Listing 1 - 10 of 20 | << page >> |
Sort by
|
Choose an application
Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.
Magnetohydrodynamics --- Astrophysical jets --- Stellar dynamics --- Mathematics --- EPUB-LIV-FT LIVPHYSI SPRINGER-B
Choose an application
Hydraulics --- Flow of water --- Water --- Fluid mechanics --- Hydraulic engineering --- Jets --- Mathematical models. --- Flow --- Distribution
Choose an application
Hydraulic engineering. --- Hydraulics. --- Flow of water --- Water --- Fluid mechanics --- Hydraulic engineering --- Jets --- Engineering, Hydraulic --- Engineering --- Hydraulics --- Shore protection --- Flow --- Distribution
Choose an application
Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.
Space research --- Astrophysics --- Theory of relativity. Unified field theory --- Geophysics --- zwaartekracht --- astrofysica --- relativiteitstheorie --- ruimtevaart --- Magnetohydrodynamics --- Astrophysical jets --- Stellar dynamics --- Mathematics --- EPUB-LIV-FT LIVPHYSI SPRINGER-B
Choose an application
Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.
Astrophysical jets -- Mathematics. --- Magnetohydrodynamics -- Mathematics. --- Stellar dynamics -- Mathematics. --- Magnetohydrodynamics --- Astrophysical jets --- Stellar dynamics --- Astronomy & Astrophysics --- Astrophysics --- Physical Sciences & Mathematics --- Mathematics --- Mathematics. --- Dynamics, Stellar --- Stars --- Magneto-hydrodynamics --- MHD (Physics) --- Dynamics --- Physics. --- Gravitation. --- Astrophysics. --- Space sciences. --- Astrophysics and Astroparticles. --- Extraterrestrial Physics, Space Sciences. --- Classical and Quantum Gravitation, Relativity Theory. --- Celestial mechanics --- Jets --- Radio sources (Astronomy) --- Fluid dynamics --- Plasma dynamics --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Field theory (Physics) --- Matter --- Antigravity --- Centrifugal force --- Relativity (Physics) --- Science and space --- Space research --- Cosmology --- Science --- Properties
Choose an application
These Lecture Notes focus on the physics of relativistic jet sources in the universe, from galactic microquasars to active galactic nuclei (AGN). The early 21st century is an epoch in which a large number of high-energy astronomical missions are underway (RossiXTE, Chandra, XMM-Newton, INTEGRAL, Swift, Suzaku). The wealth of X-ray and gamma-ray data, coupled with ground-based observations in the optical/IR/radio bands, provides an increasing amount of information on microquasars, allowing the investigation of the physical processes for the formation and the evolution of relativistic jets, as well as their relation to the accretion process. The information obtained from galactic relativistic jet systems is particularly important in that it can be compared with that from active galactic nuclei. The comparative study of these two classes of objects allows us to overcome their separate intrinsic limitations and is the only way to arrive at a comprehensive understanding of the accretion/ejection phenomenon. This book covers the topic of accretion/ejection in relativistic jet sources with a broad approach, from microquasars to AGN, discussing both observational and theoretical aspects. The aim is to present a broad view of the field and the current standpoint now that the first comparative studies have opened the way to a global study at a mass scale. Written in a pedagogical lecture notes style, the book benefits students and newcomers to jet astrophysics as well as lecturers and researchers. .
Astrophysical jets --- Quasars --- Astronomy & Astrophysics --- Astrophysics --- Physical Sciences & Mathematics --- Superluminal radio sources (Astronomy) --- Astrophysics. --- Astronomical physics --- Superlight sources (Astronomy) --- Superluminal sources (Astronomy) --- Physics. --- Gravitation. --- Space sciences. --- Extraterrestrial Physics, Space Sciences. --- Astrophysics and Astroparticles. --- Classical and Quantum Gravitation, Relativity Theory. --- Astronomy --- Cosmic physics --- Physics --- Radio sources (Astronomy) --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Field theory (Physics) --- Matter --- Antigravity --- Centrifugal force --- Relativity (Physics) --- Science and space --- Space research --- Cosmology --- Science --- Properties
Choose an application
Astronomical jets are key astrophysical phenomena observed in gamma-ray bursts, active galactic nuclei or young stars. Research on them has largely occurred within the domains of astronomical observations, astrophysical modeling and numerical simulations, but the recent advent of high energy density facilities has added experimental control to jet studies. Front-line research on jet launching and collimation requires a highly interdisciplinary approach and an elevated level of sophistication. Bridging the gaps between pure magnetohydrodynamics, thermo-chemical evolution, high angular resolution spectro-imaging and laboratory experiments is no small matter. This volume strives to bridge those very gaps. It offers a series of lectures which, taken as whole, act as a thorough reference for the foundations of this discipline. These lectures address the following: · laboratory jets physics from laser and z-pinch plasma experiments, · the magnetohydrodynamic theory of relativistic and non-relativistic stationary jets, · heating mechanisms in magnetohydrodynamic jets, from the solar magnetic reconnection to the molecular shock heating perspectives, · atomic and molecular microphysics of jet shocked material. In addition to the lectures, the book offers, in closing, a presentation of a series of observational diagnostics, thus allowing for the recovery of basic physical quantities from jet emission lines.
Astrophysical jets --- Stellar dynamics --- Magnetohydrodynamic instabilities --- Astronomy & Astrophysics --- Astronomy - General --- Astrophysics --- Physical Sciences & Mathematics --- Hydromagnetic instabilities --- Instabilities, Magnetohydrodynamic --- MHD instabilities --- Dynamics, Stellar --- Stars --- Dynamics --- Earth sciences. --- Planetology. --- Observations, Astronomical. --- Astronomy --- Astrophysics. --- Space sciences. --- Amorphous substances. --- Complex fluids. --- Earth Sciences. --- Astronomy, Observations and Techniques. --- Astrophysics and Astroparticles. --- Extraterrestrial Physics, Space Sciences. --- Soft and Granular Matter, Complex Fluids and Microfluidics. --- Observations. --- Complex liquids --- Fluids, Complex --- Amorphous substances --- Liquids --- Soft condensed matter --- Science and space --- Space research --- Cosmology --- Science --- Astronomical physics --- Cosmic physics --- Physics --- Astronomical observations --- Observations, Astronomical --- Planetary sciences --- Planetology --- Geosciences --- Environmental sciences --- Physical sciences
Choose an application
This book offers a comprehensive approach to the numerical modeling of open channel flow, based on the author’s own research in this field, as well as his experience as a lecturer. It provides the reader with: Coverage of the most important problems of open channel hydraulics, including steady and unsteady flow in a single channel and in a channel network, transport of dissolved substance, transport of energy and more; Unified derivation of the governing equations for all problems, based on the fundamental laws of mass, momentum and energy conservation; Comprehensive presentation of the numerical methods applied in open channel flow modeling, with particular regard to the solution of hyperbolic and parabolic partial differential equations, which govern many important flow and transport processes; Detailed description of the numerical algorithms applied to solve particular problems, with many examples of solutions; Accuracy analysis of the numerical algorithms using the modified equation approach; New insights into numerical solution of some classical problems of open channel hydraulics, e.g. steady varied flow in a channel of arbitrary geometry. In-depth analysis of the simplified flood routing models and their unphysical properties, including a proposition of an alternative Instantaneous Unit Hydrograph, valid for all simplified models. Written in accessible language, Numerical Modeling in Open Channel Hydraulics contains information useful for higher level undergraduate and postgraduate students of civil and environmental engineering faculties, as well as scientists and practitioners in the field of hydraulic engineering, especially those using existing numerical codes or developing their own ones.
Channels (Hydraulic engineering) -- Mathematical models. --- Channels (Hydraulic engineering) --- Mechanical Engineering --- Civil & Environmental Engineering --- Engineering & Applied Sciences --- Civil Engineering --- Hydraulic Engineering --- Mathematical models --- Hydrodynamics. --- Mathematical models. --- Engineering. --- Hydrogeology. --- Computational intelligence. --- Engineering geology. --- Engineering --- Foundations. --- Hydraulics. --- Environmental engineering. --- Biotechnology. --- Geoengineering, Foundations, Hydraulics. --- Environmental Engineering/Biotechnology. --- Computational Intelligence. --- Geology. --- Chemical engineering --- Genetic engineering --- Environmental control --- Environmental effects --- Environmental stresses --- Environmental health --- Environmental protection --- Pollution --- Sustainable engineering --- Flow of water --- Water --- Fluid mechanics --- Hydraulic engineering --- Jets --- Architecture --- Building --- Structural engineering --- Underground construction --- Caissons --- Earthwork --- Masonry --- Soil consolidation --- Soil mechanics --- Walls --- Civil engineering --- Geology, Economic --- Intelligence, Computational --- Artificial intelligence --- Soft computing --- Geohydrology --- Geology --- Hydrology --- Groundwater --- Construction --- Industrial arts --- Technology --- Flow --- Distribution --- Details --- Fluid dynamics --- Bodies of water --- River channels
Choose an application
It is not an easy task to fascinate a student with a standard course on Soil Mechanics and Geotechnical Engineering. If, however, the same material is presented as a tool to explore a natural or a man-made "disaster", both the motivation and the ability to absorb this material increase dramatically. The case studies in this book could help to build an introductory Forensic Geotechnical Engineering course, covering such basic topics as settlements, bearing capacity and excavations. The failure cases considered in this book have something in common – they can be all reasonably well explained using so called "back-of-the-envelope" calculations, i.e., without sophisticated models requiring finite element analysis. These simple methods based on clear mechanical considerations are the endangered species of the computer dominated era, though sometimes they could prevent a disaster caused by a wrong application of computer models. In particular, the upper bound limit analysis has repeatedly proven itself as a powerful tool allowing for sufficiently accurate estimates of the failure loads and leaving a lot of room for creativity. No one is exempt from making mistakes, but repeating well known mistakes reveals a gap in education. One of the objectives of this book is to attempt bridging this gap, at least partially. More failure cases covering a larger area of geotechnical problems are included into the companion book "Geomechanics of Failures: Advanced Topics" by the same authors.
Electronic books. -- local. --- Soil mechanics -- Case studies. --- Soil mechanics -- Mathematical models. --- Structural failures -- Case studies. --- Structural failures -- Mathematical models. --- Structural failures --- Structural analysis (Engineering) --- Soil mechanics --- Mechanical Engineering --- Civil & Environmental Engineering --- Engineering & Applied Sciences --- Civil Engineering --- Hydraulic Engineering --- Investigation --- Mathematics --- Mathematical models. --- Collapse of structures --- Failures, Structural --- Soil engineering --- Soils --- Soils (Engineering) --- Mechanics --- Engineering. --- Earth sciences. --- Economic geology. --- Geotechnical engineering. --- Engineering geology. --- Engineering --- Foundations. --- Hydraulics. --- Geoengineering, Foundations, Hydraulics. --- Economic Geology. --- Geotechnical Engineering & Applied Earth Sciences. --- Earth Sciences, general. --- Geology. --- Deformations (Mechanics) --- Fracture mechanics --- Reliability (Engineering) --- Safety factor in engineering --- Structural stability --- Geotechnical engineering --- Foundations --- Soil physics --- Hydraulic engineering. --- Geology, economic. --- Geography. --- Cosmography --- Earth sciences --- World history --- Economic geology --- Physical geology --- Mines and mineral resources --- Engineering, Hydraulic --- Fluid mechanics --- Hydraulics --- Shore protection --- Mathematics. --- Engineering—Geology. --- Architecture --- Building --- Structural engineering --- Underground construction --- Caissons --- Earthwork --- Masonry --- Soil consolidation --- Walls --- Civil engineering --- Geology, Economic --- Geosciences --- Environmental sciences --- Physical sciences --- Engineering, Geotechnical --- Geotechnics --- Geotechnology --- Engineering geology --- Flow of water --- Water --- Hydraulic engineering --- Jets --- Details --- Geology --- Flow --- Distribution
Choose an application
The magnitude Ms 8.0 (Mw 7.9) Wenchuan earthquake occurred on 12 May 2008 in the Longmen Shan region of China—the topographical boundary between the Tibetan Plateau and the Sichuan Basin—resulting in extensive damage throughout central and western China. To understand the seismic faulting mechanism and surface deformation features associated with the Wenchuan earthquake, including rupture length, geometric characteristics, and slip distribution of co-seismic surface rupture, our survey group traveled to the epicentral area 2 days after the earthquake and undertook 10 days of fieldwork, during which time we collected fundamental data related to rupture structures and the spatial distribution of offset along faults. Based on the results of this preliminary fieldwork, we carried out additional detailed fieldwork along the co-seismic surface rupture over the following year. This photographic atlas shows the main deformation characteristics of co-seismic surface rupture and the nature of the earthquake disaster and subsequent relief operations, based on photographs taken during our field investigations. This atlas is intended not only for geologists, seismologists, and engineers as a means of furthering their understanding of the seismic mechanisms and surface rupture deformation characteristics of large intracontinental earthquakes, but also for advanced undergraduates and graduate students as a textbook. We are grateful to the many organizations and individuals who helped to make this book possible. Thanks are also due to Professor Dong Jia and Dr. Xiaojun Wu of the Nanjing University for their assistance in the field.
Earthquakes -- China -- Wenchuan Xian (Sichuan Sheng) -- Maps. --- Earthquakes -- China -- Wenchuan Xian (Sichuan Sheng) -- Pictorial works. --- Wenchuan Earthquake, China, 2008. --- Wenchuan Xian (Sichuan Sheng, China) -- Remote-sensing images. --- Earthquakes --- Wenchuan Xian (Sichuan Sheng, China) --- Quakes (Earthquakes) --- Great Sichuan Earthquake, China, 2008 --- Sichuan Earthquake, China, 2008 --- Wen-chʻuan hsien (Sichuan Sheng, China) --- Wun-khron-rdzoṅ (Sichuan Sheng, China) --- Earth sciences. --- Geology. --- Geophysics. --- Geotechnical engineering. --- Engineering geology. --- Engineering --- Foundations. --- Hydraulics. --- Earth Sciences. --- Geophysics and Environmental Physics. --- Geoengineering, Foundations, Hydraulics. --- Geotechnical Engineering & Applied Earth Sciences. --- Geophysics/Geodesy. --- Earth movements --- Natural disasters --- Seismology --- 汶川县 (Sichuan Sheng, China) --- Hydraulic engineering. --- Physical geography. --- Geography --- Engineering, Hydraulic --- Fluid mechanics --- Hydraulics --- Shore protection --- Geognosy --- Geoscience --- Earth sciences --- Natural history --- Engineering—Geology. --- Engineering, Geotechnical --- Geotechnics --- Geotechnology --- Engineering geology --- Flow of water --- Water --- Hydraulic engineering --- Jets --- Architecture --- Building --- Structural engineering --- Underground construction --- Caissons --- Earthwork --- Masonry --- Soil consolidation --- Soil mechanics --- Walls --- Civil engineering --- Geology, Economic --- Geological physics --- Terrestrial physics --- Physics --- Flow --- Distribution --- Details --- Geology
Listing 1 - 10 of 20 | << page >> |
Sort by
|