Abstracts IIVI.Pdf

Total Page:16

File Type:pdf, Size:1020Kb

Abstracts IIVI.Pdf Conference Organizers wish to thank the SPONSORS listed below for their contribution to the success of the conference IOFFE PHYSICO- Ioffe Physical-Technical Institute of Russian TECHNICAL Academy of Sciences INSTITUTE Russian Foundation for Basic Research RUSNANO Russian Corporation of Nanotechnologies Russian Corporation of Nanotechnologies RIBER AIXTRON EXHIBITORS: ATC-Semiconductor Technologies & RIBER Bruker AXS Equipment, JSC Valtex International Intech Analytics Corporation 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia © Ioffe Physical-Technical Institute of the Russian Academy of Sciences, 2009 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia Preface Welcome at the 14th International Conference on II-VI Compounds (II-VI-2009) which is held this 2009 year, in Saint-Petersburg, Russia, for the first time. The meeting continues a series of biennial conferences, which was started in Durham, UK, in 1983. The latest conferences were held in Niagara Falls (2003), Warsaw (2005), and Jeju Island (2007). The Conference is organized by the Ioffe Physical Technical Institute of RAS, one of the leading research centers in the world in the field of semiconductor physics and technology. It is famous for numerous discoveries in the field, including pioneering studies of excitonic properties of II-VI compounds. The purpose of the current II-VI compound Conference is to bring together scientists from all over the world, which are active in the fields of basic and applied research of II-VI structures. The Conference Program reflects a revival of interest in the recent years to this group of materials due to the emergence of many fascinating ideas and prospects as well as the development of new technologies. In particular, the wide band gap semiconductors like ZnO, (Zn,Cd)Te, (Zn,Cd)Se provide unique opportunities to exploit the ideas of photonic-band engineering in specially designed quantum nanostructures. This intense activity has yet resulted in the observation of numerous original effects and emergence of new device concepts, including Bose condensation of exciton polaritons ("polariton laser"), triggered single-photon sources for quantum cryptography, optical switches and memories. Important areas that take advantage of the specific properties of II-VI compounds are quantum information processing and spintronics, since II-VI non-magnetic and diluted magnetic semiconductors and quantum dots are ideal objects for experimental modeling of the devices employing the spin degree of freedom. Among other prospective practical applications of the II-VI compounds which will be presented are yellow-to-blue lasers with different pumping types, infrared detectors, terahertz emitters, inter-subband devices like quantum cascade lasers, and nanoscale sensors. A special feature of the 14th Conference is organizing the Session of Review Lectures delivered by most prominent scientists in the field. The attendance of the present conference is relatively high and world wide: approximately 300 scientists from 26 countries. Beside the Review lecturers, we have 21 invited talks, 60 oral and ~200 poster presentations. The Conference proceedings will be published in a special issue of the Physica Status Solidi (c) not later than early spring 2010. We would like to thank on behalf of the Organizing Committee all the sponsors listed subsequently for their substantial support. Without their help it would have been impossible to hold the registration fee low for young physicists, which has allowed many of them to participate in this meeting. We wish all participants an enjoyable and successful meeting. S.A. Permogorov S.V. Ivanov A.A. Toropov Saint-Petersburg, July 10, 2009 3 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia Gottfried Landwehr’s 80th birthday celebration Prof. Dr. rer. nat. Dr. h.c. mult. Gottfried LANDWEHR was born on 22.08.1929 in Osnabrück, Germany. After studying physics at Technical University Karlsruhe, he joined the German National Bureau of Standards Physikalisch Technische Bundesanstalt (PTB), Braunschweig, starting to work on semiconductors and investigating defect-induced electrons in germanium. After his Dissertation (Ph.D.), Gottfried LANDWEHR went to the University of Illinois, Urbana, where he collaborated e.g. with Prof. John BARDEEN (1959-1961), in 1961 he became Assistant Professor there. Back in Germany he became the Head of the President´s Laboratory at the PTB and a member of faculty of Technical University Braunschweig. In 1968, he accepted a position at Würzburg Unversity, Germany, as the chairholder for Experimentelle Physik III and initiated his fundamental research on semiconductors in high magnetic fields peaking up later in the investigations of Q2D-semiconductor systems. In those days he also initiated the famous conference series “Semiconductors in High Magnetic Fields”. Between 1978 and 1983, Gottfried LANDWEHR was director of the Hochfeldmagnetlabor des Max Planck-Institutes für Festkörperforschung in Grenoble, France. Under his directorship there Klaus von KLITZING made his famous measurements on the Quantum Hall Effect, later awarded by the Nobel Prize. Back at Würzburg University, Gottfried LANDWEHR started working on II-VI semiconductor layered structures grown by molecular beam epitaxy, with substantial contributions especially in the field of semimagnetic semiconductors, but also narrow gap HgCdTe as well as ZnSe based laser diodes. His overall achievements and world- wide scientific interactions made Gottfried LANDWEHR an internationally well renowned scientist with tremendous reputation. He is a member of the Bavarian Academy of Sciences. Prof. LANDWEHR made a considerable contribution to the development of collaboration between German and Russian scientists, in particular from the Ioffe Institute. This his activity was highly evaluated by electing him as External Member of the Russian Academy of Sciences and Honorary Member of the Ioffe Institute, St. Petersburg. During the II-VI-2009 Conference a Complimentary Session will be held to mark the 80th birthday of Prof. Gottfried LANDWEHR, the Honorary Chair of the Conference. 4 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia Honorary Chair G. Landwehr Würzburg University, Germany Co - Chairmen S.A. Permogorov Ioffe Institute, Russia S.V. Ivanov Ioffe Institute, Russia Conference Secretary T.V. Shubina Ioffe Institute, Russia International Program Committee K. Ando Japan I.A. Buyanova Sweden J. Cibert France M. Dobrowolska USA J. Gutowski Germany E.L. Ivchenko Russia H. Jackson USA K. Kishino Japan V. P. Kochereshko Russia H. Kobayashi Japan V.D. Kulakovskii Russia S. Lee Korea L. Molenkamp Germany K. Prior UK U. Woggon Germany T. Wojtowicz Poland D. Wolverson UK D.R. Yakovlev Germany Program Chair A.A. Toropov Ioffe Institute, Russia 5 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia International Advisory Committee R. Bhargava USA J.J. Davies UK S. Fujita Japan J.K. Furdyna USA F. Henneberger Germany D. Hommel Germany T.W. Kang Korea C. Klingshirn Germany J. Kossut Poland S.J. Lee Korea H. Mariette France M.C. Tamargo USA A. Waag Germany A. Yoshikawa Japan Local Organizing Committee at the Ioffe Institute P.S. Kop'ev Chair T.A. Komissarova Secretary I.V. Sedova A.V. Lebedev V.N. Jmerik S.V. Sorokin E.R. Seel In association with Agency for Science and Technology INTELLECT Social Program Assistance by E. Moltchanova's Tourist Agency Contact Information Prof. S.V. Ivanov, Ioffe Physical Technical Institute, Polytekhnicheskaya 26, 194021 St.Petersburg, Russia. Phone: +7 (812) 292-7124 Fax: +7 (812) 297-1017 E-mail: [email protected] Conference website: http://www.ioffe.ru/II-VI-2009/ 6 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia CALENDAR OF EVENTS Sunday, August 23 10.00 – 18.00 Registration 10.30 – 12.30 Su1: Review Lectures I 12.30 – 14.00 Lunch 14.00 – 17.00 Su2: Review Lectures II 19.00 – 22.00 Welcome Party Monday, August 24 8.00 – 18.00 Registration 8.50 – 9.15 Mo0: Opening Session 9.15 – 10.45 Mo1: Microcavities 10.45 – 11.15 Coffee Break 11.15 – 13.00 Mo2: Nanostructures I 13.00 – 14.30 Lunch 14.30 – 16.15 Mo3: Diluted Magnetic Semiconductors I 16.15 – 16.45 Coffee Break 16.45 – 18.15 Mo4: Devices I 18.15 – 20.00 Mo5p: Poster session I Tuesday, August 25 8.00 – 18.00 Registration 9.00 – 10.45 Tu1: Spin Physics 10.45 – 11.15 Coffee Break 11.15 – 12.45 Tu2: ZnO Nanostructures 12.45 – 14.15 Lunch 14.15 – 15.45 Tu3: Diluted Magnetic Semiconductors II 15.45 – 16.15 Coffee Break 16.15 – 17.00 Tu4: Diluted Magnetic Semiconductors III 17.00 – 18.00 Tu5: Gottfried Landwehr’s Birthday Session 18.00 – 20.00 Tu6p: Poster Session II Wednesday, August 26 8.00 – 13.00 Registration 9.00 – 10.45 We1: ZnO Growth and Properties 10.45 – 11.15 Coffee Break 11.15 – 12.30 We2: Single Quantum Dots 13.00 – 20.00 Conference Excursion 7 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia 14th International Conference on II-VI Compounds, August 23-28, 2009, St. Petersburg, Russia Thursday, August 27 9.00 – 10.45 Th1: Excitonic and Spin Effects 10.45 – 11.15 Coffee Break 11.15 – 13.00 Th2: Nanostructures II 13.00 – 14.30 Lunch 14.30 – 16.00 Th3: Phonons and Defects 16.00 – 16.30 Coffee Break 16.30 – 17.45 Th4: Devices II 17.45 – 19.15 Th5p: Poster Session III 20.00 – 23.00 Conference Dinner Friday, August 28 9.00 – 10.45 Fr1: Devices III 10.45 – 11.15 Coffee Break 11.15 – 13.00 Fr2: Microcavities and photonic crystals 13.00 – 14.30 Lunch 14.30 – 15.30 Fr3: New Experimental Approaches 15.30 – 15.50 Fr4: Closing Remarks 8 14th International Conference on II-VI Compounds, August 23-28, 2009, St.
Recommended publications
  • Chronicle 2004
    The Annual Magazine of King Edward's School, Birmingham CHRONICLE 2004 CONTENTS Hellos 5 Goodbyes 16 Features 22 Dram a 38 Trips 43 Words and Pictures 62 Music 76 Houses 80 Societies 86 Sport 90 K€S Chronicle 2004 The Editorial Team Hellos & Goodbyes Matthew Gammie Features Matthew Hosty Trips Euan Stirling & Oliver Carter Drama Peter Wozniak Music Tom Cadigan Words Charles Butler Houses Amit Sinha Societies Jamie Sunderland Sport Philip Satterthwaite, Amer Shafi, & Vidu Shanmugarajah Cover Elliot Weaver Banners Tarsem Madhar Staff Tom Hosty Editorial Chronicle is the work of a large number of people. Most immediately we have to thank Sandra Bürden at the Resources Centre, who assembles the pages on her computer and who is to thank for much of the fine detail of the magazine's final appearance: I am hugely indebted to her for her energy, initiative and attention to detail. Earlier in the chain stand the section editors, whose job is to round up copy and pictures for their sections and devise the running order and general page layouts for that section. They also have to go in for a good deal of rewriting: prolixity must be trimmed, irrelevance eliminated, errors put right and facetiousness filtered out. To be a good editor requires not only a good ear for language and a high level of compétence in written English: it also calls for patience and good humour in the actual pursuit of material. Mirabile dictu, it sometimes happens that contributors to the magazine are strong on promises but weak on performance. This year's editors have been terrifie.
    [Show full text]
  • DMAAC – February 1973
    LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base.
    [Show full text]
  • Viscosity from Newton to Modern Non-Equilibrium Statistical Mechanics
    Viscosity from Newton to Modern Non-equilibrium Statistical Mechanics S´ebastien Viscardy Belgian Institute for Space Aeronomy, 3, Avenue Circulaire, B-1180 Brussels, Belgium Abstract In the second half of the 19th century, the kinetic theory of gases has probably raised one of the most impassioned de- bates in the history of science. The so-called reversibility paradox around which intense polemics occurred reveals the apparent incompatibility between the microscopic and macroscopic levels. While classical mechanics describes the motionof bodies such as atoms and moleculesby means of time reversible equations, thermodynamics emphasizes the irreversible character of macroscopic phenomena such as viscosity. Aiming at reconciling both levels of description, Boltzmann proposed a probabilistic explanation. Nevertheless, such an interpretation has not totally convinced gen- erations of physicists, so that this question has constantly animated the scientific community since his seminal work. In this context, an important breakthrough in dynamical systems theory has shown that the hypothesis of microscopic chaos played a key role and provided a dynamical interpretation of the emergence of irreversibility. Using viscosity as a leading concept, we sketch the historical development of the concepts related to this fundamental issue up to recent advances. Following the analysis of the Liouville equation introducing the concept of Pollicott-Ruelle resonances, two successful approaches — the escape-rate formalism and the hydrodynamic-mode method — establish remarkable relationships between transport processes and chaotic properties of the underlying Hamiltonian dynamics. Keywords: statistical mechanics, viscosity, reversibility paradox, chaos, dynamical systems theory Contents 1 Introduction 2 2 Irreversibility 3 2.1 Mechanics. Energyconservationand reversibility . ........................ 3 2.2 Thermodynamics.
    [Show full text]
  • User Guide to 1:250,000 Scale Lunar Maps
    CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west.
    [Show full text]
  • Astrophysics in 2006 3
    ASTROPHYSICS IN 2006 Virginia Trimble1, Markus J. Aschwanden2, and Carl J. Hansen3 1 Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575, Las Cumbres Observatory, Santa Barbara, CA: ([email protected]) 2 Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Organization ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304: ([email protected]) 3 JILA, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder CO 80309: ([email protected]) Received ... : accepted ... 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: gen- eral, planets and satellites: general, astrobiology CONTENTS 1. Introduction 6 1.1 Up 6 1.2 Down 9 1.3 Around 10 2. Solar Physics 12 2.1 The solar interior 12 2.1.1 From neutrinos to neutralinos 12 2.1.2 Global helioseismology 12 2.1.3 Local helioseismology 12 2.1.4 Tachocline structure 13 arXiv:0705.1730v1 [astro-ph] 11 May 2007 2.1.5 Dynamo models 14 2.2 Photosphere 15 2.2.1 Solar radius and rotation 15 2.2.2 Distribution of magnetic fields 15 2.2.3 Magnetic flux emergence rate 15 2.2.4 Photospheric motion of magnetic fields 16 2.2.5 Faculae production 16 2.2.6 The photospheric boundary of magnetic fields 17 2.2.7 Flare prediction from photospheric fields 17 c 2008 Springer Science + Business Media.
    [Show full text]
  • Adams Adkinson Aeschlimann Aisslinger Akkermann
    BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA.
    [Show full text]
  • Index of First Authors
    Cambridge University Press 978-0-521-51489-7 - Astronomical Applications of Astrometry: Ten Years of Exploitation of the Hipparcos Satellite Data Michael Perryman Index More information Index of first authors Aarseth, S. J. 286 Anderson, J. A. 119 Abad, C. 62, 279, 300, 310, 319, 526 Anderson, M. W. B. 130 Abadi, M. G. 527 Andrade, M. 125 Abbett, W. P. 345 Andrei,A.H.30, 60, 579 Abrahamyan, H. V. 228 Andronov, I. L. 170, 171 Abt, H. A. 34, 38, 107, 217, 219, 390, Andronova, A. A. 510 422, 447 Angione, R. J. 133 Acker, A. 454 Anglada Escude,´ G. 207 Adams, W. S. 354 Anguita, C. 255 Adelman-McCarthy, J. K. 74 Ankay, A. 447 Adelman, S. J. 160, 161, 167, 172, 186, 195, 235, 393, 427 Anosova, J. P. 309 Aerts, C. 184–188 Antonello, E. 125, 175, 176, 281, 285, 286 Agekyan, T. A. 303 Antoniucci, S. 358 Aguilar,L.A.279 Antonov, V. A. 584 Aitken, R. G. 97 Aoki, S. 14 Ak, S. 545 Appenzeller, I. 474 Akeson, R. L. 139 Applegate, J. H. 572 Alcaino, G. 547 Arellano Ferro, A. 173, 222 Alcala,´ J. M. 431 Arenou, F. 13, 61, 100, 106, 114, 115, 182, 208–211, 213, Alcobe,´ S. 526 298, 393, 470, 471, 594 Alcock, C. 173, 249, 452, 520 Arfken, G. 508 Alencar, S. H. P. 123, 419 Argus, D. F. 580 Alessi, B. S. 299 Argyle, R. W. 30, 57 Alexander, D. R. 344, 346, 349 Arias, E. F. 9, 69 Alksnis, A. 450 Arifyanto, M. I. 307, 526 Allard, F.
    [Show full text]
  • From Adam to Us Part 2 Sample
    From Adam to Us Part 2: Castles to Computers Ray and Charlene Notgrass Activities by Bethany Poore Maps by Nate McCurdy From Adam to Us Part 2 Ray and Charlene Notgrass Activities by Bethany Poore Maps by Nate McCurdy ISBN 978-1-60999-085-5 Copyright © 2016 Notgrass Company. All rights reserved. No part of this material may be reproduced without permission from the publisher. Cover Photo Credits Front Cover: Carcassonne, France (leoks/Shutterstock.com), Ship (Pixabay) St. Basil’s Cathedral in Moscow, Russia (Marina99/Shutterstock.com) Llama in Machu Picchu, Peru (Alexandra Copley/Shutterstock.com) Singapore (Patrick Foto/Shutterstock.com), Space Walk (NASA) Back Cover: Eiffel Tower in Paris, France (Pixabay), Author Photo (Mev McCurdy) All product names, brands, and other trademarks mentioned or pictured in this book are used for educational purposes only. No association with or endorsement by the owners of the trademarks is intended. Each trademark remains the property of its respective owner. Unless otherwise noted, Scripture quotations taken from the New American Standard Bible, Copyright 1960, 1962, 1963, 1971, 1972, 1973,1975, 1977, 1995 by the Lockman Foundation. Used by permission. Cover design by Mary Evelyn McCurdy Interior design by Charlene Notgrass Printed in the United States of America Notgrass Company • 975 Roaring River Road • Gainesboro, TN 38562 1-800-211-8793 • www.notgrass.com Table of Contents Unit 16 – Chivalry, Trade, and New Freedoms ..............................................................................509
    [Show full text]
  • Conditions for the Existence of Backward Surface Magnetostatic Waves in a Ferrite–Insulator–Metal Structure V
    TECHNICAL PHYSICS LETTERS VOLUME 24, NUMBER 7 JULY 1998 Conditions for the existence of backward surface magnetostatic waves in a ferrite–insulator–metal structure V. I. Zubkov and V. I. Shcheglov Institute of Radio Engineering and Electronics, Russian Academy of Sciences, Fryazino ~Submitted December 10, 1996; resubmitted March 13, 1998! Pis’ma Zh. Tekh. Fiz. 24, 1–7 ~July 12, 1998! A theoretical analysis is made of the dispersion of surface magnetostatic waves ~SMSWs! at different frequencies propagating in ferrite–insulator–metal ~FIM! structures magnetized by a uniform magnetic field. It is established that depending on the ratio between the thicknesses of the ferrite and insulating layers in FIM structures, backward SMSWs exist in different frequency ranges and have different wave numbers and directions of propagation. The conditions for which backward SMSWs may be observed directly in FIM structures are determined. © 1998 American Institute of Physics. @S1063-7850~98!00107-4# Studies of the dispersion of forward and backward sur- with varying VH , whereas the angle w is considered to be a face magnetostatic waves ~SMSWs! in ferrite–insulator– free parameter which is defined by the antenna exciting the metal ~FIM! structures are of great interest because of their SMSW (w5w0) ~Refs. 1–6!. Below we determine the rela- possible applications for analog processing of information in tionship between the frequency range of existence, the wave the microwave range ~see Ref. 1 and the literature cited numbers, and directions of propagation of backward SM- therein!. The numerous studies on the dispersion of SMSWs SWs, and we show that the type of wave cannot be accu- in FIM structures with specific parameters1–6 create the im- rately determined merely using the dispersion law.
    [Show full text]
  • Department of Physics Weber State University Program Review Self
    Department of Physics Weber State University Program Review Self-Study February 6, 2008 WSU Program Review Self-Study Format & Standards Page 1 of 64 WSU Program Review Self-Study Format & Standards Page 2 of 64 Description of the Review Process: The Review Team members are listed below. Their resumes are included as Appendix 1 of this document. • Dr. Paula Szkody, Professor, Department of Astronomy, University of Washington, • Dr. D. Mark Riffe, Associate Professor, Department of Physics, Utah State University, • Dr. Daniel Bedford, Assistant Professor, Department of Geography, Weber State University, • Dr. H. Laine Berghout, Associate Professor, Department of Chemistry, Weber State University. The Program Review Self-Study (this document) was prepared by the Chair of the Department of Physics in consultation with the departmental faculty members. Data and information within the document were obtained from the following sources: 1. Departmental Annual Summaries for the academic years 2002/03, 2003/04, 2004/05, 2005/06, and 2006/07. 2. Data provided by Weber State University’s Division of Budget and Institutional Research. 3. Departmental assessment documents. 4. Department of Physics Program Review Self-Study document, May 2002. As described in the Semester Sequence of Program Review Activities (revised June 2004), the steps that have been, or will be taken throughout the review process include: 1. The selection of the external Review Team by the Department of Physics. The Dean of the College of Science has approved the selection of the team members. 2. On November 15, 2007, the self-study document will be submitted to the Dean of the College of Science for review and approval.
    [Show full text]
  • User Guide To
    USER GUIDE TO 1 2 5 0 , 000 S CA L E L U NA R MA P S DANNY C. KINSLER Lunar Science Institute 3303 NASA Road #1 Houston, TX 77058 Telephone: 713/488-5200 Cable Address: LUNSI The Lunar Science Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration. This document constitutes LSI Contribution No. 206 March 1975 USER GUIDE TO 1 : 250 , 000 SCALE LUNAR MAPS GENERAL In 1 972 the NASA Lunar Programs Office initiated the Apoll o Photographic Data Analysis Program. The principal point of this program was a detail ed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17 . One of the requirements of this program was the production of detailed photo base maps at a useabl e scale . NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas . This paper is desi gned to present in outline form the neces- sary background information for users to become familiar with the program. MAP FORMAT The scale chosen for the project was 1:250,000* . The re- search being done required a scale that Principal Investigators (PI's) using orbital photography could use, but would also serve PI's doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. The base is compiled from vertical Metric photography from Apollo missions 15, 16, and 17.
    [Show full text]
  • The Astronomer Magazine Index
    The Astronomer Magazine Index The numbers in brackets indicate approx lengths in pages (quarto to 1982 Aug, A4 afterwards) 1964 May p1-2 (1.5) Editorial (Function of CA) p2 (0.3) Retrospective meeting after 2 issues : planned date p3 (1.0) Solar Observations . James Muirden , John Larard p4 (0.9) Domes on the Mare Tranquillitatis . Colin Pither p5 (1.1) Graze Occultation of ZC620 on 1964 Feb 20 . Ken Stocker p6-8 (2.1) Artificial Satellite magnitude estimates : Jan-Apr . Russell Eberst p8-9 (1.0) Notes on Double Stars, Nebulae & Clusters . John Larard & James Muirden p9 (0.1) Venus at half phase . P B Withers p9 (0.1) Observations of Echo I, Echo II and Mercury . John Larard p10 (1.0) Note on the first issue 1964 Jun p1-2 (2.0) Editorial (Poor initial response, Magazine name comments) p3-4 (1.2) Jupiter Observations . Alan Heath p4-5 (1.0) Venus Observations . Alan Heath , Colin Pither p5 (0.7) Remarks on some observations of Venus . Colin Pither p5-6 (0.6) Atlas Coeli corrections (5 stars) . George Alcock p6 (0.6) Telescopic Meteors . George Alcock p7 (0.6) Solar Observations . John Larard p7 (0.3) R Pegasi Observations . John Larard p8 (1.0) Notes on Clusters & Double Stars . John Larard p9 (0.1) LQ Herculis bright . George Alcock p10 (0.1) Observations of 2 fireballs . John Larard 1964 Jly p2 (0.6) List of Members, Associates & Affiliations p3-4 (1.1) Editorial (Need for more members) p4 (0.2) Summary of June 19 meeting p4 (0.5) Exploding Fireball of 1963 Sep 12/13 .
    [Show full text]