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|a UAMI
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| 245 |
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|a The Earth's core :
|b structure, properties, and dynamics /
|c Jon M. Phillips, editor.
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| 264 |
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1 |
|a New York :
|b Nova Science Publishers, Inc.,
|c [2012]
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| 300 |
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|a 1 online resource.
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|a text
|b txt
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|a computer
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|2 rdamedia
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|a Earth sciences in the 21st century
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| 504 |
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|a Includes bibliographical references and index.
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| 588 |
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|a Description based on print version record.
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| 546 |
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|a English.
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|a 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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| 505 |
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|a 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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| 505 |
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|a 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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| 505 |
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|a 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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| 505 |
8 |
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|a 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.
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|a Phillips, Jon M.,
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|t The Earth's core
|d New York : Nova Science Publishers, c2012.
|z 9781613245842 (hardcover : alk. paper)
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