Shock Papers 2014

Total Page:16

File Type:pdf, Size:1020Kb

Shock Papers 2014 Shock Physics Papers 2014 Abotula, S., Heeder, N., Chona, R. and Shukla, A. 2014 "Dynamic thermomechanical response of Hastelloy X to shock wave loading" Exper. Mech. 54 279-291 Abrosimov, S.A., Bazhulin, A.P., Bolshakov, A.P., Konov, V.I., Krasyuk, I.K., Pashinin, P.P., Ralchenko, V.G., Semenov, A.Y., Sovyk, D.N., Stuchebryukhov, I.A., Fortov, V.E., Khishchenko, K.V. and Khomich, A.K. 2014 "Experimental investigation into polycrystalline and single-crystal diamonds under negative pressures formed by picosecond laser pulses" Dokl. Physics 59 309-312 Adams, C.D., Anderson, W.W., Blumenthal, W.R. and Gray III, G.T. 2014 "Elastic precursor decay in S-200F beryllium" J. Phys.: Conf. Ser. 500 112001 Aduev, B.P., Belokurov, G.M., Grechin, S.S. and Liskov, I.Y. 2014 "On shock initiation in brisant explosives by a high-current electron beam" Tech. Phys. 59 60-65 Aduev, B.P., Belokurov, G.M., Grechin, S.S. and Liskov, I.Y. 2014 "Explosive decomposition of hexogen monocrystals induced by a pulsed electron beam" Tech. Phys. Letts 40 1045-1047 Adushkin, V.V. and Oparin, V.N. 2014 "From the alternating-sign explosion response of rocks to the pendulum waves in stressed geomedia. 3" J. Mining Sci. 50 623- 645 Agranat, M.B., Ashitkov, S.I. and Komarov, P.S. 2014 "Metal behavior near theoretical ultimate strength in experiments with femtosecond laser pulses" Mech. Solids 49 643-648 Agrawal, V. and Bhattacharya, K. 2014 "Shock wave propagation through a model one dimensional heterogeneous medium" Int. J. Solids Structures 51 3604-3618 Agrawal, V., Arya, G. and Oswald, J. 2014 "Simultaneous iterative Boltzmann inversion for coarse-graining of polyurea" Macromolecules 47 3378-3389 Aizawa, T., Matsuzawa, K., Okagawa, K. and Ishibashi, M. 2014 "Parallel seam welding of aluminum sheets by magnetic pulse welding method with collision between metal jets" Mater. Sci. Forum 767 171-176 Alexander, C.S., Key, C.T. and Schumacher, S.C. 2014 "Improved understanding of the dynamic response of anisotropic directional composite materials through the combination of experiments and modeling" J. Phys.: Conf. Ser. 500 112002 Alhadid, M.M.A., Soliman, A.M., Nehdi, M.L. and Youssef, M.A. 2014 "Critical overview of blast resistance of different concrete types" Mag. Concrete Res. 66 72-81 Aliverdiev, A.A., Batani, D., Antonelli, L., Jakubowska, K., Dezulian, R., Amirova, A.A., Gajiev, G.M., Khan, M. and Pant, H.C. 2014 "Use of multilayer targets for achieving off-Hugoniot states" Phys. Rev. E 89 053101, 059902 Alwmark, C., Alwmark-Holm, S., Ormo, J. and Sturkell, E. 2014 "Shocked quartz grains from the Malingen structure, Sweden-Evidence for a twin crater of the Lockne impact structure" Meteor. Planet. Sci. 49 1076-1082 1 An, Q., Goddard, W.A., Zybin, S.V. and Luo, S.N. 2014 "Inhibition of hotspot formation in PBXs using an interface-matching low density polymer coating at the polymer-explosive interface" J. Phys. Chem. C 118 19918-19928 Anand, R.K. 2014 "Shock jump relations for a dusty gas atmosphere" Astrophys. Space Sci. 349 181-195 Anderson, W.W., Jensen, B.J., Cherne, F.J., Owens, C.T., Ramos, K.J. and Lieber, M.A. 2014 "Enhancing impact velocity with shock interactions in a restricting die" J. Phys.: Conf. Ser. 500 142001 Anderson, E.K., Aslam, T.D. and Jackson, S.I. 2014 "Transverse initiation of an insensitive explosive in a layered slab geometry: Front shapes and post-shock flow measurements" Combust. Flame 161 1944-1954 Andrews, R.G., White, J.D.L., Durig, T. and Zimanowski, B. 2014 "Discrete blasts in granular material yield two-stage process of cavitation and granular fountaining" Geophys. Res. Letts 41 422-428 Angelsky, O.V., Besaga, V.R., Maksimyak, A.P. and Maksimyak, P.p. 2014 "Generation of shock waves in a medium with absorbing particles" Proc. SPIE 9164 91642N Antonov, O., Efimov, S., Gurovich, V.T., Yanuka, D., Shafer, D. and Krasik, Y.E. 2014 "Diagnostics of a converging strong shock wave generated by underwater explosion of spherical wire array" J. Appl. Phys. 115 223303 Ao, T., Harding, E.C., Bailey, J.E., Desjaralis, M.P., Hansen, S.B., Lemke, R.W., Rochau, G.A., Sinars, D.B., Smith, I.C., Geissel, M., Reneker, J., Kernaghan, M.D., Mix, L.P. and Wenger, D.F. 2014 "Progress toward X-ray Thomson scattering of warm dense matter on the Z accelerator" J. Phys.: Conf. Ser. 500 082001 Appleby-Thomas, G.J., Hameed, A., Vignjevic, R., Hazell, P.J., Painter, J. and Cademartori, S. 2014 "On the dynamic tensile strength of zirconium" J. Phys.: Conf. Ser. 500 112004 Appleby-Thomas, G.J., Hazell, P.J., Sheldon, R.P., Stennett, C., Hameed, A. and Wilgeroth, J.M. 2014 "The high strain-rate behaviour of selected tissue analogues" J. Mech. Behav. Biomed. Mater. 33 124-135 Arciniega-Ceballos, A., Alatorre-Ibargüengoitia, M., Scheu, B., Dingwell, D.B. and Delgado-Granados, H. 2014 "Seismological analysis of conduit dynamics in fragmentation experiments" J. Geophys. Res.: Solid Earth 119 2215-2229 Arkani-Hamed, J. and Ivanov, B.A. 2014 "Shock wave propagation in layered planetary embryos" Phys. Earth Planet. Inter. 230 45-59 Armstrong, M.R., Crowhurst, J.C., Bastea, S., Zaug, J.M. and Goncharov, A.F. 2014 "Sub-100 ps laser-driven dynamic compression of solid deuterium with a ∼40 μJ laser pulse" Appl. Phys. Letts 105 021904 Armstrong, M.R., Zaug, J.M., Grant, C.D., Crowhurst, J.C. and Bastea, S. 2014 "Ultrafast shock compression of an oxygen-balanced mixture of nitromethane and hydrogen peroxide" J. Phys. Chem. A 118 6148-6153 2 Arora, H., Kelly, M., Worley, A., Del Linz, P., Fergusson, A., Hooper, P.A. and Dear, J.P. 2014 "Compressive strength after blast of sandwich composite materials" Phil. Trans. R. Soc. A 372 20130212 Ashitkov, S.I., Komapov, P.S., Agranat, M.B., Kanel, G.I. and Fortov, V.E. 2014 "Measurements of strength of metals in a picosecond time range" J. Phys.: Conf. Ser. 500 112006 Ashuach, Y., Gissis, I. and Avinadav, C. 2014 "Magnetic gauge for free surface velocities in reinforced concrete blasted by explosives" J. Phys.: Conf. Ser. 500 142002 Aslam, T.D., Gustavsen, R.L. and Bartram, R.D. 2014 "An equation of state for polyurea aerogel based on multi-shock response" J. Phys.: Conf. Ser. 500 032001 Asphaug, E. 2014 "Impact origin of the Moon?" Ann. Rev. Earth Planet. Sci. 42 551- 578 Atzeni, S., Ribeyre, X., Schurtz, G., Schmitt, A.J., Canaud, B., Betti, R. and Perkins, L.J. 2014 "Shock ignition of thermonuclear fuel: Principles and modelling" Nuclear Fusion 54 054008 Austin, R.A., McDowell, D.L. and Benson, D.J. 2014 "The deformation and mixing of several nickel/aluminum powders under shock wave loading: Effects of initial configuration" Model. Simul. Mater. Sci. Engng 22 025018 Austin, R.A., Barton, N.R., Howard, W.M. and Fried, L.E. 2014 "Modeling pore collapse and chemical reactions in shock-loaded HMX crystals" J. Phys.: Conf. Ser. 500 052002 Bachmann, B., Kritcher, A.L., Benedetti, L.R., Falcone, R.W., Glenn, S., Hawreliak, J., Izumi, N., Kraus, D., Landen, O.L., Le Pape, S., Ma, T., Pérez, F., Swift, D. and Döppner, T. 2014 "Using penumbral imaging to measure micrometer size plasma hot spots in Gbar equation of state experiments on the National Ignition Facility" Rev. Sci. Instrum. 85 11D614 Bae, Y.K. 2014 "Table-top generation and spectroscopic study of ~10 TPa high- + energy density materials with C60 hypervelocity (~100 km/s) impact" J. Phys.: Conf. Ser. 500 122001 Baidakova, M.V., Dideikin, A.T., Pavlov, S.I., Sokolov, R.V. and Shnitov, V.V. 2014 "Formation of detonation diamond layers on silicon by the aerosol method" Tech. Phys. Letts 40 739-742 Balakrishnan, K. 2014 "Explosion-driven Rayleigh-Taylor instability in gas-particle mixtures" Phys. Fluids 26 043303 3 Balalaev, V., Voronko, O. and Smirnov, A. 2014 "Detonation pressure of plastisol compositions containing the inorganic fuel and oxidizer", in "Proc. 17th Seminar on New Trends in Research of Energetic Materials", ed. J. Pachman, J. Selesovsky and R. Matyas, pp. 563-571, (Pardubice, Czech Republic, University of Pardubice) Bambach, M.R. 2014 "Numerical simulation of the shock spalling failure of bonded fibre-epoxy strengthening systems for metallic structures" Engng Struct. 64 1- 11 Bandaru, N., Kumar, R.S., Sneed, D., Tschauner, O., Baker, J., Antonio, D., Luo, S.N., Hartmann, T., Zhao, Y.S. and Venkatt, R. 2014 "Effect of pressure and temperature on structural stability of MoS2" J. Phys. Chem. C 118 3230-3235 Banishev, A.A., Shaw, W.L., Curtis, A.D. and Dlott, D.D. 2014 "Dynamics of polymer response to nanosecond shock compression" Appl. Phys. Letts 104 101914 Banishev, A.R. and Dlott, D.D. 2014 "Ultrafast pressure-sensitive paint for shock compression spectroscopy" J. Appl. Phys. 115 203515 Bannikova, I.A., Uvarov, S.V., Bayandin, Y.V. and Naimark, O.B. 2014 "An experimental study of non-Newtonian properties of water under electroexplosive loading" Tech. Phys. Letts 40 766-768 Barenblatt, G.I. 2014 "Flow, Deformation, and Fracture" (Cambridge, Cambridge University Press) Barnes, C.W., Funk, D.J., Hockaday, M.P., Sarrao, J.L. and Stevens, M.F. 2014 "The science of dynamic compression at the mesoscale and the Matter-Radiation Interactions in Extremes (MaRIE) project" J. Phys.: Conf. Ser. 500 092001 Barnes, N.R., Hughes, A., Wood, D.C., Appleby-Thomas, G.J., Leighs, J.A., Goff, M. and Hazell, P.J. 2014 "The effect of fibre orientation on a TWCP composite" J. Phys.: Conf. Ser. 500 182045 Barnes, A.T., Ravi-Chandar, K., Kyriakides, S.
Recommended publications
  • Deep Carbon Emissions from Volcanoes Michael R
    Reviews in Mineralogy & Geochemistry Vol. 75 pp. 323-354, 2013 11 Copyright © Mineralogical Society of America Deep Carbon Emissions from Volcanoes Michael R. Burton Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy [email protected] Georgina M. Sawyer Laboratoire Magmas et Volcans, Université Blaise Pascal 5 rue Kessler, 63038 Clermont Ferrand, France and Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy Domenico Granieri Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy INTRODUCTION: VOLCANIC CO2 EMISSIONS IN THE GEOLOGICAL CARBON CYCLE Over long periods of time (~Ma), we may consider the oceans, atmosphere and biosphere as a single exospheric reservoir for CO2. The geological carbon cycle describes the inputs to this exosphere from mantle degassing, metamorphism of subducted carbonates and outputs from weathering of aluminosilicate rocks (Walker et al. 1981). A feedback mechanism relates the weathering rate with the amount of CO2 in the atmosphere via the greenhouse effect (e.g., Wang et al. 1976). An increase in atmospheric CO2 concentrations induces higher temperatures, leading to higher rates of weathering, which draw down atmospheric CO2 concentrations (Ber- ner 1991). Atmospheric CO2 concentrations are therefore stabilized over long timescales by this feedback mechanism (Zeebe and Caldeira 2008). This process may have played a role (Feulner et al. 2012) in stabilizing temperatures on Earth while solar radiation steadily increased due to stellar evolution (Bahcall et al. 2001). In this context the role of CO2 degassing from the Earth is clearly fundamental to the stability of the climate, and therefore to life on Earth.
    [Show full text]
  • Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
    General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C .
    [Show full text]
  • Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer
    Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer Edited by Neil Pearson With a special foreword by Apollo 7 astronaut Walt Cunningham “When you get back… you will be a national hero. But your photographs… they will live forever. Your only key to immortality is the quality of your photography.” Richard W. Underwood NASA Chief of Photography for Mercury, Gemini and Apollo 4 Small steps. Giant leaps. The English word ‘photograph’ is made up of the The early exploration of space is one such historical ancient Greek words ‘photos’ and ‘graphos’ which event, unrivaled among humanity’s achievements. literally mean ‘light writing’. At the time of the Apollo Fortunately space travelers were able to bring back program, that meant exposing a chemically-treated beautiful, moving and instantly recognizable images film to patterns of light and it was this process which to depict it. Those images add a new understanding made it possible to seize moments in time and share to what it means to be human, what it means to them with the world. live on a delicate little orb circling the Sun since time immemorial. A single photograph can tell a story to billions of people. It transcends language barriers, physical Not only did Apollo bring us this photographic barriers and requires no prior knowledge of testimony but many major advancements in the subject. This is the beauty of photography: photographic technology date back to the extensive it reaches out to all people and everybody can research and engineering that was part of the hugely intuitively understand its form and content.
    [Show full text]
  • Little Learners' Activity Guide
    LUNAR RECONNAISSANCE ORBITER CAMERA Little Learners’ Activity Guide Learn about the Moon with puzzles, coloring, and fun facts! Mare Imbrium Mare Serenitatis Mare Tranquillitatis Oceanus Procellarum Mare Humorum Tycho Crater Visit us online at lroc.sese.asu.edu Online resources Additional information and content, including supplemental learning activities, can be accessed at the following online locations: 1. Little Learners’ Activity Guide: lroc.sese.asu.edu/littlelearners 2. LROC website: lroc.sese.asu.edu 3. Resources for teachers: lroc.sese.asu.edu/teach 4. Learn about the Moon’s history: lroc.sese.asu.edu/learn 5. LROC Lunar Quickmap 3D: quickmap.lroc.asu.edu Copyright 2018, Lunar Reconnaissance Orbiter Camera i Lunar Reconnaissance Orbiter Camera Fun Facts for Beginners • The Moon is 363,301 kilometers (225,745 miles) from the Earth. • The surface area of the Moon is almost as large as the continent of Africa. • It takes 27 days for the Moon to orbit around the Earth. • The farside is the side of the Moon we cannot see from Earth. • South Pole Aitken is the largest impact basin on the lunar farside. • Impact basins are formed as the result of impacts from asteroids or comets and are larger than craters. • Regolith is a layer of loose dust, dirt, soil, and broken rock deposits that cover solid rock. • The two main types of rock that make up the Moon’s crust are anorthosite and basalt. • A person weighing 120 lbs on Earth weighs 20 lbs on the Moon because gravity on the Moon is 1/6 as strong as on Earth.
    [Show full text]
  • July 2019 Medicine’S Lunar Legacies • René T
    OslerianaA Medical Humanities Journal-Magazine Volume 1 • July 2019 Medicine’s Lunar Legacies • René T. H. Laennec Walter R. Bett • Leonardo da Vinci OslerianaA Medical Humanities Journal-Magazine Editor-in-Chief Nadeem Toodayan MBBS Associate Editor Zaheer Toodayan MBBS Corrigendum: As indicated in the introductory piece to this journal and in footnotes to their respective articles, both editors are Basic Physician Trainees and therefore registered members of the Royal Australasian College of Physicians (RACP). In the initial printing of this volume (on this inner cover and on page 5) the postnominal of ‘MRACP’ was used to refer to the editors’ membership status. This postnominal was first applied to the Edi- tor-in-Chief in formal correspondence from The Osler Club of London. Subsequent discussions with the RACP have confirmed that the postnominal is not formally endorsed by the College for trainee members and so it has been removed in this digital edition. Osleriana – Volume 1 Published July 2019 © The William Osler Society of Australia & New Zealand (WOSANZ) e-mail: [email protected] All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, digital, print, photocopy, recording or otherwise, without the prior written permission of WOSANZ or the individual author(s). Permission to reproduce any copyrighted images used in this publication must be obtained from the appropriate rightsholder(s). Please contact WOSANZ for further information as required. Privately printed in Brisbane, Queensland, by Clark & Mackay Printers. Journal concept and WOSANZ logo by Nadeem Toodayan. Journal design and layout by Zaheer Toodayan.
    [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]
  • ∫ K∫ K∫ Chaplygin Equations and an Infinite Set of Uniformly Divergent Gas-Dynamics Equations
    Doklady Physics, Vol. 47, No. 3, 2002, pp. 173–175. Translated from Doklady Akademii Nauk, Vol. 383, No. 1, 2002, pp. 34–36. Original Russian Text Copyright © 2002 by Rylov. PHYSICS Chaplygin Equations and an Infinite Set of Uniformly Divergent Gas-Dynamics Equations A. I. Rylov Presented by Academician G.G. ChernyÏ September 19, 2001 Received September 24, 2001 1. We consider two-dimensional potential ideal-gas (ϕ and ψ) and, as a result, a conservation law in the flows. At the hodograph plane, they are described by physical plane: the Chaplygin equations kβϕ +0,αψ ==βψ –0;αϕ (3) ϕ ψ ϕ ψ z +0,k θ ==θ –0z (1) ()αρu + βv + ()αρv – βu or the Chaplygin equations of the second order for the x y ()ρ ()ρ stream function [1–4]: = f ug+ v x +0.f v – gu x = (4) ρ 1M– 2 Remark. The solutions ϕ = f = const and ψ = g = kψθθ +0,ψ ==z ---dq, k =----------------. (2) zz ∫ q ρ2 const also allow us to obtain certain conservation laws on the (x, y)-plane. For example, substituting either Hereafter, ϕ is the potential; ψ is the stream function; q, f = 1 and g = 0 or f = 0 and g = 1 into (4), we obtain the θ, u, and v are the modulus, angle of inclination, and conservation law for either mass or circulation, respec- horizontal and vertical components of the velocity vec- tively. tor, respectively; M is the Mach number; p is pressure; 2. We consider several tentative examples of exact and ρ is the density.
    [Show full text]
  • GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
    Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins.
    [Show full text]
  • 33Rd LPSC Program Index
    Lunar and Planetary Science XXXIII (2002) lpsc2002.programindex.pdf PROGRAM INDEX * Denotes speaker. These entries are not linked to the abstracts in the program, but will provide a reference tool to help you more easily find a particular author in the program. Abe M. Between Rock/Cold Place Posters, Thu, p.m., Gymnasium Abe Y. Planetary Formation Posters, Tue, p.m., Gymnasium Abe Y. Mars Oceans Posters, Thu, p.m., Gymnasium Abell P. A.* Small Bodies, Thu, p.m., Salon A Abelman L. Future Missions Posters, Thu, p.m., Gymnasium Abe-Ouchi A. Mars Oceans Posters, Thu, p.m., Gymnasium Abreu N. M.* Carbonaceous Chondrites, Tue, p.m., Marina Plaza Ballroom Abshire J. B. Mars Remote Sensing, Wed, p.m., Marina Plaza Ballroom Accomazzi A. Future Missions Posters, Thu, p.m., Gymnasium Acton C. H. Jr. Mars Future Missions Posters, Thu, p.m., Gymnasium Acuña M. H. Lunar Geophysics Posters, Tue, p.m., Gymnasium Acuña M. H. Lunar Regolith, Tue, p.m., Salon A Acuña M. H. Mars Magnetics/Mercury, Wed, p.m., Salon A Adams P. M. Mars Infrared Spectroscopy, Tue, a.m., Salon B Adler M. Mars Landers Posters, Tue, p.m., Gymnasium Agee C. B. Planetary Formation, Tue, p.m., Salon C Agee C. B. Planetary Formation Posters, Tue, p.m., Gymnasium Agnor C. B. Print Only Origins Aharonson O. Mars History, Thu, a.m., Salon C Ahrens T. J. Cratering Processes, Tue, a.m., Salon C Ahrens T. J. IDPs/Micrometeorites Posters, Tue, p.m., Gymnasium Airieau S. Carbonaceous Chondrites, Tue, p.m., Marina Plaza Ballroom Aittola M.
    [Show full text]
  • A SEQUENCED LIST of LUNAR IMPACT FEATURES LARGER THAN 200 KM Charles J. Byrne, Image Again, [email protected]
    46th Lunar and Planetary Science Conference (2015) 1276.pdf A SEQUENCED LIST OF LUNAR IMPACT FEATURES LARGER THAN 200 KM Charles J. Byrne, Image Again, [email protected]. Introduction: Very few absolute ages are available for 4. Recently revised proposals for sequencing [Spudis, lunar features, but more features have been positioned in time et al. 2011, Fassett et al. 2012] sequence using such clues as stratigraphy or degradation. While additional sample collection and analysis would pro- Sequence Numbers of pre-Nectarian impact features: Ta- vide more evidence of absolute ages, that is for some time in ble 1 shows the list of impact features that have been deemed the future. We have a great deal of remote sensing data that to be older than the Nectaris Basin, along with their Se- can contribute to the assignment of the sequence of features. For some purposes, sequence can be used as a surrogate for quence Numbers [Byrne 2015]. age. In order to relate sequence to time, it is important to se- Table 1: Sequence of PreNectarian Impact Features quence nearly all of a class of features in order to emulate the continuity of time. Otherwise, the sequence may have large Feature Age Group Seq. No. gaps of uncertain duration. Therefore this sequenced list in- Near Side Megabasin pN.1 1 cludes the impact features that are greater than 200 km in rim Chaplygin-Mandel'shtam pN.1 2 crest diameter. A total of 71 impact features are in this list. South Pole-Aitken pN1 3 Features which may well be caused by impact but are too Marginis pN2 4 degraded for their apparent diameter and apparent depth to be Flamsteed-Billy pN2 5 measured are not included.
    [Show full text]
  • Image Map of the Moon
    U.S. Department of the Interior Prepared for the Scientific Investigations Map 3316 U.S. Geological Survey National Aeronautics and Space Administration Sheet 1 of 2 180° 0° 5555°° –55° Rowland 150°E MAP DESCRIPTION used for printing. However, some selected well-known features less that 85 km in diameter or 30°E 210°E length were included. For a complete list of the IAU-approved nomenclature for the Moon, see the This image mosaic is based on data from the Lunar Reconnaissance Orbiter Wide Angle 330°E 6060°° Gazetteer of Planetary Nomenclature at http://planetarynames.wr.usgs.gov. For lunar mission C l a v i u s –60°–60˚ Camera (WAC; Robinson and others, 2010), an instrument on the National Aeronautics and names, only successful landers are shown, not impactors or expended orbiters. Space Administration (NASA) Lunar Reconnaissance Orbiter (LRO) spacecraft (Tooley and others, 2010). The WAC is a seven band (321 nanometers [nm], 360 nm, 415 nm, 566 nm, 604 nm, 643 nm, and 689 nm) push frame imager with a 90° field of view in monochrome mode, and ACKNOWLEDGMENTS B i r k h o f f Emden 60° field of view in color mode. From the nominal 50-kilometer (km) polar orbit, the WAC This map was made possible with thanks to NASA, the LRO mission, and the Lunar Recon- Scheiner Avogadro acquires images with a 57-km swath-width and a typical length of 105 km. At nadir, the pixel naissance Orbiter Camera team. The map was funded by NASA's Planetary Geology and Geophys- scale for the visible filters (415–689 nm) is 75 meters (Speyerer and others, 2011).
    [Show full text]
  • Thedatabook.Pdf
    THE DATA BOOK OF ASTRONOMY Also available from Institute of Physics Publishing The Wandering Astronomer Patrick Moore The Photographic Atlas of the Stars H. J. P. Arnold, Paul Doherty and Patrick Moore THE DATA BOOK OF ASTRONOMY P ATRICK M OORE I NSTITUTE O F P HYSICS P UBLISHING B RISTOL A ND P HILADELPHIA c IOP Publishing Ltd 2000 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the publisher. Multiple copying is permitted in accordance with the terms of licences issued by the Copyright Licensing Agency under the terms of its agreement with the Committee of Vice-Chancellors and Principals. British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. ISBN 0 7503 0620 3 Library of Congress Cataloging-in-Publication Data are available Publisher: Nicki Dennis Production Editor: Simon Laurenson Production Control: Sarah Plenty Cover Design: Kevin Lowry Marketing Executive: Colin Fenton Published by Institute of Physics Publishing, wholly owned by The Institute of Physics, London Institute of Physics Publishing, Dirac House, Temple Back, Bristol BS1 6BE, UK US Office: Institute of Physics Publishing, The Public Ledger Building, Suite 1035, 150 South Independence Mall West, Philadelphia, PA 19106, USA Printed in the UK by Bookcraft, Midsomer Norton, Somerset CONTENTS FOREWORD vii 1 THE SOLAR SYSTEM 1
    [Show full text]