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  • 1
    Online Resource
    Online Resource
    San Diego :Elsevier Science & Technology,
    Keywords: Planets -- Atmospheres. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (427 pages)
    Edition: 1st ed.
    ISBN: 9780080530567
    Series Statement: Issn Series ; v.Volume 15
    Language: English
    Note: Front Cover -- Dust in the Solar System and Other Planetary Systems -- Copyright Page -- Contents -- Part I: Meteors and Meteoroid Streams -- Chapter 1. Meteoroid streams and meteor showers -- Chapter 2. Thermal gradients in micrometeoroids during atmospheric entry -- Chapter 3. Direct determination of the micrometeoric mass flux into the upper atmosphere -- Chapter 4. The size of meteoroid constituent grains: Implications for interstellar meteoroids -- Chapter 5. Radar meteoroids: advances and opportunities -- Chapter 6. Dynamical and orbital properties of the Arecibo micrometeors -- Chapter 7. Update on new developments of the advanced meteor orbit radar AMOR -- Chapter 8. Wavelet enhancement for detecting shower structure in radar meteoroid data: I. Methodology -- Chapter 9. Wavelet enhancement for detecting shower structure in radar meteoroid data: II Application to the AMOR data -- Chapter 10. Predictability in meteoroid stream evolution -- Chapter 11. A dust swarm detected after the main Leonid meteor shower in 1998 -- Chapter 12. Meteor Showers associated with Near-Earth Asteroids in the Taurid Complex -- Chapter 13. Dust Trails along asteroid 3200 Phaethon's orbit -- Part II: Observations of the Zodiacal Light -- Chapter 14. CCD imaging of the zodiacal light -- Chapter 15. WIZARD: New observation system of zodiacal light in Kobe University -- Chapter 16. Brightness distribution of Zodiacal light observed by a cooled CCD camera at Mauna Kea -- Chapter 17. High spatial resolution distribution of the zodiacal light brightness -- Chapter 18. Zodiacal light observations with the Infrared Space Observatory -- Part III: Interplanetary Dust -- Chapter 19. Light scattering and the nature of interplanetary dust -- Chapter 20. The size-frequency distribution of zodiacal dust band material. , Chapter 21. A dissipative mapping technique for integrating interplanetary dust particle orbits -- Chapter 22. Dust en-route to Jupiter and the Galilean satellites -- Chapter 23. CDA cruise science: Comparison of measured dust flux at 1 AU with models -- Chapter 24. Halo orbits around Saturn -- Chapter 25. Charging processes for dust particles in Saturn's magnetosphere -- Chapter 26. Mars Dust Counter (MDC) on board NOZOMI: Initial results -- Chapter 27. Dust telescopes: A new tool for dust research -- Chapter 28. Planetary aerosol monitor/Interplanetary dust analyser -- Part IV: Dust in the Outer Solar System and Other Planetary Systems -- Chapter 29. Dust in young solar systems -- Chapter 30. Aperture synthesis observations of protoplanetary disks with the Nobeyama millimeter array -- Chapter 31. DRVS and extrasolar planetary dust noise reduction -- Chapter 32. Structure of the Edgeworth-Kuiper Belt (EKB) dust disk and implications for extrasolar planet(s) in E Eridani -- Chapter 33. Dust production in the Kuiper Belt and in Vega-like systems -- Chapter 34. Migration of matter from the Edgeworth Kuiper and main asteroid belts to the Earth -- Part V: Cometary Dust -- Chapter 35. Comet dust: The view after Hale-Bopp -- Chapter 36. Infrared spectroscopy of comets with ISO: What we learned on the composition of cometary dust -- Chapter 37. A search for trends in cometary dust emission -- Chapter 38. Evolution of cometary grains from studies of comet images -- Chapter 39. High porosity for cometary dust: evidence from PROGRA2 experiment -- Patr VI: Laboratory Studies -- Chapter 40. The nature of cosmic dust: laboratory data and space observations -- Chapter 41. A new dust source for the Heidelberg dust accelerator -- Chapter 42. Development of low density dusts for impact ionization experiments. , Chapter 43. Application of new, low density projectiles to the laboratory calibration of the Cassini Cosmic Dust Analyser (CDA) -- Chapter 44. Analysis of micro-craters on metal targets formed by hyper velocity impacts -- Chapter 45. Grain-target collision experiments and astrophysical implications -- Chapter 46. Space weathering: spectral change and formation of nanophase iron due to pulse laser irradiation simulating impact heating of interplanetary dust flux -- Chapter 47. Light scattering by flakes -- Chapter 48. Aggregation experiments with magnetised dust grains. -- Chapter 49. Crystallization processes in amorphous MgSi03 -- Chapter 50. Experimental astromineralogy : Circumstellar ferromagnesiosilica dust in analogs and natural samples -- Part VII: The Near-Earth Environment -- Chapter 51. Dust characterisation in the near Earth environment -- Chapter 52. A new approach to applying interplanetary meteoroid flux models to spacecraft in gravitational fields -- Chapter 53. The new NASA orbital debris breakup model -- Chapter 54. A CCD Search for the Earth-Moon Libration Clouds and L4 -- Chapter 55. The chemistry and origin of micrometeoroid and space debris impacts on spacecraft surfaces -- Part VIII: Evidence from Meteorites -- Chapter 56. The nature and significance of meteoritic matter -- Chapter 57. Antarctic micrometeorites collected by the Japanese Antarctic Research Expedition teams during 1996-1 999 -- Chapter 58. The possibility of abiogenic synthesis of complex biochemical compounds on surfaces of dust particles -- Chapter 59. Microanalysis of cosmic dust - prospects and challenges -- Index -- Author Index -- Keyword Index.
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  • 2
    Keywords: Extrasolar planets. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (271 pages)
    Edition: 1st ed.
    ISBN: 9783540448075
    Series Statement: Lecture Notes in Physics Series ; v.577
    Language: English
    Note: Lecture Notes in Physics -- Solar and Extra-Solar Planetary Systems -- Copyright -- Preface -- Table of Contents -- List of Contributors -- Plates -- Introduction - Solar and Extra-Solar Planetary Systems -- The Solar System: An Overview -- Setting the Scene: A Star Formation Perspective -- Extrasolar Planets: A Review of Current Observations and Theory -- The Giant Planets -- The Formation of Planets -- Dynamics of the Solar System -- Photometry of Resolved Planetary Surfaces -- Mercury - Goals for a Future Mission -- Physical Processes Associated with Planetary Satellites -- Light Scattering in the Martian Atmosphere: Effects on Surface Photometry -- The Small Bodies of the Solar System -- Dust in the Solar System and in Other Planetary Systems -- Meteors, Meteor Showers and Meteoroid Streams.
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 317 (1985), S. 559-560 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SCH„RER and All¨gre1, using isotope dilution analysis of single grains and fragments of zircon, recently failed to substantiate a report by Froude et al.2, based on the ion microprobe SHRIMP3, of zircons older than 4,100 Myr from Mt Narryer, Western Australia. In their discussion, Sch¤rer and ...
    Type of Medium: Electronic Resource
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  • 4
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Fig. 1 Simplified geological map of the Mt Narryer region showing:o·, Location of dated gneisses with Sm-Nd model ages1 in Myr. +, Location of quartzite samples (+A, GSWA sample site 71932; +B, GSWA sample sites 71921 and 71924). The quartzites in which the zircons occur are part of a thick ...
    Type of Medium: Electronic Resource
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  • 5
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    Unknown
    IUCN | Gland, Switzerland
    In:  http://aquaticcommons.org/id/eprint/15795 | 9 | 2014-12-05 21:25:09 | 15795 | Central Caribbean Marine Institute
    Publication Date: 2021-07-10
    Keywords: Conservation ; Ecology ; Environment ; Fisheries
    Repository Name: AquaDocs
    Type: book_section
    Format: application/pdf
    Format: application/pdf
    Format: 191-195
    Format: 304
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  • 6
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: The structure of FO2 has been calculated for the X 2A‘ ground state using Møller–Plesset (MP) perturbation, complete-active-space self-consistent-field (CASSCF), and quadratic configuration interaction (QCI) ab initio molecular orbital methods. Basis sets with polarization and diffuse functions were used. Compared with the experimental structure, bond lengths obtained with MP perturbation methods are found to be consistently too short. CASSCF calculations yield a structure which varies considerably with the size of the active space and basis set used. Calculations using the single-configuration-based QCI in the single and double-space with perturbative inclusion of triple substitutions, denoted by QCISD (T), yield structures very close to the experimental structure of FO2. The thermochemistry of FO2 radical has been calculated using the MP, QCI, and gaussian-1 (G1) methods. The QCI method using isodesmic and isogyric schemes has predicted the heat of formation for FO2 at 0 K to be 8.9±3 kcal mol−1.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 89 (1988), S. 3044-3049 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: Dissociation energies and barriers to dissociation for XCO→X+CO have been calculated for X˜ 2A' and A˜ 2π states of FCO and HCO by ab initio molecular orbital methods. At the PUMP4//UMP2/6-311G* level, D(open circle)298 (F-CO)=22.3 kcal mol−1 and ΔH298=24.2 kcal mol−1 for dissociation of ground-state FCO; these values are much higher than the corresponding bond energy and activation enthalpy for HCO dissociation. Calculated RRKM rate constants suggests that the lifetime of FCO under stratospheric conditions is sufficient to allow bimolecular reactions to compete with dissociation. Reaction with O2 may provide an in situ source of stratospheric CO2.
    Type of Medium: Electronic Resource
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  • 8
    ISSN: 1089-7623
    Source: AIP Digital Archive
    Topics: Physics , Electrical Engineering, Measurement and Control Technology
    Notes: An electron-beam ion trap (EBIT) has just been completed in the Clarendon Laboratory, Oxford. The design is similar to the devices installed at the Lawrence Livermore National Laboratory. It is intended that the Oxford EBIT will be used for x-ray and UV spectroscopy of hydrogenic and helium-like ions, laser resonance spectroscopy of hydrogenic ions and measurements of dielectronic recombination cross sections, in order to test current understanding of simple highly charged ions.
    Type of Medium: Electronic Resource
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  • 9
    ISSN: 1525-1314
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: SHRIMP U–Pb dating and laser ablation ICP-MS trace element analyses of zircon from four eclogite samples from the north-western Dabie Mountains, central China, provide evidence for two eclogite facies metamorphic events. Three samples from the Huwan shear zone yield indistinguishable late Carboniferous metamorphic ages of 312 ± 5, 307 ± 4 and 311 ± 17 Ma, with a mean age of 309 ± 3 Ma. One sample from the Hong'an Group, 1 km south of the shear zone yields a late Triassic age of 232 ± 10 Ma, similar to the age of ultra-high pressure (UHP) metamorphism in the east Qinling–Dabie orogenic belt. REE and other trace element compositions of the zircon from two of the Huwan samples indicate metamorphic zircon growth in the presence of garnet but not plagioclase, namely in the eclogite facies, an interpretation supported by the presence of garnet, omphacite and phengite inclusions. Zircon also grew during later retrogression. Zircon cores from the Huwan shear zone have Ordovician to Devonian (440–350 Ma) ages, flat to steep heavy-REE patterns, negative Eu anomalies, and in some cases plagioclase inclusions, indicative of derivation from North China Block igneous and low pressure metamorphic source rocks. Cores from Hong'an Group zircon are Neoproterozoic (780–610 Ma), consistent with derivation from the South China Block. In the western Dabie Mountains, the first stage of the collision between the North and South China Blocks took place in the Carboniferous along a suture north of the Huwan shear zone. The major Triassic continent–continent collision occurred along a suture at the southern boundary of the shear zone. The first collision produced local eclogite facies metamorphism in the Huwan shear zone. The second produced widespread eclogite facies metamorphism throughout the Dabie Mountains–Sulu terrane and a lower grade overprint in the shear zone.
    Type of Medium: Electronic Resource
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  • 10
    ISSN: 1525-1314
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: We report SHRIMP U–Th–Pb monazite, conventional U–Pb titanite, Sm–Nd garnet and Rb–Sr muscovite and biotite ages for metamorphic rocks from the Danba Domal Metamorphic Terrane in the eastern Songpan-Garzê Orogenic Belt (eastern Tibet Plateau). These ages are used to determine the timing of polyphase metamorphic events and the subsequent cooling history. The oldest U–Th–Pb monazite and Sm–Nd garnet ages constrain an early Barrovian metamorphism (M1) in the interval c. 204–190 Ma, coincident with extensive Indosinian granitic magmatism throughout the Songpan-Garzê Orogenic Belt. A second, higher-grade sillimanite-grade metamorphic event (M2), recorded only in the northern part of the Danba terrane, was dated at c. 168–158 Ma by a combination of U–Th–Pb monazite and titanite and Sm–Nd garnet ages. It is suggested that M1 was a thermal event that affected the entire orogenic belt while M2 may represent a local thermal perturbation. Rb–Sr muscovite ages range from c. 138–100 Ma, whereas Rb–Sr biotite ages cluster at c. 34–24 Ma. These ages document regional cooling at rates of c. 2–3 °C Myr−1 following the M1 peak for most of the terrane. However, those parts of the terrane affected by the higher-temperature M2 event (e.g. the migmatite zone) experienced initially more rapid (c. 8 °C Myr−1) cooling after peak M2 before joining the regional slow cooling path defined by the rest of the terrane at c. 138 Ma. Regional slow cooling between c. 138 and c. 30 Ma is thought to be the result of post-tectonic isostatic uplift after extensive crustal thickening caused by collision of the South and North China Blocks. The clustering of biotite Rb–Sr ages marks the onset of rapid uplift across the entire terrane commencing at c. 30–20 Ma. This cooling history is shared with many other regions of the Tibet Plateau, suggesting that uplift of the Tibet Plateau (including the Songpan-Garzê Orogenic Belt) occurred predominantly in the last c. 30 Myr as a response to the continuing northwards collision of India with Eurasia.
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