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This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and exper...
This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and exper...
This book collects invited lectures and selected contributions presented at the Enzo Levi and XVIII Annual Meeting of the Fluid Dynamic Division of the Mexican Physical Society in 2012. It is intended for fourth-year undergraduate and graduate students, and for scientists in the fields of physics, engineering and chemistry with an interest in Fluid Dynamics from experimental, theoretical and computational points of view. The invited lectures are introductory in nature and avoid the use of complicated mathematics. The other selected contributions are also suitable for fourth-year undergraduate and graduate students. The Fluid Dynamics applications include oceanography, multiphase flows, convection, diffusion, heat transfer, rheology, granular materials, viscous flows, porous media flows and astrophysics. The material presented in the book includes recent advances in experimental and computational fluid dynamics and is well-suited to both teaching and research.
"This volume ... consists of a book with full texts of invited talks and attached CD-ROM with Extended Summaries of 1225 papers presented during the Congress"--p. x.
There are still many questions that remain about the Moon, which this book examines. From concentric craters to lunar swirls, water vapor and lunar reverberations on impact, Foster collects it all for a fascinating tour that will illuminate the backyard observer's understanding of this easily viewed, yet also imperfectly understood, celestial object. Data from Apollo and a flotilla of unmanned Moon orbiters, crashers, and landers have all contributed to our understanding of the Moon, but these mysteries linger despite decades of research. When Project Apollo brought back lunar rocks and soil samples, it opened a new chapter of understanding Earth's lone natural satellite, a process that cont...
From five authors with over two decades of experience teaching origins together in the classroom, this is the first textbook to offer a full-fledged discussion of the scientific narrative of origins from the Big Bang through humankind, from biblical and theological perspectives. This work gives the reader a detailed picture of mainstream scientific theories of origins along with how they fit into the story of God's creative and redemptive action.
The origin of the Moon is still a mystery. Some scientists believe that the Moon was formed before the Earth. The Earth emerged about 1,000 years after the Moon. • The Moon is shrinking. It has shrunk by around 200 meters across its diameter in the last billion years. The Moon is slowly moving away from the Earth at a rate of 3.8 cm (1.5 inches) per year. Scientists believe that the Moon was about 24,000 Km (15,000 miles) from Earth, now it is 384,400 km (238,855 miles). The Moon's days and nights are longer than the Earth's. One "Moon Day" is about 14 Earth days, same for the "Moon Nights." • The Moon is home to some massive mountains. The highest mountain is about 5,500 meters (18,045 feet) high, more than half the height of Mount Everest. • The Moon is an excellent source of building materials, water, fuel, oxygen, and other useful resources that are significant for modern electronics and batteries. The Moon has over 1 million tons of Helium-3, a non-polluting nuclear fuel. At the current rate of energy consumption, this will take care of 10,000 years of worldwide demand.
Urea as a Protein Supplement presents the significant advances that have been made in ruminant nutrition. This book examines the role of the rumen flora and fauna as synthesizers of protein from non-protein nitrogen sources such as ammonium compounds and urea. Organized into four parts encompassing 23 chapters, this book starts with an overview of the use of urea and other non-protein nitrogen sources in ruminant nutrition. This text then explores the various methods that may be used for the preparation of urea, which involves the dehydration of ammonium carbamate produced by the reaction of carbon dioxide and ammonia at high pressure and temperature. Other chapters consider the ways in which urea could be utilized to increase protein supplies. The final chapter deals with the hydrolysis of urea by urease to ammonia and carbon dioxide, which has been used as a method for determining urea for many years. Agricultural scientists and farmers will find this book useful.