Dorfi e a (16 resultados)

Hardcover. Condición: Very Good. Book has light rubbing and smudging to covers with light surface scratches to back, light bends to outer bottom corners, light scuffs to tips of outer corners of front cover, a subtle bend to front endpage, faint aging to edges of pages. otherwise in very good condition, strong binding, clean and unmarked pages; some cosmetic wear but an overall sturdy reading copy.…

Condición: New.

hardcover. Condición: New. In shrink wrap. Looks like an interesting title.

Condición: New. In English.

Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. Four lectures lead the reader from basic numerical methods for solving hyperbolic partial differential equations to the application of complex simulation codes to selected astrophysical problems. The text highlights the powerful capabilities, the use, and the pitfalls of computational astrophysics. Difficult topics pertaining to astrophysical problem solving, such as gravitation, magnetic fields, reactive flow, and relativity, are addressed. Two lectures are devoted to radiation hydrodynamics. They treat the derivation of the basic equations and numerical methods. This book will be useful to students and researchers in astrophysics and applied mathematics.…

Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. TOC:Nonlinear Conservation Laws and Finite Volume Methods.- Radition Hydrodynamics.- Radiation Hydrodynamics: Numerical Aspects and Applications.- Simulation of Astrophysical Fluid Flow.…

Condición: New. pp. xiv + 508.

Condición: New. pp. xiv + 508 1st Edition.

Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. Four lectures lead the reader from basic numerical methods for solving hyperbolic partial differential equations to the application of complex simulation codes to selected astrophysical problems. The text highlights the powerful capabilities, the use, and the pitfalls of computational astrophysics. Difficult topics pertaining to astrophysical problem solving, such as gravitation, magnetic fields, reactive flow, and relativity, are addressed. Two lectures are devoted to radiation hydrodynamics. They treat the derivation of the basic equations and numerical methods. This book will be useful to students and researchers in astrophysics and applied mathematics. 524 pp. Englisch.…

Buch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. TOC:Nonlinear Conservation Laws and Finite Volume Methods.- Radition Hydrodynamics.- Radiation Hydrodynamics: Numerical Aspects and Applications.- Simulation of Astrophysical Fluid Flow. 524 pp. Englisch.…

Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This book can be used also as a textbook for scientific modelling in fluid mechanics and astrophysicsThis book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applicat.…

Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This book can be used also as a textbook for scientific modelling in fluid mechanics and astrophysicsThis book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applicat.…

Condición: New. Print on Demand pp. xiv + 508 124 Illus. (6 Col.).

Condición: New. Print on Demand pp. xiv + 508.

Condición: New. PRINT ON DEMAND pp. xiv + 508.

Condición: New. PRINT ON DEMAND pp. xiv + 508.