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  • 1
    Online Resource
    Online Resource
    San Diego :Elsevier Science & Technology,
    Keywords: Neutrino astrophysics. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (564 pages)
    Edition: 1st ed.
    ISBN: 9780080548760
    Language: English
    Note: Front Cover -- Neutrino Physics and Astrophysics -- Copyright Page -- Contents -- Foreword -- International Neutrino Committee -- Neutrino 98 International Advisory Committee/Organizing Committee -- Part 1: Opening Lecture -- Chapter 1. Neutrinos: a glimpse beyond the Standard Model -- Part 2: Solar Neutrinos -- Chapter 2. The Homestake solar neutrino program -- Chapter 3. Solar neutrino results from SAGE -- Chapter 4. GALLEX solar neutrino results and status of GNO -- Chapter 5. Solar neutrino results from Super-Kamiokande -- Chapter 6. The Sudbury Neutrino Observatory project -- Chapter 7. Status of the BOREXINO solar neutrino experiment -- Chapter 8. Future solar neutrino projects -- Chapter 9. Standard solar models -- Chapter 10. Uncertainties in the solar neutrino flux -- Chapter 11. Helioseismology and solar neutrinos -- Chapter 12. Neutrino magnetic moment and solar neutrino experiments -- Chapter 13. New enhancement mechanism of the transitions in the Earth of the solar and atmospheric neutrinos crossing the Earth core -- Chapter 14. Towards the solution of the solar neutrino problem -- Part 3: Atmospheric Neutrinos -- Chapter 15. Atmospheric neutrino studies in Soudan 2 -- Chapter 16. Atmospheric neutrino induced muons in the MACRO detector -- Chapter 17. Atmospheric neutrino results from Super-Kamiokande and Kamiokande - Evidence for vμ , oscillations - -- Chapter 18. Fluxes of atmospheric neutrinos and related cosmic rays -- Chapter 19. Uncertainty of the atmospheric neutrino fluxes -- Chapter 20. vμ ↔v r vs vμ↔vs solutions for the atmospheric neutrino problem -- Chapter 21. On the neutrino mass spectrum and neutrino mixing from oscillation data -- Part 4: Long Baseline Experiments -- Chapter 22. Results from CHOOZ -- Chapter 23. The Palo Verde reactor neutrino oscillation experiment -- Chapter 24. Present Status of KamLAND. , Chapter 25. A pilot experiment with reactor neutrinos in Taiwan -- Chapter 26. Long baseline neutrino oscillation program in the United States -- Chapter 27. Physics projects for a future CERN-LNGS neutrino programme -- Chapter 28. Status of K2K (KEK to Kamioka long baseline neutrino oscillation experiment) -- Part 5: Short Baseline Oscillation Experiments -- Chapter 29. Neutrino oscillation results from LSND -- Chapter 30. The search for neutrino oscillations vμ-> -- ve with KARMEN -- Chapter 31. CHORUS results -- Chapter 32. A search for vμ↔ vr Oscillations Using the NOMAD Detector -- Chapter 33. Future short baseline neutrino oscillation experiments -- Part 6: Implications of the Solar and Atmospheric Neutrino Data -- Chapter 34. Implications of solar and atmospheric neutrinos -- Part 7: Accelerator and Reactor Neutrino Experiments -- Chapter 35. Result from DONUT- Direct observation of vt interaction- -- Chapter 36. Determination of sin2 θw from neutrino-nucleon scattering at NuTeV -- Chapter 37. Events with isolated charged leptons and missing momentum observed at the e+p collider HERA -- Chapter 38. Neutrino physics with a muon collider -- Chapter 39. Status of the MUNU experiment -- Part 8: Neutrino and Particle Physics -- Chapter 40. Large lepton mixing in seesaw models- Coset-space family unification -- Chapter 41. Implications of the SuperKamiokande result on the nature of new physics -- Chapter 42. Implications of a minimal SO(10) Higgs structure -- Chapter 43. Cosmic ray and neutrino tests of special relativity -- Part 9: Direct Search for Neutrino Mass -- Chapter 44. New results from the Mainz neutrino mass experiment -- Chapter 45. Neutrino mass and anomaly in the tritium beta-spectrum. Results of the "Troitsk v-mass" experiment -- Part 10: Double Beta Decay. , Chapter 46. Review on double beta decay experiments and comparison with theory -- Chapter 47. Double beta decays and neutrino nuclear responses -- Chapter 48. Results from the NEMO experiment -- Chapter 49. Double beta decay with Ge-detectors - and the future of double beta and dark matter search (GENIUS) -- Chapter 50. Present and future of low temperature detectors -- Chapter 51. Particle physics implications of neutrinoless double beta decay -- Part 11: Dark Matter Search -- Chapter 52. Direct searches for dark matter -- Chapter 53. Indirect searches for dark matter -- Chapter 54. Baryonic dark matter -- Chapter 55. Theoretical overview: emphasis on neutrinos -- Part 12: Neutrino in Cosmology and Astrophysics -- Chapter 56. Supernova neutrinos: review -- Chapter 57. Future supernova neutrino detection -- Chapter 58. Pulsar velocities without neutrino mass -- Chapter 59. The neutrino ground state in a neutron star -- Chapter 60. Neutrino mass and baryon asymmetry -- Chapter 61. Axion hunting at the turn of the millenium -- Part 13: Ultra-high energy neutrinos -- Chapter 62. High energy neutrino astrophysics -- Chapter 63. The AMANDA neutrino telescope -- Chapter 64. The Lake Baikal experiment -- Chapter 65. Neutrino telescopes under the ocean: The case for ANTARES -- Chapter 66. Extremely high energy cosmic rays and neutrinos -- Part 14: Concluslon -- Chapter 67. Beyond the Standard Model: this time for real -- Chapter 68. Comments -- Chapter 69. Concluding Words -- List of Contribution Papers -- List of Poster Presentations -- List of Participants -- Author Index -- General Information.
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Archives of gynecology and obstetrics 247 (1990), S. 83-93 
    ISSN: 1432-0711
    Keywords: PP19 ; Concentration ; Body fluids ; Placental tissue
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Summary Placental protein 19 (PP19) is one of the new placental tissue proteins identified in extracts from human term placenta by Bohn and Winkler [1]. We measured the PP19 concentration in body fluids and placental tissue by radioimmunoassay; the minimum detectable dose of standard was 1.5 ng/ml. Although ethylene diamine tetraacetic acid (EDTA-2K) inhibited the immunoreaction between PP19 (225/242) and anti-PP19 antibody (632 ZA), the PP19 concentration did not differ between serum and heparin and sodium citrate plasmas. The serum PP19 concentration was increased by hemolysis. In blood cell fractions separated by the Ficoll-Paque/Macrodex method, polymorphonuclear leukocyte fraction contained the highest PP19 concentration. The circulating serum PP19 concentration was 4.5±1.1 ng/ml (mean ± standard deviation) in the proliferative phase (n=8) and 5.1±1.6 ng/ml in the secretory phase (n=7) for nonpregnant women, and 4.6±2.2 ng/ml from men (n=12). Seminal plasma (n=8) contained 212.2±99.7 ng/ml. The maternal serum PP19 concentration in 291 normal pregnancies increased from 6.2 ng/ml (median) at 6–7 weeks of gestation to 34.1 ng/ml at 38–39 weeks. The mean PP19 concentration was higher in amniotic fluid and retroplacental blood, but lower in umbilical cord blood than that in circulating maternal serum. In hydatidiform mole, vesicular fluid contained high PP19 concentration (1154.6±659.5 ng/ml), although these maternal serum concentration was not statistically higher than normal range. The chorionic villous trophoblast contained more PP19 than decidua, chorion, and amnion. These results suggest that PP19 has an extraplacental source, even though the chorionic villous trophoblast may be the main source throughout pregnancy.
    Type of Medium: Electronic Resource
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  • 3
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    In:  EPIC3Ocean margin processes in global change (R F C Mantoura, J -M Martin, R Wollast, eds ) Dahlem workshop reports 9, Wiley & Sons, Chichester, pp. 211-234
    Publication Date: 2019-07-17
    Repository Name: EPIC Alfred Wegener Institut
    Type: Book , peerRev
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  • 4
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    PANGAEA
    In:  EPIC32nd International Conference on carbon dioxide removal24-27 October 1994, Kyoto, Japan, pp, Bremerhaven, PANGAEA, pp. 1-4
    Publication Date: 2019-07-17
    Repository Name: EPIC Alfred Wegener Institut
    Type: PANGAEA Documentation , notRev
    Format: application/pdf
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  • 5
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    In:  http://aquaticcommons.org/id/eprint/9526 | 115 | 2012-10-07 15:03:35 | 9526 | WorldFish Center
    Publication Date: 2021-07-06
    Keywords: Aquaculture ; Fisheries ; Locomotion ; Burying ; Juveniles ; Tridacna crocea
    Repository Name: AquaDocs
    Type: article
    Format: application/pdf
    Format: application/pdf
    Format: 31-35
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  • 6
    Publication Date: 2021-12-16
    Description: Height of plumes generated during explosive volcanic eruptions is commonly used to estimate the associated eruption intensity (i.e., mass eruption rate; MER). In order to quantify the relationship between plume height and MER, we performed a parametric study using a three-dimensional (3D) numerical model of volcanic plumes for different vent sizes. The results of five simulations indicate that the flow pattern in the lower region of the plume systematically changes with vent size, and hence, with MER. For MERs b4 × 107 kg s−1, the flow in the lower region has a jet-like structure (the jet-like regime). For MERs N108 kg s−1, the flow shows a fountain- like structure (the fountain-like regime). The flow pattern of plumes with 4 × 107 kg s− 1 b MERs b 108 kg s− 1 shows transitional features between the two flow regimes. Within each of the two flow regimes, the plume height increases as the MER increases, whereas plume heights remain almost constant or even decrease as MER increases in the transitional regime; as a result, the jet-like and fountain-like regimes show distinct relation- ships of plume height and MER. The different relationships between the two regimes reflect the fact that the ef- ficiency of entrainment of ambient air in the jet-like regime is substantially lower than that in the fountain-like regime. It is suggested that, in order to estimate eruption intensity from the observed plume heights, it is neces- sary to take the different flow regimes depending on MER into account.
    Description: Published
    Description: 120-126
    Description: 5V. Dinamica dei processi eruttivi e post-eruttivi
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 7
    Publication Date: 2021-12-16
    Description: We performed an inter-comparison study of three-dimensional models of volcanic plumes. A set of common volca- nological input parameters and meteorological conditions were provided for two kinds of eruptions, representing a weak and a strong eruption column. From the different models, we compared the maximum plume height, neutral buoyancy level (where plume density equals that of the atmosphere), and level of maximum radial spreading of the umbrella cloud. We also compared the vertical profiles of eruption column properties, integrated across cross- sections of the plume (integral variables). Although the models use different numerical procedures and treatments of subgrid turbulence and particle dynamics, the inter-comparison shows qualitatively consistent results. In the weak plume case (mass eruption rate 1.5 × 106 kg s− 1), the vertical profiles of plume properties (e.g., vertical veloc- ity, temperature) are similar among models, especially in the buoyant plume region. Variability among the simulat- ed maximum heights is ~ 20%, whereas neutral buoyancy level and level of maximum radial spreading vary by ~ 10%. Time-averaging of the three-dimensional (3D) flow fields indicates an effective entrainment coefficient around 0.1 in the buoyant plume region, with much lower values in the jet region, which is consistent with findings of small- scale laboratory experiments. On the other hand, the strong plume case (mass eruption rate 1.5 × 109 kg s− 1) shows greater variability in the vertical plume profiles predicted by the different models. Our analysis suggests that the un- stable flow dynamics in the strong plume enhances differences in the formulation and numerical solution of the models. This is especially evident in the overshooting top of the plume, which extends a significant portion (~1/ 8) of the maximum plume height. Nonetheless, overall variability in the spreading level and neutral buoyancy level is ~20%, whereas that of maximum height is ~10%. This inter-comparison study has highlighted the different capabilities of 3D volcanic plume models, and identified key features of weak and strong plumes, including the roles of jet stability, entrainment efficiency, and particle non-equilibrium, which deserve future investigation in field, laboratory, and numerical studies.
    Description: Published
    Description: 26-42
    Description: 5V. Dinamica dei processi eruttivi e post-eruttivi
    Description: 6V. Pericolosità vulcanica e contributi alla stima del rischio
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 8
    Publication Date: 2022-08-25
    Description: This study compares and evaluates one-dimensional (1D) and three-dimensional (3D) numerical models of volcanic eruption columns in a set of different inter-comparison exercises. The exercises were designed as a blind test in which a set of common input parameters was given for two reference eruptions, representing a strong and a weak eruption column under different meteorological conditions. Comparing the results of the different models allows us to evaluate their capabilities and target areas for future improvement. Despite their different formulations, the 1D and 3D models provide reasonably consistent predictions of some of the key global descriptors of the volcanic plumes. Variability in plume height, estimated from the standard deviation of model predictions, is within ~20% for the weak plume and ~10% for the strong plume. Predictions of neutral buoyancy level are also in reasonably good agreement among the different models, with a standard deviation ranging from 9 to 19% (the latter for the weak plume in a windy atmosphere). Overall, these discrepancies are in the range of observational uncertainty of column height. However, there are important differences amongst models in terms of local properties along the plume axis, particularly for the strong plume. Our analysis suggests that the simpli- fied treatment of entrainment in 1D models is adequate to resolve the general behaviour of the weak plume. However, it is inadequate to capture complex features of the strong plume, such as large vortices, partial column collapse, or gravitational fountaining that strongly enhance entrainment in the lower atmosphere. We conclude that there is a need to more accurately quantify entrainment rates, improve the representation of plume radius, and incorporate the effects of column instability in future versions of 1D volcanic plume models.
    Description: Published
    Description: 2-25
    Description: 5V. Dinamica dei processi eruttivi e post-eruttivi
    Description: 6V. Pericolosità vulcanica e contributi alla stima del rischio
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 9
    Publication Date: 2020-02-12
    Type: info:eu-repo/semantics/article
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  • 10
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Perpendicular magnetic anisotropy (K⊥) and related magnetic properties in Pt/Fe multilayers [compositionally modulated multilayer films (CMFs)] are investigated. It is found that Pt/Fe CMFs with about an 18-A(ring) Pt layer and Fe layer below 5 A(ring) become perpendicularly magnetized films. Surface magnetic anisotropy (Ks) and volume anisotropy (Kv) are 0.46 erg/cm2 and about − 2 × 107 erg/cm3 at room temperature, respectively. The Ks is almost equivalent to that of Pt/Co CMFs and increases with decreasing temperature. The absolute value of Kv, however, is much larger than that of the Pt/Co system. The effective magnetic anisotropy (K⊥ eff) of [Fe(4.7 A(ring))/Pt(18.5 A(ring))]80 CMF changes from positive to negative at T(approximately-equal-to)200 K with decreasing temperature.
    Type of Medium: Electronic Resource
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