Welcome to the FLASH center
The Flash Center for Computational Science at the University of Chicago has been home to several cross-disciplinary computational research projects in its 20-year existence. Anchoring our work is FLASH, a publicly available multiphysics multiscale simulation code with a wide international user base. Research projects include our High-energy Density Physics Initiative which aims to continually improve upon the capabilities of the FLASH code, and our OMEGA and NIF laser experiments.
NEWS -- ASTROPHYSICISTS SETTLE CENTURY-OLD COSMIC DEBATE ON MAGNETISM OF PLANETS AND STARS
UChicago News, 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
NEWS -- FLASH CENTER TEAM UNCLOAKS MAGNETIC FIELDS OF COSMIC EVENTS
UChicago News, By Robert Mitchum, January 4, 2018
Flash Center and MIT scientists describe a new method for acquiring quantitative, high-resolution information about magnetic fields... READ THE ARTICLE AT UCHICAGO NEWS...
*Also read our paper in REVIEW OF SCIENTIFIC INSTRUMENTS
NEWS -- THE RELEASE OF FLASH 4.5
The Flash Center Code Group is pleased to announce the release of an updated version of the FLASH code: FLASH 4.5! This update has a moderate amount of changes from FLASH 4.4, and a number of new features. The DOWNLOAD is available to all with a username and password. For new users, or to update your email address, please initiate a CODE REQUEST.
NEWS -- FLASH CENTER EXPERIMENTS USING THE OMEGA LASER SYSTEMS
VIEW A PHOTO HERE of the team at the National Laser Users Facility and the Laboratory for Laser Energetics at the University of Rochester.
NEWS -- FLASH CENTER STUDYING ORIGIN OF COSMIC MAGNETIC FIELDS USING OMEGA LASER
Magnetic fields are everywhere in the universe, from the Sun and other stars, to galaxies and clusters of galaxies. But the origin of these magnetic fields, and why they are as strong as they are, remain a mystery. Nonlinear amplification of seed magnetic fields by turbulence is a widely invoked explanation for how cosmic magnetic fields become as strong as we observe them to be. But this mechanism – which is called the turbulent dynamo – has never been demonstrated in the laboratory.
Now, an international team of scientists led by the Flash Center for Computational Science has been awarded time at the Omega laser – one of the most powerful lasers in the world – to create a magnetized turbulent plasma and see if the seed magnetic fields are amplified by an enormous amount, as scientists have postulated. To do this, the team fires intense lasers at two targets, creating two plasma jets that each flow through a grid and become turbulent. The jets then collide, making the plasma even more turbulent. The experiment is expected to produce magnetic Reynolds numbers Rm > 1000 – far greater than the value Rm > 200 theorists say is needed for the turbulent dynamo mechanism to work.
The international scientific team conducting the experiment includes members from the University of Oxford, UK; the University of Rochester; the Massachusetts Institute of Technology; Lawrence Livermore National Laboratory; ETH Zurich, Switzerland; Ecole Polytechnique, France; and the Ulsan National Institute of Science and Technology, Korea; as well as the Flash Center at the University of Chicago. The experiment at the Omega laser and the Flash Center’s research in high energy density physics are both supported by the U.S. Department of Energy National Nuclear Security Administration.
NEWS -- FLASH CENTER LASER EXPERIMENT HERALDED AS ONE OF THE TOP-TEN PHYSICS BREAKTHROUGHS OF 2014
Scientists at the Flash Center for Computational Science, along with colleagues in Europe and the U.S., have been heralded by the UK Institute of Physics for making one of the top-ten physics breakthroughs of 2014. They used one of the world's most powerful lasers to create tiny versions of supernova explosions in the laboratory. The experiment demonstrated the amplification of magnetic fields by turbulence, a mechanism thought to play a role in creating the powerful magnetic fields seen in some remnants of exploding stars, such as Cassiopeia A. SEE HOW THEY DID IT.
The Flash Center’s research in high energy density physics is supported by the U.S. Department of Energy National Nuclear Security Administration.
FLASH 3D simulation of the Omega experiment
FLASH full-physics 3D simulation of the Omega experiment. Two foil targets, machined with cylindrical wells in the center, are illuminated with lasers to drive colliding flows. In the path of the flows, two meshes are placed to stir turbulence with a controlled driving scale. The time lapses of density logarithm (rendering) and magnetic field magnitude (three-slice) show the laser-driven jets traversing the grids and colliding at the center. The self-generated Biermann battery fields are amplified to Mega-Gauss values by the induced turbulence.