J3Y8Y9, Canada Naoto Nishizuka Inst. Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, 252-5210, Japan Gunnar Pruessner Dept. Mathematics, Imperial College London, 180 Queen’s Gate, London SW7 2AZ, United Kingdom Raul Sanchez –2– Dept. Fisica, Universidad Carlos III de Madrid, Avda. -
Research Reactor Activities in Support of National Nuclear Programmes
IAEA-TECDOC-409 RESEARCH REACTOR ACTIVITIES IN SUPPORT OF NATIONAL NUCLEAR PROGRAMMES PROCEEDINGS TECHNICAA F O L COMMITTEE MEETING ON RESEARCH REACTOR ACTIVITIES IN SUPPOR NATIONAF TO L NUCLEAR PROGRAMMES HEL BUDAPESTDN I , HUNGARY, 10-13 DECEMBER 1985 AND SELECTED PAPERS FROM A SEMINAR APPLIEN O D RESEARC SERVICD HAN E ACTIVITIES FOR RESEARCH REACTOR OPERATIONS HEL COPENHAGENDN I , DENMARK, 9-13 SEPTEMBER 1985 BOTH MEETINGS ORGANIZEE TH Y DB INTERNATIONAL ATOMIC ENERGY AGENCY A TECHNICAL DOCUMENT ISSUED BY THE INTERNATIONAL ATOMIC ENERGY AGENCY, VIENNA, 1987 RESEARCH REACTOR ACTIVITIES IN SUPPORT OF NATIONAL NUCLEAR PROGRAMMES IAEA, VIENNA, 1987 IAEA-TECDOC-409 PrinteIAEe th Austri Am y db a March 1987 PLEAS AWARE EB E THAT MISSINE TH F GO L PAGEAL THIN SI S DOCUMENT WERE ORIGINALLY BLANK IAEe Th A doe t normallsno y maintain stock f reportso thin si s series. However, microfiche copies of these reports can be obtained from INIS Clearinghouse International Atomic Energy Agency Wagramerstrasse5 P.O.Box 100 A-1400 Vienna, Austria Orders should be accompanied by prepayment of Austrian Schillings 100, in the form of a cheque or in the form of IAEA microfiche service coupons orderee whicb y dhma separately fro INIe mth S Clearinghouse. FOREWORD This report is the result ot an IAEA Technical Committee Meeting on Research Rear*or Activitie n Suppori s t Nationao t l Nuclear Programmes Budapesthel; ir d . Hungary durin3 Decembe1 0 1 g re mot-tin198bTh s . wa g e hosteCentrath y b d l Research Institut r Physicto e s (KFK1 d includean ) d participants trom ten countries, plus six trom the Technical University ot Budapes d KFKIe countriean tTh . -
Interim Report on the Thermodynamics of Chemical Species Important in Aerospace Technology
AFOSR SCIENTIFIC REPORT D-& AFOSR— TR— 71 — 2584 DIIMARS NATBONAL BUREAU OF STANDARDS REPORT 10 481 INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY (The previous reports in this series have the NBS Report Nos. 6297, 6484, 6645, 6928, 7093, 7192, 7437, 7587, 7796, 8033, 8186, 8504, 8628, 8919, 9028, 9389, 9500, 9601, 9803, 9905, 10004, 10074, and 10326.) U.S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS U. S. Air Force, Office of Scientific Research Agreement No. AFOSR — ISSA— 70— 0002, Project No. 9750-01. INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY 1 July 1971 Approved for Public Release; Distribution Unlimited Qualified requestors may obtain additional copies from the Defense Decumentation Center; all others should apply to the Clearinghouse for Federal Scientific and Technical Information. NATIONAL BUREAU OF STANDARDS REPORT NBS PROJECT NBS REPORT 2320423 1 July 1971 10 481 3160401 3160404 3160405 3160426 INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY (The previous reports in this series have the NBS Report Nos. 6297, 6484, 6645, 6928, 7093, 7192, 7437, 7587, 7796, 8033, 8186, 8504, 8628, 8919, 9028, 9389, 9500, 9601, 9803, 9905, 10004, 10074, and 10326.) Reference: U. S. Air Force, Office of Scientific Research, Agreement No. AFOSR — ISSA — 70— 0002, Project No. 9750-01. IMPORTANT NOTICE NATIONAL BUREAU OF ST iss accounting documents intended for use within the Government, ; subjected to additional evaluation Approved for public release by the and review. For this reason, th 3 listing of this Report, either in whole or in part, is not autho Director of the National Institute of le Office of the Director, National Bureau of Standards, Washingt Standards and Technology (NIST) by the Government agency for which the Report has been speciticall) copies for its own use. -
Analytical Methods for Toxics Determination • Clinio Locatelli, Marcello Locatelli and Dora Melucci Analytical Methods for Toxics Determination
Analytical Methods for Toxics Determination Analytical Methods Toxics for • Clinio Locatelli, Locatelli Marcello and • Clinio Dora Melucci Analytical Methods for Toxics Determination Edited by Clinio Locatelli, Marcello Locatelli and Dora Melucci Printed Edition of the Special Issue Published in Molecules www.mdpi.com/journal/molecules Analytical Methods for Toxics Determination Analytical Methods for Toxics Determination Editors Clinio Locatelli Marcello Locatelli Dora Melucci MDPI • Basel • Beijing • Wuhan • Barcelona • Belgrade • Manchester • Tokyo • Cluj • Tianjin Editors Clinio Locatelli Marcello Locatelli Alma Mater Studiorum University of Bologna University “G. d’Annunzio” of Chieti and Pescara Italy Italy Dora Melucci Alma Mater Studiorum University of Bologna Italy Editorial Office MDPI St. Alban-Anlage 66 4052 Basel, Switzerland This is a reprint of articles from the Special Issue published online in the open access journal Molecules (ISSN 1420-3049) (available at: https://www.mdpi.com/journal/molecules/special issues/Analytical toxics Determination). For citation purposes, cite each article independently as indicated on the article page online and as indicated below: LastName, A.A.; LastName, B.B.; LastName, C.C. Article Title. Journal Name Year, Article Number, Page Range. ISBN 978-3-03936-716-0 (Hbk) ISBN 978-3-03936-717-7 (PDF) c 2020 by the authors. Articles in this book are Open Access and distributed under the Creative Commons Attribution (CC BY) license, which allows users to download, copy and build upon published articles, as long as the author and publisher are properly credited, which ensures maximum dissemination and a wider impact of our publications. The book as a whole is distributed by MDPI under the terms and conditions of the Creative Commons license CC BY-NC-ND. -
The Development of the Quantum-Mechanical Electron Theory of Metals: 1928---1933
The development of the quantum-mechanical electron theory of metals: 1S28—1933 Lillian Hoddeson and Gordon Bayrn Department of Physics, University of Illinois at Urbana-Champaign, Urbana, illinois 6180f Michael Eckert Deutsches Museum, Postfach 260102, 0-8000 Munich 26, Federal Republic of Germany We trace the fundamental developments and events, in their intellectual as well as institutional settings, of the emergence of the quantum-mechanical electron theory of metals from 1928 to 1933. This paper contin- ues an earlier study of the first phase of the development —from 1926 to 1928—devoted to finding the gen- eral quantum-mechanical framework. Solid state, by providing a large and ready number of concrete prob- lems, functioned during the period treated here as a target of application for the recently developed quan- tum mechanics; a rush of interrelated successes by numerous theoretical physicists, including Bethe, Bloch, Heisenberg, Peierls, Landau, Slater, and Wilson, established in these years the network of concepts that structure the modern quantum theory of solids. We focus on three examples: band theory, magnetism, and superconductivity, the former two immediate successes of the quantum theory, the latter a persistent failure in this period. The history revolves in large part around the theoretical physics institutes of the Universi- ties of Munich, under Sommerfeld, Leipzig under Heisenberg, and the Eidgenossische Technische Hochschule (ETH) in Zurich under Pauli. The year 1933 marked both a climax and a transition; as the lay- ing of foundations reached a temporary conclusion, attention began to shift from general formulations to computation of the properties of particular solids. CONTENTS mechanics of electrons in a crystal lattice (Bloch, 1928); these were followed by the further development in Introduction 287 1928—1933 of the quantum-mechanical basis of the I.