Abstract Information


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List of abstract titles:


Alic, Daniela


Novel techniques in the numerical modeling of relativistic astrophysical plasmas


Aloy, Miguel-Angel


Powering short GRBs by mergers of moderately magnetized neutron stars


Amano, Takanobu


Kinetic and self-consistent numerical modeling of the terrestrial inner magnetosphere


Amari, Tahar


Reconstruction algorithms for the solar coronal magnetic field


Audit, Edouard


A numerical model for multigroup radiation hydrodynamics


Balsara, Dinshaw


High Accuracy Numerical MHD with Stiff Source Terms & Multi-dimensional Riemann Solvers -- Application to Two-fluid Turbulence


Bisikalo, Dmitry


Gaseous flows in the inner part of the circum-binary disk of the T Tauri star


Blakesley, Burkhart


Bridging the Gap: Connecting ISM Turbulence Theory and Observations


Büchner, Joerg


Large-scale fluid-based and kinetic simulations of Solar Plasmas


Carroll-Nellenback, Jonathan


Seeing to the Forrest: AstroBEAR 2.0, Distributed Trees, Multi-level Updates & a Highly Parallelized AMR Multiphysics Code


Cunningham, Andrew


Isothermal Magnetized Bondi Accretion


Daldorff, Lars Kristen Selberg


Fourier Vlasov-Maxwell solver in four-dimensional phase space


Del Zanna, Luca


Parametric decay of Alfven waves: on the role of solar wind expansion


Downes, Turlough


Multifluid magnetohydrodynamic turbulence in weakly ionised astrophysical plasmas


Dumbser, Michael


Very High Order PNPM Schemes on Unstructured Meshes for Classical and Relativistic MHD Equations


Dyadechkin, Sergey


Introduction of curvilinear coordinates in FMI HYB hybrid model: Status report


Falle, S.A.E.G.


Comparison between AMR and SPH


Florinski, Vladimir


Heliospheric modeling on geodesic grids


Font, José A.


Numerical relativity simulations of the Papaloizou-Pringle instability in black hole-torus systems


Feng, Xueshang


Recent Progress & Future Avenue of 3D Solar Storm Modeling by SIP-CESE-MHD Model


Galtier, Sebastien


MHD turbulence and the solar wind


Ganse, Urs


Numerical challenges in kinetic simulations of three-wave interactions


Germaschewski, Kai


Extending global magnetosphere simulations beyond MHD


Giacomazzo, Bruno


Magnetized Binary Neutron Star Mergers


Goldstein, Melvyn


Nonlinear interactions of Alfvénic fluctuations in a spherically expanding solar wind


Hanawa, Tomoyuki


Dynamical Stability of Galactic Shocks


Hidalgo, Carlos


Influence of 3D physics on plasma rotation and transport in fusion plasmas


Howes, Gregory


Gyrokinetic Simulations of Solar Wind Turbulence


Izmodenov, Vlad


Modeling of partly ionized non-equilibrium solar wind/LISM plasma interactions


Janhunen, Pekka


New PIC simulation results of solar wind electric sail


Jiang, Yanfei


A new 3D radiation MHD code - beyond diffusion approximation


Kang, Hyesung


Nonthermal Radiation from Weak Cosmological Shocks


Karimabadi, Homa


Recent Advances in Kinetic Simulations and Analysis Techniques


Keppens, Rony


Dusty circumstellar environments: numerical simulations with MPI-AMRVAC


Kim, Woong-Tae


Gas Dynamics in Central Regions of Barred Galaxies: Two-Dimensional Hydrodynamic Simulations


Kiuchi, Kenta


Gravitational waves and neutrino emission from the merger of binary neutron stars


Klein, Richard


Radiation Hydrodynamic AMR Simulations of High Mass Star Formation: The Effects of Feedback in Cores to Clusters


Kolobov, Vladimir


Simulations of weakly ionized plasmas with adaptive Cartesian mesh


Kritsuk, Alexei


Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence


Kucharek, Harald


Hybrid Simulations for the Evolution of Ion Distributions and the Associated ENA Production at the Termination Shock


Kulpa-Dybe, Katarzyne


The effect of supernova rate on magnetic field evolution in barred and ringed galaxies


Lanzafame, Giuseppe


Semi-Lagrangian implicit integrations in SPH modelling: a model of the accretion disc in a microquasar


Lazarian, Alex


To what extent magnetic fields are frozen in astrophysical fluids?


Lee, Dongwook


Development of a Jacobian-Free Newton-Krylov implicit solver in FLASH


Li, Bo


Modeling the multi-component solar wind: a few numerical aspects and potential applications to stellar winds


Li, Shengtai


High-Order Divergence-Free AMR Method for MHD Flows


Lovelace, Richard


Numerical Modeling of Jets from Accretion Disks


Mac Low, Mordecai-Mark


MHD simulations of a supernova-driven ISM and the warm ionized medium using a positivity preserving ideal MHD scheme


Markidis, Stefano


Global Particle-in-Cell Simulations of Magnetospheres


Matsumoto, Yosuke


Multiscale simulations of the Kelvin-Helmholtz instability


McNally, Colin


Phurbas - Adaptive Lagrangian Meshless Magnetohydrodynamics


Meliani, Zakaria


Two-shell collisions in the GRB afterglow phase


Mignone, Andrea


Adaptive Mesh Computations with the PLUTO code for Astrophysical Fluid Dynamics


Miniati, Francesco


Resistive generation of intergalactic magnetic field at cosmic dawn


Minoshima, Takashi


Multi-Moment Advection scheme for Vlasov simulations


Miyoshi, Takahiro


On numerical shock instabilities of Harten-Lax-van Leer-type approximate Riemann solvers


Moiseenko, Sergey


Magnetorotational processes in core-collapse supernovae


Moreno-Insertis, Fernando


3D-modeling of the emergence of magnetized plasma from the solar interior


Müller, Bernhard


Recent Advances in Simulations of Core-Collapse Supernovae


Müller, Hans-Reinhard


Direct modeling of neutral helium in the heliosphere


Müller, Wolf


Surprises in the theory of anisotropic magnetohydrodynamic turbulence


Ng, Chung-Sang


Large-Scale High-Lundquist Number Reduced MHD Simulations of the Solar Corona using GPU Accelerated Machines


Nishikawa, Ken-ichi


Simulation of Relativistic Jets and Associated Self-consistent Radiation


Nominé, Jean-Philippe


PRACE Research Infrastructure: Petascale Computing Resources for European Scientists


Obergaulinger, Martin


MHD simulations of non-rotating stellar core collapse with neutrinos


Perucho, Manel


ICM reheating by relativistic jets


Pierrard, Viviane


Coupling the plasmasphere model with the ionosphere


Pogorelov, Nikolai


Modeling Nonstationary Heliosphere with the Multi-Scale Fluid-Kinetic Simulation Suite


Radice, David


Discontinuous Galerkin methods for general relativistic hydrodynamics


Raeder, Jimmy


Multi-scale Physics in the Magnetosphere


Rezzolla, Luciano


Modelling the dynamics of compact-object binaries in general relativity


Romanova, Marina M.


Global Simulations of MRI-driven Accretion onto Magnetized Stars


Roussev, Ilia


Global MHD Modeling of CMEs and Related Shock Waves Originating from Complex Active Regions


Ryu, Dongsu


Relativistic MHD Codes for Adiabatic and Isothermal Flows


Schmidt, Wolfram


Modeling unresolved processes in the turbulent multiphase interstellar medium


Servidio, Sergio


Numerical experiments of magnetic reconnection in two-dimensional turbulence


Shen, Fang


3-D MHD Simulation of the Two CMEs' Propagation and Interaction Using Successive Magnetized Plasma Blobs Model


Skinner, Michael


A two-moment radiation hydrodynamics module in Athena using a Godunov method


Spanier, Felix


Hybrid simulations of charged particle motion in the heliosphere


Stergioulas, Nikolaos


Magneto-elastic oscillations and magnetar QPOs


Sugiyama, Tooru


PIC calculation on GPGPU system


Toropina, Olga


MHD Simulation of Bondi-Hoyle Accretion onto Magnetized Neutron Star


Toth, Gabor


Magnetohydrodynamics with Anisotropic Ion Pressure


Usmanov, Arcadi


Three-dimensional modeling of the solar wind: From the coronal base to the outer heliosphere


Van Loo, Sven


Suppressing the star formation rate with magnetic fields


Wu, Shi


Modeling of Solar Active Region on the Basis of A Three-Dimensional, Time-Dependent Magnetohydrodynamic (MHD) Model


Yan, Huirong


Cosmic Ray Transport in MHD Turbulence: large and small scale interactions


Yee, Helen


On Numerical Methods for Hypersonic Turbulent Flows


Zank, Gary P.


The transport of low frequency turbulence in astrophysical flows: Governing model