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  • 1
    Online Resource
    Online Resource
    Cham :Springer International Publishing AG,
    Keywords: Earth sciences. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (646 pages)
    Edition: 1st ed.
    ISBN: 9783030178604
    DDC: 550
    Language: English
    Note: Intro -- Preface -- Acknowledgments -- Contents -- Chapter 1: Introduction -- 1.1 Making Descriptive and Quantitative Geosciences Work Together -- 1.2 Moving from 2D Mapping and Cross-Section Analysis to 3D Reservoir Modeling -- 1.3 Geology Is Not Random -- Why Should We Use Probability in Applied Geosciences? -- 1.4 Using Geostatistics and Statistics in Geoscience Data Analysis and Modeling -- 1.5 (Exploiting) Big Data, Not for Bigger, But for Better -- 1.6 Making Better Business Decisions with Uncertainty Analysis -- 1.7 Bridging the Great Divide in Reservoir Characterization Through Integration -- 1.8 Balancing Theory and Practicality -- 1.9 Be a Modern Geoscientist -- References -- Part I: Data Analytics -- Chapter 2: Probabilistic Analytics for Geoscience Data -- 2.1 Introduction -- 2.2 Basic Concepts -- 2.3 Probability Axioms and their Implications on Facies Analysis and Mapping -- 2.4 Conditional Probability -- 2.5 Monty Hall Problem: Importance of Understanding the Physical Condition -- 2.5.1 Lesson 1: Discerning the Non-randomness in an Indeterministic Process -- 2.5.2 Lesson 2: Value of Non-random Information -- 2.5.3 Lesson 3: Physical Process Is Important, Not Just Observed Data -- 2.6 What Is a Pure Random Process? -- 2.7 Bayesian Inference for Data Analysis and Integration -- 2.7.1 Ignoring the Likelihood Function and Relying on Prior or Global Statistics -- 2.7.2 Bayesian Inference and Interpretation Dilemma -- 2.7.3 Bayesian Inference and Base Rate or Prior Neglect -- 2.7.4 Are the Bayesian Statistics Subjective? -- 2.7.5 Bayesian Inference as a Generative Modeling Method -- 2.8 The Law of Large Numbers and Its Implications for Resource Evaluation -- 2.8.1 Remarks on the Law of Large Numbers and Spatial Data Heterogeneity -- 2.9 Probabilistic Mixture Analysis of Geoscience Data -- 2.10 Summary -- 2.11 Exercises and Problems. , References -- Chapter 3: Statistical Analysis of Geoscience Data -- 3.1 Common Statistical Parameters and Their Uses in Subsurface Data Analysis -- 3.1.1 Mean -- 3.1.1.1 Definitions -- 3.1.1.2 Weighted Mean/Average -- 3.1.1.3 Mean, Change of Scale and Sample´s Geometries -- 3.1.2 Variance, Standard Deviation, and Coefficient of Variation -- 3.1.2.1 Definitions -- 3.1.2.2 Proportional Effect and Inverse Proportional Effect -- 3.1.2.3 Variance and Change of Scale -- 3.2 Sampling Bias in Geosciences and Mitigation Methods -- 3.2.1 Areal Sampling Bias from Vertical Wells and Mitigation Methods -- 3.2.1.1 Voronoi Polygonal Tessellation -- 3.2.1.2 Propensity-Zoning Method -- 3.2.2 Vertical Sampling Bias from Vertical Wells and Mitigation -- 3.2.3 Sampling Biases from Horizontal Wells and Mitigations -- 3.2.4 Sampling Bias, Stratigraphy and Simpson´s Paradox -- 3.3 Summary -- 3.4 Exercises and Problems -- References -- Chapter 4: Correlation Analysis -- 4.1 Correlation and Covariance -- 4.2 Geological Correlation Versus Statistical Correlation -- 4.3 Correlation and Covariance Matrices -- 4.4 Partial Transitivity of Correlations -- 4.5 Effects of Other Variables on (Bivariate) Correlations -- 4.6 Correlation, Causation and Physical Laws -- 4.6.1 Correlation, Causation and Causal Diagrams -- 4.6.2 Using Physical Laws in Correlation Analysis -- 4.7 Impact of Correlation by Missing Values or Sampling Biases -- 4.8 Spearman Rank Correlation and Nonlinear Transforms -- 4.9 Correlation for Categorical Variables -- 4.9.1 Stratigraphy-Related Simpson´s Paradox -- 4.10 Trivariate Correlation and Covariance (Can Be Skipped for Beginners) -- 4.11 Summary -- 4.12 Exercises and Problems -- Appendices -- Appendix 4.1 Probabilistic Definitions of Mean, Variance and Covariance -- Appendix 4.2 Graphic Displays for Analyzing Variables´ Relationships -- References. , Chapter 5: Principal Component Analysis -- 5.1 Overview -- 5.1.1 Aims of PCA -- 5.1.2 Procedures of PCA -- 5.1.3 Example -- 5.2 Specific Issues -- 5.2.1 Using Correlation or Covariance Matrix for PCA -- 5.2.2 Relationship Between PCA and Factor Analysis -- 5.2.3 Interpretations and Rotations of Principal Components -- 5.2.4 Selection of Principal Components -- 5.3 PCA for Classifications -- 5.4 Performing PCA Conditional to a Geological Constraint -- 5.5 Cascaded PCAs for Characterizing 3D Volumes and Compaction of Data -- 5.6 PCA for Feature Detection and Noise Filtering -- 5.7 Summary -- 5.8 Exercises and Problems -- Appendices -- Appendix 5.1 Introduction to PCA with an Example -- A5.1.1 Introductory Example -- A5.1.2 Standardizing Data -- A5.1.3 Computing Correlation Matrix -- A5.1.4 Finding Eigenvectors and Eigenvalues -- A5.1.5 Finding the principal components -- A5.1.6 Basic Analytics in PCA -- References -- Chapter 6: Regression-Based Predictive Analytics -- 6.1 Introduction and Critiques -- 6.2 Bivariate Regression -- 6.2.1 Bivariate Linear Regression -- 6.2.2 Variations of Bivariate Linear Regression -- 6.2.3 Remarks -- 6.2.4 Nonlinear Bivariate Regression -- 6.3 Multivariate Linear Regression (MLR) -- 6.3.1 General -- 6.3.2 Effect of Collinearity -- 6.3.3 Subset Selection -- 6.3.4 Regularization -- 6.4 Principal Component Regression (PCR) -- 6.4.1 Selection of Principal Components for PCR -- 6.4.2 Comparison of Subset Selection, Ridge Regression and PCR -- 6.5 An Example -- 6.6 Summary -- 6.7 Exercises and Problems -- Appendices -- Appendix 6.1: Lord´s Paradox and Importance of Judgement Objectivity -- Appendix 6.2 Effects of Collinearity in Multivariate Linear Regression -- A6.2.1 Cooperative Suppression -- A6.2.2 Net Suppression -- References -- Chapter 7: Introduction to Geoscience Data Analytics Using Machine Learning. , 7.1 Overview of Artificial-Intelligence-Based Prediction and Classification Methods -- 7.1.1 Extensions of Multivariate Regressions -- 7.1.2 Ensemble of Algorithms or Combined Methods -- 7.1.3 Validation of Predictions and Classifications -- 7.2 Challenges in Machine Learning and Artificial Intelligence -- 7.2.1 Model Complexity -- 7.2.2 Generative Model Versus Discriminative Model -- 7.2.3 Trading Bias and Variance -- 7.2.4 Balancing the Overfitting and Underfitting -- 7.2.5 Collinearity and Regularization in Big Data -- 7.2.6 The No-Free-Lunch Principle -- 7.3 Basics of Artificial Neural Networks (ANN) -- 7.3.1 Back Propagation Algorithm for ANN -- 7.3.2 Unsupervised Learning and Supervised Learning -- 7.3.3 Advantages and Disadvantages of Using Neural Networks -- 7.4 Example Applications Using ANN and Ensembled Methods -- 7.4.1 Classification -- 7.4.2 Integration of Data for Predicting Continuous Geospatial Properties -- 7.4.3 Ensembled ANN and Geostatistical Method for Modeling Geospatial Properties -- 7.5 Summary -- References -- Part II: Reservoir Characterization -- Chapter 8: Multiscale Heterogeneities in Reservoir Geology and Petrophysical Properties -- 8.1 Introduction -- 8.2 Structural Elements -- 8.2.1 Anticlines -- 8.2.2 Faults and Fractures -- 8.3 Multiscale Heterogeneities in Sequence Stratigraphic Hierarchy -- 8.4 Depositional Environments, Facies Spatial and Geometric Heterogeneities -- 8.5 Facies and Lithology: Compositional Spatial Trends -- 8.5.1 Facies Lateral and Vertical Trends -- 8.5.2 Lithology Compositional Trends -- 8.6 Heterogeneities in Petrophysical Properties -- 8.6.1 Statistical Description of Heterogeneities in Petrophysical Properties -- 8.6.2 Other Non-spatial Measures of Petrophysical Properties´ Heterogeneities -- 8.6.3 Spatial Descriptions of Heterogeneities in Petrophysical Properties. , 8.6.4 Spatial Discontinuity in Petrophysical Properties -- 8.7 Data and Measurements for Describing Heterogeneities -- 8.8 Impact of Heterogeneities on Subsurface Fluid Flow and Production -- 8.9 Summary -- Appendices -- Appendix 8.1 Large-Scale Tectonic Settings and their Characteristics -- Appendix 8.2 Sequence Stratigraphic Hierarchy in Fluvial Setting -- References -- Chapter 9: Petrophysical Data Analytics for Reservoir Characterization -- 9.1 Porosity Characterization and Estimation -- 9.1.1 Total and Effective Porosities -- 9.1.2 Deriving Porosity Data at Wells -- 9.1.2.1 Porosity from a Single Well Log (Basic Principles) -- Density Porosity -- Sonic Porosity -- Neutron Porosity -- NMR Porosity -- 9.1.2.2 Deriving Porosity from Two or More Logs and Correlation Analysis -- 9.1.3 Correlation Analysis of Porosity-Measuring Logs and Lithology Mixture -- 9.1.4 Calibration of Core and Well-Log Porosities -- 9.1.5 Common Issues and Their Mitigations in Porosity Estimation -- 9.1.5.1 Borehole Conditions -- 9.1.5.2 Other Issues -- 9.1.6 Effects of Minerals and Other Contents -- 9.2 Clay Volume and Its Impacts on Other Petrophysical Parameters -- 9.3 Permeability Characterization -- 9.3.1 Factors Affecting Permeability -- 9.3.2 Relationships Between Permeability and Other Properties -- 9.3.2.1 Impacts of Geological Variables on Porosity-Permeability Relationship -- 9.3.2.2 Correlation Analysis -- 9.4 Water Saturation (Sw) Characterization -- 9.5 Reservoir Quality Analysis -- 9.5.1 Assessing reservoir Quality Using Static Properties -- 9.5.2 Reservoir Quality Index and Flow Zone Indicator -- 9.6 Summary -- Appendix 9.1: Common Well Logs, and Related Petrophysical and Geological Properties -- References -- Chapter 10: Facies and Lithofacies Classifications from Well Logs -- 10.1 Background and Introductory Example. , 10.1.1 Facies, Lithofacies, Petrofacies, Electrofacies, and Rock Types.
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  • 2
    Type of Medium: Book
    Pages: xxv, 640 Seiten , Illustrationen
    ISBN: 9783030178598
    Language: English
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  • 3
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Biochemistry 34 (1995), S. 13233-13241 
    ISSN: 1520-4995
    Source: ACS Legacy Archives
    Topics: Biology , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Biochemistry 34 (1995), S. 13242-13251 
    ISSN: 1520-4995
    Source: ACS Legacy Archives
    Topics: Biology , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 5
    ISSN: 1439-0523
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Notes: Three lines conferring resistance to powdery mildew, Pm97033, Pm97034 and Pm97035, were developed from the cross of Triticum durum-Haynaldia villosa amphidiploid TH3 and wheat cv.‘Wan7107’ via backcrosses, immature embryo and anther culture. Genomic in situ hybridization analysis showed that these lines were disomic translocation lines. Cytogenetic analysis indicated that the F1 plants of crosses between the three translocation lines and ‘Wan7107’ and crosses between the three translocation lines and substitution line 6V(6D) formed 21 bivalents at meiotic metaphase I. Aneuploid analysis with ‘Chinese Spring’ double ditelocentric stocks indicated that the translocated chromosomes were related to chromosome 6D. Biochemical and restriction fragment-length polymorphism (RFLP) analyses showed that the translocation lines lacked a specific band of 6VL of H. villosa compared with the substitution and addition lines but possessed specific markers on the short arm of the 6V chromosome of H. villosa. The three translocation lines lacked specific biochemical loci and RFLP markers located on chromosome 6DS. The results confirmed that Pm97033, Pm97034 and Pm97035 were T6DL.6VS translocation lines.
    Type of Medium: Electronic Resource
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  • 6
    ISSN: 1437-7799
    Keywords: Key words pICln ; Chloride channel ; LLC-PK1 ; ATP ; Azide ; Dihydrocytochalasin
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Abstract Background. There has been no conclusive explanation regarding the function of pICln (a 26- to 27-kDa acidic protein) on an osmo-sensitive chloride channel responsible for an outwardly rectifying anion current. We observed the effects of the hypotonic treatment of LLC-PK1 cells on the intra-cellular dynamic state of pICln. Methods. LLC-PK1 cells were cultured, and pICln in cells was observed immunohistochemically. The cells were fractionated into nuclei, mitochondrial, microsomal, and soluble fractions biochemically, and pICln was detected by an immunoblotting method after sodium dodecyl sulfate (SDS)-polyacrylamide gel electrophoresis. Results. pICln in cells was observed on nuclei and their surroundings, but not on cell membranes. pICln was present in soluble and insoluble forms. The molecular masses of the oligomeric forms in the soluble fractions were different from those previously reported with Madin-Darby canine kidney (MDCK) cells, indicating the differences in the pICln-oligomer depending on cell type. On analysis with SDS-polyacrylamide gel electrophoresis, the exposure of cells to hypotonic media elevated the ratio of soluble to insoluble forms within 5 min. This result also conflicted with those previously reported with MDCK cells. This finding suggests that the function of pICln and the signaling mechanism differ depending on the cell species. Both extracellular ATP and NaN3 inhibited this elevation of the soluble/insoluble ratio, coinciding with previous reports that extracellular nucleotides and depletion of intracellular ATP inhibited the volume-sensitive chloride channel. Dihydrocytochalasin B, an F-actin-disrupting drug, inhibited the elevation of the soluble/insoluble ratio. Conclusions. The soluble form of pICln was increased within 5 min by exposure of LLC-PK1 cells to hypotonic media. This translocation was inhibited by extracellular ATP, NaN3, and dihydrocytochalasin.
    Type of Medium: Electronic Resource
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  • 7
    Publication Date: 2014-02-15
    Description: We investigate the effects of warm dark matter (WDM) on the cosmic 21-cm signal. If dark matter exists as WDM instead of cold dark matter (CDM), its non-negligible velocities can inhibit the formation of low-mass haloes that normally form first in CDM models, therefore delaying star formation. The absence of early sources delays the build-up of UV and X-ray backgrounds that affect the 21-cm radiation signal produced by neutral hydrogen. With use of the 21CMFAST  code, we demonstrate that the pre-reionization 21-cm signal can be changed significantly in WDM models with a free-streaming length equivalent to that of a thermal relic with mass m X of up to ~10–20 keV. In such a WDM cosmology, the 21-cm signal traces the growth of more massive haloes, resulting in a delay of the 21-cm absorption signature and followed by accelerated X-ray heating. CDM models where astrophysical sources have a suppressed photon-production efficiency can delay the 21-cm signal as well, although its subsequent evolution is not as rapid as compared to WDM. This motivates using the gradient of the global 21-cm signal to differentiate between some CDM and WDM models. Finally, we show that the degeneracy between the astrophysics and m X can be broken with the 21-cm power spectrum, as WDM models should have a bias-induced excess of power on large scales. This boost in power should be detectable with current interferometers for models with m X 3 keV, while next-generation instruments will easily be able to measure this difference for all relevant WDM models.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 8
    Publication Date: 2014-04-01
    Description: Author(s): Y. Fan, X. Ma, F. Fang, J. Zhu, Q. Li, T. P. Ma, Y. Z. Wu, Z. H. Chen, H. B. Zhao, and G. Lüpke Spin angular momentum transfer into an antiferromagnetic (AFM) insulator is observed in a single-crystalline Fe/CoO/MgO(001) heterostructure by time-resolved magneto-optical Kerr effect. The transfer process is mediated by the Heisenberg exchange coupling between Fe and CoO spins. Spin angular momen... [Phys. Rev. B 89, 094428] Published Mon Mar 31, 2014
    Keywords: Magnetism
    Print ISSN: 1098-0121
    Electronic ISSN: 1095-3795
    Topics: Physics
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  • 9
    Publication Date: 2013-12-18
    Description: A maximum-likelihood method, tested as an unbiased estimator from numerical simulations, is used to estimate cosmic bulk flow from peculiar velocity surveys. The likelihood function is applied to four observational catalogues (ENEAR, SFI++, A1SN and SC) constructed from galaxy peculiar velocity surveys and Type Ia supernovae data at low redshift ( z  ≤ 0.03). We find that the Spiral Field I-band catalogue constrains the bulk flow to be V  = 290 ± 30 km s –1 towards l  = 281° ± 7°, $b=8^{\circ +6^{\circ }}_{-5^{\circ }}$ on effective scales of 58 h –1 Mpc, which is the tightest constraints achievable at the present time. By comparing the amplitudes of our estimated bulk flows with theoretical prediction, we find excellent agreement between the two. In addition, directions of estimated bulk flows are also consistent with measurements in other studies.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 10
    Publication Date: 2015-10-19
    Description: H i intensity mapping is an emerging tool to probe dark energy. Observations of the redshifted H i signal will be contaminated by instrumental noise, atmospheric and Galactic foregrounds. The latter is expected to be four orders of magnitude brighter than the H i emission we wish to detect. We present a simulation of single-dish observations including an instrumental noise model with 1/ f and white noise, and sky emission with a diffuse Galactic foreground and H i emission. We consider two foreground cleaning methods: spectral parametric fitting and principal component analysis. For a smooth frequency spectrum of the foreground and instrumental effects, we find that the parametric fitting method provides residuals that are still contaminated by foreground and 1/ f noise, but the principal component analysis can remove this contamination down to the thermal noise level. This method is robust for a range of different models of foreground and noise, and so constitutes a promising way to recover the H i signal from the data. However, it induces a leakage of the cosmological signal into the subtracted foreground of around 5 per cent. The efficiency of the component separation methods depends heavily on the smoothness of the frequency spectrum of the foreground and the 1/ f noise. We find that as long as the spectral variations over the band are slow compared to the channel width, the foreground cleaning method still works.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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