hierarchical geometrical methods scientific di hamann bernd (36 risultati)

gebundene Ausgabe. Condizione: Sehr gut. Zust: Gutes Exemplar. VI, 367 Seiten, mit Abbildungen, Englisch 648g.

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Paperback. Condizione: new. Paperback. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early in?ationary period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ?ying away from each other. We can attribute di?erent rates of this expansion to domination of di?erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using?xed, non-interactive animations has a long history. Several books and ?lms exist, ranging from Cosmic View: The Universe in Forty Jumps [3] by Kees Boeke to Powers of 10 [6,13] by Charles and Ray Eames, and the recent Imax ?lm Cosmic Voyage [15]. We have added our own contribution [9], Cosmic Clock, which is an animation based entirely on the concepts and implementation described in this paper. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Shipping may be from multiple locations in the US or from the UK, depending on stock availability.

Hardcover. Condizione: new. Hardcover. This book emerged from a DoE/NSF-sponsored workshop, held in Tahoe City, California, October 2000. About fifty invited participants presented state-of-the-art research on topics such as: - terrain modeling- multiresolution subdivision- wavelet-based scientific data compression- topology-based visualization- data structures, data organization and indexing schemes for scientific data visualization.All invited papers were carefully refereed, resulting in this collection. The book will be of great interest to researchers, graduate students and professionals dealing with scientific visualization and its applications. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Shipping may be from multiple locations in the US or from the UK, depending on stock availability.

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Condizione: New. pp. 376.

Condizione: Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher.

Buch. Condizione: Neu. Neuware -The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early ¿in ationary¿ period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ying away from each other. We can attribute di erent rates of this expansion to domination of di erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using xed, non-interactive animations has a long history. Several books and lms exist, ranging from ¿Cosmic View: The Universe in Forty Jumps¿ [3] by Kees Boeke to ¿Powers of 10¿ [6,13] by Charles and Ray Eames, and the recent Imax lm ¿Cosmic Voyage¿ [15]. We have added our own contribution [9], ¿Cosmic Clock,¿ which is an animation based entirely on the concepts and implementation described in this paper.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 376 pp. Englisch.

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early 'in ationary' period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ying away from each other. We can attribute di erent rates of this expansion to domination of di erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using xed, non-interactive animations has a long history. Several books and lms exist, ranging from 'Cosmic View: The Universe in Forty Jumps' [3] by Kees Boeke to 'Powers of 10' [6,13] by Charles and Ray Eames, and the recent Imax lm 'Cosmic Voyage' [15]. We have added our own contribution [9], 'Cosmic Clock,' which is an animation based entirely on the concepts and implementation described in this paper.

Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early 'in ationary' period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ying away from each other. We can attribute di erent rates of this expansion to domination of di erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using xed, non-interactive animations has a long history. Several books and lms exist, ranging from 'Cosmic View: The Universe in Forty Jumps' [3] by Kees Boeke to 'Powers of 10' [6,13] by Charles and Ray Eames, and the recent Imax lm 'Cosmic Voyage' [15]. We have added our own contribution [9], 'Cosmic Clock,' which is an animation based entirely on the concepts and implementation described in this paper.

Condizione: New. pp. vi + 367.

Condizione: New. Editor(s): Farin, Gerald; Hamann, Bernd; Hagen, Hans. Series: Mathematics and Visualization. Num Pages: 373 pages, biography. BIC Classification: PBKS; PBV; UMZ; UT; UYA. Category: (P) Professional & Vocational. Dimension: 235 x 155 x 20. Weight in Grams: 575. . 2012. Softcover reprint of the original 1st ed. 2003. Paperback. . . . .

Condizione: New. This book emerged from a DoE/NSF-sponsored workshop in California in 2000. About 50 participants presented research on topics such as terrain modelling, multiresolution subdivision, wavelet-based scientific data compression, topology-based visualization, data structures and data indexing schemes. Editor(s): Farin, Gerald; Hamann, B.; Hagen, H. Series: Mathematics and Visualization. Num Pages: 373 pages, biography. BIC Classification: PDE; TBJ. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 22. Weight in Grams: 708. . 2002. Hardback. . . . .

Paperback. Condizione: Brand New. 376 pages. 9.25x6.10x0.85 inches. In Stock.

Condizione: New. Editor(s): Farin, Gerald; Hamann, Bernd; Hagen, Hans. Series: Mathematics and Visualization. Num Pages: 373 pages, biography. BIC Classification: PBKS; PBV; UMZ; UT; UYA. Category: (P) Professional & Vocational. Dimension: 235 x 155 x 20. Weight in Grams: 575. . 2012. Softcover reprint of the original 1st ed. 2003. Paperback. . . . . Books ship from the US and Ireland.

Condizione: New. This book emerged from a DoE/NSF-sponsored workshop in California in 2000. About 50 participants presented research on topics such as terrain modelling, multiresolution subdivision, wavelet-based scientific data compression, topology-based visualization, data structures and data indexing schemes. Editor(s): Farin, Gerald; Hamann, B.; Hagen, H. Series: Mathematics and Visualization. Num Pages: 373 pages, biography. BIC Classification: PDE; TBJ. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 22. Weight in Grams: 708. . 2002. Hardback. . . . . Books ship from the US and Ireland.

Paperback. Condizione: new. Paperback. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early in?ationary period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ?ying away from each other. We can attribute di?erent rates of this expansion to domination of di?erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using?xed, non-interactive animations has a long history. Several books and ?lms exist, ranging from Cosmic View: The Universe in Forty Jumps [3] by Kees Boeke to Powers of 10 [6,13] by Charles and Ray Eames, and the recent Imax ?lm Cosmic Voyage [15]. We have added our own contribution [9], Cosmic Clock, which is an animation based entirely on the concepts and implementation described in this paper. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.

Hardcover. Condizione: new. Hardcover. This book emerged from a DoE/NSF-sponsored workshop, held in Tahoe City, California, October 2000. About fifty invited participants presented state-of-the-art research on topics such as: - terrain modeling- multiresolution subdivision- wavelet-based scientific data compression- topology-based visualization- data structures, data organization and indexing schemes for scientific data visualization.All invited papers were carefully refereed, resulting in this collection. The book will be of great interest to researchers, graduate students and professionals dealing with scientific visualization and its applications. The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.

Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). Although there are alternate theories, it is generally believed that the large-scale relationships and homogeneities that we see can only be explainedby having the universe expand suddenlyin a very early 'in ationary' period. Subsequent evolution of the Universe is described by the Hubble expansion, the observation that the galaxies are ying away from each other. We can attribute di erent rates of this expansion to domination of di erent cosmological processes, beginning with radiation, evolving to matter domination, and, relatively recently, to vacuum domination (the Cosmological Constant term)[4]. We assume throughout that we will be relying as much as possible on observational data, with simulations used only for limited purposes, e.g., the appearance of the Milky Wayfrom nearbyintergalactic viewpoints. The visualization of large-scale astronomical data sets using xed, non-interactive animations has a long history. Several books and lms exist, ranging from 'Cosmic View: The Universe in Forty Jumps' [3] by Kees Boeke to 'Powers of 10' [6,13] by Charles and Ray Eames, and the recent Imax lm 'Cosmic Voyage' [15]. We have added our own contribution [9], 'Cosmic Clock,' which is an animation based entirely on the concepts and implementation described in this paper. 376 pp. Englisch.

Gebunden. Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Top quality selection in a field which has a booming applications sideThe nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). .

Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Top quality selection in a field which has a booming applications sideThe nature of the physical Universe has been increasingly better understood in recent years, and cosmological concepts have undergone a rapid evolution (see, e.g., [11], [2],or [5]). .