320 likes | 333 Vues
This project focuses on modeling the magneto-rotational instability and turbulent angular momentum transport in astrophysical systems. It utilizes high-performance computing to investigate fluid turbulence and its impact on the transport of angular momentum. The results have implications for understanding the formation and evolution of stars and accretion disks.
E N D
Magneto-rotational instability and turbulent angular momentum transport (INCITE)
Magneto-rotational instability and turbulent angular momentum transport (INCITE)
Interactive Remote Delivery of 3D Visualization Results (LBNL)
Magneto-rotational instability and turbulent angular momentum transport (INCITE)
Single Nucleotide Polymorphism Visualization, Genomics Division, LBNL
Nuclear Magnetic Resonance Imaging Simulation, DOE Office of Science
Quantum Chromodynamics Lattice Gauge Simulation, DOE Office of Science
3D Volume Reconstruction from Cyro-Electron Microscopy, Life Sciences Division, LBNL
Computational Atomic Physics for Controlled Fusion Energy (SciDAC)
3D Volume Reconstruction from Cyro-Electron Microscopy, Life Sciences Division, LBNL
Visualization of Internal Energy, Protein Structure Prediction, LDRD, LBNL
3D Volume Reconstruction from Cyro-Electron Microscopy, Life Sciences Division, LBNL