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Title: |
Numerical Modeling of Space Plasma Flows: Astronum-2007
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Volume: |
385
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Year: |
2008
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View this Volume on ADS
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Editors: |
Pogorelov, Nikolai V.; Audit, Edouard; Zank, Gary P.
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Synopsis: |
This volume is based on talks given at ASTRONUM-2007. This conference is the second in a series of international conferences organized by the Institute of Geophysics and Planetary Physics of the University of California at Riverside and the Laboratory for Research of the Fundamental Laws of the Universe of the French Commissariat of Atomic Energy. The conference subjects include turbulence and cosmic ray transport, astrophysical flows, space plasma flows, kinetic and hybrid simulations, numerical methods, algorithms, and frameworks, and data handling and visualization. All of these are of great importance for scientists investigating solar structure, the heliosphere, the Sun-Earth connection, and various astrophysical phenomena. The problems discussed at the conference involved significantly different scales, regions, or particle populations for which several sets of defining equations or concepts are necessary to understand the physical system in its entirety. This book will be of interest to specialists in applied mathematics, astrophysics, space physics, and computer science who apply novel numerical algorithms to the contemporary problems in these fields. Graduate students will find it a useful reference of the fundamental approaches to solving the fluid dynamics and Boltzmann equations governing space plasma flows.
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ISBN: |
978-1-58381-333-1
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eISBN:
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978-1-58381-334-8
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Paper Title |
Page |
Authors |
Cover |
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Volume 385 Cover |
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Pogorelov, N.V.; Audit, E.; Zank, G.P. |
Front Matter |
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Volume 385 Front Matter |
1 |
Pogorelov, N.V.; Audit, E.; Zank, G.P. |
Part 1. Turbulence and Cosmic Ray Transport |
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Density Statistics of Compressible MHD Turbulence |
3 |
Lazarian, A.; Kowal, G.; Beresnyak, A. |
Implications of the Hall Effect for Turbulent Molecular Clouds |
12 |
Downes, T.P.; O'Sullivan, S. |
Four-dimensional Transport of Cosmic Rays in the Heliosphere |
18 |
Florinski, V.; Pogorelov, N.V. |
Magnetic Fluctuation Spectrum in the Interplanetary Medium |
25 |
Galtier, S. |
Time-dependent Solar Modulation of GCRs Using a Monte Carlo Simulation |
31 |
Li, G.; Webb, G.M.; le Roux, J.A.; Zank, G.P.; Wiedenbeck, M.E. |
Convective, Absolute, and Global Instabilities in Thin Rotating Disks |
38 |
Liverts, E.; Mond, M. |
Vorticity and Turbulence in the Large Scale Structure of the Universe |
44 |
Ryu, D.; Kang, H. |
Non-Kolmogorov-like Turbulence in the Local Interstellar Medium |
50 |
Shaikh, D. |
Cosmic Ray Transport in MHD Turbulence |
56 |
Yan, H.; Lazarian, A. |
A Stochastic Differential Equation Approach to Cosmic Ray Transport |
63 |
Zhang, M. |
Part 2. Astrophysical Flows |
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Fragmentation and Turbulence in the Interstellar Medium |
73 |
Audit, E.; Hennebelle, P. |
Magnetic Acceleration of Relativistic Jets |
79 |
Barkov, M.V. |
The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows |
85 |
Foglizzo, T. |
First Comparison of Two Radiative Transfer Methods: M1 and Sn Techniques |
91 |
González, M.; Velarde, P.; García-Fernández, C. |
Preliminary Results of Three-Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae |
97 |
Jordan, G.C. IV; Fisher, R.T.; Townsley, D.M.; Calder, A.C.; Graziani, C.; Asida, S.; Lamb, D.Q.; Truran, J.W. |
Cosmological Shock Waves in the Large Scale Structure of the Universe |
103 |
Kang, H.; Ryu, D. |
Magnetar Connection to Hypernovae and GRB: Numerical Simulations |
109 |
Komissarov, S.S. |
The Role of Physical Viscosity on Accretion Disc Dynamics in Close Binaries and AGN |
115 |
Lanzafame, G. |
Protoplanet–protoplanetary Disk Interaction with a Godunov Method |
121 |
Masset, F.S. |
A Combined Spectral/Godunov Code for the Simulation of Gravitational Waves from Stellar Supernova Core Collapse |
127 |
Novak, J.; Dimmelmeier, H.; Font, J.A. |
Part 3. Space Plasma Flows |
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MHD-hybrid-kinetic Simulations of Solar Wind Interacting with Bodies: Magnetized and Nonmagnetized Planets and Electric Sailing Spacecraft |
135 |
Janhunen, P. |
Challenges of Extreme Computing Using the FLASH Code |
145 |
Dubey, A.; Fisher, R.; Graziani, C.; Jordan, G.C. IV; Lamb, D.Q.; Reid, L.B.; Rich, P.; Sheeler, D.; Townsley, D.; Weide, K. |
On MHD Modeling of Coronal Mass Ejections |
151 |
Fichtner, H.; Kopp, A.; Kleimann, J.; Grauer, R. |
Magnetic Flux Conservation in Constrained Transport Adaptive Mesh MHD Codes Without Refluxing |
158 |
Loring, B.; Raeder, J. |
Numerical Simulations of Solar Wind Disturbances by Coupled Models |
167 |
Odstrcil, D.; Pizzo, V.J.; Arge, C.N.; Bissi, M.M.; Hick, P.P.; Jackson, B.V.; Ledvina, S.A.; Luhmann, J.G.; Linker, J.A.; Mikic, Z.; Riley, P. |
Numerical Modeling of Weakly Ionized Plasmas |
174 |
O'Sullivan, S.; Downes, T.P. |
MHD-neutral Model of the Outer Heliosphere |
180 |
Pogorelov, N.V.; Zank, G.P.; Borovikov, S.N.; Florinski, V.; Heerikhuisen, J.; Kryukov, I.A. |
What Do We Know About the Orientation of the Local Interstellar Magnetic Field? |
189 |
Ratkiewicz, R.; Ben-Jaffel, L.; Grygorczuk, J. |
Part 4. Kinetic and Hybrid Simulations |
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Modeling the Heliosphere with an Adaptive MHD-kinetic Code |
197 |
Borovikov, S.N.; Heerikhuisen, J.; Pogorelov, N.V.; Kryukov, I.A.; Zank, G.P. |
Modeling Kinetic Neutral Atoms in the Solar-Wind/Interstellar-Medium Interaction Region |
204 |
Heerikhuisen, J.; Pogorelov, N.V.; Florinski, V.; Zank, G.P. |
An Implicit Particle-in-cell Method |
212 |
Lapenta, G. |
Stochastic Numerics for the Boltzmann Equation |
219 |
Rjasanow, S. |
Multi-physics Plasma Simulation by the Interlocking of Two Different Hybrid Models |
228 |
Sugiyama, T.; Kusano, K. |
Part 5. Numerical Methods, Algorithms, and Frameworks |
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Parallel Explicit/Implicit Time Stepping Scheme on Block-Adaptive Grids |
237 |
Tóth, G.; De Zeeuw, D.L.; Ma, Y.; Gombosi, T.I.; Powell, K.G. |
Which Numerical Method for Protostellar Collapse? |
247 |
Commerçon, B.; Hennebelle, P.; Audit, E.; Chabrier, G.; Teyssier, R. |
A Comparison of Two Intermediate State HLLC Solvers for Ideal Magnetohydrodynamics |
253 |
Gurski, K.F. |
Cure for the Carbuncle Instability Based on the Characteristics of the MHD Equations |
259 |
Hanawa, T.; Mikami, H.; Matsumoto, T. |
A New, Three-dimensional, Adaptive Mesh Refinement Code for Modeling Flows of Partially Ionized Plasma |
265 |
Kryukov, I.A.; Borovikov, S.N.; Pogorelov, N.V.; Zank, G.P. |
A Simple Dual Implementation to Track Pressure Accurately |
273 |
Li, S. |
Robust and Efficient Riemann Solvers for MHD |
279 |
Miyoshi, T.; Kusano, K. |
Adaptive Staggered Grids in 3D |
285 |
Rosenbaum, W. |
Computational MagnetoHydrodynamics, Based on Solution of the Well-Posed Riemann Problem |
291 |
Sokolov, I.V.; Powell, K.G.; Cohen, O.; Gombosi, T.I. |
Part 6. Data Handling and Visualization |
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Coupled Analysis and Visualization of High Resolution Astrophysical Simulations |
299 |
Rast, M.; Clyne, J. |
Visualization of Scalar Adaptive Mesh Refinement Data |
309 |
Weber, G.H.; Beckner, V.E.; Childs, H.; Ligocki, T.J.; Miller, M.C.; Van Straalen, B.; Bethel, E.W. |
Parallel Software and Hardware for Capability Visualization of High Performance Computing Results |
321 |
Aguilera, D.; Carrard, T.; Colin de Verdiére, G.; Nominé, J.P.; Tabourin, V. |
Interactive Visualization of Astrophysical Plasma Simulations with SDvision |
327 |
Pomarède, D.; Fidaali, Y.; Audit, E.; Brun, A.S.; Masset, F.; Teyssier, R. |
Back Matter |
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Volume 385 Back Matter |
333 |
Pogorelov, N.V.; Audit, E.; Zank, G.P. |
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