| Description |
1 online resource. |
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text file |
| Series |
Earth sciences in the 21st century
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Earth sciences in the 21st century series.
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| Bibliography |
Includes bibliographical references and index. |
| Contents |
THE EARTH'S CORE; STRUCTURE, PROPERTIES AND DYNAMICS; EARTH SCIENCES IN THE 21ST CENTURY; Library of Congress Cataloging-in-Publication Data; CONTENTS; PREFACE; COMPUTER MODELING OF LIQUIDIRON SOLUTIONS IN THE EARTH'S CORE; ABSTRACT; 1. INTRODUCTION; 2. EMBEDDED ATOM MODEL; 3. EAM POTENTIALS FOR IRON; 3.1. General Description; 3.2. Pure Liquid Iron at Normal Pressure; 3.3. Compressed States of Pure Iron; 3.4. The Simulation at Conditions in the Earth Centre; 4. THE USING OF SHOCK COMPRESSION DATA OF IRON; 4.1. Correcting of EAM Potential. |
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4.2. Properties of Iron Models with the Corrected EAM Potential4.3. Estimation of Melting Temperature of Iron with EAM Potential; 4.4. Situation in the Earth Centre; 4.5. Verification of Grüneisen Model; 5. MODELING OF SYSTEM IRON -- SULPHUR; 5.1. EAM Potential; 5.2. Results of Simulation of Fe -- S System; CONCLUSION; REFERENCES; ORIGIN AND DEVELOPMENT OF CORESOF THE TERRESTRIAL PLANETS:EVIDENCE FROM THEIR TECTONOMAGMATICEVOLUTION AND PALEOMAGNETIC DATA; ABSTRACT; 1. GENERAL INFORMATION ON THE PRESENT EARTH'S CORE; 2. GENERAL INFORMATION ABOUT TECTONOMAGMATICDEVELOPMENT OF THE EARTH AND MOON. |
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2.1. Tectonomagmatic Development of the Earth2.1.1. Tectonomagmatic processes in the Early Precambrian; 2.1.2. Cardinal change of tectonomagmatic processes in mid-Paleoproterozoic; 2.2. Tectonomagmatic Evolution of the Moon, Venus and Mars; 3. REASONS FOR THE EVOLUTION OF THE EARTH AND TERRESTRIAL PLANETSAND THE ROLE OF THEIR CORESIN THESE PROCESSES; 3.1. Possible Reasons for the Differences in the Magmatic Evolution of theEarth and Moon; 3.2. Similarities and Differences in the Initial Composition of TerrestrialPlanets. |
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3.3. Causes of Irreversible Tectonomagmatic Evolution of the TerrestrialPlanets3.3.1. The reason for the centripetal heating of the terrestrial planets; 3.4. The Evolution of the Terrestrial Planets Cores; 3.4.1. Evolution of the Earth's core; 3.4.2. The evolution of terrestrial planets' cores; CONCLUSION; REFERENCES; A REVIEW OF THE SLICHTER MODES:AN OBSERVATIONAL CHALLENGE; ABSTRACT; INTRODUCTION; THEORETICAL EIGENPERIOD FOR THE SLICHTER MODE; DAMPING OF THE INNER CORE MOTION; EXCITATION OF THE SLICHTER MODE; SEARCH FOR THE SLICHTER TRIPLET; CONCLUSION; REFERENCES. |
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MANIFESTATIONS OF UPWELLINGMANTLE FLOW ON THE EARTH'S SURFACEABSTRACT; 1. INTRODUCTION; 2. GEOLOGICAL BACKGROUND; 3. Magnetotelluric Soundings; 3.1. Observations and Data Analysis; 3.2. Two-Dimensional Magnetotelluric Modeling; 3.3. Resistivity Structure Beneath the Asahi Mountains; 4. HELIUM ISOTOPES OF HOT SPRINGS; 5. DISCUSSION; 5.1. Geophysical and Geochemical Evidence for Latent Magmatism; 5.2. Anelastic Crustal Uplift Caused by Latent Magmatism; 6. CONCLUSIONS; ACKNOWLEDGMENTS; REFERENCES; ON SOLIDIFICATION AND FLUCTUATIONS AT THEBOUNDARY OF THE EARTH'S INNER CORE; Abstract. |
| Local Note |
eBooks on EBSCOhost EBSCO eBook Subscription Academic Collection - North America |
| Language |
English. |
| Subject |
Earth (Planet) -- Core.
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Earth (Planet) |
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Copat, Renzo. |
| Genre/Form |
Electronic books.
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Electronic books.
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| Added Author |
Phillips, Jon M., editor.
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| Other Form: |
Print version: The Earth's core New York : Nova Science Publishers, c2012. 9781613245842 (hardcover : alk. paper) (DLC) 2011014213 |
| ISBN |
9781624175046 ebook |
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162417504X |
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9781613245842 hardcover : alkaline paper |
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161324584X |
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