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Title: |
5th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2010)
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Volume: |
444
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Year: |
2011
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View this Volume on ADS
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Editors: |
Nikolai V. Pogorelov
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Synopsis: |
This Volume contains the Proceedings of ASTRONUM-2010 — the
fifth in a series of international conferences now organized by the
Center for Space Plasma and Aeronomic Research at the University of
Alabama in Huntsville and the Laboratory for Research into the
Fundamental Laws of the Universe at the French Alternative Energies
and Atomic Energy Commission. The subjects of the conference
included such topics as turbulence and cosmic ray transport, astrophysical
and space plasma flows, kinetic and hybrid simulations,
numerical methods, algorithms, and frameworks, and data handling
and visualization. All of these topics 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 are characterized by different
time and space scales, regions, or particle populations, for which different
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 working on the application of novel numerical
algorithms to contemporary problems arising in these fields. It can also
be used by graduate students wanting to get acquainted with the fundamental
approaches to solving fluid dynamics and kinetic equations
governing space plasma flows.
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ISBN: |
978-1-58381-768-1
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eISBN:
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978-1-58381-769-8
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Paper Title |
Page |
Authors |
Front Matter |
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Front Matter |
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Nikolai V. Pogorelov |
Part I. Turbulence and Cosmic Ray Transport |
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Strong Imbalanced Turbulence |
3 |
Beresnyak, A. |
Statistical Tools of Interstellar Turbulence: Bridging the Gap Between Numerics and Observations |
9 |
Burkhart, B.; Lazarian, A. |
Modeling Sub-Chandrasekhar Type Ia Supernovae |
15 |
Fink, M.; Röpke, F. K.; Hillebrandt, W.; Kromer, M.; Sim, S. A.; Seitenzahl, I. R. |
Uncertainty Quantification for Turbulent Mixing Simulations |
21 |
Kaman, T.; Glimm, J.; Sharp, D. H. |
Cosmic Ray Spectrum in Supernova Remnant Shocks |
28 |
Kang, H. |
Accretion Disk Turbulence With a Detailed Thermodynamics |
36 |
Kissmann, R.; Flaig, M.; Kley, W. |
Modeling the Effects of Turbulence in Zero- and Low-metallicity Star Formation |
42 |
Klessen, R. S.; Glover, S. C. O.; Clark, P. C.; Greif, T. H.; Bromm, V. |
Modulation of Cosmic Rays in the Heliosheath |
48 |
Kóta, J. |
The Spectral Structure of Anisotropic MHD Turbulence |
54 |
Grappin, R.; Müller, W.-C. |
Part II. Astrophysical Flows |
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GRMHD Simulations of Black Hole Accretion Disks |
63 |
Hawley, J. F. |
Nonlinear Dynamical Friction in a Gaseous Medium |
69 |
Kim, W.-T. |
Two-component Jets and the Fanaroff–Riley Dichotomy |
75 |
Meliani, Z.; Keppens, R. |
Simulation of Relativistic Shocks and Associated Radiation from Turbulent Magnetic Fields |
81 |
Nishikawa, K.-I.; Niemiec, J.; Medvedev, M.; Zhang, B.; Hardee, P.; Mizuno, Y.; Nordlund, A.; Frederiksen, J.; Sol, H.; Pohl, M.; Hartmann, D. H.; Fishman, G. J. |
Numerical Methods to Study Triggered Star Formation Around HII Regions |
87 |
Tremblin, P.; Audit, E.; Minier, V.; Schneider, N. |
Numerical Simulation of MHD Flows in Close Binaries with Strong Magnetic Field |
91 |
Zhilkin, A. G.; Bisikalo, D. V. |
Part III. Space Plasma Flows |
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Improving Data Drivers for Coronal and Solar Wind Models |
99 |
Arge, C. N.; Henney, C. J.; Koller, J.; Toussaint, W. A.; Harvey, J. W.; Young, S. |
The Effects of the Sun Rotation on the Solar Wind Propagation |
105 |
Borovikov, S. N.; Pogorelov, N. V. |
Three-Dimensional Solar Wind Structures Obtained with MHD Simulation Model Using Observation-Based Time-Varying Inner Boundary Map |
111 |
Hayashi, K.; Tokumaru, M.; Fujiki, K.; Kojima, M. |
A Solar Wind Model with Current Sheets |
117 |
Li, G.; Qin, G. |
High Lundquist Number Resistive MHD Simulations of Magnetic Reconnection: Searching for Secondary Island Formation |
124 |
Ng, C. S.; Ragunathan, S. |
Heliospheric Modeling with MS-FLUKSS: Interpretation of the IBEX Measurements
and Time-dependent Simulations |
130 |
Pogorelov, N. V.; Borovikov, S. N.; Heerikhuisen, J.; Kim, T.; Kryukov, I. A.; Zank, G. P. |
Low-frequency Waves Driven by Kelvin–Helmholtz Instability in a Bounded Plasma Flow |
137 |
Shevelev, M. M.; Burinskaya, T. M. |
A Global Solar Wind Model Based on Surface Measurements of Magnetic Field and
Transverse Velocity from GONG |
143 |
Wu, S. T.; Wang, A. H.; Wu, C.-C.; Hill, F.; Hernández, I. G.; Feng, X. S.; Dryer, M. |
Part IV. Kinetic, Particle, and Hybrid Simulations |
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Effect of Pitch Angle Scattering on Formation of the Interstellar Boundary Explorer Ribbon in the Outer Heliosheath |
153 |
Gamayunov, K.; Zhang, M.; Rassoul, H. |
Algorithmic Breakthroughs in Multiscale Particle-in-Cell Simulations |
160 |
Omelchenko, Y. A.; Karimabadi, H. |
A Numerical Method to Determine the Particle Velocity Distribution Functions in Space |
166 |
Pierrard, V. |
Numerics of the Inelastic Boltzmann Equation |
176 |
Rjasanow, S. |
Vlasov Code Simulation of Cross-scale Coupling in Space Plasmas |
182 |
Umeda, T.; Matsumoto, Y.; Nakamura, T. K. M.; Fukazawa, K.; Ogino, T. |
Part V. Numerical Methods, Algorithms, and Frameworks |
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High Lundquist Number Reconnection |
191 |
Gardiner, T. A. |
Using Automated Code Generation to Support High Performance
Extended MHD Integration in OpenGGCM |
197 |
Germaschewski, K.; Raeder, J. |
Numerical Scheme to Solve 3D Structure of Rotationally
Supported Gas Disks |
204 |
Hanawa, T.; Kikuchi, D.; Otomo, Y. |
An Energy Conserving Parallel Hybrid Plasma Solver |
211 |
Holmström, M. |
A Roe-type Riemann Solver Based on the Spectral Decomposition
of the Equations of Relativistic Magnetohydrodynamics |
217 |
Ibáñez, J. M.; Aloy, M. A.; Mimica, P.; Antón, L.; Miralles, J. A.; Martí, J. M. |
Coupling Kinetic and Hydrodynamic Models for Simulations
of Gas Flows and Weakly Ionized Plasmas |
223 |
Kolobov, V. I.; Arslanbekov, R. R. |
How Dissipation and Free Boundary Layers Can Be Better Handled in the SPH Approach |
230 |
Lanzafame, G.; Costa, V.; Belvedere, G. |
An Upwind Slope Limiter for PPM that Preserves Monotonicity in Magnetohydrodynamics |
236 |
Lee, D. |
Higher Order Divergence-Free Methods for Three-Dimensional MHD
Flows on Overlapping Grid |
242 |
Li, S. |
Relativistic Hydrodynamic Codes for Adiabatic and Isothermal Flows |
248 |
Ryu, D.; Chattopadhyay, I.; Jang, H. |
Numerical Approximation of MHD Equations for Real Gases |
254 |
Serna, S.; Marquina, A. |
The Athena Astrophysical MHD Code in Cylindrical Geometry |
260 |
Skinner, M. A.; Ostriker, E. C. |
LES of Temporally Evolving Mixing Layers by Three High Order Schemes |
266 |
Yee, H.; Sjögreen, B.; Hadjadj, A. |
Part VI. Data Handling and Visualization |
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Hybrid Parallelism for Volume Rendering on Large, Multi-core Systems |
275 |
Howison, M.; Bethel, E. W.; Childs, H. |
Petascale Global Kinetic Simulations of The Magnetosphere and Visualization Strategies for
Analysis of Very Large Multi-Variate Data Sets |
281 |
Karimabadi, H.; Loring, B.; Vu, H. X.; Omelchenko, Y.; Tatineni, M.; Majumdar, A.; Ayachit, U.; Geveci, B. |
Topology-based Feature Definition and Analysis |
292 |
Weber, G. H.; Bremer, P.-T.; Gyulassy, A.; Pascucci, V. |
Author Index |
299 |
Nikolai V. Pogorelov |
Back Matter |
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Back Matter |
301 |
Nikolai V. Pogorelov |
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