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Click the serial number on the left to view the details of the item. |
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Author | Title | Accn# | Year | Item Type | Claims |
| 1 |
Hans Goedbloed |
Magnetohydrodynamics of laboratory and astrophysical plasmas |
026584 |
2019 |
Book |
|
| 2 |
David D. Nolte |
Introduction to modern dynamics: Chaos, Networks, Space and Time |
026051 |
2015 |
Book |
|
| 3 |
N. O. Weiss |
Magnetoconvection |
025893 |
2014 |
Book |
|
| 4 |
J. K. Bhattacharjee |
Nonlinear dynamics: Near and Far From Equilibrium |
024425 |
2007 |
Book |
|
| 5 |
Stephen Wiggins |
Introduction to applied nonlinear dynamical systems and chaos |
023954 |
2003 |
Book |
|
| 6 |
Paul Manneville |
Instabilities, chaos and turbulence |
023550 |
2010 |
Book |
|
| 7 |
Steven H. Strogatz |
Nonlinear dynamics and chaos: With applications to physics, biology, chemistry and engineering |
021379 |
2001 |
Book |
|
| 8 |
M. Lakshmanan |
Nonlinear dynamics: Integrability, chaos and patterns |
018429 |
2003 |
Book |
|
| 9 |
Christian Beck |
Spatio-temporal chaos and vacuum fluctuations of quantized fields |
018224 |
2002 |
Book |
|
| 10 |
Sprott, Julien Clinton |
Chaos and time-series analysis |
018211 |
2003 |
Book |
|
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1.
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| Title | Magnetohydrodynamics of laboratory and astrophysical plasmas |
| Author(s) | Hans Goedbloed;Rony Keppens;Stefaan Poedts |
| Publication | Cambridge, Cambridge University Press, 2019. |
| Description | xx, 974p. |
| Abstract Note | With ninety per cent of visible matter in the universe existing in the plasma state, an understanding of magnetohydrodynamics is essential for anyone looking to understand solar and astrophysical processes, from stars to accretion discs and galaxies; as well as laboratory applications focused on harnessing controlled fusion energy. This introduction to magnetohydrodynamics brings together the theory of plasma behavior with advanced topics including the applications of plasma physics to thermonuclear fusion and plasma- astrophysics. Topics covered include streaming and toroidal plasmas, nonlinear dynamics, modern computational techniques, incompressible plasma turbulence and extreme transonic and relativistic plasma flows. The numerical techniques needed to apply magnetohydrodynamics are explained, allowing the reader to move from theory to application and exploit the latest algorithmic advances. Bringing together two previous volumes: Principles of Magnetohydrodynamics and Advanced Magnetohydrodynamics, and completely updated with new examples, insights and applications, this volume constitutes a comprehensive reference for students and researchers interested in plasma physics, astrophysics and thermonuclear fusion. |
| ISBN,Price | 9781107123922 : £ 110.00(HB) |
| Classification | 537.84
|
| Keyword(s) | 1. MAGNETOHYDRODYNAMICS
2. MODERN COMPUTATIONAL TECHNIQUES
3. NONLINEAR DYNAMICS
4. PLASMA ASTROPHYSICS
5. PLASMA PHYSICS
6. RELATIVISTIC PLASMA FLOWS
7. THERMONUCLEAR FUSION
|
| Item Type | Book |
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 026584 |
|
537.84/KRA/026584 |
Issued |
PS15: Snehil Pandey |
14/Jun/2024 |
|
+Copy Specific Information |
2.
 |
|
| Title | Introduction to modern dynamics: Chaos, Networks, Space and Time |
| Author(s) | David D. Nolte |
| Edition | eBooks |
| Publication | Oxford, Oxford University Press, 2015. |
| Description | xiii, 423p. |
| Abstract Note | The best parts of physics are the last topics that our students ever see. These are the exciting new frontiers of nonlinear and complex systems that are at the forefront of university research and are the basis of many high-tech businesses. Topics such as traffic on the World Wide Web, the spread of epidemics through globally-mobile populations, or the synchronization of global economies are governed by universal principles just as profound as Newton's laws. Nonetheless, the conventional university physics curriculum reserves most of these topics for advanced graduate study. Two justifications are given for this situation: first, that the mathematical tools needed to understand these topics are beyond the skill set of undergraduate students, and second, that these are speciality topics with no common theme and little overlap.
Introduction to Modern Dynamics dispels these myths. The structure of this book combines the three main topics of modern dynamics - chaos theory, dynamics on complex networks, and general relativity - into a coherent framework. |
| ISBN,Price | 9780199657049 : UKP 32.50(PB) |
| Classification | 531.3
|
| Keyword(s) | 1. 100 YEARS OF THE FIRST OBSERVATIONS OF T
2. CHAOS
3. COMPLEX SYSTEMS
4. DYNAMICS
5. EBOOK
6. EBOOK - OXFORD UNIVERSITY PRESS
7. HAMILTONIAN DYNAMICS
8. NONLINEAR DYNAMICS
9. RELATIVISTIC DYNAMICS
10. SPACE AND TIME
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 026051 |
|
531.3/NOL/026051 |
On Shelf |
|
|
|
| OB1642 |
|
531.3/NOL/ |
On Shelf |
|
|
|
+Copy Specific Information |
|
3.
|
|
| Title | Magnetoconvection |
| Author(s) | N. O. Weiss;M. R. E. Proctor |
| Publication | Cambridge, Cambridge University Press, 2014. |
| Description | xi, 397p |
| Series | (Cambridge Monographs on Mechanics) |
| Abstract Note | The last thirty years have seen great leaps forward in the subject of magnetoconvection. Computational techniques can now explain exotic nonlinear behaviour, transition to chaos and the formation of structures that can be observed on the surface of the Sun. Here, two leading experts present the current state of knowledge of the subject. They provide a mathematical and numerical treatment of the interactions between electrically conducting fluids and magnetic fields that lead to the complex structures and rich behaviour observed on the Sun and other stars, as well as in the interiors of planets like the Earth. The authors' combined analytical and computational approach provides a model for the study of a wide range of related problems. The discussion includes bifurcation theory, chaotic behaviour, pattern formation in two and three dimensions, and applications to geomagnetism and to the properties of sunspots and other features at the solar surface. |
| ISBN,Price | 9780521190558 : UKP 75.00(HB) |
| Classification | 537.84
|
| Keyword(s) | 1. CONVECTION
2. GEOMAGNETISM
3. MEGNETOCONVECTION
4. MEGNETOHYDRODYNAMICS
5. NONLINEAR DYNAMICS
6. RELATIVISTIC FLUID DYNAMICS
7. SOLAR MAGNETIC FIELDS
|
| Item Type | Book |
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 025893 |
|
537.84/WEI/025893 |
Issued |
MR06: Rajesh Mondal |
29/Nov/2024 |
|
+Copy Specific Information |
|
5.
|
|
| Title | Introduction to applied nonlinear dynamical systems and chaos |
| Author(s) | Stephen Wiggins |
| Edition | 2nd. |
| Publication | New York, Springer, 2003. |
| Description | xix, 843p. |
| Series | (Texts in applied mathematics) |
| Abstract Note | This volume is intended for advanced undergraduate or first-year graduate students as an introduction to applied nonlinear dynamics and chaos. The author has placed emphasis on teaching the techniques and ideas that will enable students to take specific dynamical systems and obtain some quantitative information about the behavior of these systems. He has included the basic core material that is necessary for higher levels of study and research. Thus, people who do not necessarily have an extensive mathematical background, such as students in engineering, physics, chemistry, and biology, will find this text as useful as students of mathematics. |
| ISBN,Price | 0387001778 : EUR 79.95(HB) |
| Classification | 517.938:536.758CHAOS
|
| Keyword(s) | 1. CHAOS
2. DIFFERENTIABLE DYNAMICAL SYSTEMS
3. DYNAMICAL SYSTEMS
4. EBOOK
5. EBOOK - SPRINGER
6. NONLINEAR DYNAMICS
7. NONLINEAR THEORIES
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 023954 |
|
517.938:536.758CHAOS/WIG/023954 |
On Shelf |
|
|
|
| I12057 |
|
517.938:536.758CHAOS/WIG/ |
On Shelf |
|
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+Copy Specific Information | |