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Title: |
Numerical Modeling of Space Plasma Flows ASTRONUM-2014
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Volume: |
498
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Year: |
2015
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View this Volume on ADS
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Editors: |
Pogorelov, N.; Audit, E.; Zank, G.
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Synopsis: |
NUMERICAL MODELING OF
SPACE PLASMA FLOWS
ASTRONUM-2014
9th Annual International Conference
Long Beach, CA, USA
23–27 June 2014
This Volume contains the Proceedings of ASTRONUM-2014, the ninth meeting in a series of international conferences organized by the Center for Space Plasma and Aeronomic Research at the University of Alabama in Huntsville, U.S.A. and Maison de la Simulation, CEA-CNRS-INRIAUPsud- UVSQ, France. 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. All of these topics are of great importance to scientists investigating solar structure, the heliosphere, the Sun-Earth connection, and various astrophysical phenomena related to plasma flows.
The plasma phenomena discussed at the conference are characterized by different temporal and spatial scales, regions, and particle populations, for which different sets of defining equations or concepts are necessary to understand the physical systems in their 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 will also be useful to graduate students who want to get acquainted with the fundamental approaches to solving magnetohydrodynamic and kinetic equations governing space plasma flows.
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ISBN: |
978-1-58381-880-0
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eISBN:
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978-1-58381-881-7
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Paper Title |
Page |
Authors |
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Book Cover |
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Front Matter |
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Front Matter |
1 |
Pogorelov, N.; Audit, E.; Zank, G. |
Part I. Turbulence and Cosmic Ray Transport |
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On the Parallel Spectrum and Anisotropy in MHD Turbulence |
3 |
Beresnyak, A. |
Magnetohydrodynamic Turbulence in Accretion Discs: A Test Case for Petascale Computing in Astrophysics |
10 |
Joos, M.; Fromang, S.; Méheut, H. |
Scaling in Supersonic Isothermal Turbulence |
16 |
Kritsuk, A. G.; Norman, M. L.; Wagner, R. |
Accretion Disk Winds by Magnetorotational Turbulence |
22 |
Suzuki, T. K. |
Effects of Two-scale Driving on Turbulence Statistics |
27 |
Yoo, H.; Cho, J. |
Part II. Astrophysical Flows |
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Gravitational Wave Signals in Black-hole-forming Core Collapse |
35 |
Aloy, M. A.; Cerdá-Durán, P.; Obergaulinger, M.; DeBrye, N.; Font, J. A. |
Precessional Density Wave as a Reason of Turbulence in Accretion Disks of Non-magnetic Close Binary Stars |
41 |
Bisikalo, D. V.; Kurbatov, E. P.; Kaygorodov, P. V. |
Pair-Instability Supernovae of Non-Zero Metallicity Stars |
47 |
Chen, K.-J.; Heger, A.; Woosley, S.; Almgren, A.; Whalen, D. J. |
Origin of Magnetic Fields in the Intracluster Medium |
53 |
Cho, J. |
Towards Robust Discontinuous Galerkin Methods for General Relativistic Neutrino Radiation Transport |
59 |
Endeve, E.; Hauck, C. D.; Xing, Y.; Mezzacappa, A. |
A Three-Dimensional Numerical Study of Supernova Remnant Interaction with Inhomogeneous Interstellar Medium |
65 |
Ermishkin, M. V.; Surzhikov, S. T. |
3D Convection-pulsation Simulations with the HERACLES Code |
71 |
Felix, S.; Audit, E.; Dintrans, B. |
Phase Transition Dynamics of The Interstellar Medium: Theory, Methodology, and Implications |
75 |
Inutsuka, S-i.; Inoue, T.; Iwasaki, K.; Stone, J. M.; Suzuki, T. K.; Tsukamoto, Y.; Takamoto, M. |
Gaseous Structures and Mass Drift in Spiral Galaxies: Effects of Arm Strength |
85 |
Kim, Y.; Kim, W.-T. |
Multi-Physics Feedback Simulations with Realistic Initial Conditions of the Formation of Star Clusters: From Large Scale Magnetized Clouds to Turbulent Clumps to Cores to Stars |
91 |
Klein, R. I.; Li, P.; McKee, C. F. |
Long-Time Sustainability of Rossby Wave Instability in Protoplanetary Disks with Dead Zone |
102 |
Li, S.; Li, H. |
A Three-Dimensional Neutrino-Driven Core Collapse Supernova Explosion of a 15 M☉ Star |
108 |
Mezzacappa, A.; Lentz, E. J.; Bruenn, S. W.; Hix, W. R.; Messer, O. E. B.; Endeve, E.; Blondin, J. M.; Harris, J. A.; Marronetti, P.; Yakunin, K. N.; Lingerfelt, E. J. |
Magnetic Field Amplification in Non-Rotating Stellar Core Collapse |
115 |
Obergaulinger, M.; Janka, H.-T.; Aloy, M. A. |
High-Order Numerical-Relativity Simulations of Binary Neutron Stars |
121 |
Radice, D.; Rezzolla, L.; Galeazzi, F. |
Computational Physics of Small Meteors |
127 |
Surzhikov, S. |
Protostellar Collapse Using Multigroup Radiation Hydrodynamics |
133 |
Vaytet, N.; Chabrier, G.; Audit, E.; Commerçon, B.; Masson, J.; González, M.; Ferguson, J.; Delahaye, F. |
Part III. Space Plasma Flows |
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Numerical Modeling of the Solar Chromosphere and Corona: What Has Been Done? What Should Be Done? |
141 |
Hansteen, V.; Carlsson, M.; Gudiksen, B. |
Details of a Hybrid Model for the Interaction between the Solar Wind and Planets Implemented in FLASH |
147 |
Holmstrom, M.; Wang, X.-D. |
Solar Differential rotation Maintained by Small- and Large-scale Convection |
154 |
Hotta, H.; Rempel, M.; Yokoyama, T. |
Mixing of the Interstellar and Solar Plasmas at the Heliospheric Interface |
160 |
Pogorelov, N. V.; Borovikov, S. N. |
Modeling the Global Distribution of Plasma Parameters on Coronal Source Surface for Different Solar Phases Using 1AU Observations |
168 |
Yang, Y.; Shen, F.; Feng, X. |
Part IV. Kinetic, Particle, and Hybrid Simulations |
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The Marriage of Gas and Dust |
177 |
Price, D. J.; Laibe, G. |
Part V. Numerical Methods, Algorithms, and Frameworks |
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A New RMHD Code for Astrophysical Applications |
185 |
Aloy, M. A.; Borovikov, S.; Pogorelov, N. |
The ANTARES Code: New Developments |
191 |
Blies, P. M.; Kupka, F.; Muthsam, H. J. |
A Simple and Robust Adaptive Time-Stepping Method for Implicit Scheme in Adaptive Mesh-Refinement Codes |
197 |
Commerçon, B.; Debout, V.; Teyssier, R. |
Wiggle Instability Revisited: The Role of Bulk Viscosity |
203 |
Hanawa, T. |
Well-balanced Schemes for Gravitationally Stratified Media |
210 |
Käppeli, R.; Mishra, S. |
Planet-Disk Interaction on the GPU: The FARGO3D code |
216 |
Masset, F. S.; Benítez-Llambay, P. |
Vlasiator: Global Kinetic Magnetospheric Modeling Tool |
222 |
Sandroos, A.; von Alfthan, S.; Hoilijoki, S.; Honkonen, I.; Kempf, Y.; Pokhotelov, D.; Palmroth, M. |
Part VI. Data Handling and Visualization |
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A Screen Space GPGPU Surface LIC Algorithm for Distributed Memory Data Parallel Sort Last Rendering Infrastructures |
231 |
Loring, B.; Karimabadi, H.; Rortershteyn, V. |
Visualizing the Big (and Large) Data from an HPC Resource |
240 |
Sisneros, R. |
Back Matter |
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Author Index |
251 |
Pogorelov, N.; Audit, E.; Zank, G. |
Back Matter |
253 |
Pogorelov, N.; Audit, E.; Zank, G. |
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