Conditions for the Existence of Backward Surface Magnetostatic Waves in a Ferrite–Insulator–Metal Structure V

Total Page:16

File Type:pdf, Size:1020Kb

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. pression that the problem of the existence of backward SM- It is known1–3,5 that SMSWs exist in a frequency range SWs in FIM structures has been well studied. However, the between a lower limit Vl and an upper limit Vu(s,w) and in absence of direct experimental evidence of their existence4–6 a range of angles w bounded by the ‘‘cutoff’’ angles is incomprehensible. Some possible reasons for this are sug- 6wc(s). We then have Vu(`,0),Vu(s,w),Vu(0,0) and gested below. wc(s),wc(0), where Vu(`,0) and Vu(0,0) and wc(`) and We shall consider an infinite FIM structure in the yz wc(0) are the upper frequencies and cutoff angles for a plane, consisting of a ferrite film of thickness d magnetized SMSW in the ferrite film (s5`) and in the ferrite–metal to saturation and an ideal conducting metal layer, separated structure (s50): by an insulating layer ~in magnetostatics, a vacuum layer! of thickness s ~subsequently, this layer is simply denoted by s!. Vl5AVH~VH11!, ~2! The x50 plane is the surface of the ferrite film closest to the Vu~`,0!5VH10.5, ~3! metal layer. The magnetizing field H0 is directed along the z 2 21 axis. In this FIM structure an SMSW propagates with the wc~`!5arccos$@V1AV 2VH~VH11!#~VH11! %, frequency v and wave vector k, whose group velocity vg is ~4! directed at the angles of w and c to the y axis. The dispersion relation for the SMSW in the FIM struc- Vu~0,0!5VH11, ~5! 7 ture is written in the form: 2 21 wc~0!5arccosA@V 2VH~VH11!#~VH11! . ~6! @b22ma coth~akd!#1~b1222pn cos w! Figure 1 shows dispersion curves Vs(ky ,d) for a SMSW 3exp~22ks!50, ~1! in an FIM structure with different values of s. It can be seen that there are three types of curves. First, in the frequency 21 2 2 1/2 2 2 2 where a5@m sin w1cos w# ; b5(n 2m 1m)cos w range Vu(`,0),V,Vu(0,0) the functions Vs(kyd) for 2 2 21 2 2 21 2m21; m511VH(VH2V ) ; n5V(VH2V ) ; SMSWs in an FIM structure with small s (0,s<sb1) have V5v(4puguM )21; V 5H (4pM )21;4pM is the a maximum at kd5k d and tend to V (`,0) for kd ` 0 H 0 0 0 max,s u → saturation magnetization of the ferrite film, g is the electron ~curves 2 and 3!. Each forward SMSW with k,kmax,s corre- gyromagnetic ratio, and p561. Only SMSWs propagating sponds to a backward SMSW with k in kmax,s,k,`. Second, in the x50 plane of the FIM structure (p51) can be both in the frequency range Vl,V,Vu(`,0) the function 1–3 forward and backward waves. Vs(kyd) for an SMSW in a FIM structure with large s The dispersion relation ~1! is considered to be the dis- (s>sb1) has a maximum and a minimum ~curves 4–7!.A persion law Vs(k) for given parameters w, d, s, and VH and backward SMSW exists for sb1,s,sb2 and in the frequency is used to determine the type of SMSW ~forward or range dV(s,0)!Vl . The forward SMSWs have wave num- 1–5 backward!. The form of the dispersion law Vs(k) depends bers k in the ranges 0,k,kmax,s and kmin,s,k,` while the on the ratio between d and s and does not vary qualitatively backward SMSWs have wave numbers in the range 1063-7850/98/24(7)/3/$15.00 499 © 1998 American Institute of Physics 500 Tech. Phys. Lett. 24 (7), July 1998 V. I. Zubkov and V. I. Shcheglov FIG. 1. Dispersion curves Vs(kyd) for SMSWs in an 4 FIM structure with different s for VH50.25 ~sb1' 3d and 1 sb2'2d!. Curves: 1—s50; 2—s5 3d; 3—s5d; 4—s51.467d; 5—s51.6d; 6—s51.733d; 7—s51.867d; 8—s52d; 9—s54d, and 10—s5`. For curves 2 and 6 the points kmax,s8 , kmin,s8 , Vu(s,0), and dVs are indicated. kmax,s,k,kmin,s ~curves 4–7!. Third, the functions Vs(kyd) points. If these are numbered according to increasing ky , for SMSWs in an FIM structure with sb2,s,` have a point forward SMSWs exist at the first and third points with back- of inflection ~curve 8!, and only forward SMSWs could exist ward SMSWs at the second. in such structures. It can be seen from the curves kz(ky) ~Fig. 2! that in FIM However, relation ~1! defines the dispersion surface structures with different s, backward SMSWs in different Vs(ky ,kz) ~ky and kz are the projections of the SMSW wave frequency ranges propagate in different ranges of variation of vector k on the y and x axes! and the dispersion law Vs(ky) the angle w and have different wave numbers. is its intersection with the plane kz50 and does not give We shall analyze SMSWs in FIM structures with small s complete information, which is obtained by additionally ~the line of direction intersects the kz(ky) curves at two studying its intersections with the planes Vi5const(ky0kz), points!. In the frequency range between Vu(`,0) and 8,9 i.e., the curves kz(ky) ~as for an SMSW in a ferrite film !. Vu(0,0) backward SMSWs exist for angles w between Figure 2 gives the curves kz(ky) for an SMSW wave with the 2wc(0) and 1wc(0), since the curves kz(ky) resemble non- frequencies V50.608, 0.695, 0.745, and 0.775 in an FIM canonical ellipses lying at ky.0 ~dotted curve 2! and the line structure with different s. In the ferrite film and the ferrite– of direction can only intersect these for uw0u,uwc(0)u. In the metal structure the curves kz(ky) resemble canonical frequency range between Vl and Vu(`,0) backward SM- 2,8,9 hyperbolas ~curves 1 and 4!. We denote these as qH(`) SWs exist in the range of angles uwc(`)u,uw0u,uwc(0)u for s5` and qH(0) for s50. The direction of propagation since the curves kz(ky) are strictly increasing functions ~solid of the SMSWs on the k y0kz plane is given by a straight line curves 2 and 3! situated between qH(0) and qH(`), and the emerging from the origin at the angle w0 ~subsequently line of direction can only intersect them in this range of called the line of direction; when discussing Fig. 2 we shall angles. The curves kz(ky) at the point with the lowest value draw this line mentally!. For uw0u,uwc,su this line intersects of ky ~ky,inf,s for kz50! are close to qH(0); ky,inf,s increases qH(`) and qH(0) at a single point at which the projection with increasing s. of the group velocity on the direction of the phase velocity We shall now analyze SMSWs in an FIM structure with shows that the SMSWs in the ferrite film and in the ferrite– large s ~the line of direction intersects the curves kz(ky)at metal structure are forward waves. In the FIM structure the three points! where two forward and one backward SMSW line of direction intersects the curves kz(ky) at two or three exist. In an FIM structure with sb1,s,sb2 the curves kz(ky) Tech. Phys. Lett. 24 (7), July 1998 V. I. Zubkov and V. I. Shcheglov 501 FIG. 2. Curves of kz(ky) for SMSWs at frequencies V50.695 ~solid curves!, 0.745 ~dashed curves!, and 0.775 ~dotted curves! in an FIM structure with different s for VH50.25. Solid and dotted curves: 1—s50; 2—s5d; 3—s52d; 4—s54d; 5—s5`.
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]
  • Of Vertebrate Fossils from the Middle Eocene Oil Shale of Messel, Germany: Implications for Their Taphonomy and Palaeoenvironment
    Palaeogeography, Palaeoclimatology, Palaeoecology 416 (2014) 92–109 Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Isotope compositions (C, O, Sr, Nd) of vertebrate fossils from the Middle Eocene oil shale of Messel, Germany: Implications for their taphonomy and palaeoenvironment Thomas Tütken ⁎ Steinmann-Institut für Geologie, Mineralogie und Paläontologie, Universität Bonn, Poppelsdorfer Schloss, 53115 Bonn, Germany article info abstract Article history: The Middle Eocene oil shale deposits of Messel are famous for their exceptionally well-preserved, articulated 47- Received 15 April 2014 Myr-old vertebrate fossils that often still display soft tissue preservation. The isotopic compositions (O, C, Sr, Nd) Received in revised form 30 July 2014 were analysed from skeletal remains of Messel's terrestrial and aquatic vertebrates to determine the condition of Accepted 5 August 2014 geochemical preservation. Authigenic phosphate minerals and siderite were also analysed to characterise the iso- Available online 17 August 2014 tope compositions of diagenetic phases. In Messel, diagenetic end member values of the volcanically-influenced 12 Keywords: and (due to methanogenesis) C-depleted anoxic bottom water of the meromictic Eocene maar lake are isoto- Strontium isotopes pically very distinct from in vivo bioapatite values of terrestrial vertebrates. This unique taphonomic setting al- Oxygen isotopes lows the assessment of the geochemical preservation of the vertebrate fossils. A combined multi-isotope Diagenesis approach demonstrates that enamel of fossil vertebrates from Messel is geochemically exceptionally well- Enamel preserved and still contains near-in vivo C, O, Sr and possibly even Nd isotope compositions while bone and den- Messel tine are diagenetically altered.
    [Show full text]
  • Geoscience and a Lunar Base
    " t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history.
    [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]
  • ADAPTATION of FORESTS and PEOPLE to CLIMATE Change – a Global Assessment Report
    International Union of Forest Research Organizations Union Internationale des Instituts de Recherches Forestières Internationaler Verband Forstlicher Forschungsanstalten Unión Internacional de Organizaciones de Investigación Forestal IUFRO World Series Vol. 22 ADAPTATION OF FORESTS AND PEOPLE TO CLIMATE CHANGE – A Global Assessment Report Prepared by the Global Forest Expert Panel on Adaptation of Forests to Climate Change Editors: Risto Seppälä, Panel Chair Alexander Buck, GFEP Coordinator Pia Katila, Content Editor This publication has received funding from the Ministry for Foreign Affairs of Finland, the Swedish International Development Cooperation Agency, the United Kingdom´s Department for International Development, the German Federal Ministry for Economic Cooperation and Development, the Swiss Agency for Development and Cooperation, and the United States Forest Service. The views expressed within this publication do not necessarily reflect official policy of the governments represented by these institutions. Publisher: International Union of Forest Research Organizations (IUFRO) Recommended catalogue entry: Risto Seppälä, Alexander Buck and Pia Katila. (eds.). 2009. Adaptation of Forests and People to Climate Change. A Global Assessment Report. IUFRO World Series Volume 22. Helsinki. 224 p. ISBN 978-3-901347-80-1 ISSN 1016-3263 Published by: International Union of Forest Research Organizations (IUFRO) Available from: IUFRO Headquarters Secretariat c/o Mariabrunn (BFW) Hauptstrasse 7 1140 Vienna Austria Tel: + 43-1-8770151 Fax: + 43-1-8770151-50 E-mail: [email protected] Web site: www.iufro.org/ Cover photographs: Matti Nummelin, John Parrotta and Erkki Oksanen Printed in Finland by Esa-Print Oy, Tampere, 2009 Preface his book is the first product of the Collabora- written so that they can be read independently from Ttive Partnership on Forests’ Global Forest Expert each other.
    [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]
  • LERMA REPORT V1.1 PART II
    LERMA 2007-2012 Contractualisation vague D Results vol. 3 Bibliography (version 1.1) Conception graphique S. Cabrit Sect. 3. Bibliography Sect. 3. Bibliography A detailed analysis of the lab's production would need a huge investment to be truly meaningful, so we better stay with simple facts. The table below shows the distribution among years and thematic poles of refereed and non refereed publications during the reporting period. Year ACL Publ. Pole 1 Pole 2 Pole 3 Pole 4 Overlap 2007 119 37 45 27 18 8 2008 133 40 57 25 21 10 2009 116 27 59 17 17 4 2010 214 50 112 25 87 60 2011 197 81 71 53 51 59 2012 77 31 29 15 10 8 Total 856 266 373 162 204 149 Table 2: Count of refereed publications from the ADS database Year Publis ACL Pôle 1 Pôle 2 Pôle 3 Pôle 4 Overlap 2007 2409 988 798 220 502 99 2008 2239 633 1166 222 290 72 2009 1489 341 852 119 196 19 2010 3283 1394 1412 213 1548 1284 2011 3035 2331 637 1345 1434 2712 2012 239 183 62 20 2 28 Totaux 12694 5870 4927 2139 3972 4214 Table 3: Count of the citations to the refereed publications from the ADS database. Beware the incompleteness of citations to plasma physics, molecular physics, remote sensing and engineering papers in this database Year ACL Publ. Pole 1 Pole 2 Pole 3 Pole 4 2007 20 27 18 8 28 2008 17 16 20 9 14 2009 13 13 14 7 12 2010 15 28 13 9 18 2011 15 29 9 25 28 2012 3 6 2 1 0 Totaux 15 22 13 13 19 Table 4: Average citation rate for the same publications Sect.
    [Show full text]
  • Smithsonian Contributions to Astrophysics
    Smithsonian Contributions to Astrophysics VOLUME 5, NUMBER 8 AN ANNOTATED BIBLIOGRAPHY ON INTERPLANETARY DUST by PAUL W. HODGE, FRANCES W. WRIGHT, AND DORRIT HOFFLEIT SMITHSONIAN INSTITUTION Washington, D.C. 1961 Publications of the Astrophysical Observatory This series, Smithsonian Contributions to Astrophysics, was inaugurated in 1956 to provide a proper communication for the results of research con- ducted at the Astrophysical Observatory of the Smithsonian Institution. Its purpose is the "increase and diffusion of knowledge" in the field of astrophysics, with particular emphasis on problems of the sun, the earth and the solar system. Its pages are open to a limited number of papers by other investigators with whom we have common interests. Another series is Annals of the Astrophysical Observatory. It was started in 1900 by the Observatory's first director, Samuel P. Langley, and has been published about every 10 years since that date. These quarto volumes, some of which are still available, record the history of the Observatory's researches and activities. Many technical papers and volumes emanating from the Astrophysical Observatory have appeared in the Smithsonian Miscellaneous Collections. Among these are Smithsonian Physical Tables, Smithsonian Meteorological Tables, and World Weather Records. Additional information concerning these publications may be secured from the Editorial and Publications Division, Smithsonian Institution, Wash- ington, D.C. FBED L. WHIPPLE, Director, Astrophysical Observatory, Cambridge, Mass. Smithsonian Institution. For sale by the Superintendent of Documents, U.S. Government Printing Office Washington 25, D.C. - Price 25 cents An Annotated Bibliography on Interplanetary Dust BY PAUL W. HODGE,1 FRANCES W. WRIGHT,1 AND DORRIT HOFFLEIT3 This annotated bibliography presents a AHNERT, E.
    [Show full text]