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  • 1
    Online Resource
    Online Resource
    Cambridge :Cambridge University Press,
    Keywords: Planets - Crust. ; Electronic books.
    Description / Table of Contents: This book explains how and why solid planets and satellites develop crusts. It presents a comprehensive survey and comparative analysis of crustal development on different planetary bodies, and is a key reference for researchers and students in geology, geochemistry, planetary science, astrobiology and astronomy.
    Type of Medium: Online Resource
    Pages: 1 online resource (402 pages)
    Edition: 1st ed.
    ISBN: 9780511463037
    Series Statement: Cambridge Planetary Science Series ; v.Series Number 10
    DDC: 551.1/3
    Language: English
    Note: Intro -- Half-title -- Title -- Copyright -- Dedication -- Contents -- Preface -- Notes and references -- Acknowledgments -- Abbreviations -- Prologue -- Notes and references -- 1 The planets: their formation and differentiation -- 1.1 Planetary formation -- 1.2 The solar nebula and the giant planets -- 1.2.1 The depletion of the volatile elements in the inner nebula -- 1.3 Planetesimals and the accretion of the terrestrial planets -- 1.4 The random nature of terrestrial planet formation -- 1.4.1 Meteorites and planetary composition -- 1.4.2 Uncompressed density and bulk planetary compositions -- 1.5 Types of crusts -- 1.6 Geochemical processes during crust formation -- 1.6.1 Europium as a universal tracer -- Synopsis -- Notes and references -- 2 A primary crust: the highland crust of the Moon -- 2.1 The composition of the Moon -- 2.2 The lunar surface -- 2.3 Structure of the crust -- 2.3.1 Tectonics -- 2.3.2 Lunar stratigraphy -- 2.4 Craters and multiring basins -- 2.4.1 A lunar cataclysm? -- 2.5 Composition of the lunar highland crust -- 2.5.1 Anorthosites -- 2.5.2 KREEP -- 2.5.3 The Mg-suite -- 2.5.4 Lunar highland terranes -- 2.5.5 The Cayley Plains: a cautionary tale -- 2.5.6 Tektites and the Moon -- Synopsis -- Notes and references -- 3 A secondary crust: the lunar maria -- 3.1 The maria -- 3.1.1 Mare basalt ages -- 3.2 Composition of the mare basalts -- 3.2.1 The interior of the Moon -- 3.3 Origin of the mare basalts -- 3.3.1 An impact origin? -- 3.4 The magma ocean -- 3.4.1 The depletion in europium -- 3.4.2 Depth of melting -- 3.5 Large-impact model for lunar origin -- Synopsis -- Notes and references -- 4 Mercury -- 4.1 The planet -- 4.1.1 The composition and internal structure of Mercury -- 4.2 Origin of Mercury -- 4.3 Surface structure -- 4.3.1 The heavily cratered terrain -- 4.3.2 The intercrater plains. , 4.3.3 The Caloris Basin: a mercurian cataclysm? -- 4.3.4 The smooth plains -- 4.4 The origin of the plains: a Cayley Plains analog? -- 4.4.1 Lobate scarps -- 4.5 The crust of Mercury -- 4.5.1 Primary and secondary crusts on Mercury? -- 4.5.2 Atmosphere -- Synopsis -- Notes and references -- 5 Mars: early differentiation and planetary composition -- 5.1 The origin of Mars -- 5.1.1 A volatile-rich and oxidized planet -- 5.2 The interior of Mars -- 5.2.1 Core -- 5.2.2 Mantle -- 5.2.3 Crust -- 5.3 Martian stratigraphy -- 5.4 Cratering record and the age of the martian surface -- 5.4.1 Crustal dichotomy -- 5.4.2 Quasi-circular depressions -- 5.4.3 Tharsis and Valles Marineris -- 5.5 Early plate tectonics? -- 5.5.1 Crustal magnetization and plate tectonics -- 5.6 Samples from Mars -- 5.6.1 Martian meteorites -- 5.6.2 Shergottite crystallization ages -- 5.7 Early differentiation on Mars and magma oceans -- 5.8 Multiple reservoirs and the age of the earliest crust -- 5.9 The composition of Mars -- 5.9.1 A cautionary note -- Synopsis -- Notes and references -- 6 Mars: crustal composition and evolution -- 6.1 Sampling martian crust -- 6.2 Crustal dimensions -- 6.2.1 Hypsometry -- 6.3 Igneous diversity in a basaltic crust -- 6.3.1 SNC meteorites and crustal contamination -- 6.3.2 Hemispheric dichotomy, Surface Types 1 and 2 and martian andesites -- 6.3.3 Gusev plains and Meridiani Planum -- 6.3.4 Alkaline volcanism and the Columbia Hills -- 6.4 The sedimentary rock cycle on Mars -- 6.4.1 Water, wind and ice -- 6.4.2 Surficial processes -- 6.4.3 Soils and dust -- 6.4.4 Sedimentary rocks on Mars -- 6.4.5 Meteoritic components -- 6.5 Bulk composition of the crust -- 6.5.1 Compositional evolution of the martian surface -- 6.6 Heat flow and crustal heat production -- 6.6.1 Compositional variation with depth -- 6.7 Crustal evolution on Mars. , 6.7.1 Tertiary crusts on Mars? -- Synopsis -- Notes and references -- 7 Venus: a twin planet to Earth? -- 7.1 The enigma of Venus -- 7.2 Surface features of Venus -- 7.2.1 Plains -- 7.2.2 Channels -- 7.2.3 Volcanoes -- 7.2.4 Coronae -- 7.2.5 Tesserae -- 7.2.6 Ishtar Terra and Aphrodite Terra -- 7.3 Impact craters and the age of the surface -- 7.4 Heat production and rates of volcanism -- 7.4.1 A one-plate planet -- 7.5 Crustal composition -- 7.5.1 Pancake domes: rhyolites on Venus? -- 7.5.2 The differentiation of Venus -- 7.6 The geological history of Venus -- 7.6.1 Water on Venus -- Synopsis -- Notes and references -- 8 The oceanic crust of the Earth -- 8.1 The sea floor and plate tectonics -- 8.2 Structure of the oceanic crust -- 8.3 Mid-ocean ridges -- 8.3.1 Formation processes at mid-ocean ridges -- 8.4 Mid-ocean ridge basalts (MORB) -- 8.4.1 Interaction with seawater -- 8.5 Oceanic island basalts (OIB) -- 8.6 Composition of the oceanic crust -- 8.7 Mantle structure -- 8.7.1 Mantle plumes -- 8.8 Composition of the Earth -- 8.8.1 Core -- 8.8.2 Mantle -- Synopsis -- Notes and references -- 9 The Hadean crust of the Earth -- 9.1 The Hadean crust and mantle -- 9.2 A terrestrial magma ocean -- 9.3 The early crust -- 9.3.1 The bombardment record -- 9.4 The early continental crustal myth -- 9.5 Isotopic constraints:… -- 9.5.1 Mantle keels in the Hadean? -- 9.6 A model for the Hadean -- Synopsis -- Notes and references -- 10 The Archean crust of the Earth -- 10.1 The Archean -- 10.1.1 The earliest Archean rocks -- 10.1.2 Akilia island, southwest Greenland -- 10.2 The Archean upper crust -- 10.2.1 Archean high-grade terrains -- 10.3 The Archean bulk crust -- 10.3.1 The Archean oceanic crust -- 10.3.2 Heat flow in the Archean -- 10.4 The formation of the TTG suite -- 10.4.1 Adakites and the TTG suite -- 10.4.2 The evidence from sanukitoids. , 10.5 Plate tectonics in the Archean? -- 10.5.1 The subcrustal lithosphere and mantle keels -- 10.6 Meteorite impacts in the Archean -- Synopsis -- Notes and references -- 11 The Post-Archean continental crust -- 11.1 The Archean Proterozoic transition -- 11.2 Changes in crustal composition during the Archean Proterozoic transition -- 11.3 The Post-Archean upper crust -- 11.3.1 Paradoxes: niobium and lead -- 11.4 The lower crust (Post-Archean) -- 11.4.1 Anorthosites -- Synopsis -- Appendices -- Area, thickness and density of the present continental crust -- Age of the continental crust -- Sedimentary rocks as crustal samples -- Notes and references -- 12 Composition and evolution of the continental crust -- 12.1 Heat flow constraints -- 12.2 Composition of the bulk crust -- 12.3 The andesite model -- 12.3.1 Delamination and its problems -- 12.3.2 The formation of andesites -- 12.3.3 Granites and granites -- 12.4 Alternatives: basaltic compositions -- 12.5 Alternatives: felsic compositions -- 12.6 Crustal growth and its episodic nature -- 12.6.1 The freeboard constraint -- 12.6.2 Recycling -- 12.6.3 Continental break-up and assembly -- Synopsis -- Notes and references -- 13 Crusts on minor bodies -- 13.1 Minor bodies in the Solar System -- 13.2 Observational problems -- 13.2.1 Nanophase iron -- 13.2.2 Eros and Itokawa -- 13.3 Vesta, a differentiated asteroid -- 13.3.1 Evolution of Vesta -- 13.3.2 Eucrites and the Moon -- 13.4 The Galilean satellites -- 13.5 The extraordinary crust of Io -- 13.5.1 Volcanic activity -- 13.5.2 Mountains -- 13.5.3 Nature of the crust -- 13.6 The thick icy crust of Europa -- 13.7 Two crusts on Ganymede -- 13.8 Callisto, an ancient crust -- 13.9 Sand dunes on Titan -- 13.10 Nitrogen ice on Triton -- Synopsis -- Notes and references -- 14 Reflections: the elusive patterns of planetary crusts -- 14.1 Too many variables. , 14.1.1 Sampling -- 14.2 Earth-like planets elsewhere? -- 14.3 Planetary evolution and plate tectonics -- Notes and references -- Author index -- Subject index.
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  • 2
    Keywords: Chemistry, Organic-Periodicals. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (333 pages)
    Edition: 1st ed.
    ISBN: 9783709187142
    Series Statement: Fortschritte der Chemie Organischer Naturstoffe Progress in the Chemistry of Organic Natural Products Series ; v.44
    Language: English
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  • 3
    Online Resource
    Online Resource
    San Diego :Elsevier Science & Technology,
    Keywords: Parallel processing (Electronic computers) -- Congresses. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (749 pages)
    Edition: 1st ed.
    ISBN: 9780080538440
    DDC: 532/.05/0285435
    Language: English
    Note: Front Cover -- Parallel Computational Fluid Dynamics: Implementations and Results Using Parallel Computers -- Copyright Page -- Preface -- Acknowledgements -- Table of Contents -- Part 1: Invited Speakers -- Chapter 1. Multiblock Structured Algorithms in Parallel CFD -- Chapter 2. Using Hundreds of Workstations for Production Running of Parallel CFD Applications -- Chapter 3. Parallel Computation of Frontal Processes -- Chapter 4. Modelling the Global Ocean Circulation on the T3D -- Chapter 5. Concurrent Distributed Visualization and Solution Steering -- Chapter 6. From R& -- D in Parallel CFD to a Tool for Computer Aided Engineering -- Chapter 7. Parallel Computation of Unsteady Supersonic Cavity Flows -- Part 2: Reacting Flows -- Chapter 8. A Data-Parallel LU Relaxation Method for Reacting Viscous Flows -- Chapter 9. Parallel Simulation on Rayleigh-Bénard Convection in 2D by the Direct Simulation Monte Carlo Method -- Chapter 10. Distributed Implementation of KIVA-3 on the Intel Paragon -- Chapter 11. A Parallel Tool for the Study of 3D Turbulent Combustion Phenomena -- Chapter 12. Numerical Simulation of Reacting Mixing Layer with Combined Parallel Approach -- Chapter 13. On the Optical Properties of a Supersonic Mixing Layer -- Chapter 14. Computation of Chemically Reacting Flow on Parallel Systems -- Chapter 15. Development of a Parallel Spectral Element Method Code Using SPMD Constructs -- Chapter 16. Parallel Computation of Turbulent Reactive Flows in Utility Boilers -- Part 3: Euler Solvers -- Chapter 17. A Comparison of Different Levels of Approximation in Implicit Parallel Solution Algorithms for the Euler Equations on Unstructured Grids -- Chapter 18. Analysis of Efficiency of Implicit CFD Methods on MIMD Computers. , Chapter 19. Parallel Solutions of Three-Dimensional Compressible Flows Using a Mixed Finite Element/Finite Volume Method on Unstructured Grids -- Chapter 20. Implementation of a Fractional Step Algorithm for the Solution of Euler Equations on Scalable Computers -- Chapter 21. Parallelization of a Highly Unstructured Euler-Solver Based on Arbitrary Polygonal Control Volumes -- Chapter 22. Performance of a Euler Solver Using a Distributed System -- Chapter 23. Implementation and Results of a Time Accurate Finite-Volume Euler Code in the NWT Parallel Computer -- Part 4: Algorithms -- Chapter 24. Development and Implementation of Parallel High Resolution Schemes in 3D Flows over Bluff Bodies -- Chapter 25. High Order Padé-type Approximation Methods for incompressible 3D CFD Problems on Massively Parallel Computers -- Chapter 26. Parallel Computations of CFD Problems Using a New Fast Poisson Solver -- Chapter 27. A Parallel Free Surface Flow Solver -- Chapter 28. A New Domain Decomposition Method Using Virtual Sub-domains -- Part 5: Spectral Methods -- Chapter 29. A Commercial CFD Application on a Shared Memory Multiprocessor using MPI -- Chapter 30. Parallel Computation with the Spectral Element Method -- Chapter 31. A Parallel Implementation of a Spectral Multi-domain Solver for Incompressible Navier-Stokes Equations -- Chapter 32. A Parallel Spectral Element Method for Compressible Hydrodynamics -- Part 6: Large Scale Applications -- Chapter 33. Large Scale Simulations of Flows about a Space Plane Using NWT -- Chapter 34. Large Scale Navier-Stokes Aerodynamic Simulations of Complete Fighter Aircraft on the Intel Paragon MPP -- Part 7: Performance Issues -- Chapter 35. Benchmarking the FLOWer Code on Different Parallel and Vector Machines -- Chapter 36. The Effect of the Grid Aspect Ratio on the Convergence of Parallel CFD Algorithms. , Chapter 37. Master-Slave Performance of Unstructured Flow Solvers on the CRAY-T3D -- Part 8: Flow Visualization -- Chapter 38. Runtime Volume Visualization for Parallel CFD -- Chapter 39. Integration of Particle Paths and Streamlines in a Spatially-Decomposed Computation -- Chapter 40. Interactive Volume Rendering on Clusters of Shared-Memory Multiprocessors -- Part 9: Multigrid Methods -- Chapter 41. Application of Parallel Multigrid Methods to Unsteady Flow: A Performance Evaluation -- Chapter 42. Multigrid Aircraft Computations Using the OPlus Parallel Library -- Chapter 43. A Parallel Multigrid Method for the Prediction of Turbulent Flows with Reynolds Stress Closure -- Part 10: Applications -- Chapter 44. Cell-Vertex Multigrid Solvers in the PARAGRID Framework -- Chapter 45. Fluid Flow in an Axisymmetric, Sudden-Expansion Geometry -- Chapter 46. Implicit Navier-Stokes Codes in Parallel for Aerospace Applications -- Chapter 47. FIESTA-HD: A Parallel Finite Element Program for Hydrodynamic Device Simulation -- Chapter 48. Parallel Computation of a Tip Vortex Induced by a Large Aircraft: Wing -- Chapter 49. Shape Design Optimization in 2D Aerodynamics Using Genetic Algorithms on Parallel Computers -- Chapter 50. A Model for Performance of a Block-structured Navier-Stokes Solver on a Cluster of Workstations -- Chapter 51. Further Acceleration of an Unsteady Navier-Stokes Solver for Cascade Flows on the NWT -- Chapter 52. Load Balancing Strategy for Parallel Vortex Methods with Distributed Adaptive Data Structure -- Chapter 53. Portable Parallelization of the Navier-Stokes Code NSFLEX -- Chapter 54. Towards an Integrated CFD System in a Parallel Environment -- Chapter 55. Parallel Multi-block Computation of Incompressible Flows for Industrial Applications -- Part 11: Turbulence -- Chapter 56. Parallel Benchmarks of Turbulence in Complex Geometries. , Chapter 57. Parallel Computation of 3-D Small-Scale Turbulence Via Additive Turbulent Decomposition -- Chapter 58. A Message-Passing, Distributed Memory Parallel Algorithm for Direct Numerical Simulation of Turbulence with Particle Tracking -- Chapter 59. Simulation of Stratified Turbulent Channel Flows on the Intel Paragon Parallel Supercomputer -- Part 12: Adaptive Schemes -- Chapter 60. Parallel Implementation of an Adaptive Scheme for 3D Unstructured Grids on a Shared-Memory Multiprocessor -- Chapter 61. A Parallel Adaptive Navier-Stokes Method and Partitioner for Hybrid Prismatic/etrahedral Grids -- Chapter 62. Parallel Adaptive hp Finite Element Approximations for Stokesian Flows: Adaptive Strategies, Load Balancing and Domain Decomposition Solvers -- Chapter 63. Parallel Processing for Solution-Adaptive Computation of Fluid Flow -- Chapter 64. Distributed CFD on Cluster of Workstations Involving Parallel Unstructured Mesh Adaptation, Finite-Volume-Galerkin Approach and Finite-Elements -- Part 13: Climate Modeling -- Chapter 65. Semi-Lagrangian Shallow Water Modeling on the CM-5 -- Chapter 66. A Reduced Grid Model for Shallow Water Flows on the Sphere -- Chapter 67. Application of a Parallel Navier-Stokes Model to Ocean Circulation -- Chapter 68. A Portable and Efficient Parallel Code for Astrophysical Fluid Dynamics -- Part 14: Navier-Stokes Solvers -- Chapter 69. Towards Modular CFD Using the CERFACS Parallel Utilities -- Chapter 70. A Fully Implicit Parallel Solver for Viscous flows -- Numerical Tests on High Performance Machines -- Chapter 71. Space- and Time-Parallel Navier-Stokes Solver for 3D Block-Adaptive Cartesian Grids -- Chapter 72. A Newton-GMRES Method for the Parallel Navier-Stokes Equations -- Chapter 73. A Parallell, Globally-Implicit Navier-Stokes Solver for Design. , Chapter 74. Parallel Solution of Viscous Incompressible Flow on Multi- Block Structured Grids Using MPI -- Chapter 75. Comparing the Performance of Multigrid and Conjugate Gradient Algorithms on the CRAY T3D -- Chapter 76. Domain Decomposition/Fictitious Domain Methods with Nonmatching Grids for Navier-Stokes Equations Parallel Implementation on a KSR1 Machine -- Chapter 77. A Parallel Implicit Time Accurate Navier-Stokes Solver -- Chapter 78. Parallel Implementation of Newton's Method for 3-D Navier- Stokes Equations -- Part 15: Distributing Computing -- Chapter 79. Dynamic Load Balancing in a 2D Parallel Delaunay Mesh Generator -- Chapter 80. Parallel Visualisation of Unstructured Grids -- Chapter 81. A Dynamic Load Balancing Technique for Solving Transonic and Supersonic Flows on Networked Workstations -- Part 16: Mesh Partitioning -- Chapter 82. Scalable Parallel Generation of Partitioned, Unstructured Meshes -- Chapter 83. Evaluation of the JOSTLE Mesh Partitioning Code for Practical Multiphysics Applications -- Part 17: Internal Flows -- Chapter 84. Parallel Computation of Unsteady Supersonic-Inlet Flows -- Chapter 85. Parallel, Axisymmetric, Aerodynamic Simulation of a Jet Engine -- Chapter 86. An Investigation of Load Balancing Strategies for CFD Applications on Parallel Computers -- Part 18: Software Tools -- Chapter 87. CPULib - A Software Library for Parallel Applications on Arbitrary Meshes -- Chapter 88. Host-node Client-Server Software Architecture for Computational Fluid Dynamics on MPP Computers -- Chapter 89. Software Tools for Parallel CFD on Composite Grids.
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  • 4
    Keywords: Lunar petrology. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (245 pages)
    Edition: 1st ed.
    ISBN: 9781483186863
    Language: English
    Note: Front Cover -- Moon Rocks and Minerals -- Copyright Page -- Table of Contents -- Dedication -- PREFACE -- ACKNOWLEDGMENTS -- CHAPTER 1. INTRODUCTION -- CHAPTER 2. THE ROCKS AND SOILS -- THE CRYSTALLINE ROCKS (TYPE A AND B) -- BRECCIAS (TYPE C) -- FINES (TYPE D) -- ALSO CALLED SOILS -- ANORTHOSITES IN THE SOILS -- SHOCK (IMPACT) METAMORPHISM -- REGOLITH AND SOIL MECHANICS -- LUNAR GLASSES -- TEKTITES -- CHAPTER 3. THE MINERALS -- AUGITE-PIGEONITE (THE PYROXENES) -- PYROXFERROITE -- PLAGIOCLASE (AND POTASSIUM FELDSPAR) -- ILMENITE -- OLIVINE -- CHROMITE-ULVOSPINEL-SPINEL -- ARMALCOLITE -- TROILITE -- IRON -- RUTILE -- CRISTOBALITE, TRIDYMITE AND QUARTZ -- APATITE -- WHITLOCKITE -- COPPER (INCLUDING BRASS) -- TIN -- ZIRCON -- BADDELEYITE -- MICA -- AMPHIBOLE -- ARAGONITE -- PENTLANDITE -- IRON-NICKEL -- COHENITE -- SCHREIBERSITE -- UNIDENTIFIED MINERALS -- CHAPTER 4. CHEMISTRY OF SAMPLES BROUGHT BY APOLLO 11 AND 12 -- INTRODUCTION -- CHEMICAL ABUNDANCE DATA -- PRIMITIVE, PRIMORDIAL OR COSMIC ABUNDANCES -- MAJOR AND MINOR ELEMENTS -- CHEMICAL CLASSIFICATION OF ROCKS -- BRECCIAS (TYPE C) -- FINE MATERIAL (SOIL) (TYPE D) -- COMPARISON OF MAJOR ELEMENT ABUNDANCES WITH TERRESTRIAL ROCKS AND METEORITES -- TRACE ELEMENT ABUNDANCES -- GEOCHEMICAL CLASSIFICATION OF THE ELEMENTS -- ARRANGEMENT OF DATA -- THE LARGE CATIONS (SEE TABLE 4-4.) -- THE RARE EARTHS (RE) (SEE TABLE 4-5.) -- EUROPIUM DEPLETION -- YTTRIUM -- THE LARGE HIGHLY CHARGED CATIONS (SEE TABLE 4-6.) -- THE FERROMAGNESIAN ELEMENTS (SEE TABLE 4-7.) -- CHALCOPHILE ELEMENTS (SEE TABLE 4-9.) -- THE PLATINUM GROUP ELEMENTS (SEE TABLE 4-10.) -- OXYGEN -- CARBON -- HALOGENS -- COMPARISON OF CHEMICAL COMPOSITION OF APOLLO Ð (TRANQUILLITY BASE) AND APOLLO 12 (OCEAN OF STORMS) SAMPLES -- APOLLO 12 ROCKS AND FINE MATERIAL -- INTERNAL VARIATIONS IN THE APOLLO 12 ROCKS. , RELATION OF TERRESTRIAL ROCKS AND METEORITES TO APOLLO 12 ROCKS -- CHAPTER 5. BIOSCIENCE AND ORGANIC MATTER -- TOTAL CARBON -- ORGANIC CARBON -- CARBIDES -- METHANE -- OXIDES OF CARBON -- ALKANE HYDROCARBONS -- AROMATIC HYDROCARBONS -- AMINO ACIDS -- PORPHYRINS -- BIOLIPIDS IN GENERAL -- ORGANIC SULFUR COMPOUNDS -- CARBONACEOUS MATERIAL -- ISOTOPE ABUNDANCES FOR CARBON AND SULFUR -- ORGANISMS -- SUMMARY -- CHAPTER 6. PETROLOGY: Experimental Studies and Origin of the Lavas -- INTRODUCTION -- EFFECTS OF HIGH PRESSURE ON LUNAR BASALTS -- MELTING BEHAVIOR OF APOLLO 11 BASALTS -- MELTING BEHAVIOR AT HIGHER PRESSURES -- SILICATE LIQUID IMMISCIBILITY -- RESIDUUM -- MESOSTASIS -- PETROGENESIS - ORIGIN OF THE LAVAS -- SOURCE OF THE LAVAS -- PARTIAL MELTING -- IMPACT MELTING -- SUBSEQUENT HISTORY OF THE MELT -- CHAPTER 7. AGE OF THE LUNAR ROCKS, ISOTOPE STUDIES, COSMIC RAY and SOLAR WIND EFFECTS -- POTASSIUM(K)-ARGON(AR) DATING -- AR 40-AR39 AGES -- RUBIDIUM(Rb)-STRONTIUM(Sr) AGES -- Rb-Sr AGES OF FINE MATERIAL -- URANIUM(U)-THORIUM(Th)-LEAD(Pb) AGES -- LEAD ROCK AGES -- LEAD DATA FOR THE FINE MATERIAL -- FURTHER SIGNIFICANCE OF LEAD ISOTOPE DATA -- SIGNIFICANCE OF ROCK AGES FOR SOURCE OF MARIA BASIN MATERIAL -- ISOTOPIC ABUNDANCES -- ISOTOPIC HOMOGENEITY IN THE SOLAR NEBULA -- LIGHT ISOTOPE FRACTIONATION -- OXYGEN ISOTOPES -- CRYSTALLIZATION TEMPERATURE -- TEKTITES -- SULFUR ISOTOPES -- CARBON ISOTOPES -- HYDROGEN -- COSMIC-RAY BOMBARDMENT OF THE LUNAR SURFACE -- RADIOGENIC NUCLIDES (EXCEPT RARE GASES) -- NUCLEAR PARTICLE TRACK STUDIES -- TRACK DENSITY vs. DEPTH -- RATES OF EROSION FROM NUCLEAR TRACK DENSITIES -- SURFACE RESIDENCE TIMES -- RARE GASES -- COSMIC RAY EXPOSURE AGES -- THE ARGON ANOMALY -- CHAPTER 8. PHYSICAL PROPERTIES -- INTRODUCTION -- THE LUNAR INTERIOR - SEISMIC EVIDENCE -- LUNAR HEAT FLOW -- DENSITY OF LUNAR ROCKS -- LUNAR LAVA VISCOSITY. , MASCONS -- CHAPTER 9. ORIGIN OF THE MOON -- INTRODUCTION -- FISSION HYPOTHESES -- CAPTURE HYPOTHESES -- DOUBLE PLANET HYPOTHESES -- GLOSSARY -- CONVERSION FACTORS -- CHEMICAL SYMBOLS AND ELEMENTS -- SUBJECT INDEX.
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  • 5
    Publication Date: 2019-07-17
    Repository Name: EPIC Alfred Wegener Institut
    Type: Conference , notRev
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  • 6
    Publication Date: 2024-05-29
    Description: This draft White Paper has been prepared as part of the Vision 2030 process being undertaken in the framework of the UN Decade of Ocean Science for Sustainable Development. The Vision 2030 process aims to achieve a common and tangible measure of success for each of the ten Ocean Decade Challenges by 2030. From a starting point of existing initiatives underway in the Ocean Decade and beyond, and through a lens of priority user needs, the process determines priority datasets, critical gaps in science and knowledge, and needs in capacity development, infrastructure and technology required for each Challenge to ensure that it can be fulfilled by the end of the Ocean Decade in 2030. The results of the process will contribute to the scoping of future Decade Actions, identification of resource mobilization priorities, and ensuring the ongoing relevance of the Challenges over time. The process identifies achievable recommendations that can be implemented in the context of the Decade, or more broadly before 2030 to achieve the identified strategic ambition and indicators that will be used to measure progress. This draft White Paper is one of a series of ten White Papers all of which have been authored by an expert Working Group. Accompanied by a synthesis report authored by the Decade Coordination Unit, this white paper was discussed at the 2024 Ocean Decade Conference (Barcelona. Spain). Input received from diverse groups through public consultation and at the Conference was reviewed and incorporated as relevant.
    Description: Published
    Description: Refereed
    Keywords: Forward look ; Vision paper ; Marine biodiversity ; Ecosystem restoration ; Marine ecosystems ; Climate change effects
    Repository Name: AquaDocs
    Type: Report
    Format: 28pp.
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  • 7
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 79 (1996), S. 1173-1175 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The deposition of antimony (Sb) clusters onto silicon substrates and on a carbon film is reported. The experimental apparatus allows evaporation of molten Sb from a heated crucible through a small nozzle orifice into a vacuum. TEM micrographs show Sb clusters with sizes between 1.2×104 and 1.3×105 atoms. This is over 1–2 orders of magnitude larger than previously reported. Film growth kinetics were studied during longer evaporation tests on Si substrates. A theory explaining the Sb loss from the crucible is presented which agrees well with experimental data. The results support cluster formation by heterogeneous nucleation on the nozzle orifice walls followed by subsequent entrainment into the vapor stream. © 1996 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    BJOG 94 (1987), S. 0 
    ISSN: 1471-0528
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Medicine
    Notes: Semen specimens from 519 men were cultured for organisms 2 weeks before oocyte recovery for in-vitro fertilization (IVF). The cultures from 72 men contained more than 5000 bacteria/ml and the IVF attempt was postponed. The IVF outcome was assessed in 382 couples in relation to the semen culture result. The pregnancy rate per cycle was significantly reduced when the semen culture contained organisms compared with axenic semen (P〈0-05). This was independent of the cleavage rate of oocytes and the number of embryos transferred. Although mycoplasma was frequently cultured, chlamydial infection was very rare and no viruses were isolated in this study.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Psychophysiology 8 (1971), S. 0 
    ISSN: 1469-8986
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Medicine , Psychology
    Notes: Studies of delayed GSR conditioning have shown that when an interstimulus interval (ISI) of sufficient duration is employed, multiple responses may occur within that interval. The studies reviewed in this article indicate that GSRs which occur early in the interval are present by the second conditioning trial. They tend to habituate, appear to be orienting responses, and, under certain circumstances, they are conditional. Those responses which occur during the later portion of the interval are minimal, if at all present, when conditioning is initiated but show a negatively accelerated growth curve across trials. These second responses are conditional and may be protective reflexes which prevent damage to the skin. It is concluded that in GSR conditioning the choice of an ISI and the specification of ISI responses may seriously affect the nature of the behavior observed, and may have serious implications for other areas of psychological investigation.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Journal of natural products 44 (1981), S. 729-731 
    ISSN: 1520-6025
    Source: ACS Legacy Archives
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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