Flow And Creep In The Solar System Observations Modeling And Theory
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Flow and Creep in the Solar System: Observations, Modeling and Theory
Author: David B. Stone
language: en
Publisher: Springer Science & Business Media
Release Date: 2013-03-09
The NATO ASI held in the Geophysical Institute, University of Alaska Fairbanks, June 17-28, 1991 was, we believe, the first attempt to bring together geoscientists from all the disciplines related to the solar system where fluid flow is a fundamental phenomenon. The various aspects of flow discussed at the meeting ranged from the flow of ice in glaciers, through motion of the solar wind, to the effects of flow in the Earth's mantle as seen in surface phenomena. A major connecting theme is the role played by convection. For a previous attempt to review the various ways in which convection plays an important role in natural phenomena one must go back to an early comprehensive study by 1. Wasiutynski in "Astro physica Norvegica" vo1. 4, 1946. This work, little known now perhaps, was a pioneering study. In understanding the evolution of bodies of the solar system, from accretion to present-day processes, ranging from interplanetary plasma to fluid cores, the understanding of flow hydrodynamics is essentia1. From the large scale in planetary atmospheres to geological processes, such as those seen in magma chambers on the Earth, one is dealing with thermal or chemical convection. Count Rumford, the founder of the Royal Institution, studied thermal convection experimentally and realized its practical importance in domestic contexts.
Tectonic Modeling
Author: Hemin A. Koyi
language: en
Publisher: Geological Society of America
Release Date: 2001
In this reference for geologists, 20 contributions from international scientists discuss the analytical, physical, and numerical modeling of tectonic processes. A sampling of topics includes types of transpressional and transtensional deformation, modeling of anisotropic grain growth in minerals, salt tectonics and sedimentation along Atlantic margins, and new apparatus for thermomechanical analogue modeling. The text is accompanied throughout by b&w illustrations. Annotation c. Book News, Inc., Portland, OR (booknews.com)
Dusty and Dirty Plasmas, Noise, and Chaos in Space and in the Laboratory
Author: H. Kikuchi
language: en
Publisher: Springer Science & Business Media
Release Date: 2012-12-06
I have been asked by Professor Kikuchi to write a foreword for this interesting book on Dusty Plasmas and other electrical phenomena. This was a somewhat daunting task due to the wide range of topics covered. In what follows I have attempted to summarize most of these topics; for this purpose I have divided them into four groups, namely (a) Dusty Plasmas, (b) The Electrical Environment, (c) Lightning and (d) The Noise Environment. I hope that I have succeeded. in indicating that each section contains much that is of great interest. It is perhaps unnecessary for me to point out that the book contains subjects which are at an exciting and important stage in their development. (a) Dusty Plasmas The subject of dusty plasmas is one of great interest. Dust particles in interplanetary space, within comets, in inter-stellar space and at ever greater distances will in general be charged. The plasma environment will ensure this, bombarding electrons will charge up the particle until it assumes a "floating potential," although time variation can occur. Ultra violet radiation can cause photoemission and in certain cases field emission is a possibility. The motion of the particles will be determined by electric and magnetic fields together with gravity. If the density of charged grains becomes sufficiently high the grains will interact with each other and collective behaviour will ensue. This newly evolving subject entails the study of all kinds of plasma waves.