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FLASH Center for Computational Science

Welcome to the FLASH center. ASTROPHYSICISTS SETTLE CENTURY-OLD COSMIC DEBATE ON MAGNETISM OF PLANETS AND STARS. By Robert Mitchum, February 9, 2018. Flash Center astrophysicists demonstrate turbulent dynamo, the mechanism thought to generate cosmic magnetic fields, using world’s most powerful lasers. READ THE ARTICLE AT UCHICAGO NEWS. Also read our paper in NATURE COMMUNICATIONS. FLASH CENTER TEAM UNCLOAKS MAGNETIC FIELDS OF COSMIC EVENTS. By Robert Mitchum, January 4, 2018. THE RELEASE OF FLASH 4.5.

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FLASH Center for Computational Science | asci.uchicago.edu Reviews
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Welcome to the FLASH center. ASTROPHYSICISTS SETTLE CENTURY-OLD COSMIC DEBATE ON MAGNETISM OF PLANETS AND STARS. By Robert Mitchum, February 9, 2018. Flash Center astrophysicists demonstrate turbulent dynamo, the mechanism thought to generate cosmic magnetic fields, using world’s most powerful lasers. READ THE ARTICLE AT UCHICAGO NEWS. Also read our paper in NATURE COMMUNICATIONS. FLASH CENTER TEAM UNCLOAKS MAGNETIC FIELDS OF COSMIC EVENTS. By Robert Mitchum, January 4, 2018. THE RELEASE OF FLASH 4.5.
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FLASH Center for Computational Science | asci.uchicago.edu Reviews

https://asci.uchicago.edu

Welcome to the FLASH center. ASTROPHYSICISTS SETTLE CENTURY-OLD COSMIC DEBATE ON MAGNETISM OF PLANETS AND STARS. By Robert Mitchum, February 9, 2018. Flash Center astrophysicists demonstrate turbulent dynamo, the mechanism thought to generate cosmic magnetic fields, using world’s most powerful lasers. READ THE ARTICLE AT UCHICAGO NEWS. Also read our paper in NATURE COMMUNICATIONS. FLASH CENTER TEAM UNCLOAKS MAGNETIC FIELDS OF COSMIC EVENTS. By Robert Mitchum, January 4, 2018. THE RELEASE OF FLASH 4.5.

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1

Flash Center for Computational Science

http://asci.uchicago.edu/site/movies

Original simulations of the Gravitationaly Confined Detonation. Weakly compressible homogeneous isoptropic turbulence. Resolution Studies of full star breakout. GCD Model with multiple bubbles. Study of Flame Bubbles under three different physical conditions. Rayleigh-Taylor driven thermonuclear combustion. Laser driven Rayleigh-Taylor Richtmyer-Meshkov instabilities. Organization of the Center. Documentation and User Support.

2

Flash Center for Computational Science

http://asci.uchicago.edu/site/flashcode

Hydrodynamics: Unsplit PPM and WENO; Split PPM; 2T Radiation. Magnetohydrodynamics: Unsplit Staggered Mesh; Split 8 wave. Equation of State: Ideal gas; Degenerate Ionized Plasma; Multimaterial. Radiation Transfer: Multigroup Flux-limited Diffusion. Diffusion and Conduction: Implicit with AMR. Laser Energy Deposition: Geometric Optics with Inverse Brensstrahlung. Opacity: Constant; Multimaterial Tabular. Particles: Tracer; Massive; Sink; Charged. Gravity: Constant; PointMass; Planar; Self Gravity. Documen...

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Flash Center for Computational Science

http://asci.uchicago.edu/site/flashcode/download

In order to login through this web page, you must provide two pieces of information:. 1 The e-mail address you provided with your request (use this as your username below). 2 The password you received with your request. If the Captcha at the end of this form does not display in your browser,. Please enable Javascript in your browser and try again. If problems persist email webmaster@flash.uchicago.edu. If you do not have an ID and password for FLASH, please visit the Code Request.

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Flash Center for Computational Science

http://asci.uchicago.edu/site/flashcode/pubs.shtml

Index of FLASH Code Publications. The Software Development Process of FLASH, a Multiphysics Simulation Code. Dubey, A. ; Antypas, K. ; Calder, A. ; Fryxell, B. ; Lamb, D. ; Ricker, P. ; Reid, L. ; Riley, K. ; Rosner, R. ; Siegel, A. ; Timmes, F. ; Vladimirova, N. ; Weide, K. Parallel algorithms for moving Lagrangian data on block structured Eulerian meshes. Dubey, Anshu ; Antypas, Katie ; Daley, Christopher. Optimization of Multigrid Based Elliptic Solver For Petascale Simulations in the FLASH Code.

5

Flash Center for Computational Science

http://asci.uchicago.edu/site/about/organization

Organization of the Center. The organizational structure of the Flash Center consists of the Director, the Associate Director, the Management Group, and three research groups. The research groups are the following:. High Energy Density Physics. Group Leader: Don Lamb). Group Leader: Petros Tzeferacos). The Astrophysics Group is carrying out simulations of Type Ia (thermonuclear-powered) and Type Ib/c and Type II (core collapse) supernovae and validating current models of these explosions against observat...

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Skip to main content. CAC acknowledges support from the following agencies:. DoE ASCI/ASAP California Institute of Technology. National Aeronautics and Space Administration. Department of Electrical and Computer Engineering. SROA, Rutgers University. Rutgers, The State University of New Jersey, an equal opportunity, affirmative action institution. Contact RU-info at 732-445-info (4636) Ask Colonel Henry. And Danang Probo Sayekti.

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FLASH Center for Computational Science

Welcome to the FLASH center. ASTROPHYSICISTS SETTLE CENTURY-OLD COSMIC DEBATE ON MAGNETISM OF PLANETS AND STARS. By Robert Mitchum, February 9, 2018. Flash Center astrophysicists demonstrate turbulent dynamo, the mechanism thought to generate cosmic magnetic fields, using world’s most powerful lasers. READ THE ARTICLE AT UCHICAGO NEWS. Also read our paper in NATURE COMMUNICATIONS. FLASH CENTER TEAM UNCLOAKS MAGNETIC FIELDS OF COSMIC EVENTS. By Robert Mitchum, January 4, 2018. THE RELEASE OF FLASH 4.5.

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